list of nearest galaxies

This is a list of known galaxies within 3.8 megaparsecs (12.4 million light-years) of the Solar System, in ascending order of heliocentric distance, or the distance to the Sun.

This encompasses about 50 major Local Group galaxies, and some that are members of neighboring galaxy groups, the M81 Group and the Centaurus A/M83 Group, and some that are currently not in any defined galaxy group.

The list aims to reflect current knowledge: not all galaxies within the 3.8 Mpc radius have been discovered. Nearby dwarf galaxies are still being discovered, and galaxies located behind the central plane of the Milky Way are extremely difficult to discern. It is possible for any galaxy to mask another located beyond it.

Intergalactic distance measurements are subject to large uncertainties. Figures listed are composites of many measurements, some of which may have had their individual error bars tightened to the point of no longer overlapping with each other.{{cite journal|doi=10.1086/382905|title=A Catalog of Neighboring Galaxies|year=2004|last1=Karachentsev|first1=Igor D.|last2=Karachentseva|first2=Valentina E.|last3=Huchtmeier|first3=Walter K.|last4=Makarov|first4=Dmitry I.|journal=The Astronomical Journal|volume=127|issue=4|pages=2031–2068|bibcode=2004AJ....127.2031K|s2cid=124129428 |doi-access=free}}

List

class="wikitable sortable" style="font-size: 90%
align="center" \|# !Picture !Galaxy !Type ! colspan="2" \|Distance from Earth ! colspan="2" \|Magnitude ! align="center" \|Group Membership !Notes ! data-sort-type="number" \|Diameter (ly)
- \|60px \|Milky Way \|Barred spiral galaxy \| 0.0265 (to the galactic center)Earth is 8,122 ± 31 parsecs (26,490 ± 100 ly) or 0.0265 million light years from the galactic center (the center of the Milky Way). The distance of Earth from the galaxy which contains it is of course "zero" \| align="center" \| 0.008 \| −20.8 \| n/a \|Local Group \|Home galaxy of Earth. Barred spiral galaxy. \|87,400 ly
1 \| \| Ursa Major III \| Dwarf spheroidal galaxy \| 0.10758 \| 0.033 \| 0.010{{Citation \|last1=Smith \|first1=Simon E. T. \|last2=Cerny \|first2=William \|last3=Hayes \|first3=Christian R. \|last4=Sestito \|first4=Federico \|last5=Jensen \|first5=Jaclyn \|last6=McConnachie \|first6=Alan W. \|last7=Geha \|first7=Marla\|author7-link= Marla Geha \|last8=Navarro \|first8=Julio \|last9=Li \|first9=Ting S. \|date=January 2024 \|title=The discovery of the faintest known Milky Way satellite using UNIONS \|journal=The Astrophysical Journal \|volume=961 \|issue=1 \|pages=92 \|doi=10.3847/1538-4357/ad0d9f \|doi-access=free \|arxiv=2311.10147 \|bibcode=2024ApJ...961...92S}} \| +2.2 \| 18.87 \| align="center"\|Local Group \| Satellite of Milky Way
2 \|File:Draco II Dwarf Galaxy.jpg \| Draco II \| dSph \| 0.0701 \| 0.0215{{cite journal\|doi=10.1093/mnras/sty1986\|title=Pristine dwarf galaxy survey – I. A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite\|year=2018\|last1=Longeard\|first1=Nicolas\|last2=Martin\|first2=Nicolas\|last3=Starkenburg\|first3=Else\|last4=Ibata\|first4=Rodrigo A.\|last5=Collins\|first5=Michelle L M.\|last6=Geha\|first6=Marla\|author6-link= Marla Geha \|last7=Laevens\|first7=Benjamin P M.\|last8=Rich\|first8=R Michael\|last9=Aguado\|first9=David S.\|last10=Arentsen\|first10=Anke\|last11=Carlberg\|first11=Raymond G.\|last12=Côté\|first12=Patrick\|last13=Hill\|first13=Vanessa\|last14=Jablonka\|first14=Pascale\|last15=González Hernández\|first15=Jonay I.\|last16=Navarro\|first16=Julio F.\|last17=Sánchez-Janssen\|first17=Rubén\|last18=Tolstoy\|first18=Eline\|last19=Venn\|first19=Kim A.\|last20=Youakim\|first20=Kris\|journal=Monthly Notices of the Royal Astronomical Society\|volume=480\|issue=2\|pages=2609–2627\|doi-access=free \|arxiv=1807.10655\|bibcode=2018MNRAS.480.2609L}} \| −0.8 \| 15.87 \| align="center"\|Local Group \| Satellite of Milky Way \| 120 ly
3 \|File:Tucana III.jpg \| Tucana III \| dSph \| 0.2445 \| 0.0747 \| 0.0229 \| −1.3 \| 15.5Calculated from the distance modulus ( $m - M$ ) and the absolute magnitude ( $M_{V}$ ) \| align="center"\|Local Group \| Satellite of Milky Way that is being tidally disrupted
4 \| \| Segue 1 \| dSph or Glob Clus \| 0.075 \| 0.023 \| −3.0 \| 13.8 \| align="center"\|Local Group \| Satellite of Milky Way \|
5 \| align="center"\| 60px \| Sagittarius Dwarf Sphr SagDEG \| dSph/E7 \| 0.078 \| 0.024{{cite journal \| author=I. D. Karachentsev \| title=The Local Group and Other Neighboring Galaxy Groups \| journal=Astronomical Journal \| date=2005 \| volume=129 \| issue=1 \| pages=178–188 \| bibcode=2005AJ....129..178K \| doi=10.1086/426368 \|arxiv = astro-ph/0410065 \| s2cid=119385141 }} \| −12.67 \| 4.5{{cite web \|title=NASA/IPAC Extragalactic Database \|url=http://nedwww.ipac.caltech.edu/ \|access-date=2008-06-20 \|archive-date=2011-05-14 \|archive-url=https://web.archive.org/web/20110514100451/http://nedwww.ipac.caltech.edu/ \|url-status=live }} Retrieved 2008. \| align="center"\|Local Group \| Satellite of Milky Way (partial accretion by Milky Way) \|10,000 ly
6 \| \| Hydrus I \| 0.09128 \| 0.09 \| 0.0276{{cite journal\|bibcode=2018MNRAS.479.5343K\|title=Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge\|last1=Koposov\|first1=Sergey E.\|last2=Walker\|first2=Matthew G.\|last3=Belokurov\|first3=Vasily\|last4=Casey\|first4=Andrew R.\|last5=Geringer-Sameth\|first5=Alex\|last6=MacKey\|first6=Dougal\|last7=Da Costa\|first7=Gary\|last8=Erkal\|first8=Denis\|last9=Jethwa\|first9=Prashin\|last10=Mateo\|first10=Mario\|last11=Olszewski\|first11=Edward W.\|last12=Bailey\|first12=John I.\|journal=Monthly Notices of the Royal Astronomical Society\|year=2018\|volume=479\|issue=4\|pages=5343\|doi=10.1093/mnras/sty1772\|doi-access=free \|arxiv=1804.06430}} \| −4.71 \| 12.49 \| align="center"\|Local Group \| Satellite of Milky Way, possibly associated with the Magellanic Clouds \| 348 ly
7 \| align="center"\| \| Carina III \| \| 0.0907 \| 0.0278 \| −2.4 \| 14.82 \| align="center"\|Local Group \| Satellite of Milky Way \| 200 ly
8 \| \| Ursa Major II Dwarf \| dSph \| 0.098 \| 0.030 \| −4.2 \| 14.3 \| align="center"\|Local Group \| Satellite of Milky Way (accretion by Milky Way) \|data-sort-value="1800"\|~1,800 ly
8 \| \| Triangulum II \| \| 0.098 \| 0.030 \| −1.8 \| 15.6 \| align="center"\|Local Group \| Satellite of Milky Way (accretion by Milky Way) \|
10 \| align="center"\| \| Reticulum II \| \| 0.102 \| 0.0314{{cite journal\|doi= 10.3847/1538-4357/aacd0e\|title= A Deeper Look at the New Milky Way Satellites: Sagittarius II, Reticulum II, Phoenix II, and Tucana III\|year= 2018\|last1= Mutlu-Pakdil\|first1= Burçin\|last2= Sand\|first2= David J.\|last3= Carlin\|first3= Jeffrey L.\|last4= Spekkens\|first4= Kristine\|last5= Caldwell\|first5= Nelson\|last6= Crnojević\|first6= Denija\|last7= Hughes\|first7= Allison K.\|last8= Willman\|first8= Beth\|last9= Zaritsky\|first9= Dennis\|journal= The Astrophysical Journal\|volume= 863\|issue= 1\|pages= 25\|arxiv= 1804.08627\|bibcode= 2018ApJ...863...25M\|s2cid= 118877962\|doi-access= free}} \| −3.1 \| 14.4 \| align="center"\|Local Group \| Satellite of Milky Way \| 378 ly
11 \| align="center"\| \| Segue 2 \| dSph \| 0.114 \| 0.035{{cite journal\|last=Belokurov\|first=V.\|author2=Walker, M.G. \|author3=Evans, N.W. \|display-authors=etal \|title=Segue 2: A Prototype of the Population of Satellites of Satellites\|date=2009\|journal=Mon. Not. R. Astron. Soc.\|volume=397\|issue=4\|pages=1748–1755\|doi=10.1111/j.1365-2966.2009.15106.x \|doi-access=free \|bibcode=2009MNRAS.397.1748B\|arxiv=0903.0818\|s2cid=20051174}} \| −2.5 \| \| align="center"\|Local Group \| Satellite of Milky Way, one of the smallest known galaxies \| 220 ly
12 \| align="center"\| \| Carina II \| \| 0.122 \| 0.0374{{cite journal\|bibcode=2018ApJ...857..145L\|title=Ships Passing in the Night: Spectroscopic Analysis of Two Ultra-faint Satellites in the Constellation Carina\|last1=Li\|first1=T. S.\|last2=Simon\|first2=J. D.\|last3=Pace\|first3=A. B.\|last4=Torrealba\|first4=G.\|last5=Kuehn\|first5=K.\|last6=Drlica-Wagner\|first6=A.\|last7=Bechtol\|first7=K.\|last8=Vivas\|first8=A. K.\|last9=Van Der Marel\|first9=R. P.\|last10=Wood\|first10=M.\|last11=Yanny\|first11=B.\|last12=Belokurov\|first12=V.\|last13=Jethwa\|first13=P.\|last14=Zucker\|first14=D. B.\|last15=Lewis\|first15=G.\|last16=Kron\|first16=R.\|last17=Nidever\|first17=D. L.\|last18=Sánchez-Conde\|first18=M. A.\|last19=Ji\|first19=A. P.\|last20=Conn\|first20=B. C.\|last21=James\|first21=D. J.\|last22=Martin\|first22=N. F.\|last23=Martinez-Delgado\|first23=D.\|last24=Noël\|first24=N. E. D.\|author25=MagLiteS Collaboration\|journal=The Astrophysical Journal\|year=2018\|volume=857\|issue=2\|pages=145\|doi=10.3847/1538-4357/aab666\|arxiv=1802.06810\|s2cid=96446126 \|doi-access=free }} \| −4.5 \| 13.36 \| align="center"\|Local Group \| Satellite of Milky Way \| 590 ly
13 \| align="center"\| \| Willman 1 \| dSph or Star Clus \| 0.124 \| 0.038 \| −2.7 \| \| align="center"\|Local Group \| Satellite of Milky Way \|
14 \| align="center"\| \| Boötes II \| dSph \| 0.137 \| 0.042{{cite journal\|author1=Martin, Nicolas F.\|author2=de Jong, Jelte T. A.\|author3=Rix, Hans-Walter\|date=September 2008\|title=A Comprehensive Maximum Likelihood Analysis of the Structural Properties of Faint Milky Way Satellites\|journal=The Astrophysical Journal\|volume=684\|issue=2\|pages=1075–1092\|bibcode=2008ApJ...684.1075M\|doi=10.1086/590336\|arxiv=0805.2945\|s2cid=17838966}} \| −2.7 \| \| align="center"\|Local Group \| Satellite of Milky Way \|
14 \| align="center"\| \| Coma Berenices Dwarf \| dSph \| 0.137 \| 0.042{{cite journal\|last=Musella\|first=Ilaria\|author2=Ripepi, Vincenzo \|author3=Clementini, Gisella \|title=Pulsating Variable Stars in the Coma Berenices Dwarf Spheroidal Galaxy\|year=2009\|journal=The Astrophysical Journal Letters\|volume=695\|issue=1\|pages=L83–1L87\|doi=10.1088/0004-637X/695/1/L83\|bibcode=2009ApJ...695L..83M \|arxiv=0902.4230 \|s2cid=11594422\|display-authors=etal}} \| −3.6 \| \| align="center"\|Local Group \| Satellite of Milky Way \|
16 \| align="center"\| \| Pictor II \| \| 0.147 \| 0.045{{cite journal\|bibcode=2016ApJ...833L...5D\|title=An Ultra-faint Galaxy Candidate Discovered in Early Data from the Magellanic Satellites Survey\|last1=Drlica-Wagner\|first1=A.\|last2=Bechtol\|first2=K.\|last3=Allam\|first3=S.\|last4=Tucker\|first4=D. L.\|last5=Gruendl\|first5=R. A.\|last6=Johnson\|first6=M. D.\|last7=Walker\|first7=A. R.\|last8=James\|first8=D. J.\|last9=Nidever\|first9=D. L.\|last10=Olsen\|first10=K. A. G.\|last11=Wechsler\|first11=R. H.\|last12=Cioni\|first12=M. R. L.\|last13=Conn\|first13=B. C.\|last14=Kuehn\|first14=K.\|last15=Li\|first15=T. S.\|last16=Mao\|first16=Y. -Y.\|last17=Martin\|first17=N. F.\|last18=Neilsen\|first18=E.\|last19=Noel\|first19=N. E. D.\|last20=Pieres\|first20=A.\|last21=Simon\|first21=J. D.\|last22=Stringfellow\|first22=G. S.\|last23=Van Der Marel\|first23=R. P.\|last24=Yanny\|first24=B.\|journal=The Astrophysical Journal\|year=2016\|volume=833\|issue=1\|pages=L5\|doi=10.3847/2041-8205/833/1/L5\|arxiv=1609.02148\|s2cid=56071154 \|doi-access=free }} \| −3.2 \| 15.1 \| align="center"\|Local Group \| Satellite of Milky Way possibly associated with the Large Magellanic Cloud \| 300 ly
17 \| align="center"\| \| Boötes III \| dSph \| 0.150 \| 0.046{{cite journal\|last=Grillmair\|first=C.J.\|title=Four New Stellar Debris Streams in the Galactic Halo\|date=2009\|journal=The Astrophysical Journal\|volume=693\|issue=2\|pages=1118–1127\|doi=10.1088/0004-637X/693/2/1118\|bibcode=2009ApJ...693.1118G\|arxiv=0811.3965 \|s2cid=17328907}} \| −5.8{{cite journal\|last1=Carlin\|first1=Jeffrey L.\|last2=Grillmair\|first2=Carl J.\|last3=Muñoz\|first3=Ricardo R.\|title=Kinematics and Metallicities in the Boötes III Stellar Overdensity: a Disrupted Dwarf Galaxy?\|date=September 2009\|journal=The Astrophysical Journal Letters\|volume=702\|issue=1\|pages=L9–L13\|doi=10.1088/0004-637X/702/1/L9\|bibcode=2009ApJ...702L...9C\|arxiv=0907.3738 \|s2cid=62784400\|display-authors=etal}} \| \| align="center"\|Local Group \| Satellite of Milky Way \|
18 \| align="center"\| \| Tucana IV \| \| 0.157 \| 0.048 \| −3.5 \| 14.9 \| align="center"\|Local Group \| Satellite of Milky Way \|
19 \| align="center"\| 60px \| Large Magellanic Cloud (LMC) \| SB(s)m \| 0.163 \| 0.050 \| −17.93 \| 0.9 \| align="center"\|Local Group \| Satellite of Milky Way \|32,200 ly
20 \| align="center"\| \| Grus II \| \| 0.179 \| 0.055 \| −3.9 \| \| align="center"\|Local Group \| Satellite of Milky Way \| 607 ly
21 \| align="center"\| \| Tucana II \| \| 0.186 \| 0.057{{cite journal\|bibcode=2016ApJ...819...53W\|arxiv=1511.06296\|doi=10.3847/0004-637X/819/1/53\|title= Magellan/M2FS Spectroscopy of Tucana 2 and Grus 1\|year=2016\|last1=Walker\|first1=Matthew G.\|last2=Mateo\|first2=Mario\|last3=Olszewski\|first3=Edward W.\|last4=Koposov\|first4=Sergey\|last5=Belokurov\|first5=Vasily\|last6=Jethwa\|first6=Prashin\|last7=Nidever\|first7=David L.\|last8=Bonnivard\|first8=Vincent\|last9=Iii\|first9=John I. Bailey\|last10=Bell\|first10=Eric F.\|last11=Loebman\|first11=Sarah R.\|journal=The Astrophysical Journal\|volume=819\|issue=1\|pages=53\|s2cid=118507573 \|doi-access=free }} \| −3.8 \| 15.0 \| align="center"\|Local Group \| Satellite of Milky Way \|1080 ly
22 \| align="center"\| 60px \| Boötes I \| dSph \| 0.197 \| 0.060 \| −5.8Belokurov, 2006 A Faint New Milky Way Satellite in Bootes \| 13.1 \| align="center"\|Local Group \| Satellite of Milky Way \|
23 \| align="center"\| 60px \| Small Magellanic Cloud (SMC, NGC 292) \| SB(s)m pec \| 0.205 \| 0.063 \| −16.35 \| 2.7 \| align="center"\|Local Group \| Satellite of Milky Way \|18,900 ly
23 \| align="center"\| 60px \| Ursa Minor Dwarf \| dE4 \| 0.205 \| 0.063 \| −7.13 \| 11.9 \| align="center"\|Local Group \| Satellite of Milky Way \|
24 \| \| Virgo II \| \| 0.235 \| 0.072 \| −1.6 \| 17.7 \| align="center" \|Local Group \| Satellite of Milky Way \|
25 \| align="center"\| \| Eridanus IV \| \| 0.250 \| 0.0767{{cite journal\|doi=10.3847/2041-8213/ac2d9a\|title=Eridanus IV: An Ultra-faint Dwarf Galaxy Candidate Discovered in the DECam Local Volume Exploration Survey\|year=2021\|last1=Cerny\|first1=W.\|last2=Pace\|first2=A. B.\|last3=Drlica-Wagner\|first3=A.\|last4=Koposov\|first4=S. E.\|last5=Vivas\|first5=A. K.\|last6=Mau\|first6=S.\|last7=Riley\|first7=A. H.\|last8=Bom\|first8=C. R.\|last9=Carlin\|first9=J. L.\|last10=Choi\|first10=Y.\|last11=Erkal\|first11=D.\|last12=Ferguson\|first12=P. S.\|last13=James\|first13=D. J.\|last14=Li\|first14=T. S.\|last15=Martínez-Delgado\|first15=D.\|last16=Martínez-Vázquez\|first16=C. E.\|last17=Munoz\|first17=R. R.\|last18=Mutlu-Pakdil\|first18=B.\|last19=Olsen\|first19=K. A. G.\|last20=Pieres\|first20=A.\|last21=Sakowska\|first21=J. D.\|last22=Sand\|first22=D. J.\|last23=Simon\|first23=J. D.\|last24=Smercina\|first24=A.\|last25=Stringfellow\|first25=G. S.\|last26=Tollerud\|first26=E. J.\|last27=Adamów\|first27=M.\|last28=Hernandez-Lang\|first28=D.\|last29=Kuropatkin\|first29=N.\|last30=Santana-Silva\|first30=L.\|journal=The Astrophysical Journal Letters\|volume=920\|issue=2\|pages=L44\|arxiv=2107.09080\|bibcode=2021ApJ...920L..44C\|s2cid=236134310\|display-authors=1 \|doi-access=free }} \| −4.7 \| 14.72 \| align="center"\|Local Group \| Satellite of Milky Way \| 489 ly
26 \| align="center"\| \| Horologium II \| \| 0.254 \| 0.078{{cite journal\|bibcode=2018ApJ...867...19K\|title=The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies\|last1=Kallivayalil\|first1=Nitya\|last2=Sales\|first2=Laura V.\|last3=Zivick\|first3=Paul\|last4=Fritz\|first4=Tobias K.\|last5=Del Pino\|first5=Andrés\|last6=Sohn\|first6=Sangmo Tony\|last7=Besla\|first7=Gurtina\|last8=Van Der Marel\|first8=Roeland P.\|last9=Navarro\|first9=Julio F.\|last10=Sacchi\|first10=Elena\|journal=The Astrophysical Journal\|year=2018\|volume=867\|issue=1\|pages=19\|doi=10.3847/1538-4357/aadfee\|arxiv=1805.01448\|s2cid=55073922 \|doi-access=free }} \| −2.6 \| 1.69 \| align="center"\|Local Group \| Satellite of Milky Way \| 287 ly{{cite journal\|bibcode=2018ApJ...860...66M\|title=A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters\|last1=Muñoz\|first1=Ricardo R.\|last2=Côté\|first2=Patrick\|last3=Santana\|first3=Felipe A.\|last4=Geha\|first4=Marla\|author4-link= Marla Geha \|last5=Simon\|first5=Joshua D.\|last6=Oyarzún\|first6=Grecco A.\|last7=Stetson\|first7=Peter B.\|last8=Djorgovski\|first8=S. G.\|journal=The Astrophysical Journal\|year=2018\|volume=860\|issue=1\|pages=66\|doi=10.3847/1538-4357/aac16b\|arxiv=1806.06891 \|doi-access=free}}
27 \| align="center"\| 60px \| Draco Dwarf (DDO 208) \| dE0 pec \| 0.258 \| 0.079 \| −8.74 \| 10.9 \| align="center"\|Local Group \| Satellite of Milky Way with a large amount of dark matter \|data-sort-value="2700"\|~2,700 × 1,900 ly
27 \| \| Horologium I \| \| 0.258 \| 0.079{{cite journal\|doi=10.1088/0004-637X/811/1/62\|title=Kinematics and Chemistry of Recently Discovered Reticulum 2 and Horologium 1 Dwarf Galaxies\|year=2015\|last1=Koposov\|first1=Sergey E.\|last2=Casey\|first2=Andrew R.\|last3=Belokurov\|first3=Vasily\|last4=Lewis\|first4=James R.\|last5=Gilmore\|first5=Gerard\|last6=Worley\|first6=Clare\|last7=Hourihane\|first7=Anna\|last8=Randich\|first8=S.\|last9=Bensby\|first9=T.\|last10=Bragaglia\|first10=A.\|last11=Bergemann\|first11=M.\|last12=Carraro\|first12=G.\|last13=Costado\|first13=M. T.\|last14=Flaccomio\|first14=E.\|last15=Francois\|first15=P.\|last16=Heiter\|first16=U.\|last17=Hill\|first17=V.\|last18=Jofre\|first18=P.\|last19=Lando\|first19=C.\|last20=Lanzafame\|first20=A. C.\|last21=Laverny\|first21=P. de\|last22=Monaco\|first22=L.\|last23=Morbidelli\|first23=L.\|last24=Sbordone\|first24=L.\|last25=Mikolaitis\|first25=Š.\|last26=Ryde\|first26=N.\|journal=The Astrophysical Journal\|volume=811\|issue=1\|pages=62\|arxiv=1504.07916\|bibcode=2015ApJ...811...62K\|s2cid=53419855}} \| -3.4 \| \| align="center"\|Local Group \| Satellite of Milky Way \| 196 ly
29 \| align="center"\| \| Pisces Overdensity \| dIrr/dSph{{cite journal \| bibcode=2009ApJ...697.1993B \| doi=10.1088/0004-637X/697/2/1993 \| arxiv=0903.3871 \| title=Aspitzerstudy of Asymptotic Giant Branch Stars. Iii. Dust Production and Gas Return in Local Group Dwarf Irregular Galaxies \| journal=The Astrophysical Journal \| volume=697 \| issue=2 \| pages=1993–2014 \| year=2009 \| last1=Boyer \| first1=Martha L \| last2=Skillman \| first2=Evan D \| last3=Van Loon \| first3=Jacco Th \| last4=Gehrz \| first4=Robert D \| last5=Woodward \| first5=Charles E \| s2cid=12162514 }} \| 0.26 \| 0.08{{citation \| display-authors=1 \| last1=Watkins \| first1=L. L. \| last2=Evans \| first2=N. W. \| last3=Belokurov \| first3=V. \| last4=Smith \| first4=M. C. \| last5=Hewett \| first5=P. C. \| last6=Bramich \| first6=D. M. \| last7=Gilmore \| first7=G. F. \| last8=Irwin \| first8=M. J. \| last9=Vidrih \| first9=S. \| last10=Wyrzykowski \| first10=Ł. \| last11=Zucker \| first11=D. B. \| title=Substructure revealed by RR Lyraes in SDSS Stripe 82 \| date=2009 \| journal=Monthly Notices of the Royal Astronomical Society \| volume=398 \| issue=4 \| pages=1757–70 \| doi=10.1111/j.1365-2966.2009.15242.x \| doi-access=free \| bibcode=2009MNRAS.398.1757W \| arxiv=0906.0498 \| s2cid=14409027 \| postscript=. }} \| −10.35 \| \| align="center"\|Local Group \| Satellite of Milky Way \|
29 \| \| Leo Minor I \| \| 0.267 \| 0.082 \| −2.4 \| 17.16 \| align="center" \|Local Group \| Satellite of Milky Way \|
29 \| \| Aquarius III \| \| 0.277 \| 0.085{{cite journal\|doi=10.3847/1538-4357/ad8eba\|doi-access=free \|title=Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy \|date=2025 \|last1=Cerny \|first1=W. \|last2=Chiti \|first2=A. \|last3=Geha \|first3=M. \|last4=Mutlu-Pakdil \|first4=B. \|last5=Drlica-Wagner \|first5=A. \|last6=Tan \|first6=C. Y. \|last7=Adamów \|first7=M. \|last8=Pace \|first8=A. B. \|last9=Simon \|first9=J. D. \|last10=Sand \|first10=D. J. \|last11=Ji \|first11=A. P. \|last12=Li \|first12=T. S. \|last13=Vivas \|first13=A. K. \|last14=Bell \|first14=E. F. \|last15=Carlin \|first15=J. L. \|last16=Carballo-Bello \|first16=J. A. \|last17=Chaturvedi \|first17=A. \|last18=Choi \|first18=Y. \|last19=Doliva-Dolinsky \|first19=A. \|last20=Gnedin \|first20=O. Y. \|last21=Limberg \|first21=G. \|last22=Martínez-Vázquez \|first22=C. E. \|last23=Mau \|first23=S. \|last24=Medina \|first24=G. E. \|last25=Navabi \|first25=M. \|last26=Noël \|first26=N. E. D. \|last27=Placco \|first27=V. M. \|last28=Riley \|first28=A. H. \|last29=Roederer \|first29=I. U. \|last30=Stringfellow \|first30=G. S. \|journal=The Astrophysical Journal \|volume=979 \|issue=2 \|page=164 \|arxiv=2410.00981 \|bibcode=2025ApJ...979..164C \|display-authors=1 }} \| −2.5 \| \| align="center" \| Local Group \| Satellite of the Milky Way \| 330 ly
30 \| \|Sextans Dwarf Sph \| dSph \| 0.280 \| 0.086 \| −7.98 \| 12 \| align="center" \|Local Group \| Satellite of Milky Way \|8,400 ly
31 \| align="center" \|60px \|Sculptor Dwarf (ESO 351-G30) \| dE3 \| 0.287 \| 0.088 \| −9.77 \| 10.1 \| align="center" \|Local Group \| Satellite of Milky Way \|
32 \| align="center" \| \| Pegasus IV \| \| 0.294 \| 0.090{{cite journal \| arxiv=2203.11788 \| doi=10.3847/1538-4357/aca1c3 \| title=Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus \| year=2023 \| last1=Cerny \| first1=W. \| last2=Simon \| first2=J. D. \| last3=Li \| first3=T. S. \| last4=Drlica-Wagner \| first4=A. \| last5=Pace \| first5=A. B. \| last6=Martínez-Vázquez \| first6=C. E. \| last7=Riley \| first7=A. H. \| last8=Mutlu-Pakdil \| first8=B. \| last9=Mau \| first9=S. \| last10=Ferguson \| first10=P. S. \| last11=Erkal \| first11=D. \| last12=Munoz \| first12=R. R. \| last13=Bom \| first13=C. R. \| last14=Carlin \| first14=J. L. \| last15=Carollo \| first15=D. \| last16=Choi \| first16=Y. \| last17=Ji \| first17=A. P. \| last18=Manwadkar \| first18=V. \| last19=Martínez-Delgado \| first19=D. \| last20=Miller \| first20=A. E. \| last21=Noël \| first21=N. E. D. \| last22=Sakowska \| first22=J. D. \| last23=Sand \| first23=D. J. \| last24=Stringfellow \| first24=G. S. \| last25=Tollerud \| first25=E. J. \| last26=Vivas \| first26=A. K. \| last27=Carballo-Bello \| first27=J. A. \| last28=Hernandez-Lang \| first28=D. \| last29=James \| first29=D. J. \| last30=Nidever \| first30=D. L. \| journal=The Astrophysical Journal \| volume=942 \| issue=2 \| page=111 \| bibcode=2023ApJ...942..111C \| s2cid=247597301 \| display-authors=1 \| doi-access=free }} \| −4.25 \| 15.52 \| align="center" \|Local Group \| Satellite of Milky Way \|
32 \| align="center" \| \| Virgo I \| \| 0.297 \| 0.091 \| −0.3 \| 19.5 \| align="center" \|Local Group \| Satellite of Milky Way \|
33 \| align="center"\| \| Reticulum III \| \| 0.300 \| 0.092{{cite journal\|doi=10.1088/0004-637X/813/2/109\|title=Eight Ultra-Faint Galaxy Candidates Discovered in Year Two of the Dark Energy Survey\|year=2015\|last1=Drlica-Wagner\|first1=A.\|last2=Bechtol\|first2=K.\|last3=Rykoff\|first3=E. S.\|last4=Luque\|first4=E.\|last5=Queiroz\|first5=A.\|last6=Mao\|first6=Y.-Y.\|last7=Wechsler\|first7=R. H.\|last8=Simon\|first8=J. D.\|last9=Santiago\|first9=B.\|last10=Yanny\|first10=B.\|last11=Balbinot\|first11=E.\|last12=Dodelson\|first12=S.\|last13=Neto\|first13=A. Fausti\|last14=James\|first14=D. J.\|last15=Li\|first15=T. S.\|last16=Maia\|first16=M. A. G.\|last17=Marshall\|first17=J. L.\|last18=Pieres\|first18=A.\|last19=Stringer\|first19=K.\|last20=Walker\|first20=A. R.\|last21=Abbott\|first21=T. M. C.\|last22=Abdalla\|first22=F. B.\|last23=Allam\|first23=S.\|last24=Benoit-Lévy\|first24=A.\|last25=Bernstein\|first25=G. M.\|last26=Bertin\|first26=E.\|last27=Brooks\|first27=D.\|last28=Buckley-Geer\|first28=E.\|author28-link=Elizabeth Buckley-Geer\|last29=Burke\|first29=D. L.\|last30=Rosell\|first30=A. Carnero\|journal=The Astrophysical Journal\|volume=813\|issue=2\|pages=109\|arxiv=1508.03622\|bibcode=2015ApJ...813..109D\|s2cid=55909299\|display-authors=29}} \| −3.3 \| 16.51 \| align="center"\|Local Group \| Satellite of Milky Way \| 420 ly
34 \| \|Ursa Major I Dwarf (UMa I dSph) \| dSph \| 0.3157 \| 0.0968 \| −6.75Willman, Dalcanton, Martinez-Delgado, et al. (2005) "A New Milky Way Dwarf Galaxy in Ursa Major", submitted to Astrophysical Journal Letters, on arXiv.org: [https://arxiv.org/abs/astro-ph/0503552 astro-ph/0503552] {{Webarchive\|url=https://web.archive.org/web/20151212194857/http://arxiv.org/abs/astro-ph/0503552 \|date=2015-12-12 }} \| \| align="center" \|Local Group \| Satellite of Milky Way \|~2,000 ly
35 \| align="center" \| \| Phoenix II \| \| 0.326 \| 0.100{{cite journal\|doi=10.1093/mnras/stz2609\|title=Search for RR Lyrae stars in DES ultra-faint systems: Grus I, Kim 2, Phoenix II, and Grus II\|year=2019\|last1=Martínez-Vázquez\|first1=C. E.\|last2=Vivas\|first2=A. K.\|last3=Gurevich\|first3=M.\|last4=Walker\|first4=A. R.\|last5=McCarthy\|first5=M.\|last6=Pace\|first6=A. B.\|last7=Stringer\|first7=K. M.\|last8=Santiago\|first8=B.\|last9=Hounsell\|first9=R.\|last10=Macri\|first10=L.\|last11=Li\|first11=T. S.\|last12=Bechtol\|first12=K.\|last13=Riley\|first13=A. H.\|last14=Kim\|first14=A. G.\|last15=Simon\|first15=J. D.\|last16=Drlica-Wagner\|first16=A.\|last17=Nadler\|first17=E. O.\|last18=Marshall\|first18=J. L.\|last19=Annis\|first19=J.\|last20=Avila\|first20=S.\|last21=Bertin\|first21=E.\|last22=Brooks\|first22=D.\|last23=Buckley-Geer\|first23=E.\|last24=Burke\|first24=D. L.\|last25=Rosell\|first25=A Carnero\|last26=Kind\|first26=M Carrasco\|last27=Da Costa\|first27=L. N.\|last28=De Vicente\|first28=J.\|last29=Desai\|first29=S.\|last30=Diehl\|first30=H. T.\|journal=Monthly Notices of the Royal Astronomical Society\|volume=490\|issue=2\|pages=2183\|doi-access=free \|arxiv=1909.06308\|bibcode=2019MNRAS.490.2183M\|display-authors=29}} \| −2.7 \| \| align="center" \|Local Group \| Satellite of Milky Way \| 290 ly
36 \|60px \| Carina Dwarf (ESO 206-G220) \| dE3 \| 0.33 \| 0.10 \| −8.97 \| 11.3 \| align="center" \|Local Group \| Satellite of Milky Way \| 1,600 ly
36 \| \| Boötes V \| \| 0.333 \| 0.102{{cite journal\|doi=10.3847/1538-4357/acdd78\|doi-access=free \|title=Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey \|date=2023 \|last1=Cerny \|first1=W. \|last2=Martínez-Vázquez \|first2=C. E. \|last3=Drlica-Wagner \|first3=A. \|last4=Pace \|first4=A. B. \|last5=Mutlu-Pakdil \|first5=B. \|last6=Li \|first6=T. S. \|last7=Riley \|first7=A. H. \|last8=Crnojević \|first8=D. \|last9=Bom \|first9=C. R. \|last10=Carballo-Bello \|first10=J. A. \|last11=Carlin \|first11=J. L. \|last12=Chiti \|first12=A. \|last13=Choi \|first13=Y. \|last14=Collins \|first14=M. L. M. \|last15=Darragh-Ford \|first15=E. \|last16=Ferguson \|first16=P. S. \|last17=Geha \|first17=M. \|last18=Martínez-Delgado \|first18=D. \|last19=Massana \|first19=P. \|last20=Mau \|first20=S. \|last21=Medina \|first21=G. E. \|last22=Muñoz \|first22=R. R. \|last23=Nadler \|first23=E. O. \|last24=Noël \|first24=N. E. D. \|last25=Olsen \|first25=K. A. G. \|last26=Pieres \|first26=A. \|last27=Sakowska \|first27=J. D. \|last28=Simon \|first28=J. D. \|last29=Stringfellow \|first29=G. S. \|last30=Tollerud \|first30=E. J. \|journal=The Astrophysical Journal \|volume=953 \|issue=1 \|page=1 \|arxiv=2209.12422 \|bibcode=2023ApJ...953....1C \|display-authors=1 }} \| −3.2 \| 16.84 \| align="center" \|Local Group \| Satellite of Milky Way \|
37 \| align="center" \| \| Aquarius II \| \| 0.3519 \| 0.1079{{cite journal\|doi=10.1093/mnras/stw2051\|title=At the survey limits: Discovery of the Aquarius 2 dwarf galaxy in the VST ATLAS and the SDSS data\|year=2016\|last1=Torrealba\|first1=G.\|last2=Koposov\|first2=S. E.\|last3=Belokurov\|first3=V.\|last4=Irwin\|first4=M.\|last5=Collins\|first5=M.\|last6=Spencer\|first6=M.\|last7=Ibata\|first7=R.\|last8=Mateo\|first8=M.\|last9=Bonaca\|first9=A.\|last10=Jethwa\|first10=P.\|journal=Monthly Notices of the Royal Astronomical Society\|volume=463\|issue=1\|pages=712–722\|doi-access=free \|arxiv=1605.05338\|bibcode=2016MNRAS.463..712T}} \| −4.36 \| 15.8 \| align="center" \|Local Group \| Satellite of Milky Way \| 1,040 ly
38 \| \| Leo VI \| \| 0.362 \| 0.111{{cite journal\|doi=10.3847/1538-4357/ad9b0c\|doi-access=free \|title=A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Ultra-faint Dwarf Galaxy with DELVE Early Data Release 3 \|date=2025 \|last1=Tan \|first1=C. Y. \|last2=Cerny \|first2=W. \|last3=Drlica-Wagner \|first3=A. \|last4=Pace \|first4=A. B. \|last5=Geha \|first5=M. \|last6=Ji \|first6=A. P. \|last7=Li \|first7=T. S. \|last8=Adamów \|first8=M. \|last9=Anbajagane \|first9=D. \|last10=Bom \|first10=C. R. \|last11=Carballo-Bello \|first11=J. A. \|last12=Carlin \|first12=J. L. \|last13=Chang \|first13=C. \|last14=Chaturvedi \|first14=A. \|last15=Chiti \|first15=A. \|last16=Choi \|first16=Y. \|last17=Collins \|first17=M. L. M. \|last18=Doliva-Dolinsky \|first18=A. \|last19=Ferguson \|first19=P. S. \|last20=Gruendl \|first20=R. A. \|last21=James \|first21=D. J. \|last22=Limberg \|first22=G. \|last23=Navabi \|first23=M. \|last24=Martínez-Delgado \|first24=D. \|last25=Martínez-Vázquez \|first25=C. E. \|last26=Medina \|first26=G. E. \|last27=Mutlu-Pakdil \|first27=B. \|last28=Nidever \|first28=D. L. \|last29=Noël \|first29=N. E. D. \|last30=Riley \|first30=A. H. \|journal=The Astrophysical Journal \|volume=979 \|issue=2 \|page=176 \|arxiv=2408.00865 \|bibcode=2025ApJ...979..176T \|display-authors=1 }} \| −3.56 \| \| align="center" \|Local Group \| Satellite of Milky Way \| 910 ly
38 \| align="center" \| \| Pictor I \| \| 0.372 \| 0.114{{cite journal\|bibcode=2015ApJ...805..130K\|title=Beasts of the Southern Wild: Discovery of Nine Ultra Faint Satellites in the Vicinity of the Magellanic Clouds\|last1=Koposov\|first1=Sergey E.\|last2=Belokurov\|first2=Vasily\|last3=Torrealba\|first3=Gabriel\|last4=Evans\|first4=N. Wyn\|journal=The Astrophysical Journal\|year=2015\|volume=805\|issue=2\|pages=130\|doi=10.1088/0004-637X/805/2/130\|arxiv=1503.02079\|s2cid=118267222}} \| −3.1 \| 20.3 \| align="center" \|Local Group \| Satellite of Milky Way \| 190 ly
39 \| align="center" \| \|Crater II \| \| 0.383 \| 0.1175 \| −8.2 \| 12.2 \| align="center" \|Local Group \| Satellite of Milky Way \|
40 \| align="center" \| \| Grus I \| \| 0.391 \| 0.120 \| −3.4 \| 17.0 \| align="center" \|Local Group \| Satellite of Milky Way \| 404 ly
41 \| align="center" \| \| Sextans II \| \| 0.411 \| 0.126{{cite journal \| last1=Homma \| first1=Daisuke \| last2=Chiba \| first2=Masashi \| last3=Komiyama \| first3=Yutaka \| last4=Tanaka \| first4=Masayuki \| last5=Okamoto \| first5=Sakurako \| last6=Tanaka \| first6=Mikito \| last7=Ishigaki \| first7=Miho N \| last8=Hayashi \| first8=Kohei \| last9=Arimoto \| first9=Nobuo \| last10=Lupton \| first10=Robert H \| last11=Strauss \| first11=Michael A \| last12=Miyazaki \| first12=Satoshi \| last13=Wang \| first13=Shiang-Yu \| last14=Murayama \| first14=Hitoshi \| title=Final results of the search for new Milky Way satellites in the Hyper Suprime-Cam Subaru Strategic Program survey: Discovery of two more candidates \| journal=Publications of the Astronomical Society of Japan \| date=2024-06-08 \| volume=76 \| issue=4 \| pages=733–752 \| issn=0004-6264 \| doi=10.1093/pasj/psae044\| arxiv=2311.05439 }} \|−3.9 \| \| align="center" \|Local Group \| Satellite of Milky Way \|
41 \| align="center" \| \| Antlia 2 \| \| 0.430 \| 0.1318{{cite journal\|doi=10.3847/1538-4357/ac1869\|title=Kinematics of Antlia 2 and Crater 2 from the Southern Stellar Stream Spectroscopic Survey (S 5)\|year=2021\|last1=Ji\|first1=Alexander P.\|last2=Koposov\|first2=Sergey E.\|last3=Li\|first3=Ting S.\|last4=Erkal\|first4=Denis\|last5=Pace\|first5=Andrew B.\|last6=Simon\|first6=Joshua D.\|last7=Belokurov\|first7=Vasily\|last8=Cullinane\|first8=Lara R.\|last9=Da Costa\|first9=Gary S.\|last10=Kuehn\|first10=Kyler\|last11=Lewis\|first11=Geraint F.\|last12=MacKey\|first12=Dougal\|last13=Shipp\|first13=Nora\|last14=Simpson\|first14=Jeffrey D.\|last15=Zucker\|first15=Daniel B.\|last16=Hansen\|first16=Terese T.\|last17=Bland-Hawthorn\|first17=Joss\|author18=S5 Collaboration\|journal=The Astrophysical Journal\|volume=921\|issue=1\|page=32\|arxiv=2106.12656\|bibcode=2021ApJ...921...32J\|s2cid=235624056 \|doi-access=free }} \| −9.86 \| \| align="center" \|Local Group \| Satellite of Milky Way, most diffuse galaxy ever found \|
42 \| align="center" \|60px \| Hercules Dwarf \| dSph \| 0.434 \| 0.133{{cite journal\|last=Sand\|first=David J.\|author2=Olszewski, Edward W. \|author3=Willman, Beth \|title=The Star Formation History and Extended Structure of the Hercules Milky Way Satellite\|date=2009\|journal=The Astrophysical Journal\|volume=704\|issue=2\|pages=898–914\|doi=10.1088/0004-637X/704/2/898\|bibcode=2009ApJ...704..898S \|arxiv=0906.4017 \|s2cid=42754875}} \| −5.3 \| 14.7 \| align="center" \|Local Group \| Satellite of Milky Way \|
43 \| align="center" \|60px \|Fornax Dwarf (ESO 356-G04) \| dSph/E2 \| 0.466 \| 0.143{{cite journal\|doi=10.3847/1538-4357/ac5b07\|title=Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal \|year=2022 \|last1=Oakes \|first1=Elias K. \|last2=Hoyt \|first2=Taylor J. \|last3=Freedman \|first3=Wendy L. \|last4=Madore \|first4=Barry F. \|last5=Tran \|first5=Quang H. \|last6=Cerny \|first6=William \|last7=Beaton \|first7=Rachael L. \|last8=Seibert \|first8=Mark \|journal=The Astrophysical Journal \|volume=929 \|issue=2 \|page=116 \|arxiv=2204.09699 \|bibcode=2022ApJ...929..116O \|s2cid=248260222 \|doi-access=free }} \| −11.5 \| 9.28 \| align="center" \|Local Group \| Satellite of Milky Way \|
44 \| align="center" \| \|Canes Venatici II Dwarf \| dSph \| 0.49 \| 0.15 \| −4.8 \| 15.1{{Cite journal \| last1 = Belokurov \| first1 = V. \| last2 = Zucker \| first2 = D. B. \| last3 = Evans \| first3 = N. W. \| last4 = Kleyna \| first4 = J. T. \| last5 = Koposov \| first5 = S. \| last6 = Hodgkin \| first6 = S. T. \| last7 = Irwin \| first7 = M. J. \| last8 = Gilmore \| first8 = G. \|author-link8 = Gerard F. Gilmore\| last9 = Wilkinson \| first9 = M. I. \| last10 = Fellhauer \| doi = 10.1086/509718 \| first10 = M. \| last11 = Bramich \| first11 = D. M. \| last12 = Hewett \| first12 = P. C. \| last13 = Vidrih \| first13 = S. \| last14 = De Jong \| first14 = J. T. A. \| last15 = Smith \| first15 = J. A. \| last16 = Rix \| first16 = H. -W. \| last17 = Bell \| first17 = E. F. \| last18 = Wyse \| first18 = R. F. G. \| last19 = Newberg \| first19 = H. J. \| last20 = Mayeur \| first20 = P. A. \| last21 = Yanny \| first21 = B. \| last22 = Rockosi \| first22 = C. M. \|author-link22=Constance M. Rockosi\| last23 = Gnedin \| first23 = O. Y. \| last24 = Schneider \| first24 = D. P. \| last25 = Beers \| first25 = T. C. \| last26 = Barentine \| first26 = J. C. \| last27 = Brewington \| first27 = H. \| last28 = Brinkmann \| first28 = J. \| last29 = Harvanek \| first29 = M. \| last30 = Kleinman \| first30 = S. J. \| title = Cats and Dogs, Hair and a Hero: A Quintet of New Milky Way Companions \| journal = The Astrophysical Journal \| volume = 654 \| issue = 2 \| pages = 897–906 \| year = 2007 \|arxiv = astro-ph/0608448 \|bibcode = 2007ApJ...654..897B \| s2cid = 18617277 }} \| align="center" \|Local Group \| Satellite of Milky Way \|
45 \| align="center" \| \| Hydra II \| dSph \| 0.492 \| 0.151{{cite journal\|bibcode=2016AJ....151..118V\|title=Variable Stars in the Field of the Hydra II Ultra-faint Dwarf Galaxy\|last1=Vivas\|first1=A. Katherina\|last2=Olsen\|first2=Knut\|last3=Blum\|first3=Robert\|last4=Nidever\|first4=David L.\|last5=Walker\|first5=Alistair R.\|last6=Martin\|first6=Nicolas F.\|last7=Besla\|first7=Gurtina\|last8=Gallart\|first8=Carme\|last9=Van Der Marel\|first9=Roeland P.\|last10=Majewski\|first10=Steven R.\|last11=Kaleida\|first11=Catherine C.\|last12=Muñoz\|first12=Ricardo R.\|last13=Saha\|first13=Abhijit\|last14=Conn\|first14=Blair C.\|last15=Jin\|first15=Shoko\|journal=The Astronomical Journal\|year=2016\|volume=151\|issue=5\|pages=118\|doi=10.3847/0004-6256/151/5/118\|arxiv=1510.05539\|s2cid=53536842 \|doi-access=free }} \| −5.1 \| \| align="center" \|Local Group \| Satellite of Milky Way \| 500 ly
45 \| align="center" \| \| Virgo III \| \| 0.492 \| 0.151 \| −2.7 \| \| align="center" \|Local Group \| Satellite of Milky Way \|
46 \| align="center" \|60px \| Leo IV Dwarf \| dSph \| 0.502 \| 0.154{{cite journal\|last1=Sand\|first1=David J. \|last2=Seth\|first2=Anil \|last3=Olszewski\|first3=Edward W. \|display-authors=etal \|title=A Deeper Look at Leo IV: Star Formation History and Extended Structure\|date=2010\|journal=The Astrophysical Journal\|volume=718\|issue=1 \|pages=530–42 \|bibcode=2010ApJ...718..530S\|doi=10.1088/0004-637X/718/1/530\|arxiv=0911.5352\|s2cid=32122744 }} \| −5.5 \| 15.9 \| align="center" \|Local Group \| Satellite of Milky Way \|
47 \| align="center" \| \| Leo V Dwarf \| dSph \| 0.571 \| 0.175{{Cite journal \| last1 = de Jong \| first1 = J. T. A. \| last2 = Martin \| first2 = N. F. \| last3 = Rix \| first3 = H. W. \| last4 = Smith \| first4 = K. W. \| last5 = Jin \| first5 = S. \| last6 = Macciò \| first6 = A. V. \| doi = 10.1088/0004-637X/710/2/1664 \| title = The Enigmatic Pair of Dwarf Galaxies Leo Iv and Leo V: Coincidence or Common Origin? \| journal = The Astrophysical Journal \| volume = 710 \| issue = 2 \| pages = 1664–1671 \| year = 2010 \|arxiv = 0912.3251 \|bibcode = 2010ApJ...710.1664D \| s2cid = 5667891 }} \| −5.2 \| \| align="center" \|Local Group \| Satellite of Milky Way \|
48 \| align="center" \| \| Pisces II \| dG{{cite journal\|bibcode=2012ApJ...756...79S\|doi=10.1088/0004-637X/756/1/79\|arxiv=1111.6608\|title=Tidal Signatures in the Faintest Milky Way Satellites: The Detailed Properties of Leo V, Pisces II, and Canes Venatici II\|journal=The Astrophysical Journal\|volume=756\|pages=79\|year=2012\|last1=Sand\|first1=David J\|last2=Strader\|first2=Jay\|last3=Willman\|first3=Beth\|last4=Zaritsky\|first4=Dennis\|last5=McLeod\|first5=Brian\|last6=Caldwell\|first6=Nelson\|last7=Seth\|first7=Anil\|last8=Olszewski\|first8=Edward\|issue=1\|s2cid=46030862}} \| 0.597 \| 0.183 \| −4.28 \| 17.03 \| align="center" \|Local Group \| Satellite of Milky Way \|
48 \| align="center"\| \| Columba I \| \| 0.597 \| 0.183{{cite journal\|bibcode=2017AJ....154..267C\|title=Deep Subaru Hyper Suprime-Cam Observations of Milky Way Satellites Columba I and Triangulum II\|last1=Carlin\|first1=Jeffrey L.\|last2=Sand\|first2=David J.\|last3=Muñoz\|first3=Ricardo R.\|last4=Spekkens\|first4=Kristine\|last5=Willman\|first5=Beth\|last6=Crnojević\|first6=Denija\|last7=Forbes\|first7=Duncan A.\|last8=Hargis\|first8=Jonathan\|last9=Kirby\|first9=Evan\|last10=Peter\|first10=Annika H. G.\|last11=Romanowsky\|first11=Aaron J.\|last12=Strader\|first12=Jay\|journal=The Astronomical Journal\|year=2017\|volume=154\|issue=6\|pages=267\|doi=10.3847/1538-3881/aa94d0\|arxiv=1710.06444\|s2cid=54537259 \|doi-access=free }} \| −4.2 \| 17.11 \| align="center"\|Local Group \| Satellite of Milky Way \| 760 ly
50 \| align="center"\| \| Boötes IV \| \| 0.682 \| 0.209{{cite journal\|doi=10.1093/pasj/psz076\|title=Boötes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem\|year=2019\|last1=Homma\|first1=Daisuke\|last2=Chiba\|first2=Masashi\|last3=Komiyama\|first3=Yutaka\|last4=Tanaka\|first4=Masayuki\|last5=Okamoto\|first5=Sakurako\|last6=Tanaka\|first6=Mikito\|last7=Ishigaki\|first7=Miho N.\|last8=Hayashi\|first8=Kohei\|last9=Arimoto\|first9=Nobuo\|last10=Carlsten\|first10=Scott G.\|last11=Lupton\|first11=Robert H.\|last12=Strauss\|first12=Michael A.\|last13=Miyazaki\|first13=Satoshi\|last14=Torrealba\|first14=Gabriel\|last15=Wang\|first15=Shiang-Yu\|last16=Murayama\|first16=Hitoshi\|journal=Publications of the Astronomical Society of Japan\|volume=71\|issue=5\|pages=94\|arxiv=1906.07332\|bibcode=2019PASJ...71...94H}} \| −4.53 \| 17.07 \| align="center"\|Local Group \| Satellite of Milky Way \| 3,000 ly
51 \| align="center" \|60px \| Leo II Dwarf (Leo B, DDO 93) \| dE0 pec \| 0.701van den Bergh, S. (2000)Updated Information on the Local Group \| 0.215 \| −9.23 \| 12.45 \| align="center" \|Local Group \| Satellite of Milky Way \|4,100 ly (tidal)
51 \| align="center" \| \| Pegasus III \| \| 0.701 \| 0.215{{cite journal\|bibcode=2016ApJ...833...16K\|title=Portrait of a Dark Horse: A Photometric and Spectroscopic Study of the Ultra-faint Milky Way Satellite Pegasus III\|last1=Kim\|first1=Dongwon\|last2=Jerjen\|first2=Helmut\|last3=Geha\|first3=Marla\|author3-link= Marla Geha \|last4=Chiti\|first4=Anirudh\|last5=Milone\|first5=Antonino P.\|last6=Da Costa\|first6=Gary\|last7=MacKey\|first7=Dougal\|last8=Frebel\|first8=Anna\|last9=Conn\|first9=Blair\|journal=The Astrophysical Journal\|year=2016\|volume=833\|issue=1\|pages=16\|doi=10.3847/0004-637X/833/1/16\|arxiv=1608.04934\|s2cid=73677994 \|doi-access=free }} \| −4.17 \| 17.50{{cite journal\|doi=10.3847/1538-4357/ac7226\|title=Structural Parameters and Possible Association of the Ultra-faint Dwarfs Pegasus III and Pisces II from Deep Hubble Space Telescope Photometry \|year=2022 \|last1=Richstein \|first1=Hannah \|last2=Patel \|first2=Ekta \|last3=Kallivayalil \|first3=Nitya \|last4=Simon \|first4=Joshua D. \|last5=Zivick \|first5=Paul \|last6=Tollerud \|first6=Erik \|last7=Fritz \|first7=Tobias \|last8=Warfield \|first8=Jack T. \|last9=Besla \|first9=Gurtina \|last10=Van Der Marel \|first10=Roeland P. \|last11=Wetzel \|first11=Andrew \|last12=Choi \|first12=Yumi \|last13=Deason \|first13=Alis \|last14=Geha \|first14=Marla\|author14-link= Marla Geha \|last15=Guhathakurta \|first15=Puragra \|last16=Jeon \|first16=Myoungwon \|last17=Kirby \|first17=Evan N. \|last18=Libralato \|first18=Mattia \|last19=Sacchi \|first19=Elena \|last20=Sohn \|first20=Sangmo Tony \|journal=The Astrophysical Journal \|volume=933 \|issue=2 \|page=217 \|arxiv=2204.01917 \|bibcode=2022ApJ...933..217R \|s2cid=247957904 \|doi-access=free }} \| align="center" \|Local Group \| Satellite of Milky Way \| 350 ly
53 \| align="center" \| \| Canes Venatici I Dwarf \| dSph \| 0.711 \| 0.218{{Cite journal \| last1 = Martin \| first1 = N. F. \| last2 = Coleman \| first2 = M. G. \| last3 = De Jong \| first3 = J. T. A. \| last4 = Rix \| first4 = H. W. \| last5 = Bell \| first5 = E. F. \| last6 = Sand \| first6 = D. J. \| last7 = Hill \| first7 = J. M. \| last8 = Thompson \| first8 = D. \| last9 = Burwitz \| first9 = V. \| last10 = Giallongo \| first10 = E. \| last11 = Ragazzoni \| first11 = R. \| last12 = Diolaiti \| first12 = E. \| last13 = Gasparo \| first13 = F. \| last14 = Grazian \| first14 = A. \| last15 = Pedichini \| first15 = F. \| last16 = Bechtold \| first16 = J. \| title = A Deep Large Binocular Telescope View of the Canes Venatici I Dwarf Galaxy \| doi = 10.1086/525559 \| journal = The Astrophysical Journal \| volume = 672 \| pages = L13–L16 \| year = 2008 \| issue = 1 \|arxiv = 0709.3365 \|bibcode = 2008ApJ...672L..13M \| s2cid = 14614201 }} \| −7.9 \| 13.9{{Cite journal \| last1 = Zucker \| first1 = D. B. \| last2 = Belokurov \| first2 = V. \| last3 = Evans \| first3 = N. W. \| last4 = Wilkinson \| first4 = M. I. \| last5 = Irwin \| first5 = M. J. \| last6 = Sivarani \| first6 = T. \| last7 = Hodgkin \| first7 = S. \| last8 = Bramich \| first8 = D. M. \| last9 = Irwin \| first9 = J. M. \| last10 = Gilmore \| doi = 10.1086/505216 \| first10 = G. \| last11 = Willman \| first11 = B. \| last12 = Vidrih \| first12 = S. \| last13 = Fellhauer \| first13 = M. \| last14 = Hewett \| first14 = P. C. \| last15 = Beers \| first15 = T. C. \| last16 = Bell \| first16 = E. F. \| last17 = Grebel \| first17 = E. K. \| last18 = Schneider \| first18 = D. P. \| last19 = Newberg \| first19 = H. J. \| last20 = Wyse \| first20 = R. F. G. \| last21 = Rockosi \| first21 = C. M. \|author-link21=Constance M. Rockosi\| last22 = Yanny \| first22 = B. \| last23 = Lupton \| first23 = R. \| last24 = Smith \| first24 = J. A. \| last25 = Barentine \| first25 = J. C. \| last26 = Brewington \| first26 = H. \| last27 = Brinkmann \| first27 = J. \| last28 = Harvanek \| first28 = M. \| last29 = Kleinman \| first29 = S. J. \| last30 = Krzesinski \| first30 = J. \| title = A New Milky Way Dwarf Satellite in Canes Venatici \| journal = The Astrophysical Journal \| volume = 643 \| issue = 2 \| pages = L103 \| year = 2006 \|arxiv = astro-ph/0604354 \|bibcode = 2006ApJ...643L.103Z \| s2cid = 119421888 }} \| align="center" \|Local Group \| Satellite of Milky Way \|
54 \| align="center" \| \| Cetus III \| \| 0.819 \| 0.251{{cite journal\|doi=10.1093/pasj/psx050\|title=Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III\|year=2018\|last1=Homma\|first1=Daisuke\|last2=Chiba\|first2=Masashi\|last3=Okamoto\|first3=Sakurako\|last4=Komiyama\|first4=Yutaka\|last5=Tanaka\|first5=Masayuki\|last6=Tanaka\|first6=Mikito\|last7=Ishigaki\|first7=Miho N.\|last8=Hayashi\|first8=Kohei\|last9=Arimoto\|first9=Nobuo\|last10=Garmilla\|first10=José A.\|last11=Lupton\|first11=Robert H.\|last12=Strauss\|first12=Michael A.\|last13=Miyazaki\|first13=Satoshi\|last14=Wang\|first14=Shiang-Yu\|last15=Murayama\|first15=Hitoshi\|journal=Publications of the Astronomical Society of Japan\|volume=70\|pages=S18\|arxiv=1704.05977\|bibcode=2018PASJ...70S..18H}} \| −2.45 \| 19.55 \| align="center" \|Local Group \| Satellite of Milky Way \| 580 ly
55 \| align="center" \|60px \| Leo I Dwarf (DDO 74, UGC 5470) \| dE3 \| 0.820 \| 0.251 \| −10.97 \| 11.18 \| align="center" \|Local Group \| Satellite of Milky Way \|
56 \| align="center" \| \| Eridanus II \| \| 1.19 \| 0.366{{cite journal\|doi=10.3847/1538-4357/aa6113\|title=Farthest Neighbor: The Distant Milky Way Satellite Eridanus II\|year=2017\|last1=Li\|first1=T. S.\|last2=Simon\|first2=J. D.\|last3=Drlica-Wagner\|first3=A.\|last4=Bechtol\|first4=K.\|last5=Wang\|first5=M. Y.\|last6=García-Bellido\|first6=J.\|last7=Frieman\|first7=J.\|last8=Marshall\|first8=J. L.\|last9=James\|first9=D. J.\|last10=Strigari\|first10=L.\|last11=Pace\|first11=A. B.\|last12=Balbinot\|first12=E.\|last13=Zhang\|first13=Y.\|last14=Abbott\|first14=T. M. C.\|last15=Allam\|first15=S.\|last16=Benoit-Lévy\|first16=A.\|last17=Bernstein\|first17=G. M.\|last18=Bertin\|first18=E.\|last19=Brooks\|first19=D.\|last20=Burke\|first20=D. L.\|last21=Rosell\|first21=A. Carnero\|last22=Kind\|first22=M. Carrasco\|last23=Carretero\|first23=J.\|last24=Cunha\|first24=C. E.\|last25=d'Andrea\|first25=C. B.\|last26=Costa\|first26=L. N. da\|last27=Depoy\|first27=D. L.\|last28=Desai\|first28=S.\|last29=Diehl\|first29=H. T.\|last30=Eifler\|first30=T. F.\|journal=The Astrophysical Journal\|volume=838\|issue=1\|pages=8\|arxiv=1611.05052\|bibcode=2017ApJ...838....8L\|s2cid=45137837\|display-authors=29 \|doi-access=free }} \| −7.1 \| \| align="center" \|Local Group \| Satellite of Milky Way \| 1,810 ly
57 \| \| Leo T Dwarf \| dIrr/dSph \| 1.35 \| 0.413{{cite journal\|doi=10.1093/mnras/stab002\|arxiv=2101.03189\|bibcode=2021MNRAS.503..176H\|title=Solo dwarfs II: The stellar structure of isolated Local Group dwarf galaxies\|year=2021\|last1=Higgs\|first1=C. R.\|last2=McConnachie\|first2=A. W.\|last3=Annau\|first3=N.\|last4=Irwin\|first4=M.\|last5=Battaglia\|first5=G.\|last6=Côté\|first6=P.\|last7=Lewis\|first7=G. F.\|last8=Venn\|first8=K.\|journal=Monthly Notices of the Royal Astronomical Society\|volume=503\|issue=1 \|pages=176–199\|doi-access=free }} \| \| 16 \| align="center" \|Local Group \| Satellite of Milky Way? \|2,300 ly
58 \| \|Leo K \| \| 1.42 \| 0.434 \| −4.86{{cite journal\|doi=10.3847/1538-4357/ad429b\|doi-access=free \|title=Discovery and Characterization of Two Ultrafaint Dwarfs outside the Halo of the Milky Way: Leo M and Leo K \|date=2024 \|last1=McQuinn \|first1=Kristen. B. W. \|last2=Mao \|first2=Yao-Yuan \|last3=Tollerud \|first3=Erik J. \|last4=Cohen \|first4=Roger E. \|last5=Shih \|first5=David \|last6=Buckley \|first6=Matthew R. \|last7=Dolphin \|first7=Andrew E. \|journal=The Astrophysical Journal \|volume=967 \|issue=2 \|page=161 \|arxiv=2307.08738 \|bibcode=2024ApJ...967..161M }} \| \| align="center" \|Local Group \| Satellite of Milky Way \|
58 \|60px \|Phoenix Dwarf Galaxy (P 6830) \| IAm \| 1.44 \| 0.44 \| −10.22 \| 13.07 \| align="center" \|Local Group \| Satellite of Milky Way \|
58 \| \|Leo M \| \| 1.50 \| 0.459 \| −5.77 \| \| align="center" \|Local Group \| Satellite of Milky Way \|
59 \| align="center" \| \| Pisces V (Andromeda XVI) \| dSph{{cite journal\|bibcode=2017ApJ...837..102S\|title=The ISLAndS Project. II. The Lifetime Star Formation Histories of Six Andromeda DSPHS\|last1=Skillman\|first1=Evan D.\|last2=Monelli\|first2=Matteo\|last3=Weisz\|first3=Daniel R.\|last4=Hidalgo\|first4=Sebastian L.\|last5=Aparicio\|first5=Antonio\|last6=Bernard\|first6=Edouard J.\|last7=Boylan-Kolchin\|first7=Michael\|last8=Cassisi\|first8=Santi\|last9=Cole\|first9=Andrew A.\|last10=Dolphin\|first10=Andrew E.\|last11=Ferguson\|first11=Henry C.\|last12=Gallart\|first12=Carme\|last13=Irwin\|first13=Mike J.\|last14=Martin\|first14=Nicolas F.\|last15=Martínez-Vázquez\|first15=Clara E.\|last16=Mayer\|first16=Lucio\|last17=McConnachie\|first17=Alan W.\|last18=McQuinn\|first18=Kristen B. W.\|last19=Navarro\|first19=Julio F.\|last20=Stetson\|first20=Peter B.\|journal=The Astrophysical Journal\|year=2017\|volume=837\|issue=2\|pages=102\|doi=10.3847/1538-4357/aa60c5\|arxiv=1606.01207\|s2cid=53958697 \|doi-access=free }} \| 1.79 \| 0.55 \| −7.6 \| 16.1 \| align="center" \| Local Group \| Satellite of Andromeda \| 985 ly
60 \| align="center" \| 60px \|Barnard's Galaxy (NGC 6822) \| IB(s)m IV-V \| 1.859 \| 0.570 \| −15.22 \| 9.32 \| align="center" \|Local Group \| It contains several large H II regions \|7,000 ly
61 \| align="center" \| 60px \|NGC 185 \| dE3 pec \| 2.05 \| 0.63 \| −14.76 \| 9.99 \| align="center" \|Local Group \| Satellite of Andromeda; possibly closest Seyfert galaxy to Earth \|
62 \| align="center" \|60px \| Andromeda II \| dE0 \| 2.22 \| 0.68 \| −12.6 \| 11.7 \| align="center" \|Local Group \| Satellite of Andromeda \| 6,820 ly
63 \| align="center" \| \| Cassiopeia II (Andromeda XXX) \| dSph \| 2.221 \| 0.681 \| −8.0{{cite journal\|bibcode=2016ApJ...833..167M\|title=The PAndAS View of the Andromeda Satellite System. II. Detailed Properties of 23 M31 Dwarf Spheroidal Galaxies\|last1=Martin\|first1=Nicolas F.\|last2=Ibata\|first2=Rodrigo A.\|last3=Lewis\|first3=Geraint F.\|last4=McConnachie\|first4=Alan\|last5=Babul\|first5=Arif\|last6=Bate\|first6=Nicholas F.\|last7=Bernard\|first7=Edouard\|last8=Chapman\|first8=Scott C.\|last9=Collins\|first9=Michelle M. L.\|last10=Conn\|first10=Anthony R.\|last11=Crnojević\|first11=Denija\|last12=Fardal\|first12=Mark A.\|last13=Ferguson\|first13=Annette M. N.\|last14=Irwin\|first14=Michael\|last15=MacKey\|first15=A. Dougal\|last16=McMonigal\|first16=Brendan\|last17=Navarro\|first17=Julio F.\|last18=Rich\|first18=R. Michael\|journal=The Astrophysical Journal\|year=2016\|volume=833\|issue=2\|pages=167\|doi=10.3847/1538-4357/833/2/167\|arxiv=1610.01158\|s2cid=73620398 \|doi-access=free }} \| 16.0 \| align="center" \|Local Group \| Satellite of Andromeda \| 1,800 ly
64 \| 60px \| IC 1613 (UGC 668) \| IAB(s)m V \| 2.24 \| 0.686 \| −14.51 \| 9.92 \| align="center" \|Local Group \| \|
65 \| align="center" \| \| Pegasus V (Andromeda XXXIV) \| \| 2.26 \| 0.692 \| −6.3 \| \| align="center" \|Local Group \| Satellite of Andromeda{{cite journal \|arxiv=2204.09068 \|last1=Collins \|first1=Michelle L. M. \|last2=Charles \|first2=Emily J. E. \|last3=Martínez-Delgado \|first3=David \|last4=Monelli \|first4=Matteo \|last5=Karim \|first5=Noushin \|last6=Donatiello \|first6=Giuseppe \|last7=Tollerud \|first7=Erik J. \|last8=Boschin \|first8=Walter \|title=Pegasus V/Andromeda XXXIV–a newly discovered ultrafaint dwarf galaxy on the outskirts of Andromeda \|journal=Monthly Notices of the Royal Astronomical Society: Letters \|year=2022 \|volume=515 \|issue=1 \|pages=L72–L77 \|doi=10.1093/mnrasl/slac063 \|doi-access=free \|bibcode=2022MNRAS.515L..72C }} \|
66 \| 60px \| Leo A (Leo III, DDO 69) \| IBm V \| 2.34 \| 0.717 \| −11.68 \| 12.92 \| align="center" \|Local Group \| Satellite of Milky Way \|
67 \| align="center" \| \| Andromeda XVII \| dSph \| 2.371 \| 0.727 \| −7.8 \| 16.6 \| align="center" \|Local Group \| Satellite of Andromeda \| 1,900 ly
68 \| align="center" \| \| Andromeda XXV \| dSph \| 2.401 \| 0.736 \| −9.0 \| 15.3 \| align="center" \|Local Group \| Satellite of Andromeda \| 3,560 ly
69 \| align="center" \| \| Andromeda XI \| dSph \| 2.41 \| 0.74{{cite journal\|title=Cosmicflows-2: The Data\|author1=Tully, R. Brent\|display-authors=etal\|journal=The Astronomical Journal\|volume=146\|issue=4\|date=2013\|bibcode=2013AJ....146...86T\|doi=10.1088/0004-6256/146/4/86\|arxiv=1307.7213\|page=86\|s2cid=118494842}} \| −7.3{{cite journal\|bibcode=2012MNRAS.419.1362Y\|title=HST/WFPC2 Imaging of the Dwarf Satellites And XI and And XIII : HB Morphology and RR Lyraes\|journal=Monthly Notices of the Royal Astronomical Society\|volume=419\|issue=2\|pages=1362\|doi=10.1111/j.1365-2966.2011.19792.x\|year=2012\|last1=Yang\|first1=S.-C\|last2=Sarajedini\|first2=A\|doi-access=free \|arxiv=1109.2038\|s2cid=119190619}} \| \| align="center" \|Local Group \| Satellite of Andromeda \|
70 \| align="center" \| \| Andromeda XX \| dSph{{cite journal\|bibcode=2013ApJ...768..172C\|title=A Kinematic Study of the Andromeda Dwarf Spheroidal System\|last1=Collins\|first1=Michelle L. M.\|last2=Chapman\|first2=Scott C.\|last3=Rich\|first3=R. Michael\|last4=Ibata\|first4=Rodrigo A.\|last5=Martin\|first5=Nicolas F.\|last6=Irwin\|first6=Michael J.\|last7=Bate\|first7=Nicholas F.\|last8=Lewis\|first8=Geraint F.\|last9=Peñarrubia\|first9=Jorge\|last10=Arimoto\|first10=Nobuo\|last11=Casey\|first11=Caitlin M.\|author-link11=Caitlin Casey\|last12=Ferguson\|first12=Annette M. N.\|last13=Koch\|first13=Andreas\|last14=McConnachie\|first14=Alan W.\|last15=Tanvir\|first15=Nial\|journal=The Astrophysical Journal\|year=2013\|volume=768\|issue=2\|pages=172\|doi=10.1088/0004-637X/768/2/172\|arxiv=1302.6590\|s2cid=67749084}} \| 2.417 \| 0.741 \| −6.4 \| 18.0 \| align="center" \|Local Group \| Satellite of Andromeda \| 590 ly
71 \| align="center" \| \| Andromeda XXIII \| dSph \| 2.440 \| 0.748 \| −9.8 \| 14.6 \| align="center" \|Local Group \| Satellite of Andromeda \| 7,770 ly
72 \| align="center" \| 60px \| IC 10 (UGC 192) \| dIrr IV/BCD \| 2.446 \| 0.750 \| −15.57 \| 12.2 \| align="center" \|Local Group \| Satellite of Andromeda \|
73 \| align="center" \|60px \| Andromeda III \| dE2 \| 2.45 \| 0.75 \| −10.1 \| 14.4 \| align="center" \|Local Group \| Satellite of Andromeda \| 2750 ly
73 \| align="center" \| File:Cassiopeia Dwarf (PGC 2807155) Hubble WikiSky.jpg \|Cassiopeia Dwarf (Cas dSph, Andromeda VII) \| dSph \| 2.45 \| 0.75{{cite journal\|doi=10.3847/1538-4357/abdec1\|title=The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. IV. The Star Formation History of Andromeda VII Derived from Long-period Variable Stars\|year=2021\|last1=Navabi\|first1=Mahdieh\|last2=Saremi\|first2=Elham\|last3=Javadi\|first3=Atefeh\|last4=Noori\|first4=Majedeh\|last5=Van Loon\|first5=Jacco Th.\|last6=Khosroshahi\|first6=Habib G.\|last7=McDonald\|first7=Iain\|last8=Alizadeh\|first8=Mina\|last9=Danesh\|first9=Arash\|last10=Gozaliasl\|first10=Ghassem\|last11=Molaeinezhad\|first11=Alireza\|last12=Parto\|first12=Tahere\|last13=Raouf\|first13=Mojtaba\|journal=The Astrophysical Journal\|volume=910\|issue=2\|page=127\|arxiv=2101.09900\|bibcode=2021ApJ...910..127N\|s2cid=231698580 \|doi-access=free }} \| −11.67 \| 13.65 \| align="center" \|Local Group \| Satellite of Andromeda \|
75 \| align="center" \| \| Andromeda XXVI \| dSph \| 2.459 \| 0.754 \| −5.8 \| 18.5 \| align="center" \|Local Group \| Satellite of Andromeda \| 980 ly
76 \| align="center" \|60px \| Cetus Dwarf \| dSph/E4 \| 2.460McConnachie, A. W. et al. 2005 Distances and Metallicities for 17 Local Group Galaxies \| 0.754 \| −10.18 \| 14.4 \| align="center" \|Local Group \| Satellite of Andromeda \|
77 \| align="center"\| \| Pisces III (Andromeda XIII) \| dSph \| 2.479 \| 0.760 \| −6.5 \| 17.8 \| align="center"\|Local Group \| Satellite of Andromeda \| 850 ly
78 \| align="center" \| \| Andromeda XV \| dSph \| 2.48 \| 0.76 \| −8.4 \| 16.0 \| align="center" \|Local Group \| Satellite of Andromeda \| 1840 ly
79 \| align="center" \| 60px \|M32 (NGC 221) \| E2 \| 2.489 \| 0.763 \| −15.96 \| 8.73 \| align="center" \|Local Group \| Close Satellite of Andromeda \|6,500 ly
80 \| \|Andromeda IX \| dE \| 2.500 \| 0.767 \| −7.5 \| \| align="center" \|Local Group \| Satellite of Andromeda \|
81 \| align="center" \| 60px \|Pisces Dwarf (LGS 3) \| dIrr/dSph \| 2.510 \| 0.770 \| −7.96 \| 16.18 \| align="center" \|Local Group \| Satellite of Triangulum{{Citation needed\|date=June 2008}} \|
82 \| align="center" \| \| Cassiopeia III (Andromeda XXXII) \| \| 2.518 \| 0.772{{cite journal\|bibcode=2013ApJ...772...15M\|title=Lacerta I and Cassiopeia III. Two Luminous and Distant Andromeda Satellite Dwarf Galaxies Found in the 3π Pan-STARRS1 Survey\|last1=Martin\|first1=Nicolas F.\|last2=Slater\|first2=Colin T.\|last3=Schlafly\|first3=Edward F.\|last4=Morganson\|first4=Eric\|last5=Rix\|first5=Hans-Walter\|last6=Bell\|first6=Eric F.\|last7=Laevens\|first7=Benjamin P. M.\|last8=Bernard\|first8=Edouard J.\|last9=Ferguson\|first9=Annette M. N.\|last10=Finkbeiner\|first10=Douglas P.\|last11=Burgett\|first11=William S.\|last12=Chambers\|first12=Kenneth C.\|last13=Hodapp\|first13=Klaus W.\|last14=Kaiser\|first14=Nicholas\|last15=Kudritzki\|first15=Rolf-Peter\|last16=Magnier\|first16=Eugene A.\|last17=Morgan\|first17=Jeffrey S.\|last18=Price\|first18=Paul A.\|last19=Tonry\|first19=John L.\|last20=Wainscoat\|first20=Richard J.\|journal=The Astrophysical Journal\|year=2013\|volume=772\|issue=1\|pages=15\|doi=10.1088/0004-637X/772/1/15\|arxiv=1305.5301\|s2cid=119262613}} \| −12.3 \| 12.15 \| align="center" \|Local Group \| Satellite of Andromeda \| 9,500 ly
83 \| \| Andromeda V \| dSph \| 2.52 \| 0.773 \| −8.41 \| 16.67 \| align="center" \|Local Group \| Satellite of Andromeda \|
84 \| align="center"\| \| Lacerta I (Andromeda XXXI) \| dSph \| 2.521 \| 0.773{{cite journal\|doi=10.3847/1538-4357/836/1/137\|title=Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN pODI\|year=2017\|last1=Rhode\|first1=Katherine L.\|last2=Crnojević\|first2=Denija\|last3=Sand\|first3=David J.\|last4=Janowiecki\|first4=Steven\|last5=Young\|first5=Michael D.\|last6=Spekkens\|first6=Kristine\|journal=The Astrophysical Journal\|volume=836\|issue=1\|pages=137\|arxiv=1701.08168\|bibcode=2017ApJ...836..137R\|s2cid=118918041 \|doi-access=free }} \| −11.4 \| 13.04 \| align="center"\|Local Group \| Satellite of Andromeda \| 4,750 ly
85 \| align="center" \| 60px \| NGC 147 (DDO 3) \| dE5 pec \| 2.53 \| 0.776 \| −14.9 \| 10.36 \| align="center" \|Local Group \| Satellite of Andromeda \|
86 \| align="center" \|60px \|Andromeda Galaxy (M31) \| SA(s)b \| 2.538 \| 0.778 \| −21.58 \| 4.17 \| align="center" \|Local Group \| Largest Galaxy in the Local Group (The Milky Way is the second largest), with at least 19 satellite galaxies. Barred spiral galaxy. \|152,000 ly
87 \| align="center" \| 60px \|Pegasus Dwarf Spheroidal (Andromeda VI) \| dSph \| 2.55 \| 0.78 \| −10.80 \| 14.05 \| align="center" \|Local Group \| Satellite of Andromeda \|
88 \| align="center"\| \| Perseus I (Andromeda XXXIII) \| \| 2.560 \| 0.785{{cite journal\|bibcode=2013ApJ...779L..10M\|title=Perseus I: A Distant Satellite Dwarf Galaxy of Andromeda\|last1=Martin\|first1=Nicolas F.\|last2=Schlafly\|first2=Edward F.\|last3=Slater\|first3=Colin T.\|last4=Bernard\|first4=Edouard J.\|last5=Rix\|first5=Hans-Walter\|last6=Bell\|first6=Eric F.\|last7=Ferguson\|first7=Annette M. N.\|last8=Finkbeiner\|first8=Douglas P.\|last9=Laevens\|first9=Benjamin P. M.\|last10=Burgett\|first10=William S.\|last11=Chambers\|first11=Kenneth C.\|last12=Draper\|first12=Peter W.\|last13=Hodapp\|first13=Klaus W.\|last14=Kaiser\|first14=Nicholas\|last15=Kudritzki\|first15=Rolf-Peter\|last16=Magnier\|first16=Eugene A.\|last17=Metcalfe\|first17=Nigel\|last18=Morgan\|first18=Jeffrey S.\|last19=Price\|first19=Paul A.\|last20=Tonry\|first20=John L.\|last21=Wainscoat\|first21=Richard J.\|last22=Waters\|first22=Christopher\|journal=The Astrophysical Journal\|year=2013\|volume=779\|issue=1\|pages=L10\|doi=10.1088/2041-8205/779/1/L10\|arxiv=1310.4170\|s2cid=55729618}} \| −10.3 \| 14.19 \| align="center"\|Local Group \| Satellite of Andromeda \| 2,600 ly
89 \| align="center"\| \| Andromeda XIV (Pisces IV) \| \| 2.586 \| 0.793 \| −8.5 \| 15.8 \| align="center"\|Local Group \| Satellite of Andromeda \| ~1,700 ly
90 \| 60px \| Andromeda I \| dE3 pec \| 2.61 \| 0.80Calculated from the distance modulus ( $m - M$ ) using the formula $d_{pc} = 10^{\frac{m - M}{5} + 1}$ \| −12.0 \| 12.7 \| align="center" \|Local Group \| Satellite of Andromeda \| 5,840 ly
91 \| align="center"\| \| Andromeda XXVIII \| dSph \| 2.645 \| 0.811{{cite journal\|bibcode=2015ApJ...806..230S\|title=A Deep Study of the Dwarf Satellites Andromeda XXVIII and Andromeda XXIX\|last1=Slater\|first1=Colin T.\|last2=Bell\|first2=Eric F.\|last3=Martin\|first3=Nicolas F.\|last4=Tollerud\|first4=Erik J.\|last5=Ho\|first5=Nhung\|journal=The Astrophysical Journal\|year=2015\|volume=806\|issue=2\|pages=230\|doi=10.1088/0004-637X/806/2/230\|arxiv=1505.02161\|s2cid=118698841}} \| −8.7 \| 15.85 \| align="center"\|Local Group \| Satellite of Andromeda \| 1,800 ly
92 \| align="center" \| 60px \|M110 (NGC 205) \| E6p \| 2.67 \| 0.82 \| −16.15 \| 8.72 \| align="center" \|Local Group \| Close Satellite of Andromeda \|
93 \| \|Andromeda VIII \| dSphMorrison et al. 2003 Andromeda VIII, a New Tidally Distorted satellite of M31 — for details see [http://www.journals.uchicago.edu/doi/pdf/10.1086/379625] {{Webarchive\|url=https://web.archive.org/web/20200708082106/https://www.journals.uchicago.edu/doi/pdf/10.1086/379625\|date=2020-07-08}} \| 2.700 \| 0.828 \| −15.6 \| 9.1 \| align="center" \|Local Group \| Tidally distorted dwarf close to Andromeda discovered 2003 \|
94 \| align="center" \| \| Andromeda XXIX \| \| 2.704 \| 0.829 \| −8.5 \| 16.09 \| align="center" \|Local Group \| Satellite of Andromeda \| 2,050 ly
95 \| align="center" \|60px \| Triangulum Galaxy (M33) \| SA(s)cd \| 2.73 \| 0.84 \| −18.87 \| 6.19 \| align="center" \|Local Group \| Most distant (difficult) naked eye object. Closest unbarred spiral galaxy to us and third largest galaxy in the Local Group. \|61,100 ly
96 \| align="center" \| \| Andromeda XXI{{Cite journal \| arxiv=0909.0399 \| author1=Martin \| display-authors=4 \| author2=McConnachie \| author3=Mike Irwin \| author4=Widrow \| author5=Ferguson \| author6=Ibata \| author7=John Dubinski \| author8=Arif Babul \| author9=Scott Chapman \| title=PAndAS' cubs: Discovery of two new dwarf galaxies in the surroundings of the Andromeda and Triangulum galaxies \| date=2009 \| doi=10.1088/0004-637X/705/1/758 \| volume=705 \| journal=The Astrophysical Journal \| issue=1 \| pages=758–765 \| bibcode=2009ApJ...705..758M\| s2cid=15277245 }} \| dSph \| 2.802 \| 0.859 \| −9.9 \| \| align="center" \|Local Group \| Satellite of Andromeda \|
97 \| align="center" \| 60px \| Tucana Dwarf \| dE5 \| 2.87 \| 0.88 \| −9.16 \| 15.7 \| align="center" \|Local Group \| Isolated group member — a 'primordial' galaxy[https://www.doi.org/10.1111/j.1365-2966.2007.11395.x See] \|
98 \| align="center" \| 60px \| Andromeda X \| dSph \| 2.90 \| 0.889 \| −8.1Zucker et al. 2007 Andromeda X, a New Dwarf Spheroidal satellite of M31:Photometry — for details see [http://www.journals.uchicago.edu/doi/abs/10.1086/516748?journalCode=apjl] \| 16.1 \| align="center" \|Local Group \| Satellite of Andromeda discovered 2006 \|
99 \| align="center"\| \| Andromeda XXIV \| dSph \| 2.929 \| 0.898 \| −8.4 \| 16.3 \| align="center"\|Local Group \| Satellite of Andromeda \| 4,440 ly
99 \| align="center" \| 60px \|Pegasus Dwarf Irregular (DDO 216) \| dIrr/dSph \| 2.929 \| 0.898 \| −11.47 \| 13.21 \| align="center" \|Local Group \| Satellite of Andromeda \|
101 \| \| Pisces VII (Triangulum III) \| \| 2.99 \| 0.916{{cite journal \| arxiv=2305.13966 \| doi=10.1093/mnras/stae199 \| doi-access=free \| bibcode=2024MNRAS.528.2614C \| title=Pisces VII/Triangulum III – M33's second dwarf satellite galaxy \| date=2024 \| last1=Collins \| first1=Michelle L M. \| last2=Karim \| first2=Noushin \| last3=Martinez-Delgado \| first3=David \| last4=Monelli \| first4=Matteo \| last5=Tollerud \| first5=Erik J. \| last6=Donatiello \| first6=Giuseppe \| last7=Navabi \| first7=Mahdieh \| last8=Charles \| first8=Emily \| last9=Boschin \| first9=Walter \| journal=Monthly Notices of the Royal Astronomical Society \| volume=528 \| issue=2 \| pages=2614–2620 }} \| −6.0 \| \| align="center" \|Local Group \| Likely satellite of Triangulum \|
102 \| align="center"\| \| Andromeda XXXV \| \| 3.023 \| 0.927{{Cite journal \|last1=Arias \|first1=Jose Marco \|last2=Bell \|first2=Eric F. \|last3=Gozman \|first3=Katya \|last4=Jang \|first4=In Sung \|last5=Stockton \|first5=Saxon \|last6=Gnedin \|first6=Oleg Y. \|last7=D’Souza \|first7=Richard \|last8=Monachesi \|first8=Antonela \|last9=Bailin \|first9=Jeremy \|last10=Nidever \|first10=David \|last11=de Jong \|first11=Roelof S. \|date=2025-03-11 \|title=Andromeda XXXV: The Faintest Dwarf Satellite of the Andromeda Galaxy \|journal=The Astrophysical Journal Letters \|volume=982 \|issue=1 \|pages=L3 \|doi=10.3847/2041-8213/adb433 \|doi-access=free \|bibcode=2025ApJ...982L...3A \|issn=2041-8205}} \| −5.2 \| \| align="center"\|Local Group \| Satellite of Andromeda \|
102 \| align="center"\| \| Andromeda XII \| dSph \| 3.027 \| 0.928{{cite journal\|bibcode=2019MNRAS.488.3231H\|title=Proper motions of the satellites of M31\|last1=Hodkinson\|first1=Ben\|last2=Scholtz\|first2=Jakub\|journal=Monthly Notices of the Royal Astronomical Society\|year=2019\|volume=488\|issue=3\|pages=3231\|doi=10.1093/mnras/stz1893\|doi-access=free \|arxiv=1904.03192}} \| −7.0 \| 17.7 \| align="center"\|Local Group \| Satellite of Andromeda \| 2,740 ly
103 \| align="center" \|60px \|Wolf-Lundmark-Melotte (WLM, DDO 221) \| IB(s)m \| 3.043 \| 0.933{{cite journal \| author1=Karachentsev \| author2=Kashibadze \| author3=Makarov \| author4=Tully \| title=The Hubble flow around the Local Group \| doi=10.1111/j.1365-2966.2008.14300.x \| date=2009 \| journal=Monthly Notices of the Royal Astronomical Society \| volume=393 \| issue=4 \| pages=1265 \| doi-access=free \| arxiv=0811.4610 \|bibcode = 2009MNRAS.393.1265K \| s2cid=13912040 }} \| −14.06 \| 11.03 \| align="center" \|Local Group \| Isolated member at the edge of the local group \|11,500 ly
103 \| \|Andromeda XIXA Trio of New Local Group Galaxies with Extreme Properties, Alan W. McConnachie et al. 2008, ApJ 688 1009–1020, https://arxiv.org/abs/0806.3988 {{Webarchive\|url=https://web.archive.org/web/20171201182050/https://arxiv.org/abs/0806.3988 \|date=2017-12-01 }} \| dSph \| 3.043 \| 0.933 \| −9.3 \| \| align="center" \|Local Group \| Satellite of Andromeda, spread over 1.7 kpc \|2,200 ly
105 \| align="center" \| \|Andromeda XXII \| dSph \| 3.219 \| 0.987 \| \| 18.0 \| align="center" \|Local Group \| Satellite of Andromeda \|
106 \| align="center" \| 60px \| Aquarius Dwarf Galaxy (DDO 210) \| Im V \| 3.22 \| 0.988 \| −11.09 \| 14.0 \| align="center" \|Local Group \| Isolated group member \|
107 \| align="center" \|60px \| Sagittarius Dwarf Irregular Galaxy (SagDIG) \| IB(s)m V \| 3.907 \| 1.198 \| −11.49 \| 15.5 \| align="center" \|Local Group \| Isolated, star forming group member \|3,000 ly
108 \| align="center" \| 60px \| UGC 4879 (VV124){{cite journal \| author1=Kopylov \| display-authors=4 \| author2=Tikhonov \| author3=Sergey Fabrika \| author4=Igor Drozdovsky \| author5=Valeev \| title=VV124 (UGC4879): A new transitional dwarf galaxy in the periphery of the Local Group \| doi=10.1111/j.1745-3933.2008.00482.x \| date=2008 \| journal=Monthly Notices of the Royal Astronomical Society: Letters \| volume=387 \| issue=1 \| pages=L45–L49 \| doi-access=free \| arxiv=0803.1107 \|bibcode = 2008MNRAS.387L..45K \| s2cid=17166212 }} \| IAm \| 3.956 \| 1.213 \| −11.5 \| 13.2 \| align="center" \|Local Group \| Isolated, star forming group member \|3,000 ly
109 \| align="center" \| 60px \| Andromeda XVIII \| dSph \| 3.960 \| 1.214 \| −9.2 \| 16.2 \| align="center" \|Local Group \| 1,700 \|≈ 1,200 ly
110 \| align="center" \| 60px \| Antlia Dwarf \| dE3.5 \| 4.28 \| 1.31 \| −9.63 \| 16.19 \| align="center" \|Local GroupGalaxies of small Antlia-Sextans Group, which is considered as part of Local Group, but membership of it is uncertain. \| May have interacted with NGC 3109 \|3,000 ly
111 \| align="center" \| 60px \| Sextans A (UGCA 205, DDO 75) \| IBm \| 4.31Dolphin, Andrew E. et al. 2003 Deep Hubble Space Telescope Imaging of Sextans A. II. Cepheids and Distance \| 1.32 \| −13.95 \| 11.86 \| align="center" \|Local Group \| Contains cluster of young hot blue stars \|5,000 ly
112 \| align="center" \| 60px \| NGC 3109 \| SB(s)m \| 4.338 \| 1.35Soszynski "et al."(2006) The Araucaria Project: Distance to the Local Group Galaxy NGC 3109 from Near-Infrared Photometry of Cepheids see [http://www.journals.uchicago.edu/doi/abs/10.1086/505789?journalCode=apj] {{Webarchive\|url=https://web.archive.org/web/20200201224641/https://www.journals.uchicago.edu/doi/abs/10.1086/505789?journalCode=apj\|date=2020-02-01}} \| −15.68 \| 10.39 \| align="center" \|Local Group \| Possibly spiral galaxy \|25,000 ly
113 \| align="center" \| \| Antlia B \|dSph/Irr \| 4.40 \| 1.35{{cite journal\|doi=10.3847/1538-4357/ab58d2\|title=Hubble Space Telescope Imaging of Antlia B: Star Formation History and a New Tip of the Red Giant Branch Distance\|year=2020\|last1=Hargis\|first1=J. R.\|last2=Albers\|first2=S.\|last3=Crnojević\|first3=D.\|last4=Sand\|first4=D. J.\|last5=Weisz\|first5=D. R.\|last6=Carlin\|first6=J. L.\|last7=Spekkens\|first7=K.\|last8=Willman\|first8=B.\|last9=Peter\|first9=A. H. G.\|last10=Grillmair\|first10=C. J.\|last11=Dolphin\|first11=A. E.\|journal=The Astrophysical Journal\|volume=888\|issue=1\|pages=31\|bibcode=2020ApJ...888...31H\|hdl=10150/640977\|s2cid=197431299\|hdl-access=free \|doi-access=free }} \| −9.7 \| 15.95 \| align="center" \|Local Group \| Satellite of NGC 3109 \| 1,780 ly
114 \| align="center" \| \| Sculptor A \| \| 4.40 \| 1.35{{cite journal\|bibcode=2024ApJ...977L...5S\|arxiv=2409.16345\|doi=10.3847/2041-8213/ad927c\|doi-access=free \|title=Three Quenched, Faint Dwarf Galaxies in the Direction of NGC 300: New Probes of Reionization and Internal Feedback \|date=2024 \|last1=Sand \|first1=David J. \|last2=Mutlu-Pakdil \|first2=Burçin \|last3=Jones \|first3=Michael G. \|last4=Karunakaran \|first4=Ananthan \|last5=Andrews \|first5=Jennifer E. \|last6=Bennet \|first6=Paul \|last7=Crnojević \|first7=Denija \|last8=Donatiello \|first8=Giuseppe \|last9=Drlica-Wagner \|first9=Alex \|last10=Fielder \|first10=Catherine \|last11=Martínez-Delgado \|first11=David \|last12=Martínez-Vázquez \|first12=Clara E. \|last13=Spekkens \|first13=Kristine \|last14=Doliva-Dolinsky \|first14=Amandine \|last15=Hunter \|first15=Laura C. \|last16=Carlin \|first16=Jeffrey L. \|last17=Cerny \|first17=William \|last18=Hai \|first18=Tehreem N. \|last19=McQuinn \|first19=Kristen B.W. \|last20=Pace \|first20=Andrew B. \|last21=Smercina \|first21=Adam \|journal=The Astrophysical Journal Letters \|volume=977 \|pages=L5 }} \| −6.9 \| \| align="center" \|Local Group \| \|
114 \| align="center" \| 60px \| Sextans B (UGC 5373) \| IM IV-V \| 4.47 \| 1.37 \| −14.08 \| 11.85 \| align="center" \|Local Group \| One of the smallest galaxies with planetary nebulae \|6,000 ly
114 \| align="center" \| \| Tucana B \|dSph \| 4.56 \| 1.4{{cite journal\|doi=10.3847/2041-8213/ac85ee\|title=Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 MPC \|year=2022 \|last1=Sand \|first1=David J. \|last2=Mutlu-Pakdil \|first2=Burçin \|last3=Jones \|first3=Michael G. \|last4=Karunakaran \|first4=Ananthan \|last5=Wang \|first5=Feige \|last6=Yang \|first6=Jinyi \|last7=Chiti \|first7=Anirudh \|last8=Bennet \|first8=Paul \|last9=Crnojević \|first9=Denija \|last10=Spekkens \|first10=Kristine \|journal=The Astrophysical Journal Letters \|volume=935 \|issue=1 \|pages=L17 \|s2cid=251615833 \|hdl=10261/309130 \|hdl-access=free \|doi-access=free \|arxiv=2205.09129 \|bibcode=2022ApJ...935L..17S }} \| −6.9 \| 18.85 \| align="center" \|Local Group \| Isolated group member \| 522 ly
115 \| \|Cassiopeia 1 \|Irr \|5.19 \|1.59{{Cite journal \|last=Tikhonov \|first=N. A. \|date=2019-12-01 \|title=Distance to Irregular Galaxy Cas 1 Located near the Milky Way \|url=https://ui.adsabs.harvard.edu/abs/2019AstBu..74..396T \|journal=Astrophysical Bulletin \|volume=74 \|issue=4 \|pages=396–402 \|doi=10.1134/S1990341319040060\|bibcode=2019AstBu..74..396T \|s2cid=213381996 }} \| -14.2 \|14.62 \|Isolated \|Isolated galaxy \|
116 \| align="center" \| 60px \| Leo P \| Irr \| 5.28 \| 1.62 \| -9.27 \| 16.89 \| align="center" \| Local Group \| Extremely low metallicity \| 3,690 ly
117 \| align="center" \| 60px \| IC 5152 \| IA(s)m \| 5.68 \| 1.74 \| −15.56 \| 11.06 \| align="center" \| Local Group ? \| Possible outlying member of Local Group \|4,000 ly
118 \| align="center" \| 60px \| NGC 300 \| SA(s)d \| 6.07 \| 1.86 \| −17.92 \| 8.95 \| align="center" \|between LG and Sculptor Group \| Closest spiral galaxy to Local Group forms pair with NGC 55 \|94,000 ly
119 \| align="center" \|60px \| KKR 25 \| Irr \| 6.20 \| 1.90 \| −9.94 \| 17.0 \| between LG and M81 \| \|
120 \| align="center" \|60px \| ESO 410-G005 \| E3 \| 6.213 \| 1.905 \| −11.60 \| 14.85 \| align="center" \| NGC 55 & 300 \| \|≈ 2,500 ly
121 \| align="center" \| 60px \| ESO 294-010 \| dS0/Im \| 6.36Karachentsev, I. D. et al. (2003) Distances to Nearby Galaxies in Sculptor \| 1.96 \| −10.95 \| 15.6 \| align="center" \| NGC 55 & 300 \| \|
122 \| align="center" \| \| Pavo \| \| 6.49 \| 1.99{{cite journal\|doi=10.3847/2041-8213/ad0130\|doi-access=free \|title=Pavo: Discovery of a Star-forming Dwarf Galaxy Just Outside the Local Group \|date=2023 \|last1=Jones \|first1=Michael G. \|last2=Mutlu-Pakdil \|first2=Burçin \|last3=Sand \|first3=David J. \|last4=Donnerstein \|first4=Richard \|last5=Crnojević \|first5=Denija \|last6=Bennet \|first6=Paul \|last7=Fielder \|first7=Catherine E. \|last8=Karunakaran \|first8=Ananthan \|last9=Spekkens \|first9=Kristine \|last10=Strader \|first10=Jay \|last11=Urquhart \|first11=Ryan \|last12=Zaritsky \|first12=Dennis \|journal=The Astrophysical Journal Letters \|volume=957 \|issue=1 \|pages=L5 \|arxiv=2310.01478 \|bibcode=2023ApJ...957L...5J }} \| −10.0 \| \| align="center" \| \| \|
122 \| align="center" \| 60px \| NGC 55 \| SB(s)m \| 6.52 \| 2.00 \| −18.47 \| 8.84 \| align="center" \|between LG and Sculptor Group \| Forms pair with NGC 300 \|70,000 ly
123 \| align="center" \| \| Sculptor C \| \| 6.65 \| 2.04 \| −9.1 \| \| align="center" \| \| Satellite of NGC 300 \|
123 \| align="center" \| \| KKs 3 \| dSph \| 6.91 \| 2.12{{cite journal\|bibcode=2017MNRAS.471.1955S\|doi=10.1093/mnras/stx1605\|arxiv=1706.07344\|title=Nuclei of dwarf spheroidal galaxies KKs 3 and ESO 269−66 and their counterparts in our Galaxy\|journal=Monthly Notices of the Royal Astronomical Society\|volume=471\|issue=2\|pages=1955\|year=2017\|last1=Sharina\|first1=M. E\|last2=Shimansky\|first2=V. V\|last3=Kniazev\|first3=A. Y\|doi-access=free }} \| −12.3 \| 14.47 \| align="center" \| \| \| 4,900 ly
124 \| align="center" \|60px \| KKR 3 (KK 230) \| dIrr \| 6.98 \| 2.14 \| −9.8 \| 17.90 \| align="center" \| Inner edge of M94 Group \| \|980 ly
125 \| align="center" \| \| UGCA 438 (ESO 407-018) \| IB(s)m pec: \| 7.24 \| 2.22 \| −12.92 \| 13.86 \| align="center" \| NGC 55 & 300 \| \|
126 \| align="center" \| \| KK 258 (ESO 468–20) \| dTr \| 7.27 \| 2.23{{cite journal\|doi=10.1093/mnras/stu1217\|title=KK258, a new transition dwarf galaxy neighbouring the Local Group\|year=2014\|last1=Karachentsev\|first1=I. D.\|last2=Makarova\|first2=L. N.\|last3=Tully\|first3=R. B.\|last4=Wu\|first4=Po-Feng\|last5=Kniazev\|first5=A. Y.\|journal=Monthly Notices of the Royal Astronomical Society\|volume=443\|issue=2\|pages=1281–1290\|doi-access=free \|arxiv=1406.4479\|bibcode=2014MNRAS.443.1281K}} \| −10.3 \| \| align="center" \| NGC 55 & 300 \| \|
127 \| align="center" \|60px \| UGC 9128 (DDO 187) \| ImIV-V \| 7.31 \| 2.24 \| −12.47 \| 14.38 \| align="center" \| Inner edge of M94 Group \| \|
128 \| align="center" \| 60px \| IC 3104 \| IB(s)m \| 7.40 \| 2.27 \| −14.85 \| 13.63 \| \| On the way to Circinus galaxy \|
129 \| align="center" \| \| Dw1907+63 \| \| 7.8 \| 2.4 \| \| 17.0 \| align="center" \| \| \|
129 \| align="center" \|60px \| GR 8 (DDO 155, UGC 8091) \| ImV \| 7.8 \| 2.4 \| −12.14 \| 14.65 \| align="center" \| Inner edge of M94 Group \| "footprint galaxy" \|
129 \| \| Hedgehog Galaxy \| \| 7.86 \| 2.41{{cite journal\|doi=10.3847/2041-8213/ad5b59\|doi-access=free \|title=Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 MPC \|date=2024 \|last1=Li 李 \|first1=Jiaxuan 嘉轩 \|last2=Greene \|first2=Jenny E. \|last3=Carlsten \|first3=Scott G. \|last4=Danieli \|first4=Shany \|journal=The Astrophysical Journal Letters \|volume=975 \|issue=1 \|pages=L23 \|arxiv=2406.00101 \|bibcode=2024ApJ...975L..23L }} \| \| −9.84 \| \| Isolated dwarf \|
130 \| align="center" \| 60px \| IC 4662 (ESO 102-14) \| IBm \| 7.96 \| 2.44 \| −15.56 \| 11.74 \| \| On the way to Circinus galaxy \|7,000 ly
131 \| align="center" \|60px \| KKH 98 \| Irr \| 7.99 \| 2.45 \| −10.78 \| 16.7 \| align="center" \|IC 342/Maffei Group \| \|
131 \| align="center" \| \| Sculptor B \| \| 8.09 \| 2.48 \| −8.1 \| \| align="center" \| \| \|
131 \| align="center" \|File:SMDG 0956+82.png \| SMDG 0956+82 \| \| 8.48 \| 2.6{{cite journal\|doi=10.1093/mnrasl/slae111 \|doi-access=free \|title=New radial velocities for 40 nearby dwarf galaxies \|date=2025 \|last1=Karachentsev \|first1=Igor D. \|last2=Chazov \|first2=Maxim I. \|last3=Kaisin \|first3=Serafim S. \|journal=Monthly Notices of the Royal Astronomical Society: Letters \|volume=537 \|pages=L21–L25 \|arxiv=2411.15603 }} \| \| 18.1 \| align="center" \| \| \|
132 \| align="center" \| 60px \| UGC 8508 (I Zw 060) \| IAm \| 8.35{{cite journal\|doi=10.1051/0004-6361:20011741\|title=The M 81 group of galaxies: New distances, kinematics and structure\|year=2002\|last1=Karachentsev\|first1=I. D.\|last2=Dolphin\|first2=A. E.\|last3=Geisler\|first3=D.\|last4=Grebel\|first4=E. K.\|last5=Guhathakurta\|first5=P.\|last6=Hodge\|first6=P. W.\|last7=Karachentseva\|first7=V. E.\|last8=Sarajedini\|first8=A.\|last9=Seitzer\|first9=P.\|last10=Sharina\|first10=M. E.\|journal=Astronomy & Astrophysics\|volume=383\|pages=125–136\|bibcode=2002A&A...383..125K\|doi-access=free}} \| 2.69 \| −13.09 \| 14.40 \| align="center" \|M94 Group \| \|
133 \| align="center" \| 60px \| KKH 86 \| Irr \| 8.48 \| 2.60 \| −10.30 \| 16.8 \| \| Isolated (M94/Cent A) \|
134 \| align="center" \| 60px \| DDO 99 (UGC 6817) \| Im \| 8.61 \| 2.64–3.9 \| −13.52 \| 13.4 \| align="center" \|M94 Group \| \|
135 \| align="center" \| \| Dw1245+61 \| \| 8.81 \| 2.7 \| \| 18.4 \| align="center" \| \| \|
135 \| align="center" \| \| ESO 6-1 \| Ir \| 8.81 \| 2.70 \| −12.41 \| 14.75{{cite journal\|doi=10.3847/1538-4357/acb048\|title=A Nearby Isolated Dwarf: Star Formation and Structure of ESO 006–001 \|year=2023 \|last1=Makarova \|first1=Lidia N. \|last2=Tully \|first2=R. Brent \|last3=Anand \|first3=Gagandeep S. \|last4=Lambert \|first4=Trystan S. \|last5=Sharina \|first5=Margarita E. \|last6=Koribalski \|first6=Bärbel S. \|last7=Kraan-Korteweg \|first7=Renée C. \|journal=The Astrophysical Journal \|volume=943 \|issue=2 \|page=139 \|arxiv=2301.12789 \|bibcode=2023ApJ...943..139M \|s2cid=256390080 \|doi-access=free }} \| align="center" \| \| Blue compact dwarf galaxy \|
136 \| align="center" \| 60px \| UGC 7577 (DDO 125) \| Im \| 8.94 \| 2.74 \| −14.32 \| 12.84 \| align="center" \|M94 Group \| \|
137 \| align="center" \| \| KDG 162 \| \| 9.13 \| 2.8 \| \| 17.3 \| align="center" \| \| \|
137 \| align="center" \| 60px \| Dwingeloo 1 \| SB(s)cd \| 9.13 \| 2.8 \| −18.78 \| 19.8 \| align="center" \|IC 342/Maffei Group \| \|35,000 ly
138 \| align="center" \| 60px \| UGC 9240 (DDO 190) \| IAm \| 9.13 \| 2.80 \| −14.19 \| 13.25 \| align="center" \|M94 Group \| \|15,000 ly
139 \| align="center" \| 60px \| NGC 4190 \| Irr (BCD) \| 9.19 \| 2.82{{cite journal\|bibcode=2013AJ....145..101K\|title=Updated Nearby Galaxy Catalog\|last1=Karachentsev\|first1=Igor D.\|last2=Makarov\|first2=Dmitry I.\|last3=Kaisina\|first3=Elena I.\|s2cid=118585268\|journal=The Astronomical Journal\|year=2013\|volume=145\|issue=4\|page=101\|doi=10.1088/0004-6256/145/4/101\|arxiv=1303.5328}} \| \| 13.50 \| align="center" \| \| Satellite of NGC 4214 \|
140 \| align="center" \| \| Dw1645+46 \| \| 11.09 \| 2.9 \| \| 17.6 \| align="center" \| \| \|
140 \| align="center" \| \| KKs 53 (Cen 7) \| dSph{{cite journal \| first1=S. \| last1=Côté \| first2=K. C. \| last2=Freeman \| first3=C. \| last3=Carigan \| first4=P. J. \| last4=Quinn \| title=Discovery of Numerous Dwarf Galaxies in the Two Nearest Groups of Galaxies \| journal=Astronomical Journal \| year=1997 \| volume=114 \| pages=1313 \| bibcode=1997AJ....114.1313C \| doi=10.1086/118565 \| arxiv=astro-ph/9704030 \| s2cid=119495338 }} \| 9.56 \| 2.93{{cite journal\|bibcode=2015ApJ...802L..25T\|doi=10.1088/2041-8205/802/2/L25\|title=Two Planes of Satellites in the Centaurus A Group\|year=2015\|last1=Tully\|first1=R. Brent\|last2=Libeskind\|first2=Noam I.\|last3=Karachentsev\|first3=Igor D.\|last4=Karachentseva\|first4=Valentina E.\|last5=Rizzi\|first5=Luca\|last6=Shaya\|first6=Edward J.\|journal=The Astrophysical Journal\|volume=802\|issue=2\|pages=L25\|arxiv=1503.05599\|s2cid=118512897}} \| −10.86 \| 17.30 \| align="center" \|Centaurus A/M83 Group \| \|
141 \| align="center" \| 60px \| NGC 4214 (UGC 7278) \| IAB(s)m \| 9.59 \| 2.94 \| \| 10.24 \| align="center" \|M94 Group \| Starburst galaxy \|
142 \| align="center" \| 60px \| UGCA 276 (DDO 113) \| Im \| 9.62 \| 2.95{{cite journal\|doi=10.1093/mnras/stz3526\| arxiv=1908.11367\|title=The case for strangulation in low-mass hosts: DDO 113\|year=2020\|last1=Garling\|first1=Christopher T.\|last2=Peter\|first2=Annika H G.\|last3=Kochanek\|first3=Christopher S.\|last4=Sand\|first4=David J.\|last5=Crnojević\|first5=Denija\|journal=Monthly Notices of the Royal Astronomical Society\|volume=492\|issue=2\|pages=1713–1730\|doi-access=free}} \| \| 15.40 \| align="center" \|M94 Group \| \|
143 \| align="center" \|60px \| UGCA 133 (DDO 44) \| Im \| 9.65 \| 2.96{{cite journal\|arxiv=1906.08260\|doi=10.3847/1538-4357/ab4c32\|title=Tidal Destruction in a Low-mass Galaxy Environment: The Discovery of Tidal Tails around DDO 44\|year=2019\|last1=Carlin\|first1=Jeffrey L.\|last2=Garling\|first2=Christopher T.\|last3=Peter\|first3=Annika H. G.\|last4=Crnojević\|first4=Denija\|last5=Forbes\|first5=Duncan A.\|last6=Hargis\|first6=Jonathan R.\|last7=Mutlu-Pakdil\|first7=Burçin\|last8=Pucha\|first8=Ragadeepika\|last9=Romanowsky\|first9=Aaron J.\|last10=Sand\|first10=David J.\|last11=Spekkens\|first11=Kristine\|last12=Strader\|first12=Jay\|last13=Willman\|first13=Beth\|journal=The Astrophysical Journal\|volume=886\|issue=2\|page=109\|bibcode=2019ApJ...886..109C\|s2cid=195218404 \|doi-access=free }} \| −12.9 \| 15.54 \| align="center" \|M81 Group \| Likely satellite of NGC 2403 \|
143 \| align="center" \| 60px \| NGC 4163 (NGC 4167) \| dIrr \| 9.65 \| 2.96{{Cite web \|url=http://www.iop.org/EJ/article/1538-3881/131/3/1361/205003.tb1.html \|access-date=2009-09-21 \|title=Archived copy \|archive-date=2020-09-25 \|archive-url=https://web.archive.org/web/20200925123153/https://www.iop.org/EJ/article/1538-3881/131/3/1361/205003.tb1.html \|url-status=dead }} \| \| 14.5 \| align="center" \|M94 Group \| \|4,000 ly
144 \| align="center" \| 60px \| UGCA 86 \| SAB(s)m \| 9.72 \| 2.98{{cite journal\|doi=10.1051/0004-6361/202037993\|title=KKH 22, the first dwarf spheroidal satellite of IC 342\|year=2020\|last1=Karachentsev\|first1=Igor D.\|last2=Makarova\|first2=Lidia N.\|last3=Brent Tully\|first3=R.\|last4=Anand\|first4=Gagandeep S.\|last5=Rizzi\|first5=Luca\|last6=Shaya\|first6=Edward J.\|last7=Afanasiev\|first7=Viktor L.\|s2cid=218538458\|journal=Astronomy & Astrophysics\|volume=638\|pages=A111\|arxiv=2005.03132\|bibcode=2020A&A...638A.111K}} \| \| 13.5 \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|20,000 ly
145 \| align="center" \|60px \| NGC 1560 \| SA(s)d HII \| 9.75 \| 2.99 \| −16.87 \| 12.16 \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|
146 \| \| MADCASH-2 (MADCASH J121007+352635-dw) \| dSph \| 9.78 \| 3.00{{cite journal\|doi=10.3847/1538-4357/abe040\|arxiv=2012.09174\|bibcode=2021ApJ...909..211C\|title=Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH\|year=2021\|last1=Carlin\|first1=Jeffrey L.\|last2=Mutlu-Pakdil\|first2=Burçin\|last3=Crnojević\|first3=Denija\|last4=Garling\|first4=Christopher T.\|last5=Karunakaran\|first5=Ananthan\|last6=Peter\|first6=Annika H. G.\|last7=Tollerud\|first7=Erik\|last8=Forbes\|first8=Duncan A.\|last9=Hargis\|first9=Jonathan R.\|last10=Lim\|first10=Sungsoon\|last11=Romanowsky\|first11=Aaron J.\|last12=Sand\|first12=David J.\|last13=Spekkens\|first13=Kristine\|last14=Strader\|first14=Jay\|journal=The Astrophysical Journal\|volume=909\|issue=2\|page=211\|s2cid=229297953 \|doi-access=free }} \| −9.15 \| 18.24 \| align="center" \|M94 Group \| Likely satellite of NGC 4214 \|
147 \| \| Dwingeloo 2 \| Im? \| 9.8 \| 3.0 \| −14.55 \| 20.5 \| align="center" \|IC 342/Maffei Group \| \|20,000 ly
147 \| \| KKH 11 (ZOAG G135.74-04.53) \| dE/N \| 9.8 \| 3.0 \| −13.35 \| 16.2 \| align="center" \|IC 342/Maffei Group \| \|
147 \| \| KKH 12 \| Irr \| 9.8 \| 3.0 \| −13.03 \| 17.8 \| align="center" \| IC 342/Maffei Group \| \|
147 \| \| MB 3 \| dSph \| 9.8 \| 3.0 \| −13.65 \| 19.8 \| align="center" \|IC 342/Maffei Group \| \|10,000 ly
147 \| \| MB 1 (KK 21) \| SAB(s)d? \| 9.8 \| 3.0 \| −14.81 \| 20.5 \| align="center" \|IC 342/Maffei Group \| \|5,000 ly
147 \| align="center" \|60px \| Maffei 1 \| S0- pec \| 9.8 \| 3.0 \| −18.97 \| 11.4 \| align="center" \|IC 342/Maffei Group \| \|55,000 ly
153 \| align="center" \| 60px \| Maffei 2 \| SAB(rs)bc \| 9.801 \| 3.005 \| −20.15 \| 14.77 \| align="center" \|IC 342/Maffei Group \| \|60,000 ly
154 \| align="center" \| 60px \| UGC 8651 (DDO 181) \| Im \| 9.82 \| 3.01 \| \| 14.7 \| align="center" \|M94 Group \| \|
155 \| align="center" \| 60px \| Donatiello I \| dSph \| 9.88 \| 3.04 \| \| \| align="center" \| \| Possible satellite of NGC 404 \|
156 \| align="center" \| 60px \| NGC 2403 \| SAB(s)cd HII \| 9.92 \| 3.04 \| −19.29 \| 8.93 \| align="center" \|Inner edge of M81 Group \| \| 50,000 ly
157 \| align="center" \| 60px \| NGC 404 \| SA(s)0-: \| 10.05 \| 3.08 \| −16.61 \| 11.21 \| align="center" \| \| 'Mirach's Ghost' \|
158 \| align="center" \| 60x60px \| ESO 274-01{{cite journal\|doi= 10.1086/510125\|title= The Hubble Flow around the Centaurus A/M83 Galaxy Complex\|year= 2007\|last1= Karachentsev\|first1= Igor D.\|last2= Tully\|first2= R. Brent\|last3= Dolphin\|first3= Andrew\|last4= Sharina\|first4= Margarita\|last5= Makarova\|first5= Lidia\|last6= Makarov\|first6= Dmitry\|last7= Sakai\|first7= Shoko\|last8= Shaya\|first8= Edward J.\|last9= Kashibadze\|first9= Olga G.\|last10= Karachentseva\|first10= Valentina\|last11= Rizzi\|first11= Luca\|journal= The Astronomical Journal\|volume= 133\|issue= 2\|pages= 504–517\|arxiv= astro-ph/0603091\|bibcode= 2007AJ....133..504K\|s2cid= 120584}} \| SAd: \| 10.1 \| 3.09 \| \| 11.7 \| align="center" \|Centaurus A/M83 Group \| \|
159 \| align="center" \| \| Dw1558+67 \| \| 10.1 \| 3.1 \| \| 16.8 \| align="center" \| \| \|
159 \| align="center" \| \| GALFA-Dw4{{cite journal\|doi=10.3847/1538-4357/ac356c\|title=Hubble Space Telescope Imaging of Isolated Local Volume Dwarfs GALFA-Dw3 and Dw4\|year=2022\|last1=Bennet\|first1=P.\|last2=Sand\|first2=D. J.\|last3=Crnojević\|first3=D.\|last4=Weisz\|first4=D. R.\|last5=Caldwell\|first5=N.\|last6=Guhathakurta\|first6=P.\|last7=Hargis\|first7=J. R.\|last8=Karunakaran\|first8=A.\|last9=Mutlu-Pakdil\|first9=B.\|last10=Olszewski\|first10=E.\|last11=Salzer\|first11=J. J.\|last12=Seth\|first12=A. C.\|last13=Simon\|first13=J. D.\|last14=Spekkens\|first14=K.\|last15=Stark\|first15=D. P.\|last16=Strader\|first16=J.\|last17=Tollerud\|first17=E. J.\|last18=Toloba\|first18=E.\|last19=Willman\|first19=B.\|journal=The Astrophysical Journal\|volume=924\|issue=2\|page=98\|arxiv=2101.08270\|bibcode=2022ApJ...924...98B\|s2cid=231662303 \|doi-access=free }} \| dIrr \| 10.1 \| 3.10 \| −11.8 \| 15.7 \| align="center" \| \| Isolated \|
160 \| \| KKH 22 \| dSph \| 10.17 \| 3.12 \| –12.19 \| 15.28 \| align="center"\|IC 342/Maffei Group \| Satellite of IC 342 \|
161 \| align="center" \| 60px \| NGC 3741 \| ImIII/BCD \| 10.21 \| 3.13 \| \| 14.3 \| align="center" \|M94 Group \| \|
162 \| \| KK 35 \| Irr \| 10.31 \| 3.16 \| −14.30 \| 17.2 \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|
162 \| \| HIPASS J1247-77 \| Im \| 10.31 \| 3.16 \| \| 17.B \| \| Aligned with IC 3104 \|
164 \| align="center" \|60px \| NGC 2366 \| IB(s)m \| 10.40 \| 3.19 \| \| 11.43 \| align="center" \|M81 Group \| \|
164 \| align="center" \| 60px \| NGC 1569 (UGC 3056) \| IBm;Sbrst \| 10.40 \| 3.19 \| −18.17 \| 11.86 \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|6,000 ly
164 \| align="center" \| 60px \| ESO 321-014 \| IBm \| 10.40 \| 3.19 \| \| 15.16 \| align="center" \|Centaurus A/M83 Group \| \|
167 \| align="center" \| 60px \| UGC 8833 \| Im \| 10.41 \| 3.19 \| \| 16.5 \| align="center" \|M94 Group \| \|
168 \| align="center" \| 60px \| Sculptor dIG (ESO 349–31) \| dIrr \| 10.44 \| 3.2{{cite journal\|arxiv=1211.0137\|doi=10.1051/0004-6361/201220193\|bibcode=2013A&A...549A..47L\|title=The star formation history of the Sculptor Dwarf Irregular Galaxy\|year=2013\|last1=Lianou\|first1=S.\|last2=Cole\|first2=A. A.\|s2cid=55237783\|journal=Astronomy & Astrophysics\|volume=549\|pages=A47}} \| −11.87 \| 15.5 \| align="center" \|Sculptor Group \| Satellite of NGC 7793 \|
169 \| align="center" \| 60px \| UGC 4483 \| dIrr \| 10.47 \| 3.21 \| \| 15.2 \| align="center" \|M81 Group \| \|
169 \| align="center" \| \| dw0910p7326 ("Blobby") \| dSph \| 10.47 \| 3.21{{cite journal \| arxiv=2211.00629 \| doi=10.1093/mnras/stad352 \| title=Discovery of a red backsplash galaxy candidate near M81 \| year=2023 \| last1=Casey \| first1=Kirsten J. \| last2=Greco \| first2=Johnny P. \| last3=Peter \| first3=Annika H G. \| last4=Davis \| first4=A Bianca \| journal=Monthly Notices of the Royal Astronomical Society \| volume=520 \| issue=3 \| pages=4715–4729 \| doi-access=free }} \| 11.57 \| 15.96 \| align="center" \|M81 Group \| \|
170 \| \| UGC 8760 (DDO 183) \| I \| 10.50 \| 3.22 \| align="center"\| \| −13.08 \| 14.78{{cite simbad\|title=UGC 8760\|access-date=2025-02-08}} \| \|
170 \| align="center" \|60px \| UGCA 92 \| Im? \| 10.50 \| 3.22 \| \| 13 \| align="center" \| IC 342/Maffei Group{{Cite journal \|title=see article at \|journal=The Astrophysical Journal Supplement Series \|date=September 1999 \|volume=124 \|issue=1 \|pages=33–93 \|doi=10.1086/313255 \|s2cid=119907629 \|last1=Buta \|first1=Ronald J. \|last2=McCall \|first2=Marshall L. \|doi-access=free }} \| Satellite of IC 342 \|
171 \| align="center" \| 60px \| IC 342 \| SAB(rs)cd \| 10.70 \| 3.28 \| −20.69 \| 9.37 \| align="center" \|IC 342/Maffei Group \| "the hidden galaxy" \|75,000 ly
173 \| align="center" \| 60px \| UGCA 15 (DDO 6) \| IB(s)m \| 10.90 \| 3.34 \| −12.50 \| 15.19 \| align="center" \|Sculptor group \| \|
174 \| \| KKs 58 \| dSph \| 10.96 \| 3.36{{cite journal\|doi=10.1051/0004-6361/201935807\|title=The dwarf galaxy satellite system of Centaurus A\|year=2019\|last1=Müller\|first1=Oliver\|last2=Rejkuba\|first2=Marina\|last3=Pawlowski\|first3=Marcel S.\|last4=Ibata\|first4=Rodrigo\|last5=Lelli\|first5=Federico\|last6=Hilker\|first6=Michael\|last7=Jerjen\|first7=Helmut\|journal=Astronomy & Astrophysics\|volume=629\|pages=A18\|arxiv=1907.02012\|bibcode=2019A&A...629A..18M\|s2cid=195791783}} \| −11.93 \| \| align="center" \|Centaurus A/M83 Group \| \|
175 \| align="center" \|60px \| KKH 37 (Mai 16) \| S/Irr \| 11.06 \| 3.39{{cite journal\|doi=10.1086/500013\|title=Advanced Camera for Surveys Imaging of 25 Galaxies in Nearby Groups and in the Field\|year=2006\|last1=Karachentsev\|first1=Igor D.\|last2=Dolphin\|first2=Andrew\|last3=Tully\|first3=R. Brent\|last4=Sharina\|first4=Margarita\|last5=Makarova\|first5=Lidia\|last6=Makarov\|first6=Dmitry\|last7=Karachentseva\|first7=Valentina\|last8=Sakai\|first8=Shoko\|last9=Shaya\|first9=Edward J.\|journal=The Astronomical Journal\|volume=131\|issue=3\|pages=1361–1376\|arxiv=astro-ph/0511648\|bibcode=2006AJ....131.1361K\|s2cid=16689229}} \| \| 16.4 \| align="center" \|IC 342/Maffei Group \| \|
175 \| align="center" \| 60px \| UGCA 105 \| Im? \| 11.06 \| 3.39 \| −16.81 \| 13.9 \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|
175 \| align="center" \| 60px \| Holmberg II (DDO 50, UGC 4305) \| Im \| 11.06 \| 3.39 \| \| 11.1 \| align="center" \|M81 Group \| \|
175 \| align="center" \| \| Dw1559+46 \| \| 11.09 \| 3.4 \| \| 17.1 \| align="center" \| \| \|
175 \| align="center" \| 60px \| NGC 5102 \| SA0- HII \| 11.09 \| 3.40 \| −18.0856 \| 10.35 \| align="center" \|Centaurus A/M83 Group \| \|
175 \| align="center" \| 60px \| NGC 5237 \| I0? \| 11.09 \| 3.40 \| \| 13.23 \| align="center" \|Centaurus A/M83 Group \| \|
175 \| align="center" \| 60px \| ESO 325-11 \| \| 11.09 \| 3.40 \| \| 13.99 \| align="center" \|Centaurus A/M83 Group \| \|
175 \| align="center" \| 60px \| ESO 540-030 (KDG 2) \| IABm \| 11.09 \| 3.40 \| −11.39 \| 16.45 \| align="center" \|Sculptor group \| \|
182 \| align="center" \| 60px \| NGC 247 \| SAB(s)d \| 11.1 \| 3.4 \| −20.00 \| 9.9 \| align="center" \|Sculptor group \| \|
183 \| \| MADCASH-1 (MADCASH J074238+652501-dw) \| dSph \| 11.12 \| 3.41 \| −7.81 \| 19.85 \| align="center" \|M81 Group \| Likely satellite of NGC 2403 \|
184 \| \| F6D1 (FM 1, PGC 3097828) \| dSph{{cite journal\|doi=10.1088/0004-6256/137/2/3009\|title=Discovery of New Dwarf Galaxies in the M81 Group\|year=2009\|last1=Chiboucas\|first1=Kristin\|last2=Karachentsev\|first2=Igor D.\|last3=Tully\|first3=R. Brent\|s2cid=14156955\|journal=The Astronomical Journal\|volume=137\|issue=2\|pages=3009–3037\|arxiv=0805.1250\|bibcode=2009AJ....137.3009C}} \| 11.15 \| 3.42 \| \| 17.5 \| align="center" \|M81 Group \| \|
184 \| align="center" \| 60px \| ESO 540-032 \| IAB(s)m pec: \| 11.15 \| 3.42 \| −11.32 \| 16.55 \| align="center" \|Sculptor group \| \|
186 \| align="center" \| 60px \| ESO 383-087 (ISG 39) \| SB(s)dm \| 11.25 \| 3.45 \| −15.16 \| 11.03 \| align="center" \|Centaurus A/M83 Group \| \|
187 \| align="center" \| 60px \| NGC 5206 \| SB0 \| 11.32 \| 3.47 \| \| \| align="center" \|Centaurus A/M83 Group \| \|
188 \| align="center" \| 60px \| KK 179 (ESO 269-37) \| IABm: \| 11.4 \| 3.48 \| \| \| align="center" \|Centaurus A/M83 Group \| \|
188 \| align="center" \| \| Corvus A \| \| 11.4 \| 3.48{{cite journal \| doi=10.3847/2041-8213/ad676e \| doi-access=free \| title=Corvus A: A Low-mass, Isolated Galaxy at 3.5 MPC \| date=2024 \| last1=Jones \| first1=Michael G. \| last2=Sand \| first2=David J. \| last3=Mutlu-Pakdil \| first3=Burçin \| last4=Fielder \| first4=Catherine E. \| last5=Crnojević \| first5=Denija \| last6=Bennet \| first6=Paul \| last7=Spekkens \| first7=Kristine \| last8=Donnerstein \| first8=Richard \| last9=Doliva-Dolinsky \| first9=Amandine \| last10=Karunakaran \| first10=Ananthan \| last11=Strader \| first11=Jay \| last12=Zaritsky \| first12=Dennis \| journal=The Astrophysical Journal Letters \| volume=971 \| issue=2 \| pages=L37 \| arxiv=2407.03393 \| bibcode=2024ApJ...971L..37J }} \| −11.2 \| \| align="center" \| \| \|
193 \| align="center" \| \|Scl-MM-dw3 \| \| 11.35 \| 3.48 \| −7.24 \| \| align="center" \|Sculptor Group \| \|
189 \| align="center" \| 60px \| Sculptor Galaxy (NGC 253) \| SAB(s)c \| 11.40 \| 3.49 \| \| 8.0 \| align="center" \|Sculptor group \| \|90,000 ly
190 \| align="center" \| 60px \| DDO 71 (UGC 5428) \| Im \| 11.42 \| 3.50 \| \| 18 \| align="center" \|M81 Group \| \|
191 \| \| Camelopardalis B \| Irr \| 11.46 \| 3.50 \| −11.85 \| 16.1 \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|
192 \| align="center" \| 60px \|Messier 82 \| I0;Sbrst HII \| 11.42 \| 3.53 \| −19.63 \| 9.30 \| align="center" \|M81 Group \| \|37,000 ly, possibly up to 100,000 ly
193 \| align="center" \| 60px \|NGC 5253 \| Im pec \| 11.51 \| 3.53 \| \| 10.9 \| align="center" \|Centaurus A/M83 Group \|Nearest Wolf-Rayet galaxy to us. \|
193 \| align="center" \| \|Scl-MM-dw1 \| \| 11.51 \| 3.53 \| −8.75{{cite journal \| doi=10.3847/1538-4357/ac4418 \| doi-access=free \| arxiv=2108.09312 \| bibcode=2022ApJ...926...77M \| title=Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies \| date=2022 \| last1=Mutlu-Pakdil \| first1=Burçin \| last2=Sand \| first2=David J. \| last3=Crnojević \| first3=Denija \| last4=Jones \| first4=Michael G. \| last5=Caldwell \| first5=Nelson \| last6=Guhathakurta \| first6=Puragra \| last7=Seth \| first7=Anil C. \| last8=Simon \| first8=Joshua D. \| last9=Spekkens \| first9=Kristine \| last10=Strader \| first10=Jay \| last11=Toloba \| first11=Elisa \| journal=The Astrophysical Journal \| volume=926 \| issue=1 \| page=77 }} \| \| align="center" \| Sculptor Group \| \|
193 \| align="center" \| \|Scl-MM-dw2 \| \| 11.51 \| 3.53 \| −12.10 \| \| align="center" \|Sculptor Group \| \|
194 \| \|M81 Dwarf A (KDG 52) \| I? \| 11.58 \| 3.55 \| −11.49 \| 16.5 \| align="center" \|M81 Group \| \|
194 \| align="center" \| 60px \| KK 77 (F12D1) \| dSph \| 11.58 \| 3.55 \| \| 16.2 \| align="center" \|M81 Group \| \|
196 \| align="center" \| 60px \| NGC 2976 \| SAc pec HII \| 11.61 \| 3.56 \| −17.1 \| 10.82 \| align="center" \|M81 Group \| \|
196 \| \| Camelopardalis A \| \| 11.61 \| 3.56 \| \| \| align="center" \|IC 342/Maffei Group \| Satellite of IC 342 \|
198 \| \| KK 211 (AM 1339–445) \| dSph{{cite journal\|bibcode=2008ApJ...674..909P\|doi=10.1086/525038\|title=VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies\|year=2008\|last1=Puzia\|first1=Thomas H.\|last2=Sharina\|first2=Margarita E.\|journal=The Astrophysical Journal\|volume=674\|issue=2\|pages=909–926\|arxiv=0710.1550 \|s2cid=14231914}} \| 11.68 \| 3.58 \| −11.93 \| 16.32 \| align="center" \|Centaurus A/M83 Group \| Satellite of NGC 5128 \|
198 \| \| PGC 51659 (UKS 1424–460) \| IBm{{cite journal\|doi=10.1093/mnras/stu1646\|title=Deep near-infrared surface photometry and properties of Local Volume dwarf irregular galaxies\|year=2014\|last1=Young\|first1=T.\|last2=Jerjen\|first2=H.\|last3=López-Sánchez\|first3=Á. R.\|last4=Koribalski\|first4=B. S.\|journal=Monthly Notices of the Royal Astronomical Society\|volume=444\|issue=4\|pages=3052–3077\|doi-access=free \|arxiv=1408.2609}} \| 11.68 \| 3.58 \| −11.83 \| 16.50 \| align="center" \|Centaurus A/M83 Group \| \|
198 \| \| KDG 61 \| dE/dSph \| 11.68 \| 3.58{{cite journal\|doi=10.1111/j.1365-2966.2010.16746.x\|title=Star formation history of KDG 61 and KDG 64 from spectroscopy and colour-magnitude diagrams\|year=2010\|last1=Makarova\|first1=Lidia\|last2=Koleva\|first2=Mina\|last3=Makarov\|first3=Dmitry\|last4=Prugniel\|first4=Philippe\|journal=Monthly Notices of the Royal Astronomical Society\|volume=406\|issue=2\|page=1152\|doi-access=free \|arxiv=1003.6061\|bibcode=2010MNRAS.406.1152M\|s2cid=119281422}} \| −12.84 \| 14.93 \| align="center" \|M81 Group \| \|
201 \| align="center" \| 60px \| NGC 4945 \| SB(s)cd:sp \| 11.70I. D. Karachentsev et al.(2002) New distances to galaxies in the Centaurus A group \| 3.59 \| −20.51 \| 9.3 \| align="center" \|Centaurus A/M83 Group \| \|
202 \| align="center" \| 60px \| NGC 6789 \| Im \| 11.74 \| 3.6 \| −14.32 \| 13.76 \| \| In the Local Void{{cite journal\|bibcode=2014MNRAS.445.1694L\|doi=10.1093/mnras/stu1804\|arxiv=1409.1239\|title=The triggering of starbursts in low-mass galaxies\|year=2014\|last1=Lelli\|first1=Federico\|last2=Verheijen\|first2=Marc\|last3=Fraternali\|first3=Filippo\|journal=Monthly Notices of the Royal Astronomical Society\|volume=445\|issue=2\|pages=1694–1712\|doi-access=free }} \|
202 \| align="center" \| 60px \| Messier 81 \| SA(s)ab, LINER \| 11.74 \| 3.6 \| \| 6.94 \| align="center" \|M81 Group \| Brightest galaxy in M81 Group \| 90,000 ly
202 \| align="center" \| \| UGC 6451 \| \| 11.74 \| 3.6 \| \| 15.4 \| align="center" \| \| \|
204 \| align="center" \| 60px \| Holmberg IX (UGC 5336, DDO 66) \| Irr \| 11.77 \| 3.61 \| \| 14.53 \| align="center" \|M81 Group \| Contains ultraluminous X-ray source (ULX) Holmberg IX X-1 \|
204 \| align="center" \| 60px \| UGCA 292 (CVn I dwA) \| ImIV-V \| 11.77 \| 3.61 \| \| 16.0 \| align="center" \|M94 Group \| \|
206 \| \| BK 5N \| dSph \| 11.84 \| 3.63 \| \| 17.49 \| align="center" \|M81 Group \| \|
207 \| \| DDO 78 (KK 89) \| dSph \| 11.94 \| 3.66{{cite journal\|bibcode=2009ApJS..183...67D\|doi=10.1088/0067-0049/183/1/67\|title=The ACS Nearby Galaxy Survey Treasury\|year=2009\|last1=Dalcanton\|first1=Julianne J.\|last2=Williams\|first2=Benjamin F.\|last3=Seth\|first3=Anil C.\|last4=Dolphin\|first4=Andrew\|last5=Holtzman\|first5=Jon\|last6=Rosema\|first6=Keith\|last7=Skillman\|first7=Evan D.\|last8=Cole\|first8=Andrew\|last9=Girardi\|first9=Léo\|last10=Gogarten\|first10=Stephanie M.\|last11=Karachentsev\|first11=Igor D.\|last12=Olsen\|first12=Knut\|last13=Weisz\|first13=Daniel\|last14=Christensen\|first14=Charlotte\|last15=Freeman\|first15=Ken\|last16=Gilbert\|first16=Karoline\|last17=Gallart\|first17=Carme\|last18=Harris\|first18=Jason\|last19=Hodge\|first19=Paul\|last20=De Jong\|first20=Roelof S.\|last21=Karachentseva\|first21=Valentina\|last22=Mateo\|first22=Mario\|last23=Stetson\|first23=Peter B.\|last24=Tavarez\|first24=Maritza\|last25=Zaritsky\|first25=Dennis\|last26=Governato\|first26=Fabio\|last27=Quinn\|first27=Thomas\|journal=The Astrophysical Journal Supplement Series\|volume=183\|issue=1\|pages=67–108\|arxiv=0905.3737\|s2cid=5032304}} \| \| 16.50 \| align="center" \|M81 Group \| \|
207 \| \| F8D1 \| dSph \| 11.94 \| 3.66 \| −12.20{{cite journal\|doi=10.1088/0004-637X/739/1/5\|title=The ACS Nearby Galaxy Survey Treasury. VIII. The Global Star Formation Histories of 60 Dwarf Galaxies in the Local Volume\|year=2011\|last1=Weisz\|first1=Daniel R.\|last2=Dalcanton\|first2=Julianne J.\|last3=Williams\|first3=Benjamin F.\|last4=Gilbert\|first4=Karoline M.\|last5=Skillman\|first5=Evan D.\|last6=Seth\|first6=Anil C.\|last7=Dolphin\|first7=Andrew E.\|last8=McQuinn\|first8=Kristen B. W.\|last9=Gogarten\|first9=Stephanie M.\|last10=Holtzman\|first10=Jon\|last11=Rosema\|first11=Keith\|last12=Cole\|first12=Andrew\|last13=Karachentsev\|first13=Igor D.\|last14=Zaritsky\|first14=Dennis\|journal=The Astrophysical Journal\|volume=739\|issue=1\|page=5\|arxiv=1101.1093\|bibcode=2011ApJ...739....5W\|s2cid=119230989}} \| 15.70 \| align="center" \|M81 Group \| \|
209 \| align="center" \|60px \| UGC 4459 (DDO 53) \| Im \| 12.00 \| 3.68{{cite journal\|doi=10.1093/mnras/stab2710\|arxiv=2109.08526\|title=Star formation in the nearby dwarf galaxy DDO 53: Interplay between gas accretion and stellar feedback\|year=2021\|last1=Egorov\|first1=Oleg V.\|last2=Lozinskaya\|first2=Tatiana A.\|last3=Vasiliev\|first3=Konstantin I.\|last4=Yarovova\|first4=Anastasiya D.\|last5=Gerasimov\|first5=Ivan S.\|last6=Kreckel\|first6=Kathryn\|last7=Moiseev\|first7=Alexei V.\|journal=Monthly Notices of the Royal Astronomical Society\|volume=508\|issue=2\|pages=2650–2667\|doi-access=free }} \| −13.37 \| 14.48 \| align="center" \|M81 Group \| \|
210 \| align="center" \| 60px \| Centaurus A (NGC 5128) \| S0 pec \| 12.01 \| 3.68 \| \| 6.84 \| align="center" \|Centaurus A/M83 Group \| Brightest galaxy in Centaurus A Group and brightest and nearest radio galaxy \| 60,000 ly
211 \| \| KDG 64 (UGC 5442) \| dE/dSph \| 12.07 \| 3.70 \| −12.55 \| 15.29 \| align="center" \|M81 Group \| \|
212 \| \| IKN \| dE \| 12.23 \| 3.75 \| −14.29{{cite journal\|doi=10.3847/1538-4357/ab44a7\|title=Stellar Population and Structural Properties of Dwarf Galaxies and Young Stellar Systems in the M81 Group\|year=2019\|last1=Okamoto\|first1=Sakurako\|last2=Arimoto\|first2=Nobuo\|last3=Ferguson\|first3=Annette M. N.\|last4=Irwin\|first4=Mike J.\|last5=Bernard\|first5=Edouard J.\|last6=Utsumi\|first6=Yousuke\|journal=The Astrophysical Journal\|volume=884\|issue=2\|page=128\|arxiv=1909.12997\|bibcode=2019ApJ...884..128O\|s2cid=203593758 \|doi-access=free }} \| \| align="center" \|M81 Group \| \|
212 \| \| KKs 54 \| dSph \| 12.23 \| 3.75 \| −10.41 \| \| align="center" \|Centaurus A/M83 Group \| \|
213 \|align="center"\| 60px \| NGC 5011C (ESO 269–68) \| dE/Im{{cite journal\|doi=10.1086/512157\|title=NGC 5011C: An Overlooked Dwarf Galaxy in the Centaurus A Group\|last1=Saviane\|first1=Ivo\|last2=Jerjen\|first2=Helmut\|year=2007\|journal=The Astronomical Journal\|volume=133\|issue=4\|pages=1756–1762\|arxiv=astro-ph/0701280\|bibcode=2007AJ....133.1756S\|s2cid=14755909 }} \| 12.3 \| 3.77{{cite journal \| title=Dual Stellar Halos in the Standard Elliptical Galaxy M105 and Formation of Massive Early-type Galaxies \| last1=Lee \| first1=Myung Gyoon \| last2=Jang \| first2=In Sung \| journal=The Astrophysical Journal \| volume=822 \| issue=2 \| id=70 \| pages=17 \| date=May 2016 \| doi=10.3847/0004-637X/822/2/70 \| bibcode=2016ApJ...822...70L \| arxiv=1601.06798 \| s2cid=118372642 \| doi-access=free }} \| −14.74 \| 13.47 \| align="center" \|Centaurus A/M83 Group \| \|
213 \| align="center" \| \| Centaurus N \| \| 12.3 \| 3.77{{cite journal\|doi=10.1051/0004-6361/200913429\|title=A close look at the Centaurus a group of galaxies\|year=2010\|last1=Crnojević\|first1=D.\|last2=Grebel\|first2=E. K.\|last3=Koch\|first3=A.\|journal=Astronomy and Astrophysics\|volume=516\|pages=A85\|doi-access=free\|arxiv=1002.0341}} \| −11.15 \| \| align="center" \|Centaurus A/M83 Group \| \|
213 \| align="center" \| \| KK 213 \| dSph \| 12.3 \| 3.77 \| \| 18.00 \| align="center" \|Centaurus A/M83 Group \| \|
213 \| align="center" \| \| KK 203 \| dSph \| 12.30 \| 3.77{{cite journal\|doi=10.1051/0004-6361/202039359\|title=The properties of dwarf spheroidal galaxies in the Cen A group. Stellar populations, internal dynamics, and a heart-shaped Hα ring\|year=2021\|last1=Müller\|first1=Oliver\|last2=Fahrion\|first2=Katja\|last3=Rejkuba\|first3=Marina\|last4=Hilker\|first4=Michael\|last5=Lelli\|first5=Federico\|last6=Lutz\|first6=Katharina\|last7=Pawlowski\|first7=Marcel S.\|last8=Coccato\|first8=Lodovico\|last9=Anand\|first9=Gagandeep S.\|last10=Jerjen\|first10=Helmut\|journal=Astronomy & Astrophysics\|volume=645\|pages=A92\|arxiv=2011.04990\|s2cid=226289648\|bibcode=2021A&A...645A..92M}} \| −11.7 \| \| align="center" \|Centaurus A/M83 Group \| In Centaurus A Group; contains a ring of Hα emission \|
rowspan="2" align="center"\|# ! rowspan="2" \| ! rowspan="2" \|Galaxy ! rowspan="2" \|Type ! colspan="2" \|Dist from Earth ! colspan="2" \|Magnitude ! rowspan="2" align="center"\|Group Membership ! rowspan="2" \|Notes !
Mly ! Mpc ! M ! m !

class="wikitable sortable" style="font-size: 90%

align="center" |#

!Picture

!Galaxy

!Type

! colspan="2" |Distance from Earth

! colspan="2" |Magnitude

! align="center" |Group
Membership

!Notes

! data-sort-type="number" |Diameter (ly)

|60px

|Milky Way

|Barred spiral galaxy

| 0.0265
(to the galactic center)Earth is 8,122 ± 31 parsecs (26,490 ± 100 ly) or 0.0265 million light years from the galactic center (the center of the Milky Way). The distance of Earth from the galaxy which contains it is of course "zero"

| align="center" | 0.008

| −20.8

| n/a

|Local Group

|Home galaxy of Earth. Barred spiral galaxy.

|87,400 ly

| Ursa Major III

| Dwarf spheroidal galaxy

| 0.10758

| 0.033

| 0.010{{Citation |last1=Smith |first1=Simon E. T. |last2=Cerny |first2=William |last3=Hayes |first3=Christian R. |last4=Sestito |first4=Federico |last5=Jensen |first5=Jaclyn |last6=McConnachie |first6=Alan W. |last7=Geha |first7=Marla|author7-link= Marla Geha |last8=Navarro |first8=Julio |last9=Li |first9=Ting S. |date=January 2024 |title=The discovery of the faintest known Milky Way satellite using UNIONS |journal=The Astrophysical Journal |volume=961 |issue=1 |pages=92 |doi=10.3847/1538-4357/ad0d9f |doi-access=free |arxiv=2311.10147 |bibcode=2024ApJ...961...92S}}

| +2.2

| 18.87

| align="center"|Local Group

| Satellite of Milky Way

|File:Draco II Dwarf Galaxy.jpg

| Draco II

| dSph

| 0.0701

| 0.0215{{cite journal|doi=10.1093/mnras/sty1986|title=Pristine dwarf galaxy survey – I. A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite|year=2018|last1=Longeard|first1=Nicolas|last2=Martin|first2=Nicolas|last3=Starkenburg|first3=Else|last4=Ibata|first4=Rodrigo A.|last5=Collins|first5=Michelle L M.|last6=Geha|first6=Marla|author6-link= Marla Geha |last7=Laevens|first7=Benjamin P M.|last8=Rich|first8=R Michael|last9=Aguado|first9=David S.|last10=Arentsen|first10=Anke|last11=Carlberg|first11=Raymond G.|last12=Côté|first12=Patrick|last13=Hill|first13=Vanessa|last14=Jablonka|first14=Pascale|last15=González Hernández|first15=Jonay I.|last16=Navarro|first16=Julio F.|last17=Sánchez-Janssen|first17=Rubén|last18=Tolstoy|first18=Eline|last19=Venn|first19=Kim A.|last20=Youakim|first20=Kris|journal=Monthly Notices of the Royal Astronomical Society|volume=480|issue=2|pages=2609–2627|doi-access=free |arxiv=1807.10655|bibcode=2018MNRAS.480.2609L}}

| −0.8

| 15.87

| align="center"|Local Group

| Satellite of Milky Way

| 120 ly

|File:Tucana III.jpg

| Tucana III

| dSph

| 0.2445

| 0.0747

| 0.0229

| −1.3

| 15.5Calculated from the distance modulus ( $m - M$ ) and the absolute magnitude ( $M_{V}$ )

| align="center"|Local Group

| Satellite of Milky Way that is being tidally disrupted

| Segue 1

| dSph or Glob Clus

| 0.075

| 0.023

| −3.0

| 13.8

| align="center"|Local Group

| Satellite of Milky Way

| align="center"| 60px

| Sagittarius Dwarf Sphr SagDEG

| dSph/E7

| 0.078

| 0.024{{cite journal

| author=I. D. Karachentsev

| title=The Local Group and Other Neighboring Galaxy Groups

| journal=Astronomical Journal

| date=2005

| volume=129

| issue=1

| pages=178–188

| bibcode=2005AJ....129..178K | doi=10.1086/426368

|arxiv = astro-ph/0410065 | s2cid=119385141

}}

| −12.67

| 4.5{{cite web |title=NASA/IPAC Extragalactic Database |url=http://nedwww.ipac.caltech.edu/ |access-date=2008-06-20 |archive-date=2011-05-14 |archive-url=https://web.archive.org/web/20110514100451/http://nedwww.ipac.caltech.edu/ |url-status=live }} Retrieved 2008.

| align="center"|Local Group

| Satellite of Milky Way (partial accretion by Milky Way)

|10,000 ly

| Hydrus I

| 0.09128

| 0.09

| 0.0276{{cite journal|bibcode=2018MNRAS.479.5343K|title=Snake in the Clouds: A new nearby dwarf galaxy in the Magellanic bridge|last1=Koposov|first1=Sergey E.|last2=Walker|first2=Matthew G.|last3=Belokurov|first3=Vasily|last4=Casey|first4=Andrew R.|last5=Geringer-Sameth|first5=Alex|last6=MacKey|first6=Dougal|last7=Da Costa|first7=Gary|last8=Erkal|first8=Denis|last9=Jethwa|first9=Prashin|last10=Mateo|first10=Mario|last11=Olszewski|first11=Edward W.|last12=Bailey|first12=John I.|journal=Monthly Notices of the Royal Astronomical Society|year=2018|volume=479|issue=4|pages=5343|doi=10.1093/mnras/sty1772|doi-access=free |arxiv=1804.06430}}

| −4.71

| 12.49

| align="center"|Local Group

| Satellite of Milky Way, possibly associated with the Magellanic Clouds

| 348 ly

| align="center"|

| Carina III

| 0.0907

| 0.0278

| −2.4

| 14.82

| align="center"|Local Group

| Satellite of Milky Way

| 200 ly

| Ursa Major II Dwarf

| dSph

| 0.098

| 0.030

| −4.2

| 14.3

| align="center"|Local Group

| Satellite of Milky Way (accretion by Milky Way)

|data-sort-value="1800"|~1,800 ly

| Triangulum II

| 0.098

| 0.030

| −1.8

| 15.6

| align="center"|Local Group

| Satellite of Milky Way (accretion by Milky Way)

| align="center"|

| Reticulum II

| 0.102

| 0.0314{{cite journal|doi= 10.3847/1538-4357/aacd0e|title= A Deeper Look at the New Milky Way Satellites: Sagittarius II, Reticulum II, Phoenix II, and Tucana III|year= 2018|last1= Mutlu-Pakdil|first1= Burçin|last2= Sand|first2= David J.|last3= Carlin|first3= Jeffrey L.|last4= Spekkens|first4= Kristine|last5= Caldwell|first5= Nelson|last6= Crnojević|first6= Denija|last7= Hughes|first7= Allison K.|last8= Willman|first8= Beth|last9= Zaritsky|first9= Dennis|journal= The Astrophysical Journal|volume= 863|issue= 1|pages= 25|arxiv= 1804.08627|bibcode= 2018ApJ...863...25M|s2cid= 118877962|doi-access= free}}

| −3.1

| 14.4

| align="center"|Local Group

| Satellite of Milky Way

| 378 ly

| align="center"|

| Segue 2

| dSph

| 0.114

| 0.035{{cite journal|last=Belokurov|first=V.|author2=Walker, M.G. |author3=Evans, N.W. |display-authors=etal |title=Segue 2: A Prototype of the Population of Satellites of Satellites|date=2009|journal=Mon. Not. R. Astron. Soc.|volume=397|issue=4|pages=1748–1755|doi=10.1111/j.1365-2966.2009.15106.x

|doi-access=free |bibcode=2009MNRAS.397.1748B|arxiv=0903.0818|s2cid=20051174}}

| −2.5

| align="center"|Local Group

| Satellite of Milky Way, one of the smallest known galaxies

| 220 ly

| align="center"|

| Carina II

| 0.122

| 0.0374{{cite journal|bibcode=2018ApJ...857..145L|title=Ships Passing in the Night: Spectroscopic Analysis of Two Ultra-faint Satellites in the Constellation Carina|last1=Li|first1=T. S.|last2=Simon|first2=J. D.|last3=Pace|first3=A. B.|last4=Torrealba|first4=G.|last5=Kuehn|first5=K.|last6=Drlica-Wagner|first6=A.|last7=Bechtol|first7=K.|last8=Vivas|first8=A. K.|last9=Van Der Marel|first9=R. P.|last10=Wood|first10=M.|last11=Yanny|first11=B.|last12=Belokurov|first12=V.|last13=Jethwa|first13=P.|last14=Zucker|first14=D. B.|last15=Lewis|first15=G.|last16=Kron|first16=R.|last17=Nidever|first17=D. L.|last18=Sánchez-Conde|first18=M. A.|last19=Ji|first19=A. P.|last20=Conn|first20=B. C.|last21=James|first21=D. J.|last22=Martin|first22=N. F.|last23=Martinez-Delgado|first23=D.|last24=Noël|first24=N. E. D.|author25=MagLiteS Collaboration|journal=The Astrophysical Journal|year=2018|volume=857|issue=2|pages=145|doi=10.3847/1538-4357/aab666|arxiv=1802.06810|s2cid=96446126 |doi-access=free }}

| −4.5

| 13.36

| align="center"|Local Group

| Satellite of Milky Way

| 590 ly

| align="center"|

| Willman 1

| dSph or Star Clus

| 0.124

| 0.038

| −2.7

| align="center"|Local Group

| Satellite of Milky Way

| align="center"|

| Boötes II

| dSph

| 0.137

| 0.042{{cite journal|author1=Martin, Nicolas F.|author2=de Jong, Jelte T. A.|author3=Rix, Hans-Walter|date=September 2008|title=A Comprehensive Maximum Likelihood Analysis of the Structural Properties of Faint Milky Way Satellites|journal=The Astrophysical Journal|volume=684|issue=2|pages=1075–1092|bibcode=2008ApJ...684.1075M|doi=10.1086/590336|arxiv=0805.2945|s2cid=17838966}}

| −2.7

| align="center"|Local Group

| Satellite of Milky Way

| align="center"|

| Coma Berenices Dwarf

| dSph

| 0.137

| 0.042{{cite journal|last=Musella|first=Ilaria|author2=Ripepi, Vincenzo |author3=Clementini, Gisella |title=Pulsating Variable Stars in the Coma Berenices Dwarf Spheroidal Galaxy|year=2009|journal=The Astrophysical Journal Letters|volume=695|issue=1|pages=L83–1L87|doi=10.1088/0004-637X/695/1/L83|bibcode=2009ApJ...695L..83M |arxiv=0902.4230 |s2cid=11594422|display-authors=etal}}

| −3.6

| align="center"|Local Group

| Satellite of Milky Way

| align="center"|

| Pictor II

| 0.147

| 0.045{{cite journal|bibcode=2016ApJ...833L...5D|title=An Ultra-faint Galaxy Candidate Discovered in Early Data from the Magellanic Satellites Survey|last1=Drlica-Wagner|first1=A.|last2=Bechtol|first2=K.|last3=Allam|first3=S.|last4=Tucker|first4=D. L.|last5=Gruendl|first5=R. A.|last6=Johnson|first6=M. D.|last7=Walker|first7=A. R.|last8=James|first8=D. J.|last9=Nidever|first9=D. L.|last10=Olsen|first10=K. A. G.|last11=Wechsler|first11=R. H.|last12=Cioni|first12=M. R. L.|last13=Conn|first13=B. C.|last14=Kuehn|first14=K.|last15=Li|first15=T. S.|last16=Mao|first16=Y. -Y.|last17=Martin|first17=N. F.|last18=Neilsen|first18=E.|last19=Noel|first19=N. E. D.|last20=Pieres|first20=A.|last21=Simon|first21=J. D.|last22=Stringfellow|first22=G. S.|last23=Van Der Marel|first23=R. P.|last24=Yanny|first24=B.|journal=The Astrophysical Journal|year=2016|volume=833|issue=1|pages=L5|doi=10.3847/2041-8205/833/1/L5|arxiv=1609.02148|s2cid=56071154 |doi-access=free }}

| −3.2

| 15.1

| align="center"|Local Group

| Satellite of Milky Way possibly associated with the Large Magellanic Cloud

| 300 ly

| align="center"|

| Boötes III

| dSph

| 0.150

| 0.046{{cite journal|last=Grillmair|first=C.J.|title=Four New Stellar Debris Streams in the Galactic Halo|date=2009|journal=The Astrophysical Journal|volume=693|issue=2|pages=1118–1127|doi=10.1088/0004-637X/693/2/1118|bibcode=2009ApJ...693.1118G|arxiv=0811.3965 |s2cid=17328907}}

| −5.8{{cite journal|last1=Carlin|first1=Jeffrey L.|last2=Grillmair|first2=Carl J.|last3=Muñoz|first3=Ricardo R.|title=Kinematics and Metallicities in the Boötes III Stellar Overdensity: a Disrupted Dwarf Galaxy?|date=September 2009|journal=The Astrophysical Journal Letters|volume=702|issue=1|pages=L9–L13|doi=10.1088/0004-637X/702/1/L9|bibcode=2009ApJ...702L...9C|arxiv=0907.3738 |s2cid=62784400|display-authors=etal}}

| align="center"|Local Group

| Satellite of Milky Way

| align="center"|

| Tucana IV

| 0.157

| 0.048

| −3.5

| 14.9

| align="center"|Local Group

| Satellite of Milky Way

| align="center"| 60px

| Large Magellanic Cloud (LMC)

| SB(s)m

| 0.163

| 0.050

| −17.93

| 0.9

| align="center"|Local Group

| Satellite of Milky Way

|32,200 ly

| align="center"|

| Grus II

| 0.179

| 0.055

| −3.9

| align="center"|Local Group

| Satellite of Milky Way

| 607 ly

| align="center"|

| Tucana II

| 0.186

| 0.057{{cite journal|bibcode=2016ApJ...819...53W|arxiv=1511.06296|doi=10.3847/0004-637X/819/1/53|title= Magellan/M2FS Spectroscopy of Tucana 2 and Grus 1|year=2016|last1=Walker|first1=Matthew G.|last2=Mateo|first2=Mario|last3=Olszewski|first3=Edward W.|last4=Koposov|first4=Sergey|last5=Belokurov|first5=Vasily|last6=Jethwa|first6=Prashin|last7=Nidever|first7=David L.|last8=Bonnivard|first8=Vincent|last9=Iii|first9=John I. Bailey|last10=Bell|first10=Eric F.|last11=Loebman|first11=Sarah R.|journal=The Astrophysical Journal|volume=819|issue=1|pages=53|s2cid=118507573 |doi-access=free }}

| −3.8

| 15.0

| align="center"|Local Group

| Satellite of Milky Way

|1080 ly

| align="center"| 60px

| Boötes I

| dSph

| 0.197

| 0.060

| −5.8Belokurov, 2006 A Faint New Milky Way Satellite in Bootes

| 13.1

| align="center"|Local Group

| Satellite of Milky Way

| align="center"| 60px

| Small Magellanic Cloud (SMC, NGC 292)

| SB(s)m pec

| 0.205

| 0.063

| −16.35

| 2.7

| align="center"|Local Group

| Satellite of Milky Way

|18,900 ly

| align="center"| 60px

| Ursa Minor Dwarf

| dE4

| 0.205

| 0.063

| −7.13

| 11.9

| align="center"|Local Group

| Satellite of Milky Way

| Virgo II

| 0.235

| 0.072

| −1.6

| 17.7

| align="center" |Local Group

| Satellite of Milky Way

| align="center"|

| Eridanus IV

| 0.250

| 0.0767{{cite journal|doi=10.3847/2041-8213/ac2d9a|title=Eridanus IV: An Ultra-faint Dwarf Galaxy Candidate Discovered in the DECam Local Volume Exploration Survey|year=2021|last1=Cerny|first1=W.|last2=Pace|first2=A. B.|last3=Drlica-Wagner|first3=A.|last4=Koposov|first4=S. E.|last5=Vivas|first5=A. K.|last6=Mau|first6=S.|last7=Riley|first7=A. H.|last8=Bom|first8=C. R.|last9=Carlin|first9=J. L.|last10=Choi|first10=Y.|last11=Erkal|first11=D.|last12=Ferguson|first12=P. S.|last13=James|first13=D. J.|last14=Li|first14=T. S.|last15=Martínez-Delgado|first15=D.|last16=Martínez-Vázquez|first16=C. E.|last17=Munoz|first17=R. R.|last18=Mutlu-Pakdil|first18=B.|last19=Olsen|first19=K. A. G.|last20=Pieres|first20=A.|last21=Sakowska|first21=J. D.|last22=Sand|first22=D. J.|last23=Simon|first23=J. D.|last24=Smercina|first24=A.|last25=Stringfellow|first25=G. S.|last26=Tollerud|first26=E. J.|last27=Adamów|first27=M.|last28=Hernandez-Lang|first28=D.|last29=Kuropatkin|first29=N.|last30=Santana-Silva|first30=L.|journal=The Astrophysical Journal Letters|volume=920|issue=2|pages=L44|arxiv=2107.09080|bibcode=2021ApJ...920L..44C|s2cid=236134310|display-authors=1 |doi-access=free }}

| −4.7

| 14.72

| align="center"|Local Group

| Satellite of Milky Way

| 489 ly

| align="center"|

| Horologium II

| 0.254

| 0.078{{cite journal|bibcode=2018ApJ...867...19K|title=The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies|last1=Kallivayalil|first1=Nitya|last2=Sales|first2=Laura V.|last3=Zivick|first3=Paul|last4=Fritz|first4=Tobias K.|last5=Del Pino|first5=Andrés|last6=Sohn|first6=Sangmo Tony|last7=Besla|first7=Gurtina|last8=Van Der Marel|first8=Roeland P.|last9=Navarro|first9=Julio F.|last10=Sacchi|first10=Elena|journal=The Astrophysical Journal|year=2018|volume=867|issue=1|pages=19|doi=10.3847/1538-4357/aadfee|arxiv=1805.01448|s2cid=55073922 |doi-access=free }}

| −2.6

| 1.69

| align="center"|Local Group

| Satellite of Milky Way

| 287 ly{{cite journal|bibcode=2018ApJ...860...66M|title=A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters|last1=Muñoz|first1=Ricardo R.|last2=Côté|first2=Patrick|last3=Santana|first3=Felipe A.|last4=Geha|first4=Marla|author4-link= Marla Geha |last5=Simon|first5=Joshua D.|last6=Oyarzún|first6=Grecco A.|last7=Stetson|first7=Peter B.|last8=Djorgovski|first8=S. G.|journal=The Astrophysical Journal|year=2018|volume=860|issue=1|pages=66|doi=10.3847/1538-4357/aac16b|arxiv=1806.06891 |doi-access=free}}

| align="center"| 60px

| Draco Dwarf (DDO 208)

| dE0 pec

| 0.258

| 0.079

| −8.74

| 10.9

| align="center"|Local Group

| Satellite of Milky Way with a large amount of dark matter

|data-sort-value="2700"|~2,700 × 1,900 ly

| Horologium I

| 0.258

| 0.079{{cite journal|doi=10.1088/0004-637X/811/1/62|title=Kinematics and Chemistry of Recently Discovered Reticulum 2 and Horologium 1 Dwarf Galaxies|year=2015|last1=Koposov|first1=Sergey E.|last2=Casey|first2=Andrew R.|last3=Belokurov|first3=Vasily|last4=Lewis|first4=James R.|last5=Gilmore|first5=Gerard|last6=Worley|first6=Clare|last7=Hourihane|first7=Anna|last8=Randich|first8=S.|last9=Bensby|first9=T.|last10=Bragaglia|first10=A.|last11=Bergemann|first11=M.|last12=Carraro|first12=G.|last13=Costado|first13=M. T.|last14=Flaccomio|first14=E.|last15=Francois|first15=P.|last16=Heiter|first16=U.|last17=Hill|first17=V.|last18=Jofre|first18=P.|last19=Lando|first19=C.|last20=Lanzafame|first20=A. C.|last21=Laverny|first21=P. de|last22=Monaco|first22=L.|last23=Morbidelli|first23=L.|last24=Sbordone|first24=L.|last25=Mikolaitis|first25=Š.|last26=Ryde|first26=N.|journal=The Astrophysical Journal|volume=811|issue=1|pages=62|arxiv=1504.07916|bibcode=2015ApJ...811...62K|s2cid=53419855}}

| -3.4

| align="center"|Local Group

| Satellite of Milky Way

| 196 ly

| align="center"|

| Pisces Overdensity

| dIrr/dSph{{cite journal | bibcode=2009ApJ...697.1993B | doi=10.1088/0004-637X/697/2/1993 | arxiv=0903.3871 | title=Aspitzerstudy of Asymptotic Giant Branch Stars. Iii. Dust Production and Gas Return in Local Group Dwarf Irregular Galaxies | journal=The Astrophysical Journal | volume=697 | issue=2 | pages=1993–2014 | year=2009 | last1=Boyer | first1=Martha L | last2=Skillman | first2=Evan D | last3=Van Loon | first3=Jacco Th | last4=Gehrz | first4=Robert D | last5=Woodward | first5=Charles E | s2cid=12162514 }}

| 0.26

| 0.08{{citation | display-authors=1 | last1=Watkins | first1=L. L. | last2=Evans | first2=N. W. | last3=Belokurov | first3=V. | last4=Smith | first4=M. C. | last5=Hewett | first5=P. C. | last6=Bramich | first6=D. M. | last7=Gilmore | first7=G. F. | last8=Irwin | first8=M. J. | last9=Vidrih | first9=S. | last10=Wyrzykowski | first10=Ł. | last11=Zucker | first11=D. B. | title=Substructure revealed by RR Lyraes in SDSS Stripe 82 | date=2009 | journal=Monthly Notices of the Royal Astronomical Society | volume=398 | issue=4 | pages=1757–70 | doi=10.1111/j.1365-2966.2009.15242.x | doi-access=free | bibcode=2009MNRAS.398.1757W | arxiv=0906.0498 | s2cid=14409027 | postscript=. }}

| −10.35

| align="center"|Local Group

| Satellite of Milky Way

| Leo Minor I

| 0.267

| 0.082

| −2.4

| 17.16

| align="center" |Local Group

| Satellite of Milky Way

| Aquarius III

| 0.277

| 0.085{{cite journal|doi=10.3847/1538-4357/ad8eba|doi-access=free |title=Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy |date=2025 |last1=Cerny |first1=W. |last2=Chiti |first2=A. |last3=Geha |first3=M. |last4=Mutlu-Pakdil |first4=B. |last5=Drlica-Wagner |first5=A. |last6=Tan |first6=C. Y. |last7=Adamów |first7=M. |last8=Pace |first8=A. B. |last9=Simon |first9=J. D. |last10=Sand |first10=D. J. |last11=Ji |first11=A. P. |last12=Li |first12=T. S. |last13=Vivas |first13=A. K. |last14=Bell |first14=E. F. |last15=Carlin |first15=J. L. |last16=Carballo-Bello |first16=J. A. |last17=Chaturvedi |first17=A. |last18=Choi |first18=Y. |last19=Doliva-Dolinsky |first19=A. |last20=Gnedin |first20=O. Y. |last21=Limberg |first21=G. |last22=Martínez-Vázquez |first22=C. E. |last23=Mau |first23=S. |last24=Medina |first24=G. E. |last25=Navabi |first25=M. |last26=Noël |first26=N. E. D. |last27=Placco |first27=V. M. |last28=Riley |first28=A. H. |last29=Roederer |first29=I. U. |last30=Stringfellow |first30=G. S. |journal=The Astrophysical Journal |volume=979 |issue=2 |page=164 |arxiv=2410.00981 |bibcode=2025ApJ...979..164C |display-authors=1 }}

| −2.5

| align="center" | Local Group

| Satellite of the Milky Way

| 330 ly

|Sextans Dwarf Sph

| dSph

| 0.280

| 0.086

| −7.98

| 12

| align="center" |Local Group

| Satellite of Milky Way

|8,400 ly

| align="center" |60px

|Sculptor Dwarf (ESO 351-G30)

| dE3

| 0.287

| 0.088

| −9.77

| 10.1

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Pegasus IV

| 0.294

| 0.090{{cite journal | arxiv=2203.11788 | doi=10.3847/1538-4357/aca1c3 | title=Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus | year=2023 | last1=Cerny | first1=W. | last2=Simon | first2=J. D. | last3=Li | first3=T. S. | last4=Drlica-Wagner | first4=A. | last5=Pace | first5=A. B. | last6=Martínez-Vázquez | first6=C. E. | last7=Riley | first7=A. H. | last8=Mutlu-Pakdil | first8=B. | last9=Mau | first9=S. | last10=Ferguson | first10=P. S. | last11=Erkal | first11=D. | last12=Munoz | first12=R. R. | last13=Bom | first13=C. R. | last14=Carlin | first14=J. L. | last15=Carollo | first15=D. | last16=Choi | first16=Y. | last17=Ji | first17=A. P. | last18=Manwadkar | first18=V. | last19=Martínez-Delgado | first19=D. | last20=Miller | first20=A. E. | last21=Noël | first21=N. E. D. | last22=Sakowska | first22=J. D. | last23=Sand | first23=D. J. | last24=Stringfellow | first24=G. S. | last25=Tollerud | first25=E. J. | last26=Vivas | first26=A. K. | last27=Carballo-Bello | first27=J. A. | last28=Hernandez-Lang | first28=D. | last29=James | first29=D. J. | last30=Nidever | first30=D. L. | journal=The Astrophysical Journal | volume=942 | issue=2 | page=111 | bibcode=2023ApJ...942..111C | s2cid=247597301 | display-authors=1 | doi-access=free }}

| −4.25

| 15.52

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Virgo I

| 0.297

| 0.091

| −0.3

| 19.5

| align="center" |Local Group

| Satellite of Milky Way

| align="center"|

| Reticulum III

| 0.300

| 0.092{{cite journal|doi=10.1088/0004-637X/813/2/109|title=Eight Ultra-Faint Galaxy Candidates Discovered in Year Two of the Dark Energy Survey|year=2015|last1=Drlica-Wagner|first1=A.|last2=Bechtol|first2=K.|last3=Rykoff|first3=E. S.|last4=Luque|first4=E.|last5=Queiroz|first5=A.|last6=Mao|first6=Y.-Y.|last7=Wechsler|first7=R. H.|last8=Simon|first8=J. D.|last9=Santiago|first9=B.|last10=Yanny|first10=B.|last11=Balbinot|first11=E.|last12=Dodelson|first12=S.|last13=Neto|first13=A. Fausti|last14=James|first14=D. J.|last15=Li|first15=T. S.|last16=Maia|first16=M. A. G.|last17=Marshall|first17=J. L.|last18=Pieres|first18=A.|last19=Stringer|first19=K.|last20=Walker|first20=A. R.|last21=Abbott|first21=T. M. C.|last22=Abdalla|first22=F. B.|last23=Allam|first23=S.|last24=Benoit-Lévy|first24=A.|last25=Bernstein|first25=G. M.|last26=Bertin|first26=E.|last27=Brooks|first27=D.|last28=Buckley-Geer|first28=E.|author28-link=Elizabeth Buckley-Geer|last29=Burke|first29=D. L.|last30=Rosell|first30=A. Carnero|journal=The Astrophysical Journal|volume=813|issue=2|pages=109|arxiv=1508.03622|bibcode=2015ApJ...813..109D|s2cid=55909299|display-authors=29}}

| −3.3

| 16.51

| align="center"|Local Group

| Satellite of Milky Way

| 420 ly

|Ursa Major I Dwarf (UMa I dSph)

| dSph

| 0.3157

| 0.0968

| −6.75Willman, Dalcanton, Martinez-Delgado, et al. (2005) "A New Milky Way Dwarf Galaxy in

Ursa Major", submitted to Astrophysical Journal Letters, on arXiv.org: [https://arxiv.org/abs/astro-ph/0503552 astro-ph/0503552] {{Webarchive|url=https://web.archive.org/web/20151212194857/http://arxiv.org/abs/astro-ph/0503552 |date=2015-12-12 }}

| align="center" |Local Group

| Satellite of Milky Way

|~2,000 ly

| align="center" |

| Phoenix II

| 0.326

| 0.100{{cite journal|doi=10.1093/mnras/stz2609|title=Search for RR Lyrae stars in DES ultra-faint systems: Grus I, Kim 2, Phoenix II, and Grus II|year=2019|last1=Martínez-Vázquez|first1=C. E.|last2=Vivas|first2=A. K.|last3=Gurevich|first3=M.|last4=Walker|first4=A. R.|last5=McCarthy|first5=M.|last6=Pace|first6=A. B.|last7=Stringer|first7=K. M.|last8=Santiago|first8=B.|last9=Hounsell|first9=R.|last10=Macri|first10=L.|last11=Li|first11=T. S.|last12=Bechtol|first12=K.|last13=Riley|first13=A. H.|last14=Kim|first14=A. G.|last15=Simon|first15=J. D.|last16=Drlica-Wagner|first16=A.|last17=Nadler|first17=E. O.|last18=Marshall|first18=J. L.|last19=Annis|first19=J.|last20=Avila|first20=S.|last21=Bertin|first21=E.|last22=Brooks|first22=D.|last23=Buckley-Geer|first23=E.|last24=Burke|first24=D. L.|last25=Rosell|first25=A Carnero|last26=Kind|first26=M Carrasco|last27=Da Costa|first27=L. N.|last28=De Vicente|first28=J.|last29=Desai|first29=S.|last30=Diehl|first30=H. T.|journal=Monthly Notices of the Royal Astronomical Society|volume=490|issue=2|pages=2183|doi-access=free |arxiv=1909.06308|bibcode=2019MNRAS.490.2183M|display-authors=29}}

| −2.7

| align="center" |Local Group

| Satellite of Milky Way

| 290 ly

|60px

| Carina Dwarf (ESO 206-G220)

| dE3

| 0.33

| 0.10

| −8.97

| 11.3

| align="center" |Local Group

| Satellite of Milky Way

| 1,600 ly

| Boötes V

| 0.333

| 0.102{{cite journal|doi=10.3847/1538-4357/acdd78|doi-access=free |title=Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey |date=2023 |last1=Cerny |first1=W. |last2=Martínez-Vázquez |first2=C. E. |last3=Drlica-Wagner |first3=A. |last4=Pace |first4=A. B. |last5=Mutlu-Pakdil |first5=B. |last6=Li |first6=T. S. |last7=Riley |first7=A. H. |last8=Crnojević |first8=D. |last9=Bom |first9=C. R. |last10=Carballo-Bello |first10=J. A. |last11=Carlin |first11=J. L. |last12=Chiti |first12=A. |last13=Choi |first13=Y. |last14=Collins |first14=M. L. M. |last15=Darragh-Ford |first15=E. |last16=Ferguson |first16=P. S. |last17=Geha |first17=M. |last18=Martínez-Delgado |first18=D. |last19=Massana |first19=P. |last20=Mau |first20=S. |last21=Medina |first21=G. E. |last22=Muñoz |first22=R. R. |last23=Nadler |first23=E. O. |last24=Noël |first24=N. E. D. |last25=Olsen |first25=K. A. G. |last26=Pieres |first26=A. |last27=Sakowska |first27=J. D. |last28=Simon |first28=J. D. |last29=Stringfellow |first29=G. S. |last30=Tollerud |first30=E. J. |journal=The Astrophysical Journal |volume=953 |issue=1 |page=1 |arxiv=2209.12422 |bibcode=2023ApJ...953....1C |display-authors=1 }}

| −3.2

| 16.84

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Aquarius II

| 0.3519

| 0.1079{{cite journal|doi=10.1093/mnras/stw2051|title=At the survey limits: Discovery of the Aquarius 2 dwarf galaxy in the VST ATLAS and the SDSS data|year=2016|last1=Torrealba|first1=G.|last2=Koposov|first2=S. E.|last3=Belokurov|first3=V.|last4=Irwin|first4=M.|last5=Collins|first5=M.|last6=Spencer|first6=M.|last7=Ibata|first7=R.|last8=Mateo|first8=M.|last9=Bonaca|first9=A.|last10=Jethwa|first10=P.|journal=Monthly Notices of the Royal Astronomical Society|volume=463|issue=1|pages=712–722|doi-access=free |arxiv=1605.05338|bibcode=2016MNRAS.463..712T}}

| −4.36

| 15.8

| align="center" |Local Group

| Satellite of Milky Way

| 1,040 ly

| Leo VI

| 0.362

| 0.111{{cite journal|doi=10.3847/1538-4357/ad9b0c|doi-access=free |title=A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Ultra-faint Dwarf Galaxy with DELVE Early Data Release 3 |date=2025 |last1=Tan |first1=C. Y. |last2=Cerny |first2=W. |last3=Drlica-Wagner |first3=A. |last4=Pace |first4=A. B. |last5=Geha |first5=M. |last6=Ji |first6=A. P. |last7=Li |first7=T. S. |last8=Adamów |first8=M. |last9=Anbajagane |first9=D. |last10=Bom |first10=C. R. |last11=Carballo-Bello |first11=J. A. |last12=Carlin |first12=J. L. |last13=Chang |first13=C. |last14=Chaturvedi |first14=A. |last15=Chiti |first15=A. |last16=Choi |first16=Y. |last17=Collins |first17=M. L. M. |last18=Doliva-Dolinsky |first18=A. |last19=Ferguson |first19=P. S. |last20=Gruendl |first20=R. A. |last21=James |first21=D. J. |last22=Limberg |first22=G. |last23=Navabi |first23=M. |last24=Martínez-Delgado |first24=D. |last25=Martínez-Vázquez |first25=C. E. |last26=Medina |first26=G. E. |last27=Mutlu-Pakdil |first27=B. |last28=Nidever |first28=D. L. |last29=Noël |first29=N. E. D. |last30=Riley |first30=A. H. |journal=The Astrophysical Journal |volume=979 |issue=2 |page=176 |arxiv=2408.00865 |bibcode=2025ApJ...979..176T |display-authors=1 }}

| −3.56

| align="center" |Local Group

| Satellite of Milky Way

| 910 ly

| align="center" |

| Pictor I

| 0.372

| 0.114{{cite journal|bibcode=2015ApJ...805..130K|title=Beasts of the Southern Wild: Discovery of Nine Ultra Faint Satellites in the Vicinity of the Magellanic Clouds|last1=Koposov|first1=Sergey E.|last2=Belokurov|first2=Vasily|last3=Torrealba|first3=Gabriel|last4=Evans|first4=N. Wyn|journal=The Astrophysical Journal|year=2015|volume=805|issue=2|pages=130|doi=10.1088/0004-637X/805/2/130|arxiv=1503.02079|s2cid=118267222}}

| −3.1

| 20.3

| align="center" |Local Group

| Satellite of Milky Way

| 190 ly

| align="center" |

|Crater II

| 0.383

| 0.1175

| −8.2

| 12.2

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Grus I

| 0.391

| 0.120

| −3.4

| 17.0

| align="center" |Local Group

| Satellite of Milky Way

| 404 ly

| align="center" |

| Sextans II

| 0.411

| 0.126{{cite journal | last1=Homma | first1=Daisuke | last2=Chiba | first2=Masashi | last3=Komiyama | first3=Yutaka | last4=Tanaka | first4=Masayuki | last5=Okamoto | first5=Sakurako | last6=Tanaka | first6=Mikito | last7=Ishigaki | first7=Miho N | last8=Hayashi | first8=Kohei | last9=Arimoto | first9=Nobuo | last10=Lupton | first10=Robert H | last11=Strauss | first11=Michael A | last12=Miyazaki | first12=Satoshi | last13=Wang | first13=Shiang-Yu | last14=Murayama | first14=Hitoshi | title=Final results of the search for new Milky Way satellites in the Hyper Suprime-Cam Subaru Strategic Program survey: Discovery of two more candidates | journal=Publications of the Astronomical Society of Japan | date=2024-06-08 | volume=76 | issue=4 | pages=733–752 | issn=0004-6264 | doi=10.1093/pasj/psae044| arxiv=2311.05439 }}

|−3.9

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Antlia 2

| 0.430

| 0.1318{{cite journal|doi=10.3847/1538-4357/ac1869|title=Kinematics of Antlia 2 and Crater 2 from the Southern Stellar Stream Spectroscopic Survey (S 5)|year=2021|last1=Ji|first1=Alexander P.|last2=Koposov|first2=Sergey E.|last3=Li|first3=Ting S.|last4=Erkal|first4=Denis|last5=Pace|first5=Andrew B.|last6=Simon|first6=Joshua D.|last7=Belokurov|first7=Vasily|last8=Cullinane|first8=Lara R.|last9=Da Costa|first9=Gary S.|last10=Kuehn|first10=Kyler|last11=Lewis|first11=Geraint F.|last12=MacKey|first12=Dougal|last13=Shipp|first13=Nora|last14=Simpson|first14=Jeffrey D.|last15=Zucker|first15=Daniel B.|last16=Hansen|first16=Terese T.|last17=Bland-Hawthorn|first17=Joss|author18=S5 Collaboration|journal=The Astrophysical Journal|volume=921|issue=1|page=32|arxiv=2106.12656|bibcode=2021ApJ...921...32J|s2cid=235624056 |doi-access=free }}

| −9.86

| align="center" |Local Group

| Satellite of Milky Way, most diffuse galaxy ever found

| align="center" |60px

| Hercules Dwarf

| dSph

| 0.434

| 0.133{{cite journal|last=Sand|first=David J.|author2=Olszewski, Edward W. |author3=Willman, Beth |title=The Star Formation History and Extended Structure of the Hercules Milky Way Satellite|date=2009|journal=The Astrophysical Journal|volume=704|issue=2|pages=898–914|doi=10.1088/0004-637X/704/2/898|bibcode=2009ApJ...704..898S |arxiv=0906.4017 |s2cid=42754875}}

| −5.3

| 14.7

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |60px

|Fornax Dwarf (ESO 356-G04)

| dSph/E2

| 0.466

| 0.143{{cite journal|doi=10.3847/1538-4357/ac5b07|title=Distances to Local Group Galaxies via Population II, Stellar Distance Indicators. II. The Fornax Dwarf Spheroidal |year=2022 |last1=Oakes |first1=Elias K. |last2=Hoyt |first2=Taylor J. |last3=Freedman |first3=Wendy L. |last4=Madore |first4=Barry F. |last5=Tran |first5=Quang H. |last6=Cerny |first6=William |last7=Beaton |first7=Rachael L. |last8=Seibert |first8=Mark |journal=The Astrophysical Journal |volume=929 |issue=2 |page=116 |arxiv=2204.09699 |bibcode=2022ApJ...929..116O |s2cid=248260222 |doi-access=free }}

| −11.5

| 9.28

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

|Canes Venatici II Dwarf

| dSph

| 0.49

| 0.15

| −4.8

| 15.1{{Cite journal | last1 = Belokurov | first1 = V. | last2 = Zucker | first2 = D. B. | last3 = Evans | first3 = N. W. | last4 = Kleyna | first4 = J. T. | last5 = Koposov | first5 = S. | last6 = Hodgkin | first6 = S. T. | last7 = Irwin | first7 = M. J. | last8 = Gilmore | first8 = G. |author-link8 = Gerard F. Gilmore| last9 = Wilkinson | first9 = M. I. | last10 = Fellhauer | doi = 10.1086/509718 | first10 = M. | last11 = Bramich | first11 = D. M. | last12 = Hewett | first12 = P. C. | last13 = Vidrih | first13 = S. | last14 = De Jong | first14 = J. T. A. | last15 = Smith | first15 = J. A. | last16 = Rix | first16 = H. -W. | last17 = Bell | first17 = E. F. | last18 = Wyse | first18 = R. F. G. | last19 = Newberg | first19 = H. J. | last20 = Mayeur | first20 = P. A. | last21 = Yanny | first21 = B. | last22 = Rockosi | first22 = C. M. |author-link22=Constance M. Rockosi| last23 = Gnedin | first23 = O. Y. | last24 = Schneider | first24 = D. P. | last25 = Beers | first25 = T. C. | last26 = Barentine | first26 = J. C. | last27 = Brewington | first27 = H. | last28 = Brinkmann | first28 = J. | last29 = Harvanek | first29 = M. | last30 = Kleinman | first30 = S. J. | title = Cats and Dogs, Hair and a Hero: A Quintet of New Milky Way Companions | journal = The Astrophysical Journal | volume = 654 | issue = 2 | pages = 897–906 | year = 2007 |arxiv = astro-ph/0608448 |bibcode = 2007ApJ...654..897B | s2cid = 18617277 }}

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Hydra II

| dSph

| 0.492

| 0.151{{cite journal|bibcode=2016AJ....151..118V|title=Variable Stars in the Field of the Hydra II Ultra-faint Dwarf Galaxy|last1=Vivas|first1=A. Katherina|last2=Olsen|first2=Knut|last3=Blum|first3=Robert|last4=Nidever|first4=David L.|last5=Walker|first5=Alistair R.|last6=Martin|first6=Nicolas F.|last7=Besla|first7=Gurtina|last8=Gallart|first8=Carme|last9=Van Der Marel|first9=Roeland P.|last10=Majewski|first10=Steven R.|last11=Kaleida|first11=Catherine C.|last12=Muñoz|first12=Ricardo R.|last13=Saha|first13=Abhijit|last14=Conn|first14=Blair C.|last15=Jin|first15=Shoko|journal=The Astronomical Journal|year=2016|volume=151|issue=5|pages=118|doi=10.3847/0004-6256/151/5/118|arxiv=1510.05539|s2cid=53536842 |doi-access=free }}

| −5.1

| align="center" |Local Group

| Satellite of Milky Way

| 500 ly

| align="center" |

| Virgo III

| 0.492

| 0.151

| −2.7

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |60px

| Leo IV Dwarf

| dSph

| 0.502

| 0.154{{cite journal|last1=Sand|first1=David J. |last2=Seth|first2=Anil |last3=Olszewski|first3=Edward W. |display-authors=etal |title=A Deeper Look at Leo IV: Star Formation History and Extended Structure|date=2010|journal=The Astrophysical Journal|volume=718|issue=1 |pages=530–42 |bibcode=2010ApJ...718..530S|doi=10.1088/0004-637X/718/1/530|arxiv=0911.5352|s2cid=32122744 }}

| −5.5

| 15.9

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Leo V Dwarf

| dSph

| 0.571

| 0.175{{Cite journal | last1 = de Jong | first1 = J. T. A. | last2 = Martin | first2 = N. F. | last3 = Rix | first3 = H. W. | last4 = Smith | first4 = K. W. | last5 = Jin | first5 = S. | last6 = Macciò | first6 = A. V. | doi = 10.1088/0004-637X/710/2/1664 | title = The Enigmatic Pair of Dwarf Galaxies Leo Iv and Leo V: Coincidence or Common Origin? | journal = The Astrophysical Journal | volume = 710 | issue = 2 | pages = 1664–1671 | year = 2010 |arxiv = 0912.3251 |bibcode = 2010ApJ...710.1664D | s2cid = 5667891 }}

| −5.2

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Pisces II

| dG{{cite journal|bibcode=2012ApJ...756...79S|doi=10.1088/0004-637X/756/1/79|arxiv=1111.6608|title=Tidal Signatures in the Faintest Milky Way Satellites: The Detailed Properties of Leo V, Pisces II, and Canes Venatici II|journal=The Astrophysical Journal|volume=756|pages=79|year=2012|last1=Sand|first1=David J|last2=Strader|first2=Jay|last3=Willman|first3=Beth|last4=Zaritsky|first4=Dennis|last5=McLeod|first5=Brian|last6=Caldwell|first6=Nelson|last7=Seth|first7=Anil|last8=Olszewski|first8=Edward|issue=1|s2cid=46030862}}

| 0.597

| 0.183

| −4.28

| 17.03

| align="center" |Local Group

| Satellite of Milky Way

| align="center"|

| Columba I

| 0.597

| 0.183{{cite journal|bibcode=2017AJ....154..267C|title=Deep Subaru Hyper Suprime-Cam Observations of Milky Way Satellites Columba I and Triangulum II|last1=Carlin|first1=Jeffrey L.|last2=Sand|first2=David J.|last3=Muñoz|first3=Ricardo R.|last4=Spekkens|first4=Kristine|last5=Willman|first5=Beth|last6=Crnojević|first6=Denija|last7=Forbes|first7=Duncan A.|last8=Hargis|first8=Jonathan|last9=Kirby|first9=Evan|last10=Peter|first10=Annika H. G.|last11=Romanowsky|first11=Aaron J.|last12=Strader|first12=Jay|journal=The Astronomical Journal|year=2017|volume=154|issue=6|pages=267|doi=10.3847/1538-3881/aa94d0|arxiv=1710.06444|s2cid=54537259 |doi-access=free }}

| −4.2

| 17.11

| align="center"|Local Group

| Satellite of Milky Way

| 760 ly

| align="center"|

| Boötes IV

| 0.682

| 0.209{{cite journal|doi=10.1093/pasj/psz076|title=Boötes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem|year=2019|last1=Homma|first1=Daisuke|last2=Chiba|first2=Masashi|last3=Komiyama|first3=Yutaka|last4=Tanaka|first4=Masayuki|last5=Okamoto|first5=Sakurako|last6=Tanaka|first6=Mikito|last7=Ishigaki|first7=Miho N.|last8=Hayashi|first8=Kohei|last9=Arimoto|first9=Nobuo|last10=Carlsten|first10=Scott G.|last11=Lupton|first11=Robert H.|last12=Strauss|first12=Michael A.|last13=Miyazaki|first13=Satoshi|last14=Torrealba|first14=Gabriel|last15=Wang|first15=Shiang-Yu|last16=Murayama|first16=Hitoshi|journal=Publications of the Astronomical Society of Japan|volume=71|issue=5|pages=94|arxiv=1906.07332|bibcode=2019PASJ...71...94H}}

| −4.53

| 17.07

| align="center"|Local Group

| Satellite of Milky Way

| 3,000 ly

| align="center" |60px

| Leo II Dwarf (Leo B, DDO 93)

| dE0 pec

| 0.701van den Bergh, S. (2000)Updated Information on the Local Group

| 0.215

| −9.23

| 12.45

| align="center" |Local Group

| Satellite of Milky Way

|4,100 ly (tidal)

| align="center" |

| Pegasus III

| 0.701

| 0.215{{cite journal|bibcode=2016ApJ...833...16K|title=Portrait of a Dark Horse: A Photometric and Spectroscopic Study of the Ultra-faint Milky Way Satellite Pegasus III|last1=Kim|first1=Dongwon|last2=Jerjen|first2=Helmut|last3=Geha|first3=Marla|author3-link= Marla Geha |last4=Chiti|first4=Anirudh|last5=Milone|first5=Antonino P.|last6=Da Costa|first6=Gary|last7=MacKey|first7=Dougal|last8=Frebel|first8=Anna|last9=Conn|first9=Blair|journal=The Astrophysical Journal|year=2016|volume=833|issue=1|pages=16|doi=10.3847/0004-637X/833/1/16|arxiv=1608.04934|s2cid=73677994 |doi-access=free }}

| −4.17

| 17.50{{cite journal|doi=10.3847/1538-4357/ac7226|title=Structural Parameters and Possible Association of the Ultra-faint Dwarfs Pegasus III and Pisces II from Deep Hubble Space Telescope Photometry |year=2022 |last1=Richstein |first1=Hannah |last2=Patel |first2=Ekta |last3=Kallivayalil |first3=Nitya |last4=Simon |first4=Joshua D. |last5=Zivick |first5=Paul |last6=Tollerud |first6=Erik |last7=Fritz |first7=Tobias |last8=Warfield |first8=Jack T. |last9=Besla |first9=Gurtina |last10=Van Der Marel |first10=Roeland P. |last11=Wetzel |first11=Andrew |last12=Choi |first12=Yumi |last13=Deason |first13=Alis |last14=Geha |first14=Marla|author14-link= Marla Geha |last15=Guhathakurta |first15=Puragra |last16=Jeon |first16=Myoungwon |last17=Kirby |first17=Evan N. |last18=Libralato |first18=Mattia |last19=Sacchi |first19=Elena |last20=Sohn |first20=Sangmo Tony |journal=The Astrophysical Journal |volume=933 |issue=2 |page=217 |arxiv=2204.01917 |bibcode=2022ApJ...933..217R |s2cid=247957904 |doi-access=free }}

| align="center" |Local Group

| Satellite of Milky Way

| 350 ly

| align="center" |

| Canes Venatici I Dwarf

| dSph

| 0.711

| 0.218{{Cite journal | last1 = Martin | first1 = N. F. | last2 = Coleman | first2 = M. G. | last3 = De Jong | first3 = J. T. A. | last4 = Rix | first4 = H. W. | last5 = Bell | first5 = E. F. | last6 = Sand | first6 = D. J. | last7 = Hill | first7 = J. M. | last8 = Thompson | first8 = D. | last9 = Burwitz | first9 = V. | last10 = Giallongo | first10 = E. | last11 = Ragazzoni | first11 = R. | last12 = Diolaiti | first12 = E. | last13 = Gasparo | first13 = F. | last14 = Grazian | first14 = A. | last15 = Pedichini | first15 = F. | last16 = Bechtold | first16 = J. | title = A Deep Large Binocular Telescope View of the Canes Venatici I Dwarf Galaxy | doi = 10.1086/525559 | journal = The Astrophysical Journal | volume = 672 | pages = L13–L16 | year = 2008 | issue = 1 |arxiv = 0709.3365 |bibcode = 2008ApJ...672L..13M | s2cid = 14614201 }}

| −7.9

| 13.9{{Cite journal | last1 = Zucker | first1 = D. B. | last2 = Belokurov | first2 = V. | last3 = Evans | first3 = N. W. | last4 = Wilkinson | first4 = M. I. | last5 = Irwin | first5 = M. J. | last6 = Sivarani | first6 = T. | last7 = Hodgkin | first7 = S. | last8 = Bramich | first8 = D. M. | last9 = Irwin | first9 = J. M. | last10 = Gilmore | doi = 10.1086/505216 | first10 = G. | last11 = Willman | first11 = B. | last12 = Vidrih | first12 = S. | last13 = Fellhauer | first13 = M. | last14 = Hewett | first14 = P. C. | last15 = Beers | first15 = T. C. | last16 = Bell | first16 = E. F. | last17 = Grebel | first17 = E. K. | last18 = Schneider | first18 = D. P. | last19 = Newberg | first19 = H. J. | last20 = Wyse | first20 = R. F. G. | last21 = Rockosi | first21 = C. M. |author-link21=Constance M. Rockosi| last22 = Yanny | first22 = B. | last23 = Lupton | first23 = R. | last24 = Smith | first24 = J. A. | last25 = Barentine | first25 = J. C. | last26 = Brewington | first26 = H. | last27 = Brinkmann | first27 = J. | last28 = Harvanek | first28 = M. | last29 = Kleinman | first29 = S. J. | last30 = Krzesinski | first30 = J. | title = A New Milky Way Dwarf Satellite in Canes Venatici | journal = The Astrophysical Journal | volume = 643 | issue = 2 | pages = L103 | year = 2006 |arxiv = astro-ph/0604354 |bibcode = 2006ApJ...643L.103Z | s2cid = 119421888 }}

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Cetus III

| 0.819

| 0.251{{cite journal|doi=10.1093/pasj/psx050|title=Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III|year=2018|last1=Homma|first1=Daisuke|last2=Chiba|first2=Masashi|last3=Okamoto|first3=Sakurako|last4=Komiyama|first4=Yutaka|last5=Tanaka|first5=Masayuki|last6=Tanaka|first6=Mikito|last7=Ishigaki|first7=Miho N.|last8=Hayashi|first8=Kohei|last9=Arimoto|first9=Nobuo|last10=Garmilla|first10=José A.|last11=Lupton|first11=Robert H.|last12=Strauss|first12=Michael A.|last13=Miyazaki|first13=Satoshi|last14=Wang|first14=Shiang-Yu|last15=Murayama|first15=Hitoshi|journal=Publications of the Astronomical Society of Japan|volume=70|pages=S18|arxiv=1704.05977|bibcode=2018PASJ...70S..18H}}

| −2.45

| 19.55

| align="center" |Local Group

| Satellite of Milky Way

| 580 ly

| align="center" |60px

| Leo I Dwarf (DDO 74, UGC 5470)

| dE3

| 0.820

| 0.251

| −10.97

| 11.18

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Eridanus II

| 1.19

| 0.366{{cite journal|doi=10.3847/1538-4357/aa6113|title=Farthest Neighbor: The Distant Milky Way Satellite Eridanus II|year=2017|last1=Li|first1=T. S.|last2=Simon|first2=J. D.|last3=Drlica-Wagner|first3=A.|last4=Bechtol|first4=K.|last5=Wang|first5=M. Y.|last6=García-Bellido|first6=J.|last7=Frieman|first7=J.|last8=Marshall|first8=J. L.|last9=James|first9=D. J.|last10=Strigari|first10=L.|last11=Pace|first11=A. B.|last12=Balbinot|first12=E.|last13=Zhang|first13=Y.|last14=Abbott|first14=T. M. C.|last15=Allam|first15=S.|last16=Benoit-Lévy|first16=A.|last17=Bernstein|first17=G. M.|last18=Bertin|first18=E.|last19=Brooks|first19=D.|last20=Burke|first20=D. L.|last21=Rosell|first21=A. Carnero|last22=Kind|first22=M. Carrasco|last23=Carretero|first23=J.|last24=Cunha|first24=C. E.|last25=d'Andrea|first25=C. B.|last26=Costa|first26=L. N. da|last27=Depoy|first27=D. L.|last28=Desai|first28=S.|last29=Diehl|first29=H. T.|last30=Eifler|first30=T. F.|journal=The Astrophysical Journal|volume=838|issue=1|pages=8|arxiv=1611.05052|bibcode=2017ApJ...838....8L|s2cid=45137837|display-authors=29 |doi-access=free }}

| −7.1

| align="center" |Local Group

| Satellite of Milky Way

| 1,810 ly

| Leo T Dwarf

| dIrr/dSph

| 1.35

| 0.413{{cite journal|doi=10.1093/mnras/stab002|arxiv=2101.03189|bibcode=2021MNRAS.503..176H|title=Solo dwarfs II: The stellar structure of isolated Local Group dwarf galaxies|year=2021|last1=Higgs|first1=C. R.|last2=McConnachie|first2=A. W.|last3=Annau|first3=N.|last4=Irwin|first4=M.|last5=Battaglia|first5=G.|last6=Côté|first6=P.|last7=Lewis|first7=G. F.|last8=Venn|first8=K.|journal=Monthly Notices of the Royal Astronomical Society|volume=503|issue=1 |pages=176–199|doi-access=free }}

| 16

| align="center" |Local Group

| Satellite of Milky Way?

|2,300 ly

|Leo K

| 1.42

| 0.434

| −4.86{{cite journal|doi=10.3847/1538-4357/ad429b|doi-access=free |title=Discovery and Characterization of Two Ultrafaint Dwarfs outside the Halo of the Milky Way: Leo M and Leo K |date=2024 |last1=McQuinn |first1=Kristen. B. W. |last2=Mao |first2=Yao-Yuan |last3=Tollerud |first3=Erik J. |last4=Cohen |first4=Roger E. |last5=Shih |first5=David |last6=Buckley |first6=Matthew R. |last7=Dolphin |first7=Andrew E. |journal=The Astrophysical Journal |volume=967 |issue=2 |page=161 |arxiv=2307.08738 |bibcode=2024ApJ...967..161M }}

| align="center" |Local Group

| Satellite of Milky Way

|60px

|Phoenix Dwarf Galaxy (P 6830)

| IAm

| 1.44

| 0.44

| −10.22

| 13.07

| align="center" |Local Group

| Satellite of Milky Way

|Leo M

| 1.50

| 0.459

| −5.77

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Pisces V (Andromeda XVI)

| dSph{{cite journal|bibcode=2017ApJ...837..102S|title=The ISLAndS Project. II. The Lifetime Star Formation Histories of Six Andromeda DSPHS|last1=Skillman|first1=Evan D.|last2=Monelli|first2=Matteo|last3=Weisz|first3=Daniel R.|last4=Hidalgo|first4=Sebastian L.|last5=Aparicio|first5=Antonio|last6=Bernard|first6=Edouard J.|last7=Boylan-Kolchin|first7=Michael|last8=Cassisi|first8=Santi|last9=Cole|first9=Andrew A.|last10=Dolphin|first10=Andrew E.|last11=Ferguson|first11=Henry C.|last12=Gallart|first12=Carme|last13=Irwin|first13=Mike J.|last14=Martin|first14=Nicolas F.|last15=Martínez-Vázquez|first15=Clara E.|last16=Mayer|first16=Lucio|last17=McConnachie|first17=Alan W.|last18=McQuinn|first18=Kristen B. W.|last19=Navarro|first19=Julio F.|last20=Stetson|first20=Peter B.|journal=The Astrophysical Journal|year=2017|volume=837|issue=2|pages=102|doi=10.3847/1538-4357/aa60c5|arxiv=1606.01207|s2cid=53958697 |doi-access=free }}

| 1.79

| 0.55

| −7.6

| 16.1

| align="center" | Local Group

| Satellite of Andromeda

| 985 ly

| align="center" | 60px

|Barnard's Galaxy (NGC 6822)

| IB(s)m IV-V

| 1.859

| 0.570

| −15.22

| 9.32

| align="center" |Local Group

| It contains several large H II regions

|7,000 ly

| align="center" | 60px

|NGC 185

| dE3 pec

| 2.05

| 0.63

| −14.76

| 9.99

| align="center" |Local Group

| Satellite of Andromeda; possibly closest Seyfert galaxy to Earth

| align="center" |60px

| Andromeda II

| dE0

| 2.22

| 0.68

| −12.6

| 11.7

| align="center" |Local Group

| Satellite of Andromeda

| 6,820 ly

| align="center" |

| Cassiopeia II (Andromeda XXX)

| dSph

| 2.221

| 0.681

| −8.0{{cite journal|bibcode=2016ApJ...833..167M|title=The PAndAS View of the Andromeda Satellite System. II. Detailed Properties of 23 M31 Dwarf Spheroidal Galaxies|last1=Martin|first1=Nicolas F.|last2=Ibata|first2=Rodrigo A.|last3=Lewis|first3=Geraint F.|last4=McConnachie|first4=Alan|last5=Babul|first5=Arif|last6=Bate|first6=Nicholas F.|last7=Bernard|first7=Edouard|last8=Chapman|first8=Scott C.|last9=Collins|first9=Michelle M. L.|last10=Conn|first10=Anthony R.|last11=Crnojević|first11=Denija|last12=Fardal|first12=Mark A.|last13=Ferguson|first13=Annette M. N.|last14=Irwin|first14=Michael|last15=MacKey|first15=A. Dougal|last16=McMonigal|first16=Brendan|last17=Navarro|first17=Julio F.|last18=Rich|first18=R. Michael|journal=The Astrophysical Journal|year=2016|volume=833|issue=2|pages=167|doi=10.3847/1538-4357/833/2/167|arxiv=1610.01158|s2cid=73620398 |doi-access=free }}

| 16.0

| align="center" |Local Group

| Satellite of Andromeda

| 1,800 ly

| 60px

| IC 1613 (UGC 668)

| IAB(s)m V

| 2.24

| 0.686

| −14.51

| 9.92

| align="center" |Local Group

| align="center" |

| Pegasus V (Andromeda XXXIV)

| 2.26

| 0.692

| −6.3

| align="center" |Local Group

| Satellite of Andromeda{{cite journal |arxiv=2204.09068 |last1=Collins |first1=Michelle L. M. |last2=Charles |first2=Emily J. E. |last3=Martínez-Delgado |first3=David |last4=Monelli |first4=Matteo |last5=Karim |first5=Noushin |last6=Donatiello |first6=Giuseppe |last7=Tollerud |first7=Erik J. |last8=Boschin |first8=Walter |title=Pegasus V/Andromeda XXXIV–a newly discovered ultrafaint dwarf galaxy on the outskirts of Andromeda |journal=Monthly Notices of the Royal Astronomical Society: Letters |year=2022 |volume=515 |issue=1 |pages=L72–L77 |doi=10.1093/mnrasl/slac063 |doi-access=free |bibcode=2022MNRAS.515L..72C }}

| 60px

| Leo A (Leo III, DDO 69)

| IBm V

| 2.34

| 0.717

| −11.68

| 12.92

| align="center" |Local Group

| Satellite of Milky Way

| align="center" |

| Andromeda XVII

| dSph

| 2.371

| 0.727

| −7.8

| 16.6

| align="center" |Local Group

| Satellite of Andromeda

| 1,900 ly

| align="center" |

| Andromeda XXV

| dSph

| 2.401

| 0.736

| −9.0

| 15.3

| align="center" |Local Group

| Satellite of Andromeda

| 3,560 ly

| align="center" |

| Andromeda XI

| dSph

| 2.41

| 0.74{{cite journal|title=Cosmicflows-2: The Data|author1=Tully, R. Brent|display-authors=etal|journal=The Astronomical Journal|volume=146|issue=4|date=2013|bibcode=2013AJ....146...86T|doi=10.1088/0004-6256/146/4/86|arxiv=1307.7213|page=86|s2cid=118494842}}

| −7.3{{cite journal|bibcode=2012MNRAS.419.1362Y|title=HST/WFPC2 Imaging of the Dwarf Satellites And XI and And XIII : HB Morphology and RR Lyraes|journal=Monthly Notices of the Royal Astronomical Society|volume=419|issue=2|pages=1362|doi=10.1111/j.1365-2966.2011.19792.x|year=2012|last1=Yang|first1=S.-C|last2=Sarajedini|first2=A|doi-access=free |arxiv=1109.2038|s2cid=119190619}}

| align="center" |Local Group

| Satellite of Andromeda

| align="center" |

| Andromeda XX

| dSph{{cite journal|bibcode=2013ApJ...768..172C|title=A Kinematic Study of the Andromeda Dwarf Spheroidal System|last1=Collins|first1=Michelle L. M.|last2=Chapman|first2=Scott C.|last3=Rich|first3=R. Michael|last4=Ibata|first4=Rodrigo A.|last5=Martin|first5=Nicolas F.|last6=Irwin|first6=Michael J.|last7=Bate|first7=Nicholas F.|last8=Lewis|first8=Geraint F.|last9=Peñarrubia|first9=Jorge|last10=Arimoto|first10=Nobuo|last11=Casey|first11=Caitlin M.|author-link11=Caitlin Casey|last12=Ferguson|first12=Annette M. N.|last13=Koch|first13=Andreas|last14=McConnachie|first14=Alan W.|last15=Tanvir|first15=Nial|journal=The Astrophysical Journal|year=2013|volume=768|issue=2|pages=172|doi=10.1088/0004-637X/768/2/172|arxiv=1302.6590|s2cid=67749084}}

| 2.417

| 0.741

| −6.4

| 18.0

| align="center" |Local Group

| Satellite of Andromeda

| 590 ly

| align="center" |

| Andromeda XXIII

| dSph

| 2.440

| 0.748

| −9.8

| 14.6

| align="center" |Local Group

| Satellite of Andromeda

| 7,770 ly

| align="center" | 60px

| IC 10 (UGC 192)

| dIrr IV/BCD

| 2.446

| 0.750

| −15.57

| 12.2

| align="center" |Local Group

| Satellite of Andromeda

| align="center" |60px

| Andromeda III

| dE2

| 2.45

| 0.75

| −10.1

| 14.4

| align="center" |Local Group

| Satellite of Andromeda

| 2750 ly

| align="center" | File:Cassiopeia Dwarf (PGC 2807155) Hubble WikiSky.jpg

|Cassiopeia Dwarf (Cas dSph, Andromeda VII)

| dSph

| 2.45

| 0.75{{cite journal|doi=10.3847/1538-4357/abdec1|title=The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies. IV. The Star Formation History of Andromeda VII Derived from Long-period Variable Stars|year=2021|last1=Navabi|first1=Mahdieh|last2=Saremi|first2=Elham|last3=Javadi|first3=Atefeh|last4=Noori|first4=Majedeh|last5=Van Loon|first5=Jacco Th.|last6=Khosroshahi|first6=Habib G.|last7=McDonald|first7=Iain|last8=Alizadeh|first8=Mina|last9=Danesh|first9=Arash|last10=Gozaliasl|first10=Ghassem|last11=Molaeinezhad|first11=Alireza|last12=Parto|first12=Tahere|last13=Raouf|first13=Mojtaba|journal=The Astrophysical Journal|volume=910|issue=2|page=127|arxiv=2101.09900|bibcode=2021ApJ...910..127N|s2cid=231698580 |doi-access=free }}

| −11.67

| 13.65

| align="center" |Local Group

| Satellite of Andromeda

| align="center" |

| Andromeda XXVI

| dSph

| 2.459

| 0.754

| −5.8

| 18.5

| align="center" |Local Group

| Satellite of Andromeda

| 980 ly

| align="center" |60px

| Cetus Dwarf

| dSph/E4

| 2.460McConnachie, A. W. et al. 2005 Distances and Metallicities for 17 Local Group Galaxies

| 0.754

| −10.18

| 14.4

| align="center" |Local Group

| Satellite of Andromeda

| align="center"|

| Pisces III (Andromeda XIII)

| dSph

| 2.479

| 0.760

| −6.5

| 17.8

| align="center"|Local Group

| Satellite of Andromeda

| 850 ly

| align="center" |

| Andromeda XV

| dSph

| 2.48

| 0.76

| −8.4

| 16.0

| align="center" |Local Group

| Satellite of Andromeda

| 1840 ly

| align="center" | 60px

|M32 (NGC 221)

| E2

| 2.489

| 0.763

| −15.96

| 8.73

| align="center" |Local Group

| Close Satellite of Andromeda

|6,500 ly

|Andromeda IX

| dE

| 2.500

| 0.767

| −7.5

| align="center" |Local Group

| Satellite of Andromeda

| align="center" | 60px

|Pisces Dwarf (LGS 3)

| dIrr/dSph

| 2.510

| 0.770

| −7.96

| 16.18

| align="center" |Local Group

| Satellite of Triangulum{{Citation needed|date=June 2008}}

| align="center" |

| Cassiopeia III (Andromeda XXXII)

| 2.518

| 0.772{{cite journal|bibcode=2013ApJ...772...15M|title=Lacerta I and Cassiopeia III. Two Luminous and Distant Andromeda Satellite Dwarf Galaxies Found in the 3π Pan-STARRS1 Survey|last1=Martin|first1=Nicolas F.|last2=Slater|first2=Colin T.|last3=Schlafly|first3=Edward F.|last4=Morganson|first4=Eric|last5=Rix|first5=Hans-Walter|last6=Bell|first6=Eric F.|last7=Laevens|first7=Benjamin P. M.|last8=Bernard|first8=Edouard J.|last9=Ferguson|first9=Annette M. N.|last10=Finkbeiner|first10=Douglas P.|last11=Burgett|first11=William S.|last12=Chambers|first12=Kenneth C.|last13=Hodapp|first13=Klaus W.|last14=Kaiser|first14=Nicholas|last15=Kudritzki|first15=Rolf-Peter|last16=Magnier|first16=Eugene A.|last17=Morgan|first17=Jeffrey S.|last18=Price|first18=Paul A.|last19=Tonry|first19=John L.|last20=Wainscoat|first20=Richard J.|journal=The Astrophysical Journal|year=2013|volume=772|issue=1|pages=15|doi=10.1088/0004-637X/772/1/15|arxiv=1305.5301|s2cid=119262613}}

| −12.3

| 12.15

| align="center" |Local Group

| Satellite of Andromeda

| 9,500 ly

| Andromeda V

| dSph

| 2.52

| 0.773

| −8.41

| 16.67

| align="center" |Local Group

| Satellite of Andromeda

| align="center"|

| Lacerta I (Andromeda XXXI)

| dSph

| 2.521

| 0.773{{cite journal|doi=10.3847/1538-4357/836/1/137|title=Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN pODI|year=2017|last1=Rhode|first1=Katherine L.|last2=Crnojević|first2=Denija|last3=Sand|first3=David J.|last4=Janowiecki|first4=Steven|last5=Young|first5=Michael D.|last6=Spekkens|first6=Kristine|journal=The Astrophysical Journal|volume=836|issue=1|pages=137|arxiv=1701.08168|bibcode=2017ApJ...836..137R|s2cid=118918041 |doi-access=free }}

| −11.4

| 13.04

| align="center"|Local Group

| Satellite of Andromeda

| 4,750 ly

| align="center" | 60px

| NGC 147 (DDO 3)

| dE5 pec

| 2.53

| 0.776

| −14.9

| 10.36

| align="center" |Local Group

| Satellite of Andromeda

| align="center" |60px

|Andromeda Galaxy (M31)

| SA(s)b

| 2.538

| 0.778

| −21.58

| 4.17

| align="center" |Local Group

| Largest Galaxy in the Local Group (The Milky Way is the second largest), with at least 19 satellite galaxies. Barred spiral galaxy.

|152,000 ly

| align="center" | 60px

|Pegasus Dwarf Spheroidal (Andromeda VI)

| dSph

| 2.55

| 0.78

| −10.80

| 14.05

| align="center" |Local Group

| Satellite of Andromeda

| align="center"|

| Perseus I (Andromeda XXXIII)

| 2.560

| 0.785{{cite journal|bibcode=2013ApJ...779L..10M|title=Perseus I: A Distant Satellite Dwarf Galaxy of Andromeda|last1=Martin|first1=Nicolas F.|last2=Schlafly|first2=Edward F.|last3=Slater|first3=Colin T.|last4=Bernard|first4=Edouard J.|last5=Rix|first5=Hans-Walter|last6=Bell|first6=Eric F.|last7=Ferguson|first7=Annette M. N.|last8=Finkbeiner|first8=Douglas P.|last9=Laevens|first9=Benjamin P. M.|last10=Burgett|first10=William S.|last11=Chambers|first11=Kenneth C.|last12=Draper|first12=Peter W.|last13=Hodapp|first13=Klaus W.|last14=Kaiser|first14=Nicholas|last15=Kudritzki|first15=Rolf-Peter|last16=Magnier|first16=Eugene A.|last17=Metcalfe|first17=Nigel|last18=Morgan|first18=Jeffrey S.|last19=Price|first19=Paul A.|last20=Tonry|first20=John L.|last21=Wainscoat|first21=Richard J.|last22=Waters|first22=Christopher|journal=The Astrophysical Journal|year=2013|volume=779|issue=1|pages=L10|doi=10.1088/2041-8205/779/1/L10|arxiv=1310.4170|s2cid=55729618}}

| −10.3

| 14.19

| align="center"|Local Group

| Satellite of Andromeda

| 2,600 ly

| align="center"|

| Andromeda XIV (Pisces IV)

| 2.586

| 0.793

| −8.5

| 15.8

| align="center"|Local Group

| Satellite of Andromeda

| ~1,700 ly

| 60px

| Andromeda I

| dE3 pec

| 2.61

| 0.80Calculated from the distance modulus ( $m - M$ ) using the formula $d_{pc} = 10^{\frac{m - M}{5} + 1}$

| −12.0

| 12.7

| align="center" |Local Group

| Satellite of Andromeda

| 5,840 ly

| align="center"|

| Andromeda XXVIII

| dSph

| 2.645

| 0.811{{cite journal|bibcode=2015ApJ...806..230S|title=A Deep Study of the Dwarf Satellites Andromeda XXVIII and Andromeda XXIX|last1=Slater|first1=Colin T.|last2=Bell|first2=Eric F.|last3=Martin|first3=Nicolas F.|last4=Tollerud|first4=Erik J.|last5=Ho|first5=Nhung|journal=The Astrophysical Journal|year=2015|volume=806|issue=2|pages=230|doi=10.1088/0004-637X/806/2/230|arxiv=1505.02161|s2cid=118698841}}

| −8.7

| 15.85

| align="center"|Local Group

| Satellite of Andromeda

| 1,800 ly

| align="center" | 60px

|M110 (NGC 205)

| E6p

| 2.67

| 0.82

| −16.15

| 8.72

| align="center" |Local Group

| Close Satellite of Andromeda

|Andromeda VIII

| dSphMorrison et al. 2003 Andromeda VIII, a New Tidally Distorted satellite of M31 — for details see [http://www.journals.uchicago.edu/doi/pdf/10.1086/379625] {{Webarchive|url=https://web.archive.org/web/20200708082106/https://www.journals.uchicago.edu/doi/pdf/10.1086/379625|date=2020-07-08}}

| 2.700

| 0.828

| −15.6

| 9.1

| align="center" |Local Group

| Tidally distorted dwarf close to Andromeda discovered 2003

| align="center" |

| Andromeda XXIX

| 2.704

| 0.829

| −8.5

| 16.09

| align="center" |Local Group

| Satellite of Andromeda

| 2,050 ly

| align="center" |60px

| Triangulum Galaxy (M33)

| SA(s)cd

| 2.73

| 0.84

| −18.87

| 6.19

| align="center" |Local Group

| Most distant (difficult) naked eye object. Closest unbarred spiral galaxy to us and third largest galaxy in the Local Group.

|61,100 ly

| align="center" |

| Andromeda XXI{{Cite journal | arxiv=0909.0399 | author1=Martin | display-authors=4 | author2=McConnachie | author3=Mike Irwin | author4=Widrow | author5=Ferguson | author6=Ibata | author7=John Dubinski | author8=Arif Babul | author9=Scott Chapman | title=PAndAS' cubs: Discovery of two new dwarf galaxies in the surroundings of the Andromeda and Triangulum galaxies | date=2009 | doi=10.1088/0004-637X/705/1/758 | volume=705 | journal=The Astrophysical Journal | issue=1 | pages=758–765 | bibcode=2009ApJ...705..758M| s2cid=15277245 }}

| dSph

| 2.802

| 0.859

| −9.9

| align="center" |Local Group

| Satellite of Andromeda

| align="center" | 60px

| Tucana Dwarf

| dE5

| 2.87

| 0.88

| −9.16

| 15.7

| align="center" |Local Group

| Isolated group member — a 'primordial' galaxy[https://www.doi.org/10.1111/j.1365-2966.2007.11395.x See]

| align="center" | 60px

| Andromeda X

| dSph

| 2.90

| 0.889

| −8.1Zucker et al. 2007 Andromeda X, a New Dwarf Spheroidal satellite of M31:Photometry — for details see [http://www.journals.uchicago.edu/doi/abs/10.1086/516748?journalCode=apjl]

| 16.1

| align="center" |Local Group

| Satellite of Andromeda discovered 2006

| align="center"|

| Andromeda XXIV

| dSph

| 2.929

| 0.898

| −8.4

| 16.3

| align="center"|Local Group

| Satellite of Andromeda

| 4,440 ly

| align="center" | 60px

|Pegasus Dwarf Irregular (DDO 216)

| dIrr/dSph

| 2.929

| 0.898

| −11.47

| 13.21

| align="center" |Local Group

| Satellite of Andromeda

101

| Pisces VII (Triangulum III)

| 2.99

| 0.916{{cite journal | arxiv=2305.13966 | doi=10.1093/mnras/stae199 | doi-access=free | bibcode=2024MNRAS.528.2614C | title=Pisces VII/Triangulum III – M33's second dwarf satellite galaxy | date=2024 | last1=Collins | first1=Michelle L M. | last2=Karim | first2=Noushin | last3=Martinez-Delgado | first3=David | last4=Monelli | first4=Matteo | last5=Tollerud | first5=Erik J. | last6=Donatiello | first6=Giuseppe | last7=Navabi | first7=Mahdieh | last8=Charles | first8=Emily | last9=Boschin | first9=Walter | journal=Monthly Notices of the Royal Astronomical Society | volume=528 | issue=2 | pages=2614–2620 }}

| −6.0

| align="center" |Local Group

| Likely satellite of Triangulum

102

| align="center"|

| Andromeda XXXV

| 3.023

| 0.927{{Cite journal |last1=Arias |first1=Jose Marco |last2=Bell |first2=Eric F. |last3=Gozman |first3=Katya |last4=Jang |first4=In Sung |last5=Stockton |first5=Saxon |last6=Gnedin |first6=Oleg Y. |last7=D’Souza |first7=Richard |last8=Monachesi |first8=Antonela |last9=Bailin |first9=Jeremy |last10=Nidever |first10=David |last11=de Jong |first11=Roelof S. |date=2025-03-11 |title=Andromeda XXXV: The Faintest Dwarf Satellite of the Andromeda Galaxy |journal=The Astrophysical Journal Letters |volume=982 |issue=1 |pages=L3 |doi=10.3847/2041-8213/adb433 |doi-access=free |bibcode=2025ApJ...982L...3A |issn=2041-8205}}

| −5.2

| align="center"|Local Group

| Satellite of Andromeda

102

| align="center"|

| Andromeda XII

| dSph

| 3.027

| 0.928{{cite journal|bibcode=2019MNRAS.488.3231H|title=Proper motions of the satellites of M31|last1=Hodkinson|first1=Ben|last2=Scholtz|first2=Jakub|journal=Monthly Notices of the Royal Astronomical Society|year=2019|volume=488|issue=3|pages=3231|doi=10.1093/mnras/stz1893|doi-access=free |arxiv=1904.03192}}

| −7.0

| 17.7

| align="center"|Local Group

| Satellite of Andromeda

| 2,740 ly

103

| align="center" |60px

|Wolf-Lundmark-Melotte (WLM, DDO 221)

| IB(s)m

| 3.043

| 0.933{{cite journal | author1=Karachentsev | author2=Kashibadze | author3=Makarov | author4=Tully | title=The Hubble flow around the Local Group | doi=10.1111/j.1365-2966.2008.14300.x | date=2009 | journal=Monthly Notices of the Royal Astronomical Society | volume=393 | issue=4 | pages=1265 | doi-access=free | arxiv=0811.4610 |bibcode = 2009MNRAS.393.1265K | s2cid=13912040 }}

| −14.06

| 11.03

| align="center" |Local Group

| Isolated member at the edge of the local group

|11,500 ly

103

|Andromeda XIXA Trio of New Local Group Galaxies with Extreme Properties, Alan W. McConnachie et al. 2008, ApJ 688 1009–1020, https://arxiv.org/abs/0806.3988 {{Webarchive|url=https://web.archive.org/web/20171201182050/https://arxiv.org/abs/0806.3988 |date=2017-12-01 }}

| dSph

| 3.043

| 0.933

| −9.3

| align="center" |Local Group

| Satellite of Andromeda, spread over 1.7 kpc

|2,200 ly

105

| align="center" |

|Andromeda XXII

| dSph

| 3.219

| 0.987

| 18.0

| align="center" |Local Group

| Satellite of Andromeda

106

| align="center" | 60px

| Aquarius Dwarf Galaxy (DDO 210)

| Im V

| 3.22

| 0.988

| −11.09

| 14.0

| align="center" |Local Group

| Isolated group member

107

| align="center" |60px

| Sagittarius Dwarf Irregular Galaxy (SagDIG)

| IB(s)m V

| 3.907

| 1.198

| −11.49

| 15.5

| align="center" |Local Group

| Isolated, star forming group member

|3,000 ly

108

| align="center" | 60px

| UGC 4879 (VV124){{cite journal | author1=Kopylov | display-authors=4 | author2=Tikhonov | author3=Sergey Fabrika | author4=Igor Drozdovsky | author5=Valeev | title=VV124 (UGC4879): A new transitional dwarf galaxy in the periphery of the Local Group | doi=10.1111/j.1745-3933.2008.00482.x | date=2008 | journal=Monthly Notices of the Royal Astronomical Society: Letters | volume=387 | issue=1 | pages=L45–L49 | doi-access=free | arxiv=0803.1107 |bibcode = 2008MNRAS.387L..45K | s2cid=17166212 }}

| IAm

| 3.956

| 1.213

| −11.5

| 13.2

| align="center" |Local Group

| Isolated, star forming group member

|3,000 ly

109

| align="center" | 60px

| Andromeda XVIII

| dSph

| 3.960

| 1.214

| −9.2

| 16.2

| align="center" |Local Group

| 1,700

|≈ 1,200 ly

110

| align="center" | 60px

| Antlia Dwarf

| dE3.5

| 4.28

| 1.31

| −9.63

| 16.19

| align="center" |Local GroupGalaxies of small Antlia-Sextans Group, which is considered as part of Local Group, but membership of it is uncertain.

| May have interacted with NGC 3109

|3,000 ly

111

| align="center" | 60px

| Sextans A (UGCA 205, DDO 75)

| IBm

| 4.31Dolphin, Andrew E. et al. 2003 Deep Hubble Space Telescope Imaging of Sextans A. II. Cepheids and Distance

| 1.32

| −13.95

| 11.86

| align="center" |Local Group

| Contains cluster of young hot blue stars

|5,000 ly

112

| align="center" | 60px

| NGC 3109

| SB(s)m

| 4.338

| 1.35Soszynski "et al."(2006) The Araucaria Project: Distance to the Local Group Galaxy NGC 3109 from Near-Infrared Photometry of Cepheids see [http://www.journals.uchicago.edu/doi/abs/10.1086/505789?journalCode=apj] {{Webarchive|url=https://web.archive.org/web/20200201224641/https://www.journals.uchicago.edu/doi/abs/10.1086/505789?journalCode=apj|date=2020-02-01}}

| −15.68

| 10.39

| align="center" |Local Group

| Possibly spiral galaxy

|25,000 ly

113

| align="center" |

| Antlia B

|dSph/Irr

| 4.40

| 1.35{{cite journal|doi=10.3847/1538-4357/ab58d2|title=Hubble Space Telescope Imaging of Antlia B: Star Formation History and a New Tip of the Red Giant Branch Distance|year=2020|last1=Hargis|first1=J. R.|last2=Albers|first2=S.|last3=Crnojević|first3=D.|last4=Sand|first4=D. J.|last5=Weisz|first5=D. R.|last6=Carlin|first6=J. L.|last7=Spekkens|first7=K.|last8=Willman|first8=B.|last9=Peter|first9=A. H. G.|last10=Grillmair|first10=C. J.|last11=Dolphin|first11=A. E.|journal=The Astrophysical Journal|volume=888|issue=1|pages=31|bibcode=2020ApJ...888...31H|hdl=10150/640977|s2cid=197431299|hdl-access=free |doi-access=free }}

| −9.7

| 15.95

| align="center" |Local Group

| Satellite of NGC 3109

| 1,780 ly

114

| align="center" |

| Sculptor A

| 4.40

| 1.35{{cite journal|bibcode=2024ApJ...977L...5S|arxiv=2409.16345|doi=10.3847/2041-8213/ad927c|doi-access=free |title=Three Quenched, Faint Dwarf Galaxies in the Direction of NGC 300: New Probes of Reionization and Internal Feedback |date=2024 |last1=Sand |first1=David J. |last2=Mutlu-Pakdil |first2=Burçin |last3=Jones |first3=Michael G. |last4=Karunakaran |first4=Ananthan |last5=Andrews |first5=Jennifer E. |last6=Bennet |first6=Paul |last7=Crnojević |first7=Denija |last8=Donatiello |first8=Giuseppe |last9=Drlica-Wagner |first9=Alex |last10=Fielder |first10=Catherine |last11=Martínez-Delgado |first11=David |last12=Martínez-Vázquez |first12=Clara E. |last13=Spekkens |first13=Kristine |last14=Doliva-Dolinsky |first14=Amandine |last15=Hunter |first15=Laura C. |last16=Carlin |first16=Jeffrey L. |last17=Cerny |first17=William |last18=Hai |first18=Tehreem N. |last19=McQuinn |first19=Kristen B.W. |last20=Pace |first20=Andrew B. |last21=Smercina |first21=Adam |journal=The Astrophysical Journal Letters |volume=977 |pages=L5 }}

| −6.9

| align="center" |Local Group

114

| align="center" | 60px

| Sextans B (UGC 5373)

| IM IV-V

| 4.47

| 1.37

| −14.08

| 11.85

| align="center" |Local Group

| One of the smallest galaxies with planetary nebulae

|6,000 ly

114

| align="center" |

| Tucana B

|dSph

| 4.56

| 1.4{{cite journal|doi=10.3847/2041-8213/ac85ee|title=Tucana B: A Potentially Isolated and Quenched Ultra-faint Dwarf Galaxy at D ≈ 1.4 MPC |year=2022 |last1=Sand |first1=David J. |last2=Mutlu-Pakdil |first2=Burçin |last3=Jones |first3=Michael G. |last4=Karunakaran |first4=Ananthan |last5=Wang |first5=Feige |last6=Yang |first6=Jinyi |last7=Chiti |first7=Anirudh |last8=Bennet |first8=Paul |last9=Crnojević |first9=Denija |last10=Spekkens |first10=Kristine |journal=The Astrophysical Journal Letters |volume=935 |issue=1 |pages=L17 |s2cid=251615833 |hdl=10261/309130 |hdl-access=free |doi-access=free |arxiv=2205.09129 |bibcode=2022ApJ...935L..17S }}

| −6.9

| 18.85

| align="center" |Local Group

| Isolated group member

| 522 ly

115

|Cassiopeia 1

|Irr

|5.19

|1.59{{Cite journal |last=Tikhonov |first=N. A. |date=2019-12-01 |title=Distance to Irregular Galaxy Cas 1 Located near the Milky Way |url=https://ui.adsabs.harvard.edu/abs/2019AstBu..74..396T |journal=Astrophysical Bulletin |volume=74 |issue=4 |pages=396–402 |doi=10.1134/S1990341319040060|bibcode=2019AstBu..74..396T |s2cid=213381996 }}

| -14.2

|14.62

|Isolated

|Isolated galaxy

116

| align="center" | 60px

| Leo P

| Irr

| 5.28

| 1.62

| -9.27

| 16.89

| align="center" | Local Group

| Extremely low metallicity

| 3,690 ly

117

| align="center" | 60px

| IC 5152

| IA(s)m

| 5.68

| 1.74

| −15.56

| 11.06

| align="center" | Local Group ?

| Possible outlying member of Local Group

|4,000 ly

118

| align="center" | 60px

| NGC 300

| SA(s)d

| 6.07

| 1.86

| −17.92

| 8.95

| align="center" |between LG and Sculptor Group

| Closest spiral galaxy to Local Group
forms pair with NGC 55

|94,000 ly

119

| align="center" |60px

| KKR 25

| Irr

| 6.20

| 1.90

| −9.94

| 17.0

| between LG and M81

120

| align="center" |60px

| ESO 410-G005

| E3

| 6.213

| 1.905

| −11.60

| 14.85

| align="center" | NGC 55 & 300

|≈ 2,500 ly

121

| align="center" | 60px

| ESO 294-010

| dS0/Im

| 6.36Karachentsev, I. D. et al. (2003) Distances to Nearby Galaxies in Sculptor

| 1.96

| −10.95

| 15.6

| align="center" | NGC 55 & 300

122

| align="center" |

| Pavo

| 6.49

| 1.99{{cite journal|doi=10.3847/2041-8213/ad0130|doi-access=free |title=Pavo: Discovery of a Star-forming Dwarf Galaxy Just Outside the Local Group |date=2023 |last1=Jones |first1=Michael G. |last2=Mutlu-Pakdil |first2=Burçin |last3=Sand |first3=David J. |last4=Donnerstein |first4=Richard |last5=Crnojević |first5=Denija |last6=Bennet |first6=Paul |last7=Fielder |first7=Catherine E. |last8=Karunakaran |first8=Ananthan |last9=Spekkens |first9=Kristine |last10=Strader |first10=Jay |last11=Urquhart |first11=Ryan |last12=Zaritsky |first12=Dennis |journal=The Astrophysical Journal Letters |volume=957 |issue=1 |pages=L5 |arxiv=2310.01478 |bibcode=2023ApJ...957L...5J }}

| −10.0

| align="center" |

122

| align="center" | 60px

| NGC 55

| SB(s)m

| 6.52

| 2.00

| −18.47

| 8.84

| align="center" |between LG and Sculptor Group

| Forms pair with NGC 300

|70,000 ly

123

| align="center" |

| Sculptor C

| 6.65

| 2.04

| −9.1

| align="center" |

| Satellite of NGC 300

123

| align="center" |

| KKs 3

| dSph

| 6.91

| 2.12{{cite journal|bibcode=2017MNRAS.471.1955S|doi=10.1093/mnras/stx1605|arxiv=1706.07344|title=Nuclei of dwarf spheroidal galaxies KKs 3 and ESO 269−66 and their counterparts in our Galaxy|journal=Monthly Notices of the Royal Astronomical Society|volume=471|issue=2|pages=1955|year=2017|last1=Sharina|first1=M. E|last2=Shimansky|first2=V. V|last3=Kniazev|first3=A. Y|doi-access=free }}

| −12.3

| 14.47

| align="center" |

| 4,900 ly

124

| align="center" |60px

| KKR 3 (KK 230)

| dIrr

| 6.98

| 2.14

| −9.8

| 17.90

| align="center" | Inner edge of M94 Group

|980 ly

125

| align="center" |

| UGCA 438 (ESO 407-018)

| IB(s)m pec:

| 7.24

| 2.22

| −12.92

| 13.86

| align="center" | NGC 55 & 300

126

| align="center" |

| KK 258 (ESO 468–20)

| dTr

| 7.27

| 2.23{{cite journal|doi=10.1093/mnras/stu1217|title=KK258, a new transition dwarf galaxy neighbouring the Local Group|year=2014|last1=Karachentsev|first1=I. D.|last2=Makarova|first2=L. N.|last3=Tully|first3=R. B.|last4=Wu|first4=Po-Feng|last5=Kniazev|first5=A. Y.|journal=Monthly Notices of the Royal Astronomical Society|volume=443|issue=2|pages=1281–1290|doi-access=free |arxiv=1406.4479|bibcode=2014MNRAS.443.1281K}}

| −10.3

| align="center" | NGC 55 & 300

127

| align="center" |60px

| UGC 9128 (DDO 187)

| ImIV-V

| 7.31

| 2.24

| −12.47

| 14.38

| align="center" | Inner edge of M94 Group

128

| align="center" | 60px

| IC 3104

| IB(s)m

| 7.40

| 2.27

| −14.85

| 13.63

| On the way to Circinus galaxy

129

| align="center" |

| Dw1907+63

| 7.8

| 2.4

| 17.0

| align="center" |

129

| align="center" |60px

| GR 8 (DDO 155, UGC 8091)

| ImV

| 7.8

| 2.4

| −12.14

| 14.65

| align="center" | Inner edge of M94 Group

| "footprint galaxy"

129

| Hedgehog Galaxy

| 7.86

| 2.41{{cite journal|doi=10.3847/2041-8213/ad5b59|doi-access=free |title=Hedgehog: An Isolated Quiescent Dwarf Galaxy at 2.4 MPC |date=2024 |last1=Li 李 |first1=Jiaxuan 嘉轩 |last2=Greene |first2=Jenny E. |last3=Carlsten |first3=Scott G. |last4=Danieli |first4=Shany |journal=The Astrophysical Journal Letters |volume=975 |issue=1 |pages=L23 |arxiv=2406.00101 |bibcode=2024ApJ...975L..23L }}

| −9.84

| Isolated dwarf

130

| align="center" | 60px

| IC 4662 (ESO 102-14)

| IBm

| 7.96

| 2.44

| −15.56

| 11.74

| On the way to Circinus galaxy

|7,000 ly

131

| align="center" |60px

| KKH 98

| Irr

| 7.99

| 2.45

| −10.78

| 16.7

| align="center" |IC 342/Maffei Group

131

| align="center" |

| Sculptor B

| 8.09

| 2.48

| −8.1

| align="center" |

131

| align="center" |File:SMDG 0956+82.png

| SMDG 0956+82

| 8.48

| 2.6{{cite journal|doi=10.1093/mnrasl/slae111 |doi-access=free |title=New radial velocities for 40 nearby dwarf galaxies |date=2025 |last1=Karachentsev |first1=Igor D. |last2=Chazov |first2=Maxim I. |last3=Kaisin |first3=Serafim S. |journal=Monthly Notices of the Royal Astronomical Society: Letters |volume=537 |pages=L21–L25 |arxiv=2411.15603 }}

| 18.1

| align="center" |

132

| align="center" | 60px

| UGC 8508 (I Zw 060)

| IAm

| 8.35{{cite journal|doi=10.1051/0004-6361:20011741|title=The M 81 group of galaxies: New distances, kinematics and structure|year=2002|last1=Karachentsev|first1=I. D.|last2=Dolphin|first2=A. E.|last3=Geisler|first3=D.|last4=Grebel|first4=E. K.|last5=Guhathakurta|first5=P.|last6=Hodge|first6=P. W.|last7=Karachentseva|first7=V. E.|last8=Sarajedini|first8=A.|last9=Seitzer|first9=P.|last10=Sharina|first10=M. E.|journal=Astronomy & Astrophysics|volume=383|pages=125–136|bibcode=2002A&A...383..125K|doi-access=free}}

| 2.69

| −13.09

| 14.40

| align="center" |M94 Group

133

| align="center" | 60px

| KKH 86

| Irr

| 8.48

| 2.60

| −10.30

| 16.8

| Isolated (M94/Cent A)

134

| align="center" | 60px

| DDO 99 (UGC 6817)

| Im

| 8.61

| 2.64–3.9

| −13.52

| 13.4

| align="center" |M94 Group

135

| align="center" |

| Dw1245+61

| 8.81

| 2.7

| 18.4

| align="center" |

135

| align="center" |

| ESO 6-1

| Ir

| 8.81

| 2.70

| −12.41

| 14.75{{cite journal|doi=10.3847/1538-4357/acb048|title=A Nearby Isolated Dwarf: Star Formation and Structure of ESO 006–001 |year=2023 |last1=Makarova |first1=Lidia N. |last2=Tully |first2=R. Brent |last3=Anand |first3=Gagandeep S. |last4=Lambert |first4=Trystan S. |last5=Sharina |first5=Margarita E. |last6=Koribalski |first6=Bärbel S. |last7=Kraan-Korteweg |first7=Renée C. |journal=The Astrophysical Journal |volume=943 |issue=2 |page=139 |arxiv=2301.12789 |bibcode=2023ApJ...943..139M |s2cid=256390080 |doi-access=free }}

| align="center" |

| Blue compact dwarf galaxy

136

| align="center" | 60px

| UGC 7577 (DDO 125)

| Im

| 8.94

| 2.74

| −14.32

| 12.84

| align="center" |M94 Group

137

| align="center" |

| KDG 162

| 9.13

| 2.8

| 17.3

| align="center" |

137

| align="center" | 60px

| Dwingeloo 1

| SB(s)cd

| 9.13

| 2.8

| −18.78

| 19.8

| align="center" |IC 342/Maffei Group

|35,000 ly

138

| align="center" | 60px

| UGC 9240 (DDO 190)

| IAm

| 9.13

| 2.80

| −14.19

| 13.25

| align="center" |M94 Group

|15,000 ly

139

| align="center" | 60px

| NGC 4190

| Irr (BCD)

| 9.19

| 2.82{{cite journal|bibcode=2013AJ....145..101K|title=Updated Nearby Galaxy Catalog|last1=Karachentsev|first1=Igor D.|last2=Makarov|first2=Dmitry I.|last3=Kaisina|first3=Elena I.|s2cid=118585268|journal=The Astronomical Journal|year=2013|volume=145|issue=4|page=101|doi=10.1088/0004-6256/145/4/101|arxiv=1303.5328}}

| 13.50

| align="center" |

| Satellite of NGC 4214

140

| align="center" |

| Dw1645+46

| 11.09

| 2.9

| 17.6

| align="center" |

140

| align="center" |

| KKs 53 (Cen 7)

| dSph{{cite journal | first1=S. | last1=Côté | first2=K. C. | last2=Freeman | first3=C. | last3=Carigan | first4=P. J. | last4=Quinn | title=Discovery of Numerous Dwarf Galaxies in the Two Nearest Groups of Galaxies | journal=Astronomical Journal | year=1997 | volume=114 | pages=1313 | bibcode=1997AJ....114.1313C | doi=10.1086/118565 | arxiv=astro-ph/9704030 | s2cid=119495338 }}

| 9.56

| 2.93{{cite journal|bibcode=2015ApJ...802L..25T|doi=10.1088/2041-8205/802/2/L25|title=Two Planes of Satellites in the Centaurus A Group|year=2015|last1=Tully|first1=R. Brent|last2=Libeskind|first2=Noam I.|last3=Karachentsev|first3=Igor D.|last4=Karachentseva|first4=Valentina E.|last5=Rizzi|first5=Luca|last6=Shaya|first6=Edward J.|journal=The Astrophysical Journal|volume=802|issue=2|pages=L25|arxiv=1503.05599|s2cid=118512897}}

| −10.86

| 17.30

| align="center" |Centaurus A/M83 Group

141

| align="center" | 60px

| NGC 4214 (UGC 7278)

| IAB(s)m

| 9.59

| 2.94

| 10.24

| align="center" |M94 Group

| Starburst galaxy

142

| align="center" | 60px

| UGCA 276 (DDO 113)

| Im

| 9.62

| 2.95{{cite journal|doi=10.1093/mnras/stz3526| arxiv=1908.11367|title=The case for strangulation in low-mass hosts: DDO 113|year=2020|last1=Garling|first1=Christopher T.|last2=Peter|first2=Annika H G.|last3=Kochanek|first3=Christopher S.|last4=Sand|first4=David J.|last5=Crnojević|first5=Denija|journal=Monthly Notices of the Royal Astronomical Society|volume=492|issue=2|pages=1713–1730|doi-access=free}}

| 15.40

| align="center" |M94 Group

143

| align="center" |60px

| UGCA 133 (DDO 44)

| Im

| 9.65

| 2.96{{cite journal|arxiv=1906.08260|doi=10.3847/1538-4357/ab4c32|title=Tidal Destruction in a Low-mass Galaxy Environment: The Discovery of Tidal Tails around DDO 44|year=2019|last1=Carlin|first1=Jeffrey L.|last2=Garling|first2=Christopher T.|last3=Peter|first3=Annika H. G.|last4=Crnojević|first4=Denija|last5=Forbes|first5=Duncan A.|last6=Hargis|first6=Jonathan R.|last7=Mutlu-Pakdil|first7=Burçin|last8=Pucha|first8=Ragadeepika|last9=Romanowsky|first9=Aaron J.|last10=Sand|first10=David J.|last11=Spekkens|first11=Kristine|last12=Strader|first12=Jay|last13=Willman|first13=Beth|journal=The Astrophysical Journal|volume=886|issue=2|page=109|bibcode=2019ApJ...886..109C|s2cid=195218404 |doi-access=free }}

| −12.9

| 15.54

| align="center" |M81 Group

| Likely satellite of NGC 2403

143

| align="center" | 60px

| NGC 4163 (NGC 4167)

| dIrr

| 9.65

| 2.96{{Cite web |url=http://www.iop.org/EJ/article/1538-3881/131/3/1361/205003.tb1.html |access-date=2009-09-21 |title=Archived copy |archive-date=2020-09-25 |archive-url=https://web.archive.org/web/20200925123153/https://www.iop.org/EJ/article/1538-3881/131/3/1361/205003.tb1.html |url-status=dead }}

| 14.5

| align="center" |M94 Group

|4,000 ly

144

| align="center" | 60px

| UGCA 86

| SAB(s)m

| 9.72

| 2.98{{cite journal|doi=10.1051/0004-6361/202037993|title=KKH 22, the first dwarf spheroidal satellite of IC 342|year=2020|last1=Karachentsev|first1=Igor D.|last2=Makarova|first2=Lidia N.|last3=Brent Tully|first3=R.|last4=Anand|first4=Gagandeep S.|last5=Rizzi|first5=Luca|last6=Shaya|first6=Edward J.|last7=Afanasiev|first7=Viktor L.|s2cid=218538458|journal=Astronomy & Astrophysics|volume=638|pages=A111|arxiv=2005.03132|bibcode=2020A&A...638A.111K}}

| 13.5

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

|20,000 ly

145

| align="center" |60px

| NGC 1560

| SA(s)d HII

| 9.75

| 2.99

| −16.87

| 12.16

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

146

| MADCASH-2 (MADCASH J121007+352635-dw)

| dSph

| 9.78

| 3.00{{cite journal|doi=10.3847/1538-4357/abe040|arxiv=2012.09174|bibcode=2021ApJ...909..211C|title=Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH|year=2021|last1=Carlin|first1=Jeffrey L.|last2=Mutlu-Pakdil|first2=Burçin|last3=Crnojević|first3=Denija|last4=Garling|first4=Christopher T.|last5=Karunakaran|first5=Ananthan|last6=Peter|first6=Annika H. G.|last7=Tollerud|first7=Erik|last8=Forbes|first8=Duncan A.|last9=Hargis|first9=Jonathan R.|last10=Lim|first10=Sungsoon|last11=Romanowsky|first11=Aaron J.|last12=Sand|first12=David J.|last13=Spekkens|first13=Kristine|last14=Strader|first14=Jay|journal=The Astrophysical Journal|volume=909|issue=2|page=211|s2cid=229297953 |doi-access=free }}

| −9.15

| 18.24

| align="center" |M94 Group

| Likely satellite of NGC 4214

147

| Dwingeloo 2

| Im?

| 9.8

| 3.0

| −14.55

| 20.5

| align="center" |IC 342/Maffei Group

|20,000 ly

147

| KKH 11 (ZOAG G135.74-04.53)

| dE/N

| 9.8

| 3.0

| −13.35

| 16.2

| align="center" |IC 342/Maffei Group

147

| KKH 12

| Irr

| 9.8

| 3.0

| −13.03

| 17.8

| align="center" | IC 342/Maffei Group

147

| MB 3

| dSph

| 9.8

| 3.0

| −13.65

| 19.8

| align="center" |IC 342/Maffei Group

|10,000 ly

147

| MB 1 (KK 21)

| SAB(s)d?

| 9.8

| 3.0

| −14.81

| 20.5

| align="center" |IC 342/Maffei Group

|5,000 ly

147

| align="center" |60px

| Maffei 1

| S0- pec

| 9.8

| 3.0

| −18.97

| 11.4

| align="center" |IC 342/Maffei Group

|55,000 ly

153

| align="center" | 60px

| Maffei 2

| SAB(rs)bc

| 9.801

| 3.005

| −20.15

| 14.77

| align="center" |IC 342/Maffei Group

|60,000 ly

154

| align="center" | 60px

| UGC 8651 (DDO 181)

| Im

| 9.82

| 3.01

| 14.7

| align="center" |M94 Group

155

| align="center" | 60px

| Donatiello I

| dSph

| 9.88

| 3.04

| align="center" |

| Possible satellite of NGC 404

156

| align="center" | 60px

| NGC 2403

| SAB(s)cd HII

| 9.92

| 3.04

| −19.29

| 8.93

| align="center" |Inner edge of M81 Group

| 50,000 ly

157

| align="center" | 60px

| NGC 404

| SA(s)0-:

| 10.05

| 3.08

| −16.61

| 11.21

| align="center" |

| 'Mirach's Ghost'

158

| align="center" | 60x60px

| ESO 274-01{{cite journal|doi= 10.1086/510125|title= The Hubble Flow around the Centaurus A/M83 Galaxy Complex|year= 2007|last1= Karachentsev|first1= Igor D.|last2= Tully|first2= R. Brent|last3= Dolphin|first3= Andrew|last4= Sharina|first4= Margarita|last5= Makarova|first5= Lidia|last6= Makarov|first6= Dmitry|last7= Sakai|first7= Shoko|last8= Shaya|first8= Edward J.|last9= Kashibadze|first9= Olga G.|last10= Karachentseva|first10= Valentina|last11= Rizzi|first11= Luca|journal= The Astronomical Journal|volume= 133|issue= 2|pages= 504–517|arxiv= astro-ph/0603091|bibcode= 2007AJ....133..504K|s2cid= 120584}}

| SAd:

| 10.1

| 3.09

| 11.7

| align="center" |Centaurus A/M83 Group

159

| align="center" |

| Dw1558+67

| 10.1

| 3.1

| 16.8

| align="center" |

159

| align="center" |

| GALFA-Dw4{{cite journal|doi=10.3847/1538-4357/ac356c|title=Hubble Space Telescope Imaging of Isolated Local Volume Dwarfs GALFA-Dw3 and Dw4|year=2022|last1=Bennet|first1=P.|last2=Sand|first2=D. J.|last3=Crnojević|first3=D.|last4=Weisz|first4=D. R.|last5=Caldwell|first5=N.|last6=Guhathakurta|first6=P.|last7=Hargis|first7=J. R.|last8=Karunakaran|first8=A.|last9=Mutlu-Pakdil|first9=B.|last10=Olszewski|first10=E.|last11=Salzer|first11=J. J.|last12=Seth|first12=A. C.|last13=Simon|first13=J. D.|last14=Spekkens|first14=K.|last15=Stark|first15=D. P.|last16=Strader|first16=J.|last17=Tollerud|first17=E. J.|last18=Toloba|first18=E.|last19=Willman|first19=B.|journal=The Astrophysical Journal|volume=924|issue=2|page=98|arxiv=2101.08270|bibcode=2022ApJ...924...98B|s2cid=231662303 |doi-access=free }}

| dIrr

| 10.1

| 3.10

| −11.8

| 15.7

| align="center" |

| Isolated

160

| KKH 22

| dSph

| 10.17

| 3.12

| –12.19

| 15.28

| align="center"|IC 342/Maffei Group

| Satellite of IC 342

161

| align="center" | 60px

| NGC 3741

| ImIII/BCD

| 10.21

| 3.13

| 14.3

| align="center" |M94 Group

162

| KK 35

| Irr

| 10.31

| 3.16

| −14.30

| 17.2

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

162

| HIPASS J1247-77

| Im

| 10.31

| 3.16

| 17.B

| Aligned with IC 3104

164

| align="center" |60px

| NGC 2366

| IB(s)m

| 10.40

| 3.19

| 11.43

| align="center" |M81 Group

164

| align="center" | 60px

| NGC 1569 (UGC 3056)

| IBm;Sbrst

| 10.40

| 3.19

| −18.17

| 11.86

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

|6,000 ly

164

| align="center" | 60px

| ESO 321-014

| IBm

| 10.40

| 3.19

| 15.16

| align="center" |Centaurus A/M83 Group

167

| align="center" | 60px

| UGC 8833

| Im

| 10.41

| 3.19

| 16.5

| align="center" |M94 Group

168

| align="center" | 60px

| Sculptor dIG (ESO 349–31)

| dIrr

| 10.44

| 3.2{{cite journal|arxiv=1211.0137|doi=10.1051/0004-6361/201220193|bibcode=2013A&A...549A..47L|title=The star formation history of the Sculptor Dwarf Irregular Galaxy|year=2013|last1=Lianou|first1=S.|last2=Cole|first2=A. A.|s2cid=55237783|journal=Astronomy & Astrophysics|volume=549|pages=A47}}

| −11.87

| 15.5

| align="center" |Sculptor Group

| Satellite of NGC 7793

169

| align="center" | 60px

| UGC 4483

| dIrr

| 10.47

| 3.21

| 15.2

| align="center" |M81 Group

169

| align="center" |

| dw0910p7326 ("Blobby")

| dSph

| 10.47

| 3.21{{cite journal | arxiv=2211.00629 | doi=10.1093/mnras/stad352 | title=Discovery of a red backsplash galaxy candidate near M81 | year=2023 | last1=Casey | first1=Kirsten J. | last2=Greco | first2=Johnny P. | last3=Peter | first3=Annika H G. | last4=Davis | first4=A Bianca | journal=Monthly Notices of the Royal Astronomical Society | volume=520 | issue=3 | pages=4715–4729 | doi-access=free }}

| 11.57

| 15.96

| align="center" |M81 Group

170

| UGC 8760 (DDO 183)

| I

| 10.50

| 3.22

| align="center"|

| −13.08

| 14.78{{cite simbad|title=UGC 8760|access-date=2025-02-08}}

170

| align="center" |60px

| UGCA 92

| Im?

| 10.50

| 3.22

| 13

| align="center" | IC 342/Maffei Group{{Cite journal |title=see article at |journal=The Astrophysical Journal Supplement Series |date=September 1999 |volume=124 |issue=1 |pages=33–93 |doi=10.1086/313255 |s2cid=119907629 |last1=Buta |first1=Ronald J. |last2=McCall |first2=Marshall L. |doi-access=free }}

| Satellite of IC 342

171

| align="center" | 60px

| IC 342

| SAB(rs)cd

| 10.70

| 3.28

| −20.69

| 9.37

| align="center" |IC 342/Maffei Group

| "the hidden galaxy"

|75,000 ly

173

| align="center" | 60px

| UGCA 15 (DDO 6)

| IB(s)m

| 10.90

| 3.34

| −12.50

| 15.19

| align="center" |Sculptor group

174

| KKs 58

| dSph

| 10.96

| 3.36{{cite journal|doi=10.1051/0004-6361/201935807|title=The dwarf galaxy satellite system of Centaurus A|year=2019|last1=Müller|first1=Oliver|last2=Rejkuba|first2=Marina|last3=Pawlowski|first3=Marcel S.|last4=Ibata|first4=Rodrigo|last5=Lelli|first5=Federico|last6=Hilker|first6=Michael|last7=Jerjen|first7=Helmut|journal=Astronomy & Astrophysics|volume=629|pages=A18|arxiv=1907.02012|bibcode=2019A&A...629A..18M|s2cid=195791783}}

| −11.93

| align="center" |Centaurus A/M83 Group

175

| align="center" |60px

| KKH 37 (Mai 16)

| S/Irr

| 11.06

| 3.39{{cite journal|doi=10.1086/500013|title=Advanced Camera for Surveys Imaging of 25 Galaxies in Nearby Groups and in the Field|year=2006|last1=Karachentsev|first1=Igor D.|last2=Dolphin|first2=Andrew|last3=Tully|first3=R. Brent|last4=Sharina|first4=Margarita|last5=Makarova|first5=Lidia|last6=Makarov|first6=Dmitry|last7=Karachentseva|first7=Valentina|last8=Sakai|first8=Shoko|last9=Shaya|first9=Edward J.|journal=The Astronomical Journal|volume=131|issue=3|pages=1361–1376|arxiv=astro-ph/0511648|bibcode=2006AJ....131.1361K|s2cid=16689229}}

| 16.4

| align="center" |IC 342/Maffei Group

175

| align="center" | 60px

| UGCA 105

| Im?

| 11.06

| 3.39

| −16.81

| 13.9

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

175

| align="center" | 60px

| Holmberg II (DDO 50, UGC 4305)

| Im

| 11.06

| 3.39

| 11.1

| align="center" |M81 Group

175

| align="center" |

| Dw1559+46

| 11.09

| 3.4

| 17.1

| align="center" |

175

| align="center" | 60px

| NGC 5102

| SA0- HII

| 11.09

| 3.40

| −18.0856

| 10.35

| align="center" |Centaurus A/M83 Group

175

| align="center" | 60px

| NGC 5237

| I0?

| 11.09

| 3.40

| 13.23

| align="center" |Centaurus A/M83 Group

175

| align="center" | 60px

| ESO 325-11

| 11.09

| 3.40

| 13.99

| align="center" |Centaurus A/M83 Group

175

| align="center" | 60px

| ESO 540-030 (KDG 2)

| IABm

| 11.09

| 3.40

| −11.39

| 16.45

| align="center" |Sculptor group

182

| align="center" | 60px

| NGC 247

| SAB(s)d

| 11.1

| 3.4

| −20.00

| 9.9

| align="center" |Sculptor group

183

| MADCASH-1 (MADCASH J074238+652501-dw)

| dSph

| 11.12

| 3.41

| −7.81

| 19.85

| align="center" |M81 Group

| Likely satellite of NGC 2403

184

| F6D1 (FM 1, PGC 3097828)

| dSph{{cite journal|doi=10.1088/0004-6256/137/2/3009|title=Discovery of New Dwarf Galaxies in the M81 Group|year=2009|last1=Chiboucas|first1=Kristin|last2=Karachentsev|first2=Igor D.|last3=Tully|first3=R. Brent|s2cid=14156955|journal=The Astronomical Journal|volume=137|issue=2|pages=3009–3037|arxiv=0805.1250|bibcode=2009AJ....137.3009C}}

| 11.15

| 3.42

| 17.5

| align="center" |M81 Group

184

| align="center" | 60px

| ESO 540-032

| IAB(s)m pec:

| 11.15

| 3.42

| −11.32

| 16.55

| align="center" |Sculptor group

186

| align="center" | 60px

| ESO 383-087 (ISG 39)

| SB(s)dm

| 11.25

| 3.45

| −15.16

| 11.03

| align="center" |Centaurus A/M83 Group

187

| align="center" | 60px

| NGC 5206

| SB0

| 11.32

| 3.47

| align="center" |Centaurus A/M83 Group

188

| align="center" | 60px

| KK 179 (ESO 269-37)

| IABm:

| 11.4

| 3.48

| align="center" |Centaurus A/M83 Group

188

| align="center" |

| Corvus A

| 11.4

| 3.48{{cite journal | doi=10.3847/2041-8213/ad676e | doi-access=free | title=Corvus A: A Low-mass, Isolated Galaxy at 3.5 MPC | date=2024 | last1=Jones | first1=Michael G. | last2=Sand | first2=David J. | last3=Mutlu-Pakdil | first3=Burçin | last4=Fielder | first4=Catherine E. | last5=Crnojević | first5=Denija | last6=Bennet | first6=Paul | last7=Spekkens | first7=Kristine | last8=Donnerstein | first8=Richard | last9=Doliva-Dolinsky | first9=Amandine | last10=Karunakaran | first10=Ananthan | last11=Strader | first11=Jay | last12=Zaritsky | first12=Dennis | journal=The Astrophysical Journal Letters | volume=971 | issue=2 | pages=L37 | arxiv=2407.03393 | bibcode=2024ApJ...971L..37J }}

| −11.2

| align="center" |

193

| align="center" |

|Scl-MM-dw3

| 11.35

| 3.48

| −7.24

| align="center" |Sculptor Group

189

| align="center" | 60px

| Sculptor Galaxy
(NGC 253)

| SAB(s)c

| 11.40

| 3.49

| 8.0

| align="center" |Sculptor group

|90,000 ly

190

| align="center" | 60px

| DDO 71 (UGC 5428)

| Im

| 11.42

| 3.50

| 18

| align="center" |M81 Group

191

| Camelopardalis B

| Irr

| 11.46

| 3.50

| −11.85

| 16.1

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

192

| align="center" | 60px

|Messier 82

| I0;Sbrst HII

| 11.42

| 3.53

| −19.63

| 9.30

| align="center" |M81 Group

|37,000 ly, possibly up to 100,000 ly

193

| align="center" | 60px

|NGC 5253

| Im pec

| 11.51

| 3.53

| 10.9

| align="center" |Centaurus A/M83 Group

|Nearest Wolf-Rayet galaxy to us.

193

| align="center" |

|Scl-MM-dw1

| 11.51

| 3.53

| −8.75{{cite journal | doi=10.3847/1538-4357/ac4418 | doi-access=free | arxiv=2108.09312 | bibcode=2022ApJ...926...77M | title=Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies | date=2022 | last1=Mutlu-Pakdil | first1=Burçin | last2=Sand | first2=David J. | last3=Crnojević | first3=Denija | last4=Jones | first4=Michael G. | last5=Caldwell | first5=Nelson | last6=Guhathakurta | first6=Puragra | last7=Seth | first7=Anil C. | last8=Simon | first8=Joshua D. | last9=Spekkens | first9=Kristine | last10=Strader | first10=Jay | last11=Toloba | first11=Elisa | journal=The Astrophysical Journal | volume=926 | issue=1 | page=77 }}

| align="center" | Sculptor Group

193

| align="center" |

|Scl-MM-dw2

| 11.51

| 3.53

| −12.10

| align="center" |Sculptor Group

194

|M81 Dwarf A (KDG 52)

| I?

| 11.58

| 3.55

| −11.49

| 16.5

| align="center" |M81 Group

194

| align="center" | 60px

| KK 77 (F12D1)

| dSph

| 11.58

| 3.55

| 16.2

| align="center" |M81 Group

196

| align="center" | 60px

| NGC 2976

| SAc pec HII

| 11.61

| 3.56

| −17.1

| 10.82

| align="center" |M81 Group

196

| Camelopardalis A

| 11.61

| 3.56

| align="center" |IC 342/Maffei Group

| Satellite of IC 342

198

| KK 211 (AM 1339–445)

| dSph{{cite journal|bibcode=2008ApJ...674..909P|doi=10.1086/525038|title=VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies|year=2008|last1=Puzia|first1=Thomas H.|last2=Sharina|first2=Margarita E.|journal=The Astrophysical Journal|volume=674|issue=2|pages=909–926|arxiv=0710.1550 |s2cid=14231914}}

| 11.68

| 3.58

| −11.93

| 16.32

| align="center" |Centaurus A/M83 Group

| Satellite of NGC 5128

198

| PGC 51659 (UKS 1424–460)

| IBm{{cite journal|doi=10.1093/mnras/stu1646|title=Deep near-infrared surface photometry and properties of Local Volume dwarf irregular galaxies|year=2014|last1=Young|first1=T.|last2=Jerjen|first2=H.|last3=López-Sánchez|first3=Á. R.|last4=Koribalski|first4=B. S.|journal=Monthly Notices of the Royal Astronomical Society|volume=444|issue=4|pages=3052–3077|doi-access=free |arxiv=1408.2609}}

| 11.68

| 3.58

| −11.83

| 16.50

| align="center" |Centaurus A/M83 Group

198

| KDG 61

| dE/dSph

| 11.68

| 3.58{{cite journal|doi=10.1111/j.1365-2966.2010.16746.x|title=Star formation history of KDG 61 and KDG 64 from spectroscopy and colour-magnitude diagrams|year=2010|last1=Makarova|first1=Lidia|last2=Koleva|first2=Mina|last3=Makarov|first3=Dmitry|last4=Prugniel|first4=Philippe|journal=Monthly Notices of the Royal Astronomical Society|volume=406|issue=2|page=1152|doi-access=free |arxiv=1003.6061|bibcode=2010MNRAS.406.1152M|s2cid=119281422}}

| −12.84

| 14.93

| align="center" |M81 Group

201

| align="center" | 60px

| NGC 4945

| SB(s)cd:sp

| 11.70I. D. Karachentsev et al.(2002) New distances to galaxies in the Centaurus A group

| 3.59

| −20.51

| 9.3

| align="center" |Centaurus A/M83 Group

202

| align="center" | 60px

| NGC 6789

| Im

| 11.74

| 3.6

| −14.32

| 13.76

| In the Local Void{{cite journal|bibcode=2014MNRAS.445.1694L|doi=10.1093/mnras/stu1804|arxiv=1409.1239|title=The triggering of starbursts in low-mass galaxies|year=2014|last1=Lelli|first1=Federico|last2=Verheijen|first2=Marc|last3=Fraternali|first3=Filippo|journal=Monthly Notices of the Royal Astronomical Society|volume=445|issue=2|pages=1694–1712|doi-access=free }}

202

| align="center" | 60px

| Messier 81

| SA(s)ab, LINER

| 11.74

| 3.6

| 6.94

| align="center" |M81 Group

| Brightest galaxy in M81 Group

| 90,000 ly

202

| align="center" |

| UGC 6451

| 11.74

| 3.6

| 15.4

| align="center" |

204

| align="center" | 60px

| Holmberg IX (UGC 5336, DDO 66)

| Irr

| 11.77

| 3.61

| 14.53

| align="center" |M81 Group

| Contains ultraluminous X-ray source (ULX) Holmberg IX X-1

204

| align="center" | 60px

| UGCA 292 (CVn I dwA)

| ImIV-V

| 11.77

| 3.61

| 16.0

| align="center" |M94 Group

206

| BK 5N

| dSph

| 11.84

| 3.63

| 17.49

| align="center" |M81 Group

207

| DDO 78 (KK 89)

| dSph

| 11.94

| 3.66{{cite journal|bibcode=2009ApJS..183...67D|doi=10.1088/0067-0049/183/1/67|title=The ACS Nearby Galaxy Survey Treasury|year=2009|last1=Dalcanton|first1=Julianne J.|last2=Williams|first2=Benjamin F.|last3=Seth|first3=Anil C.|last4=Dolphin|first4=Andrew|last5=Holtzman|first5=Jon|last6=Rosema|first6=Keith|last7=Skillman|first7=Evan D.|last8=Cole|first8=Andrew|last9=Girardi|first9=Léo|last10=Gogarten|first10=Stephanie M.|last11=Karachentsev|first11=Igor D.|last12=Olsen|first12=Knut|last13=Weisz|first13=Daniel|last14=Christensen|first14=Charlotte|last15=Freeman|first15=Ken|last16=Gilbert|first16=Karoline|last17=Gallart|first17=Carme|last18=Harris|first18=Jason|last19=Hodge|first19=Paul|last20=De Jong|first20=Roelof S.|last21=Karachentseva|first21=Valentina|last22=Mateo|first22=Mario|last23=Stetson|first23=Peter B.|last24=Tavarez|first24=Maritza|last25=Zaritsky|first25=Dennis|last26=Governato|first26=Fabio|last27=Quinn|first27=Thomas|journal=The Astrophysical Journal Supplement Series|volume=183|issue=1|pages=67–108|arxiv=0905.3737|s2cid=5032304}}

| 16.50

| align="center" |M81 Group

207

| F8D1

| dSph

| 11.94

| 3.66

| −12.20{{cite journal|doi=10.1088/0004-637X/739/1/5|title=The ACS Nearby Galaxy Survey Treasury. VIII. The Global Star Formation Histories of 60 Dwarf Galaxies in the Local Volume|year=2011|last1=Weisz|first1=Daniel R.|last2=Dalcanton|first2=Julianne J.|last3=Williams|first3=Benjamin F.|last4=Gilbert|first4=Karoline M.|last5=Skillman|first5=Evan D.|last6=Seth|first6=Anil C.|last7=Dolphin|first7=Andrew E.|last8=McQuinn|first8=Kristen B. W.|last9=Gogarten|first9=Stephanie M.|last10=Holtzman|first10=Jon|last11=Rosema|first11=Keith|last12=Cole|first12=Andrew|last13=Karachentsev|first13=Igor D.|last14=Zaritsky|first14=Dennis|journal=The Astrophysical Journal|volume=739|issue=1|page=5|arxiv=1101.1093|bibcode=2011ApJ...739....5W|s2cid=119230989}}

| 15.70

| align="center" |M81 Group

209

| align="center" |60px

| UGC 4459 (DDO 53)

| Im

| 12.00

| 3.68{{cite journal|doi=10.1093/mnras/stab2710|arxiv=2109.08526|title=Star formation in the nearby dwarf galaxy DDO 53: Interplay between gas accretion and stellar feedback|year=2021|last1=Egorov|first1=Oleg V.|last2=Lozinskaya|first2=Tatiana A.|last3=Vasiliev|first3=Konstantin I.|last4=Yarovova|first4=Anastasiya D.|last5=Gerasimov|first5=Ivan S.|last6=Kreckel|first6=Kathryn|last7=Moiseev|first7=Alexei V.|journal=Monthly Notices of the Royal Astronomical Society|volume=508|issue=2|pages=2650–2667|doi-access=free }}

| −13.37

| 14.48

| align="center" |M81 Group

210

| align="center" | 60px

| Centaurus A (NGC 5128)

| S0 pec

| 12.01

| 3.68

| 6.84

| align="center" |Centaurus A/M83 Group

| Brightest galaxy in Centaurus A Group and brightest and nearest radio galaxy

| 60,000 ly

211

| KDG 64 (UGC 5442)

| dE/dSph

| 12.07

| 3.70

| −12.55

| 15.29

| align="center" |M81 Group

212

| IKN

| dE

| 12.23

| 3.75

| −14.29{{cite journal|doi=10.3847/1538-4357/ab44a7|title=Stellar Population and Structural Properties of Dwarf Galaxies and Young Stellar Systems in the M81 Group|year=2019|last1=Okamoto|first1=Sakurako|last2=Arimoto|first2=Nobuo|last3=Ferguson|first3=Annette M. N.|last4=Irwin|first4=Mike J.|last5=Bernard|first5=Edouard J.|last6=Utsumi|first6=Yousuke|journal=The Astrophysical Journal|volume=884|issue=2|page=128|arxiv=1909.12997|bibcode=2019ApJ...884..128O|s2cid=203593758 |doi-access=free }}

| align="center" |M81 Group

212

| KKs 54

| dSph

| 12.23

| 3.75

| −10.41

| align="center" |Centaurus A/M83 Group

213

|align="center"| 60px

| NGC 5011C (ESO 269–68)

| dE/Im{{cite journal|doi=10.1086/512157|title=NGC 5011C: An Overlooked Dwarf Galaxy in the Centaurus A Group|last1=Saviane|first1=Ivo|last2=Jerjen|first2=Helmut|year=2007|journal=The Astronomical Journal|volume=133|issue=4|pages=1756–1762|arxiv=astro-ph/0701280|bibcode=2007AJ....133.1756S|s2cid=14755909 }}

| 12.3

| 3.77{{cite journal

| title=Dual Stellar Halos in the Standard Elliptical Galaxy M105 and Formation of Massive Early-type Galaxies

| last1=Lee | first1=Myung Gyoon | last2=Jang | first2=In Sung

| journal=The Astrophysical Journal

| doi=10.3847/0004-637X/822/2/70

| bibcode=2016ApJ...822...70L | arxiv=1601.06798 | s2cid=118372642 | doi-access=free }}

| −14.74

| 13.47

| align="center" |Centaurus A/M83 Group

213

| align="center" |

| Centaurus N

| 12.3

| 3.77{{cite journal|doi=10.1051/0004-6361/200913429|title=A close look at the Centaurus a group of galaxies|year=2010|last1=Crnojević|first1=D.|last2=Grebel|first2=E. K.|last3=Koch|first3=A.|journal=Astronomy and Astrophysics|volume=516|pages=A85|doi-access=free|arxiv=1002.0341}}

| −11.15

| align="center" |Centaurus A/M83 Group

213

| align="center" |

| KK 213

| dSph

| 12.3

| 3.77

| 18.00

| align="center" |Centaurus A/M83 Group

213

| align="center" |

| KK 203

| dSph

| 12.30

| 3.77{{cite journal|doi=10.1051/0004-6361/202039359|title=The properties of dwarf spheroidal galaxies in the Cen A group. Stellar populations, internal dynamics, and a heart-shaped Hα ring|year=2021|last1=Müller|first1=Oliver|last2=Fahrion|first2=Katja|last3=Rejkuba|first3=Marina|last4=Hilker|first4=Michael|last5=Lelli|first5=Federico|last6=Lutz|first6=Katharina|last7=Pawlowski|first7=Marcel S.|last8=Coccato|first8=Lodovico|last9=Anand|first9=Gagandeep S.|last10=Jerjen|first10=Helmut|journal=Astronomy & Astrophysics|volume=645|pages=A92|arxiv=2011.04990|s2cid=226289648|bibcode=2021A&A...645A..92M}}

| −11.7

| align="center" |Centaurus A/M83 Group

| In Centaurus A Group; contains a ring of Hα emission

rowspan="2" align="center"|#

! rowspan="2" |

! rowspan="2" |Galaxy

! rowspan="2" |Type

! colspan="2" |Dist from Earth

! colspan="2" |Magnitude

! rowspan="2" align="center"|Group
Membership

! rowspan="2" |Notes

Mly

! Mpc

! M

! m

Notes

References

External links

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{{cite journal

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|title = Deep Hubble Space Telescope Imaging of Sextans A. II. Cepheids and Distance

|journal = The Astronomical Journal

|volume = 125

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|url = http://www.iop.org/EJ/article/1538-3881/125/3/1261/202477.html

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{{cite journal

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{{cite journal

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| name-list-style=vanc

| author2=I. D.

| display-authors=2

| last3=Huchtmeier

| first3=Walter K.

| last4=Makarov

| first4=Dmitry I.

| doi-access=free

}}

{{cite journal

| author=Karachentsev, I. D.

| title=The Local Group and Other Neighbouring Galaxy Groups

| journal=Astronomical Journal

| date=2005

| volume=129

| issue=1

| pages=178–188

| url=http://www.iop.org/EJ/abstract/1538-3881/129/1/178

| doi=10.1086/426368

| bibcode=2005AJ....129..178K

|arxiv = astro-ph/0410065 | s2cid=119385141

}}

{{cite journal

| author=McConnachie

| date=2005

| title=Distances and Metallicities for 17 Local Group Galaxies

| journal=MNRAS

| volume=356

| issue=3

| pages=979–997

| arxiv=astro-ph/0410489

| doi=10.1111/j.1365-2966.2004.08514.x

| bibcode=2005MNRAS.356..979M

| name-list-style=vanc

| author2=A. W.

| display-authors=2

| last3=Ferguson

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| last4=Ibata

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| last5=Lewis

| first5=G. F.

| last6=Tanvir

| first6=N.

| doi-access=free

}}

{{cite journal

| author=Tonry

| title=The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances

| journal=Astrophysical Journal

| date=2001

| volume=546

| issue=2

| pages=681–693

| bibcode=2001ApJ...546..681T | doi=10.1086/318301

|arxiv = astro-ph/0011223

| name-list-style=vanc

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| display-authors=2

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| last4=Ajhar

| first4=Edward A.

| last5=Fletcher

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| last6=Luppino

| first6=Gerard A.

| last7=Metzger

| first7=Mark R.

| last8=Moore

| first8=Christopher B. | s2cid=17628238

}}

{{cite journal

|author = Van den Bergh, S.

|date = April 2000

|title = Updated Information on the Local Group

|journal = The Publications of the Astronomical Society of the Pacific

|volume = 112

|issue = 770

|pages = 529–536

|doi = 10.1086/316548

|bibcode = 2000PASP..112..529V

|arxiv = astro-ph/0001040

|s2cid = 1805423

}}

Nearest galaxies

nearest galaxies

list of nearest galaxies

List

See also

Notes

References

External links