:List of star systems within 20–25 light-years

This is a list of star systems within 20–25 light years of Earth. So far, 84 such objects have been found, of which only 7 are bright enough to be visible without a telescope.

class="wikitable sortable" style="font-size:1.00em; line-height:1.5em;"

|+Key

| style="background-color: lightblue"| {{Hash-tag|alt=visible to naked eye}}

|Visible to the unaided eye

style="background-color: lightgreen"| {{Dollar sign}}

|Bright star (absolute magnitude of +8.5 or brighter)

style="background-color:#F5F5DC"| {{Double-dagger|alt=white dwarf}}

|White dwarf

style="background-color:#D8BD98"| §

|Brown dwarf or sub-brown dwarf

style="background-color: pink"| {{Asterisk}}

|Nearest in constellation

scope="col" \| System←→←→ ! Star or (sub-) brown dwarf ! scope="col" \| Distance (ly) ! Constellation ! Coordinates: RA, Dec (Ep J2000, Eq J2000) ! scope="col" \| Stellar class ! scope="col" \| Apparent magnitude (V) ! scope="col" \| Parallax (mas) ! scope="col" \| Notes and additional references
class="wikitable sortable" style="font-size:90%; line-height:1.5em; position:relative"
colspan = '2' \| Gliese 784 (HD 191849)	20.1062{{±\|0.0028}}	Telescopium	{{RA\|20\|13\|53.4}} {{DEC
45\|09\|50}}	style="background: {{star-color\|M}};" \| M0V	7.97	162.2171{{±\|0.0225}}	has 1 candidate planet {{cite arXiv\|last1=Barnes\|first1=J. R.\|last2=Kiraga\|first2=M.\|last3=Diaz\|first3=M.\|last4=Berdiñas\|first4=Z.\|last5=Jenkins\|first5=J. S.\|last6=Keiser\|first6=S.\|last7=Thompson\|first7=I.\|last8=Crane\|first8=J. D.\|last9=Shectman\|first9=S. A.\|display-authors=1\|date=2019-06-11\|title=Frequency of planets orbiting M dwarfs in the Solar neighbourhood\|class=astro-ph.EP\|eprint=1906.04644\|language=en}}
colspan = '2' style="background: #D8BD98" \| WISE J2209+2711§	20.17{{±\|0.25}}	style="background-color: pink" \| Pegasus{{Asterisk}}	{{RA\|22\|09\|05.7}} {{DEC\|+27\|11\|44}}	style="background: {{star-color\|Y}};" \| Y0		{{val\|161.7\|2.0}}
colspan = '2' style="background: #F5F5DC" \| G 240-72 (LHS 455, GJ 1221, EGGR 372){{Double-dagger\|alt=white dwarf}} \| 20.2588{{±\|0.0015}} \| Draco \| {{RA\|17\|48\|08.2}} {{DEC\|+70\|52\|35}} \| style="background: #F5F5DC" \| DXP9 \| 14.22 \| 160.9952{{±\|0.0119}} \|
colspan = '2' \| Gliese 555 (Wolf 1481, HN Librae, {{nowrap\|BD-11 3759}})	20.3947{{±\|0.0070}}	Libra	{{RA\|14\|34\|16.8}} {{DEC
12\|31\|10}}	style="background: {{star-color\|M}};" \| M4.0V	10.3–10.33	159.9225{{±\|0.0546}}	BY Draconis variable; has 1 known planet
rowspan='2' \| EQ Pegasi (Gliese 896, BD+19 5116)	A	rowspan='2' \| 20.4277{{±\|0.0044}}	rowspan='2' \| Pegasus	rowspan='2' \| {{RA\|23\|31\|52.2}} {{DEC\|+19\|56\|14}}	style="background: {{star-color\|M}};" \| M3.5V	10.35	rowspan='2' \| 159.6634{{±\|0.0341}}	rowspan='2' \| both components are flare stars; has 1 known planet orbiting star A of the binary system {{cite journal \|arxiv=2208.14553 \|last1=Curiel \|first1=Salvador \|last2=Ortiz-León \|first2=Gisela N. \|last3=Mioduszewski \|first3=Amy J. \|last4=Sanchez-Bermudez \|first4=Joel \|date=31 May 2022\|publication-date=1 September 2022 \|title=3D Orbital Architecture of a Dwarf Binary System and Its Planetary Companion \|journal=The Astronomical Journal \|volume=164:93 \|issue=3 \|pages=23pp \|doi=10.3847/1538-3881/ac7c66\|doi-access=free \|bibcode=2022AJ....164...93C}}
\| B	style="background: {{star-color\|M}};" \| M4.5V	12.4
colspan = '2' \| Gliese 581 (Wolf 562, HO Librae)	20.5494{{±\|0.0039}}	Libra	{{RA\|15\|19\|26.8}} {{DEC\|−07\|43\|20}}	style="background: {{star-color\|M}};" \| M3.0V	10.56–10.58	158.7183{{±\|0.0301}}	BY Draconis variable; has 3 known planets
colspan = '2' style="background: #D8BD98" \|WISE 1405+5534§ \| 20.62{{±\|0.34}} \| Ursa Major	{{RA\|14\|05\|18.3}} {{DEC\|+55\|34\|21}} \| style="background: {{star-color\|Y}};" \| Y0.5 \| \| {{Val\|158.2\|2.6}} \|{{Cite journal\|last1=Kirkpatrick\|first1=J. Davy\|last2=Gelino\|first2=Christopher R.\|last3=Faherty\|first3=Jacqueline K.\|author3-link=Jackie Faherty\|last4=Meisner\|first4=Aaron M.\|last5=Caselden\|first5=Dan\|last6=Schneider\|first6=Adam C.\|last7=Marocco\|first7=Federico\|last8=Cayago\|first8=Alfred J.\|last9=Smart\|first9=R. L.\|last10=Eisenhardt\|first10=Peter R.\|last11=Kuchner\|first11=Marc J.\|title=The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs\|journal=The Astrophysical Journal Supplement Series\|year=2021\|volume=253\|issue=1\|page=7\|doi=10.3847/1538-4365/abd107\|arxiv=2011.11616\|bibcode=2021ApJS..253....7K\|s2cid=227126954 \|doi-access=free }}
rowspan='2' \| ADS 7251 (HD 79210, Gliese 338, MCC 541)	A	rowspan='2'\| 20.6575{{±\|0.0026}}	rowspan='2'\| Ursa Major	rowspan='2'\| {{RA\|09\|14\|22.8}} {{DEC\|+52\|41\|12}}	style="background: {{star-color\|M}};" \| M0V	7.64	rowspan='2'\| 157.8879{{±\|0.0197}}	rowspan='2' \| has 1 known planet orbiting star B of the binary system {{Cite journal\|last1=González-Álvarez\|first1=E.\|last2=Osorio\|first2=M. R. Zapatero\|last3=Caballero\|first3=J. A.\|last4=Sanz-Forcada\|first4=J.\|last5=Béjar\|first5=V. J. S.\|last6=González-Cuesta\|first6=L.\|last7=Dreizler\|first7=S.\|last8=Bauer\|first8=F. F.\|last9=Rodríguez\|first9=E.\|last10=Tal-Or\|first10=L.\|last11=Zechmeister\|first11=M.\|date=May 2020\|title=The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B)\|arxiv=2003.13052\|journal=Astronomy & Astrophysics\|volume=637\|pages=A93\|doi=10.1051/0004-6361/201937050\|bibcode=2020A&A...637A..93G\|issn=0004-6361\|doi-access=free}}
\| B	style="background: {{star-color\|K}};" \| K7V	7.70
colspan = '2' \| LHS 2090 ({{nowrap\|LP 368-128}})	20.7388{{±\|0.0071}}	Cancer	{{RA\|09\|00\|23.6}} {{DEC\|+21\|50\|05}}	style="background: {{star-color\|M}};" \| M6.5V	16.10	157.2686{{±\|0.0535}}
rowspan='2' \| Furuhjelm 46 (HD 155876, Gliese 661)	A	rowspan='2' \| 20.82{{±\|0.18}}	rowspan='2' \| Hercules	rowspan='2' \| {{RA\|17\|12\|07.9}} {{DEC\|+45\|39\|57}}	style="background: {{star-color\|M}};" \| M3 V	9.93	rowspan='2' \| {{val\|156.66\|1.37}}	rowspan='2' \|
\| B	style="background: {{star-color\|M}};" \| M3.5 V	10.35
colspan = '2' style="background: #D8BD98" \| 2MASS 1503+2525§	20.94{{±\|0.10}}	Boötes	{{RA\|15\|03\|19.6}} {{DEC\|+25\|25\|20}}	style="background: {{star-color\|T}};" \| T5.5		155.7758{{±\|0.7557}}
colspan = '2' style="background: #D8BD98" \| LP 944-20§	20.9615{{±\|0.0070}}	style="background-color: pink" \| Fornax{{Asterisk}}	{{RA\|03\|39\|35.2}} {{DEC\|–35\|25\|44}}	style="background: {{star-color\|M}};" \| M9V	18.69	155.5982{{±\|0.0522}}
colspan = '2' style="background: #F5F5DC"; \| LP 658-2 (EGGR 45){{Double-dagger\|alt=white dwarf}}	21.0102{{±\|0.0024}}	Orion	{{RA\|05\|55\|09.5}} {{DEC\|−04\|10\|07}}	style="background: #F5F5DC" \| DZ11	14.45	{{val\|155.2373\|0.0175}}
colspan = '2' \| GL Virginis (G 12-30)	21.0832{{±\|0.0061}}	Virgo	{{RA\|12\|18\|59.4}} {{DEC\|+11\|07\|34}}	style="background: {{star-color\|M}};" \| M5Ve	13.79	{{val\|154.6999\|0.0445}}	flare star
colspan = '2' \| Gliese 625 (AC 54 1646-56, G 202-48)	21.1309{{±\|0.0022}}	Draco	{{RA\|16\|25\|24.6}} {{DEC\|+54\|18\|15}}	style="background: {{star-color\|M}};" \| M2.0V	10.17	{{val\|154.3503\|0.0161}}	{{Cite journal\|arxiv = 1705.06537\|doi = 10.1051/0004-6361/201730957\|title = HADES RV Programme with HARPS-N at TNG\|year = 2017\|last1 = Suárez Mascareño\|first1 = A.\|last2 = González Hernández\|first2 = J. I.\|last3 = Rebolo\|first3 = R.\|last4 = Velasco\|first4 = S.\|last5 = Toledo-Padrón\|first5 = B.\|last6 = Affer\|first6 = L.\|last7 = Perger\|first7 = M.\|last8 = Micela\|first8 = G.\|last9 = Ribas\|first9 = I.\|last10 = Maldonado\|first10 = J.\|last11 = Leto\|first11 = G.\|last12 = Zanmar Sanchez\|first12 = R.\|last13 = Scandariato\|first13 = G.\|last14 = Damasso\|first14 = M.\|last15 = Sozzetti\|first15 = A.\|last16 = Esposito\|first16 = M.\|last17 = Covino\|first17 = E.\|last18 = Maggio\|first18 = A.\|last19 = Lanza\|first19 = A. F.\|last20 = Desidera\|first20 = S.\|last21 = Rosich\|first21 = A.\|last22 = Bignamini\|first22 = A.\|last23 = Claudi\|first23 = R.\|last24 = Benatti\|first24 = S.\|last25 = Borsa\|first25 = F.\|last26 = Pedani\|first26 = M.\|last27 = Molinari\|first27 = E.\|last28 = Morales\|first28 = J. C.\|last29 = Herrero\|first29 = E.\|last30 = Lafarga\|first30 = M.\|journal = Astronomy & Astrophysics\|volume = 605\|pages = A92\| bibcode=2017A&A...605A..92S \|s2cid = 119003137}} has 1 known planet
rowspan='5' \| V1054 Ophiuchi (HD 152751)	Gliese 644 A	rowspan='5' \| 21.1961{{±\|0.0065}}	rowspan='5' \| Ophiuchus	rowspan='5' \| {{RA\|16\|55\|25.2}} {{DEC
08\|19\|21}}	style="background: {{star-color\|M}};" \| M3 V	9.74	rowspan='5' \| {{val\|153.8754\|0.0474}}	rowspan='5' \| components Ab and Ac are flare stars
\| Gliese 644 Ba	style="background: {{star-color\|M}};" \| M4 Ve	10.34
\| Gliese 644 Bb	style="background: {{star-color\|M}};" \| M4 Ve	10.84
\| Gliese 643	style="background: {{star-color\|M}};" \| M3.5 V	11.74
\| vB 8 (Gliese 644 C)	style="background: {{star-color\|M}};" \| M7.0 V	16.80
colspan = '2' \| GJ 1128 (L 100-115)	21.2121{{±\|0.0034}}	Carina	{{RA\|09\|42\|46.3}} {{DEC
68\|53\|06}}	style="background: {{star-color\|M}};" \| M4.0V	12.78	{{val\|153.7593\|0.0249}}
colspan = '2' style="background: lightgreen;" \| HD 219134 (HR 8832, Gliese 892){{Dollar sign}}	21.3364{{±\|0.0069}}	Cassiopeia	{{RA\|23\|13\|17.0}} {{DEC\|+57\|10\|06}}	style="background: {{star-color\|K}};" \| K3V	style="background: lightblue;" \| 5.574{{Hash-tag\|alt=visible to naked eye}}	{{val\|152.8640\|0.0494}}	[http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=HD+219134&type=PLANET_HOST HD 219134 PLANET HOST OVERVIEW PAGE] has 6 known planets
colspan = '2' style="background: #D8BD98" \|WISE 0825+2805§ \|21.37{{±\|0.28}} \| Cancer	{{RA\|08\|25\|07.4}} {{DEC\|+28\|05\|49}} \| style="background: {{star-color\|Y}};" \| Y0.5 \| \| {{Val\|152.6\|2.0}} \|{{Cite journal\|last1=Schneider\|first1=Adam C.\|last2=Cushing\|first2=Michael C.\|last3=Kirkpatrick\|first3=J. Davy\|last4=Gelino\|first4=Christopher R.\|last5=Mace\|first5=Gregory N.\|last6=Wright\|first6=Edward L.\|last7=Eisenhardt\|first7=Peter R.\|last8=Skrutskie\|first8=M. F.\|last9=Griffith\|first9=Roger L.\|last10=Marsh\|first10=Kenneth A.\|date=2015-05-01\|title=Hubble Space Telescope Spectroscopy of Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer\|bibcode=2015ApJ...804...92S\|journal=The Astrophysical Journal\|volume=804\|issue=2\|pages=92\|doi=10.1088/0004-637X/804/2/92\|arxiv=1502.05365\|issn=0004-637X\|hdl=2152/34928\|s2cid=6563025\|hdl-access=free}}
colspan = '2' style="background: #D8BD98" \| WISE 0410+1502§	21.56{{±\|0.29}}	style="background-color: pink" \| Taurus{{Asterisk}}	{{RA\|04\|10\|22.8}} {{DEC\|+15\|02\|47}}	style="background: {{star-color\|Y}};" \| Y0		{{val\|151.3\|2.0}}
colspan = '2' style="background: #D8BD98" \|WISE J0521+1025§ \|21.71{{±\|0.44}} \| Orion	{{RA\|05\|21\|26.4}} {{DEC\|+10\|25\|27}} \| style="background: {{star-color\|T}};" \| T7.5 \| \|{{Val\|150.2\|3.0}} \|
colspan = '2' \| GJ 3737 (LHS 337, L 471-42)	21.7324{{±\|0.0047}}	Centaurus	{{RA\|12\|38\|49.1}} {{DEC
38\|22\|53}}	style="background: {{star-color\|M}};" \| M4.5V:	12.74	{{val\|150.0781\|0.0322}}
colspan='2' \| Gliese 408 (Ross 104)	22.0081{{±\|0.0038}}	Leo	{{RA\|11\|00\|04.3}} {{DEC\|+22\|49\|59}}	style="background: {{star-color\|M}};" \| M3.0V	10.02	{{val\|148.1986\|0.0253}}
rowspan='2' \| Xi Boötis	style="background: lightgreen;" \| A{{Dollar sign}}	rowspan='2' \| 22.0109{{±\|0.0081}}	rowspan='2' \| Boötes	rowspan='2' \| {{RA\|14\|51\|23.4}} {{DEC\|+19\|06\|02}}	style="background: {{star-color\|G}};" \| G8Ve	style="background: lightblue;" \| 4.70{{Hash-tag\|alt=visible to naked eye}}	rowspan='2' \| {{val\|148.1793\|0.0546}}	rowspan='2' \| BY Draconis variable
style="background: lightgreen;" \| B{{Dollar sign}}	style="background: {{star-color\|K}};" \| K4Ve	6.97
colspan = '2' \| Gliese 299 (Ross 619)	22.079{{±\|0.014}}	Cancer	{{RA\|08\|11\|57.6}} {{DEC\|+08\|46\|22}}	style="background: {{star-color\|M}};" \| M4.5V	12.83	{{val\|147.7218\|0.0950}}
rowspan='3' \| GJ 3522 (G 41-14)	A	rowspan='3' \| 22.08{{±\|0.30}}	rowspan='3' \| Cancer	rowspan='3' \| {{RA\|08\|58\|56.3}} {{DEC\|+08\|28\|26}}	style="background: {{star-color\|M}};" \| M3.5V	rowspan='3' \| 10.92	rowspan='3' \| {{val\|147.66\|1.98}}	rowspan='3' \|
\| B	style="background: {{star-color\|M}};" \| M
\| C	style="background: {{star-color\|M}};" \| M
rowspan='2' \| Gliese 829 (Ross 775)	A	rowspan='2' \| 22.1129{{±\|0.0039}}	rowspan='2' \| Pegasus	rowspan='2' \| {{RA\|21\|29\|36.8}} {{DEC\|+17\|38\|36}}	style="background: {{star-color\|M}};" \| M3+M	rowspan='2'\| 10.30	rowspan='2' \| {{val\|147.4958\|0.0257}}	rowspan='2' \|
\| B	style="background: {{star-color\|M}};" \| M
rowspan='2' \|Scholz's Star \| A \| rowspan='2' \|22.17{{±\|0.18}} \| rowspan='2' \| Monoceros \| rowspan='2' \|{{RA\|07\|20\|03.3}} {{DEC\|−08\|46\|50}} \| style="background: {{star-color\|M}};" \| M9.5 \|18.3 \| rowspan='2' \|{{Val\|147.1\|1.2}}{{cite journal \|last1=Wizinowich \|first1=Peter \|last2=Wetherell \|first2=Ed \|last3=Ragland \|first3=Sam \|last4=Mawet \|first4=Dimitri \|last5=Lilley \|first5=Scott \|last6=Jovanovic \|first6=Nemanja \|last7=Delorme \|first7=Jacques-Robert \|last8=Chun \|first8=Mark \|last9=Cetre \|first9=Sylvain \|last10=Bond \|first10=Charlotte Z. \|last11=Shappee \|first11=B. J. \|last12=Payne \|first12=Anna V. \|last13=Do \|first13=Aaron \|last14=Tremblin \|first14=Pascal \|last15=Metchev \|first15=Stanimir A. \|last16=Forveille \|first16=Thierry \|last17=Chabrier \|first17=Gilles \|last18=Baraffe \|first18=Isabelle \|last19=Zhang \|first19=Zhoujian \|last20=Tucker \|first20=Michael A. \|last21=Mann \|first21=Andrew W. \|last22=Best \|first22=William M. J. \|last23=Liu \|first23=Michael C. \|last24=Dupuy \|first24=Trent J. \|title=WISE J072003.20-084651.2B Is A Massive T Dwarf \|journal=The Astronomical Journal \|date=19 August 2019 \|volume=158 \|issue=5 \|pages=174 \|doi=10.3847/1538-3881/ab3cd1 \|language=en\|arxiv=1908.06994 \|bibcode=2019AJ....158..174D \|s2cid=201103740 \|doi-access=free }} \| rowspan='2' \|passed through the Solar System's Oort Cloud 70,000 years ago
style="background: #D8BD98" \| B§ \| style="background: {{star-color\|T}};" \| T5.5 \|
colspan = '2' style="background: #D8BD98" \|WISE 1928+2356§	22.28{{±\|0.18}}	style="background-color: pink" \| Vulpecula{{Asterisk}}	{{RA\|19\|28\|41.5}} {{DEC\|+23\|56\|02}}	style="background: {{star-color\|T}};" \| T6		{{Val\|146.4067\|1.2001}}
colspan = '2' style="background: #D8BD98" \|WISE J0254+0223§ \|22.32{{±\|0.23}} \| Cetus	{{RA\|02\|54\|09.6}} {{DEC\|+02\|23\|59}} \| style="background: {{star-color\|T}};" \| T8 \| \|{{Val\|146.1\|1.5}}{{cite journal\|title=Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime\|display-authors=etal\|first1=J. Davy\|last1=Kirkpatrick\|first2=Emily C.\|last2=Martin\|first3=Richard L.\|last3=Smart\|first4=Alfred J.\|last4=Cayago\|first5=Charles A.\|last5=Beichman\|first6=Federico\|last6=Marocco\|date=February 2019\|journal=The Astrophysical Journal Supplement Series\|volume=240\|issue=2\|pages=69\|id=19\|doi=10.3847/1538-4365/aaf6af\|arxiv=1812.01208\|bibcode=2019ApJS..240...19K\|doi-access=free}} \|
rowspan='3' \| LTT 1445 (BD-17 588)	A	rowspan='3' \| 22.3867{{±\|0.0037}}	rowspan='3' \| Eridanus	rowspan='3' \| {{RA\|03\|01\|51.4}} {{DEC
16\|35\|36}}	style="background: {{star-color\|M}};" \| M3.0	11.22	rowspan='3' \| 145.6922{{±\|0.0244}}	rowspan='3' \| has 2-3 known planets orbiting star A{{cite journal\|last1=Almenara\|first1=Jose-Manuel\|last2=Berlind\|first2=Perry\|last3=Bouchy\|first3=Franois\|last4=Burke\|first4=Chris J.\|last5=Delfosse\|first5=Xavier\|last6=D'iaz\|first6=Rodrigo F.\|last7=Dressing\|first7=Courtney D.\|last8=Esquerdo\|first8=Gilbert A.\|last9=Figueira \|first9=Pedro \|display-authors=etal \|date=2019-06-24\|title=Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs \|volume=158 \|issue=152\|doi=10.3847/1538-3881/ab364d\|arxiv=1906.10147\|s2cid=195584444\|language=en \|journal=The Astronomical Journal \|doi-access=free }}{{Cite web\|url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GJ+3192&submit=submit+id\|title = Gj 3192}}
\| B	style="background: {{star-color\|M}};" \| M3.5	rowspan='2'\| 11.37
\| C	style="background: {{star-color\|M}};" \| M
colspan = '2' \| Gliese 880 (HD 216899)	22.3973{{±\|0.0039}}	Pegasus	{{RA\|22\|56\|34.8}} {{DEC\|+16\|33\|12}}	style="background: {{star-color\|M}};" \| M2.0V	8.64	{{val\|145.6234\|0.0254}}	has 1 candidate planet
colspan = '2' style="background: #D8BD98" \|CWISE J1055+5443§ \|22.5{{±\|2.6\|2.0}} \| Ursa Major	{{RA\|10\|55\|12.1}} {{DEC\|+54\|43\|28}} \| style="background: {{star-color\|Y}};" \| Y0 (pec) \| \|{{Val\|145.0\|14.7}} \|possibly a young low mass object (4−6 {{jupiter mass}})
colspan = '2' \| Gliese 402 (EE Leonis, Wolf 358)	22.7225{{±\|0.0045}}	Leo	{{RA\|10\|50\|52.0}} {{DEC\|+06\|48\|29.2}}	style="background: {{star-color\|M}};" \| M5.0V	11.68	{{val\|143.5391\|0.0286}}	BY Draconis variable; member of the Hercules-Lyra association
colspan = '2' \| Gliese 393 (BD+01 2447)	22.9534{{±\|0.0034}}	Sextans	{{RA\|10\|28\|55.6}} {{DEC\|+00\|50\|28}}	style="background: {{star-color\|M}};" \| M2.5V	9.65	{{val\|142.0951\|0.0212}}	Member of the AB Doradus moving group; has 1 known planet
colspan='2' \| Gliese 809 (HD 199305)	22.9600{{±\|0.0026}}	Cepheus	{{RA\|20\|53\|19.8}} {{DEC\|+62\|09\|16}}	style="background: {{star-color\|M}};" \| M2.0V	8.60	{{val\|142.0543\|0.0160}}
colspan = '2' \| LSPM J2146+3813 (UCAC4 642-113039)	22.9858{{±\|0.0034}}	Cygnus	{{RA\|21\|46\|22.1}} {{DEC\|+38\|13\|05}}	style="background: {{star-color\|M}};" \| M5V		{{val\|141.8946\|0.0212}}
colspan = '2' \| LHS 3003 (GJ 3877, LP 914-54)	23.003{{±\|0.010}}	Hydra	{{RA\|14\|56\|38.3}} {{DEC
28\|09\|47}}	style="background: {{star-color\|M}};" \| M7.0V	17.14	{{val\|141.7891\|0.0617}}
colspan = '2' style="background: #D8BD98" \| WISE 2056+1459§	23.16{{±\|0.33}}	style="background-color: pink" \| Delphinus{{Asterisk}}	{{RA\|20\|56\|28.9}} {{DEC\|+14\|59\|54}}	style="background: {{star-color\|Y}};" \| Y0		{{val\|140.8\|2.0}}
colspan = '2' \| GJ 1068 (L 230-188)	23.1816{{±\|0.0035}}	style="background-color: pink" \| Dorado{{Asterisk}}	{{RA\|04\|10\|28.1}} {{DEC
53\|36\|08}}	style="background: {{star-color\|M}};" \| M4.5	13.58	{{val\|140.6961\|0.0214}}
colspan = '2' style="background: #D8BD98" \| WISE J004945.61+215120.0§	23.23{{±\|0.35}}	Andromeda	{{RA\|00\|49\|45.6}} {{DEC\|+21\|51\|20}}	style="background: {{star-color\|T}};" \| T8.5		{{Val\|140.4\|2.1}}
colspan = '2' \| GJ 1286 (G 157-77)	23.4074{{±\|0.0074}}	Pisces	{{RA\|23\|35\|10.5}} {{DEC
02\|23\|21}}	style="background: {{star-color\|M}};" \| M5.5V	14.69	{{val\|139.3389\|0.0441}}
rowspan='3' \| Gliese 105 (268 G. Ceti, HD 16160)	style="background: lightgreen;" \| A{{Dollar sign}}	rowspan='3' \| 23.5599{{±\|0.0071}}	rowspan='3' \| Cetus	rowspan='3' \| {{RA\|02\|36\|04.9}} {{DEC\|+06\|53\|13}}	style="background: {{star-color\|K}};" \| K3V	style="background: lightblue;" \| 5.82{{Hash-tag\|alt=visible to naked eye}}	rowspan='3' \| {{val\|138.4371\|0.0420}}	rowspan='3' \| star B is a BY Draconis variable
\| B	style="background: {{star-color\|M}};" \| M4.5V	11.66
\| C	style="background: {{star-color\|M}};" \| M6V	16.9
colspan = '2' style="background: #D8BD98" \|2MASS J08354256-0819237§ \|23.581{{±\|0.037}} \| Hydra	{{RA\|08\|35\|42.6}} {{DEC
08\|19\|24}} \| style="background: {{star-color\|L}};" \| L5 \| \|{{Val\|138.3147\|0.2145}} \|
colspan = '2' \| GJ 4274 (L 788-34)	23.5955{{±\|0.0082}}	Aquarius	{{RA\|22\|23\|07.0}} {{DEC
17\|36\|26}}	style="background: {{star-color\|M}};" \| M4.5Ve	13.30	{{val\|138.2280\|0.0482}}
rowspan='3' \| Gliese 667 (142 G. Scorpii)	style="background: lightgreen;" \| A{{Dollar sign}}	rowspan='3'\| 23.6232{{±\|0.0048}}	rowspan='3'\| Scorpius	rowspan='3'\| {{RA\|17\|18\|57.2}} {{DEC\|−34\|59\|23}}	style="background: {{star-color\|K}};" \| K3V	7.07	rowspan='3'\| {{val\|138.0663\|0.0283}}	rowspan='3' \| star C has 2 known planets
style="background: lightgreen;" \| B{{Dollar sign}}	style="background: {{star-color\|K}};" \| K5V	8.02
\| C	style="background: {{star-color\|M}};" \| M1.5V	11.03
colspan = '2' style="background: #D8BD98" \| WISE 0607+2429§	23.624{{±\|0.089}}	Gemini	{{RA\|06\|07\|38.7}} {{DEC\|+24\|29\|54}}	style="background: {{star-color\|L}};" \| L8	14.22 ± 0.03 (J)	138.0616{{±\|0.5185}}	{{cite Gaia EDR3}}
colspan = '2' style="background: #D8BD98" \| WISE 0313+7807§	24.05{{±\|0.51}}	Cepheus	{{RA\|03\|13\|26.0}} {{DEC\|+78\|07\|44}}	style="background: {{star-color\|T}};" \| T8.5		{{Val\|135.6\|2.8}}
colspan = '2' style="background: #D8BD98" \| 2MASS 1507-1627§	24.169{{±\|0.047}}	Libra	{{RA\|15\|07\|47.7}} {{DEC\|−16\|27\|389}}	style="background: {{star-color\|L}};" \| L5.5	22.14	{{val\|134.9474\|0.2611}}
colspan = '2' style="background: lightgreen;" \| HD 4628 (96 G. Piscium, Gliese 33){{Dollar sign}}	24.250{{±\|0.010}}	Pisces	{{RA\|00\|48\|23.0}} {{DEC\|+05\|16\|50}}	style="background: {{star-color\|K}};" \| K2.5V	style="background: lightblue;" \| 5.75{{Hash-tag\|alt=visible to naked eye}}	{{val\|134.4948\|0.0578}}
colspan = '2' style="background: lightgreen;" \| Beta Hydri{{Dollar sign}}	24.327{{±\|0.020}}	style="background-color: pink" \| Hydrus{{Asterisk}}	{{RA\|00\|25\|45.1}} {{DEC\|–77\|15\|15}}	style="background: {{star-color\|G}};" \| G2IV	style="background: lightblue;" \| 2.79{{Hash-tag\|alt=visible to naked eye}}	{{val\|134.07\|0.11}}{{citation \| first1=F. \| last1=van Leeuwen \|date=November 2007 \| title=Validation of the new Hipparcos reduction \| journal=Astronomy and Astrophysics \| volume=474 \| issue=2 \| pages=653–664 \| bibcode=2007A&A...474..653V \| doi=10.1051/0004-6361:20078357 \|arxiv = 0708.1752 \| s2cid=18759600 }}
colspan = '2' style="background: #D8BD98" \|WISE J2000+3629§ \|24.45{{±\|0.41}} \| Cygnus	{{RA\|20\|00\|50.2}} {{DEC\|+36\|29\|50}} \| style="background: {{star-color\|T}};" \| T8 \| \|{{Val\|133.4\|2.2}} \|
rowspan='2' \| GJ 3991 (G 203-47)	A	rowspan='2' \| 24.784{{±\|0.081}}	rowspan='2' \| Hercules	rowspan='2' \| {{RA\|17\|09\|32.0}} {{DEC\|+43\|40\|49}}	style="background: {{star-color\|M}};" \| M3.5V	13.671	rowspan='2' \| {{val\|131.5996\|0.4285}}	rowspan='2' \|
style="background: #F5F5DC" \| B	style="background: #F5F5DC" \| D?
\| {{nowrap\|Alpha Piscis Austrini}}	style="background: lightgreen;" \| B (TW PsA){{Dollar sign}}	24.7929{{±\|0.0052}}	{{nowrap\|Piscis Austrinus}}	{{RA\|22\|56\|24.17}} {{DEC\|−31\|33\|56}}	style="background: {{star-color\|K}};" \| K5Vp	style="background: lightblue;" \| 6.48{{Hash-tag\|alt=visible to naked eye}}	{{val\|131.5525\|0.0275}}{{cite Gaia EDR3}}	component B of triple system
colspan = '2' style="background: lightgreen;" \| 107 Piscium{{Dollar sign}}	24.805{{±\|0.029}}	Pisces	{{RA\|01\|42\|29.8}} {{DEC\|+20\|16\|07}}	style="background: {{star-color\|K}};" \| K1V	style="background: lightblue;" \| 5.24{{Hash-tag\|alt=visible to naked eye}}	{{val\|131.4903\|0.1515}}{{cite Gaia DR2}}
colspan = '2' \| G 141-36	24.8445{{±\|0.0075}}	Aquila	{{RA\|18\|48\|17.5}} {{DEC\|+07\|41\|21}}	style="background: {{star-color\|M}};" \| M6V		{{val\|131.2790\|0.0398}}
colspan = '2' \| Gliese 514 (BD+11 2576)	24.8782{{±\|0.0051}}	Virgo	{{RA\|13\|29\|59.8}} {{DEC\|+10\|22\|38}}	style="background: {{star-color\|M}};" \| M1.0V	9.02	{{val\|131.1013\|0.0270}}	has 1 known planet
colspan = '2' style="background: #D8BD98" \|WISE 1738+2732§ \|24.92{{±\|0.41}} \| Hercules	{{RA\|17\|38\|35.5}} {{DEC\|+27\|32\|59}} \| style="background: {{star-color\|Y}};" \| Y0 \| \|{{Val\|130.9\|2.1}} \|
colspan = '2' \| GJ 4053 (G 258-33)	24.9254{{±\|0.0041}}	Draco	{{RA\|18\|18\|57.2}} {{DEC\|+66\|11\|33}}	style="background: {{star-color\|M}};" \| M4.5V	13.46	{{val\|130.8531\|0.0217}}
colspan = '2' style="background: #D8BD98" \| WISE J2354+0240§ \|24.97{{±\|0.65}} \| Pisces	{{RA\|23\|54\|02.8}} {{DEC\|+02\|40\|14}} \| style="background: {{star-color\|Y}};" \| Y1 \| \|{{Val\|130.6\|3.3}} \|
scope="col" \| System ! Star or (sub-) brown dwarf ! scope="col" \| Distance (ly) ! Constellation ! Coordinates: RA, Dec (Ep J2000, Eq J2000) ! scope="col" \| Stellar class ! scope="col" \| Apparent magnitude (V) ! scope="col" \| Parallax (mas) ! scope="col" \| Notes and additional references

References

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}}

Category:Lists of stars

Category:Star systems

Category:Lists by distance

scope="col" \| System←→←→ ! Star or (sub-) brown dwarf ! scope="col" \| Distance (ly) ! Constellation ! Coordinates: RA, Dec (Ep J2000, Eq J2000) ! scope="col" \| Stellar class ! scope="col" \| Apparent magnitude (V) ! scope="col" \| Parallax (mas) ! scope="col" \| Notes and additional references
class="wikitable sortable" style="font-size:90%; line-height:1.5em; position:relative"
colspan = '2' \| Gliese 784 (HD 191849)	20.1062{{±\|0.0028}}	Telescopium	{{RA\|20\|13\|53.4}} {{DEC
45\|09\|50}}	style="background: {{star-color\|M}};" \| M0V	7.97	162.2171{{±\|0.0225}}	has 1 candidate planet {{cite arXiv\|last1=Barnes\|first1=J. R.\|last2=Kiraga\|first2=M.\|last3=Diaz\|first3=M.\|last4=Berdiñas\|first4=Z.\|last5=Jenkins\|first5=J. S.\|last6=Keiser\|first6=S.\|last7=Thompson\|first7=I.\|last8=Crane\|first8=J. D.\|last9=Shectman\|first9=S. A.\|display-authors=1\|date=2019-06-11\|title=Frequency of planets orbiting M dwarfs in the Solar neighbourhood\|class=astro-ph.EP\|eprint=1906.04644\|language=en}}
colspan = '2' style="background: #D8BD98" \| WISE J2209+2711§	20.17{{±\|0.25}}	style="background-color: pink" \| Pegasus{{Asterisk}}	{{RA\|22\|09\|05.7}} {{DEC\|+27\|11\|44}}	style="background: {{star-color\|Y}};" \| Y0		{{val\|161.7\|2.0}}
colspan = '2' style="background: #F5F5DC" \| G 240-72 (LHS 455, GJ 1221, EGGR 372){{Double-dagger\|alt=white dwarf}} \| 20.2588{{±\|0.0015}} \| Draco \| {{RA\|17\|48\|08.2}} {{DEC\|+70\|52\|35}} \| style="background: #F5F5DC" \| DXP9 \| 14.22 \| 160.9952{{±\|0.0119}} \|
colspan = '2' \| Gliese 555 (Wolf 1481, HN Librae, {{nowrap\|BD-11 3759}})	20.3947{{±\|0.0070}}	Libra	{{RA\|14\|34\|16.8}} {{DEC
12\|31\|10}}	style="background: {{star-color\|M}};" \| M4.0V	10.3–10.33	159.9225{{±\|0.0546}}	BY Draconis variable; has 1 known planet
rowspan='2' \| EQ Pegasi (Gliese 896, BD+19 5116)	A	rowspan='2' \| 20.4277{{±\|0.0044}}	rowspan='2' \| Pegasus	rowspan='2' \| {{RA\|23\|31\|52.2}} {{DEC\|+19\|56\|14}}	style="background: {{star-color\|M}};" \| M3.5V	10.35	rowspan='2' \| 159.6634{{±\|0.0341}}	rowspan='2' \| both components are flare stars; has 1 known planet orbiting star A of the binary system {{cite journal \|arxiv=2208.14553 \|last1=Curiel \|first1=Salvador \|last2=Ortiz-León \|first2=Gisela N. \|last3=Mioduszewski \|first3=Amy J. \|last4=Sanchez-Bermudez \|first4=Joel \|date=31 May 2022\|publication-date=1 September 2022 \|title=3D Orbital Architecture of a Dwarf Binary System and Its Planetary Companion \|journal=The Astronomical Journal \|volume=164:93 \|issue=3 \|pages=23pp \|doi=10.3847/1538-3881/ac7c66\|doi-access=free \|bibcode=2022AJ....164...93C}}
\| B	style="background: {{star-color\|M}};" \| M4.5V	12.4
colspan = '2' \| Gliese 581 (Wolf 562, HO Librae)	20.5494{{±\|0.0039}}	Libra	{{RA\|15\|19\|26.8}} {{DEC\|−07\|43\|20}}	style="background: {{star-color\|M}};" \| M3.0V	10.56–10.58	158.7183{{±\|0.0301}}	BY Draconis variable; has 3 known planets
colspan = '2' style="background: #D8BD98" \|WISE 1405+5534§ \| 20.62{{±\|0.34}} \| Ursa Major	{{RA\|14\|05\|18.3}} {{DEC\|+55\|34\|21}} \| style="background: {{star-color\|Y}};" \| Y0.5 \| \| {{Val\|158.2\|2.6}} \|{{Cite journal\|last1=Kirkpatrick\|first1=J. Davy\|last2=Gelino\|first2=Christopher R.\|last3=Faherty\|first3=Jacqueline K.\|author3-link=Jackie Faherty\|last4=Meisner\|first4=Aaron M.\|last5=Caselden\|first5=Dan\|last6=Schneider\|first6=Adam C.\|last7=Marocco\|first7=Federico\|last8=Cayago\|first8=Alfred J.\|last9=Smart\|first9=R. L.\|last10=Eisenhardt\|first10=Peter R.\|last11=Kuchner\|first11=Marc J.\|title=The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs\|journal=The Astrophysical Journal Supplement Series\|year=2021\|volume=253\|issue=1\|page=7\|doi=10.3847/1538-4365/abd107\|arxiv=2011.11616\|bibcode=2021ApJS..253....7K\|s2cid=227126954 \|doi-access=free }}
rowspan='2' \| ADS 7251 (HD 79210, Gliese 338, MCC 541)	A	rowspan='2'\| 20.6575{{±\|0.0026}}	rowspan='2'\| Ursa Major	rowspan='2'\| {{RA\|09\|14\|22.8}} {{DEC\|+52\|41\|12}}	style="background: {{star-color\|M}};" \| M0V	7.64	rowspan='2'\| 157.8879{{±\|0.0197}}	rowspan='2' \| has 1 known planet orbiting star B of the binary system {{Cite journal\|last1=González-Álvarez\|first1=E.\|last2=Osorio\|first2=M. R. Zapatero\|last3=Caballero\|first3=J. A.\|last4=Sanz-Forcada\|first4=J.\|last5=Béjar\|first5=V. J. S.\|last6=González-Cuesta\|first6=L.\|last7=Dreizler\|first7=S.\|last8=Bauer\|first8=F. F.\|last9=Rodríguez\|first9=E.\|last10=Tal-Or\|first10=L.\|last11=Zechmeister\|first11=M.\|date=May 2020\|title=The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B)\|arxiv=2003.13052\|journal=Astronomy & Astrophysics\|volume=637\|pages=A93\|doi=10.1051/0004-6361/201937050\|bibcode=2020A&A...637A..93G\|issn=0004-6361\|doi-access=free}}
\| B	style="background: {{star-color\|K}};" \| K7V	7.70
colspan = '2' \| LHS 2090 ({{nowrap\|LP 368-128}})	20.7388{{±\|0.0071}}	Cancer	{{RA\|09\|00\|23.6}} {{DEC\|+21\|50\|05}}	style="background: {{star-color\|M}};" \| M6.5V	16.10	157.2686{{±\|0.0535}}
rowspan='2' \| Furuhjelm 46 (HD 155876, Gliese 661)	A	rowspan='2' \| 20.82{{±\|0.18}}	rowspan='2' \| Hercules	rowspan='2' \| {{RA\|17\|12\|07.9}} {{DEC\|+45\|39\|57}}	style="background: {{star-color\|M}};" \| M3 V	9.93	rowspan='2' \| {{val\|156.66\|1.37}}	rowspan='2' \|
\| B	style="background: {{star-color\|M}};" \| M3.5 V	10.35
colspan = '2' style="background: #D8BD98" \| 2MASS 1503+2525§	20.94{{±\|0.10}}	Boötes	{{RA\|15\|03\|19.6}} {{DEC\|+25\|25\|20}}	style="background: {{star-color\|T}};" \| T5.5		155.7758{{±\|0.7557}}
colspan = '2' style="background: #D8BD98" \| LP 944-20§	20.9615{{±\|0.0070}}	style="background-color: pink" \| Fornax{{Asterisk}}	{{RA\|03\|39\|35.2}} {{DEC\|–35\|25\|44}}	style="background: {{star-color\|M}};" \| M9V	18.69	155.5982{{±\|0.0522}}
colspan = '2' style="background: #F5F5DC"; \| LP 658-2 (EGGR 45){{Double-dagger\|alt=white dwarf}}	21.0102{{±\|0.0024}}	Orion	{{RA\|05\|55\|09.5}} {{DEC\|−04\|10\|07}}	style="background: #F5F5DC" \| DZ11	14.45	{{val\|155.2373\|0.0175}}
colspan = '2' \| GL Virginis (G 12-30)	21.0832{{±\|0.0061}}	Virgo	{{RA\|12\|18\|59.4}} {{DEC\|+11\|07\|34}}	style="background: {{star-color\|M}};" \| M5Ve	13.79	{{val\|154.6999\|0.0445}}	flare star
colspan = '2' \| Gliese 625 (AC 54 1646-56, G 202-48)	21.1309{{±\|0.0022}}	Draco	{{RA\|16\|25\|24.6}} {{DEC\|+54\|18\|15}}	style="background: {{star-color\|M}};" \| M2.0V	10.17	{{val\|154.3503\|0.0161}}	{{Cite journal\|arxiv = 1705.06537\|doi = 10.1051/0004-6361/201730957\|title = HADES RV Programme with HARPS-N at TNG\|year = 2017\|last1 = Suárez Mascareño\|first1 = A.\|last2 = González Hernández\|first2 = J. I.\|last3 = Rebolo\|first3 = R.\|last4 = Velasco\|first4 = S.\|last5 = Toledo-Padrón\|first5 = B.\|last6 = Affer\|first6 = L.\|last7 = Perger\|first7 = M.\|last8 = Micela\|first8 = G.\|last9 = Ribas\|first9 = I.\|last10 = Maldonado\|first10 = J.\|last11 = Leto\|first11 = G.\|last12 = Zanmar Sanchez\|first12 = R.\|last13 = Scandariato\|first13 = G.\|last14 = Damasso\|first14 = M.\|last15 = Sozzetti\|first15 = A.\|last16 = Esposito\|first16 = M.\|last17 = Covino\|first17 = E.\|last18 = Maggio\|first18 = A.\|last19 = Lanza\|first19 = A. F.\|last20 = Desidera\|first20 = S.\|last21 = Rosich\|first21 = A.\|last22 = Bignamini\|first22 = A.\|last23 = Claudi\|first23 = R.\|last24 = Benatti\|first24 = S.\|last25 = Borsa\|first25 = F.\|last26 = Pedani\|first26 = M.\|last27 = Molinari\|first27 = E.\|last28 = Morales\|first28 = J. C.\|last29 = Herrero\|first29 = E.\|last30 = Lafarga\|first30 = M.\|journal = Astronomy & Astrophysics\|volume = 605\|pages = A92\| bibcode=2017A&A...605A..92S \|s2cid = 119003137}} has 1 known planet
rowspan='5' \| V1054 Ophiuchi (HD 152751)	Gliese 644 A	rowspan='5' \| 21.1961{{±\|0.0065}}	rowspan='5' \| Ophiuchus	rowspan='5' \| {{RA\|16\|55\|25.2}} {{DEC
08\|19\|21}}	style="background: {{star-color\|M}};" \| M3 V	9.74	rowspan='5' \| {{val\|153.8754\|0.0474}}	rowspan='5' \| components Ab and Ac are flare stars
\| Gliese 644 Ba	style="background: {{star-color\|M}};" \| M4 Ve	10.34
\| Gliese 644 Bb	style="background: {{star-color\|M}};" \| M4 Ve	10.84
\| Gliese 643	style="background: {{star-color\|M}};" \| M3.5 V	11.74
\| vB 8 (Gliese 644 C)	style="background: {{star-color\|M}};" \| M7.0 V	16.80
colspan = '2' \| GJ 1128 (L 100-115)	21.2121{{±\|0.0034}}	Carina	{{RA\|09\|42\|46.3}} {{DEC
68\|53\|06}}	style="background: {{star-color\|M}};" \| M4.0V	12.78	{{val\|153.7593\|0.0249}}
colspan = '2' style="background: lightgreen;" \| HD 219134 (HR 8832, Gliese 892){{Dollar sign}}	21.3364{{±\|0.0069}}	Cassiopeia	{{RA\|23\|13\|17.0}} {{DEC\|+57\|10\|06}}	style="background: {{star-color\|K}};" \| K3V	style="background: lightblue;" \| 5.574{{Hash-tag\|alt=visible to naked eye}}	{{val\|152.8640\|0.0494}}	[http://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=HD+219134&type=PLANET_HOST HD 219134 PLANET HOST OVERVIEW PAGE] has 6 known planets
colspan = '2' style="background: #D8BD98" \|WISE 0825+2805§ \|21.37{{±\|0.28}} \| Cancer	{{RA\|08\|25\|07.4}} {{DEC\|+28\|05\|49}} \| style="background: {{star-color\|Y}};" \| Y0.5 \| \| {{Val\|152.6\|2.0}} \|{{Cite journal\|last1=Schneider\|first1=Adam C.\|last2=Cushing\|first2=Michael C.\|last3=Kirkpatrick\|first3=J. Davy\|last4=Gelino\|first4=Christopher R.\|last5=Mace\|first5=Gregory N.\|last6=Wright\|first6=Edward L.\|last7=Eisenhardt\|first7=Peter R.\|last8=Skrutskie\|first8=M. F.\|last9=Griffith\|first9=Roger L.\|last10=Marsh\|first10=Kenneth A.\|date=2015-05-01\|title=Hubble Space Telescope Spectroscopy of Brown Dwarfs Discovered with the Wide-field Infrared Survey Explorer\|bibcode=2015ApJ...804...92S\|journal=The Astrophysical Journal\|volume=804\|issue=2\|pages=92\|doi=10.1088/0004-637X/804/2/92\|arxiv=1502.05365\|issn=0004-637X\|hdl=2152/34928\|s2cid=6563025\|hdl-access=free}}
colspan = '2' style="background: #D8BD98" \| WISE 0410+1502§	21.56{{±\|0.29}}	style="background-color: pink" \| Taurus{{Asterisk}}	{{RA\|04\|10\|22.8}} {{DEC\|+15\|02\|47}}	style="background: {{star-color\|Y}};" \| Y0		{{val\|151.3\|2.0}}
colspan = '2' style="background: #D8BD98" \|WISE J0521+1025§ \|21.71{{±\|0.44}} \| Orion	{{RA\|05\|21\|26.4}} {{DEC\|+10\|25\|27}} \| style="background: {{star-color\|T}};" \| T7.5 \| \|{{Val\|150.2\|3.0}} \|
colspan = '2' \| GJ 3737 (LHS 337, L 471-42)	21.7324{{±\|0.0047}}	Centaurus	{{RA\|12\|38\|49.1}} {{DEC
38\|22\|53}}	style="background: {{star-color\|M}};" \| M4.5V:	12.74	{{val\|150.0781\|0.0322}}
colspan='2' \| Gliese 408 (Ross 104)	22.0081{{±\|0.0038}}	Leo	{{RA\|11\|00\|04.3}} {{DEC\|+22\|49\|59}}	style="background: {{star-color\|M}};" \| M3.0V	10.02	{{val\|148.1986\|0.0253}}
rowspan='2' \| Xi Boötis	style="background: lightgreen;" \| A{{Dollar sign}}	rowspan='2' \| 22.0109{{±\|0.0081}}	rowspan='2' \| Boötes	rowspan='2' \| {{RA\|14\|51\|23.4}} {{DEC\|+19\|06\|02}}	style="background: {{star-color\|G}};" \| G8Ve	style="background: lightblue;" \| 4.70{{Hash-tag\|alt=visible to naked eye}}	rowspan='2' \| {{val\|148.1793\|0.0546}}	rowspan='2' \| BY Draconis variable
style="background: lightgreen;" \| B{{Dollar sign}}	style="background: {{star-color\|K}};" \| K4Ve	6.97
colspan = '2' \| Gliese 299 (Ross 619)	22.079{{±\|0.014}}	Cancer	{{RA\|08\|11\|57.6}} {{DEC\|+08\|46\|22}}	style="background: {{star-color\|M}};" \| M4.5V	12.83	{{val\|147.7218\|0.0950}}
rowspan='3' \| GJ 3522 (G 41-14)	A	rowspan='3' \| 22.08{{±\|0.30}}	rowspan='3' \| Cancer	rowspan='3' \| {{RA\|08\|58\|56.3}} {{DEC\|+08\|28\|26}}	style="background: {{star-color\|M}};" \| M3.5V	rowspan='3' \| 10.92	rowspan='3' \| {{val\|147.66\|1.98}}	rowspan='3' \|
\| B	style="background: {{star-color\|M}};" \| M
\| C	style="background: {{star-color\|M}};" \| M
rowspan='2' \| Gliese 829 (Ross 775)	A	rowspan='2' \| 22.1129{{±\|0.0039}}	rowspan='2' \| Pegasus	rowspan='2' \| {{RA\|21\|29\|36.8}} {{DEC\|+17\|38\|36}}	style="background: {{star-color\|M}};" \| M3+M	rowspan='2'\| 10.30	rowspan='2' \| {{val\|147.4958\|0.0257}}	rowspan='2' \|
\| B	style="background: {{star-color\|M}};" \| M
rowspan='2' \|Scholz's Star \| A \| rowspan='2' \|22.17{{±\|0.18}} \| rowspan='2' \| Monoceros \| rowspan='2' \|{{RA\|07\|20\|03.3}} {{DEC\|−08\|46\|50}} \| style="background: {{star-color\|M}};" \| M9.5 \|18.3 \| rowspan='2' \|{{Val\|147.1\|1.2}}{{cite journal \|last1=Wizinowich \|first1=Peter \|last2=Wetherell \|first2=Ed \|last3=Ragland \|first3=Sam \|last4=Mawet \|first4=Dimitri \|last5=Lilley \|first5=Scott \|last6=Jovanovic \|first6=Nemanja \|last7=Delorme \|first7=Jacques-Robert \|last8=Chun \|first8=Mark \|last9=Cetre \|first9=Sylvain \|last10=Bond \|first10=Charlotte Z. \|last11=Shappee \|first11=B. J. \|last12=Payne \|first12=Anna V. \|last13=Do \|first13=Aaron \|last14=Tremblin \|first14=Pascal \|last15=Metchev \|first15=Stanimir A. \|last16=Forveille \|first16=Thierry \|last17=Chabrier \|first17=Gilles \|last18=Baraffe \|first18=Isabelle \|last19=Zhang \|first19=Zhoujian \|last20=Tucker \|first20=Michael A. \|last21=Mann \|first21=Andrew W. \|last22=Best \|first22=William M. J. \|last23=Liu \|first23=Michael C. \|last24=Dupuy \|first24=Trent J. \|title=WISE J072003.20-084651.2B Is A Massive T Dwarf \|journal=The Astronomical Journal \|date=19 August 2019 \|volume=158 \|issue=5 \|pages=174 \|doi=10.3847/1538-3881/ab3cd1 \|language=en\|arxiv=1908.06994 \|bibcode=2019AJ....158..174D \|s2cid=201103740 \|doi-access=free }} \| rowspan='2' \|passed through the Solar System's Oort Cloud 70,000 years ago
style="background: #D8BD98" \| B§ \| style="background: {{star-color\|T}};" \| T5.5 \|
colspan = '2' style="background: #D8BD98" \|WISE 1928+2356§	22.28{{±\|0.18}}	style="background-color: pink" \| Vulpecula{{Asterisk}}	{{RA\|19\|28\|41.5}} {{DEC\|+23\|56\|02}}	style="background: {{star-color\|T}};" \| T6		{{Val\|146.4067\|1.2001}}
colspan = '2' style="background: #D8BD98" \|WISE J0254+0223§ \|22.32{{±\|0.23}} \| Cetus	{{RA\|02\|54\|09.6}} {{DEC\|+02\|23\|59}} \| style="background: {{star-color\|T}};" \| T8 \| \|{{Val\|146.1\|1.5}}{{cite journal\|title=Preliminary Trigonometric Parallaxes of 184 Late-T and Y Dwarfs and an Analysis of the Field Substellar Mass Function into the "Planetary" Mass Regime\|display-authors=etal\|first1=J. Davy\|last1=Kirkpatrick\|first2=Emily C.\|last2=Martin\|first3=Richard L.\|last3=Smart\|first4=Alfred J.\|last4=Cayago\|first5=Charles A.\|last5=Beichman\|first6=Federico\|last6=Marocco\|date=February 2019\|journal=The Astrophysical Journal Supplement Series\|volume=240\|issue=2\|pages=69\|id=19\|doi=10.3847/1538-4365/aaf6af\|arxiv=1812.01208\|bibcode=2019ApJS..240...19K\|doi-access=free}} \|
rowspan='3' \| LTT 1445 (BD-17 588)	A	rowspan='3' \| 22.3867{{±\|0.0037}}	rowspan='3' \| Eridanus	rowspan='3' \| {{RA\|03\|01\|51.4}} {{DEC
16\|35\|36}}	style="background: {{star-color\|M}};" \| M3.0	11.22	rowspan='3' \| 145.6922{{±\|0.0244}}	rowspan='3' \| has 2-3 known planets orbiting star A{{cite journal\|last1=Almenara\|first1=Jose-Manuel\|last2=Berlind\|first2=Perry\|last3=Bouchy\|first3=Franois\|last4=Burke\|first4=Chris J.\|last5=Delfosse\|first5=Xavier\|last6=D'iaz\|first6=Rodrigo F.\|last7=Dressing\|first7=Courtney D.\|last8=Esquerdo\|first8=Gilbert A.\|last9=Figueira \|first9=Pedro \|display-authors=etal \|date=2019-06-24\|title=Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs \|volume=158 \|issue=152\|doi=10.3847/1538-3881/ab364d\|arxiv=1906.10147\|s2cid=195584444\|language=en \|journal=The Astronomical Journal \|doi-access=free }}{{Cite web\|url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GJ+3192&submit=submit+id\|title = Gj 3192}}
\| B	style="background: {{star-color\|M}};" \| M3.5	rowspan='2'\| 11.37
\| C	style="background: {{star-color\|M}};" \| M
colspan = '2' \| Gliese 880 (HD 216899)	22.3973{{±\|0.0039}}	Pegasus	{{RA\|22\|56\|34.8}} {{DEC\|+16\|33\|12}}	style="background: {{star-color\|M}};" \| M2.0V	8.64	{{val\|145.6234\|0.0254}}	has 1 candidate planet
colspan = '2' style="background: #D8BD98" \|CWISE J1055+5443§ \|22.5{{±\|2.6\|2.0}} \| Ursa Major	{{RA\|10\|55\|12.1}} {{DEC\|+54\|43\|28}} \| style="background: {{star-color\|Y}};" \| Y0 (pec) \| \|{{Val\|145.0\|14.7}} \|possibly a young low mass object (4−6 {{jupiter mass}})
colspan = '2' \| Gliese 402 (EE Leonis, Wolf 358)	22.7225{{±\|0.0045}}	Leo	{{RA\|10\|50\|52.0}} {{DEC\|+06\|48\|29.2}}	style="background: {{star-color\|M}};" \| M5.0V	11.68	{{val\|143.5391\|0.0286}}	BY Draconis variable; member of the Hercules-Lyra association
colspan = '2' \| Gliese 393 (BD+01 2447)	22.9534{{±\|0.0034}}	Sextans	{{RA\|10\|28\|55.6}} {{DEC\|+00\|50\|28}}	style="background: {{star-color\|M}};" \| M2.5V	9.65	{{val\|142.0951\|0.0212}}	Member of the AB Doradus moving group; has 1 known planet
colspan='2' \| Gliese 809 (HD 199305)	22.9600{{±\|0.0026}}	Cepheus	{{RA\|20\|53\|19.8}} {{DEC\|+62\|09\|16}}	style="background: {{star-color\|M}};" \| M2.0V	8.60	{{val\|142.0543\|0.0160}}
colspan = '2' \| LSPM J2146+3813 (UCAC4 642-113039)	22.9858{{±\|0.0034}}	Cygnus	{{RA\|21\|46\|22.1}} {{DEC\|+38\|13\|05}}	style="background: {{star-color\|M}};" \| M5V		{{val\|141.8946\|0.0212}}
colspan = '2' \| LHS 3003 (GJ 3877, LP 914-54)	23.003{{±\|0.010}}	Hydra	{{RA\|14\|56\|38.3}} {{DEC
28\|09\|47}}	style="background: {{star-color\|M}};" \| M7.0V	17.14	{{val\|141.7891\|0.0617}}
colspan = '2' style="background: #D8BD98" \| WISE 2056+1459§	23.16{{±\|0.33}}	style="background-color: pink" \| Delphinus{{Asterisk}}	{{RA\|20\|56\|28.9}} {{DEC\|+14\|59\|54}}	style="background: {{star-color\|Y}};" \| Y0		{{val\|140.8\|2.0}}
colspan = '2' \| GJ 1068 (L 230-188)	23.1816{{±\|0.0035}}	style="background-color: pink" \| Dorado{{Asterisk}}	{{RA\|04\|10\|28.1}} {{DEC
53\|36\|08}}	style="background: {{star-color\|M}};" \| M4.5	13.58	{{val\|140.6961\|0.0214}}
colspan = '2' style="background: #D8BD98" \| WISE J004945.61+215120.0§	23.23{{±\|0.35}}	Andromeda	{{RA\|00\|49\|45.6}} {{DEC\|+21\|51\|20}}	style="background: {{star-color\|T}};" \| T8.5		{{Val\|140.4\|2.1}}
colspan = '2' \| GJ 1286 (G 157-77)	23.4074{{±\|0.0074}}	Pisces	{{RA\|23\|35\|10.5}} {{DEC
02\|23\|21}}	style="background: {{star-color\|M}};" \| M5.5V	14.69	{{val\|139.3389\|0.0441}}
rowspan='3' \| Gliese 105 (268 G. Ceti, HD 16160)	style="background: lightgreen;" \| A{{Dollar sign}}	rowspan='3' \| 23.5599{{±\|0.0071}}	rowspan='3' \| Cetus	rowspan='3' \| {{RA\|02\|36\|04.9}} {{DEC\|+06\|53\|13}}	style="background: {{star-color\|K}};" \| K3V	style="background: lightblue;" \| 5.82{{Hash-tag\|alt=visible to naked eye}}	rowspan='3' \| {{val\|138.4371\|0.0420}}	rowspan='3' \| star B is a BY Draconis variable
\| B	style="background: {{star-color\|M}};" \| M4.5V	11.66
\| C	style="background: {{star-color\|M}};" \| M6V	16.9
colspan = '2' style="background: #D8BD98" \|2MASS J08354256-0819237§ \|23.581{{±\|0.037}} \| Hydra	{{RA\|08\|35\|42.6}} {{DEC
08\|19\|24}} \| style="background: {{star-color\|L}};" \| L5 \| \|{{Val\|138.3147\|0.2145}} \|
colspan = '2' \| GJ 4274 (L 788-34)	23.5955{{±\|0.0082}}	Aquarius	{{RA\|22\|23\|07.0}} {{DEC
17\|36\|26}}	style="background: {{star-color\|M}};" \| M4.5Ve	13.30	{{val\|138.2280\|0.0482}}
rowspan='3' \| Gliese 667 (142 G. Scorpii)	style="background: lightgreen;" \| A{{Dollar sign}}	rowspan='3'\| 23.6232{{±\|0.0048}}	rowspan='3'\| Scorpius	rowspan='3'\| {{RA\|17\|18\|57.2}} {{DEC\|−34\|59\|23}}	style="background: {{star-color\|K}};" \| K3V	7.07	rowspan='3'\| {{val\|138.0663\|0.0283}}	rowspan='3' \| star C has 2 known planets
style="background: lightgreen;" \| B{{Dollar sign}}	style="background: {{star-color\|K}};" \| K5V	8.02
\| C	style="background: {{star-color\|M}};" \| M1.5V	11.03
colspan = '2' style="background: #D8BD98" \| WISE 0607+2429§	23.624{{±\|0.089}}	Gemini	{{RA\|06\|07\|38.7}} {{DEC\|+24\|29\|54}}	style="background: {{star-color\|L}};" \| L8	14.22 ± 0.03 (J)	138.0616{{±\|0.5185}}	{{cite Gaia EDR3}}
colspan = '2' style="background: #D8BD98" \| WISE 0313+7807§	24.05{{±\|0.51}}	Cepheus	{{RA\|03\|13\|26.0}} {{DEC\|+78\|07\|44}}	style="background: {{star-color\|T}};" \| T8.5		{{Val\|135.6\|2.8}}
colspan = '2' style="background: #D8BD98" \| 2MASS 1507-1627§	24.169{{±\|0.047}}	Libra	{{RA\|15\|07\|47.7}} {{DEC\|−16\|27\|389}}	style="background: {{star-color\|L}};" \| L5.5	22.14	{{val\|134.9474\|0.2611}}
colspan = '2' style="background: lightgreen;" \| HD 4628 (96 G. Piscium, Gliese 33){{Dollar sign}}	24.250{{±\|0.010}}	Pisces	{{RA\|00\|48\|23.0}} {{DEC\|+05\|16\|50}}	style="background: {{star-color\|K}};" \| K2.5V	style="background: lightblue;" \| 5.75{{Hash-tag\|alt=visible to naked eye}}	{{val\|134.4948\|0.0578}}
colspan = '2' style="background: lightgreen;" \| Beta Hydri{{Dollar sign}}	24.327{{±\|0.020}}	style="background-color: pink" \| Hydrus{{Asterisk}}	{{RA\|00\|25\|45.1}} {{DEC\|–77\|15\|15}}	style="background: {{star-color\|G}};" \| G2IV	style="background: lightblue;" \| 2.79{{Hash-tag\|alt=visible to naked eye}}	{{val\|134.07\|0.11}}{{citation \| first1=F. \| last1=van Leeuwen \|date=November 2007 \| title=Validation of the new Hipparcos reduction \| journal=Astronomy and Astrophysics \| volume=474 \| issue=2 \| pages=653–664 \| bibcode=2007A&A...474..653V \| doi=10.1051/0004-6361:20078357 \|arxiv = 0708.1752 \| s2cid=18759600 }}
colspan = '2' style="background: #D8BD98" \|WISE J2000+3629§ \|24.45{{±\|0.41}} \| Cygnus	{{RA\|20\|00\|50.2}} {{DEC\|+36\|29\|50}} \| style="background: {{star-color\|T}};" \| T8 \| \|{{Val\|133.4\|2.2}} \|
rowspan='2' \| GJ 3991 (G 203-47)	A	rowspan='2' \| 24.784{{±\|0.081}}	rowspan='2' \| Hercules	rowspan='2' \| {{RA\|17\|09\|32.0}} {{DEC\|+43\|40\|49}}	style="background: {{star-color\|M}};" \| M3.5V	13.671	rowspan='2' \| {{val\|131.5996\|0.4285}}	rowspan='2' \|
style="background: #F5F5DC" \| B	style="background: #F5F5DC" \| D?
\| {{nowrap\|Alpha Piscis Austrini}}	style="background: lightgreen;" \| B (TW PsA){{Dollar sign}}	24.7929{{±\|0.0052}}	{{nowrap\|Piscis Austrinus}}	{{RA\|22\|56\|24.17}} {{DEC\|−31\|33\|56}}	style="background: {{star-color\|K}};" \| K5Vp	style="background: lightblue;" \| 6.48{{Hash-tag\|alt=visible to naked eye}}	{{val\|131.5525\|0.0275}}{{cite Gaia EDR3}}	component B of triple system
colspan = '2' style="background: lightgreen;" \| 107 Piscium{{Dollar sign}}	24.805{{±\|0.029}}	Pisces	{{RA\|01\|42\|29.8}} {{DEC\|+20\|16\|07}}	style="background: {{star-color\|K}};" \| K1V	style="background: lightblue;" \| 5.24{{Hash-tag\|alt=visible to naked eye}}	{{val\|131.4903\|0.1515}}{{cite Gaia DR2}}
colspan = '2' \| G 141-36	24.8445{{±\|0.0075}}	Aquila	{{RA\|18\|48\|17.5}} {{DEC\|+07\|41\|21}}	style="background: {{star-color\|M}};" \| M6V		{{val\|131.2790\|0.0398}}
colspan = '2' \| Gliese 514 (BD+11 2576)	24.8782{{±\|0.0051}}	Virgo	{{RA\|13\|29\|59.8}} {{DEC\|+10\|22\|38}}	style="background: {{star-color\|M}};" \| M1.0V	9.02	{{val\|131.1013\|0.0270}}	has 1 known planet
colspan = '2' style="background: #D8BD98" \|WISE 1738+2732§ \|24.92{{±\|0.41}} \| Hercules	{{RA\|17\|38\|35.5}} {{DEC\|+27\|32\|59}} \| style="background: {{star-color\|Y}};" \| Y0 \| \|{{Val\|130.9\|2.1}} \|
colspan = '2' \| GJ 4053 (G 258-33)	24.9254{{±\|0.0041}}	Draco	{{RA\|18\|18\|57.2}} {{DEC\|+66\|11\|33}}	style="background: {{star-color\|M}};" \| M4.5V	13.46	{{val\|130.8531\|0.0217}}
colspan = '2' style="background: #D8BD98" \| WISE J2354+0240§ \|24.97{{±\|0.65}} \| Pisces	{{RA\|23\|54\|02.8}} {{DEC\|+02\|40\|14}} \| style="background: {{star-color\|Y}};" \| Y1 \| \|{{Val\|130.6\|3.3}} \|
scope="col" \| System ! Star or (sub-) brown dwarf ! scope="col" \| Distance (ly) ! Constellation ! Coordinates: RA, Dec (Ep J2000, Eq J2000) ! scope="col" \| Stellar class ! scope="col" \| Apparent magnitude (V) ! scope="col" \| Parallax (mas) ! scope="col" \| Notes and additional references

:List of star systems within 20–25 light-years

See also

References