List of multiplanetary systems
{{Short description|List of systems with multiple planets}}
{{Further|Planetary system}}
[[File:Confirmed exoplanets by methods EPE.svg|right|thumb|350px|Number of extrasolar planet discoveries per year through 2023. Colors indicate method of detection.
{{Col-begin}}
{{Col-break}}
{{legend|#1f77b4|Direct imaging}}
{{legend|#ff7f0e|Gravitational microlensing}}
{{legend|#9467bd|Pulsar timing}}
{{legend|#d62728|Radial velocity}}
{{legend|#2ca02c|Transit photometry}}
{{col-end}}
]]
From the total of {{Extrasolar planet counts|system_count}} stars known to have exoplanets (as of {{Extrasolar planet counts|asof|mdy}}), there are a total of {{Extrasolar planet counts|multiplanetsystem_count}} known multiplanetary systems,{{cite encyclopedia |title=Interactive Extra-solar Planets Catalog |url=https://exoplanet.eu/catalog/ |last=Schneider |first=Jean |date=6 December 2016 |encyclopedia=Extrasolar Planets Encyclopaedia |access-date=2016-12-06 |archive-date=2016-12-09 |archive-url=https://web.archive.org/web/20161209220644/http://exoplanet.eu/catalog/ |url-status=live }} or stars with at least two confirmed planets, beyond the Solar System. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are the Sun (the Solar System's star) and Kepler-90, with 8 confirmed planets each, followed by TRAPPIST-1 with 7 planets.
The {{Extrasolar planet counts|multiplanetsystem_count}} multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has at least one confirmed planet (b, along with the candidate d and the disputed c). The nearest system with four or more confirmed planets is Barnard Star, with four known. The farthest confirmed multiplanetary system is OGLE-2012-BLG-0026L, at {{convert|13,300|ly|pc}} away.{{Cite web |first1=Jean-Philippe |last1=Beaulieu |first2=D. P. |last2=Bennett |first3=Virginie |last3=Batista |first4=A.
|last4=Fukui |date=January 2016 |title=Revisiting the microlensing event OGLE 2012-BLG-0026: A solar mass star with two cold giant planets |url=https://www.researchgate.net/publication/290028818 |website=researchgate.net}}
The table below contains information about the coordinates, spectral and physical properties, and the number of confirmed (unconfirmed) planets for systems with at least 2 planets and 1 not confirmed. The two most important stellar properties are mass and metallicity because they determine how these planetary systems form. Systems with higher mass and metallicity tend to have more planets and more massive planets. However, although low metallicity stars tend to have fewer massive planets, particularly hot-Jupiters, they also tend to have a larger number of close-in planets, orbiting at less than 1 AU.{{cite journal |last1=Brewer |first1=John M. |last2=Wang |first2=Songhu |last3=Fischer |first3=Debra A. |last4=Foreman-Mackey |first4=Daniel |title=Compact multi-planet systems are more common around metal poor hosts|journal=The Astrophysical Journal |volume=867 |at=L3 |arxiv=1810.10009 |doi=10.3847/2041-8213/aae710 |date=2018-10-24 |issue=1 |bibcode=2018ApJ...867L...3B |s2cid=67832557 |doi-access=free }}
Multiplanetary systems
{{Dynamic list}}
| class="wikitable" |
| style="background: #eaeaea" colspan=8|Color indicates number of planets |
|---|
| bgcolor="#fdfdfd" width=30 style="text-align: center" |2 (x)
| bgcolor="#cddafb" width=30 style="text-align: center" |3 | bgcolor="#aaeee9" width=30 style="text-align: center" |4 | bgcolor="#90e090" width=30 style="text-align: center" |5 | bgcolor="#ccdd66" width=30 style="text-align: center" |6 | bgcolor="#e0c066" width=30 style="text-align: center" |7 | bgcolor="#f08a6c" width=30 style="text-align: center" |8 | bgcolor="#f76879" width=30 style="text-align: center" |9 |
{{clear}}
{{Multiplanetary systems list/Top}}
{{Multiplanetary systems list
| Star = Sun
| Constellation = -
| Right ascension = -
| Declination = -
| Apparent magnitude = −26.74
| Distance = 0.000016
| Spectral type = G2V
| Mass = 1.000
| Radius = 1.000
| Temperature = 5778
| Metallicity = 0.000
| Age = 4.572
| Confirmed planets = 8
|Unconfirmed planets = 1
| Notes = Pluto was considered a planet before 2006. The hypothesised Planet Nine remains unconfirmed.
}}
{{Multiplanetary systems list
| Star = Proxima Centauri
| Constellation = Centaurus
| Right ascension = {{RA|14|29|42.94853}}
| Declination = {{DEC|−62|40|46.1631}}
| Apparent magnitude = 10.43 to 11.11{{cite journal |bibcode=2009yCat....102025S |title=VizieR online data catalog: General catalogue of variable stars (Samus+ 2007–2013) |journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S |volume=1 |display-authors=etal |last1=Samus |first1=N. N. |last2=Durlevich |first2=O. V. |year=2009}}
| Distance = 4.244
| Spectral type = M5.5Ve{{cite journal |bibcode=1991AJ....101..662B |title=The late-M dwarfs |journal=The Astronomical Journal |volume=101 |pages=662 |last1=Bessell |first1=M. S. |year=1991 |doi=10.1086/115714|doi-access=free }}
| Mass = 0.1221
| Radius = 0.1542
| Temperature = 3042
| Metallicity = 0.21
| Age = 4.85
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Closest star to the Sun and closest star to the Sun with a multiplanetary system. Planet b is potentially habitable.{{cite journal |last1=Mascareño |first1=A. Suárez |last2=Faria |first2=J. P. |last3=Figueira |first3=P. |last4=Lovis |first4=C. |last5=Damasso |first5=M. |last6=Hernández |first6=J. I. González |last7=Rebolo |first7=R. |last8=Cristiani |first8=S. |last9=Pepe |first9=F. |last10=Santos |first10=N. C. |last11=Osorio |first11=M. R. Zapatero |last12=Adibekyan |first12=V. |last13=Hojjatpanah |first13=S. |last14=Sozzetti |first14=A. |last15=Murgas |first15=F. |last16=Abreu |first16=M. |last17=Affolter |first17=M. |last18=Alibert |first18=Y. |last19=Aliverti |first19=M. |last20=Allart |first20=R. |last21=Prieto |first21=C. Allende |last22=Alves |first22=D. |last23=Amate |first23=M. |last24=Avila |first24=G. |last25=Baldini |first25=V. |last26=Bandi |first26=T. |last27=Barros |first27=S. C. C. |last28=Bianco |first28=A. |last29=Benz |first29=W. |last30=Bouchy |first30=F. |last31=Broeng |first31=C. |last32=Cabral |first32=A. |last33=Calderone |first33=G. |last34=Cirami |first34=R. |last35=Coelho |first35=J. |last36=Conconi |first36=P. |last37=Coretti |first37=I. |last38=Cumani |first38=C. |last39=Cupani |first39=G. |last40=D’Odorico |first40=V. |last41=Deiries |first41=S. |last42=Delabre |first42=B. |last43=Marcantonio |first43=P. Di |last44=Dumusque |first44=X. |last45=Ehrenreich |first45=D. |last46=Fragoso |first46=A. |last47=Genolet |first47=L. |last48=Genoni |first48=M. |last49=Santos |first49=R. Génova |last50=Hughes |first50=I. |last51=Iwert |first51=O. |last52=Kerber |first52=F. |last53=Knusdstrup |first53=J. |last54=Landoni |first54=M. |last55=Lavie |first55=B. |last56=Lillo-Box |first56=J. |last57=Lizon |first57=J. |last58=Curto |first58=G. Lo |last59=Maire |first59=C. |last60=Manescau |first60=A. |last61=Martins |first61=C. J. a. P. |last62=Mégevand |first62=D. |last63=Mehner |first63=A. |last64=Micela |first64=G. |last65=Modigliani |first65=A. |last66=Molaro |first66=P. |last67=Monteiro |first67=M. A. |last68=Monteiro |first68=M. J. P. F. G. |last69=Moschetti |first69=M. |last70=Mueller |first70=E. |last71=Nunes |first71=N. J. |last72=Oggioni |first72=L. |last73=Oliveira |first73=A. |last74=Pallé |first74=E. |last75=Pariani |first75=G. |last76=Pasquini |first76=L. |last77=Poretti |first77=E. |last78=Rasilla |first78=J. L. |last79=Redaelli |first79=E. |last80=Riva |first80=M. |last81=Tschudi |first81=S. Santana |last82=Santin |first82=P. |last83=Santos |first83=P. |last84=Segovia |first84=A. |last85=Sosnowska |first85=D. |last86=Sousa |first86=S. |last87=Spanò |first87=P. |last88=Tenegi |first88=F. |last89=Udry |first89=S. |last90=Zanutta |first90=A. |last91=Zerbi |first91=F. |title=Revisiting Proxima with ESPRESSO |journal=Astronomy & Astrophysics |date=1 July 2020 |volume=639 |pages=A77 |doi=10.1051/0004-6361/202037745 |arxiv=2005.12114 |bibcode=2020A&A...639A..77S |s2cid=218869742 |url=https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |language=en |issn=0004-6361 |access-date=9 May 2022 |archive-date=27 June 2022 |archive-url=https://web.archive.org/web/20220627141045/https://www.aanda.org/articles/aa/abs/2020/07/aa37745-20/aa37745-20.html |url-status=live }}{{cite journal |last1=Del Genio |first1=Anthony D. |last2=Way |first2=Michael J. |last3=Amundsen |first3=David S. |last4=Aleinov |first4=Igor |last5=Kelley |first5=Maxwell |last6=Kiang |first6=Nancy Y. |last7=Clune |first7=Thomas L. |title=Habitable Climate Scenarios for Proxima Centauri b with a Dynamic Ocean |journal=Astrobiology |date=January 2019 |volume=19 |issue=1 |pages=99–125 |doi=10.1089/ast.2017.1760 |pmid=30183335 |arxiv=1709.02051 |bibcode=2019AsBio..19...99D |s2cid=52165056 |url=https://www.liebertpub.com/doi/full/10.1089/ast.2017.1760 |issn=1531-1074}} Planet c initially appeared likely but has since been disputed.{{cite journal|last1=Artigau|first1=Étienne|last2=Cadieux|first2=Charles|last3=Cook|first3=Neil J.|last4=Doyon|first4=René|last5=Vandal|first5=Thomas|last6=Donati|first6=Jean-Françcois|last7=Moutou|first7=Claire|last8=Delfosse|first8=Xavier|last9=Fouqué|first9=Pascal|last10=Martioli|first10=Eder|last11=Bouchy|first11=François|last12=Parsons|first12=Jasmine|last13=Carmona|first13=Andres|last14=Dumusque|first14=Xavier|last15=Astudillo-Defru|first15=Nicola|last16=Bonfils|first16=Xavier|last17=Mignon|first17=Lucille|display-authors=5|title=Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry|journal=The Astronomical Journal|volume=164:84|issue=3|pages=18pp|arxiv=2207.13524|bibcode=2022AJ....164...84A|doi=10.3847/1538-3881/ac7ce6|doi-access=free|date=June 23, 2022|publication-date=August 8, 2022}}
}}
{{Multiplanetary systems list
| Star = Barnard's Star
| Constellation = Ophiuchus
| Right ascension = {{RA|17|57|48.4985}}
| Declination = {{DEC|+04|41|36.1139}}
| Apparent magnitude = 9.511
| Distance = 5.96
| Spectral type = M4.0V{{cite journal|bibcode=1997AJ....113..806G|title=M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale|journal=The Astronomical Journal|volume=113|issue=2|pages=806–822|last=Gizis|first=John E. |date=February 1997|doi=10.1086/118302|arxiv=astro-ph/9611222|s2cid=16863021}}
| Mass = 0.162
| Radius = 0.187
| Temperature = 3195
| Metallicity = -0.56
| Age = 10
| Confirmed planets = 4
|Unconfirmed planets = 0
| Notes = Closest single star to the Sun with a confirmed multiplanetary system.{{cite journal |last1=Basant |first1=Ritvik |last2=Luque |first2=Rafael |display-authors=etal |date=March 2025 |title=Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO |journal=The Astrophysical Journal Letters |volume=982 |issue=|pages=L1 |doi=10.3847/2041-8213/adb8d5 |doi-access=free |arxiv=2503.08095}}
}}
{{Multiplanetary systems list
| Star = Lalande 21185
| Constellation = Ursa Major
| Right ascension = {{RA|11|03|20.1940}}
| Declination = {{DEC|+35|58|11.5682}}
| Apparent magnitude = 7.520{{citation | last=Oja | first=T. | title=Photoelectric photometry of stars near the north Galactic pole. II | journal=Astronomy and Astrophysics Supplement Series | volume=61 | pages=331–339 |date=August 1985 | bibcode=1985A&AS...61..331O }}
| Distance = 8.3044{{±|0.0007}}
| Spectral type = M2V
| Mass = 0.390
| Radius = 0.392{{±|0.004}}
| Temperature = 3601{{±|51}}
| Metallicity = -0.09{{±|0.16}}
| Age = 8.047
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Brightest red dwarf star in the northern celestial hemisphere.{{cite web
| url =http://www.universetoday.com/111716/14-red-dwarf-stars-to-view-with-backyard-telescopes/
| title =14 Red Dwarf Stars to View with Backyard Telescopes
| last =Dickinson
| first =David
| date =2015-12-23
| publisher =Universe Today
| access-date =2016-12-04
| archive-date =2021-02-11
| archive-url =https://web.archive.org/web/20210211185356/https://www.universetoday.com/111716/14-red-dwarf-stars-to-view-with-backyard-telescopes/
| url-status =live
| url =http://kencroswell.com/thebrightestreddwarf.html
| title =The Brightest Red Dwarf
| last =Croswell
| first =Ken
| date =July 2002
| website =KenCroswell.com
| access-date =2016-12-04
| archive-date =2018-10-20
| archive-url =https://web.archive.org/web/20181020223954/http://www.kencroswell.com/thebrightestreddwarf.html
| url-status =live
}}
}}
{{Multiplanetary systems list
| Star = Lacaille 9352
| Constellation = Piscis Austrinus
| Right ascension = {{RA|23|05|52.04}}
| Declination = {{DEC|−35|51|11.05}}
| Apparent magnitude = 7.34
| Distance = 10.721
| Spectral type = M0.5V
| Mass = 0.486
| Radius = 0.47{{±|0.001}}
| Temperature = 3688{{±|86}}
| Metallicity = -0.06{{±|0.08}}
| Age = 4.57
| Confirmed planets = 2
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = Luyten's Star
| Constellation = Canis Minor
| Right ascension = {{RA|07|27|24.4991}}
| Declination = {{DEC|05|13|32.827}}
| Apparent magnitude = 9.872
| Distance = 11.20
| Spectral type = M3.5V
| Mass = 0.26
| Radius = 0.35
| Temperature = 3150
| Metallicity = -0.16
| Age =
| Confirmed planets = 2
|Unconfirmed planets = 2
| Notes = Stellar activity level and rotational rate suggest an age higher than 8 billion years.{{cite journal
|last1=Pozuelos |first1=Francisco J. |last2=Suárez |first2=Juan C.
|last3=de Elía |first3=Gonzalo C. |last4=Berdiñas |first4=Zaira M.
|last5=Bonfanti |first5=Andrea |last6=Dugaro |first6=Agustín
|last7=Gillon |first7=Michaël |last8=Jehin |first8=Emmanuël
|last9=Günther |first9=Maximilian N. |last10=van Grootel |first10=Valérie
|last11=Garcia |first11=Lionel J. |last12=Thuillier |first12=Antoine
|last13=Delrez |first13=Laetitia |last14=Rodón |first14=Jose R.
|display-authors=6
|year=2020
|title=GJ 273: On the formation, dynamical evolution, and habitability of a planetary system hosted by an M dwarf at 3.75 parsec
|journal=Astronomy & Astrophysics
|volume=641 |pages=A23
|doi=10.1051/0004-6361/202038047 |arxiv=2006.09403
|bibcode=2020A&A...641A..23P |s2cid=219721292 |quote=GJ 273 is a planetary system orbiting an M dwarf only 3.75 pc away, composed of two confirmed planets, GJ 273b and GJ 273c, and two promising candidates, GJ 273d and GJ 273e ... the system remained stable only for values of inclinations ranging from 90◦ to ~72◦
}}
Planet b is potentially habitable.{{cite journal
|doi = 10.1051/0004-6361/201630153
|last1 = Astudillo-Defru
|first1 = Nicola
|last2 = Forveille
|first2 = Thierry
|last3 = Bonfils
|first3 = Xavier
|last4 = Ségransan
|first4 = Damien
|last5 = Bouchy
|first5 = François
|last6 = Delfosse
|first6 = Xavier
|last7 = Lovis
|first7 = Christophe
|last8 = Mayor
|first8 = Michel
|last9 = Murgas
|first9 = Felipe
|last10 = Pepe
|first10 = Francesco
|last11 = Santos
|first11 = Nuno C.
|last12 = Udry
|first12 = Stéphane
|last13 = Wünsche
|first13 = Anaël
|display-authors = 6
|year = 2017
|title = The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293
|journal = Astronomy and Astrophysics
|volume = 602
|at = A88
|arxiv = 1703.05386
|bibcode = 2017A&A...602A..88A
|s2cid = 119418595
|url = https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|access-date = 2022-02-25
|archive-date = 2022-09-28
|archive-url = https://web.archive.org/web/20220928032005/https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|url-status = live
}}
}}
{{Multiplanetary systems list
| Star = YZ Ceti
| Constellation = Cetus
| Right ascension = {{RA|01|12|30.64}}
| Declination = {{DEC|−16|59|56.3}}
| Apparent magnitude = 12.07
| Distance = 11.74
| Spectral type = M4.5V
| Mass = 0.13
| Radius = 0.168
| Temperature = 3056
| Metallicity = -0.26
| Age = 4.0
| Confirmed planets = 3
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = Gliese 1061
| Constellation = Horologium (constellation){{!}}Horologium
| Right ascension = {{RA|03|35|59.69}}
| Declination = {{DEC|-44|30|45.3}}
| Apparent magnitude = 13.03
| Distance = 12.04
| Spectral type = M5.5V
| Mass = 0.113
| Radius =
| Temperature = 2953
| Metallicity = -0.09
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Planets c and d are potentially habitable.{{Cite journal |journal=Monthly Notices of the Royal Astronomical Society
|last1=Dreizler |first1=S.
|last2=Jeffers |first2=S. V.
|last3=Rodríguez |first3=E.
|last4=Zechmeister |first4=M.
|last5=Barnes |first5 = J.R.
|last6=Haswell |first6=C.A.
|last7=Coleman |first7=G. A. L.
|last8=Lalitha |first8=S.
|last9=Hidalgo Soto |first9=D.
|last10=Strachan |first10=J.B.P.
|last11=Hambsch |first11=F-J.
|last12=López-González |first12=M. J.
|last13=Morales |first13=N.
|last14=Rodríguez López |first14=C.
|last15=Berdiñas |first15=Z. M.
|last16=Ribas |first16=I.
|last17=Pallé |first17=E.
|last18=Reiners |first18=Ansgar
|last19=Anglada-Escudé |first19=G.
|date=2019-08-13 |title=Red Dots: A temperate 1.5 Earth-mass planet in a compact multi-terrestrial planet system around GJ1061 |volume=493 |issue=1 |pages=536–550 |doi=10.1093/mnras/staa248 |doi-access=free |arxiv=1908.04717| s2cid=199551874 |language=en}}
}}
{{Multiplanetary systems list
| Star = Teegarden's Star
| Constellation = Aries (constellation){{!}}Aries
| Right ascension = {{RA|02|53|00.89}}
| Declination = {{DEC|+16|52|53}}
| Apparent magnitude = 15.13
| Distance = 12.497
| Spectral type = M7V
| Mass = 0.097
| Radius = 0.120
| Temperature = 3034
| Metallicity = -0.11±0.28
| Age = 8
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Teegarden's Star b and Teegarden's Star c are likely Earth-mass planets that orbit in the habitable zone.{{cite journal |last1=Caballero |first1=J. A. |last2=Reiners |first2=Ansgar |last3=Ribas |first3=I. |last4=Dreizler |first4=S. |last5=Zechmeister |first5=M. |display-authors=etal |date=12 June 2019 |title=The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star |journal=Astronomy & Astrophysics |volume=627 |pages=A49 |language=en |doi=10.1051/0004-6361/201935460 |arxiv=1906.07196 |issn=0004-6361 |bibcode=2019A&A...627A..49Z |s2cid=189999121 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Wolf 1061
| Constellation = Ophiuchus (constellation){{!}}Ophiuchus
| Right ascension = {{RA|16|30|18.0584}}
| Declination = {{DEC|-12|39|45.325}}
| Apparent magnitude = 10.07
| Distance = 14.050 ± 0.002
| Spectral type = M3.5V
| Mass = 0.294
| Radius = 0.307
| Temperature = 3342
| Metallicity = -0.09
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Planet c is potentially habitable.{{cite journal |last1=Davison |first1=Cassy L. |last2=White |first2=Russel J. |last3=Henry |first3=Todd J. |last4=Riedel |first4=Adric R. |last5=Jao |first5=Wei-Chun |last6=Bailey III |first6=John I. |last7=Quinn |first7=Samuel N. |last8=Justin R. |first8=Cantrell |last9=John P. |first9=Subasavage |last10=Jen G. |first10=Winters |title=A 3D Search for Companions to 12 Nearby M-Dwarfs |year=2015 |arxiv=1501.05012 |doi=10.1088/0004-6256/149/3/106 |volume=149 |issue=3 |journal=The Astronomical Journal |page=106|bibcode = 2015AJ....149..106D |s2cid=9719725 }}{{cite web|author=Stuart Gary|url=http://www.abc.net.au/news/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824|title=Potentially habitable super-Earth discovered orbiting star 14 light years from Earth|publisher=ABC News (Australia)|date=17 December 2015|access-date=2022-05-10|archive-date=2017-06-09|archive-url=https://web.archive.org/web/20170609122527/http://www.abc.net.au/news/science/2015-12-17/nearest-habitable-zone-superearth-terrestrial-planet-wolf1061/7033824|url-status=live}}{{citation
| title=Characterization of the Wolf 1061 Planetary System
| last1=Kane | first1=Stephen R. | last2=von Braun | first2=Kaspar
| last3=Henry | first3=Gregory W. | last4=Waters | first4=Miranda A.
| last5=Boyajian | first5=Tabetha S. | last6=Mann | first6=Andrew W.
| journal=The Astrophysical Journal | display-authors=1
| volume=835 | issue=2 | id=200 | pages=9 | date=February 2017
| doi=10.3847/1538-4357/835/2/200 | bibcode=2017ApJ...835..200K
| arxiv=1612.09324 | s2cid=30738573 | postscript=. | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Gliese 876
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|53|16.73}}
| Declination = {{DEC|−14|15|49.3}}
| Apparent magnitude = 10.17
| Distance = 15.25
| Spectral type = M4V
| Mass = 0.334
| Radius = 0.356
| Temperature = 3348
| Metallicity = 0.054
| Age = 4.893
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Planet b is a gas giant which orbits in the habitable zone.{{cite journal | title=Prospects for Habitable "Earths" in Known Exoplanetary Systems | last1=Jones | first1=Barrie W. | last2=Underwood | first2=David R. | last3=Sleep | first3=P. Nick | display-authors=1 | journal=The Astrophysical Journal | volume=622 | issue=2 | pages=1091–1101 | year=2005 | arxiv=astro-ph/0503178 | bibcode=2005ApJ...622.1091J | bibcode-access=free | doi=10.1086/428108 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = 82 G. Eridani
| Constellation = Eridanus (constellation){{!}}Eridanus
| Right ascension = {{RA|03|19|55.65}}
| Declination = {{DEC|−43|04|11.2}}
| Apparent magnitude = 4.254
| Distance = 19.71
| Spectral type = G8V
| Mass = 0.70
| Radius = 0.92
| Temperature = 5401
| Metallicity = −0.40
| Age = 5.76
| Confirmed planets = 3
|Unconfirmed planets = 3
| Notes = This star also has a dust disk{{cite journal | display-authors=1
|last1=Wyatt |first1=M. C. |last2=Kennedy |first2=G. |last3=Sibthorpe |first3=B. |last4=Moro-Martín |first4=A. |last5=Lestrade |first5=J.-F. |last6=Ivison |first6=R. J. |last7=Matthews |first7=B. |last8=Udry |first8=S. |last9=Greaves |first9=J. S. |last10=Kalas |first10=P. |last11=Lawler |first11=S. |last12=Su |first12=K. Y. L. |last13=Rieke |first13=G. H. |last14=Booth |first14=M. |last15=Bryden |first15=G. |last16=Horner |first16=J. |last17=Kavelaars |first17=J. J. |last18=Wilner |first18=D.
|date = 2012 | journal=Monthly Notices of the Royal Astronomical Society
|volume=424 |issue=2 |pages=1206 |title = Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems
|arxiv = 1206.2370 | doi=10.1111/j.1365-2966.2012.21298.x
|doi-access=free |bibcode=2012MNRAS.424.1206W |s2cid=54056835 }} with a semi-major axis at approximately 19 AU.{{Cite journal | doi = 10.1093/mnras/stv511| title = Kuiper belt structure around nearby super-Earth host stars| journal = Monthly Notices of the Royal Astronomical Society| volume = 449| issue = 3| pages = 3121| year = 2015| last1 = Kennedy | first1 = G. M.| last2 = Matra | first2 = L.| last3 = Marmier | first3 = M.| last4 = Greaves | first4 = J. S.| last5 = Wyatt | first5 = M. C.| last6 = Bryden | first6 = G.| last7 = Holland | first7 = W.| last8 = Lovis | first8 = C.| last9 = Matthews | first9 = B. C.| last10 = Pepe | first10 = F.| last11 = Sibthorpe | first11 = B.| last12 = Udry | first12 = S.| doi-access = free|arxiv = 1503.02073 |bibcode = 2015MNRAS.449.3121K | s2cid = 53638901}}
}}
{{Multiplanetary systems list
| Star = Gliese 581
| Constellation = Libra (constellation){{!}}Libra
| Right ascension = {{RA|15|19|26.83}}
| Declination = {{DEC|−07|43|20.2}}
| Apparent magnitude = 10.56
| Distance = 20.56
| Spectral type = M3V
| Mass = 0.311
| Radius = 0.378
| Temperature = 3484
| Metallicity = −0.335
| Age = 4.326
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes = The disputed planet d is potentially habitable.{{cite news |title=Reanalysis of data suggests 'habitable' planet GJ 581d really could exist |url=http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |date=9 March 2015 |work=Astronomy Now |access-date=27 May 2015 |archive-date=20 May 2015 |archive-url=https://web.archive.org/web/20150520175016/http://astronomynow.com/2015/03/09/reanalysis-of-data-suggests-habitable-planet-gj581d-really-does-exist/ |url-status=live }}
}}
{{Multiplanetary systems list
| Star = Gliese 667 C
| Constellation = Scorpius
| Right ascension = {{RA|17|18|57.16}}
| Declination = {{DEC|−34|59|23.14}}
| Apparent magnitude = 10.20
| Distance = 21
| Spectral type = M1.5V
| Mass = 0.31
| Radius = 0.42
| Temperature = 3700
| Metallicity = −0.59
| Age = 2.000
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Triple star system - all exoplanets orbit around Star C. Planet c is potentially habitable, and there are more unconfirmed planets.{{cite journal|title=A Planetary System around the nearby M Dwarf GJ 667C with At Least One Super-Earth in Its Habitable Zone|author1=Anglada-Escudé, Guillem |author2=Arriagada, Pamela |author3=Vogt, Steven S. |author4=Rivera, Eugenio J. |author5=Butler, R. Paul |author6=Crane, Jeffrey D. |author7=Shectman, Stephen A. |author8=Thompson, Ian B. |author9=Minniti, Dante |author10=Haghighipour, Nader |author11=Carter, Brad D. |author12=Tinney, C. G. |author13=Wittenmyer, Robert A. |author14=Bailey, Jeremy A. |author15=O'Toole, Simon J. |author16=Jones, Hugh R. A. |author17=Jenkins, James S. |year=2012|journal=The Astrophysical Journal Letters|volume=751|issue=1|pages= |at= L16|doi=10.1088/2041-8205/751/1/L16|bibcode=2012ApJ...751L..16A|arxiv=1202.0446|s2cid=16531923 }}{{cite journal|title=A dynamically-packed planetary system around GJ 667C with three super-Earths in its habitable zone |url=http://www.eso.org/public/archives/releases/sciencepapers/eso1328/eso1328a.pdf |date=2013-06-07 |author=Anglada-Escudé, Guillem |display-authors=etal |journal=Astronomy & Astrophysics |doi=10.1051/0004-6361/201321331 |access-date=2013-06-25 |arxiv=1306.6074 |bibcode=2013A&A...556A.126A |volume=556 |pages=A126 |s2cid=14559800 |url-status=dead |archive-url=https://web.archive.org/web/20130630214924/http://www.eso.org/public/archives/releases/sciencepapers/eso1328/eso1328a.pdf |archive-date=2013-06-30 }}{{Cite journal |doi = 10.1088/0004-637X/780/2/124|title = Dynamical Evolution and Spin-Orbit Resonances of Potentially Habitable Exoplanets. The Case of Gj 667C|journal = The Astrophysical Journal|volume = 780|issue = 2|pages = 124|year = 2013|last1 = Makarov|first1 = Valeri V.|last2 = Berghea|first2 = Ciprian|arxiv = 1311.4831|s2cid = 118700510}}
}}
{{Multiplanetary systems list
| Star = HD 219134
| Constellation = Cassiopeia (constellation){{!}}Cassiopeia
| Right ascension = {{RA|23|13|14.74}}
| Declination = {{DEC|57|10|03.5}}
| Apparent magnitude = 5.57
| Distance = 21
| Spectral type = K3Vvar
| Mass = 0.794
| Radius = 0.778
| Temperature = 4699
| Metallicity = 0.11
| Age = 12.66
| Confirmed planets = 6
|Unconfirmed planets =
| Notes = Closest star to the Sun with exactly six{{cite journal |arxiv=1509.07912 |last1=Vogt |first1=Steven S. |display-authors=etal |title=Six Planets Orbiting HD 219134 |date=November 2015 |doi=10.1088/0004-637X/814/1/12 |volume=814 |issue=1 |journal=The Astrophysical Journal |page=12 |bibcode=2015ApJ...814...12V|s2cid=45438051 }} exoplanets, and closest K-type main sequence star to the Sun with a multiplanetary system. One of the oldest stars with a multiplanetary system, although it is still more metal-rich than the Sun. None of the known planets is in the habitable zone.{{cite journal |author-link= |arxiv=2112.05337 |title= An Integrative Analysis of the HD 219134 Planetary System and the Inner solar system: Extending DYNAMITE with Enhanced Orbital Dynamical Stability Criteria|last1= Dietrich|first1= Jeremy|last2= Apai|first2= Dániel|last3= Malhotra|first3= Renu|journal=The Astronomical Journal |year= 2022|volume=163 |issue=2 |page=88 |doi=10.3847/1538-3881/ac4166 |bibcode=2022AJ....163...88D |s2cid=245117944 |doi-access=free }}
}}
{{Multiplanetary systems list
| Star = 61 Virginis
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|13|18|24.31}}
| Declination = {{DEC|−18|18|40.3}}
| Apparent magnitude = 4.74
| Distance = 28
| Spectral type = G5V
| Mass = 0.954
| Radius = 0.945
| Temperature = 5531
| Metallicity = −0.008
| Age = 8.960
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Planet d remains unconfirmed,{{Cite journal | last1=Wyatt | first1=M. C. | last2=Kennedy | first2=G. | last3=Sibthorpe | first3=B. | last4=Moro-Martín | first4=A. | last5=Lestrade | first5=J.-F. | last6=Ivison | first6=R. J. | last7=Matthews | first7=B. | last8=Udry | first8=S. | last9=Greaves | first9=J. S. | last10=Kalas | first10=P. | last11=Lawler | first11=S. | last12=Su | first12=K. Y. L. | last13=Rieke | first13=G. H. | last14=Booth | first14=M. | last15=Bryden | first15=G. | last16=Horner | first16=J. | last17=Kavelaars | first17=J. J. | last18=Wilner | first18=D. | display-authors=1 | title=Herschel imaging of 61 Vir: implications for the prevalence of debris in low-mass planetary systems | journal=MNRAS | date=2012 | bibcode = 2012MNRAS.424.1206W | doi = 10.1111/j.1365-2966.2012.21298.x | arxiv=1206.2370 | volume=424 | issue=2 | pages=1206–1223| doi-access=free | s2cid=54056835 }} and a 2021 study found that it was likely a false positive.{{cite journal |arxiv=2105.11583|doi=10.3847/1538-4365/abe23c|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|year=2021|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973 |doi-access=free }} 61 Virginis also has a debris disk.
}}
{{Multiplanetary systems list
| Star = Gliese 433
| Constellation = Hydra (constellation){{!}}Hydra
| Right ascension = {{RA|11|35|26.9485}}
| Declination = {{DEC|-25|10|08.9}}
| Apparent magnitude = 9.79
| Distance = 29.8±0.1
| Spectral type = M1.5V
| Mass = 0.48
| Radius = 0.48±0.01
| Temperature = 3550±100
| Metallicity = -0.02±0.05
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = An infrared excess around this star suggests a circumstellar disk.{{cite journal
| title=Kuiper belt analogues in nearby M-type planet-host systems
| last1=Kennedy | first1=G. M. | last2=Bryden | first2=G.
| last3=Ardila | first3=D. | last4=Eiroa | first4=C.
| last5=Lestrade | first5=J. -F. | last6=Marshall | first6=J. P.
| last7=Matthews | first7=B. C. | last8=Moro-Martin | first8=A.
| last9=Wyatt | first9=M. C. | display-authors=1
| journal=Monthly Notices of the Royal Astronomical Society
| volume=476 | issue=4 | pages=4584–4591 | date=June 2018
| doi=10.1093/mnras/sty492 | doi-access=free | arxiv=1803.02832
| bibcode=2018MNRAS.476.4584K }}
}}
{{Multiplanetary systems list
| Star = Gliese 357
| Constellation = Hydra (constellation){{!}}Hydra
| Right ascension = {{RA|09|36|01.6373}}
| Declination = {{DEC|-21|39|38.878}}
| Apparent magnitude = 10.906
| Distance = 30.776
| Spectral type = M2.5V
| Mass = 0.362
| Radius = 0.333
| Temperature = 3488
| Metallicity = -0.14
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Planet d is a potentially habitable Super-Earth.Falconer, Rebecca, [https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html Newly uncovered super-Earth 31 light-years away may be habitable] {{Webarchive|url=https://web.archive.org/web/20191218061126/https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html |date=2019-12-18 }}, Axios, August 1, 2019{{Cite web|url=https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|title=TESS Discovers Habitable Zone Planet in GJ 357 System|last1=Reddy|first1=Francis|last2=Center|first2=NASA’s Goddard Space Flight|date=2019-07-31|website=SciTechDaily|language=en-US|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801162521/https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|url-status=live}}{{Cite web|url=https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|title=Potentially habitable 'super-Earth' discovered just 31 light-years away|website=NBC News|date=31 July 2019|language=en|access-date=2019-08-01|archive-date=2019-07-31|archive-url=https://web.archive.org/web/20190731230808/https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|url-status=live}}{{Cite web|url=http://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world|title=NASA's TESS Helps Find Intriguing New World|last=Garner|first=Rob|date=2019-07-30|website=NASA|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801045621/https://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world/|url-status=live}}
}}
{{Multiplanetary systems list
| Star = L 98-59
| Constellation = Volans
| Right ascension = {{RA|08|18|07.62}}
| Declination = {{DEC|-68|18|46.8}}
| Apparent magnitude = 11.69
| Distance = 34.6
| Spectral type = M3V
| Mass = 0.312
| Radius = 0.314
| Temperature = 3412
| Metallicity = -0.5
| Age =
| Confirmed planets = 4
|Unconfirmed planets = 1
| Notes = The unconfirmed planet f orbits in the habitable zone.{{cite journal
|display-authors = etal
|first1 = Oliver D. S.
|last1 = Demangeon
|first2 = M. R.
|last2 = Zapatero Osorio
|first3 = Y.
|last3 = Alibert
|first4 = S. C. C.
|last4 = Barros
|first5 = V.
|last5 = Adibekyan
|first6 = H. M.
|last6 = Tabernero
|title = A warm terrestrial planet with half the mass of Venus transiting a nearby star
|url = https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf
|date = July 2021
|journal = Astronomy & Astrophysics
|volume = 653
|pages = 38
|doi = 10.1051/0004-6361/202140728
|s2cid = 236957385
|arxiv = 2108.03323
|bibcode = 2021A&A...653A..41D
|access-date = 2022-03-03
|archive-date = 2021-11-13
|archive-url = https://web.archive.org/web/20211113184620/https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf
|url-status = live
}}
}}
{{Multiplanetary systems list
| Star = Gliese 414 A
| Constellation = Ursa Major
| Right ascension = {{RA|11|11|05.88}}
| Declination = {{DEC|30|26|42.61}}
| Apparent magnitude = 8.31
| Distance = 38.76
| Spectral type = K7V
| Mass = 0.65
| Radius = 0.679
| Temperature = 4120
| Metallicity = 0.24
| Age = 12.4
| Confirmed planets = 2
|Unconfirmed planets = 0
| Notes = {{Cite journal |last1=Dedrick |first1=Cayla M. |last2=Fulton |first2=Benjamin J. |last3=Knutson |first3=Heather A. |last4=Howard |first4=Andrew W. |last5=Beatty |first5=Thomas G. |last6=Cargile |first6=Phillip A. |last7=Gaudi |first7=B. Scott |last8=Hirsch |first8=Lea A. |last9=Kuhn |first9=Rudolf B. |last10=Lund |first10=Michael B. |last11=James |first11=David J. |last12=Kosiarek |first12=Molly R. |last13=Pepper |first13=Joshua |last14=Petigura |first14=Erik A. |last15=Rodriguez |first15=Joseph E. |date=January 2021 |title=Two Planets Straddling the Habitable Zone of the Nearby K Dwarf Gl 414A |journal=The Astronomical Journal |language=en |volume=161 |issue=2 |pages=86 |doi=10.3847/1538-3881/abd0ef |doi-access=free |arxiv=2009.06503 |bibcode=2021AJ....161...86D |issn=1538-3881}}{{Cite web |title=GJ 414 Overview |url=https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414 |access-date=January 4, 2024 |website=NASA Exoplanet Archive |archive-date=December 9, 2023 |archive-url=https://web.archive.org/web/20231209091347/https://exoplanetarchive.ipac.caltech.edu/overview/GJ%20414 |url-status=live }}
}}
{{Multiplanetary systems list
| Star = Gliese 806
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|20|45|04.099}}
| Declination = {{DEC|+44|29|56.6}}
| Apparent magnitude = 10.79
| Distance = 39.3
| Spectral type = M1.5V
| Mass = 0.423
| Radius = 0.414
| Temperature = 3586
| Metallicity = -0.28
| Age = 3.0
| Confirmed planets = 2
|Unconfirmed planets = 1
|
}}
{{Multiplanetary systems list
| Star = TRAPPIST-1
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|23|06|29.283}}
| Declination = {{DEC|-05|02|28.59}}
| Apparent magnitude = 18.80
| Distance = 39.5
| Spectral type = M8V
| Mass = 0.089
| Radius = 0.114
| Temperature = 2550
| Metallicity = 0.04
| Age = 7.6
| Confirmed planets = 7
|Unconfirmed planets =
| Notes = Planets d, e, f and g are potentially habitable. Only star known with exactly seven confirmed planets. All seven terrestrial planets lie within only 0.07 AU of the star.
}}
{{Multiplanetary systems list
| Star = 55 Cancri|Copernicus
| Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|08|52|35.81}}
| Declination = {{DEC|+28|19|50.9}}
| Apparent magnitude = 5.95
| Distance = 40
| Spectral type = K0IV-V
| Mass = 1.026
| Radius = 0.887
| Temperature = 5217
| Metallicity = 0.290
| Age = 7.4
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = All five known planets orbit around star A (none are circumbinary or orbit around star B). Closest system with exactly five confirmed planets.
}}
{{Multiplanetary systems list
| Star = Gliese 180
| Constellation = Eridanus (constellation){{!}}Eridanus
| Right ascension = {{RA|04|53|49.9798}}
| Declination = {{DEC|-17|46|24.294}}
| Apparent magnitude = 10.894
| Distance = 40.3
| Spectral type = M2V{{cite journal
| title=The CARMENES search for exoplanets around M dwarfs. Different roads to radii and masses of the target stars
| display-authors=1 | last1=Schweitzer | first1=A.
| last2=Passegger | first2=V. M. | last3=Cifuentes | first3=C.
| last4=Béjar | first4=Victor J. S. | last5=Cortés-Contreras | first5=M.
| last6=Caballero | first6=José A. | last7=del Burgo | first7=Carlos
| last8=Czesla | first8=Stefan | last9=Kürster | first9=Martin
| last10=Montes | first10=David | last11=Zapatero-Osorio | first11=María Rosa
| last12=Ribas | first12=Ignasi | last13=Reiners | first13=Ansgar
| last14=Quirrenbach | first14=Andreas | last15=Amado | first15=Pedro J.
| last16=Aceituno | first16=J. | last17=Anglada-Escudé | first17=Guillem
| last18=Bauer | first18=Florian F. | last19=Dreizler | first19=Stefan
| last20=Jeffers | first20=Sandra V. | last21=Guenther | first21=E. W.
| last22=Henning | first22=Thomas K. | last23=Kaminski | first23=Adrian
| last24=Lafarga | first24=M. | last25=Marfil | first25=E.
| last26=Morales | first26=Juan Carlos | last27=Schmitt | first27=Jürgen H. M. M.
| last28=Seifert | first28=Walter | last29=Solano | first29=E.
| last30=Tabernero | first30=H. M. | last31=Zechmeister | first31=Mathias
| journal=Astronomy & Astrophysics
| volume=625 | id=A68 | pages=16 | date=May 2019
| arxiv=1904.03231 | bibcode=2019A&A...625A..68S
| doi=10.1051/0004-6361/201834965 | s2cid=102351979 }} or M3V{{citation
| title=Dwarf K and M stars of high proper motion found in a hemispheric survey
| last=Stephenson | first=C. B. | postscript=.
| journal=The Astronomical Journal
| volume=92 | pages=139–165 | date=July 1986
| bibcode=1986AJ.....92..139S | doi=10.1086/114146 | doi-access=free }}
| Mass = 0.39
| Radius = 0.42
| Temperature = 3562
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = The habitability of planets b and c is disputed.{{cite news | last=Sutherland | first=Paul | date=March 5, 2014 | title=Habitable planets common around red dwarf stars | url=http://sen.com/news/habitable-planets-common-around-red-dwarf-stars | website=Sen | publisher=Sen Corporation Ltd. | access-date=July 28, 2022 | archive-date=November 12, 2020 | archive-url=https://web.archive.org/web/20201112041601/https://www.sen.com/news/habitable-planets-common-around-red-dwarf-stars | url-status=live }}{{citation
| title=Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics
| display-authors=1 | last1=Tuomi | first1=Mikko
| last2=Jones | first2=Hugh R. A. | last3=Barnes | first3=John R.
| last4=Anglada-Escudé | first4=Guillem | last5=Jenkins | first5=James S.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=441 | issue=2 | pages=1545–1569 | year=2014
| doi=10.1093/mnras/stu358 | doi-access=free | arxiv=1403.0430 | postscript=.
| bibcode=2014MNRAS.441.1545T | s2cid=32965505 }}
}}
{{Multiplanetary systems list
| Star = HD 69830
| Constellation = Puppis
| Right ascension = {{RA|08|18|23.95}}
| Declination = {{DEC|−12|37|55.8}}
| Apparent magnitude = 5.95
| Distance = 41
| Spectral type = K0V
| Mass = 0.856
| Radius = 0.895
| Temperature = 5385
| Metallicity = −0.045
| Age = 7.446
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = A debris disk exterior to the three exoplanets was detected by the Spitzer Space Telescope in 2005.{{cite journal | title=An extrasolar planetary system with three Neptune-mass planets | url=http://obswww.unige.ch/~pernier/publications-www/articles-pdf-ps/2006Natur.441..305L.pdf | last1=Lovis | first1=Christophe | last2=Mayor | first2=Michel | last3=Pepe | first3=Francesco | last4=Alibert | first4=Yann | last5=Benz | first5=Willy | last6=Bouchy | first6=François | last7=Correia | first7=Alexandre C. M. | last8=Laskar | first8=Jacques | last9=Mordasini | first9=Christoph | last10=Queloz | first10=Didier | last11=Santos | first11=Nuno C. | last12=Udry | first12=Stéphane | last13=Bertaux | first13=Jean-Loup | last14=Sivan | first14=Jean-Pierre | display-authors=1 | journal=Nature | volume=441 | issue=7091 | pages=305–309 | date=2006 | arxiv=astro-ph/0703024 | bibcode=2006Natur.441..305L | doi=10.1038/nature04828 | pmid=16710412 | s2cid=4343578 | access-date=2022-02-24 | archive-date=2016-03-03 | archive-url=https://web.archive.org/web/20160303232248/http://obswww.unige.ch/~pernier/publications-www/articles-pdf-ps/2006Natur.441..305L.pdf | url-status=dead }}
}}
{{Multiplanetary systems list
| Star = HD 40307
| Constellation = Pictor
| Right ascension = {{RA|05|54|04.24}}
| Declination = {{DEC|−60|01|24.5}}
| Apparent magnitude = 7.17
| Distance = 42
| Spectral type = K2.5V
| Mass = 0.752
| Radius = 0.716
| Temperature = 4977
| Metallicity = −0.308
| Age = 1.198
| Confirmed planets = 4
|Unconfirmed planets = 2
| Notes = The existence of planets e and g are disputed.{{cite journal | title=The HARPS search for southern extra-solar planets. XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles | url=https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | last1=Díaz | first1=R. F. | last2=Ségransan | first2=D. | last3=Udry | first3=S. | last4=Lovis | first4=C. | last5=Pepe | first5=F. | last6=Dumusque | first6=X. | last7=Marmier | first7=M. | last8=Alonso | first8=R. | last9=Benz | first9=W. | last10=Bouchy | first10=F. | last11=Coffinet | first11=A. | last12=Collier Cameron | first12=A. | last13=Deleuil | first13=M. | last14=Figueira | first14=P. | last15=Gillon | first15=M. | last16=Lo Curto | first16=G. | last17=Mayor | first17=M. | last18=Mordasini | first18=C. | last19=Motalebi | first19=F. | last20=Moutou | first20=C. | last21=Pollacco | first21=D. | last22=Pompei | first22=E. | last23=Queloz | first23=D. | last24=Santos | first24=N. | last25=Wyttenbach | first25=A. | display-authors=1 | journal=Astronomy and Astrophysics | volume=585 | at=A134 | year=2016 | arxiv=1510.06446 | bibcode=2016A&A...585A.134D | doi=10.1051/0004-6361/201526729 | s2cid=118531921 | access-date=2022-02-24 | archive-date=2021-02-24 | archive-url=https://web.archive.org/web/20210224090311/https://www.aanda.org/articles/aa/full_html/2016/01/aa26729-15/aa26729-15.html | url-status=live }} If confirmed, planet g is potentially habitable.{{cite journal |doi=10.1051/0004-6361/201220268 |last1=Tuomi |first1=Mikko |last2=Anglada-Escudé |first2=Guillem |last3=Gerlach |first3=Enrico |last4=Jones |first4=Hugh R. A. |last5=Reiners |first5=Ansgar |last6=Rivera |first6=Eugenio J. |last7=Vogt |first7=Steven S. |last8=Butler |first8=R. Paul |title=Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307 |journal=Astronomy & Astrophysics |date=17 December 2012 |volume=549 |pages=A48 |arxiv=1211.1617 |bibcode=2013A&A...549A..48T |s2cid=7424216 }}
}}
{{Multiplanetary systems list
| Star = Upsilon Andromedae|Titawin
| Constellation = Andromeda (constellation){{!}}Andromeda
| Right ascension = {{RA|01|36|47.84}}
| Declination = {{DEC|+41|24|19.7}}
| Apparent magnitude = 4.09
| Distance = 44
| Spectral type = F8V
| Mass = 1.27
| Radius = 1.699
| Temperature = 6107
| Metallicity = 0.086
| Age = 3.781
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Nearest F-type main sequence star with a multiplanetary system. Second-brightest star in the night sky with a multiplanetary system after 7 Canis Majoris. All exoplanets orbit around star A in the binary system.
}}
{{Multiplanetary systems list
| Star = 47 Ursae Majoris|Chalawan
| Constellation = Ursa Major
| Right ascension = {{RA|10|59|27.97}}
| Declination = {{DEC|+40|25|48.9}}
| Apparent magnitude = 5.10
| Distance = 46
| Spectral type = G0V
| Mass = 1.029
| Radius = 1.241
| Temperature = 5892
| Metallicity = 0.003
| Age = 7.434
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Planet Taphao Thong was discovered in 1996 and was one of the first exoplanets to be discovered.
{{cite journal
| author=R. P. Butler
| title=A Planet Orbiting 47 Ursae Majoris
| journal=Astrophysical Journal Letters
| volume=464 | issue=2 | date=1996
| pages=L153–L156
| doi=10.1086/310102
| bibcode=1996ApJ...464L.153B
| last2=Marcy
| first2=Geoffrey W.
| doi-access=free
}} The planet was the first long-period extrasolar planet discovered. The other planets were discovered later.
{{cite journal
|author=P. C. Gregory
|author2=D. A. Fischer
|date=2010
|title=A Bayesian periodogram finds evidence for three planets in 47 Ursae Majoris
|journal=Monthly Notices of the Royal Astronomical Society
|volume=403 |issue=2 |pages=731–747
|doi=10.1111/j.1365-2966.2009.16233.x
|doi-access=free
|bibcode=2010MNRAS.403..731G
|arxiv = 1003.5549 |s2cid=16722873
}}
}}
{{Multiplanetary systems list
| Star = Nu2 Lupi
| Constellation = Lupus (constellation){{!}}Lupus
| Right ascension = {{RA|15|21|49.57}}
| Declination = {{DEC|−48|19|01.1}}
| Apparent magnitude = 5.65
| Distance = 47
| Spectral type = G2V
| Mass = 0.906
| Radius = 1.012
| Temperature = 5664
| Metallicity = -0.34
| Age = 10.36
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = One of the oldest stars in the solar neighbourhood.{{cite journal | title=Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog | last1=Takeda | first1=Genya |display-authors=etal | date=2007 | arxiv=astro-ph/0607235 | bibcode=2007ApJS..168..297T | doi=10.1086/509763 | volume=168 | journal=The Astrophysical Journal Supplement Series | issue=2 | pages=297–318| s2cid=18775378 }}{{cite journal | author=Sousa, S. G. | title=Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. Stellar [Fe/H] and the frequency of exo-Neptunes. | journal=Astronomy and Astrophysics | volume=487 | issue=1 |date=August 2008 | pages=373–381 | doi=10.1051/0004-6361:200809698 | bibcode=2008A&A...487..373S | display-authors=1 | last2=Santos | first2=N. C. | last3=Mayor | first3=M. | last4=Udry | first4=S. | last5=Casagrande | first5=L. | last6=Israelian | first6=G. | last7=Pepe | first7=F. | last8=Queloz | first8=D. | last9=Monteiro | first9=M. J. P. F. G. |arxiv = 0805.4826 | s2cid=18173201 }}{{cite arXiv | title=The HARPS search for southern extra-solar planets. XXXI. Magnetic activity cycles in solar-type stars: statistics and impact on precise radial velocities | last1=Lovis | first1=C. |display-authors=etal | date=2011 | class=astro-ph.SR | eprint=1107.5325}}
}}
{{Multiplanetary systems list
| Star = LHS 1140
| Constellation = Cetus (constellation){{!}}Cetus
| Right ascension = {{RA|00|44|59.31}}
| Declination = {{DEC|-15|16|16.7}}
| Apparent magnitude = 14.18
| Distance = 48.9
| Mass = 0.179
| Radius = 0.2139
| Temperature = 3216{{±|39}}
| Metallicity = -0.24
| Age = 5
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Planet b is a potentially habitable Super-Earth.{{cite news |last=Overbye |first=Dennis |author-link=Dennis Overbye |title=A new exoplanet may be most promising yet in search for life |url=https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |date=19 April 2017 |work=New York Times |access-date=20 April 2017 |archive-date=11 November 2020 |archive-url=https://web.archive.org/web/20201111202355/https://www.nytimes.com/2017/04/19/science/exoplanet-signs-of-life.html |url-status=live }}
}}
{{Multiplanetary systems list
| Star = Gliese 163
| Constellation = Dorado
| Right ascension = {{RA|04|09|16}}
| Declination = {{DEC|−53|22|25}}
| Apparent magnitude = 11.8
| Distance = 49
| Spectral type = M3.5V
| Mass = 0.4
| Radius =
| Temperature =
| Metallicity =
| Age = 3
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = Planet c is possibly a potentially habitable Super-Earth but is probably too hot or massive.{{cite web
| last=Méndez
| first=Abel
| date=August 29, 2012
| title=A Hot Potential Habitable Exoplanet around Gliese 163
| url=http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163
| publisher=University of Puerto Rico at Arecibo (Planetary Habitability Laboratory)
| accessdate=September 20, 2012
| archive-date=October 21, 2019
| archive-url=https://web.archive.org/web/20191021202448/http://phl.upr.edu/press-releases/ahotpotentialhabitableexoplanetaroundgliese163
| url-status=dead
| last=Redd
| first=Nola Taylor
| title=Newfound Alien Planet a Top Contender to Host Life
| url=http://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html
| date=September 20, 2012
| publisher=Space.com
| accessdate=September 20, 2012
| archive-date=December 26, 2019
| archive-url=https://web.archive.org/web/20191226102330/https://www.space.com/17684-alien-planet-gliese-163c-extraterrestrial-life.html
| url-status=live
}}
}}
{{Multiplanetary systems list
| Star = Mu Arae|Cervantes
| Constellation = Ara (constellation){{!}}Ara
| Right ascension = {{RA|17|44|08.70}}
| Declination = {{DEC|−51|50|02.6}}
| Apparent magnitude = 5.15
| Distance = 51
| Spectral type = G3IV-V
| Mass = 1.077
| Radius = 1.246
| Temperature = 5704
| Metallicity = 0.277
| Age = 6.413
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Planet Quijote orbits in the circumstellar habitable zone. However, it is a gas giant, so it itself is uninhabitable although a large moon orbiting around it may be habitable.
}}
{{Multiplanetary systems list
| Star = GJ 3929
| Constellation = Corona Borealis
| Right ascension = {{RA|15|58|18.8}}
| Declination = {{DEC|35|24|24.3}}
| Apparent magnitude = 12.67
| Distance = 51.58
| Spectral type = M3.5V
| Mass = 0.313
| Radius = 0.32
| Temperature = 3384
| Metallicity = -0.02
| Age =
| Confirmed planets = 2
|Unconfirmed planets = 0
| Notes = {{Cite web |title=Simbad - Object view |url=https://simbad.cds.unistra.fr/mobile/object.html?object_name=G%20180-18 |access-date=2024-01-04 |website=simbad.cds.unistra.fr}}{{Cite journal |last1=Beard |first1=Corey |last2=Robertson |first2=Paul |last3=Kanodia |first3=Shubham |last4=Lubin |first4=Jack |last5=Cañas |first5=Caleb I. |last6=Gupta |first6=Arvind F. |last7=Holcomb |first7=Rae |last8=Jones |first8=Sinclaire |last9=Libby-Roberts |first9=Jessica E. |last10=Lin |first10=Andrea S. J. |last11=Mahadevan |first11=Suvrath |last12=Stefánsson |first12=Guđmundur |last13=Bender |first13=Chad F. |last14=Blake |first14=Cullen H. |last15=Cochran |first15=William D. |date=2022-08-30 |title=GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion |journal=The Astrophysical Journal |volume=936 |issue=1 |pages=55 |doi=10.3847/1538-4357/ac8480 |doi-access=free |arxiv=2207.10672 |bibcode=2022ApJ...936...55B |issn=0004-637X}}
}}
{{Multiplanetary systems list
| Star = Gliese 676 A
| Constellation = Ara (constellation){{!}}Ara
| Right ascension = {{RA|17|30|11.2042}}
| Declination = {{DEC|-51|38|13.116}}
| Apparent magnitude = 9.59
| Distance = 53
| Spectral type = M0V
| Mass = 0.71
| Radius =
| Temperature =
| Metallicity = 0.23
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Held the record for widest range of masses in a planetary system in 2012.{{cite journal
|last=Anglada-Escudé
|first=Guillem
|author2=Tuomi, Mikko
|date=2012
|title=A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems
|arxiv=1206.7118
|bibcode=2012A&A...548A..58A
|doi=10.1051/0004-6361/201219910
|volume=548
|journal=Astronomy
|pages=A58
|s2cid=17115882
|url=http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9595/aa19910-12.pdf?sequence=2
}}{{Dead link|date=February 2024 |bot=InternetArchiveBot |fix-attempted=yes }}
}}
{{Multiplanetary systems list
| Star = HD 7924
| Constellation = Cassiopeia (constellation){{!}}Cassiopeia
| Right ascension = {{RA|01|21|59.12}}
| Declination = {{DEC|+76|42|37.0}}
| Apparent magnitude = 7.19
| Distance = 55
| Spectral type = K0V
| Mass = 0.832
| Radius = 0.78
| Temperature = 5177
| Metallicity = -0.15
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = These planets may be potentially habitable Super-Earths.{{cite journal
| title=Three Super-Earths Orbiting HD 7924
| last1=Fulton | first1=Benjamin J. | last2=Weiss | first2=Lauren M.
| last3=Sinukoff | first3=Evan | last4=Isaacson | first4=Howard
| last5=Howard | first5=Andrew W. | last6=Marcy | first6=Geoffrey W.
| last7=Henry | first7=Gregory W. | last8=Holden | first8=Bradford P.
| last9=Kibrick | first9=Robert I. | display-authors=1
| journal=The Astrophysical Journal
| volume=805 | issue=2 | pages=175 | year=2015
| arxiv=1504.06629 | bibcode=2015ApJ...805..175F
| doi=10.1088/0004-637X/805/2/175 | s2cid=7969255 }}
}}
{{Multiplanetary systems list
| Star = Pi Mensae
| Constellation = Mensa_(constellation){{!}}Mensa
| Right ascension = {{RA|05|37|09.8851}}
| Declination = {{DEC|−80|28|08.8313}}
| Apparent magnitude = 5.65
| Distance = 59.62{{±|0.07}}
| Spectral type = G0V
| Mass = 1.11
| Radius = 1.15
| Temperature = 6013
| Metallicity = 0.09
| Age = 3.4
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Outer planet is likely a brown dwarf.{{citation|arxiv=2007.06410|title=A precise architecture characterization of the π Mensae planetary system|year=2020|doi=10.1051/0004-6361/202038416|last1=Damasso|first1=M.|last2=Sozzetti|first2=A.|last3=Lovis|first3=C.|last4=Barros|first4=S. C. C.|last5=Sousa|first5=S. G.|last6=Demangeon|first6=O. D. S.|last7=Faria|first7=J. P.|last8=Lillo-Box|first8=J.|last9=Cristiani|first9=S.|last10=Pepe|first10=F.|last11=Rebolo|first11=R.|last12=Santos|first12=N. C.|last13=Zapatero Osorio|first13=M. R.|last14=González Hernández|first14=J. I.|last15=Amate|first15=M.|last16=Pasquini|first16=L.|last17=Zerbi|first17=F. M.|last18=Adibekyan|first18=V.|last19=Abreu|first19=M.|last20=Affolter|first20=M.|last21=Alibert|first21=Y.|last22=Aliverti|first22=M.|last23=Allart|first23=R.|last24=Allende Prieto|first24=C.|last25=Álvarez|first25=D.|last26=Alves|first26=D.|last27=Avila|first27=G.|last28=Baldini|first28=V.|last29=Bandy|first29=T.|last30=Benz|first30=W.|journal=Astronomy & Astrophysics|volume=642|pages=A31|bibcode=2020A&A...642A..31D|s2cid=220496034|display-authors=1}}
}}
{{Multiplanetary systems list
| Star = Gliese 3293
| Constellation = Eridanus (constellation){{!}}Eridanus
| Right ascension = {{RA|04|28|35.72}}
| Declination = {{DEC|-25|10|08.9}}
| Apparent magnitude = 11.96
| Distance = 59
| Spectral type = M2.5V
| Mass = 0.42
| Radius = 0.40±0.03
| Temperature = 3466±49
| Metallicity = 0.02±0.09
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Planets b and d orbit in the habitable zone.{{cite journal
|doi = 10.1051/0004-6361/201630153
|last1 = Astudillo-Defru
|first1 = Nicola
|last2 = Forveille
|first2 = Thierry
|last3 = Bonfils
|first3 = Xavier
|last4 = Ségransan
|first4 = Damien
|last5 = Bouchy
|first5 = François
|last6 = Delfosse
|first6 = Xavier
|last7 = Lovis
|first7 = Christophe
|last8 = Mayor
|first8 = Michel
|last9 = Murgas
|first9 = Felipe
|last10 = Pepe
|first10 = Francesco
|last11 = Santos
|first11 = Nuno C.
|last12 = Udry
|first12 = Stéphane
|last13 = Wünsche
|first13 = Anaël
|display-authors = 6
|year = 2017
|title = The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293
|journal = Astronomy and Astrophysics
|volume = 602
|at = A88
|arxiv = 1703.05386
|bibcode = 2017A&A...602A..88A
|s2cid = 119418595
|url = https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|access-date = 2022-02-25
|archive-date = 2022-09-28
|archive-url = https://web.archive.org/web/20220928032005/https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html
|url-status = live
}}
}}
{{Multiplanetary systems list
| Star = LHS 1678
| Constellation = Caelum
| Right ascension = {{Ra|04|32|43}}
| Declination = {{Dec|-39|47|21}}
| Apparent magnitude = 12
| Distance = 64.8
| Spectral type = M2V
| Mass = 0.345
| Radius = 0.329
| Temperature = 3490
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 0
}}
{{Multiplanetary systems list
| Star = HD 104067
| Constellation = Corvus (constellation){{!}}Corvus
| Right ascension = {{RA|11|59|10.0}}
| Declination = {{DEC|-20|21|13.6}}
| Apparent magnitude = 7.92
| Distance = 66.3
| Spectral type = K3V
| Mass = 0.82
| Radius = 0.77
| Temperature = 4942
| Metallicity = 0.11
| Age = 4.8
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = The innermost planet, which is unconfirmed, might suffer from significant tidal heating.{{cite journal |last1=Kane |first1=Stephen R. |last2=Fetherolf |first2=Tara |display-authors=etal |date=March 2024 |title=A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World |journal=The Astronomical Journal |volume= 167|issue= 5|page=239 |doi= 10.3847/1538-3881/ad3820|doi-access=free |arxiv=2403.17062|bibcode=2024AJ....167..239K }}
}}
{{Multiplanetary systems list
| Star = HD 142
| Constellation = Phoenix (constellation){{!}}Phoenix
| Right ascension = {{RA|00|06|19.0}}
| Declination = {{DEC|-49|04|30}}
| Apparent magnitude = 5.70
| Distance = 67
| Spectral type = G1 IV
| Mass = 1.1
| Radius = 0.86
| Temperature = 6180
| Metallicity = 0.04
| Age = 5.93
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 215152
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|43|21}}
| Declination = {{DEC|-06|24|03}}
| Apparent magnitude = 8.13
| Distance = 70
| Spectral type = G8IV
| Mass = 1.019
| Radius = 1.080
| Temperature = 5646
| Metallicity = 0.367
| Age = 7.320
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 164922
| Constellation = Hercules (constellation){{!}}Hercules
| Right ascension = {{RA|18|02|30.86}}
| Declination = {{DEC|+26|18|46.8}}
| Apparent magnitude = 7.01
| Distance = 72
| Mass = 0.874
| Radius = 0.999
| Temperature = 5293
| Metallicity = 0.16
| Age = 13.4
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Oldest star with a multiplanetary system. Despite its age, it is more metal-rich than the Sun.
}}
{{Multiplanetary systems list
| Star = HD 63433
| Constellation = Gemini (constellation){{!}}Gemini
| Right ascension = {{RA|07|49|55.0}}
| Declination = {{DEC|+27|21|47.4}}
| Apparent magnitude = 6.92
| Distance = 73
| Spectral type = G5V
| Mass = 0.99
| Radius = 0.912
| Temperature =5640
| Metallicity = 0.03
| Age = 0.4
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = HIP 57274
| Constellation = Ursa Major
| Right ascension = {{RA|11|44|41}}
| Declination = {{DEC|+30|57|33}}
| Apparent magnitude = 8.96
| Distance = 85
| Spectral type = K5V
| Mass = 0.73
| Radius = 0.68
| Temperature = 4640
| Metallicity = 0.09
| Age = 7.87
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 39194
| Constellation = Mensa (constellation){{!}}Mensa
| Right ascension = {{RA|05|44|32}}
| Declination = {{DEC|-70|08|37}}
| Apparent magnitude = 8.08
| Distance = 86.2
| Spectral type = K0V
| Mass =
| Radius =
| Temperature =5205
| Metallicity =-0.61
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = LP 791-18
| Constellation = Crater
| Right ascension = {{RA|11|02|45.95}}
| Declination = {{DEC|-16|24|22.3}}
| Apparent magnitude = 16.9
| Distance = 86.9
| Spectral type = M6V/M7V
| Mass = 0.139
| Radius = 0.17
| Temperature =2960
| Metallicity =-0.09
| Age = 0.5
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = HD 181433
| Constellation = Pavo (constellation){{!}}Pavo
| Right ascension = {{RA|19|25|09.57}}
| Declination = {{DEC|−66|28|07.7}}
| Apparent magnitude = 8.38
| Distance = 87
| Spectral type = K5V
| Mass = 0.777
| Radius = 0.786
| Temperature = 4962
| Metallicity = 0.327
| Age = 8.974
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 134606
| Constellation = Apus
| Right ascension = {{RA|15|15|15}}
| Declination = {{DEC|-70|31|11}}
| Apparent magnitude = 6.85
| Distance = 87
| Spectral type = G6IV
| Mass =
| Radius =
| Temperature =
| Metallicity =
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = The planets have moderately eccentric orbits.{{citation
| first1=M. | last1=Mayor | first2=M. | last2=Marmier
| first3=C. | last3=Lovis | first4=S. | last4=Udry
| first5=D. | last5=Ségransan | first6=F. | last6=Pepe
| first7=W. | last7=Benz | first8=J.-L. | last8=Bertaux
| first9=F. | last9=Bouchy | first10=X. | last10=Dumusque
| first11=G. | last11=Lo Curto | first12=C. | last12=Mordasini
| first13=D. | last13=Queloz | first14=N. C. | last14=Santos
| title=The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets
| date=September 13, 2011 | arxiv=1109.2497 }}
}}
{{Multiplanetary systems list
| Star = HD 158259
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|17|25|24.0}}
| Declination = {{DEC|+52|47|26}}
| Apparent magnitude = 6.46
| Distance = 89
| Spectral type = G0
| Mass = 1.08
| Radius = 1.21
| Temperature =
| Metallicity =
| Age =
| Confirmed planets = 5
|Unconfirmed planets = 1
| Notes = A G-type star slightly more massive than the Sun.{{cite journal|last1=Hara|first1=N. C.|last2=Bouchy|first2=F.|last3=Stalport|first3=M.|last4=Boisse|first4=I.|last5=Rodrigues|first5=J.|last6=Delisle|first6=J. B.|last7=Santerne|first7=A.|last8=Henry|first8=G. W.|last9=Arnold|first9=L.|last10=Astudillo-Defru|first10=N.|last11=Borgniet|first11=S.|last12=Bonfils|first12=X.|last13=Bourrier|first13=V.|last14=Brugger|first14=B.|last15=Courcol|first15=B.|last16=Dalal|first16=S.|last17=Deleuil|first17=M.|last18=Delfosse|first18=X.|last19=Demangeon|first19=O.|last20=Díaz|first20=R. F.|last21=Dumusque|first21=X.|last22=Forveille|first22=T.|last23=Hébrard|first23=G.|last24=Hobson|first24=M. J.|last25=Kiefer|first25=F.|last26=Lopez|first26=T.|last27=Mignon|first27=L.|last28=Mousis|first28=O.|last29=Moutou|first29=C.|last30=Pepe|first30=F.|last31=Rey|first31=J.|last32=Santos|first32=N. C.|last33=Ségransan|first33=D.|last34=Udry|first34=S.|last35=Wilson|first35=P. A.|title=The SOPHIE search for northern extrasolar planets XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain|date=March 10, 2020|journal=Astronomy & Astrophysics|volume=636|issue=1|page=L6|doi=10.1051/0004-6361/201937254|arxiv=1911.13296|bibcode=2020A&A...636L...6H|s2cid=208512859}} Planet g remains unconfirmed.
}}
{{Multiplanetary systems list
| Star = HD 82943
| Constellation = Hydra (constellation){{!}}Hydra
| Right ascension = {{RA|09|34|50.74}}
| Declination = {{DEC|−12|07|46.4}}
| Apparent magnitude = 6.54
| Distance = 90
| Spectral type = F9V Fe+0.5{{citation | display-authors=1 | last1=Gray | first1=R. O. | last2=Corbally | first2=C. J. | last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T. | last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E. | last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R. | title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | journal=The Astronomical Journal | volume=132 | issue=1 | pages=161–170 |date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | s2cid=119476992 }}
| Mass = 1.175
| Radius = 1.124
| Temperature = 5874
| Metallicity = 0.273
| Age = 3.080
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Planets b and c are in a 2:1 orbital resonance.{{cite journal | title=On the 2:1 Orbital Resonance in the HD 82943 Planetary System | last1=Lee | first1=Man Hoi | last2=Butler | first2=R. Paul | last3=Fischer | first3=Debra A. | last4=Marcy | first4=Geoffrey W. | last5=Vogt | first5=Steven S. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=641 | issue=2 | pages=1178–1187 | arxiv=astro-ph/0512551 | bibcode=2006ApJ...641.1178L | doi=10.1086/500566 | s2cid=119432579 }} Planet b orbits in the habitable zone, but it and planet c are massive enough to be brown dwarfs. HD 82943 has an unusual lithium-6 abundance.{{cite press release | title=The Harsh Destiny of a Planet? | date=May 9, 2001 | publisher=European Southern Observatory | location=Garching, Germany | url=http://www.eso.org/public/news/eso0118/ | access-date=December 30, 2012 | archive-date=September 21, 2020 | archive-url=https://web.archive.org/web/20200921074543/https://www.eso.org/public/news/eso0118/ | url-status=live }}
}}
{{Multiplanetary systems list
| Star = Gliese 3138
| Constellation = Cetus (constellation){{!}}Cetus
| Right ascension = {{RA|02|09|10.90}}
| Declination = {{DEC|-16|20|22.53}}
| Apparent magnitude = 10.877
| Distance = 92.9
| Spectral type =
| Mass = 0.681
| Radius =
| Temperature = 3717{{±|49}}
| Metallicity = -0.30
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = GJ 9827
| Constellation = Pisces (constellation){{!}}Pisces
| Right ascension = {{RA|23|27|04.84}}
| Declination = {{DEC|−01|17|10.59}}
| Apparent magnitude = 10.10
| Distance = 96.8{{±|0.2}}
| Spectral type = K6V
| Mass = 0.593
| Radius = 0.579
| Temperature = 4294{{±|52}}
| Metallicity = -0.26
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Also known as K2-135. Planet b is extremely dense, with at least half of its mass being iron.{{cite journal | bibcode=2018AJ....155...72R | doi=10.3847/1538-3881/aaa292 | arxiv=1709.01957| title=A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc| journal=The Astronomical Journal| volume=155| issue=2| pages=72| year=2018| last1=Rodriguez| first1=Joseph E| last2=Vanderburg| first2=Andrew| last3=Eastman| first3=Jason D| last4=Mann| first4=Andrew W| last5=Crossfield| first5=Ian J. M| last6=Ciardi| first6=David R| last7=Latham| first7=David W| last8=Quinn| first8=Samuel N| s2cid=55459523 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = K2-239
| Constellation = Sextans{{!}}Sextans
| Right ascension = {{RA|10|42|22.63}}
| Declination = {{DEC|+04|26|28.86}}
| Apparent magnitude = 14.5
| Distance = 101.5
| Spectral type = M3V
| Mass = 0.40
| Radius = 0.36
| Temperature = 3420
| Metallicity = -0.1
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = TOI-700
| Constellation = Dorado (constellation){{!}}Dorado
| Right ascension = {{RA|06|28|22.97}}
| Declination = {{DEC|−65|34|43.01}}
| Apparent magnitude = 13.10
| Distance = 101.61
| Spectral type = M2V
| Mass = 0.416
| Radius = 0.42
| Temperature = 3480
| Metallicity = -0.07
| Age = 1.5
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Planets d and e are potentially habitable.{{cite news |last1=Andreolo |first1=Claire |last2=Cofield |first2=Calla |last3=Kazmierczak |first3=Jeanette |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.jpl.nasa.gov/news/news.php?feature=7569 |date=6 January 2020 |work=NASA |access-date=6 January 2020 |archive-date=14 April 2020 |archive-url=https://web.archive.org/web/20200414070820/https://www.jpl.nasa.gov/news/news.php?feature=7569 |url-status=live }}{{cite news |last1=Garner |first1=Rob |title=NASA Planet Hunter Finds Earth-Size Habitable-Zone World |url=https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |date=6 January 2020 |work=NASA |access-date=6 January 2020 |archive-date=5 April 2020 |archive-url=https://web.archive.org/web/20200405004715/https://www.nasa.gov/feature/goddard/2020/nasa-planet-hunter-finds-its-1st-earth-size-habitable-zone-world |url-status=live }}{{cite news |last=Wall |first=Mike |title=NASA's TESS Planet Hunter Finds Its 1st Earth-Size World in 'Habitable Zone' |url=https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |date=6 January 2020 |work=Space.com |access-date=6 January 2020 |archive-date=8 April 2020 |archive-url=https://web.archive.org/web/20200408031443/https://www.space.com/nasa-tess-first-earth-size-habitable-exoplanet-toi-700d.html |url-status=live }}
}}
{{Multiplanetary systems list
| Star = HD 17926
| Constellation = Fornax
| Right ascension = {{RA|02|51|56.16}}
| Declination = {{DEC|−30|48|53.2}}
| Apparent magnitude = 6.38
| Distance = 105
| Spectral type = F6V
| Mass = 1.145
| Radius = 1.31
| Temperature = 6201
| Metallicity = -0.14
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = The star forms a binary with a red dwarf.{{cite journal
| title=TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR 858
| journal=The Astrophysical Journal | volume=881 | issue=1 | pages=L19 | last1=Vanderburg | first1=Andrew | last2=Huang | first2=Chelsea X.
| last3=Rodriguez | first3=Joseph E. | last4=Becker | first4=Juliette C.
| last5=Ricker | first5=George R. | last6=Vanderspek | first6=Roland K.
| last7=Latham | first7=David W. | last8=Seager | first8=Sara
| last9=Winn | first9=Joshua N. | last10=Jenkins | first10=Jon M.
| last11=Addison | first11=Brett | last12=Bieryla | first12=Allyson
| last13=Briceño | first13=Cesar | last14=Bowler | first14=Brendan P.
| last15=Burke | first15=Christopher J. | last16=Burt | first16=Jennifer A.
| last17=Caldwell | first17=Douglas A. | last18=Clark | first18=Jake T.
| last19=Crossfield | first19=Ian | last20=Dittmann | first20=Jason A.
| last21=Dynes | first21=Scott | last22=Guerrero | first22=Natalia
| last23=Horner | first23=Jonathan | last24=Kane | first24=Stephen R.
| last25=Kielkopf | first25=John | last26=Kraus | first26=Adam L.
| last27=Law | first27=Nicolas | last28=Mann | first28=Andrew W.
| last29=Mengel | first29=Matthew W. | last30=Morton | first30=Timothy D.
| display-authors=1 | year=2019
| arxiv=1905.05193 | doi=10.3847/2041-8213/ab322d | bibcode=2019ApJ...881L..19V | s2cid=153311715 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = HD 37124
| Constellation = Taurus (constellation){{!}}Taurus
| Right ascension = {{RA|05|37|02.49}}
| Declination = {{DEC|+20|43|50.8}}
| Apparent magnitude = 7.68
| Distance = 110
| Spectral type = G4V
| Mass = 0.830
| Radius = 0.824
| Temperature = 5606
| Metallicity = −0.442
| Age = 3.327
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 20781
| Constellation = Fornax
| Right ascension = {{RA|03|20|03}}
| Declination = {{DEC|-28|47|02}}
| Apparent magnitude = 8.44
| Distance = 115
| Spectral type = G9.5V
| Mass = 0.7
| Radius =
| Temperature =5256±29
| Metallicity =−0.11
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
|Notes= Located in binary star system.{{citation|arxiv=1705.05153|title=The HARPS search for southern extra-solar planets. XLII. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions|year=2019|doi=10.1051/0004-6361/201731173|last1=Udry|first1=S.|last2=Dumusque|first2=X.|last3=Lovis|first3=C.|last4=Segransan|first4=D.|last5=Diaz|first5=R. F.|last6=Benz|first6=W.|last7=Bouchy|first7=F.|last8=Coffinet|first8=A.|last9=Lo Curto|first9=G.|last10=Mayor|first10=M.|last11=Mordasini|first11=C.|last12=Motalebi|first12=F.|last13=Pepe|first13=F.|last14=Queloz|first14=D.|last15=Santos|first15=N. C.|last16=Wyttenbach|first16=A.|last17=Alonso|first17=R.|last18=Collier Cameron|first18=A.|last19=Deleuil|first19=M.|last20=Figueira|first20=P.|last21=Gillon|first21=M.|last22=Moutou|first22=C.|last23=Pollacco|first23=D.|last24=Pompei|first24=E.|journal=Astronomy & Astrophysics|volume=A37|page=622|bibcode=2019A&A...622A..37U|s2cid=119095511}}{{cite arXiv|eprint=1109.2497|class=astro-ph|title=The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets|author=Mayor, M.|author2=Marmier, M.|author3=Lovis, C.|author4=Udry, S.|author5=Ségransan, D.|author6=Pepe, F.|author7=Benz, W.|author8=Bertaux, J.-L.|author9=Bouchy, F.|author10=Dumusque, G.|author11=Curto, Lo|author12=Mordasini, C.|author13=Queloz, D.|author14=Santos, N. C.|date=2011|display-authors=etal}}
}}
{{Multiplanetary systems list
| Star = Kepler-444
| Constellation = Lyra
| Right ascension = {{RA|19|19|01}}
| Declination = {{DEC|41|38|05}}
| Apparent magnitude = 9.0
| Distance = 117
| Spectral type = K0V
| Mass = 0.758
| Radius = 0.752
| Temperature = 5040
| Metallicity = -0.55
| Age = 11.23
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = Nearest multiplanetary system where the planets were discovered by the Kepler space telescope.
}}
{{Multiplanetary systems list
| Star = HD 141399
| Constellation = Boötes
| Right ascension = {{RA|15|46|54.0}}
| Declination = {{DEC|+46|59|11}}
| Apparent magnitude = 7.2
| Distance = 118
| Spectral type = K0V
| Mass = 1.07
| Radius = 1.46
| Temperature = 5600
| Metallicity = 0.35
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-42
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|28|53}}
| Declination = {{DEC|+44|37|10}}
| Apparent magnitude = 16.12
| Distance = 126
| s2cid=14889361}}
| Mass = 0.13
| Radius = 0.17
| Temperature = 3068
| Metallicity = -0.48
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 31527
| Constellation = Lepus
| Right ascension = {{RA|04|55|38}}
| Declination = {{DEC|-23|14|31}}
| Apparent magnitude = 7.48
| Distance = 126
| Spectral type = G0V
| Mass =
| Radius =
| Temperature =
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 10180
| Constellation = Hydrus
| Right ascension = {{RA|01|37|53.58}}
| Declination = {{DEC|−60|30|41.5}}
| Apparent magnitude = 7.33
| Distance = 127
| Spectral type = G1V
| Mass = 1.055
| Radius = 1.085
| Temperature = 5911
| Metallicity = 0.083
| Age = 4.335
| Confirmed planets = 6
|Unconfirmed planets = 3
| Notes = Has three unconfirmed candidates. If these candidate exoplanets were confirmed, HD 10180 would have the largest planetary system of any star.{{cite journal|last=Tuomi|first=Mikko|title=Evidence for 9 planets in the 10180 system|journal=Astronomy & Astrophysics|volume=543|pages=A52|date=6 April 2012|arxiv=1204.1254v1|doi=10.1051/0004-6361/201118518|bibcode = 2012A&A...543A..52T |s2cid=15876919}}
}}
{{Multiplanetary systems list
| Star = HD 23472
| Constellation = Reticulum{{!}}Reticulum
| Right ascension = {{RA|03|41|50.3988}}
| Declination = {{DEC|-62|46|01.4772}}
| Apparent magnitude = 9.72
| Distance = 127.48
| Spectral type = K3.5V
| Mass = 0.67
| Radius = 0.71
| Temperature = 4684{{±|99}}
| Metallicity = -0.2
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = HR 8799
| Constellation = Pegasus
| Right ascension = {{RA|23|07|28.72}}
| Declination = {{DEC|+21|08|03.3}}
| Apparent magnitude = 5.96
| Distance = 129
| Spectral type = A5V
| Mass = 1.472
| Radius = 1.339
| Temperature = 7429
| Metallicity = −0.466
| Age = 0.064
| Confirmed planets = 4
|Unconfirmed planets = 1
| Notes = Only A-type main sequence star with a known multiplanetary system, and hottest and most massive single main sequence star with a multiplanetary system. All four planets are massive super-Jupiters.
}}
{{Multiplanetary systems list
| Star = HD 27894
| Constellation = Reticulum
| Right ascension = {{RA|04|20|47.05}}
| Declination = {{DEC|−59|24|39.0}}
| Apparent magnitude = 9.42
| Distance = 138
| Spectral type = K2V
| Mass = 0.8
| Radius =
| Temperature = 4875
| Metallicity = 0.3
| Age = 3.9
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 93385
| Constellation = Vela (constellation){{!}}Vela
| Right ascension = {{RA|10|46|15.1160}}
| Declination = {{DEC|-41|27|51.7261}}
| Apparent magnitude = 7.486
| Distance = 141.6
| Spectral type = G2V
| Mass = 1.07
| Radius = 1.17
| Temperature = 5823
| Metallicity = -0.05
| Age = 4.13
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-3
| Constellation = Leo (constellation){{!}}Leo
| Right ascension = {{RA|11|29|20.3918}}
| Declination = {{DEC|-01|27|17.280}}
| Apparent magnitude = 12.168
| Distance = 143.9{{±|0.4}}
| Spectral type = M0V
| Mass = 0.601
| Radius = 0.561±0.068
| Temperature = 3835±70
| Metallicity = -0.01±0.09
| Age = 1
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = The outermost planet orbits in the habitable zone.{{Cite web |url=http://www.sci-news.com/astronomy/science-three-super-earths-red-dwarf-02412.html |title=Three Super-Earths Found Circling Nearby Red Dwarf |access-date=2022-02-27 |archive-date=2019-01-02 |archive-url=https://web.archive.org/web/20190102064436/http://www.sci-news.com/astronomy/science-three-super-earths-red-dwarf-02412.html |url-status=live }}
}}
{{Multiplanetary systems list
| Star = HD 34445
| Constellation = Orion (constellation){{!}}Orion
| Right ascension = {{RA|05|17|41.0}}
| Declination = {{DEC|+07|21|12}}
| Apparent magnitude = 7.31
| Distance = 152
| Spectral type = G0V
| Mass = 1.07
| Radius = 1.38
| Temperature = 5836
| Metallicity = 0.14
| Age = 8.5
| Confirmed planets = 1
|Unconfirmed planets = 5
}}
{{Multiplanetary systems list
| Star = HD 204313
| Constellation = Capricornus
| Right ascension = {{RA|21|28|12.21}}
| Declination = {{DEC|–21|43|34.5}}
| Apparent magnitude = 7.99
| Distance = 154
| Spectral type = G5V
| Mass = 1.045
| Radius =
| Temperature = 5767
| Metallicity = 0.18
| Age = 3.38
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 3167
| Constellation = Pisces (constellation){{!}}Pisces
| Right ascension = {{RA|00|34|57.5}}
| Declination = {{DEC|+04|22|53}}
| Apparent magnitude = 8.97
| Distance = 154.4
| Spectral type = K0V
| Mass = 0.852
| Radius = 0.871
| Temperature = 5300
| Metallicity = 0.04
| Age = 10.2
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HIP 34269
| Constellation = Puppis (constellation){{!}}Puppis
| Right ascension = {{RA|07|06|13.98}}
| Declination = {{DEC|-47|35|13.87}}
| Apparent magnitude = 10.59
| Distance = 154.81
| Spectral type =
| Mass = 0.74
| Radius =
| Temperature = 4440{{±|100}}
| Metallicity =
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = HD 133131
| Constellation = Libra (constellation){{!}}Libra
| Right ascension = {{RA|15|03|35.80651}}
| Declination = {{DEC|-27|50|27.5520}}
| Apparent magnitude = 8.4
| Distance = 168
| Mass = 0.95
| Radius =
| Temperature = 5799±19
| Metallicity = -0.3
| Age = 6
| Confirmed planets = 3
|Unconfirmed planets =
|Notes = 2 planets around primary, and 1 planet around secondary star.{{cite journal|bibcode=2016AJ....152..167T|doi=10.3847/0004-6256/152/6/167|arxiv=1608.06216|title=The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B|journal=The Astronomical Journal|volume=152|issue=6|pages=167|year=2016|last1=Teske|first1=Johanna K|last2=Shectman|first2=Stephen A|last3=Vogt|first3=Steve S|last4=Díaz|first4=Matías|last5=Butler|first5=R. Paul|last6=Crane|first6=Jeffrey D|last7=Thompson|first7=Ian B|last8=Arriagada|first8=Pamela|s2cid=118852162 |doi-access=free }}
}}
{{Multiplanetary systems list
| Star = K2-136
| Constellation = Taurus (constellation){{!}}Taurus
| Right ascension = {{RA|04|29|38.99}}
| Declination = {{DEC|+22|52|57.80}}
| Apparent magnitude = 11.2
| Distance = 173
| Spectral type = K5V
| Mass = 0.71
| Radius = 0.71
| Temperature = 4364{{±|70}}
| Metallicity = 0.15
| Age = 0.7
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = HIP 14810
| Constellation = Aries (constellation){{!}}Aries
| Right ascension = {{RA|03|11|14.23}}
| Declination = {{DEC|+21|05|50.5}}
| Apparent magnitude = 8.51
| Distance = 174
| Spectral type = G5V
| Mass = 0.989
| Radius = 1.024
| Temperature = 5485
| Metallicity = 0.230
| Age = 5.271
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 191939
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|20|08|05.75}}
| Declination = {{DEC|+66|51|2.1}}
| Apparent magnitude = 8.971
| Distance = 175
| Spectral type = G9V
| Mass = 0.81
| Radius = 0.94
| Temperature = 5348
| Metallicity = -0.15
| Age = 8.7
| Confirmed planets = 6
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 125612
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|14|20|53.51}}
| Declination = {{DEC|−17|28|53.5}}
| Apparent magnitude = 8.33
| Distance = 177
| Spectral type = G3V
| Mass = 1.099
| Radius = 1.052
| Temperature = 5897
| Metallicity = 0.244
| Age = 2.150
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 184010
| Constellation = Vulpecula
| Right ascension = {{RA|19|31|22.0}}
| Declination = {{DEC|+26|37|02}}
| Apparent magnitude = 5.9
| Distance = 200
| Spectral type = KOIII-IV
| Mass = 1.35
| Radius = 4.86
| Temperature = 4971
| Metallicity = -0.17
| Age = 2.76
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 109271
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|12|33|36.0}}
| Declination = {{DEC|-11|37|19}}
| Apparent magnitude = 8.05
| Distance = 202
| Spectral type = G5
| Mass = 1.047
| Radius =
| Temperature = 5783
| Metallicity = 0.1
| Age = 7.3
| Confirmed planets = 2
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = HD 38677
| Constellation = Orion (constellation){{!}}Orion
| Right ascension = {{RA|05|47|06.0}}
| Declination = {{DEC|−10|37|49″}}
| Apparent magnitude = 8.0
| Distance = 202
| Spectral type = F8V
| Mass = 1.21
| Radius = 1.26
| Temperature = 6196.0
| Metallicity =
| Age = 2.01
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = TOI-178
| Constellation = Sculptor (constellation){{!}}Sculptor
| Right ascension = {{RA|00|29|12.30}}
| Declination = {{DEC|30|27|13.46}}
| Apparent magnitude = 11.95
| Distance = 205.16
| Mass = 0.65
| Radius = 0.651
| Temperature = 4316{{±|70}}
| Metallicity = -0.23
| Age = 7.1
| Confirmed planets = 6
|Unconfirmed planets =
| Notes = The planets are in an orbital resonance.
}}
{{Multiplanetary systems list
| Star = HD 108236
| Constellation = Centaurus
| Right ascension = {{RA|12|26|17.89}}
| Declination = {{DEC|-51|21|46.21}}
| Apparent magnitude = 9.24
| Distance = 211
| Spectral type = G3V
| Mass = 0.97
| Radius = 0.888
| Temperature = 5730
| Metallicity = -0.3
| Age = 5.8
| Confirmed planets = 5
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-37
| Constellation = Lyra
| Right ascension = {{RA|18|58|23.1}}
| Declination = {{DEC|44|31|05}}
| Apparent magnitude = 9.77
| Distance = 215
| Spectral type = G8V
| Mass = 0.803
| Radius = 0.770
| Temperature = 5417
| Metallicity = −0.32
| Age = 6
| Confirmed planets = 3
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = K2-72
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|18|29.2548}}
| Declination = {{DEC|-09|36|44.3824}}
| Apparent magnitude = 15.04
| Distance = 217
| Spectral type = M2V
| Mass = 0.27
| Radius = 0.33
| Temperature = 3497
| Metallicity = -0.271
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = 2 planets in habitable zone
}}
{{Multiplanetary systems list
| Star = Kepler-138
| Constellation = Lyra
| Right ascension = {{RA|19|21|32.0}}
| Declination = {{DEC|+43|17|35}}
| Apparent magnitude = 13.5
| Distance = 218.5
| Spectral type = M1V
| Mass = 0.57
| Radius = 0.54
| Temperature = 3871
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-233
| Constellation = Libra (constellation){{!}}Libra
| Right ascension = {{RA|15|21|55.2}}
| Declination = {{DEC|-20|13|54}}
| Apparent magnitude = 10.0
| Distance = 221
| Spectral type = K3
| Mass = 0.80
| Radius = 0.74
| Temperature = 4950
| Metallicity = 0.07
| Age = 0.36
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = TOI-1260
| Constellation = Ursa Major
| Right ascension = {{RA|10|28|35.03}}
| Declination = {{DEC|+65|51|16.38}}
| Apparent magnitude = 11.973
| Distance = 239.5
| Spectral type =
| Mass = 0.66
| Radius = 0.672
| Temperature = 4227{{±|85}}
| Metallicity = -0.1
| Age = 6.7
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = LP 358-499
| Constellation = Taurus (constellation){{!}}Taurus
| Right ascension = {{RA|04|40|35.64}}
| Declination = {{DEC|+25|00|36.05}}
| Apparent magnitude = 13.996
| Distance = 245.3
| Spectral type =
| Mass = 0.46
| Radius =
| Temperature = 3655{{±|80}}
| Metallicity =
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Also known as K2-133
}}
{{Multiplanetary systems list
| Star = K2-266
| Constellation = Sextans{{!}}Sextans
| Right ascension = {{RA|10|31|44.5}}
| Declination = {{DEC|+00|56|15}}
| Apparent magnitude =
| Distance = 252
| Spectral type = K
| Mass = 0.69
| Radius = 0.7
| Temperature = 4285
| Metallicity = -0.12
| Age = 8.4
| Confirmed planets = 4
|Unconfirmed planets = 2
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-155
| Constellation = Taurus (constellation){{!}}Taurus
| Right ascension = {{RA|04|21|52.5}}
| Declination = {{DEC|+21|21|13}}
| Apparent magnitude = 12.8
| Distance = 267
| Spectral type = K7
| Mass = 0.65
| Radius = 0.58
| Temperature = 4258
| Metallicity = -0.3
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-384
| Constellation = Cetus (constellation){{!}}Cetus
| Right ascension = {{RA|01|21|59.86}}
| Declination = {{DEC|00|45|04.41}}
| Apparent magnitude = 16.12
| Distance = 270
| Spectral type = M?V
| Mass = 0.33
| Radius =
| Temperature = 3623{{±|138}}
| Metallicity =
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = TOI-1136
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|12|48|44.38 }}
| Declination = {{DEC|+64|51|18.99}}
| Apparent magnitude = 9.534
| Distance = 275.8
| Spectral type =
| Mass = 1.022
| Radius = 0.968
| Temperature = 5770{{±|50}}
| Metallicity = 0.07
| Age = 0.7
| Confirmed planets = 6
|Unconfirmed planets = 1
| Notes = The planets are in an orbital resonance.{{cite journal |last1=Dai |first1=Fei |last2=Masuda |first2=Kento |display-authors=etal |date=February 2023 |title=TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain |journal=The Astronomical Journal |volume=165 |issue=2 |page=33 |doi=10.3847/1538-3881/aca327 |doi-access=free |arxiv=2210.09283 |bibcode=2023AJ....165...33D}}
}}
{{Multiplanetary systems list
| Star = TOI-561
| Constellation = Sextans (constellation){{!}}Sextans
| Right ascension = {{RA|09|52|44.44}}
| Declination = {{DEC|+06|12|57.97}}
| Apparent magnitude = 10.252
| Distance = 279
| Spectral type = G9V
| Mass = 0.785
| Radius = 0.849
| Temperature = 5455
| Metallicity = -0.33
| Age = 5
| Confirmed planets = 4
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = Kepler-445
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|54|57.0}}
| Declination = {{DEC|+46|29|55}}
| Apparent magnitude = 18
| Distance = 294
| Spectral type =
| Mass = 0.18
| Radius = 0.21
| Temperature = 3157
| Metallicity = 0.19
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = TOI-763
| Constellation = Centaurus (constellation){{!}}Centaurus
| Right ascension = {{RA|12|57|52.45}}
| Declination = {{DEC|−39|45|27.71}}
| Apparent magnitude = 10.156
| Distance = 311
| Spectral type =
| Mass = 0.917
| Radius = 0.897
| Temperature = 5444
| Metallicity = 0.01
| Age = 6.2
| Confirmed planets = 2
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = K2-229
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|12|27|29.5848}}
| Declination = {{DEC|−06|43|18.7660}}
| Apparent magnitude = 10.985
| Distance = 335
| Spectral type = K2V
| Mass = 0.837
| Radius = 0.793
| Temperature = 5185
| Metallicity = −0.06
| Age = 5.4
| Confirmed planets = 3
|Unconfirmed planets =
|Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-102
| Constellation = Lyra
| Right ascension = {{RA|18|45|55.9}}
| Declination = {{DEC|+47|12|29}}
| Apparent magnitude = 11.492
| Distance = 340
| Spectral type = K3V{{cite simbad|title=KOI-82|access-date=20 March 2022}}
| Mass = 0.81
| Radius = 0.76
| Temperature = 4809
| Metallicity = 0.18
| Age = 1.41
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = V1298 Tauri
| Constellation = Taurus (constellation){{!}}Taurus
| Right ascension = {{RA|04|05|19.5912}}
| Declination = {{DEC|+20|09|25.5635}}
| Apparent magnitude = 10.31
| Distance = 354
| Mass = 1.101
| Radius = 1.345
| Temperature = 4970
| Metallicity =
| Age = 0.023
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = This star is a young T Tauri variable.{{Cite journal|last1=David|first1=Trevor J.|last2=Petigura|first2=Erik A.|last3=Luger|first3=Rodrigo|last4=Foreman-Mackey|first4=Daniel|last5=Livingston|first5=John H.|last6=Mamajek|first6=Eric E.|last7=Hillenbrand|first7=Lynne A.|date=2019-10-29|title=Four Newborn Planets Transiting the Young Solar Analog V1298 Tau|journal=The Astrophysical Journal|volume=885|issue=1|pages=L12|arxiv=1910.04563|bibcode=2019ApJ...885L..12D|doi=10.3847/2041-8213/ab4c99|s2cid=204008446|issn=2041-8213 |doi-access=free }}
}}
{{Multiplanetary systems list
| Star = K2-302
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|20|22.7764}}
| Declination = {{DEC|-09|30|34.2934}}
| Apparent magnitude = 11.98
| Distance = 359.3
| Spectral type =
| Mass =
| Radius = 0.25
| Temperature = 3297{{±|73}}
| Metallicity = -0.33
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
|Notes =
}}
{{Multiplanetary systems list
| Star = K2-198
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|13|15|22.5}}
| Declination = {{DEC|-06|27|54}}
| Apparent magnitude = 11.0
| Distance = 362
| Spectral type =
| Mass = 0.8
| Radius = 0.76
| Temperature = 5213
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = TOI-125
| Constellation = Hydrus{{!}}Hydrus
| Right ascension = {{RA|01|34|22.73}}
| Declination = {{DEC|-66|40|32.95}}
| Apparent magnitude = 11.02
| Distance = 363
| Spectral type =
| Mass = 0.859
| Radius =
| Temperature = 5320
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 2
| Notes =
}}
{{Multiplanetary systems list
| Star = HIP 41378
| Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|08|26|28.0}}
| Declination = {{DEC|+10|04|49}}
| Apparent magnitude = 8.9
| Distance = 378
| Spectral type = F8
| Mass = 1.15
| Radius = 1.4
| Temperature = 6199
| Metallicity = -0.11
| Age =
| Confirmed planets = 5
|Unconfirmed planets = 2
| Notes = Planet f has an unusually low density, and might have rings or an extended atmosphere.{{Cite journal|last1=Akinsanmi|first1=B.|last2=Santos|first2=N. C.|last3=Faria|first3=J. P.|last4=Oshagh|first4=M.|last5=Barros|first5=S. C. C.|last6=Santerne|first6=A.|last7=Charnoz|first7=S.|date=2020-03-01|title=Can planetary rings explain the extremely low density of HIP 41378 𝑓?|url=https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|journal=Astronomy & Astrophysics|language=en|volume=635|pages=L8|doi=10.1051/0004-6361/202037618|arxiv=2002.11422|issn=0004-6361|doi-access=free|access-date=2022-03-19|archive-date=2021-10-28|archive-url=https://web.archive.org/web/20211028001745/https://www.aanda.org/articles/aa/abs/2020/03/aa37618-20/aa37618-20.html|url-status=live}}{{cite arXiv|eprint=1911.07355|last1=Santerne|first1=A.|title=An extremely low-density and temperate giant exoplanet|last2=Malavolta|first2=L.|last3=Kosiarek|first3=M. R.|last4=Dai|first4=F.|last5=Dressing|first5=C. D.|last6=Dumusque|first6=X.|last7=Hara|first7=N. C.|last8=Lopez|first8=T. A.|last9=Mortier|first9=A.|last10=Vanderburg|first10=A.|last11=Adibekyan|first11=V.|last12=Armstrong|first12=D. J.|last13=Barrado|first13=D.|last14=Barros|first14=S. C. C.|last15=Bayliss|first15=D.|last16=Berardo|first16=D.|last17=Boisse|first17=I.|last18=Bonomo|first18=A. S.|last19=Bouchy|first19=F.|last20=Brown|first20=D. J. A.|last21=Buchhave|first21=L. A.|last22=Butler|first22=R. P.|last23=Collier Cameron|first23=A.|last24=Cosentino|first24=R.|last25=Crane|first25=J. D.|last26=Crossfield|first26=I. J. M.|last27=Damasso|first27=M.|last28=Deleuil|first28=M. R.|last29=Delgado Mena|first29=E.|last30=Demangeon|first30=O.|display-authors=29|class=astro-ph.EP|year=2019}} More planets are still suspected.{{Cite journal| author = Andrew Vanderburg|display-authors=etal
| author-link =
| arxiv =1606.08441
| title =Five Planets Transiting a Ninth Magnitude Star
| journal =The Astrophysical Journal
| volume =827
| issue =1
| pages =L10
| language =en
| year =2016
| doi =10.3847/2041-8205/827/1/L10
| bibcode =2016ApJ...827L..10V
|s2cid=8794583
|doi-access=free
}}
}}
{{Multiplanetary systems list
| Star = Kepler-446
| Constellation = Lyra
| Right ascension = {{RA|18|49|00.0}}
| Declination = {{DEC|+44|55|16}}
| Apparent magnitude = 16.5
| Distance = 391
| Spectral type = M4V
| Mass = 0.22
| Radius = 0.24
| Temperature = 3359
| Metallicity = -0.3
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = HD 33142
| Constellation = Lepus (constellation){{!}}Lepus
| Right ascension = {{RA|05|07|35.54}}
| Declination = {{DEC|-13|59|11.34}}
| Apparent magnitude = 7.96
| Distance = 394.3
| Spectral type =
| Mass = 1.52
| Radius =
| Temperature = 5025{{±|24|16}}
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Host star is
a giant star with spectral type of K0III.{{Cite web |last=Martin |first=Pierre-Yves |date=2022 |title=Planet HD 33142 c |url=https://exoplanet.eu/catalog/hd_33142_c--6882/ |access-date=2024-02-03 |website=exoplanet.eu |language=en |archive-date=2024-02-03 |archive-url=https://web.archive.org/web/20240203050836/https://exoplanet.eu/catalog/hd_33142_c--6882/ |url-status=live }}
}}
{{Multiplanetary systems list
| Star = WASP-132
| Constellation = Lupus (constellation){{!}}Lupus
| Right ascension = {{RA|14|30|26.2}}
| Declination = {{DEC|-46|09|33}}
| Apparent magnitude = 11.938
| Distance = 403
| Spectral type = K4V
| Mass = 0.782
| Radius = 0.753
| Temperature = 4714
| Metallicity = 0.18
| Age = 7.2
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-148
| Constellation = Cetus (constellation){{!}}Cetus
| Right ascension = {{RA|00|58|04.28}}
| Declination = {{DEC|-00|11|35.36}}
| Apparent magnitude = 13.05
| Distance = 407
| Spectral type = K7V
| Mass = 0.65
| Radius = 0.63
| Temperature = 4079{{±|70}}
| Metallicity = -0.11
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-68
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|24|07.76}}
| Declination = {{DEC|+49|02|25.0}}
| Apparent magnitude = 8.588
| Distance = 440
| Spectral type = G1V
| Mass = 1.079
| Radius = 1.243
| Temperature = 5793
| Metallicity = 0.12
| Age = 6.3
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes = Planet d, the outermost confirmed planet, is a Jupiter-sized planet which orbits in the habitable zone.{{cite journal | title=Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants | last1=Gilliland | first1=Ronald L. | last2=Marcy | first2=Geoffrey W. | last3=Rowe | first3=Jason F. | last4=Rogers | first4=Leslie | last5=Torres | first5=Guillermo | last6=Fressin | first6=Francois | last7=Lopez | first7=Eric D. | last8=Buchhave | first8=Lars A. | last9=Christensen-Dalsgaard | first9=Jørgen | last10=Désert | first10=Jean-Michel | last11=Henze | first11=Christopher E. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Lissauer | first14=Jack J. | last15=Chaplin | first15=William J. | last16=Basu | first16=Sarbani | last17=Metcalfe | first17=Travis S. | last18=Elsworth | first18=Yvonne | last19=Handberg | first19=Rasmus | last20=Hekker | first20=Saskia | last21=Huber | first21=Daniel | last22=Karoff | first22=Christoffer | last23=Kjeldsen | first23=Hans | last24=Lund | first24=Mikkel N. | last25=Lundkvist | first25=Mia | last26=Miglio | first26=Andrea | last27=Charbonneau | first27=David | last28=Ford | first28=Eric B. | last29=Fortney | first29=Jonathan J. | last30=Haas | first30=Michael R. | display-authors=1 | journal=The Astrophysical Journal | volume=766 | issue=1 | at=40 | year=2013 | arxiv=1302.2596 | bibcode=2013ApJ...766...40G | bibcode-access=free | doi=10.1088/0004-637X/766/1/40 | doi-access=free }} Radial velocity measurements discovered an additional signal, which could be a fourth planet or a stellar companion.{{cite journal | title=Long-period Giant Companions to Three Compact, Multiplanet Systems | last1=Mills | first1=Sean M. | last2=Howard | first2=Andrew W. | last3=Weiss | first3=Lauren M. | last4=Steffen | first4=Jason H. | last5=Isaacson | first5=Howard | last6=Fulton | first6=Benjamin J. | last7=Petigura | first7=Erik A. | last8=Kosiarek | first8=Molly R. | last9=Hirsch | first9=Lea A. | last10=Boisvert | first10=John H. | display-authors=1 | journal=The Astronomical Journal | volume=157 | issue=4 | at=145 | year=2019 | arxiv=1903.07186 | bibcode=2019AJ....157..145M | doi=10.3847/1538-3881/ab0899 | s2cid=119197547 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = HD 28109
| Constellation = Hydrus (constellation){{!}}Hydrus
| Right ascension = {{RA|04|20|57.13}}
| Declination = {{DEC|-68|06|09.51}}
| Apparent magnitude = 9.38
| Distance = 457
| Spectral type =
| Mass = 1.26
| Radius =
| Temperature = 6120{{±|50}}
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = COROT-7
| Constellation = Monoceros
| Right ascension = {{RA|06|43|49.47}}
| Declination = {{DEC|−01|03|46.9}}
| Apparent magnitude = 11.73
| Distance = 489
| Spectral type = K0V
| Mass = 0.93
| Radius = 0.87
| Temperature = 5275
| Metallicity = 0.03
| Age = 1.5
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = XO-2
| Constellation = Lynx (constellation){{!}}Lynx
| Right ascension = {{RA|07|48|07.4814}}
| Declination = {{DEC|+50|13|03.2578}}
| Apparent magnitude = 11.18
| Distance = 496±3
| Spectral type = K0V+K0V
| Mass =
| Radius =
| Temperature =
| Metallicity =
| Age = 6.3
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Binary with each star orbited by two planets.{{cite journal | title=The GAPS programme with HARPS-N at TNG. IV. A planetary system around XO-2S | url=https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | last1=Desidera | first1=S. | last2=Bonomo | first2=A. S. | last3=Claudi | first3=R. U. | last4=Damasso | first4=M. | last5=Biazzo | first5=K. | last6=Sozzetti | first6=A. | last7=Marzari | first7=F. | last8=Benatti | first8=S. | last9=Gandolfi | first9=D. | last10=Gratton | first10=R. | last11=Lanza | first11=A. F. | last12=Nascimbeni | first12=V. | last13=Andreuzzi | first13=G. | last14=Affer | first14=L. | last15=Barbieri | first15=M. | last16=Bedin | first16=L. R. | last17=Bignamini | first17=A. | last18=Bonavita | first18=M. | last19=Borsa | first19=F. | last20=Calcidese | first20=P. | last21=Christille | first21=J. M. | last22=Cosentino | first22=R. | last23=Covino | first23=E. | last24=Esposito | first24=M. | last25=Giacobbe | first25=P. | last26=Harutyunyan | first26=A. | last27=Latham | first27=D. | last28=Lattanzi | first28=M. | last29=Leto | first29=G. | last30=Lodato | first30=G. | display-authors=1 | journal=Astronomy and Astrophysics | volume=567 | issue=6 | at=L6 | year=2014 | arxiv=1407.0251 | bibcode=2014A&A...567L...6D | doi=10.1051/0004-6361/201424339 | s2cid=118567085 | access-date=2022-06-25 | archive-date=2021-05-11 | archive-url=https://web.archive.org/web/20210511170517/https://www.aanda.org/articles/aa/full_html/2014/07/aa24339-14/aa24339-14.html | url-status=live }}{{cite journal | title=A comprehensive analysis of the XO-2 stellar and planetary systems | last1=Damasso | first1=M. | last2=Biazzo | first2=K. | last3=Bonomo | first3=A. S. | last4=Desidera | first4=S. | last5=Lanza | first5=A. F. | last6=Nascimbeni | first6=V. | last7=Esposito | first7=M. | last8=Scandariato | first8=G. | last9=Sozzetti | first9=A. | last10=Cosentino | first10=R. | last11=Gratton | first11=R. | last12=Malavolta | first12=L. | last13=Rainer | first13=M. | last14=Gandolfi | first14=D. | last15=Poretti | first15=E. | last16=Zanmar Sanchez | first16=R. | last17=Ribas | first17=I. | last18=Santos | first18=N. | last19=Affer | first19=L. | last20=Andreuzzi | first20=G. | last21=Barbieri | first21=M. | last22=Bedin | first22=L. R. | last23=Benatti | first23=S. | last24=Bernagozzi | first24=A. | last25=Bertolini | first25=E. | last26=Bonavita | first26=M. | last27=Borsa | first27=F. | last28=Borsato | first28=L. | last29=Boschin | first29=W. | last30=Calcidese | first30=P. | last31=Carbognani | first31=A. | last32=Cenadelli | first32=D. | last33=Christille | first33=J. M. | last34=Claudi | first34=R. U. | last35=Covino | first35=E. | last36=Cunial | first36=A. | last37=Giacobbe | first37=P. | last38=Granata | first38=V. | last39=Harutyunyan | first39=A. | last40=Lattanzi | first40=M. G. | last41=Leto | first41=G. | last42=Libralato | first42=M. | last43=Lodato | first43=G. | last44=Lorenzi | first44=V. | last45=Mancini | first45=L. | last46=Martinez Fiorenzano | first46=A. F. | last47=Marzari | first47=F. | last48=Masiero | first48=S. | last49=Micela | first49=G. | last50=Molinari | first50=E. | last51=Molinaro | first51=M. | last52=Munari | first52=U. | last53=Murabito | first53=S. | last54=Pagano | first54=I. | last55=Pedani | first55=M. | last56=Piotto | first56=G. | last57=Rosenberg | first57=A. | last58=Silvotti | first58=R. | last59=Southworth | first59=J. | display-authors=1 | journal=Astronomy & Astrophysics | volume=575 | at=A111 | year=2015 | doi=10.1051/0004-6361/201425332 | doi-access=free | arxiv=1501.01424 }}
}}
{{Multiplanetary systems list
| Star = Kepler-411
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|10|25.3}}
| Declination = {{DEC|+49|31|24}}
| Apparent magnitude = 12.5
| Distance = 499.4
| Spectral type = K3V
| Mass = 0.83
| Radius = 0.79
| Temperature = 4974
| Metallicity = 0.23
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-381
| Constellation = Sagittarius (constellation){{!}}Sagittarius
| Right ascension = {{RA|19|12|06.46}}
| Declination = {{DEC|-21|00|27.51}}
| Apparent magnitude = 13.01
| Distance = 505
| Spectral type = K2
| Mass = 0.754
| Radius =
| Temperature = 4473{{±|138}}
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-285
| Constellation = Pisces (constellation){{!}}Pisces
| Right ascension = {{RA|23|17|32.2}}
| Declination = {{DEC|+01|18|01}}
| Apparent magnitude = 12.03
| Distance = 508
| Spectral type = K2V
| Mass = 0.83
| Radius = 0.79
| Temperature = 4975
| Metallicity =
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-32
| Constellation = Ophiuchus (constellation){{!}}Ophiuchus
| Right ascension = {{RA|16|49|42.2602}}
| Declination = {{DEC|−19|32|34.151}}
| Apparent magnitude = 12.31
| Distance = 510
| Spectral type = G9V
| Mass = 0.856
| Radius = 0.845
| Temperature = 5275
| Metallicity = -0.02
| Age = 7.9
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = TOI-1246
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|16|44|27.96}}
| Declination = {{DEC|70|25|46.70}}
| Apparent magnitude = 11.6
| Distance = 558
| Spectral type =
| Mass = 1.12
| Radius =
| Temperature = 5217{{±|50}}
| Metallicity =
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-352
| Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|09|21|46.8434}}
| Declination = {{DEC|+18|28|10.34710}}
| Apparent magnitude = 11.12
| Distance = 577
| Spectral type = G2V
| Mass = 0.98
| Radius = 0.95
| Temperature = 5791
| Metallicity = -0.05
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-398
| Constellation = Lyra
| Right ascension = {{RA|19|25|52.5}}
| Declination = {{DEC|+40|20|38}}
| Apparent magnitude =
| Distance = 578
| Spectral type = K5V
| Mass = 0.72
| Radius = 0.67
| Temperature = 4493
| Metallicity = -0.046
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-186
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|54|36.6}}
| Declination = {{DEC|+43|57|18}}
| Mass = 0.478
| Radius = 0.472
| Temperature = 3788
| Metallicity = -0.28
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = Planet f is the first Earth-size exoplanet discovered that orbits in the habitable zone.{{Cite journal| doi = 10.1126/science.1249403| title = An Earth-Sized Planet in the Habitable Zone of a Cool Star| journal = Science| volume = 344| issue = 6181| pages = 277–280| date = 2014-04-18| arxiv=1404.5667| last1 = Quintana | first1 = E. V.| last2 = Barclay | first2 = T.| last3 = Raymond | first3 = S. N.| last4 = Rowe | first4 = J. F.| last5 = Bolmont | first5 = E.| last6 = Caldwell | first6 = D. A.| last7 = Howell | first7 = S. B.| last8 = Kane | first8 = S. R.| last9 = Huber | first9 = D.| last10 = Crepp | first10 = J. R.| last11 = Lissauer | first11 = J. J. | author-link11=Jack J. Lissauer| last12 = Ciardi | first12 = D. R.| last13 = Coughlin | first13 = J. L.| last14 = Everett | first14 = M. E.| last15 = Henze | first15 = C. E.| last16 = Horch | first16 = E.| last17 = Isaacson | first17 = H.| last18 = Ford | first18 = E. B.| last19 = Adams | first19 = F. C.| last20 = Still | first20 = M.| last21 = Hunter | first21 = R. C.| last22 = Quarles | first22 = B.| last23 = Selsis | first23 = F.|bibcode = 2014Sci...344..277Q | pmid=24744370| s2cid = 1892595}} free version = http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf {{Webarchive|url=https://web.archive.org/web/20140418183443/http://www.nasa.gov/sites/default/files/files/kepler186_main_final.pdf |date=2014-04-18 }}
}}
{{Multiplanetary systems list
| Star = K2-37
| Constellation = Scorpius (constellation){{!}}Scorpius
| Right ascension = {{RA|16|13|48.2445}}
| Declination = {{DEC|-24|47|13.4279}}
| Apparent magnitude = 12.52
| Distance = 590
| Spectral type = G3V
| Mass = 0.9
| Radius = 0.85
| Temperature = 5413
| Metallicity = -0.03
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-58
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|15|17.2364}}
| Declination = {{DEC|-14|02|59.3151}}
| Apparent magnitude = 12.13
| Distance = 596
| Spectral type = K2V
| Mass = 0.89
| Radius = 0.86
| Temperature = 5038
| Metallicity = 0.25
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-138
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|23|15|47.77}}
| Declination = {{DEC|-10|50|58.91}}
| Apparent magnitude = 12.21
| Distance = 597{{±|55}}
| Spectral type = K1V
| Mass = 0.93
| Radius = 0.86
| Temperature = 5378±60
| Metallicity = +0.16 ± 0.04
| Age = 2.3
| Confirmed planets = 6
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = K2-38
| Constellation = Scorpius
| Right ascension = {{RA|16|00|08.06}}
| Declination = {{DEC|-23|11|21.33}}
| Apparent magnitude = 11.34
| Distance = 630
| Spectral type = G3V
| Mass = 1.03
| Radius = 1.10
| Temperature = 5731{{±|66}}
| Metallicity = 0.28
| Age =
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Dust disk in system
}}
{{Multiplanetary systems list
| Star = WASP-47
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|04|49.0}}
| Declination = {{DEC|-12|01|08}}
| Apparent magnitude = 11.9
| Distance = 652
| Spectral type = G9V
| Mass = 1.084
| Radius = 1.15
| Temperature = 5400
| Metallicity = 0.18
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = One planet is a gas giant which orbits in the habitable zone.{{Cite journal|last1=Becker|first1=Juliette C.|last2=Vanderburg|first2=Andrew|last3=Adams|first3=Fred C.|last4=Rappaport|first4=Saul A.|last5=Schwengeler|first5=Hans Martin|title=Wasp-47: A Hot Jupiter System with Two Additional Planets Discovered by K2|date=2015-10-12|journal=The Astrophysical Journal|language=en|volume=812|issue=2|pages=L18|doi=10.1088/2041-8205/812/2/L18|issn=2041-8213|arxiv=1508.02411|bibcode=2015ApJ...812L..18B|s2cid=14681933}}{{cite journal | title=Hot Jupiters with relatives: Discovery of additional planets in orbit around WASP-41 and WASP-47 | url=https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | last1=Neveu-VanMalle | first1=M. | last2=Queloz | first2=D. | last3=Anderson | first3=D. R. | last4=Brown | first4=D. J. A. | last5=Collier Cameron | first5=A. | last6=Delrez | first6=L. | last7=Díaz | first7=R. F. | last8=Gillon | first8=M. | last9=Hellier | first9=C. | last10=Jehin | first10=E. | last11=Lister | first11=T. | last12=Pepe | first12=F. | last13=Rojo | first13=P. | last14=Ségransan | first14=D. | last15=Triaud | first15=A. H. M. J. | last16=Turner | first16=O. D. | last17=Udry | first17=S. | display-authors=1 | journal=Astronomy and Astrophysics | volume=586 | at=A93 | year=2016 | arxiv=1509.07750 | bibcode=2016A&A...586A..93N | doi=10.1051/0004-6361/201526965 | s2cid=53354547 | access-date=2022-05-08 | archive-date=2022-02-28 | archive-url=https://web.archive.org/web/20220228025245/https://www.aanda.org/articles/aa/full_html/2016/02/aa26965-15/aa26965-15.html | url-status=live }} WASP-47 is the only planetary system known to have both planets near the hot Jupiter and another planet much further out.{{cite web|url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|title=WASP-47|website=exoplanetarchive.ipac.caltech.edu|access-date=2022-05-08|archive-date=2022-05-08|archive-url=https://web.archive.org/web/20220508114227/https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=WASP-47&type=PLANET_HOST|url-status=live}}
}}
{{Multiplanetary systems list
| Star = K2-368
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|10|32.58}}
| Declination = {{DEC|-11|09|58.02}}
| Apparent magnitude = 13.54
| Distance = 674
| Spectral type = K3
| Mass = 0.746
| Radius =
| Temperature = 4663{{±|138}}
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes =
}}
{{Multiplanetary systems list
| Star = HAT-P-13
| Constellation = Ursa Major
| Right ascension = {{RA|08|39|31.81}}
| Declination = {{DEC|+47|21|07.3}}
| Apparent magnitude = 10.62
| Distance = 698
| Spectral type = G4
| Mass = 1.22
| Radius = 1.56
| Temperature = 5638
| Metallicity = 0.43
| Age = 5
| Confirmed planets = 2
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = Kepler-19
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|21|41}}
| Declination = {{DEC|+37|51|06}}
| Apparent magnitude = 15.178
| Distance = 717
| Spectral type = G
| Mass = 0.936
| Radius = 0.85
| Temperature = 5541
| Metallicity = -0.13
| Age = 1.9
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-296
| Constellation = Lyra
| Right ascension = {{RA|19|06|09.6}}
| Declination = {{DEC|+49|26|14.4}}
| Apparent magnitude = 12.6
| Distance = 737.113
| Mass =
| Radius = 0.557
| Temperature = 4249
| Metallicity = 0.168
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = All planets orbit around the primary star. Planets e and f are potentially habitable.{{cite journal|bibcode=2015ApJ...809....7B|doi=10.1088/0004-637X/809/1/7|arxiv=1505.01845|title=The Five Planets in the Kepler-296 Binary System All Orbit the Primary: A Statistical and Analytical Analysis|journal=The Astrophysical Journal|volume=809|pages=7|year=2015|last1=Barclay|first1=Thomas|last2=Quintana|first2=Elisa V|last3=Adams|first3=Fred C|last4=Ciardi|first4=David R|last5=Huber|first5=Daniel|last6=Foreman-Mackey|first6=Daniel|last7=Montet|first7=Benjamin T|last8=Caldwell|first8=Douglas|issue=1|s2cid=37742564}}
}}
{{Multiplanetary systems list
| Star = Kepler-454
| Constellation = Lyra
| Right ascension = {{RA|19|09|55.0}}
| Declination = {{DEC|+38|13|44}}
| Apparent magnitude = 11.57
| Distance = 753
| Spectral type = G
| Mass = 1.028
| Radius = 1.066
| Temperature = 5687
| Metallicity = 0.32
| Age = 5.25
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-25
| Constellation = Lyra
| Right ascension = {{RA|19|06|33.0}}
| Declination = {{DEC|+39|29|16}}
| Apparent magnitude = 11
| Distance = 799
| Spectral type = F{{citation
|first1=Jean
|last1=Schneider
|title=Star: Kepler-25
|url=http://exoplanet.eu/star.php?st=Kepler-25
|access-date=2013-12-18
|url-status=dead
|archive-url=https://web.archive.org/web/20120616125118/http://exoplanet.eu/star.php?st=Kepler-25
|encyclopedia=Extrasolar Planets Encyclopaedia
|archive-date=2012-06-16
}}
| Mass = 1.22
| Radius = 1.36
| Temperature = 6190
| Metallicity = 0.01
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Two planets were discovered by transit-timing variations,{{cite journal | title=Transit timing observations from Kepler - III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations | last1=Steffen | first1=Jason H. | last2=Fabrycky | first2=Daniel C. | last3=Ford | first3=Eric B. | last4=Carter | first4=Joshua A. | last5=Désert | first5=Jean-Michel | last6=Fressin | first6=Francois | last7=Holman | first7=Matthew J. | last8=Lissauer | first8=Jack J. | last9=Moorhead | first9=Althea V. | last10=Rowe | first10=Jason F. | last11=Ragozzine | first11=Darin | last12=Welsh | first12=William F. | last13=Batalha | first13=Natalie M. | last14=Borucki | first14=William J. | last15=Buchhave | first15=Lars A. | last16=Bryson | first16=Steve | last17=Caldwell | first17=Douglas A. | last18=Charbonneau | first18=David | last19=Ciardi | first19=David R. | last20=Cochran | first20=William D. | last21=Endl | first21=Michael | last22=Everett | first22=Mark E. | last23=Gautier | first23=Thomas N. | last24=Gilliland | first24=Ron L. | last25=Girouard | first25=Forrest R. | last26=Jenkins | first26=Jon M. | last27=Horch | first27=Elliott | last28=Howell | first28=Steve B. | last29=Isaacson | first29=Howard | last30=Klaus | first30=Todd C. | display-authors=1 | journal=Monthly Notices of the Royal Astronomical Society | volume=421 | issue=3 | pages=2342–2354 | year=2012 | arxiv=1201.5412 | bibcode=2012MNRAS.421.2342S | bibcode-access=free | doi=10.1111/j.1365-2966.2012.20467.x | doi-access=free }} and the third planet was discovered by follow-up radial velocity measurements.{{cite journal | title=Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets | last1=Marcy | first1=Geoffrey W. | last2=Isaacson | first2=Howard | last3=Howard | first3=Andrew W. | last4=Rowe | first4=Jason F. | last5=Jenkins | first5=Jon M. | last6=Bryson | first6=Stephen T. | last7=Latham | first7=David W. | last8=Howell | first8=Steve B. | last9=Gautier | first9=Thomas N. | last10=Batalha | first10=Natalie M. | last11=Rogers | first11=Leslie | last12=Ciardi | first12=David | last13=Fischer | first13=Debra A. | last14=Gilliland | first14=Ronald L. | last15=Kjeldsen | first15=Hans | last16=Christensen-Dalsgaard | first16=Jørgen | last17=Huber | first17=Daniel | last18=Chaplin | first18=William J. | last19=Basu | first19=Sarbani | last20=Buchhave | first20=Lars A. | last21=Quinn | first21=Samuel N. | last22=Borucki | first22=William J. | last23=Koch | first23=David G. | last24=Hunter | first24=Roger | last25=Caldwell | first25=Douglas A. | last26=Van Cleve | first26=Jeffrey | last27=Kolbl | first27=Rea | last28=Weiss | first28=Lauren M. | last29=Petigura | first29=Erik | last30=Seager | first30=Sara | display-authors=1 | journal=The Astrophysical Journal Supplement Series | volume=210 | issue=2 | at=20 | year=2014 | arxiv=1401.4195 | bibcode=2014ApJS..210...20M | bibcode-access=free | doi=10.1088/0067-0049/210/2/20 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Kepler-114
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|36|29.0}}
| Declination = {{DEC|+48|20|58}}
| Apparent magnitude = 13.7
| Distance = 846
| Spectral type = K
| Mass = 0.71
| Radius = 0.65
| Temperature = 4450
| Metallicity = -0.003
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-54
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|39|06.0}}
| Declination = {{DEC|+43|03|23}}
| Apparent magnitude = 16.3
| Distance = 886
| Spectral type = M
| Mass = 0.52
| Radius = 0.55
| Temperature = 3705
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-20
| Constellation = Lyra
| Right ascension = {{RA|19|10|47.524}}
| Declination = {{DEC|42|20|19.30}}
| Apparent magnitude = 12.51
| Distance = 950
| Spectral type = G8V
| Mass = 0.912
| Radius = 0.944
| Temperature = 5466
| Metallicity = 0.02
| Age = 8.8
| Confirmed planets = 6
|Unconfirmed planets =
| Notes = Planets e and f were the first Earth-sized planets to be discovered.{{cite journal |last=Hand |first=Eric |title=Kepler discovers first Earth-sized exoplanets |doi=10.1038/nature.2011.9688 |date=20 December 2011 |journal=Nature|s2cid=122575277 }}
}}
{{Multiplanetary systems list
| Star = K2-19
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|11|39|50.4804}}
| Declination = {{DEC|+00|36|12.8773}}
| Apparent magnitude = 13.002
| Distance = 976
| Spectral type = K0V{{cite journal | title=Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations | url=https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | last1=Nespral | first1=D. | last2=Gandolfi | first2=D. | last3=Deeg | first3=H. J. | last4=Borsato | first4=L. | last5=Fridlund | first5=M. C. V. | last6=Barragán | first6=O. | last7=Alonso | first7=R. | last8=Grziwa | first8=S. | last9=Korth | first9=J. | last10=Albrecht | first10=S. | last11=Cabrera | first11=J. | last12=Csizmadia | first12=Sz. | last13=Nowak | first13=G. | last14=Kuutma | first14=T. | last15=Saario | first15=J. | last16=Eigmüller | first16=P. | last17=Erikson | first17=A. | last18=Guenther | first18=E. W. | last19=Hatzes | first19=A. P. | last20=Montañés Rodríguez | first20=P. | last21=Palle | first21=E. | last22=Pätzold | first22=M. | last23=Prieto-Arranz | first23=J. | last24=Rauer | first24=H. | last25=Sebastian | first25=D. | display-authors=1 | journal=Astronomy and Astrophysics | volume=601 | at=A128 | year=2017 | arxiv=1604.01265 | bibcode=2017A&A...601A.128N | doi=10.1051/0004-6361/201628639 | s2cid=55978628 | access-date=2022-03-18 | archive-date=2022-05-04 | archive-url=https://web.archive.org/web/20220504003941/https://www.aanda.org/articles/aa/full_html/2017/05/aa28639-16/aa28639-16.html | url-status=live }} or G9V{{cite journal | title=Eleven Multiplanet Systems From K2 Campaigns 1 and 2 and the Masses of Two Hot Super-Earths | last1=Sinukoff | first1=Evan | last2=Howard | first2=Andrew W. | last3=Petigura | first3=Erik A. | last4=Schlieder | first4=Joshua E. | last5=Crossfield | first5=Ian J. M. | last6=Ciardi | first6=David R. | last7=Fulton | first7=Benjamin J. | last8=Isaacson | first8=Howard | last9=Aller | first9=Kimberly M. | last10=Baranec | first10=Christoph | last11=Beichman | first11=Charles A. | last12=Hansen | first12=Brad M. S. | last13=Knutson | first13=Heather A. | last14=Law | first14=Nicholas M. | last15=Liu | first15=Michael C. | last16=Riddle | first16=Reed | last17=Dressing | first17=Courtney D. | display-authors=1 | journal=The Astrophysical Journal | volume=827 | issue=1 | at=78 | year=2016 | arxiv=1511.09213 | bibcode=2016ApJ...827...78S | doi=10.3847/0004-637X/827/1/78 | doi-access=free }}
| Mass = 0.918
| Radius = 0.881±0.111
| Temperature = 5250±70
| Metallicity = 0.10±0.05
| Age = 8
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = PSR B1257+12|Lich
| Constellation = Virgo (constellation){{!}}Virgo
| Right ascension = {{RA|13|00|03.58}}
| Declination = {{DEC|+12|40|56.5}}
| Apparent magnitude = 24.31
| Distance = 980
| Spectral type = pulsar
| Mass = 1.444
| Radius = 0.000023
| Temperature = 28856
| Metallicity =
| Age = 0.797
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Only pulsar with a multiplanetary system, and first exoplanets and multiplanetary system to be confirmed.{{cite web |url=http://www.astro.psu.edu/users/alex/pulsar_planets.htm |title=Pulsar Planets |url-status=dead |archive-url=https://web.archive.org/web/20051230112904/http://www.astro.psu.edu/users/alex/pulsar_planets.htm |archive-date=30 December 2005 }}{{cite journal|bibcode=1992Natur.355..145W|author=Wolszczan, A.|author2=Frail, D.|title=A planetary system around the millisecond pulsar PSR1257 + 12|journal=Nature|volume=355|issue=6356|pages=145–147|date=1992|doi=10.1038/355145a0|s2cid=4260368}} Star with dimmest apparent magnitude to have a multiplanetary system.
}}
{{Multiplanetary systems list
| Star = Kepler-62
| Constellation = Lyra
| Right ascension = {{RA|18|52|51.060}}
| Declination = {{DEC|+45|20|59.507}}
| Distance = 990
| Mass = 0.69
| Radius = 0.64
| Temperature = 4925
| Metallicity = –0.37
| Age = 7
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = Planets e and f orbit in the habitable zone.{{Cite journal | last=Borucki | first=William J. | author-link=William J. Borucki | display-authors=etal | title=Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone | journal=Science Express | date=18 April 2013 | doi=10.1126/science.1234702 | access-date=18 March 2022 | url=https://www.science.org/doi/10.1126/science.1234702 | arxiv=1304.7387 | bibcode=2013Sci...340..587B | pmid=23599262 | volume=340 | issue=6132 | pages=587–90 | hdl=1721.1/89668 | s2cid=21029755 | archive-date=2 May 2022 | archive-url=https://web.archive.org/web/20220502115940/https://www.science.org/doi/10.1126/science.1234702 | url-status=live }}{{cite web |last1=Johnson |first1=Michele |last2=Harrington |first2=J.D. |title=NASA's Kepler Discovers Its Smallest 'Habitable Zone' Planets to Date |url=http://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |date=18 April 2013 |work=NASA |access-date=18 March 2022 |archive-date=8 May 2020 |archive-url=https://web.archive.org/web/20200508010029/https://www.nasa.gov/mission_pages/kepler/news/kepler-62-kepler-69.html |url-status=dead }}
}}
{{Multiplanetary systems list
| Star = Kepler-48
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|56|33.41}}
| Declination = {{DEC|+40|56|56.47}}
| Apparent magnitude = 13.04
| Distance = 1000
| Spectral type = K
| Mass = 0.88
| Radius = 0.89
| Temperature = 5190
| Metallicity = -0.216
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-100
| Constellation = Lyra
| Right ascension = {{RA|19|25|32.6}}
| Declination = {{DEC|+41|59|24}}
| Apparent magnitude =
| Distance = 1011
| Spectral type = G1IV
| Mass = 1.109
| Radius = 1.5131
| Temperature = 5825
| Metallicity = 0.02
| Age = 6.5
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-49
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|29|11.0}}
| Declination = {{DEC|+40|35|30}}
| Apparent magnitude = 15.5
| Distance = 1015
| Spectral type = K
| Mass = 0.55
| Radius = 0.56
| Temperature = 3974
| Metallicity =
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-65
| Constellation = Lyra
| Right ascension = {{RA|19|14|45.3}}
| Declination = {{DEC|+41|09|04.2}}
| Apparent magnitude = 11.018
| Distance = 1019
| Spectral type = F6IV
| Mass = 1.199
| Radius = 1.399
| Temperature = 6211
| Metallicity = 0.17
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-52
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|19|06|57.0}}
| Declination = {{DEC|+49|58|33}}
| Apparent magnitude = 15.5
| Distance = 1049
| Spectral type = K
| Mass = 0.58
| Radius = 0.56
| Temperature = 4075
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-314
| Constellation = Libra (constellation){{!}}Libra
| Right ascension = {{RA|15|13|00.0}}
| Declination = {{DEC|-16|43|29}}
| Apparent magnitude = 11.4
| Distance = 1059
| Spectral type = G8IV/V
| Mass = 1.05
| Radius = 1.71
| Temperature = 5430
| Metallicity = 0.2
| Age = 9.0
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-219
| Constellation = Pisces (constellation){{!}}Pisces
| Right ascension = {{RA|00|51|22.9}}
| Declination = {{DEC|+08|52|04}}
| Apparent magnitude = 12.09
| Distance = 1071
| Spectral type = G2
| Mass = 1.02
| Radius = 1.19
| Temperature = 5753{{±|50}}
| Metallicity = 0.13
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-268
| Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|08|54|50.2862}}
| Declination = {{DEC|+11|50|53.7745}}
| Apparent magnitude = 13.85
| Distance = 1079
| Spectral type =
| Mass =
| Radius =
| Temperature =
| Metallicity =
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = K2-183
| Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|08|20|01.7184}}
| Declination = {{DEC|14|01|10.0711}}
| Apparent magnitude = 12.85
| Distance = 1083
| Spectral type =
| Mass =
| Radius = 0.87
| Temperature = 5482{{±|50}}
| Metallicity = 0.09
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
|Notes =
}}
{{Multiplanetary systems list
| Star = K2-187
| Constellation = Cancer (constellation){{!}}Cancer
| Right ascension = {{RA|08|50|05.6682}}
| Declination = {{DEC|23|11|33.3712}}
| Apparent magnitude = 12.864
| Distance = 1090
| Spectral type = G?V
| Mass = 0.967
| Radius = 0.895
| Temperature = 5438{{±|63}}
| Metallicity = 0.26
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
|Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-1542
| Constellation = Lyra
| Right ascension = {{RA|19|02|54.8}}
| Declination = {{DEC|+42|39|16}}
| Apparent magnitude =
| Distance = 1096
| Spectral type = G5V
| Mass = 0.94
| Radius = 0.99
| Temperature = 5564
| Metallicity = 0.06
| Age =
| Confirmed planets = 4
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = Kepler-26
| Constellation = Lyra
| Right ascension = {{RA|18|59|46}}
| Declination = {{DEC|+46|34|00}}
| Apparent magnitude = 16
| Distance = 1100
| Spectral type = M0V
| Mass = 0.65
| Radius = 0.59
| Temperature = 4500
| Metallicity = -0.21
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Transiting exoplanets{{citation|arxiv=1201.5412|title=Transit Timing Observations from Kepler: III. Confirmation of 4 Multiple Planet Systems by a Fourier-Domain Study of Anti-correlated Transit Timing Variations|year=2012|doi=10.1111/j.1365-2966.2012.20467.x|last1=Steffen|first1=Jason H.|last2=Fabrycky|first2=Daniel C.|last3=Ford|first3=Eric B.|last4=Carter|first4=Joshua A.|last5=Desert|first5=Jean-Michel|last6=Fressin|first6=Francois|last7=Holman|first7=Matthew J.|last8=Lissauer|first8=Jack J.|last9=Moorhead|first9=Althea V.|last10=Rowe|first10=Jason F.|last11=Ragozzine|first11=Darin|last12=Welsh|first12=William F.|last13=Batalha|first13=Natalie M.|last14=Borucki|first14=William J.|last15=Buchhave|first15=Lars A.|last16=Bryson|first16=Steve|last17=Caldwell|first17=Douglas A.|last18=Charbonneau|first18=David|last19=Ciardi|first19=David R.|last20=Cochran|first20=William D.|last21=Endl|first21=Michael|last22=Everett|first22=Mark E.|last23=Gautier III|first23=Thomas N.|last24=Gilliland|first24=Ron L.|last25=Girouard|first25=Forrest R.|last26=Jenkins|first26=Jon M.|last27=Horch|first27=Elliott|last28=Howell|first28=Steve B.|last29=Isaacson|first29=Howard|last30=Klaus|first30=Todd C.|journal=Monthly Notices of the Royal Astronomical Society |volume=421 |issue=3 |doi-access=free |bibcode=2012MNRAS.421.2342S |s2cid=11898578|display-authors=29}} which are low-density planets below the size of Neptune.{{citation|arxiv=1611.09236|title=An overabundance of low-density Neptune-like planets|year=2016|doi=10.1093/mnras/stw3103|last1=Cubillos|first1=Patricio|last2=Erkaev|first2=Nikolai V.|last3=Juvan|first3=Ines|last4=Fossati|first4=Luca|last5=Johnstone|first5=Colin P.|last6=Lammer|first6=Helmut|last7=Lendl|first7=Monika|last8=Odert|first8=Petra|last9=Kislyakova|first9=Kristina G.|journal=Monthly Notices of the Royal Astronomical Society|volume=466|issue=2|pages=1868–1879|doi-access=free |s2cid=119408956}}{{citation|arxiv=1512.02003|title=Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 M🜨 with Diverse Densities and Incident Fluxes|year=2015|doi=10.3847/0004-637X/820/1/39|last1=Jontof-Hutter|first1=Daniel|last2=Ford|first2=Eric B.|last3=Rowe|first3=Jason F.|last4=Lissauer|first4=Jack J.|last5=Fabrycky|first5=Daniel C.|author6=Christa Van Laerhoven|last7=Agol|first7=Eric|last8=Deck|first8=Katherine M.|last9=Holczer|first9=Tomer|last10=Mazeh|first10=Tsevi|journal=The Astrophysical Journal |volume=820 |issue=1 |page=39 |s2cid=11322397 |doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Kepler-167
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|30|38.0}}
| Declination = {{DEC|+38|20|43}}
| Apparent magnitude =
| Distance = 1119 ± 6
| Spectral type =
| Mass = 0.76
| Radius = 0.7
| Temperature = 4796
| Metallicity = 0.052
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Planet e is the first transiting Jupiter analog discovered.{{cite journal |last1=Kipping |first1=David M. |last2=Torres |first2=Guillermo |display-authors=etal |date=April 2016 |title=A Transiting Jupiter Analog |journal=The Astrophysical Journal |volume=820 |issue=2 |pages=112 |doi=10.3847/0004-637X/820/2/112 |arxiv=1603.00042 |bibcode=2016ApJ...820..112K|s2cid=1892262 |doi-access=free }}{{cite journal |last1=Chachan |first1=Yayaati |last2=Dalba |first2=Paul A. |display-authors=etal |date=February 2022 |title=Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths |journal=The Astrophysical Journal |volume=926 |issue=1 |pages=62 |doi=10.3847/1538-4357/ac3ed6 |arxiv=2112.00747 |bibcode=2022ApJ...926...62C|s2cid=244799213 |doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Kepler-81
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|34|32.9}}
| Declination = {{DEC|+42|49|30}}
| Apparent magnitude = 15.56
| Distance = 1136
| Spectral type = K?V
| Mass = 0.648
| Radius = 0.578
| Temperature = 4391
| Metallicity = -0.2
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-132
| Constellation = Lyra
| Right ascension = {{RA|18|52|56.6}}
| Declination = {{DEC|+41|20|35}}
| Apparent magnitude =
| Distance = 1140
| Spectral type = F9
| Mass = 0.98
| Radius = 1.18
| Temperature = 6003
| Metallicity = -0.053
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-80
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|44|27.0}}
| Declination = {{DEC|+39|58|44}}
| Apparent magnitude = 14.804
| Distance = 1218
| Spectral type = M0V{{cite simbad|title=Kepler-80|access-date=10 January 2017}}
| Mass = 0.730
| Radius = 0.738
| Temperature = 4250
| Metallicity = -0.56
| Age =
| Confirmed planets = 6
|Unconfirmed planets =
| Notes = Red dwarf star with six confirmed planets.{{cite journal|last1=Xie|first1=J.-W.|year=2013|title=Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems|journal=Astrophysical Journal Supplement Series|volume=208|issue=2|pages=22|arxiv=1208.3312|bibcode=2013ApJS..208...22X|doi=10.1088/0067-0049/208/2/22|s2cid=17160267}}{{cite journal|last1=Shallue|first1=C. J.|last2=Vanderburg|first2=A.|date=2017|title=Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90|url=https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|journal=The Astrophysical Journal|volume=155|issue=2|pages=94|arxiv=1712.05044|bibcode=2018AJ....155...94S|doi=10.3847/1538-3881/aa9e09|s2cid=4535051|access-date=2017-12-15|doi-access=free|archive-date=2017-12-24|archive-url=https://web.archive.org/web/20171224094458/https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf|url-status=live}} Five of them are in an orbital resonance.{{Cite journal|last1=MacDonald|first1=Mariah G.|last2=Ragozzine|first2=Darin|last3=Fabrycky|first3=Daniel C.|last4=Ford|first4=Eric B.|last5=Holman|first5=Matthew J.|last6=Isaacson|first6=Howard T.|last7=Lissauer|first7=Jack J.|last8=Lopez|first8=Eric D.|last9=Mazeh|first9=Tsevi|date=2016-01-01|title=A Dynamical Analysis of the Kepler-80 System of Five Transiting Planets|url=http://stacks.iop.org/1538-3881/152/i=4/a=105|journal=The Astronomical Journal|volume=152|issue=4|pages=105|doi=10.3847/0004-6256/152/4/105|arxiv = 1607.07540 |bibcode = 2016AJ....152..105M |s2cid=119265122 |doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Kepler-159
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|48|16.8}}
| Declination = {{DEC|+40|52|08}}
| Apparent magnitude =
| Distance = 1219
| Spectral type = K
| Mass = 0.63
| Radius = 0.66
| Temperature = 4625
| Metallicity = -0.911
| Age =
| Confirmed planets = 2
|Unconfirmed planets = 1
| Notes = Star has a very low metallicity.
}}
{{Multiplanetary systems list
| Star = K2-299
| Constellation = Aquarius (constellation){{!}}Aquarius
| Right ascension = {{RA|22|05|06.5342}}
| Declination = {{DEC|-14|07|18.0135}}
| Apparent magnitude = 13.12
| Distance = 1220
| Spectral type =
| Mass =
| Radius = 1.1
| Temperature = 5724{{±|72}}
| Metallicity = -0.22
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
|Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-88
| Constellation = Lyra (constellation){{!}}Lyra
| Right ascension = {{RA|19|24|35.5431}}
| Declination = {{DEC|+40|40|09.8098}}
| Apparent magnitude = 13.5
| Distance = 1243
| Spectral type = G8IV
| Mass = 1.022
| Radius = 0.961
| Temperature = 5513{{±|67}}
| Metallicity = 0.37
| Age = 2.45
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-174
| Constellation = Lyra
| Right ascension = {{RA|19|09|45.4}}
| Declination = {{DEC|+43|49:56}}
| Apparent magnitude =
| Distance = 1269
| Spectral type = K
| Mass =
| Radius = 0.62
| Temperature = 4880
| Metallicity = -0.556
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Planet d may orbit in the habitable zone.
}}
{{Multiplanetary systems list
| Star = Kepler-32
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|51|22.0}}
| Declination = {{DEC|+46|34|27}}
| Apparent magnitude = 16
| Distance = 1301.1
| Spectral type = M1V
| Mass = 0.58
| Radius = 0.53
| Temperature = 3900
| Metallicity = 0
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 2
}}
{{Multiplanetary systems list
| Star = Kepler-83
| Constellation = Lyra
| Right ascension = {{RA|18|48|55.8}}
| Declination = {{DEC|+43|39|56}}
| Apparent magnitude = 16.51
| Distance = 1306
| Spectral type = K7V
| Mass = 0.664
| Radius = 0.539
| Temperature = 4164
| Metallicity = -0.2
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = TOI-1338
| Constellation = Pictor
| Right ascension = {{RA|06|08|31.97}}
| Declination = {{DEC|+59|32|28.1}}
| Apparent magnitude = 11.72
| Distance = 1318
| Spectral type = F8
M
| Mass = 1.127
| Radius = 1.331/0.309
| Temperature = 6160
| Metallicity = 0.01
| Age = 4.4
| Confirmed planets = 2
|Unconfirmed planets = 0
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-271
| Constellation = Lyra
| Right ascension = {{RA|18|52|00.7}}
| Declination = {{DEC|+44|17|03}}
| Apparent magnitude =
| Distance = 1319
| Spectral type = G7V
| Mass = 0.9
| Radius = 0.88
| Temperature = 5524
| Metallicity = -0.951
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Metal-poor star
}}
{{Multiplanetary systems list
| Star = Kepler-169
| Constellation =
| Right ascension = {{RA|19|03|60.0}}
| Declination = {{DEC|+40|55:10}}
| Apparent magnitude = 12.186
| Distance = 1326
| Spectral type = K2V
| Mass = 0.86
| Radius = 0.76
| Temperature = 4997
| Metallicity = 0.238
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-451
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|38|32.61}}
| Declination = {{DEC|46|03|59.1}}
| Apparent magnitude =
| Distance = 1340
| Spectral type = sdB
M
| Mass = 0.48+0.12
| Radius =
| Temperature = 29564
| Metallicity =
| Age = 6
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Three circumbinary planets orbit around the Kepler-451 binary pair.{{citation|arxiv=2202.02118|year=2022|title=Detection of two additional circumbinary planets around Kepler-451|author1=Ekrem Murat Esmer|last2=Baştürk|first2=Özgür|author3=Selim Osman Selam|last4=Aliş|first4=Sinan|journal=Monthly Notices of the Royal Astronomical Society |volume=511 |issue=4 |pages=5207–5216 |doi=10.1093/mnras/stac357 |doi-access=free |bibcode=2022MNRAS.511.5207E }}
}}
{{Multiplanetary systems list
| Star = Kepler-304
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|37|46.0}}
| Declination = {{DEC|+40|33|27}}
| Apparent magnitude =
| Distance = 1418
| Spectral type = K
| Mass = 0.8
| Radius = 0.73
| Temperature = 4731
| Metallicity = 0.523
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-18
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|52|19.06}}
| Declination = {{DEC|+44|44|46.76}}
| Apparent magnitude = 13.549
| Distance = 1430
| Spectral type = G7V
| Mass = 0.97
| Radius = 1.11
| Temperature = 5345
| Metallicity = +0.19
| Age = 10
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-106
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|20|03|27.4}}
| Declination = {{DEC|+44|20|15}}
| Apparent magnitude = 12.882
| Distance = 1449
| Spectral type = G1V
| Mass = 1
| Radius = 1.04
| Temperature = 5858
| Metallicity = -0.12
| Age = 4.83
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-92
| Constellation = Lyra
| Right ascension = {{RA|19|16|21.0}}
| Declination = {{DEC|+41|33|47}}
| Apparent magnitude = 11.6
| Distance = 1463
| Spectral type = G1IV
| Mass = 1.209
| Radius = 1.716
| Temperature = 5871
| Metallicity = 0.17
| Age = 5.52
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-450
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|41|56.8}}
| Declination = {{DEC|+51|00|49}}
| Apparent magnitude = 11.684
| Distance = 1487
| Spectral type = F
| Mass = 1.19
| Radius = 1.64
| Temperature = 6152
| Metallicity = -0.342
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-89
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|49|20.0}}
| Declination = {{DEC|+41|53|28}}
| Apparent magnitude = 12.4
| Distance = 1580
| Spectral type = F8V
| Mass = 1.25
| Radius = 1.656
| Temperature = 6116
| Metallicity = -0.01
| Age = 3.9
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Farthest F-type main sequence star from the Sun with a multiplanetary system. One study found hints of additional planets orbiting Kepler-89.{{Cite journal|arxiv=1310.5771|title=Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse|journal=The Astrophysical Journal|volume=778|issue=2|pages=185–200|last1=Masuda|first1=Kento|last2=Hirano|first2=Teruyuki|last3=Taruya|first3=Atsushi|last4=Nagasawa|first4=Makiko|last5=Suto|first5=Yasushi|year=2013|doi=10.1088/0004-637X/778/2/185|bibcode = 2013ApJ...778..185M |s2cid=119264400}}
}}
{{Multiplanetary systems list
| Star = Kepler-1388
| Constellation = Lyra
| Right ascension = {{RA|18|53|20.6}}
| Declination = {{DEC|+47|10|28}}
| Apparent magnitude =
| Distance = 1604
| Spectral type =
| Mass = 0.63
| Radius = 0.61
| Temperature = 4098
| Metallicity = 0.02
| Age =
| Confirmed planets = 4
|Unconfirmed planets = 1
}}
{{Multiplanetary systems list
| Star = K2-282
| Constellation = Pisces (constellation){{!}}Pisces
| Right ascension = {{RA|00|53|43.6833}}
| Declination = {{DEC|07|59|43.1397}}
| Apparent magnitude = 14.04
| Distance = 1638
| Spectral type = G?V
| Mass = 0.94
| Radius = 1
| Temperature = 5499{{±|109}}
| Metallicity = -0.23
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-107
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|48|06.8}}
| Declination = {{DEC|+48|12|31}}
| Apparent magnitude = 12.7
| Distance = 1714
| Mass = 1.238
| Radius = 1.41
| Temperature = 5851
| Metallicity = -0.092
| Age = 4.29
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-1047
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|14|35.1}}
| Declination = {{DEC|+50|47|20}}
| Apparent magnitude =
| Distance = 1846
| Spectral type = G2V
| Mass = 1.08
| Radius = 1.13
| Temperature = 5754
| Metallicity = 0.29
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-55
| Constellation = Lyra
| Right ascension = {{RA|19|00|40.0}}
| Declination = {{DEC|+44|01|35}}
| Apparent magnitude = 16.3
| Distance = 1888
| Spectral type = K
| Mass = 0.62
| Radius = 0.58
| Temperature = 4362
| Metallicity =
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = Planet c may orbit in the inner habitable zone.
}}
{{Multiplanetary systems list
| Star = Kepler-166
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|32|38.4}}
| Declination = {{DEC|+48|52|52}}
| Apparent magnitude =
| Distance = 1968
| Spectral type = G
| Mass = 0.88
| Radius = 0.74
| Temperature = 5413
| Metallicity = -0.286
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-11
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|48|27.62}}
| Declination = {{DEC|+41|54|32.9}}
| Apparent magnitude = 13.69
| Distance = 2150 {{±|20}}
| Mass = 0.954
| Radius = 1.102
| Temperature = 5681
| Metallicity = 0.003
| Age = 7.834
| Confirmed planets = 6
|Unconfirmed planets =
| Notes = Farthest star from the Sun with exactly six exoplanets. First system discovered with six transiting planets.{{cite journal | title=A closely packed system of low-mass, low-density planets transiting Kepler-11 | last1=Lissauer | first1=Jack J. | last2=Fabrycky | first2=Daniel C. | last3=Ford | first3=Eric B. | last4=Borucki | first4=William J. | last5=Fressin | first5=Francois | last6=Marcy | first6=Geoffrey W. | last7=Orosz | first7=Jerome A. | last8=Rowe | first8=Jason F. | last9=Torres | first9=Guillermo | last10=Welsh | first10=William F. | last11=Batalha | first11=Natalie M. | last12=Bryson | first12=Stephen T. | last13=Buchhave | first13=Lars A. | last14=Caldwell | first14=Douglas A. | last15=Carter | first15=Joshua A. | last16=Charbonneau | first16=David | last17=Christiansen | first17=Jessie L. | last18=Cochran | first18=William D. | last19=Desert | first19=Jean-Michel | last20=Dunham | first20=Edward W. | last21=Fanelli | first21=Michael N. | last22=Fortney | first22=Jonathan J. | last23=Gautier III | first23=Thomas N. | last24=Geary | first24=John C. | last25=Gilliland | first25=Ronald L. | last26=Haas | first26=Michael R. | last27=Hall | first27=Jennifer R. | last28=Holman | first28=Matthew J. | last29=Koch | first29=David G. | last30=Latham | first30=David W. | s2cid=4388001 | display-authors=1 | journal=Nature | volume=470 | issue=7332 | pages=53–58 | year=2011 | arxiv=1102.0291 | bibcode=2011Natur.470...53L | doi=10.1038/nature09760 | pmid=21293371 }} The planets have low densities.{{cite journal | title=All Six Planets Known to Orbit Kepler-11 Have Low Densities | last1=Lissauer | first1=Jack J. | last2=Jontof-Hutter | first2=Daniel | last3=Rowe | first3=Jason F. | last4=Fabrycky | first4=Daniel C. | last5=Lopez | first5=Eric D. | last6=Agol | first6=Eric | last7=Marcy | first7=Geoffrey W. | last8=Deck | first8=Katherine M. | last9=Fischer | first9=Debra A. | last10=Fortney | first10=Jonathan J. | last11=Howell | first11=Steve B. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Kolbl | first14=Rea | last15=Sasselov | first15=Dimitar | last16=Short | first16=Donald R. | last17=Welsh | first17=William F. | display-authors=1 | journal=The Astrophysical Journal | volume=770 | issue=2 | at=131 | year=2013 | arxiv=1303.0227 | bibcode=2013ApJ...770..131L | bibcode-access=free | doi=10.1088/0004-637X/770/2/131 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Kepler-1254
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|19|34|59.3}}
| Declination = {{DEC|+45|06|26}}
| Apparent magnitude =
| Distance = 2205
| Spectral type =
| Mass = 0.78
| Radius = 0.75
| Temperature = 4985
| Metallicity = -0.1
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-289
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|49|51.7}}
| Declination = {{DEC|+42|52|58}}
| Apparent magnitude = 12.9
| Distance = 2283
| Spectral type = G0V
| Mass = 1.08
| Radius = 1.0
| Temperature = 5990
| Metallicity = 0.05
| Age = 0.65
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-85
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|23|54.0}}
| Declination = {{DEC|+45|17|25}}
| Apparent magnitude = 15.0
| Distance = 2495
| Spectral type = G
| Mass = 0.92
| Radius = 0.89
| Temperature = 5666
| Metallicity =
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-157
| Constellation = Lyra
| Right ascension = {{RA|19|24|23.3}}
| Declination = {{DEC|+38|52|32}}
| Apparent magnitude =
| Distance = 2523
| Spectral type = G2V
| Mass = 1.02
| Radius = 1.03
| Temperature = 5774
| Metallicity = -0.108
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-342
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|24|23.3}}
| Declination = {{DEC|+38|52|32}}
| Apparent magnitude =
| Distance = 2549
| Spectral type = F
| Mass = 1.13
| Radius = 1.47
| Temperature = 6175
| Metallicity = -0.053
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-148
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|19|08.7}}
| Declination = {{DEC|+46|51|32}}
| Apparent magnitude =
| Distance = 2580
| Spectral type = K?V
| Mass = 0.83
| Radius = 0.85
| Temperature = 5019.0±122.0
| Metallicity = 0.143
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-51
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|45|55.0}}
| Declination = {{DEC|+49|56|16}}
| Apparent magnitude = 15.0
| Distance = 2610
| Spectral type = G?V
| Mass = 1.0
| Radius = 0.91
| Temperature = 5803
| Metallicity = -0.079
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Super-puff planets with some of the lowest densities known.{{cite journal
| title=The Featureless Transmission Spectra of Two Super-puff Planets
| first1=Jessica E. | last1=Libby-Roberts | first2=Zachory K. | last2=Berta-Thompson
| first3=Jean-Michel | last3=Desert | first4=Kento | last4=Masuda
| first5=Caroline V. | last5=Morley | first6=Eric D. | last6=Lopez
| first7=Katherine M. | last7=Deck | first8=Daniel | last8=Fabrycky
| first9=Jonathan J. | last9=Fortney | first10=Michael R. | last10=Line
| first11=Roberto | last11=Sanchis-Ojeda | first12=Joshua N. | last12=Winn
| journal=The Astronomical Journal | year=2020 | volume=159 | issue=2 | page=57 | display-authors=1 | doi=10.3847/1538-3881/ab5d36 | arxiv=1910.12988 | bibcode=2020AJ....159...57L | s2cid=204950000 | doi-access=free }}
}}
{{Multiplanetary systems list
| Star = Kepler-403
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|19|41.1}}
| Declination = {{DEC|+46|44|40}}
| Apparent magnitude =
| Distance = 2741
| Spectral type = F9IV-V
| Mass = 1.25
| Radius = 1.45
| Temperature = 6090
| Metallicity = -0.145
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-9
| Constellation = Lyra
| Right ascension = {{RA|19|02|17.76}}
| Declination = {{DEC|+38|24|03.2}}
| Apparent magnitude = 13.91
| Distance = 2754
| Spectral type = G2V
| Mass = 0.998
| Radius = 1.095
| Temperature = 5722
| Metallicity = 0.167
| Age = 3.008
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = First multiplanetary system to be discovered by the Kepler Space Telescope.{{cite web |url=http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |title=Kepler Discovers Multi-Planet System |author=Nancy Atkinson |date=26 August 2010 |publisher=Universe Today |access-date=13 January 2011 |archive-date=24 February 2012 |archive-url=https://web.archive.org/web/20120224041800/http://www.universetoday.com/72104/kepler-discovers-multi-planet-system/ |url-status=live }}{{Cite journal | title=Kepler-9: A System of Multiple Planets Transiting a Sun-Like Star, Confirmed by Timing Variations | url=http://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | last1=Holman | first1=M. J. | last2=Fabrycky | first2=D. C. | last3=Ragozzine | first3=D. | last4=Ford | first4=E. B. | last5=Steffen | first5=J. H. | last6=Welsh | first6=W. F. | last7=Lissauer | first7=J. J. | last8=Latham | first8=D. W. | last9=Marcy | first9=G. W. | last10=Walkowicz | first10=L. M. | last11=Batalha | first11=N. M. | last12=Jenkins | first12=J. M. | last13=Rowe | first13=J. F. | last14=Cochran | first14=W. D. | last15=Fressin | first15=F. | last16=Torres | first16=G. | last17=Buchhave | first17=L. A. | last18=Sasselov | first18=D. D. | last19=Borucki | first19=W. J. | last20=Koch | first20=D. G. | last21=Basri | first21=G. | last22=Brown | first22=T. M. | last23=Caldwell | first23=D. A. | last24=Charbonneau | first24=D. | last25=Dunham | first25=E. W. | last26=Gautier | first26=T. N. | last27=Geary | first27=J. C. | last28=Gilliland | first28=R. L. | last29=Haas | first29=M. R. | last30=Howell | first30=S. B. | display-authors=1 | journal=Science | volume=330 | issue=6000 | pages=51–54 | year=2010 | bibcode=2010Sci...330...51H | doi=10.1126/science.1195778 | pmid=20798283 | s2cid=8141085 | access-date=2022-06-17 | archive-date=2022-12-07 | archive-url=https://web.archive.org/web/20221207160620/https://www.astro.ubc.ca/people/gladman/a520/Holmanetal2010.pdf | url-status=live }}
}}
{{Multiplanetary systems list
| Star = Kepler-23
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|36|52.0}}
| Declination = {{DEC|+49|28|45}}
| Apparent magnitude = 14
| Distance = 2790
| Spectral type = G5V
| Mass = 1.11
| Radius = 1.52
| Temperature = 5760
| Metallicity = -0.09
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-46
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|17|05.0}}
| Declination = {{DEC|+42|36|15}}
| Apparent magnitude = 15.3
| Distance = 2795
| Spectral type = K?V
| Mass = 0.902
| Radius = 0.94
| Temperature = 5155
| Metallicity = 0.41
| Age = 9.9
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-305
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|56|53.83}}
| Declination = {{DEC|+40|20|35.46}}
| Apparent magnitude = 15.812
| Distance = 2833
| Spectral type = K
| Mass = 0.85
| Radius = 0.9
| Temperature = 4918
| Metallicity = -0.071
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-90
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|18|57|44.0}}
| Declination = {{DEC|+49|18|19}}
| Apparent magnitude = 14.0
| Distance = 2840 ± 40
| Spectral type = F9 IV/V
| Mass = 1.13
| Radius = 1.2
| Temperature = 5930
| Metallicity = -0.17
| Age = 2
| Confirmed planets = 8
|Unconfirmed planets =
| Notes = All eight exoplanets are larger than Earth and are within 1.1 AU of the parent star. Only star apart from the Sun with at least eight planets.{{cite web |last1=Chou |first1=Felicia |last2=Hawkes |first2=Alison |last3=Landau |first3=Elizabeth |title=Artificial Intelligence, NASA Data Used to Discover Eighth Planet Circling Distant Star |url=https://www.jpl.nasa.gov/news/news.php?feature=7026 |date=14 December 2017 |work=NASA |access-date=15 December 2017 |archive-date=5 May 2020 |archive-url=https://web.archive.org/web/20200505042830/https://www.jpl.nasa.gov/news/news.php?feature=7026 |url-status=live }} A Hill stability test shows that the system is stable.{{cite journal|last1= Schmitt|first1=J. R.|last2= Wang|first2= J.|last3= Fischer|first3=D. A.|last4= Jek|first4=K. J.|last5= Moriarty|first5=J. C.|last6= Boyajian|first6=T. S.|last7= Schwamb|first7=M. E.|last8= Lintott|first8= C.|last9= Lynn|first9=S.|last10= Smith|first10=A. M.|last11= Parrish|first11= M.|last12= Schawinski|first12= K.|last13= Simpson|first13= R.|last14= LaCourse|first14= D.|last15= Omohundro|first15=M. R.|last16= Winarski|first16= T.|last17= Goodman|first17=S. J.|last18= Jebson|first18= T.|last19= Schwengeler|first19=H. M.|last20= Paterson|first20=D. A.|last21= Sejpka|first21= J.|last22= Terentev|first22= I.|last23= Jacobs|first23= T.|last24= Alsaadi|first24 =N.|last25= Bailey|first25=R. C.|last26= Ginman|first26= T.|last27= Granado|first27= P.|last28= Guttormsen|first28=K. V.|last29= Mallia|first29= F.|last30= Papillon|first30=A. L.|last31= Rossi|first31= F.|last32= Socolovsky|first32= M.|last33= Stiak|first33= L.|title= Planet Hunters. VI. An Independent Characterization of KOI-351 and Several Long Period Planet Candidates From the Kepler Archival Data|journal= The Astronomical Journal|volume= 148|issue= 28|date= 2014-06-26|page=28|doi= 10.1088/0004-6256/148/2/28 |arxiv= 1310.5912|bibcode=2014AJ....148...28S|s2cid=119238163}} Planet h orbits in the habitable zone.
}}
{{Multiplanetary systems list
| Star = Kepler-150
| Constellation = Lyra
| Right ascension = {{RA|19|12|56.2}}
| Declination = {{DEC|+40|31|15}}
| Apparent magnitude =
| Distance = 2906
| Spectral type = G?V
| Mass = 0.97
| Radius = 0.91
| Temperature = 5560
| Metallicity = -0.136
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = Planet f orbits in the habitable zone.
}}
{{Multiplanetary systems list
| Star = Kepler-82
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|31|29.61}}
| Declination = {{DEC|+42|57|58.09}}
| Apparent magnitude = 15.158
| Distance = 2949
| Spectral type = G?V
| Mass = 0.91
| Radius = 0.9
| Temperature = 5512
| Metallicity = -0.014
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-154
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|19|07.3}}
| Declination = {{DEC|+49|53|48}}
| Apparent magnitude =
| Distance = 2985
| Spectral type = G3V
| Mass = 0.98
| Radius = 1.0
| Temperature = 5690
| Metallicity = -0.391
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-56
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|35|02.0}}
| Declination = {{DEC|+41|52|19}}
| Apparent magnitude = 13
| Distance = 3060
| Spectral type = K?III
| Mass = 1.32
| Radius = 4.23
| Temperature = 4840
| Metallicity = 0.2
| Age = 3.5
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-350
| Constellation = Lyra
| Right ascension = {{RA|19|01|41.0}}
| Declination = {{DEC|+39|42|22}}
| Apparent magnitude = 13.8
| Distance = 3121
| Spectral type = F
| Mass = 1.03
| Radius = 1.25
| Temperature = 6215
| Metallicity = -0.308
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-603
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|37|07.4}}
| Declination = {{DEC|+42|17|27}}
| Apparent magnitude =
| Distance = 3134
| Spectral type = G2V
| Mass = 1.01
| Radius = 1.01
| Temperature = 5808
| Metallicity = 0.03
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-160
| Constellation = Lyra
| Right ascension = {{RA|19|11|05.65}}
| Declination = {{DEC|+42|52|09.5}}
| Apparent magnitude = 13.101
| Distance = 3140
| Spectral type = G2V
| Mass =
| Radius = 1.18
| Temperature =5470
| Metallicity =-0.361
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 1
| Notes = The unconfirmed planet Kepler-160e (or KOI-456.04) is a potentially habitable planet.{{Cite web|last=Patel|first=Neel V.|date=2020-06-05|title=Astronomers have found a planet like Earth orbiting a star like the sun|url=https://www.technologyreview.com/2020/06/05/1002831/kepler-160-koi-456-04-earth-sun-exoplanet-habitable/|access-date=2020-06-07|website=MIT Technology Review|language=en|archive-date=2023-05-25|archive-url=https://web.archive.org/web/20230525031722/https://www.technologyreview.com/2020/06/05/1002831/kepler-160-koi-456-04-earth-sun-exoplanet-habitable/|url-status=live}}
}}
{{Multiplanetary systems list
| Star = Kepler-401
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|20|19.9}}
| Declination = {{DEC|+50|51|49}}
| Apparent magnitude =
| Distance = 3149
| Spectral type = F8V
| Mass = 1.17
| Radius = 1.29
| Temperature = 6117
| Metallicity = -0.297
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-58
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|45|26.0}}
| Declination = {{DEC|+39|06|55}}
| Apparent magnitude = 15.3
| Distance = 3161
| Spectral type = G1V
| Mass = 1.04
| Radius = 1.13
| Temperature = 5843
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-79
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|20|02|04.11}}
| Declination = {{DEC|+44|22|53.69}}
| Apparent magnitude = 13.914
| Distance = 3329
| Spectral type = F
| Mass = 1.17
| Radius = 1.3
| Temperature = 6187
| Metallicity = -0.263
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-60
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|15|50.70}}
| Declination = {{DEC|+42|15|54.04}}
| Apparent magnitude = 13.959
| Distance = 3343
| Spectral type = G
| Mass = 1.04
| Radius = 1.26
| Temperature = 5915
| Metallicity = -0.116
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-122
| Constellation =
| Right ascension = {{RA|19|24|26.9}}
| Declination = {{DEC|+39|56|57}}
| Apparent magnitude =
| Distance = 3351
| Spectral type = F
| Mass = 1.08
| Radius = 1.22
| Temperature = 6050
| Metallicity = -0.202
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-279
| Constellation = Lyra
| Right ascension = {{RA|19|09|34.0}}
| Declination = {{DEC|+42|11|42}}
| Apparent magnitude = 13.7
| Distance = 3383
| Spectral type = F
| Mass = 1.1
| Radius = 1.07
| Temperature = 6562
| Metallicity = -0.57
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-255
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|44|15.4}}
| Declination = {{DEC|+45|58|37}}
| Apparent magnitude =
| Distance = 3433
| Spectral type = G6V
| Mass = 0.90
| Radius = 0.86
| Temperature = 5573
| Metallicity = 0.212
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-47
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|41|11.5}}
| Declination = {{DEC|+46|55|13.69}}
| Apparent magnitude = 15.178
| Distance = 3442
| Spectral type = G
M
| Mass = 1.043
| Radius = 0.964/0.3506
| Temperature = 5636(A)
(B is unknown)
| Metallicity = -0.25†(A)
(B is unknown)
| Age = 4.5
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = Circumbinary planets, with one of the planets orbiting in the habitable zone.{{Cite journal|arxiv= 1208.5489 |title= Kepler-47: A Transiting Circumbinary Multi-Planet System|journal= Science|volume= 337|issue= 6101|pages= 1511–4|last1= Orosz|first1= Jerome A.|last2= Welsh|first2= William F.|last3= Carter|first3= Joshua A.|last4= Fabrycky|first4= Daniel C.|last5= Cochran|first5= William D.|last6= Endl|first6= Michael|last7= Ford|first7= Eric B.|last8= Haghighipour|first8= Nader|last9= MacQueen|first9= Phillip J.|last10= Mazeh|first10= Tsevi|last11= Sanchis-Ojeda|first11= Roberto|last12= Short|first12= Donald R.|last13= Torres|first13= Guillermo|last14= Agol|first14= Eric|last15= Buchhave|first15= Lars A.|last16= Doyle|first16= Laurance R.|last17= Isaacson|first17= Howard|last18= Lissauer|first18= Jack J.|last19= Marcy|first19= Geoffrey W.|last20= Shporer|first20= Avi|last21= Windmiller|first21= Gur|last22= Barclay|first22= Thomas|last23= Boss|first23= Alan P.|last24= Clarke|first24= Bruce D.|last25= Fortney|first25= Jonathan|last26= Geary|first26= John C.|last27= Holman|first27= Matthew J.|last28= Huber|first28= Daniel|last29= Jenkins|first29= Jon M.|last30= Kinemuchi|first30= Karen|display-authors= 29|year= 2012|doi= 10.1126/science.1228380 |pmid=22933522|bibcode = 2012Sci...337.1511O |s2cid= 44970411 }}{{cite news|url=http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|title=NASA's Kepler Discovers Multiple Planets Orbiting a Pair of Stars|date=28 August 2012|publisher=NASA|website=exoplanets.nasa.gov|quote=Kepler mission has discovered multiple transiting planets orbiting two suns for the first time|access-date=2 September 2012|archive-date=31 October 2012|archive-url=https://web.archive.org/web/20121031024345/http://www.nasa.gov/mission_pages/kepler/news/kepler-47.html|url-status=dead}}{{cite journal |url=https://www.sciencedaily.com/releases/2012/08/120828190127.htm |title=NASA's Kepler discovers multiple planets orbiting a pair of stars |doi=10.1126/science.1228380 |publisher=Sciencedaily.com |date=28 August 2012 |access-date=4 November 2012 |arxiv=1208.5489 |bibcode=2012Sci...337.1511O |last1=Orosz |first1=Jerome A. |last2=Welsh |first2=William F. |last3=Carter |first3=Joshua A. |last4=Fabrycky |first4=Daniel C. |last5=Cochran |first5=William D. |last6=Endl |first6=Michael |last7=Ford |first7=Eric B. |last8=Haghighipour |first8=Nader |last9=MacQueen |first9=Phillip J. |last10=Mazeh |first10=Tsevi |last11=Sanchis-Ojeda |first11=Roberto |last12=Short |first12=Donald R. |last13=Torres |first13=Guillermo |last14=Agol |first14=Eric |last15=Buchhave |first15=Lars A. |last16=Doyle |first16=Laurance R. |last17=Isaacson |first17=Howard |last18=Lissauer |first18=Jack J. |last19=Marcy |first19=Geoffrey W. |last20=Shporer |first20=Avi |last21=Windmiller |first21=Gur |last22=Barclay |first22=Thomas |last23=Boss |first23=Alan P. |last24=Clarke |first24=Bruce D. |last25=Fortney |first25=Jonathan |last26=Geary |first26=John C. |last27=Holman |first27=Matthew J. |last28=Huber |first28=Daniel |last29=Jenkins |first29=Jon M. |last30=Kinemuchi |first30=Karen |journal=Science |volume=337 |issue=6101 |pages=1511–4 |pmid=22933522 |s2cid=44970411 |display-authors=29 |archive-date=21 September 2022 |archive-url=https://web.archive.org/web/20220921182959/https://www.sciencedaily.com/releases/2012/08/120828190127.htm |url-status=live }}
}}
{{Multiplanetary systems list
| Star = Kepler-292
| Constellation =
| Right ascension = {{RA|19|43|03.84}}
| Declination = {{DEC|+43|25|27.4}}
| Apparent magnitude = 13.97
| Distance = 3446
| Spectral type = K0V
| Mass = 0.85
| Radius = 0.826
| Temperature = 5299
| Metallicity = 0.077
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-27
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|28|56.82}}
| Declination = {{DEC|+41|05|9.15}}
| Apparent magnitude = 15.855
| Distance = 3500
| Spectral type = G5V
| Mass = 0.65
| Radius = 0.59
| Temperature = 5400
| Metallicity = +0.41
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-351
| Constellation = Lyra
| Right ascension = {{RA|19|05|48.6}}
| Declination = {{DEC|+42|39|28}}
| Apparent magnitude =
| Distance = 3535
| Spectral type = G?V
| Mass = 0.89
| Radius = 0.85
| Temperature = 5643
| Metallicity = -0.134
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-276
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|34|16}}
| Declination = {{DEC|+39|02|11}}
| Apparent magnitude = 15.368
| Distance = 3734
| Spectral type = G?V
| Mass = 1.1
| Radius = 1.03
| Temperature = 5812
| Metallicity = 0.012
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-24
| Constellation = Lyra
| Right ascension = {{RA|19|21|39.18}}
| Declination = {{DEC|+38|20|37.51}}
| Apparent magnitude = 14.925
| Distance = 3910
| Spectral type = G1V
| Mass = 1.03
| Radius = 1.07
| Temperature = 5800
| Metallicity = -0.24
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-87
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|51|40.0}}
| Declination = {{DEC|+46|57|54}}
| Apparent magnitude = 15
| Distance = 4021
| Spectral type = G4IV
| Mass = 1.1
| Radius = 1.82
| Temperature = 5600
| Metallicity = -0.17
| Age = 7.5
| Confirmed planets = 2
|Unconfirmed planets = 2
| Notes = Farthest system from the Sun with an unconfirmed exoplanet candidate.
}}
{{Multiplanetary systems list
| Star = Kepler-33
| Constellation = Lyra
| Right ascension = {{RA|19|16|18.61}}
| Declination = {{DEC|+46|00|18.8}}
| Apparent magnitude = 13.988
| Distance = 4090
| Spectral type = G1IV
| Mass = 1.164
| Radius = 1.615
| Temperature = 5849
| Metallicity = 0.12
| Age = 4.27
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-282
| Constellation = Lyra
| Right ascension = {{RA|18|58|43.0}}
| Declination = {{DEC|+44|47|51}}
| Apparent magnitude = 15.2
| Distance = 4363
| Spectral type = G?V
| Mass = 0.97
| Radius = 0.89
| Temperature = 5876
| Metallicity = -0.374
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-758
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|32|20.3}}
| Declination = {{DEC|+41|08|08}}
| Apparent magnitude =
| Distance = 4413
| Spectral type =
| Mass = 1.16
| Radius = 1.42
| Temperature = 6228
| Metallicity = -0.1
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes = Farthest system from the Sun with exactly four confirmed exoplanets.
}}
{{Multiplanetary systems list
| Star = Kepler-53
| Constellation = Lyra
| Right ascension = {{RA|19|21|51.0}}
| Declination = {{DEC|+40|33|45}}
| Apparent magnitude = 16
| Distance = 4455
| Spectral type = G?V
| Mass = 0.98
| Radius = 0.89
| Temperature = 5858
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-30
| Constellation = Lyra
| Right ascension = {{RA|19|01|08.07}}
| Declination = {{DEC|+38|56|50.21}}
| Apparent magnitude = 15.403
| Distance = 4560
| Spectral type = G6V
| Mass = 0.99
| Radius = 0.95
| Temperature = 5498
| Metallicity = +0.18
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-84
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|53|00.49}}
| Declination = {{DEC|+40|29|45.87}}
| Apparent magnitude = 14.764
| Distance = 4700
| Spectral type = G3IV
| Mass = 1
| Radius = 1.43
| Temperature = 5755
| Metallicity = -0.131
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-385
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|37|21.23}}
| Declination = {{DEC|+50|20|11.55}}
| Apparent magnitude = 15.76
| Distance = 4900
| Spectral type = F8V
| Mass = 0.99
| Radius = 1.09
| Temperature = 5835
| Metallicity = 0.010
| Age =
| Confirmed planets = 3
|Unconfirmed planets = 4
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-31
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|36|06.0}}
| Declination = {{DEC|+45|51|11}}
| Apparent magnitude = 15.5
| Distance = 5429
| Spectral type = F
| Mass = 1.21
| Radius = 1.22
| Temperature = 6340
| Metallicity = -0.08
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes = The three planets are in an orbital resonance.{{citation|arxiv=1903.09474|title=The role of dissipative evolution for three-planet, near-resonant extrasolar systems|year=2019|doi=10.1051/0004-6361/201935259|last1=Pichierri|first1=Gabriele|last2=Batygin|first2=Konstantin|last3=Morbidelli|first3=Alessandro|journal=Astronomy & Astrophysics|volume=625|pages=A7|bibcode=2019A&A...625A...7P|s2cid=85459759}}
}}
{{Multiplanetary systems list
| Star = Kepler-238
| Constellation = Lyra
| Right ascension = {{RA|19|11|35}}
| Declination = {{DEC|+40|38|16}}
| Apparent magnitude = 15.084
| Distance = 5867
| Spectral type = G5IV
| Mass = 1.06
| Radius = 1.43
| Temperature = 5614
| Metallicity = 0.143
| Age =
| Confirmed planets = 5
|Unconfirmed planets =
| Notes = One of the farthest systems from the Sun with a multiplanetary system, and the farthest system where exoplanets were discovered by the Kepler space telescope.
}}
{{Multiplanetary systems list
| Star = Kepler-245
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|26|33.4}}
| Declination = {{DEC|+42|26|11}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.8
| Radius = 0.8
| Temperature = 5100
| Metallicity = -0.028
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-218
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|41|39.1}}
| Declination = {{DEC|+46|15|59}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.06
| Temperature = 5502
| Metallicity = 0.194
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-217
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|32|09.1}}
| Declination = {{DEC|+46|16|39}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.8
| Temperature = 6171
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-192
| Constellation = Lyra
| Right ascension = {{RA|19|11|40.3}}
| Declination = {{DEC|+45|35|34}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.01
| Temperature = 5479
| Metallicity = -0.153
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-191
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|24|44.0}}
| Declination = {{DEC|+45|19|23}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.85
| Radius = 0.79
| Temperature = 5282
| Metallicity = 0.006
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-176
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|38|40.3}}
| Declination = {{DEC|+43|51|12}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 0.89
| Temperature = 5232
| Metallicity = 0.072
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-431
| Constellation = Lyra
| Right ascension = {{RA|18|44|26.9}}
| Declination = {{DEC|+43|13|40}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.071
| Radius = 1.092
| Temperature = 6004
| Metallicity = 0.07
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-338
| Constellation = Lyra
| Right ascension = {{RA|18|51|54.9}}
| Declination = {{DEC|+40|47|04}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.1
| Radius = 1.74
| Temperature = 5923
| Metallicity = -0.106
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-197
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|40|54.3}}
| Declination = {{DEC|+50|33|32}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.12
| Temperature = 6004
| Metallicity = -0.533
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-247
| Constellation = Lyra
| Right ascension = {{RA|19|14|34.2}}
| Declination = {{DEC|+43|02|21}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.884
| Radius = 0.791
| Temperature = 5094
| Metallicity = 0.21
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-104
| Constellation = Lyra
| Right ascension = {{RA|19|10|25.1}}
| Declination = {{DEC|+42|10|00}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.81
| Radius = 1.35
| Temperature = 5711
| Metallicity = -0.777
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-126
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|17|23.4}}
| Declination = {{DEC|+44|12|31}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.36
| Temperature = 6239
| Metallicity =
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-127
| Constellation = Lyra
| Right ascension = {{RA|19|00|45.6}}
| Declination = {{DEC|+46|01|41}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.36
| Temperature = 6106
| Metallicity = -0.154
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-130
| Constellation = Lyra
| Right ascension = {{RA|19|13|48.2}}
| Declination = {{DEC|+40|14|43}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.0
| Radius = 1.13
| Temperature = 5884
| Metallicity = 0.02
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-164
| Constellation = Lyra
| Right ascension = {{RA|19|11|07.4}}
| Declination = {{DEC|+47|37|48}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.11
| Radius = 1.15
| Temperature = 5888
| Metallicity = -0.125
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-171
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|47|05.3}}
| Declination = {{DEC|+41|45|20}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 0.84
| Temperature = 5642
| Metallicity = -0.151
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-172
| Constellation = Lyra
| Right ascension = {{RA|19|47|05.3}}
| Declination = {{DEC|+41|45|20}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.86
| Radius = 1.08
| Temperature = 5526
| Metallicity = 0.012
| Age =
| Confirmed planets = 4
|Unconfirmed planets =
}}
{{Multiplanetary systems list
| Star = Kepler-149
| Constellation = Lyra
| Right ascension = {{RA|19|03|24.9}}
| Declination = {{DEC|+38|23|03}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 0.95
| Temperature = 5381
| Metallicity = 0.147
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-142
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|40|28.5}}
| Declination = {{DEC|+48|28|53}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.99
| Radius = 1.27
| Temperature = 5790
| Metallicity = -0.274
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-124
| Constellation = Draco (constellation){{!}}Draco
| Right ascension = {{RA|19|07|00.7}}
| Declination = {{DEC|+49|03|54}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 0.64
| Temperature = 4984
| Metallicity = -0.535
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-402
| Constellation = Lyra
| Right ascension = {{RA|19|13|28.9}}
| Declination = {{DEC|+43|21|17}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.26
| Temperature = 6090
| Metallicity = -0.22
| Age =
| Confirmed planets = 4
|Unconfirmed planets = 1
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-399
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|58|00.4}}
| Declination = {{DEC|+40|40|15}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 0.68
| Temperature = 5502
| Metallicity = -0.827
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-374
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|36|33.1}}
| Declination = {{DEC|+42|22|14}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.84
| Radius = 0.91
| Temperature = 5977
| Metallicity = -0.441
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-372
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|25|01.5}}
| Declination = {{DEC|+49|15|32}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.15
| Radius = 1.14
| Temperature = 6509
| Metallicity = -0.137
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-363
| Constellation = Lyra
| Right ascension = {{RA|18|52|46.1}}
| Declination = {{DEC|+41|18|19}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.23
| Radius = 1.49
| Temperature = 5593
| Metallicity = 0.299
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-359
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|33|10.5}}
| Declination = {{DEC|+42|11|47}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.07
| Radius = 1.09
| Temperature = 6248
| Metallicity = -0.039
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-357
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|24|58.3}}
| Declination = {{DEC|+44|00|31}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.78
| Radius = 0.83
| Temperature = 5036
| Metallicity = 0.051
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-354
| Constellation = Lyra
| Right ascension = {{RA|19|03|00.4}}
| Declination = {{DEC|+41|20|08}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.65
| Radius = 0.67
| Temperature = 4648
| Metallicity = -0.036
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-206
| Constellation = Lyra
| Right ascension = {{RA|19|26|32.3}}
| Declination = {{DEC|+41|50|02}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.94
| Radius = 1.19
| Temperature = 5764
| Metallicity = -0.149
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-203
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|01|23.3}}
| Declination = {{DEC|+41|45|43}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.98
| Radius = 1.11
| Temperature = 5821
| Metallicity = -0.107
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-194
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|27|53.1}}
| Declination = {{DEC|+47|51|51}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.02
| Temperature = 6089
| Metallicity = -0.298
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-184
| Constellation = Lyra
| Right ascension = {{RA|19|27|48.5}}
| Declination = {{DEC|+43|04|29}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 0.87
| Temperature = 5788
| Metallicity = -0.338
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-178
| Constellation = Lyra
| Right ascension = {{RA|19|08|24.3}}
| Declination = {{DEC|+46|53|47}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass =
| Radius = 1.07
| Temperature = 5676
| Metallicity = -0.188
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-336
| Constellation = Lyra
| Right ascension = {{RA|19|20|57.0}}
| Declination = {{DEC|+41|19|53}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.89
| Radius = 1.3
| Temperature = 5867
| Metallicity = -0.401
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-334
| Constellation = Lyra
| Right ascension = {{RA|19|08|33.8}}
| Declination = {{DEC|+47|06|55}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 1.0
| Radius = 1.07
| Temperature = 5828
| Metallicity = -0.074
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-332
| Constellation = Lyra
| Right ascension = {{RA|19|06|39.1}}
| Declination = {{DEC|+47|24|49}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.8
| Radius = 0.72
| Temperature = 4955
| Metallicity = 0.05
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-331
| Constellation = Lyra
| Right ascension = {{RA|19|27|20.2}}
| Declination = {{DEC|+39|18|26}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.51
| Radius = 0.49
| Temperature = 4347
| Metallicity = -0.85
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-327
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|30|34.2}}
| Declination = {{DEC|44|05|16}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.55
| Radius = 0.49
| Temperature = 3799
| Metallicity = -0.042
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-326
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|37|18.1}}
| Declination = {{DEC|+46|00|08}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.98
| Radius = 0.8
| Temperature = 5105
| Metallicity = 0.133
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list
| Star = Kepler-325
| Constellation = Cygnus (constellation){{!}}Cygnus
| Right ascension = {{RA|19|19|20.5}}
| Declination = {{DEC|+49|49|32}}
| Apparent magnitude =
| Distance =
| Spectral type =
| Mass = 0.87
| Radius = 1.0
| Temperature = 5752
| Metallicity = -0.171
| Age =
| Confirmed planets = 3
|Unconfirmed planets =
| Notes =
}}
{{Multiplanetary systems list/Bottom}}
Stars orbited by both planets and brown dwarfs
Stars orbited by objects on both sides of the ~13 Jupiter mass dividing line.
- 54 Piscium (HD 3651){{cite journal | display-authors=1 | last1=Mugrauer | first1=M. | last2=Seifahrt | first2=A. | last3=Neuhäuser | first3=R. | last4=Mazeh | first4=T. | title=HD 3651 B: the first directly imaged brown dwarf companion of an exoplanet host star | journal=Monthly Notices of the Royal Astronomical Society: Letters | volume=373 | issue=1 | pages=L31–L35 | date=2006 | doi=10.1111/j.1745-3933.2006.00237.x | doi-access=free | type=abstract | arxiv=astro-ph/0608484 | bibcode=2006MNRAS.373L..31M | s2cid=15608344 }}
- HD 168443{{cite journal
| title=Two New Planets in Eccentric Orbits
| last1=Marcy | first1=Geoffrey W. | last2=Butler | first2=R. Paul
| last3=Vogt | first3=Steven S. | last4=Fischer | first4=Debra
| last5=Liu | first5=Michael C. | display-authors=1
| journal=The Astrophysical Journal
| volume=520 | issue=1 | pages=239–247 | year=1999
| arxiv=astro-ph/9904275 | bibcode=1999ApJ...520..239M
| doi=10.1086/307451 | s2cid=16827678 }}{{cite journal
| title=Two Substellar Companions Orbiting HD 168443
| last1=Marcy | first1=Geoffrey W. | last2=Butler | first2=R. Paul
| last3=Vogt | first3=Steven S. | last4=Liu | first4=Michael C.
| last5=Laughlin | first5=Gregory | last6=Apps | first6=Kevin
| last7=Graham | first7=J. R. | last8=Lloyd | first8=J.
| last9=Luhman | first9=Kevin L. | first10=Ray | last10=Jayawardhana
| display-authors=1 | journal=The Astrophysical Journal
| volume=555 | issue=1 | pages=418–425 | year=2001
| bibcode=2001ApJ...555..418M | doi=10.1086/321445 | doi-access=free }}
| title=Direct imaging of an ultracool substellar companion to the exoplanet host star HD 4113 A
| last1=Cheetham | first1=A. | last2=Ségransan | first2=D.
| last3=Peretti | first3=S. | last4=Delisle | first4=J. -B.
| last5=Hagelberg | first5=J. | last6=Beuzit | first6=J. -L.
| last7=Forveille | first7=T. | last8=Marmier | first8=M.
| last9=Udry | first9=S. | last10=Wildi | first10=F.
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=614 | id=A16 | pages=19 | date=June 2018
| arxiv=1712.05217 | bibcode=2018A&A...614A..16C
| doi=10.1051/0004-6361/201630136 | s2cid=119084543 }}
- Gliese 229 A{{cite web|title=Astronomers Announce First Clear Evidence of a Brown Dwarf|url=http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/48/|publisher=Space Telescope Science Institute news release STScI-1995-48|date=November 29, 1995|access-date=24 September 2013|archive-date=9 July 2008|archive-url=https://web.archive.org/web/20080709002411/http://hubblesite.org/newscenter/newsdesk/archive/releases/1995/48/|url-status=live}}{{cite encyclopedia |title=Planet GJ 229 A b |url=https://exoplanet.eu/catalog/gj_229_a_b--1533/ |date=1995 |encyclopedia=Extrasolar Planets Encyclopaedia |access-date=7 September 2022}}{{cite encyclopedia |title=Planet GJ 229 A c|url=https://exoplanet.eu/catalog/gj_229_a_c--7263/ |date=1995 |encyclopedia=Extrasolar Planets Encyclopaedia|access-date=7 September 2022}}
- Epsilon Indi A{{Citation | title=Detection of the nearest Jupiter analog in radial velocity and astrometry data | first1=Fabo | last1=Feng | first2=Guillem | last2=Anglada-Escudé | first3=Mikko | last3=Tuomi | first4=Hugh R. A. | last4=Jones | first5=Julio | last5=Chanamé | first6=Paul R. | last6=Butler | first7=Markus | last7=Janson | journal=Monthly Notices of the Royal Astronomical Society | arxiv=1910.06804 | date=14 October 2019 | volume=490 | issue=4 | pages=5002–5016 | doi=10.1093/mnras/stz2912 | doi-access=free | bibcode=2019MNRAS.490.5002F | s2cid=204575783 }}{{cite news|last=Scholz |first=Ralf-Dieter |author2=McCaughrean, Mark |date=2003-01-13 |title=Discovery of Nearest Known Brown Dwarf: Bright Southern Star Epsilon Indi Has Cool, Substellar Companion |publisher=European Southern Observatory |url=http://www.eso.org/public/outreach/press-rel/pr-2003/pr-01-03.html |access-date=2006-05-24 |url-status=dead |archive-url=https://web.archive.org/web/20071014191814/http://eso.org/public/outreach/press-rel/pr-2003/pr-01-03.html |archive-date=October 14, 2007 }}{{cite journal | last=Scholz | first=R.-D. | author2=McCaughrean, M. J. | author3=Lodieu, N. | author4=Kuhlbrodt, B. | title=ε Indi B: A new benchmark T dwarf | journal=Astronomy and Astrophysics | date=February 2003 | volume=398 | issue=3 | pages=L29–L33 | bibcode=2003A&A...398L..29S | doi=10.1051/0004-6361:20021847 | arxiv=astro-ph/0212487 | s2cid=119474823 }}
- HD 82943{{cite journal | title=Catalog of Nearby Exoplanets | last1=Butler | first1=R. P. | last2=Wright | first2=J. T. | last3=Marcy | first3=G. W. | last4=Fischer | first4=D. A. | last5=Vogt | first5=S. S. | last6=Tinney | first6=C. G. | last7=Jones | first7=H. R. A. | last8=Carter | first8=B. D. | last9=Johnson | first9=J. A. | display-authors=1 | journal=The Astrophysical Journal | date=2006 | volume=646 | issue=1 | pages=505–522 | arxiv=astro-ph/0607493 | bibcode=2006ApJ...646..505B | doi=10.1086/504701 | s2cid=119067572 }}
- Pi Mensae{{cite journal |last1=Feng |first1=Fabo |last2=Butler |first2=R. Paul |display-authors=etal |date=August 2022 |title=3D Selection of 167 Substellar Companions to Nearby Stars |journal=The Astrophysical Journal Supplement Series |volume=262 |issue=21 |page=21 |doi=10.3847/1538-4365/ac7e57 |arxiv=2208.12720 |bibcode=2022ApJS..262...21F|s2cid=251864022 |doi-access=free }}{{cite journal | arxiv=2203.01018| doi=10.3847/1538-3881/ac5dcb| title=A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit| year=2022| last1=Hatzes| first1=Artie P.| last2=Gandolfi| first2=Davide| last3=Korth| first3=Judith| last4=Rodler| first4=Florian| last5=Sabotta| first5=Silvia| last6=Esposito| first6=Massimiliano| last7=Barragán| first7=Oscar| last8=Van Eylen| first8=Vincent| last9=Livingston| first9=John H.| last10=Serrano| first10=Luisa Maria| last11=Luque| first11=Rafael| last12=Smith| first12=Alexis M. S.| last13=Redfield| first13=Seth| last14=Persson| first14=Carina M.| last15=Pätzold| first15=Martin| last16=Palle| first16=Enric| last17=Nowak| first17=Grzegorz| last18=Osborne| first18=Hannah L. M.| last19=Narita| first19=Norio| last20=Mathur| first20=Savita| last21=Lam| first21=Kristine W. F.| last22=Kabáth| first22=Petr| last23=Johnson| first23=Marshall C.| last24=Guenther| first24=Eike W.| last25=Grziwa| first25=Sascha| last26=Goffo| first26=Elisa| last27=Fridlund| first27=Malcolm| last28=Endl| first28=Michael| last29=Deeg| first29=Hans J.| last30=Csizmadia| first30=Szilard| journal=The Astronomical Journal| volume=163| issue=5| page=223| bibcode=2022AJ....163..223H| s2cid=247218413| display-authors=1| doi-access=free}}
- HD 38529{{cite journal | title=A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529 | last1=Fischer | first1=Debra A. | last2=Marcy | first2=Geoffrey W. | last3=Butler | first3=R. Paul | last4=Vogt | first4=Steven S. | last5=Henry | first5=Gregory W. | last6=Pourbaix | first6=Dimitri | last7=Walp | first7=Bernard | last8=Misch | first8=Anthony A. | last9=Wright | first9=Jason T. | display-authors=1 | journal=The Astrophysical Journal | volume=586 | issue=2 | pages=1394–1408 | year=2003 | bibcode=2003ApJ...586.1394F | bibcode-access=free | doi=10.1086/367889 | doi-access=free }}
- HD 245134{{Cite journal |last1=Khandelwal |first1=Akanksha |last2=Sharma |first2=Rishikesh |last3=Chakraborty |first3=Abhijit |last4=Chaturvedi |first4=Priyanka |last5=Ulmer-Moll |first5=Solène |last6=Ciardi |first6=David R. |last7=Boyle |first7=Andrew W. |last8=Baliwal |first8=Sanjay |last9=Bieryla |first9=Allyson |last10=Latham |first10=David W. |last11=Prasad |first11=Neelam J. S. S. V. |last12=Nayak |first12=Ashirbad |last13=Lendl |first13=Monika |last14=Mordasini |first14=Christoph |date=2023-04-01 |title=Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603 |url=https://www.aanda.org/articles/aa/abs/2023/04/aa45608-22/aa45608-22.html |journal=Astronomy & Astrophysics |language=en |volume=672 |pages=L7 |doi=10.1051/0004-6361/202245608 |issn=0004-6361 |doi-access=free |arxiv=2303.11841 |bibcode=2023A&A...672L...7K |access-date=2023-12-15 |archive-date=2024-02-28 |archive-url=https://web.archive.org/web/20240228142329/https://www.aanda.org/articles/aa/abs/2023/04/aa45608-22/aa45608-22.html |url-status=live }}
- KMT-2020-BLG-0414L{{cite journal |last1=Zhang |first1=Keming |last2=Zang |first2=Weicheng |last3=El-Badry |first3=Kareem |last4=Lu |first4=Jessica R. |display-authors=etal |date=September 2024 |title=An Earth-mass planet and a brown dwarf in orbit around a white dwarf |journal=Nature Astronomy |volume= 8|issue= 12|pages= 1575–1582|doi=10.1038/s41550-024-02375-9 |arxiv=2409.02157 |bibcode=2024NatAs...8.1575Z}}
See also
{{cmn|
- Lists of exoplanets
- Methods of detecting exoplanets
- List of exoplanet firsts
- List of exoplanet extremes
- List of brown dwarfs
- Lists of stars
- List of nearest stars
- List of stars with proplyds
- Lists of astronomical objects
For links to specific lists of exoplanets see:
- List of exoplanets detected by microlensing
- List of exoplanets detected by radial velocity
- List of exoplanets detected by timing
- List of directly imaged exoplanets
- List of transiting exoplanets
- List of nearest terrestrial exoplanet candidates
Online archives:
}}
Notes
{{notelist}}
References
{{Reflist}}
{{exoplanet}}
{{Portal bar|Astronomy|Stars|Spaceflight|Outer space|Solar System}}
{{DEFAULTSORT:Multiplanetary systems}}