For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum mass for more information)
| class="wikitable plainrowheaders sortable" style="width: 100%; font-size: 83%; text-align: center;"
!Name
!data-sort-type="number"|Mass ({{Jupiter mass}})
!data-sort-type="number"|Radius ({{Jupiter radius}})
!data-sort-type="number"|Period (days)
!data-sort-type="number"|Semi-major axis (AU)
!data-sort-type="number"|Temp. (K)[{{Cite web]
|url = https://exoplanet.eu/catalog/
|title = The Extrasolar Planets Encyclopaedia
|date = 1995
|access-date = 2015-11-09}}
!Discovery method
!data-sort-type="number"|Distance (ly)
!data-sort-type="number"|Host star mass ({{solar mass|link=yes}})
!data-sort-type="number"|Host star temp. (K)
!Remarks |
| 75 Ceti b
|3
|
|691.9
|2.1
|
|style="background:#00FF00"|radial vel.
|266
|2.49
|4846
| |
| {{vanchor|BD+20 274 b}}
|4.2
|
|578.2
|1.3
|
|style="background:#00FF00"|radial vel.
|4500{{±|300}}
|0.8
|4296
|[{{citation|arxiv=1207.0488|year=2012|title=Planets Around the K-Giants Bd+20 274 and Hd 219415|doi=10.1088/0004-637X/756/1/53|last1=Gettel|first1=S.|last2=Wolszczan|first2=A.|last3=Niedzielski|first3=A.|last4=Nowak|first4=G.|last5=Adamów|first5=M.|last6=Zieliński|first6=P.|last7=MacIejewski|first7=G.|journal=The Astrophysical Journal|volume=756|issue=1|page=53|bibcode=2012ApJ...756...53G|s2cid=119234699}}] |
| BD+48 740 b
|1.7{{±|0.7}}
|
|733{{±|5|8}}
|1.7{{±|0.1}}
|
|style="background:#00FF00"|radial vel.
|2214{{±|72}}
|1.09{{±|0.16}}
|4534{{±|8}}
|[{{cite journal |bibcode=2012ApJ...754L..15A |title=BD+48 740—Li Overabundant Giant Star with a Planet: A Case of Recent Engulfment? |last1=Adamów |first1=M. |last2=Niedzielski |first2=A. |last3=Villaver |first3=E. |last4=Nowak |first4=G. |last5=Wolszczan |first5=A. |journal=The Astrophysical Journal |year=2012 |volume=754 |issue=1 |pages=L15 |doi=10.1088/2041-8205/754/1/L15 |arxiv=1206.4938 |s2cid=53550985}}] Confirmed in 2018.[{{citation|arxiv=1801.04379|year=2018|title=Tracking Advanced Planetary Systems (TAPAS) with HARPS-N|doi=10.1051/0004-6361/201732161|last1=Adamów|first1=M.|last2=Niedzielski|first2=A.|last3=Kowalik|first3=K.|last4=Villaver|first4=E.|last5=Wolszczan|first5=A.|last6=MacIejewski|first6=G.|last7=Gromadzki|first7=M.|journal=Astronomy & Astrophysics|volume=613|pages=A47|s2cid=56091464}}] |
| CoRoT-21b
|2.26
|1.3
|2.72
|0.0417
|1867
|style="background:#FFFF00"|transit
|4600{{±|900}}
|1.29
|6200
|[[https://www.aanda.org/articles/aa/abs/2012/09/aa18425-11/aa18425-11.html Transiting exoplanets from the CoRoT space mission XXIII. CoRoT-21b: a doomed large Jupiter around a faint subgiant star]] |
| Epsilon Coronae Borealis b
|6.7
|
|417.9
|1.3
|
|style="background:#00FF00"|radial vel.
|229.7
|1.7
|4406
|[{{cite journal|author1=Lee, B.-C. |author2=Han, I. |author3=Park, M.-G. |author4=Mkrtichian, D. E. |author5=Kim, K.-M. |date=2012|title=A planetary companion around the K giant ɛ Corona Borealis|journal=Astronomy & Astrophysics|volume=546|id=A5|pages=5|bibcode=2012A&A...546A...5L|doi=10.1051/0004-6361/201219347|arxiv=1209.1187|s2cid=55260442 }}] |
| Gliese 676 Ad
|0.014
|
|3.6005
|0.0413{{±|0.0014}}
|
|style="background:#00FF00"|radial vel.
|52.29{{±|0.03}}
|0.71{{±|0.04}}
|3734
|[{{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}}] |
| Gliese 676 Ae
|0.025
|
|35.39
|0.187{{±|0.007}}
|
|style="background:#00FF00"|radial vel.
|52.29{{±|0.03}}
|0.71{{±|0.04}}
|3734
| |
| Gliese 3470 b
|0.043
|0.346
|3.3366487
|0.031
|
|style="background:#00FF00"|radial vel.
|82
|0.51
|3652
|[{{Cite journal |doi=10.1051/0004-6361/201219623 |arxiv=1206.5307 |title=A hot Uranus transiting the nearby M dwarf GJ3470. Detected with HARPS velocimetry. Captured in transit with TRAPPIST photometry |journal=Astronomy & Astrophysics |volume=546 |pages=A27 |last1=Bonfils |first1=Xavier |last2=Gillon |first2=Michaël |last3=Udry |first3=Stéphane |last4=Armstrong |first4=David |last5=Bouchy |first5=François |last6=Delfosse |first6=Xavier |last7=Forveille |first7=Thierry |last8=Fumel |first8=Aurélie |last9=Jehin |first9=Emmanuël |last10=Lendl |first10=Monika |last11=Lovis |first11=Christophe |last12=Mayor |first12=Michel |last13=McCormac |first13=James |last14=Neves |first14=Vasco |last15=Pepe |first15=Francesco |last16=Perrier |first16=Christian |last17=Pollacco |first17=Don L. |last18=Queloz |first18=Didier |last19=Santos |first19=Nuno C. |year=2012 |bibcode=2012A&A...546A..27B |s2cid=12963626 |url=http://orbi.ulg.ac.be/jspui/handle/2268/135085 }}] |
| HAT-P-34b
|7.01
|1.35
|5.45265
|0.06774
|1520
|style="background:#FFFF00"|transit
|818.94
|4.26
|6442
|[ Proper name Ġgantija] |
| HAT-P-35b
|7.52
|3.55
|3.64671
|0.0498
|1581
|style="background:#FFFF00"|transit
|1677
|23.56
|6096
| |
| HAT-P-36b
|1.8482
|1.277
|1.32734683
|0.0241
|1781
|style="background:#FFFF00"|transit
|968.49
|1.03
|5620
|[ Proper name Bran] |
| HAT-P-37b
|1.169
|1.178
|2.797436
|0.0379
|1271
|style="background:#FFFF00"|transit
|1341
|0.93
|5500
|[{{citation|arxiv=1201.0659|title=HAT-P-34b-HAT-P-37b: FOUR TRANSITING PLANETS MORE MASSIVE THAN JUPITER ORBITING MODERATELY BRIGHT STARS|year=2012|doi=10.1088/0004-6256/144/1/19|last1=Bakos|first1=G. Á.|last2=Hartman|first2=J. D.|last3=Torres|first3=G.|last4=Béky|first4=B.|last5=Latham|first5=D. W.|last6=Buchhave|first6=L. A.|last7=Csubry|first7=Z.|last8=Kovács|first8=G.|last9=Bieryla|first9=A.|last10=Quinn|first10=S.|last11=Szklenár|first11=T.|last12=Esquerdo|first12=G. A.|last13=Shporer|first13=A.|last14=Noyes|first14=R. W.|last15=Fischer|first15=D. A.|last16=Johnson|first16=J. A.|last17=Howard|first17=A. W.|last18=Marcy|first18=G. W.|last19=Sato|first19=B.|last20=Penev|first20=K.|last21=Everett|first21=M.|last22=Sasselov|first22=D. D.|last23=Fűrész|first23=G.|last24=Stefanik|first24=R. P.|last25=Lázár|first25=J.|last26=Papp|first26=I.|last27=Sári|first27=P.|journal=The Astronomical Journal|volume=144|issue=1|page=19|bibcode=2012AJ....144...19B|s2cid=119291677}}] Additional planets in system are suspected[{{citation|arxiv=2112.04724|year=2022|title=The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b|last1=A-thano|first1=Napaporn|last2=Jiang|first2=Ing-Guey|last3=Awiphan|first3=Supachai|last4=Rattanamala|first4=Ronnakrit|last5=Su|first5=Li-Hsin|last6=Hengpiya|first6=Torik|last7=Sariya|first7=Devesh P.|last8=Yeh|first8=Li-Chin|last9=Shlyapnikov|first9=A. A.|last10=Gorbachev|first10=Mark A.|last11=Rublevski|first11=Alexey N.|author12=Vineet Kumar Mannaday|last13=Thakur|first13=Parijat|last14=Sahu|first14=D. K.|last15=Mkrtichian|first15=David|last16=Griv|first16=Evgeny|journal=The Astronomical Journal |volume=163 |issue=2 |page=77 |doi=10.3847/1538-3881/ac416d |s2cid=245006237 |doi-access=free |bibcode=2022AJ....163...77A }}] |
| HAT-P-38b
|0.267
|0.825
|4.640382
|0.0523
|
|style="background:#FFFF00"|transit
|810
|0.89
|5330
|[{{citation|arxiv=1201.5075|year=2012|title=HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star|doi=10.1093/pasj/64.5.97|last1=Sato|first1=Bun'ei|last2=Hartman|first2=Joel D.|last3=Bakos|first3=Gáspár Á.|last4=Béky|first4=Bence|last5=Torres|first5=Guillermo|last6=Latham|first6=David W.|last7=Kovács|first7=Géza|last8=Csubry|first8=Zoltán|last9=Penev|first9=Kaloyan|last10=Noyes|first10=Robert W.|last11=Buchhave|first11=Lars A.|last12=Quinn|first12=Samuel N.|last13=Everett|first13=Mark|last14=Esquerdo|first14=Gilbert A.|last15=Fischer|first15=Debra A.|last16=Howard|first16=Andrew W.|last17=Johnson|first17=John A.|last18=Marcy|first18=Geoff W.|last19=Sasselov|first19=Dimitar D.|last20=Szklenár|first20=Tamás|last21=Lázár|first21=József|last22=Papp|first22=István|last23=Sári|first23=Pál|journal=Publications of the Astronomical Society of Japan|volume=64|issue=5|page=97}}] Proper name Hiisi |
| HAT-P-39b
|0.599
|1.571
|3.54387
|0.0509
|
|style="background:#FFFF00"|transit
|2090
|1.4
|6430
| |
| HAT-P-40b
|0.615
|1.73
|4.457243
|0.0608
|
|style="background:#FFFF00"|transit
|1630
|1.51
|6080
|[ Proper name Vytis] |
| HAT-P-41b
|0.8
|1.685
|2.694047
|0.0426
|
|style="background:#FFFF00"|transit
|1120
|1.42
|6390
|[{{cite journal|arxiv=2010.08551|title=Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed|year=2020|doi=10.3847/2041-8213/abb77f|last1=Lewis|first1=N. K.|display-authors=etal|journal=The Astrophysical Journal|volume=902|issue=1|pages=L19|bibcode=2020ApJ...902L..19L|s2cid=224706001 |doi-access=free }}][{{cite journal|arxiv=1207.3344|title=HAT-P-39b–HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters|year=2012|bibcode=2012AJ....144..139H|last1=Hartman|first1=J. D.|display-authors=etal|journal=The Astronomical Journal|volume=144|issue=5|page=139|doi=10.1088/0004-6256/144/5/139|s2cid=118457589}}][{{cite journal|arxiv=2010.09659|title=The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b|year=2021|last1=Sheppard|first1=Kyle B.|journal=The Astronomical Journal|volume=161|issue=2|page=51|doi=10.3847/1538-3881/abc8f4|bibcode=2021AJ....161...51S|s2cid=224710738|display-authors=etal |doi-access=free }}] |
| HAT-P-42b
|1.044
|1.28
|4.641878
|0.0575
|1427
|style="background:#FFFF00"|transit
|1460
|1.18
|5743
|[{{citation|arxiv=1212.6448|year=2012|title=HAT-P-42b and HAT-P-43b|doi=10.1051/0004-6361/201220993|last1=Boisse|first1=I.|last2=Hartman|first2=J. D.|last3=Bakos|first3=G. Á.|last4=Penev|first4=K.|last5=Csubry|first5=Z.|last6=Béky|first6=B.|last7=Latham|first7=D. W.|last8=Bieryla|first8=A.|last9=Torres|first9=G.|last10=Kovács|first10=G.|last11=Buchhave|first11=L. A.|last12=Hansen|first12=T.|last13=Everett|first13=M.|last14=Esquerdo|first14=G. A.|last15=Szklenár|first15=T.|last16=Falco|first16=E.|last17=Shporer|first17=A.|last18=Fulton|first18=B. J.|last19=Noyes|first19=R. W.|last20=Stefanik|first20=R. P.|last21=Lázár|first21=J.|last22=Papp|first22=I.|last23=Sári|first23=P.|journal=Astronomy & Astrophysics|volume=558|pages=A86|s2cid=119209692}}] Proper name Iolaus |
| HAT-P-43b
|0.662
|1.281
|3.332687
|0.0443
|1361
|style="background:#FFFF00"|transit
|1770
|1.05
|5645
| |
| HATS-1b
|1.855
|1.302
|3.446459
|0.0444
|
|style="background:#FFFF00"|transit
|990
|0.99
|5870
|[{{citation|arxiv=1206.1524|year=2012|title=HATS-1b: THE FIRST TRANSITING PLANET DISCOVERED BY THE HATSouth SURVEY|doi=10.1088/0004-6256/145/1/5|last1=Penev|first1=K.|last2=Bakos|first2=G. Á.|last3=Bayliss|first3=D.|last4=Jordán|first4=A.|last5=Mohler|first5=M.|last6=Zhou|first6=G.|last7=Suc|first7=V.|last8=Rabus|first8=M.|last9=Hartman|first9=J. D.|last10=Mancini|first10=L.|last11=Béky|first11=B.|last12=Csubry|first12=Z.|last13=Buchhave|first13=L.|last14=Henning|first14=T.|last15=Nikolov|first15=N.|last16=Csák|first16=B.|last17=Brahm|first17=R.|last18=Espinoza|first18=N.|last19=Conroy|first19=P.|last20=Noyes|first20=R. W.|last21=Sasselov|first21=D. D.|last22=Schmidt|first22=B.|last23=Wright|first23=D. J.|last24=Tinney|first24=C. G.|last25=Addison|first25=B. C.|last26=Lázár|first26=J.|last27=Papp|first27=I.|last28=Sári|first28=P.|journal=The Astronomical Journal|volume=145|page=5|s2cid=118556930}}] |
| HD 142 c
|5.3
|
|6005
|6.8
|
|style="background:#00FF00"|radial vel.
|83.6
|1.23
|6245
|[{{citation|arxiv=1205.2765|year=2012|title=The Anglo-Australian Planet Search. Xxii. Two New Multi-Planet Systems|doi=10.1088/0004-637X/753/2/169|last1=Wittenmyer|first1=Robert A.|last2=Horner|first2=J.|last3=Tuomi|first3=Mikko|last4=Salter|first4=G. S.|last5=Tinney|first5=C. G.|last6=Butler|first6=R. P.|last7=Jones|first7=H. R. A.|last8=o'Toole|first8=S. J.|last9=Bailey|first9=J.|last10=Carter|first10=B. D.|last11=Jenkins|first11=J. S.|last12=Zhang|first12=Z.|last13=Vogt|first13=S. S.|last14=Rivera|first14=Eugenio J.|journal=The Astrophysical Journal|volume=753|issue=2|page=169|bibcode=2012ApJ...753..169W|s2cid=2941264}}] |
| HD 4732 b
|2.37
|
|360.2
|1.19
|
|style="background:#00FF00"|radial vel.
|184
|1.74
|4959
|[{{cite journal | title=A Double Planetary System around the Evolved Intermediate-mass Star HD 4732 | last1=Sato | first1=Bun'ei | last2=Omiya | first2=Masashi | last3=Wittenmyer | first3=Robert A. | last4=Harakawa | first4=Hiroki | last5=Nagasawa | first5=Makiko | last6=Izumiura | first6=Hideyuki | last7=Kambe | first7=Eiji | last8=Takeda | first8=Yoichi | last9=Yoshida | first9=Michitoshi | last10=Itoh | first10=Yoichi | last11=Ando | first11=Hiroyasu | last12=Kokubo | first12=Eiichiro | last13=Ida | first13=Shigeru | display-authors=1 | journal=The Astrophysical Journal | volume=762 | issue=1 | at=9 | date=2013 | arxiv=1210.6798 | bibcode=2013ApJ...762....9S | doi=10.1088/0004-637X/762/1/9| s2cid=67838183 }}] |
| HD 4732 c
|2.37
|
|2732
|4.6
|
|style="background:#00FF00"|radial vel.
|184
|1.74
|4959
| |
| HD 5608 b
|1.4
|
|792.6
|1.9
|
|style="background:#00FF00"|radial vel.
|189.7
|1.55
|4854
| |
| HD 24040 b
|4.10{{±|0.12}}
|
|3490{{±|25}}
|4.637{{±|0.067}}
|
|style="background:#00FF00"|radial vel.
|152.3{{±|0.4}}
|1.14{{±|0.02}}
|5917{{±|52}}
|[{{citation |doi=10.1051/0004-6361/201118419 |arxiv=1205.5835 |url=http://www.aanda.org/articles/aa/full_html/2012/09/aa18419-11/aa18419-11.html |title=The SOPHIE search for northern extrasolar planets V. Follow-up of ELODIE candidates: Jupiter-analogs around Sun-like stars |year=2012 |last1=Boisse |first1=Isabelle |last2=Pepe |first2=Francesco |last3=Perrier |first3=Christian |last4=Queloz |first4=Didier |last5=Bonfils |first5=Xavier |last6=Bouchy |first6=François |last7=Santos |first7=Nuno C. |last8=Arnold |first8=Luc |last9=Beuzit |first9=Jean-Luc |last10=Dìaz |first10=Rodrigo F. |last11=Delfosse |first11=Xavier |last12=Eggenberger |first12=Anne |last13=Ehrenreich |first13=David |last14=Forveille |first14=Thierry |last15=Hébrard |first15=Guillaume |last16=Lagrange |first16=Anne-Marie |last17=Lovis |first17=Christophe |last18=Mayor |first18=Michel |last19=Moutou |first19=Claire |last20=Naef |first20=Dominique |last21=Santerne |first21=Alexandre |last22=Ségransan |first22=Damien |last23=Sivan |first23=Jean-Pierre |last24=Udry |first24=Stéphane |journal=Astronomy and Astrophysics |volume=545 |pages=A55 |bibcode=2012A&A...545A..55B |s2cid=119109836 }}] Suspected since 2006 |
| HD 27631 b
|1.45
|
|2208
|3.25
|
|style="background:#00FF00"|radial vel.
|145.3
|0.94
|5737
| |
| HD 37605 c
|3.366
|
|2720
|3.814
|
|style="background:#00FF00"|radial vel.
|139.9
|1
|5448
|[{{Cite journal|title=The Discovery of HD 37605c and a Dispositive Null Detection of Transits of HD 37605b|last1=Wang Xuesong|first1=Sharon|last2=Wright|first2=Jason T.|last3=Cochran|first3=William|last4=Kane|first4=Stephen R.|last5=Henry|first5=Gregory W.|last6=Payne|first6=Matthew J.|last7=Endl|first7=Michael|last8=MacQueen|first8=Phillip J.|last9=Valenti|first9=Jeff A.|last10=Antoci|first10=Victoria|last11=Dragomir|first11=Diana|last12=Matthews|first12=Jaymie M.| last13=Howard|first13=Andrew W.|last14=Marcy|first14=Geoffrey W.|last15=Isaacson| first15=Howard|last16=Ford|first16=Eric B.|last17=Mahadevan|first17=Suvrath |last18=von Braun|first18=Kaspar|display-authors=1|journal=Astrophysical Journal|year=2012|volume=761|issue=1|pages=46|arxiv=1210.6985| bibcode=2012ApJ...761...46W|doi=10.1088/0004-637X/761/1/46|s2cid=118679173}}] |
| HD 40307 e
|0.0110{{±|0.0044}}
|
|34.62{{±|0.21|0.20}}
|0.1886{{±|0.083|0.0104}}
|
|style="background:#00FF00"|radial vel.
|41.8
|0.77
|4956
|[{{citation|arxiv=1211.1617|year=2012|title=Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307|doi=10.1051/0004-6361/201220268|last1=Tuomi|first1=M.|last2=Anglada-Escudé|first2=G.|last3=Gerlach|first3=E.|last4=Jones|first4=H. R. A.|last5=Reiners|first5=A.|last6=Rivera|first6=E. J.|last7=Vogt|first7=S. S.|last8=Butler|first8=R. P.|journal=Astronomy & Astrophysics|volume=549|pages=A48|s2cid=7424216}}] |
| HD 40307 f
|0.0164
|
|51.76
|0.247
|
|style="background:#00FF00"|radial vel.
|41.8
|0.77
|4956
| |
| HD 40307 g
|0.0223
|
|197.8
|0.6
|
|style="background:#00FF00"|radial vel.
|41.8
|0.77
|4956
| |
| HD 66141 b
|6
|
|480.5
|1.2
|
|style="background:#00FF00"|radial vel.
|261.1
|1.1
|4323
|[{{citation|arxiv=1211.2054|year=2012|title=Detection of an exoplanet around the evolved K giant HD 66141|doi=10.1051/0004-6361/201118014|last1=Lee|first1=B.-C.|last2=Mkrtichian|first2=D. E.|last3=Han|first3=I.|last4=Park|first4=M.-G.|last5=Kim|first5=K.-M.|journal=Astronomy & Astrophysics|volume=548|pages=A118|bibcode=2012A&A...548A.118L|s2cid=54984721}}] |
| HD 77338b
|0.05
|
|5.7361
|0.0614
|
|style="background:#00FF00"|radial vel.
|134.6
|0.93
|5370
|[{{citation|arxiv=1207.1012|year=2012|title=A Hot Uranus Orbiting the Super Metal-Rich Star Hd 77338 and the Metallicity-Mass Connection|doi=10.1088/0004-637X/766/2/67|last1=Jenkins|first1=J. S.|last2=Jones|first2=H. R. A.|last3=Tuomi|first3=M.|last4=Murgas|first4=F.|last5=Hoyer|first5=S.|last6=Jones|first6=M. I.|last7=Barnes|first7=J. R.|last8=Pavlenko|first8=Y. V.|last9=Ivanyuk|first9=O.|last10=Rojo|first10=P.|last11=Jordán|first11=A.|last12=Day-Jones|first12=A. C.|last13=Ruiz|first13=M. T.|last14=Pinfield|first14=D. J.|journal=The Astrophysical Journal|volume=766|issue=2|page=67|s2cid=16971803}}] |
| HD 79498 b
|1.34
|
|1807
|2.98
|
|style="background:#00FF00"|radial vel.
|159.89
|1.08
|5748
| |
| HD 98649 b
|6.8
|
|4951
|5.6
|
|style="background:#00FF00"|radial vel.
|139.5
|1
|5759
| |
| HD 106515 Ab
|9.61
|
|3630
|4.59
|
|style="background:#00FF00"|radial vel.
|118.6
|0.97
|5362
| |
| HD 150706 b
|2.71
|
|5894
|6.7
|
|style="background:#00FF00"|radial vel.
|88.8
|1.17
|5961
| |
| HD 159868 c
|0.73
|
|352.3
|1
|
|style="background:#00FF00"|radial vel.
|171.9
|1.09
|5558
| |
| HD 166724 b
|3.53
|
|5144
|5.42
|
|style="background:#00FF00"|radial vel.
|140.2
|0.81
|5127
| |
| HD 197037 b
|0.79
|
|1035.7
|2.07
|
|style="background:#00FF00"|radial vel.
|107.1
|1.063{{±|0.022}}
|6137{{±|20}}
| |
| HD 207832 b
|0.56
|
|161.97
|0.57
|
|style="background:#00FF00"|radial vel.
|180.4
|0.94
|5710
|[{{citation|arxiv=1207.2806|year=2012|title=The Lick-Carnegie Survey: A New Two-Planet System Around the Star Hd 207832|doi=10.1088/0004-637X/756/1/91|last1=Haghighipour|first1=Nader|last2=Butler|first2=R. Paul|last3=Rivera|first3=Eugenio J.|last4=Henry|first4=Gregory W.|last5=Vogt|first5=Steven S.|journal=The Astrophysical Journal|volume=756|issue=1|page=91|bibcode=2012ApJ...756...91H|s2cid=1137984}}] Suspected false positive[{{citation|arxiv=2004.13734|year=2020|title=Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars|doi=10.3847/1538-3881/ab855a|last1=Luhn|first1=Jacob K.|last2=Wright|first2=Jason T.|last3=Howard|first3=Andrew W.|last4=Isaacson|first4=Howard|journal=The Astronomical Journal|volume=159|issue=5|page=235|bibcode=2020AJ....159..235L|s2cid=216642215 |doi-access=free }}] |
| HD 207832 c
|0.73
|
|1155.7
|2.112
|
|style="background:#00FF00"|radial vel.
|180.4
|0.94
|5710
|[ Suspected false positive] |
| HD 208527 b
|9.9
|
|875.5
|2.1
|
|style="background:#00FF00"|radial vel.
|1148.4
|1.6
|4035
| |
| HD 219077 b
|10.39
|
|5501
|6.22
|
|style="background:#00FF00"|radial vel.
|95
|1.05
|5362
| |
| HD 219415 b
|1
|
|2093.3
|3.2
|
|style="background:#00FF00"|radial vel.
|553.7
|1
|4820
| |
| HD 220074 b
|11.1
|
|672.1
|1.6
|
|style="background:#00FF00"|radial vel.
|942.7
|1.2
|3935
|[{{citation|arxiv=1211.2051|year=2012|title=Planetary companions orbiting M giants HD 208527 and HD 220074|doi=10.1051/0004-6361/201220301|last1=Lee|first1=B.-C.|last2=Han|first2=I.|last3=Park|first3=M.-G.|journal=Astronomy & Astrophysics|volume=549|pages=A2|s2cid=73522393}}] |
| HD 220689 b
|1.06
|
|2209
|3.36
|
|style="background:#00FF00"|radial vel.
|147.5
|1.04
|5921
| |
| HD 220773 b
|1.45
|
|3724.7
|4.94
|
|style="background:#00FF00"|radial vel.
|159.82
|1.16
|5940
|[{{cite journal|author1=Robertson, Paul |author2=Endl, Michael |author3=Cochran, William D. |author4=MacQueen, Phillip J. |author5=Wittenmyer, Robert A. |author6=Horner, J. |author7=Brugamyer, Erik J. |author8=Simon, Attila E. |author9=Barnes, Stuart I. |author10=Caldwell, Caroline |date=2012|title=The McDonald Observatory Planet Search: New Long-period Giant Planets and Two Interacting Jupiters in the HD 155358 System|journal=The Astrophysical Journal|volume=749|issue=1|pages=17 pp|bibcode=2012ApJ...749...39R|arxiv=1202.0265 |doi=10.1088/0004-637X/749/1/39|s2cid=59273311 }}] |
| HD 222155 b
|2.12
|
|3999
|5.14
|
|style="background:#00FF00"|radial vel.
|165.3
|1.21
|5701
| |
| HW Virginis b
|14.3
|
|4640
|4.69
|
|style="background:#FF7519"|timing
|590
|0.485
|
|[{{cite journal|title=The quest for companions to post-common envelope binaries. III. A reexamination of HW Virginis|author1=Beuermann, K. |author2=Dreizler, S. |author3=Hessman, F. V. |author4=Deller, J. |date=2012|journal=Astronomy & Astrophysics|volume=543|pages=id.A138|doi=10.1051/0004-6361/201219391|bibcode=2012A&A...543A.138B|arxiv=1206.3080|s2cid=53680945}}] Likely false positive[{{cite arXiv|title=Wobbling Ancient Binaries - Here Be Planets?|author1=Jonathan Horner |author2=Robert Wittenmyer |author3=Tobias Hinse |author4=Jonathan Marshall |author5=Alex Mustill |date=2014|eprint=1401.6742|class=astro-ph.EP}}] |
| Kappa Andromedae b
|13.616
|
|
|55
|1850
|style="background:#FF6CDA"|imaging
|169.7
|2.6
|10900
|Has a reddish color, and may be a brown dwarf[{{cite journal|title=Direct Imaging Discovery of a 'Super-Jupiter' Around the late B-Type Star Kappa And|date=November 15, 2012|arxiv=1211.3744|author1=Carson|author2=Thalmann|author3=Janson|author4=Kozakis|author5=Bonnefoy|author6=Biller|author7=Schlieder|author8=Currie|author9=McElwain|doi=10.1088/2041-8205/763/2/L32|volume=763|issue=2|journal=The Astrophysical Journal|page=L32|bibcode=2013ApJ...763L..32C|s2cid=119253577}}] |
| KELT-1b
|27.23
|1.11
|1.217514
|0.02466
|2423
|style="background:#FFFF00"|transit
|850
|1.32
|6518
|[{{citation|arxiv=1201.5415|year=2012|title=Transit Timing Observations Fromkepler. Iv. Confirmation of Four Multiple-Planet Systems by Simple Physical Models|doi=10.1088/0004-637X/750/2/114|last1=Fabrycky|first1=Daniel C.|last2=Ford|first2=Eric B.|last3=Steffen|first3=Jason H.|last4=Rowe|first4=Jason F.|last5=Carter|first5=Joshua A.|last6=Moorhead|first6=Althea V.|last7=Batalha|first7=Natalie M.|last8=Borucki|first8=William J.|last9=Bryson|first9=Steve|last10=Buchhave|first10=Lars A.|last11=Christiansen|first11=Jessie L.|last12=Ciardi|first12=David R.|last13=Cochran|first13=William D.|last14=Endl|first14=Michael|last15=Fanelli|first15=Michael N.|last16=Fischer|first16=Debra|last17=Fressin|first17=Francois|last18=Geary|first18=John|last19=Haas|first19=Michael R.|last20=Hall|first20=Jennifer R.|last21=Holman|first21=Matthew J.|last22=Jenkins|first22=Jon M.|last23=Koch|first23=David G.|last24=Latham|first24=David W.|last25=Li|first25=Jie|last26=Lissauer|first26=Jack J.|last27=Lucas|first27=Philip|last28=Marcy|first28=Geoffrey W.|last29=Mazeh|first29=Tsevi|last30=McCauliff|first30=Sean|journal=The Astrophysical Journal|volume=750|issue=2|page=114|bibcode=2012ApJ...750..114F|s2cid=9075167|display-authors=1}}] |
| KELT-2Ab
|1.522
|1.286
|4.1137912
|0.05496
|
|style="background:#FFFF00"|transit
|405.2
|1.31
|6151
|[{{cite journal | title=KELT-2Ab: A Hot Jupiter Transiting the Bright (V = 8.77) Primary Star of a Binary System | last1=Beatty | first1=Thomas G. | last2=Pepper | first2=Joshua | last3=Siverd | first3=Robert J. | last4=Eastman | first4=Jason D. | last5=Bieryla | first5=Allyson | last6=Latham | first6=David W. | last7=Buchhave | first7=Lars A. | last8=Jensen | first8=Eric L. N. | last9=Manner | first9=Mark | last10=Stassun | first10=Keivan G. | last11=Gaudi | first11=B. Scott | last12=Berlind | first12=Perry | last13=Calkins | first13=Michael L. | last14=Collins | first14=Karen | last15=DePoy | first15=Darren L. | last16=Esquerdo | first16=Gilbert A. | last17=Fulton | first17=Benjamin J. | last18=Fűrész | first18=Gábor | last19=Geary | first19=John C. | last20=Gould | first20=Andrew | last21=Hebb | first21=Leslie | last22=Kielkopf | first22=John F. | last23=Marshall | first23=Jennifer L. | last24=Pogge | first24=Richard | last25=Stanek | first25=K. Z. | last26=Stefanik | first26=Robert P. | last27=Street | first27=Rachel | last28=Szentgyorgyi | first28=Andrew H. | last29=Trueblood | first29=Mark | last30=Trueblood | first30=Patricia | last31=Stutz | first31=Amelia M. | display-authors=1 | journal=The Astrophysical Journal Letters | volume=756 | issue=2 | at=L39 | year=2012 | arxiv=1206.1592 | bibcode=2012ApJ...756L..39B | doi=10.1088/2041-8205/756/2/L39 | hdl=1969.1/178896| s2cid=14271501 }}] |
| Kepler-30b
|0.036
|0.348
|29.33434
|0.18
|
|style="background:#FFFF00"|transit
|4600
|0.99
|5498
|[{{citation|arxiv=1201.5415|title=Transit Timing Observations Fromkepler. Iv. Confirmation of Four Multiple-Planet Systems by Simple Physical Models|year=2012|doi=10.1088/0004-637X/750/2/114|last1=Fabrycky|first1=Daniel C.|last2=Ford|first2=Eric B.|last3=Steffen|first3=Jason H.|last4=Rowe|first4=Jason F.|last5=Carter|first5=Joshua A.|last6=Moorhead|first6=Althea V.|last7=Batalha|first7=Natalie M.|last8=Borucki|first8=William J.|last9=Bryson|first9=Steve|last10=Buchhave|first10=Lars A.|last11=Christiansen|first11=Jessie L.|last12=Ciardi|first12=David R.|last13=Cochran|first13=William D.|last14=Endl|first14=Michael|last15=Fanelli|first15=Michael N.|last16=Fischer|first16=Debra|last17=Fressin|first17=Francois|last18=Geary|first18=John|last19=Haas|first19=Michael R.|last20=Hall|first20=Jennifer R.|last21=Holman|first21=Matthew J.|last22=Jenkins|first22=Jon M.|last23=Koch|first23=David G.|last24=Latham|first24=David W.|last25=Li|first25=Jie|last26=Lissauer|first26=Jack J.|last27=Lucas|first27=Philip|last28=Marcy|first28=Geoffrey W.|last29=Mazeh|first29=Tsevi|last30=McCauliff|first30=Sean|journal=The Astrophysical Journal|volume=750|issue=2|page=114|bibcode=2012ApJ...750..114F|s2cid=9075167|display-authors=1}}] |
| Kepler-30c
|2.01
|1.097
|60.323105
|0.3
|
|style="background:#FFFF00"|transit
|4600
|0.99
|5498
| |
| Kepler-30d
|0.073
|0.785
|143.34394
|0.5
|
|style="background:#FFFF00"|transit
|4600
|0.99
|5498
| |
| Kepler-32d
|
|0.241
|22.7802
|0.13
|
|style="background:#FFFF00"|transit
|990
|0.58
|3900
| |
| Kepler-32e
|
|0.134
|2.896
|0.033
|
|style="background:#FFFF00"|transit
|990
|0.58
|3900
|Weak evidence |
| Kepler-32f
|
|0.073
|0.74296
|0.013
|
|style="background:#FFFF00"|transit
|990
|0.58
|3900
|Weak evidence |
| Kepler-33f
|0.03036
|0.398
|41.02902
|0.2535
|
|style="background:#FFFF00"|transit
|4086
|1.29
|5904
|[{{cite journal|arxiv=1201.5424|title=Almost All of Kepler's Multiple Planet Candidates are Planets|first1=Jack J.|last1=Lissauer|first2=Geoffrey W.|last2=Marcy|first3=Jason F.|last3=Rowe|first4=Stephen T.|last4=Bryson|first5=Elisabeth|last5=Adams|first6=Lars A.|last6=Buchhave|first7=David R.|last7=Ciardi|first8=William D.|last8=Cochran|first9=Daniel C.|last9=Fabrycky|first10=Eric B.|last10=Ford|first11=Francois|last11=Fressin|first12=John|last12=Geary|first13=Ronald L.|last13=Gilliland|first14=Matthew J.|last14=Holman|first15=Steve B.|last15=Howell|first16=Jon M.|last16=Jenkins|first17=Karen|last17=Kinemuchi|first18=David G.|last18=Koch|first19=Robert C.|last19=Morehead|first20=Darin|last20=Ragozzine|first21=Shawn E.|last21=Seader|first22=Peter G.|last22=Tanenbaum|first23=Guillermo|last23=Torres|first24=Joseph D.|last24=Twicken|date=10 May 2012|journal=The Astrophysical Journal|volume=750|issue=2|pages=112|doi=10.1088/0004-637X/750/2/112|bibcode=2012ApJ...750..112L|s2cid=30549908}}] |
| Kepler-34b
|0.22
|0.764
|288.822
|1.0896
|
|style="background:#FFFF00"|transit
|4889
|1.05
|5913
|[{{cite journal | title=Transiting circumbinary planets Kepler-34 b and Kepler-35 b | last1=Welsh | first1=William F. | last2=Orosz | first2=Jerome A. | last3=Carter | first3=Joshua A. | last4=Fabrycky | first4=Daniel C. | last5=Ford | first5=Eric B. | last6=Lissauer | first6=Jack J. | last7=Prša | first7=Andrej | last8=Quinn | first8=Samuel N. | last9=Ragozzine | first9=Darin | last10=Short | first10=Donald R. | last11=Torres | first11=Guillermo | last12=Winn | first12=Joshua N. | last13=Doyle | first13=Laurance R. | last14=Barclay | first14=Thomas | last15=Batalha | first15=Natalie | last16=Bloemen | first16=Steven | last17=Brugamyer | first17=Erik | last18=Buchhave | first18=Lars A. | last19=Caldwell | first19=Caroline | last20=Caldwell | first20=Douglas A. | last21=Christiansen | first21=Jessie L. | last22=Ciardi | first22=David R. | last23=Cochran | first23=William D. | last24=Endl | first24=Michael | last25=Fortney | first25=Jonathan J. | last26=Gautier III | first26=Thomas N. | last27=Gilliland | first27=Ronald L. | last28=Haas | first28=Michael R. | last29=Hall | first29=Jennifer R. | last30=Holman | first30=Matthew J. | display-authors=1 | journal=Nature | volume=481 | issue=7382 | pages=475–479 | year=2012 | arxiv=1204.3955 | bibcode=2012Natur.481..475W | doi=10.1038/nature10768 | pmid=22237021 | s2cid=4426222}}] |
| Kepler-35b
|0.127
|0.728
|131.458
|0.60347
|
|style="background:#FFFF00"|transit
|5365
|0.89
|5606
| |
| Kepler-36b
|0.014
|0.133
|13.83989
|0.1153
|
|style="background:#FFFF00"|transit
|1500
|1.07
|5911
|[{{cite journal | title=Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities | last1=Carter | first1=J. A. | last2=Agol | first2=E. | last3=Chaplin | first3=W. J. | last4=Basu | first4=S. | last5=Bedding | first5=T. R. | last6=Buchhave | first6=L. A. | last7=Christensen-Dalsgaard | first7=J. | last8=Deck | first8=K. M. | last9=Elsworth | first9=Y. | last10=Fabrycky | first10=D. C. | last11=Ford | first11=E. B. | last12=Fortney | first12=J. J. | last13=Hale | first13=S. J. | last14=Handberg | first14=R. | last15=Hekker | first15=S. | last16=Holman | first16=M. J. | last17=Huber | first17=D. | last18=Karoff | first18=C. | last19=Kawaler | first19=S. D. | last20=Kjeldsen | first20=H. | last21=Lissauer | first21=J. J. | last22=Lopez | first22=E. D. | last23=Lund | first23=M. N. | last24=Lundkvist | first24=M. | last25=Metcalfe | first25=T. S. | last26=Miglio | first26=A. | last27=Rogers | first27=L. A. | last28=Stello | first28=D. | last29=Borucki | first29=W. J. | last30=Bryson | first30=S. | display-authors=1 | journal=Science | volume=337 | issue=6094 | pages=556–559 | year=2012 | arxiv=1206.4718 | bibcode=2012Sci...337..556C | doi=10.1126/science.1223269 |pmid=22722249| s2cid=40245894 }}] |
| Kepler-36c
|0.025
|0.328
|16.23855
|0.1283
|
|style="background:#FFFF00"|transit
|1500
|1.07
|5911
| |
| Kepler-38b
|0.384
|0.384
|105.599
|0.4632
|
|style="background:#FFFF00"|transit
|2000
|0.94
|5623
|[{{citation|arxiv=1208.3712|year=2012|title=THE NEPTUNE-SIZED CIRCUMBINARY PLANET KEPLER-38b|doi=10.1088/0004-637X/758/2/87|last1=Orosz|first1=Jerome A.|last2=Welsh|first2=William F.|last3=Carter|first3=Joshua A.|last4=Brugamyer|first4=Erik|last5=Buchhave|first5=Lars A.|last6=Cochran|first6=William D.|last7=Endl|first7=Michael|last8=Ford|first8=Eric B.|last9=MacQueen|first9=Phillip|last10=Short|first10=Donald R.|last11=Torres|first11=Guillermo|last12=Windmiller|first12=Gur|last13=Agol|first13=Eric|last14=Barclay|first14=Thomas|last15=Caldwell|first15=Douglas A.|last16=Clarke|first16=Bruce D.|last17=Doyle|first17=Laurance R.|last18=Fabrycky|first18=Daniel C.|last19=Geary|first19=John C.|last20=Haghighipour|first20=Nader|last21=Holman|first21=Matthew J.|last22=Ibrahim|first22=Khadeejah A.|last23=Jenkins|first23=Jon M.|last24=Kinemuchi|first24=Karen|last25=Li|first25=Jie|last26=Lissauer|first26=Jack J.|last27=Prša|first27=Andrej|last28=Ragozzine|first28=Darin|last29=Shporer|first29=Avi|last30=Still|first30=Martin|journal=The Astrophysical Journal|volume=758|issue=2|page=87|bibcode=2012ApJ...758...87O|s2cid=119226095|display-authors=1}}] |
| Kepler-46b
|6
|0.808
|33.60134
|0.1968
|
|style="background:#FFFF00"|transit
|2790
|0.9
|5309
|[{{cite journal | title=The Detection and Characterization of a Nontransiting Planet by Transit Timing Variations | last1=Nesvorny | first1=D. | last2=Kipping | first2=D. M. | last3=Buchhave | first3=L. A. | last4=Bakos | first4=G. A. | last5=Hartman | first5=J. | last6=Schmitt | first6=A. R. | display-authors=1 | journal=Science | volume=336 | issue=6085 | pages=1133–6 | year=2012 | arxiv=1208.0942 | bibcode=2012Sci...336.1133N | doi=10.1126/science.1221141 | pmid=22582018 | s2cid=41455466}}] |
| Kepler-46c
|0.376
|
|57.011
|0.2799
|
|style="background:#FF7519"|timing
|2790
|0.9
|5309
| |
| Kepler-47b
|2
|0.27
|49.532
|0.2962
|
|style="background:#FFFF00"|transit
|4900
|1.05
|5636
|[{{Cite journal|arxiv= 1208.5489v1 |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}}] |
| Kepler-47c
|28
|0.411
|303.137
|0.991
|
|style="background:#FFFF00"|transit
|4900
|1.05
|5636
| |
| |Kepler-48b
|0.0124
|0.168
|4.778
|
|
|style="background:#FFFF00"|transit
|1009{{±|5}}
|0.88
|5194
|[{{citation|arxiv=1208.3499|year=2012|title=Transit timing observations from Kepler – VII. Confirmation of 27 planets in 13 multiplanet systems via transit timing variations and orbital stability|doi=10.1093/mnras/sts090|last1=Steffen|first1=Jason H.|last2=Fabrycky|first2=Daniel C.|last3=Agol|first3=Eric|last4=Ford|first4=Eric B.|last5=Morehead|first5=Robert C.|last6=Cochran|first6=William D.|last7=Lissauer|first7=Jack J.|last8=Adams|first8=Elisabeth R.|last9=Borucki|first9=William J.|last10=Bryson|first10=Steve|last11=Caldwell|first11=Douglas A.|last12=Dupree|first12=Andrea|last13=Jenkins|first13=Jon M.|last14=Robertson|first14=Paul|last15=Rowe|first15=Jason F.|last16=Seader|first16=Shawn|last17=Thompson|first17=Susan|last18=Twicken|first18=Joseph D.|journal=Monthly Notices of the Royal Astronomical Society|volume=428|issue=2|pages=1077–1087|doi-access=free }}] |
| |Kepler-48c
|0.04597
|0.242
|9.67395
|
|
|style="background:#FFFF00"|transit
|1009{{±|5}}
|0.88
|5194
| |
| |{{interlanguage link|Kepler-49|lt=Kepler-49b|ru|Kepler-49}}
|0.98
|0.243
|7.2037945
|
|
|style="background:#FFFF00"|transit
|1024{{±|8}}
|0.55
|4252
| |
| |{{interlanguage link|Kepler-49|lt=Kepler-49c|ru|Kepler-49}}
|0.72
|0.227
|10.9129343
|
|
|style="background:#FFFF00"|transit
|1024{{±|8}}
|0.55
|4252
| |
| |{{interlanguage link|Kepler-50|lt=Kepler-50b|ru|Kepler-50}}
|
|0.153
|7.81254
|0.077
|
|style="background:#FFFF00"|transit
|821{{±|6}}
|1.24
|6225
| |
| |{{interlanguage link|Kepler-50|lt=Kepler-50c|ru|Kepler-50}}
|
|0.194
|9.37647
|0.087
|
|style="background:#FFFF00"|transit
|821{{±|6}}
|1.24
|6225
| |
| Kepler-51b
|0.007
|0.633
|45.154
|0.2514
|543
|style="background:#FFFF00"|transit
|2610{{±|50}}
|1.04
|6018
| |
| Kepler-51c
|0.013
|0.803
|85.312
|0.384
|439
|style="background:#FFFF00"|transit
|2610{{±|50}}
|1.04
|6018
| |
| |{{interlanguage link|Kepler-52|lt=Kepler-52b|ru|Kepler-52}}
|8.7
|0.187
|7.8773565
|
|
|style="background:#FFFF00"|transit
|1058{{±|7}}
|0.54
|4263
| |
| |{{interlanguage link|Kepler-52|lt=Kepler-52c|ru|Kepler-52}}
|10.41
|0.164
|16.3850021
|
|
|style="background:#FFFF00"|transit
|1058{{±|7}}
|0.54
|4263
| |
| |{{interlanguage link|Kepler-53|lt=Kepler-53b|ru|Kepler-53}}
|18.41
|0.258
|18.6489525
|
|
|style="background:#FFFF00"|transit
|4600{{±|200}}
|0.98
|5858
| |
| |{{interlanguage link|Kepler-53|lt=Kepler-53c|ru|Kepler-53}}
|15.74
|0.283
|38.5583038
|
|
|style="background:#FFFF00"|transit
|4600{{±|200}}
|0.98
|5858
| |
| |{{interlanguage link|Kepler-54|lt=Kepler-54b|ru|Kepler-54}}
|0.92
|0.187
|8.0109434
|
|
|style="background:#FFFF00"|transit
|893{{±|9}}
|0.51
|4252
| |
| |{{interlanguage link|Kepler-54|lt=Kepler-54c|ru|Kepler-54}}
|0.37
|0.11
|12.0717249
|
|
|style="background:#FFFF00"|transit
|893{{±|9}}
|0.51
|4252
| |
| |{{interlanguage link|Kepler-55|lt=Kepler-55b|ru|Kepler-55}}
|1.49
|0.217
|27.9481449
|
|
|style="background:#FFFF00"|transit
|1920{{±|30}}
|0.62
|4503
| |
| |{{interlanguage link|Kepler-55|lt=Kepler-55c|ru|Kepler-55}}
|1.11
|0.197
|42.1516418
|
|
|style="background:#FFFF00"|transit
|1920{{±|30}}
|0.62
|4503
| |
| Kepler-56b
|0.07
|0.581
|10.5016
|0.1028
|
|style="background:#FFFF00"|transit
|3060{{±|80}}
|1.32
|4840
| |
| Kepler-56c
|0.57
|0.874
|21.40239
|0.1652
|
|style="background:#FFFF00"|transit
|3060{{±|80}}
|1.32
|4840
| |
| |{{interlanguage link|Kepler-57|lt=Kepler-57b|ru|Kepler-57}}
|18.86
|0.195
|5.7293196
|0.057
|
|style="background:#FFFF00"|transit
|3140{{±|30}}
|0.83
|5145
| |
| |{{interlanguage link|Kepler-57|lt=Kepler-57c|ru|Kepler-57}}
|6.95
|0.138
|11.6092567
|0.092
|631
|style="background:#FFFF00"|transit
|3140{{±|30}}
|0.83
|5145
| |
| |{{interlanguage link|Kepler-58|lt=Kepler-58b|ru|Kepler-58}}
|1.39
|0.248
|10.2184954
|
|
|style="background:#FFFF00"|transit
|3250{{±|80}}
|0.95
|6099
| |
| |{{interlanguage link|Kepler-58|lt=Kepler-58c|ru|Kepler-58}}
|2.19
|0.255
|15.5741568
|
|
|style="background:#FFFF00"|transit
|3250{{±|80}}
|0.95
|6099
| |
| Kepler-59b
|2.05
|0.098
|11.8681707
|
|
|style="background:#FFFF00"|transit
|3925{{±|75}}
|1.04
|6074
| |
| Kepler-59c
|1.37
|0.177
|17.9801235
|
|
|style="background:#FFFF00"|transit
|3925{{±|75}}
|1.04
|6074
| |
| |{{interlanguage link|Kepler-60|lt=Kepler-60b|ru|Kepler-60}}
|0.01318
|0.153
|7.1334
|
|
|style="background:#FFFF00"|transit
|3440{{±|70}}
|1.04
|5905
| |
| |{{interlanguage link|Kepler-60|lt=Kepler-60c|ru|Kepler-60}}
|0.01211
|0.17
|8.9187
|
|
|style="background:#FFFF00"|transit
|3440{{±|70}}
|1.04
|5905
| |
| Kepler-60d
|0.01309
|0.178
|11.8981
|
|
|style="background:#FFFF00"|transit
|3440{{±|70}}
|1.04
|5905
| |
| Kepler-64b
|0.531
|0.551
|138.317
|0.652
|
|style="background:#FFFF00"|transit
|6200{{±|1000}}
|1.53
|6407
|[{{Cite journal|last1=Kostov|first1=V. B.|last2=McCullough|first2=P. R.|last3=Hinse|first3=T. C.|last4=Tsvetanov|first4=Z. I.|last5=Hébrard|first5=G.|last6=Díaz|first6=R. F.|last7=Deleuil|first7=M.|last8=Valenti|first8=J. A.|date=2013-01-01|title=A Gas Giant Circumbinary Planet Transiting the F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the Two Transiting Planets in the Kepler-47 System|journal=The Astrophysical Journal|language=en|volume=770|issue=1|pages=52|doi=10.1088/0004-637X/770/1/52|issn=0004-637X|arxiv = 1210.3850 |bibcode = 2013ApJ...770...52K |s2cid=119279690}}] Quadruple star system |
| Kepler-79b
|0.0343
|0.31
|13.4845
|0.117
|868
|style="background:#FFFF00"|transit
|3430{{±|60}}
|1.17
|6174
| |
| Kepler-79c
|0.019
|0.332
|27.4029
|0.187
|685
|style="background:#FFFF00"|transit
|3430{{±|60}}
|1.17
|6174
| |
| Kepler-80b
|0.0218
|0.238
|7.05246
|0.0648
|
|style="background:#FFFF00"|transit
|1160
|0.73
|4540
| |
| Kepler-80c
|0.02121
|0.244
|9.52355
|0.0792
|
|style="background:#FFFF00"|transit
|1160
|0.73
|4540
| |
| Kepler-81b
|
|0.216
|5.955
|
|646
|style="background:#FFFF00"|transit
|1147{{±|10}}
|0.64
|4500
| |
| Kepler-81c
|
|0.211
|12.04
|
|513
|style="background:#FFFF00"|transit
|1147{{±|10}}
|0.64
|4500
| |
| Kepler-82b
|
|0.357
|26.444
|
|581
|style="background:#FFFF00"|transit
|3030{{±|80}}
|0.85
|5428
|[{{citation|arxiv=1208.3312|title=Transit Timing Variation of Near-Resonance Planetary Pairs: Confirmation of 12 Multiple-Planet Systems|year=2012|doi=10.1088/0067-0049/208/2/22|last1=Xie|first1=Ji-Wei|journal=The Astrophysical Journal Supplement Series|volume=208|issue=2|page=22|bibcode=2013ApJS..208...22X |s2cid=17160267}}] |
| Kepler-82c
|
|0.477
|51.538
|
|464
|style="background:#FFFF00"|transit
|3030{{±|80}}
|0.85
|5428
| |
| Kepler-83b
|
|0.252
|9.77
|
|
|style="background:#FFFF00"|transit
|1320{{±|17}}
|0.66
|4648
|[{{citation|arxiv=1402.6534|year=2014|title=Validation Ofkepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-Planet Systems|doi=10.1088/0004-637X/784/1/45|last1=Rowe|first1=Jason F.|last2=Bryson|first2=Stephen T.|last3=Marcy|first3=Geoffrey W.|last4=Lissauer|first4=Jack J.|last5=Jontof-Hutter|first5=Daniel|last6=Mullally|first6=Fergal|last7=Gilliland|first7=Ronald L.|last8=Issacson|first8=Howard|last9=Ford|first9=Eric|last10=Howell|first10=Steve B.|last11=Borucki|first11=William J.|last12=Haas|first12=Michael|last13=Huber|first13=Daniel|last14=Steffen|first14=Jason H.|last15=Thompson|first15=Susan E.|last16=Quintana|first16=Elisa|last17=Barclay|first17=Thomas|last18=Still|first18=Martin|last19=Fortney|first19=Jonathan|last20=Gautier|first20=T. N.|last21=Hunter|first21=Roger|last22=Caldwell|first22=Douglas A.|last23=Ciardi|first23=David R.|last24=Devore|first24=Edna|last25=Cochran|first25=William|last26=Jenkins|first26=Jon|last27=Agol|first27=Eric|last28=Carter|first28=Joshua A.|last29=Geary|first29=John|journal=The Astrophysical Journal|volume=784|issue=1|page=45|bibcode=2014ApJ...784...45R|s2cid=119118620}}] |
| Kepler-83c
|
|0.211
|20.09
|
|
|style="background:#FFFF00"|transit
|1320{{±|17}}
|0.66
|4648
| |
| Kepler-84b
|
|0.199
|8.726
|
|937
|style="background:#FFFF00"|transit
|4700{{±|500}}
|1
|6031
| |
| Kepler-84c
|
|0.211
|12.883
|
|821
|style="background:#FFFF00"|transit
|4700{{±|500}}
|1
|6031
| |
| Kepler-85b
|
|0.176
|8.306
|
|
|style="background:#FFFF00"|transit
|2550{{±|50}}
|0.92
|5436
|[ KOI-2038][{{citation|arxiv=1308.0996|title=Eight Planets in Four Multi-Planet Systems Via Transit Timing Variations in 1350 Days|year=2013|doi=10.1088/0004-637X/778/2/110|last1=Yang|first1=Ming|last2=Liu|first2=Hui-Gen|last3=Zhang|first3=Hui|last4=Yang|first4=Jia-Yi|last5=Zhou|first5=Ji-Lin|journal=The Astrophysical Journal|volume=778|issue=2|page=110|bibcode=2013ApJ...778..110Y|s2cid=117080296}}] |
| Kepler-85c
|
|0.194
|12.513
|
|
|style="background:#FFFF00"|transit
|2550{{±|50}}
|0.92
|5436
|[ KOI-2038] |
| {{ill|MOA-2011-BLG-293Lb|ja|MOA-2011-BLG-293Lb}}
|2.4{{±|1.4|0.9}}
|
|
|1.0{{±|0.1}}
|
|style="background:#0099FF"|microlensing
|23000{{±|2000}}
|0.675{{±|0.525}}
|
|[{{citation|arxiv=1201.1002|year=2012|title=MOA-2011-BLG-293Lb: A TEST OF PURE SURVEY MICROLENSING PLANET DETECTIONS|doi=10.1088/0004-637X/755/2/102 |last1=Yee |first1=J. C. |last2=Shvartzvald |first2=Y. |last3=Gal-Yam |first3=A. |last4=Bond |first4=I. A. |last5=Udalski |first5=A. |last6=Kozłowski |first6=S. |last7=Han |first7=C. |last8=Gould |first8=A. |last9=Skowron |first9=J. |last10=Suzuki |first10=D. |last11=Abe |first11=F. |last12=Bennett |first12=D. P. |last13=Botzler |first13=C. S. |last14=Chote |first14=P. |last15=Freeman |first15=M. |last16=Fukui |first16=A. |last17=Furusawa |first17=K. |last18=Itow |first18=Y. |last19=Kobara |first19=S. |last20=Ling |first20=C. H. |last21=Masuda |first21=K. |last22=Matsubara |first22=Y. |last23=Miyake |first23=N. |last24=Muraki |first24=Y. |last25=Ohmori |first25=K. |last26=Ohnishi |first26=K. |last27=Rattenbury |first27=N. J. |last28=Saito |first28=To. |last29=Sullivan |first29=D. J. |last30=Sumi |first30=T. |journal=The Astrophysical Journal |volume=755 |issue=2 |page=102 |bibcode=2012ApJ...755..102Y |display-authors=1 }}] |
| MOA-2010-BLG-073Lb
|11
|
|
|1.21
|
|style="background:#0099FF"|microlensing
|9100
|0.16
|
|Possibly brown dwarf[{{citation|arxiv=1211.3782|year=2012|title=Moa-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary|doi=10.1088/0004-637X/763/1/67|last1=Street|first1=R. A.|last2=Choi|first2=J.-Y.|last3=Tsapras|first3=Y.|last4=Han|first4=C.|last5=Furusawa|first5=K.|last6=Hundertmark|first6=M.|last7=Gould|first7=A.|last8=Sumi|first8=T.|last9=Bond|first9=I. A.|last10=Wouters|first10=D.|last11=Zellem|first11=R.|last12=Udalski|first12=A.|last13=Snodgrass|first13=C.|last14=Horne|first14=K.|last15=Dominik|first15=M.|last16=Browne|first16=P.|last17=Kains|first17=N.|last18=Bramich|first18=D. M.|last19=Bajek|first19=D.|last20=Steele|first20=I. A.|last21=Ipatov|first21=S.|last22=Abe|first22=F.|last23=Bennett|first23=D. P.|last24=Botzler|first24=C. S.|last25=Chote|first25=P.|last26=Freeman|first26=M.|last27=Fukui|first27=A.|last28=Harris|first28=P.|last29=Itow|first29=Y.|last30=Ling|first30=C. H.|journal=The Astrophysical Journal|volume=763|page=67|s2cid=53710373|display-authors=1}}] |
| MOA-2010-BLG-477Lb
|1.4{{±|0.3}}
|
|
|2.8{{±|0.5}}
|
|style="background:#0099FF"|microlensing
|7500{{±|2000}}
|0.53{{±|0.11}}
|5950{{±|150}}
|[{{cite journal|arxiv=1205.6323|bibcode=2012ApJ...754...73B|title=MOA-2010-BLG-477Lb: Constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light|last1=Bachelet|first1=E.|last2=Shin|first2=I.-G.|last3=Han|first3=C.|last4=Fouqué|first4=P.|last5=Gould|first5=A.|last6=Menzies|first6=J. W.|last7=Beaulieu|first7=J.-P.|last8=Bennett|first8=D. P.|last9=Bond|first9=I. A. |journal=The Astrophysical Journal|display-authors=8 |year=2012|volume=754|issue=1|page=73|doi=10.1088/0004-637X/754/1/73|s2cid=119223374}}] White dwarf host star[{{citation|arxiv=2110.07934|year=2021|title=A Jovian analogue orbiting a white dwarf star|doi=10.1038/s41586-021-03869-6|last1=Blackman|first1=J. W.|last2=Beaulieu|first2=J. P.|last3=Bennett|first3=D. P.|last4=Danielski|first4=C.|last5=Alard|first5=C.|last6=Cole|first6=A. A.|last7=Vandorou|first7=A.|last8=Ranc|first8=C.|last9=Terry|first9=S. K.|last10=Bhattacharya|first10=A.|last11=Bond|first11=I.|last12=Bachelet|first12=E.|last13=Veras|first13=D.|last14=Koshimoto|first14=N.|last15=Batista|first15=V.|last16=Marquette|first16=J. B.|journal=Nature|volume=598|issue=7880|pages=272–275|pmid=34646001|bibcode=2021Natur.598..272B|s2cid=238860454}}] |
| MOA-bin-1Lb
|3.7{{±|2.1}}
|
|
|8.3{{±|4.5|2.7}}
|
|style="background:#0099FF"|microlensing
|17000
|0.75{{±|0.33|0.41}}
|
|[{{citation|arxiv=1203.4560|title=Planetary and Other Short Binary Microlensing Events from the Moa Short-Event Analysis|year=2012|doi=10.1088/0004-637X/757/2/119|last1=Bennett|first1=D. P.|last2=Sumi|first2=T.|last3=Bond|first3=I. A.|last4=Kamiya|first4=K.|last5=Abe|first5=F.|last6=Botzler|first6=C. S.|last7=Fukui|first7=A.|last8=Furusawa|first8=K.|last9=Itow|first9=Y.|last10=Korpela|first10=A. V.|last11=Kilmartin|first11=P. M.|last12=Ling|first12=C. H.|last13=Masuda|first13=K.|last14=Matsubara|first14=Y.|last15=Miyake|first15=N.|last16=Muraki|first16=Y.|last17=Ohnishi|first17=K.|last18=Rattenbury|first18=N. J.|last19=Saito|first19=To.|last20=Sullivan|first20=D. J.|last21=Suzuki|first21=D.|last22=Sweatman|first22=W. L.|last23=Tristram|first23=P. J.|last24=Wada|first24=K.|last25=Yock|first25=P. C. M.|author26=MOA Collaboration|journal=The Astrophysical Journal|volume=757|issue=2|page=119|bibcode=2012ApJ...757..119B|s2cid=118493329}}] |
| Mu2 Octantis b
|6.9
|
|3638
|5.02
|
|style="background:#00FF00"|radial vel.
|142.1
|1.29
|6017
|[{{cite journal | title=The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets | last1=Marmier | first1=M. | last2=Ségransan | first2=D. | last3=Udry | first3=S. | last4=Mayor | first4=M. | last5=Pepe | first5=F. | last6=Queloz | first6=D. | last7=Lovis | first7=C. | last8=Naef | first8=D. | last9=Santos | first9=N. C. | last10=Alonso | first10=R. | last11=Alves | first11=S. | last12=Berthet | first12=S. | last13=Chazelas | first13=B. | last14=Demory | first14=B.-O. | last15=Dumusque | first15=X. | last16=Eggenberger | first16=A. | last17=Figueira | first17=P. | last18=Gillon | first18=M. | last19=Hagelberg | first19=J. | last20=Lendl | first20=M. | last21=Mardling | first21=R. A. | last22=Mégevand | first22=D. | last23=Neveu | first23=M. | last24=Sahlmann | first24=J. | last25=Sosnowska | first25=D. | last26=Tewes | first26=M. | last27=Triaud | first27=A. H. M. J. | display-authors=1 | journal=Astronomy and Astrophysics | volume=551 | at=A90 | year=2013 | arxiv=1211.6444 | bibcode=2013A&A...551A..90M | doi=10.1051/0004-6361/201219639 | s2cid=59467665}}] |
| Nu Ophiuchi b
|24
|
|530.32
|1.9
|
|style="background:#00FF00"|radial vel.
|152.8
|3.04
|4928
|Brown dwarf or small star |
| Nu Ophiuchi c
|27
|
|3186
|6.1
|
|style="background:#00FF00"|radial vel.
|152.8
|3.04
|4928
|Brown dwarf or small star |
| OGLE-2012-BLG-0026Lb
|0.145
|
|
|4
|
|style="background:#0099FF"|microlensing
|13110
|1.06
|
|[{{citation|arxiv=1210.4265|title=THE SECOND MULTIPLE-PLANET SYSTEM DISCOVERED BY MICROLENSING: OGLE-2012-BLG-0026Lb, c—A PAIR OF JOVIAN PLANETS BEYOND THE SNOW LINE|year=2012|doi=10.1088/2041-8205/762/2/L28|last1=Han|first1=C.|last2=Udalski|first2=A.|last3=Choi|first3=J.-Y.|last4=Yee|first4=J. C.|last5=Gould|first5=A.|last6=Christie|first6=G.|last7=Tan|first7=T.-G.|last8=Szymański|first8=M. K.|last9=Kubiak|first9=M.|last10=Soszyński|first10=I.|last11=Pietrzyński|first11=G.|last12=Poleski|first12=R.|last13=Ulaczyk|first13=K.|last14=Pietrukowicz|first14=P.|last15=Kozłowski|first15=S.|last16=Skowron|first16=J.|last17=Wyrzykowski|first17=Ł.|last18=Almeida|first18=L. A.|last19=Batista|first19=V.|last20=Depoy|first20=D. L.|last21=Dong|first21=Subo|last22=Drummond|first22=J.|last23=Gaudi|first23=B. S.|last24=Hwang|first24=K.-H.|last25=Jablonski|first25=F.|last26=Jung|first26=Y.-K.|last27=Lee|first27=C.-U.|last28=Koo|first28=J.-R.|last29=McCormick|first29=J.|last30=Monard|first30=L. A. G.|journal=The Astrophysical Journal|volume=762|issue=2|pages=L28|s2cid=118797226|display-authors=1}}] |
| OGLE-2012-BLG-0026Lc
|0.86
|
|
|4.8
|
|style="background:#0099FF"|microlensing
|13110
|1.06
|
| |
| Omicron Coronae Borealis b
|1.5
|
|187.83
|0.83
|
|style="background:#00FF00"|radial vel.
|274.1
|2.13
|4749
| |
| Omicron Ursae Majoris b
|4.1
|
|1630
|3.9
|
|style="background:#00FF00"|radial vel.
|183.7
|3.09
|5242
|[{{cite journal | title=Substellar Companions to Seven Evolved Intermediate-Mass Stars | last1=Sato | first1=Bun'ei | last2=Omiya | first2=Masashi | last3=Harakawa | first3=Hiroki | last4=Izumiura | first4=Hideyuki | last5=Kambe | first5=Eiji | last6=Takeda | first6=Yoichi | last7=Yoshida | first7=Michitoshi | last8=Itoh | first8=Yoichi | last9=Ando | first9=Hiroyasu | last10=Kokubo | first10=Eiichiro | last11=Ida | first11=Shigeru | display-authors=1 | journal=Publications of the Astronomical Society of Japan | volume=64 | issue=6 | at=135 | year=2012 | arxiv=1207.3141 | bibcode=2012PASJ...64..135S | doi=10.1093/pasj/64.6.135 | s2cid=119197073}}] |
| Pr0201 b
|0.54
|
|4.4264
|
|
|style="background:#00FF00"|radial vel.
|610
|1.23
|6174
|[ In Beehive Cluster] |
| Pr0211 b
|1.88
|
|2.1461
|0.03176
|
|style="background:#00FF00"|radial vel.
|610
|0.94
|5300
|[{{cite journal |doi=10.1088/2041-8205/756/2/L33| title=TWO "b"s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER| journal=The Astrophysical Journal| volume=756| issue=2| pages=L33| year=2012| last1=Quinn| first1=Samuel N.| last2=White| first2=Russel J.| last3=Latham| first3=David W.| last4=Buchhave| first4=Lars A.| last5=Cantrell| first5=Justin R.| last6=Dahm| first6=Scott E.| last7=Fűrész| first7=Gabor| last8=Szentgyorgyi| first8=Andrew H.| last9=Geary| first9=John C.| last10=Torres| first10=Guillermo| last11=Bieryla| first11=Allyson| last12=Berlind| first12=Perry| last13=Calkins| first13=Michael C.| last14=Esquerdo| first14=Gilbert A.| last15=Stefanik| first15=Robert P.| arxiv=1207.0818| bibcode=2012ApJ...756L..33Q| s2cid=118825401}}] Multi-planet system In Beehive Cluster |
| RR Caeli b
|3.0{{±|0.3}}
|
|1900{{±|40}}
|5.2{{±|0.1}}
|
|style="background:#FF7519"|timing
|69.10{{±|0.03}}
|0.18+0.44
|3100+7540
|Circumbinary planet around red and white dwarfs.[{{citation|arxiv=2109.09397|year=2021|title=Two circumbinary planets in RR Cae eclipsing binary system|last1=Rattanamala|first1=R.|last2=Awiphan|first2=S.|last3=Komonjinda|first3=S.|last4=Phriksee|first4=A.|last5=Sappankum|first5=P.|last6=A-thano|first6=N.|last7=Chitchak|first7=S.|last8=Rittipruk|first8=P.|last9=Sawangwit|first9=U.|last10=Poshyachinda|first10=S.|last11=Reichart|first11=D. E.|last12=Haislip|first12=J. B.}}][{{Cite journal | last1 = Qian | first1 = S. B. | last2 = Liu | first2 = L. | last3 = Zhu | first3 = L. Y. | last4 = Dai | first4 = Z. B. | last5 = Fernández Lajús | first5 = E. | last6 = Baume | first6 = G. L. | doi = 10.1111/j.1745-3933.2012.01228.x | title = A circumbinary planet in orbit around the short-period white dwarf eclipsing binary RR Cae | journal = Monthly Notices of the Royal Astronomical Society: Letters | volume = 422 | pages = L24–L27 | year = 2012 | issue = 1 | doi-access = free |arxiv = 1201.4205 |bibcode = 2012MNRAS.422L..24Q | s2cid = 119190656}}] |
| Tau Ceti e
|0.0124
|
|162.87
|0.538
|
|style="background:#00FF00"|radial vel.
|12
|0.78
|
|[{{cite journal|arxiv=1212.4277|bibcode=2012yCat..35510079T |doi=10.1051/0004-6361/201220509 |year=2013|title=Signals embedded in the radial velocity noise |journal=Astronomy & Astrophysics |volume=551 |pages=A79 |last1=Tuomi |first1=M |last2=Jones |first2=H R A |last3=Jenkins |first3=J S |last4=Tinney |first4=C G |last5=Butler |first5=R P |last6=Vogt |first6=S S |last7=Barnes |first7=J R |last8=Wittenmyer |first8=R A |last9=o'Toole |first9=S |last10=Horner |first10=J |last11=Bailey |first11=J |last12=Carter |first12=B D |last13=Wright |first13=D J |last14=Salter |first14=G S |last15=Pinfield |first15=D |s2cid=2390534 }}] Potentially habitable exoplanet |
| Tau Ceti f
|0.0124
|
|636.13
|1.334
|
|style="background:#00FF00"|radial vel.
|12
|0.78
|
| |
| WASP-42b
|0.527
|1.122
|4.9816819
|0.0561
|1021{{±|19}}
|style="background:#FFFF00"|transit
|520
|0.95
|5315
| |
| WASP-47b
|1.21
|1.15
|4.16071
|0.052
|1275
|style="background:#FFFF00"|transit
|650
|1.11
|5576
|[{{citation|arxiv=1204.5095|title=Seven transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b and WASP-67b|year=2012|doi=10.1111/j.1365-2966.2012.21780.x|last1=Hellier|first1=Coel|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Jehin|first7=E.|last8=Lendl|first8=M.|last9=Maxted|first9=P. F. L.|last10=Pepe|first10=F.|last11=Pollacco|first11=D.|last12=Queloz|first12=D.|last13=Ségransan|first13=D.|last14=Smalley|first14=B.|last15=Smith|first15=A. M. S.|last16=Southworth|first16=J.|last17=Triaud|first17=A. H. M. J.|last18=Udry|first18=S.|last19=West|first19=R. G.|journal=Monthly Notices of the Royal Astronomical Society|volume=426|issue=1|pages=739–750|doi-access=free |bibcode=2012MNRAS.426..739H|s2cid=54713354}}] |
| WASP-49b
|0.378
|1.115
|2.7817387
|0.0379
|1369{{±|39}}
|style="background:#FFFF00"|transit
|550
|0.94
|5600
|[{{citation|arxiv=1205.2757|title=WASP-42 b and WASP-49 b: Two new transiting sub-Jupiters|year=2012|doi=10.1051/0004-6361/201219585|last1=Lendl|first1=M.|last2=Anderson|first2=D. R.|last3=Collier-Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Gillon|first5=M.|last6=Hellier|first6=C.|last7=Jehin|first7=E.|last8=Lister|first8=T. A.|last9=Maxted|first9=P. F. L.|last10=Pepe|first10=F.|last11=Pollacco|first11=D.|last12=Queloz|first12=D.|last13=Smalley|first13=B.|last14=Ségransan|first14=D.|last15=Smith|first15=A. M. S.|last16=Triaud|first16=A. H. M. J.|last17=Udry|first17=S.|last18=West|first18=R. G.|last19=Wheatley|first19=P. J.|journal=Astronomy & Astrophysics|volume=544|pages=A72|bibcode=2012A&A...544A..72L|s2cid=54186638}}] |
| WASP-52b
|0.46
|1.27
|1.7497798
|0.0272
|1315{{±|35}}
|style="background:#FFFF00"|transit
|460
|0.87
|5000
|[{{citation|arxiv=1211.0810|title=WASP-52b, WASP-58b, WASP-59b, and WASP-60b: Four new transiting close-in giant planets|year=2012|doi=10.1051/0004-6361/201220363|last1=Hébrard|first1=G.|last2=Collier Cameron|first2=A.|last3=Brown|first3=D. J. A.|last4=Díaz|first4=R. F.|last5=Faedi|first5=F.|last6=Smalley|first6=B.|last7=Anderson|first7=D. R.|last8=Armstrong|first8=D.|last9=Barros|first9=S. C. C.|last10=Bento|first10=J.|last11=Bouchy|first11=F.|last12=Doyle|first12=A. P.|last13=Enoch|first13=B.|last14=Gómez Maqueo Chew|first14=Y.|last15=Hébrard|first15=É. M.|last16=Hellier|first16=C.|last17=Lendl|first17=M.|last18=Lister|first18=T. A.|last19=Maxted|first19=P. F. L.|last20=McCormac|first20=J.|last21=Moutou|first21=C.|last22=Pollacco|first22=D.|last23=Queloz|first23=D.|last24=Santerne|first24=A.|last25=Skillen|first25=I.|last26=Southworth|first26=J.|last27=Tregloan-Reed|first27=J.|last28=Triaud|first28=A. H. M. J.|last29=Udry|first29=S.|last30=Vanhuysse|first30=M.|journal=Astronomy & Astrophysics|volume=549|pages=A134|s2cid=54502046|display-authors=1}}] Proper name Göktürk |
| WASP-54b
|0.636
|1.653
|3.6936411
|0.04987
|1742{{±|49|69}}
|style="background:#FFFF00"|transit
|650
|1.21
|6100
| |
| WASP-55b
|0.627
|1.335
|4.4656291
|0.0558
|1290
|style="background:#FFFF00"|transit
|1100
|1.16
|6070
| |
| WASP-56b
|0.571
|1.092
|4.617101
|0.05458
|1200
|style="background:#FFFF00"|transit
|830
|1.03
|5600
|[{{cite journal|last1=Faedi|first1=F.|display-authors=etal|year=2013|title=WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP|journal=Astronomy & Astrophysics|volume=551|pages=A73|arxiv=1210.2329|bibcode=2013A&A...551A..73F|doi=10.1051/0004-6361/201220520|s2cid=14346225}}] |
| WASP-57b
|0.644
|1.05
|2.83891856
|0.03769
|1338{{±|29}}
|style="background:#FFFF00"|transit
|1480
|0.89
|5600
| |
| WASP-58b
|0.89
|1.37
|5.01718
|0.0561
|1270{{±|80}}
|style="background:#FFFF00"|transit
|980
|0.94
|5800
| |
| WASP-59b
|0.863
|0.775
|7.919585
|0.0697
|670{{±|35}}
|style="background:#FFFF00"|transit
|410
|0.72
|4650
| |
| WASP-60b
|0.514
|0.86
|4.3050011
|0.0531
|1479{{±|35}}
|style="background:#FFFF00"|transit
|1300
|1.08
|5900
|[ Proper name Vlasina] |
| WASP-61b
|2.06
|1.24
|3.8559
|0.0514
|1565{{±|35}}
|style="background:#FFFF00"|transit
|1600
|1.22
|6320
| |
| WASP-62b
|0.57
|1.39
|4.411953
|0.0567
|1329.6{{±|44.8}}
|style="background:#FFFF00"|transit
|520
|1.25
|6280
|[ Proper name Krotoa] |
| WASP-63b
|0.38
|1.43
|4.37809
|0.0574
|1536{{±|37}}
|style="background:#FFFF00"|transit
|1100
|1.32
|5570
| |
| WASP-64b
|1.271
|1.271
|1.5732918
|0.02648
|1989{{±|87|88}}
|style="background:#FFFF00"|transit
|1100
|1
|5400
|[{{citation|arxiv=1210.4257|title=WASP-64 b and WASP-72 b: Two new transiting highly irradiated giant planets|year=2012|doi=10.1051/0004-6361/201220561|last1=Gillon|first1=M.|last2=Anderson|first2=D. R.|last3=Collier-Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Hellier|first6=C.|last7=Jehin|first7=E.|last8=Lendl|first8=M.|last9=Maxted|first9=P. F. L.|last10=Montalbán|first10=J.|last11=Pepe|first11=F.|last12=Pollacco|first12=D.|last13=Queloz|first13=D.|last14=Ségransan|first14=D.|last15=Smith|first15=A. M. S.|last16=Smalley|first16=B.|last17=Southworth|first17=J.|last18=Triaud|first18=A. H. M. J.|last19=Udry|first19=S.|last20=West|first20=R. G.|journal=Astronomy & Astrophysics|volume=552|pages=A82|s2cid=53687206}}] Proper name Agouto |
| WASP-66b
|2.32
|1.39
|4.086052
|0.0546
|1790{{±|60}}
|style="background:#FFFF00"|transit
|1200
|1.3
|6580
| |
| WASP-67b
|0.42
|1.4
|4.61442
|0.0517
|1050
|style="background:#FFFF00"|transit
|730
|0.87
|5240
| |
| WASP-71b
|2.242
|1.46
|2.9036747
|0.04619
|2016.1{{±|67.0|52.5}}
|style="background:#FFFF00"|transit
|1130
|1.56
|6059
|[{{citation|arxiv=1211.3045|title=WASP-71b: A bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star|year=2013|doi=10.1051/0004-6361/201220727|last1=Smith|first1=A. M. S.|last2=Anderson|first2=D. R.|last3=Bouchy|first3=F.|last4=Collier Cameron|first4=A.|last5=Doyle|first5=A. P.|last6=Fumel|first6=A.|last7=Gillon|first7=M.|last8=Hébrard|first8=G.|last9=Hellier|first9=C.|last10=Jehin|first10=E.|last11=Lendl|first11=M.|last12=Maxted|first12=P. F. L.|last13=Moutou|first13=C.|last14=Pepe|first14=F.|last15=Pollacco|first15=D.|last16=Queloz|first16=D.|last17=Santerne|first17=A.|last18=Segransan|first18=D.|last19=Smalley|first19=B.|last20=Southworth|first20=J.|last21=Triaud|first21=A. H. M. J.|last22=Udry|first22=S.|last23=West|first23=R. G.|journal=Astronomy & Astrophysics|volume=552|pages=A120|bibcode=2013A&A...552A.120S|s2cid=118575479}}] Proper name Tanzanite |
| WASP-72b
|1.5461
|1.27
|2.2167421
|0.03708
|2210{{±|120|130}}
|style="background:#FFFF00"|transit
|1100
|1.39
|6250
|[ Proper name Cuptor] |
| WASP-77Ab
|1.76
|1.21
|1.3600309
|0.024
|1715
|style="background:#FFFF00"|transit
|300
|1
|5500
|Orbiting primary star of binary star system[{{citation|arxiv=1211.6033|title=WASP-77 Ab: A Transiting Hot Jupiter Planet in a Wide Binary System1|year=2012|doi=10.1086/669231|last1=Maxted|first1=P. F. L.|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Hellier|first7=C.|last8=Jehin|first8=E.|last9=Lendl|first9=M.|last10=Pepe|first10=F.|last11=Pollacco|first11=D. L.|last12=Queloz|first12=D.|last13=Ségransan|first13=D.|last14=Smalley|first14=B.|last15=Southworth|first15=K.|last16=Smith|first16=A. M. S.|last17=Triaud|first17=A. H. M. J.|last18=Udry|first18=S.|last19=West|first19=R. G.|journal=Publications of the Astronomical Society of the Pacific|volume=125|issue=923|pages=48–55|s2cid=53552999}}] |
| WASP-78b
|0.89
|1.7
|2.17517632
|0.0362
|2350
|style="background:#FFFF00"|transit
|1800
|1.17
|6100
| |
| WASP-79b
|0.9
|2.09
|3.6623866
|0.0535
|1900{{±|50}}
|style="background:#FFFF00"|transit
|780
|1.38
|6600
|[{{citation|arxiv=1206.1177|title=WASP-78b and WASP-79b: Two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus|year=2012|doi=10.1051/0004-6361/201219731|last1=Smalley|first1=B.|last2=Anderson|first2=D. R.|last3=Collier-Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Hellier|first7=C.|last8=Jehin|first8=E.|last9=Lendl|first9=M.|last10=Maxted|first10=P. F. L.|last11=Pepe|first11=F.|last12=Pollacco|first12=D.|last13=Queloz|first13=D.|last14=Ségransan|first14=D.|last15=Smith|first15=A. M. S.|last16=Southworth|first16=J.|last17=Triaud|first17=A. H. M. J.|last18=Udry|first18=S.|last19=West|first19=R. G.|journal=Astronomy & Astrophysics|volume=547|pages=A61|bibcode=2012A&A...547A..61S|s2cid=119233646}}] Proper name Pollera |
| WISE 1217+1626 B
|22
|0.934
|
|8
|450
|style="background:#FF6CDA"|imaging
|29{{±|3}}
|0.03
|575
|Brown dwarf[{{cite journal | last=Liu |first=Michael C. |author2=Dupuy, Trent J. |author3=Bowler, Brendan P. |author4=Leggett, S. K. |author5=Best, William M. J. | title=Two Extraordinary Substellar Binaries at the T/Y Transition and the Y-band Fluxes of the Coolest Brown Dwarfs | year=2012 | journal=The Astrophysical Journal | volume=758 | issue=1 | pages=57 | arxiv=1206.4044 | doi=10.1088/0004-637X/758/1/57 | bibcode=2012ApJ...758...57L|s2cid=118402490 }}] |
| WTS-1b
|4.01
|1.49
|3.352057
|0.047
|1500{{±|100}}
|style="background:#FFFF00"|transit
|8100{{±|1000}}
|1.2
|6250
|[[https://www.researchgate.net/publication/231609171_The_first_planet_detected_in_the_WTS_An_inflated_hot_Jupiter_in_a_335d_orbit_around_a_late_F_star The first planet detected in the WTS: An inflated hot Jupiter in a 3.35d orbit around a late F star]] |