Lista de exoplanetas descobertos em 2018: diferenças entre revisões

Origem: Wikipédia, a enciclopédia livre.
Explorar interativamente o histórico
← Ver a alteração anteriorVer a alteração posterior →
Conteúdo apagado Conteúdo adicionado
VisualTexto wiki
Atualização!
Atualização!
Linha 1: Linha 1:
Esta é uma '''Lista de exoplanetas descobertos em 2018'''.
Esta é uma '''Lista de exoplanetas descobertos em 2018'''.<ref>{{citar web|título=NASA Exoplanet Archive|url=https://exoplanetarchive.ipac.caltech.edu/index.html|website=exoplanetarchive.ipac.caltech.edu|publicado=California Institute of Technology|acessodata=27 de março de 2018}}</ref>


Para [[exoplaneta]]s detectados apenas pela [[Métodos de detecção de exoplanetas#Velocidade radial|velocidade radial]], o valor da massa é na verdade um limite inferior. (Consulte a [[massa mínima]] para obter mais informações)
Para [[exoplaneta]]s detectados apenas pela [[Métodos de detecção de exoplanetas#Velocidade radial|velocidade radial]], o valor da massa é na verdade um limite inferior. (Consulte a [[massa mínima]] para obter mais informações)
Linha 16: Linha 16:
!Observações
!Observações
|-
|-
|[[24 Boötis b]]
|[[24 Boötis#Sistema planetário|24 Boötis b]]
|0.91{{±|0.13|0.10}}
|0.91{{±|0.13|0.10}}
|
|
Linha 26: Linha 26:
|0.99{{±|0.19|0.13}}
|0.99{{±|0.19|0.13}}
|4893{{±|15}}
|4893{{±|15}}
|<ref name=Takarada2018>{{citar periódico | título=Planets around the evolved stars 24 Booties and γ Libra: A 30d-period planet and a double giant-planet system in possible 7:3 MMR |último1=Takarada |primeiro1=Takuya |último2=Sato |primeiro2=Bun'ei |último3=Omiya |primeiro3=Masashi |último4=Harakawa |primeiro4=Hiroki |último5=Nagasawa |primeiro5=Makiko |último6=Izumiura |primeiro6=Hideyuki |último7=Kambe |primeiro7=Eiji |último8=Takeda |primeiro8=Yoichi |último9=Yoshida |primeiro9=Michitoshi |último10=Itoh |primeiro10=Yoichi |último11=Ando |primeiro11=Hiroyasu |último12=Kokubo |primeiro12=Eiichiro |último13=Ida |primeiro13=Shigeru |periódico=Publications of the Astronomical Society of Japan |numero-autores=1 | arxiv=1804.04008 |ano=2018 | volume=70 |número=4 | doi=10.1093/pasj/psy052 | s2cid=119027104 }}</ref>
|
|-
|-
|[[40 Eridani Ab]]
|[[40 Eridani Ab]]
Linha 38: Linha 38:
|0.78{{±|0.08}}
|0.78{{±|0.08}}
|5072{{±|53}}
|5072{{±|53}}
|<ref>{{citar periódico | doi=10.1093/mnras/sty1933 |bibcode=2018MNRAS.480.2411M | arxiv=1807.07098 |título=The first super-Earth Detection from the High Cadence and High Radial Velocity Precision Dharma Planet Survey |periódico=Monthly Notices of the Royal Astronomical Society |volume=480 |número=2 |páginas=2411 |ano=2018 |último1=Ma |primeiro1=Bo |último2=Ge |primeiro2=Jian |último3=Muterspaugh |primeiro3=Matthew |último4=Singer |primeiro4=Michael A |último5=Henry |primeiro5=Gregory W |último6=González Hernández |primeiro6=Jonay I |último7=Sithajan |primeiro7=Sirinrat |último8=Jeram |primeiro8=Sarik |último9=Williamson |primeiro9=Michael |último10=Stassun |primeiro10=Keivan |último11=Kimock |primeiro11=Benjamin |último12=Varosi |primeiro12=Frank |último13=Schofield |primeiro13=Sidney |último14=Liu |primeiro14=Jian |último15=Powell |primeiro15=Scott |último16=Cassette |primeiro16=Anthony |último17=Jakeman |primeiro17=Hali |último18=Avner |primeiro18=Louis |último19=Grieves |primeiro19=Nolan |último20=Barnes |primeiro20=Rory |último21=Gilda |primeiro21=Sankalp |último22=Grantham |primeiro22=Jim |último23=Stafford |primeiro23=Greg |último24=Savage |primeiro24=David |último25=Bland |primeiro25=Steve |último26=Ealey |primeiro26=Brent |numero-autores=1 }}</ref>
|
|-
|-
|[[Barnard's Star b]]
|[[Barnard's Star b]]
Linha 50: Linha 50:
|0.144
|0.144
|3134
|3134
|<ref name="Ribas Tuomi Reiners Butler 2018 pp. 365–368">{{citar periódico|último1= Ribas|primeiro1= I.|último2= Tuomi |primeiro2= M.|último3= Reiners |primeiro3= Ansgar|último4= Butler |primeiro4= R. P.|último5= Morales |primeiro5= J. C.|último6= Perger |primeiro6= M.|último7= Dreizler |primeiro7= S.|último8= Rodríguez-López |primeiro8= C.|último9= González Hernández |primeiro9= J. I.|último10= Rosich |primeiro10= A.|último11= Feng |primeiro11= F.|último12= Trifonov |primeiro12= T.|último13= Vogt |primeiro13= S. S.|último14= Caballero |primeiro14= J. A.|último15= Hatzes |primeiro15= A.|último16= Herrero |primeiro16= E.|último17= Jeffers |primeiro17= S. V.|último18= Lafarga |primeiro18= M.|último19= Murgas |primeiro19= F.|último20= Nelson |primeiro20= R. P.|último21= Rodríguez |primeiro21= E.|último22= Strachan |primeiro22= J. B. P.|último23= Tal-Or |primeiro23= L.|último24= Teske |primeiro24= J.|último25= Toledo-Padrón |primeiro25= B.|último26= Zechmeister |primeiro26= M.|último27= Quirrenbach |primeiro27= A.|último28= Amado |primeiro28= P. J.|último29= Azzaro |primeiro29= M.|último30= Béjar |primeiro30= V. J. S.|último31= Barnes |primeiro31= J. R.|último32= Berdiñas |primeiro32= Z. M.|último33= Burt |primeiro33= J.|último34= Coleman |primeiro34= G.|último35= Cortés-Contreras |primeiro35= M.|último36= Crane |primeiro36= J.|último37= Engle |primeiro37= S. G.|último38= Guinan |primeiro38= E. F.|último39= Haswell |primeiro39= C. A.|último40= Henning |primeiro40= Th.|último41= Holden |primeiro41= B.|último42= Jenkins |primeiro42= J.|último43= Jones |primeiro43= H. R. A.|último44= Kaminski |primeiro44= A.|último45= Kiraga |primeiro45= M.|último46= Kürster |primeiro46= Martin|último47= Lee |primeiro47= M. H.|último48= López-González |primeiro48= M. J.|último49= Montes |primeiro49= D.|último50= Morin |primeiro50= J.|último51= Ofir |primeiro51= A.|último52= Pallé |primeiro52= E.|último53= Rebolo |primeiro53= Rafael|último54= Reffert |primeiro54= S.|último55= Schweitzer |primeiro55= A.|último56= Seifert |primeiro56= W.|último57= Shectman |primeiro57= S. A.|último58= Staab |primeiro58= D.|último59= Street |primeiro59= R. A.|último60= Suárez Mascareño |primeiro60= A.|último61= Tsapras |primeiro61= Y.|último62= Wang |primeiro62= S. X.|último63= Anglada-Escudé |primeiro63= G.|numero-autores= 4|data= 2018-11-14| título= A candidate super-Earth planet orbiting near the snow line of Barnard's star| url = https://www.eso.org/public/archives/releases/sciencepapers/eso1837/eso1837a.pdf| urlmorta = não|periódico= [[Nature (journal)|Nature]]|publicado= [[Omega Space Exploration or OSE]]| volume = 563|número= 7731|páginas = 365–368| arxiv = 1811.05955| bibcode = 2018Natur.563..365R| doi = 10.1038/s41586-018-0677-y| issn = 0028-0836| oclc = 716177853|arquivourl= https://web.archive.org/web/20190326185022/https://www.eso.org/public/archives/releases/sciencepapers/eso1837/eso1837a.pdf|arquivodata= 2019-03-26| pmid = 30429552| hdl = 2299/21132}}</ref>
|
|-
|-
|[[COROT-20c]]
|[[COROT-20c]]
Linha 62: Linha 62:
|1.14{{±|0.08}}
|1.14{{±|0.08}}
|6050{{±|200}}
|6050{{±|200}}
|[[Anã marrom]] (possivelmente)<ref>{{citation|arxiv=1807.01229|ano=2018|título=A 4.6-year period brown-dwarf companion interacting with the hot-Jupiter CoRoT-20 b}}</ref>
|[[Anã marrom]] (possivelmente)
|-
|[[COROT-21b]]
|2.26{{±|0.31}}
|1.30{{±|0.14}}
|2.72474{{±|0.00014}}
|0.0417{{±|0.0011}}
|
|style="background:#FFFF00"|Trânsito
|4560{{±|930}}
|1.29{{±|0.09}}
|6200{{±|100}}
|
|-
|-
|[[DE Canum Venaticorum b]]
|[[DE Canum Venaticorum b]]
Linha 86: Linha 74:
|0.51
|0.51
|
|
|<ref>[https://iopscience.iop.org/article/10.3847/1538-4357/aae64d/pdf DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet]</ref>
|
|-
|-
|[[Gamma Librae b]]
|[[Gamma Librae#Sistema planetário|Gamma Librae b]]
|1.02{{±|0.14}}
|1.02{{±|0.14}}
|
|
Linha 98: Linha 86:
|1.47{{±|0.20}}
|1.47{{±|0.20}}
|4822{{±|15}}
|4822{{±|15}}
|<ref name=Takarada2018/>
|
|-
|-
|[[Gamma Librae c]]
|[[Gamma Librae#Sistema planetário|Gamma Librae c]]
|4.58{{±|0.45|0.43}}
|4.58{{±|0.45|0.43}}
|
|
Linha 110: Linha 98:
|1.47{{±|0.20}}
|1.47{{±|0.20}}
|4822{{±|15}}
|4822{{±|15}}
|<ref name=Takarada2018/>
|
|-
|-
|[[Gliese 15 Ac]]
|[[Gliese 15 Ac]]
Linha 122: Linha 110:
|0.38
|0.38
|3567
|3567
|<ref>{{citar periódico|bibcode=2018A&A...617A.104P|título=The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction|periódico=Astronomy and Astrophysics|volume=617|pages=A104|último1=Pinamonti|primeiro1=M.|último2=Damasso|primeiro2=M.|último3=Marzari|primeiro3=F.|último4=Sozzetti|primeiro4=A.|último5=Desidera|primeiro5=S.|último6=Maldonado|primeiro6=J.|último7=Scandariato|primeiro7=G.|último8=Affer|primeiro8=L.|último9=Lanza|primeiro9=A. F.|último10=Bignamini|primeiro10=A.|último11=Bonomo|primeiro11=A. S.|último12=Borsa|primeiro12=F.|último13=Claudi|primeiro13=R.|último14=Cosentino|primeiro14=R.|último15=Giacobbe|primeiro15=P.|último16=González-Álvarez|primeiro16=E.|último17=González Hernández|primeiro17=J. I.|último18=Gratton|primeiro18=R.|último19=Leto|primeiro19=G.|último20=Malavolta|primeiro20=L.|último21=Martinez Fiorenzano|primeiro21=A.|último22=Micela|primeiro22=G.|último23=Molinari|primeiro23=E.|último24=Pagano|primeiro24=I.|último25=Pedani|primeiro25=M.|último26=Perger|primeiro26=M.|último27=Piotto|primeiro27=G.|último28=Rebolo|primeiro28=R.|último29=Ribas|primeiro29=I.|último30=Suárez Mascareño|primeiro30=A.|numero-autores=29|ano=2018|arxiv=1804.03476|doi=10.1051/0004-6361/201732535}}</ref>
|<ref>{{citar periódico|bibcode=2018A&A...617A.104P|título=The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction|periódico=Astronomy and Astrophysics|volume=617|páginas=A104|último1=Pinamonti|primeiro1=M.|último2=Damasso|primeiro2=M.|último3=Marzari|primeiro3=F.|último4=Sozzetti|primeiro4=A.|último5=Desidera|primeiro5=S.|último6=Maldonado|primeiro6=J.|último7=Scandariato|primeiro7=G.|último8=Affer|primeiro8=L.|último9=Lanza|primeiro9=A. F.|último10=Bignamini|primeiro10=A.|último11=Bonomo|primeiro11=A. S.|último12=Borsa|primeiro12=F.|último13=Claudi|primeiro13=R.|último14=Cosentino|primeiro14=R.|último15=Giacobbe|primeiro15=P.|último16=González-Álvarez|primeiro16=E.|último17=González Hernández|primeiro17=J. I.|último18=Gratton|primeiro18=R.|último19=Leto|primeiro19=G.|último20=Malavolta|primeiro20=L.|último21=Martinez Fiorenzano|primeiro21=A.|último22=Micela|primeiro22=G.|último23=Molinari|primeiro23=E.|último24=Pagano|primeiro24=I.|último25=Pedani|primeiro25=M.|último26=Perger|primeiro26=M.|último27=Piotto|primeiro27=G.|último28=Rebolo|primeiro28=R.|último29=Ribas|primeiro29=I.|último30=Suárez Mascareño|primeiro30=A.|numero-autores=29|ano=2018|arxiv=1804.03476|doi=10.1051/0004-6361/201732535}}</ref>
|-
|-
|[[Gliese 96 b]]
|[[Gliese 96 b]]
Linha 134: Linha 122:
|0.60{{±|0.07}}
|0.60{{±|0.07}}
|3785{{±|62}}
|3785{{±|62}}
|<ref>{{citation|arxiv=1806.10958|ano=2018|título=The SOPHIE search for northern extrasolar planets XIII. Two planets around M-dwarfs Gl617A and Gl96}}</ref>
|
|-
|-
|[[Gliese 317 c]]
|[[Gliese 143 b]]
|1.54{{±|1.26|0.57}}
|0.09637{{±|0.00827|0.00840}}
|0.2280839{{±|0.0282262}}
|35.589{{±|0.006|0.005}}
|0.1932{{±|0.0002}}
|
|
|style="background:#FFFF00"|Trânsito
|5312{{±|758|1248}}
|53.25{{±|0.02}}
|
|0.76{{±|0.03|0.02}}
|
|style="background:#00FF00"|Vel. radial
|49.25{{±|0.72}}
|0.42{{±|0.05}}
|3510{{±|50}}
|
|
|<ref name=Trifonov2018/>
|-
|-
|[[Gliese 1132 c]]
|[[Gliese 1132#Sistema planetário|Gliese 1132 c]]
|0.00831{{±|0.00138}}
|0.00831{{±|0.00138}}
|
|
Linha 158: Linha 146:
|0.181{{±|0.019}}
|0.181{{±|0.019}}
|3270{{±|140}}
|3270{{±|140}}
|<ref>{{citation|arxiv=1806.03870|ano=2018|título=Radial velocity follow-up of GJ1132 with HARPS. A precise mass for planet 'b' and the discovery of a second planet}}</ref>
|
|-
|-
|[[Gliese 1265 b]]
|[[Gliese 1265 b]]
Linha 170: Linha 158:
|0.18{{±|0.02}}
|0.18{{±|0.02}}
|3236{{±|51}}
|3236{{±|51}}
|Estrela-mãe também conhecida como LP 819-052<ref name=Luque2018>{{citation|arxiv=1810.07572|ano=2018|título=The CARMENES search for exoplanets around M dwarfs: The warm super-Earths in twin orbits around the mid-type M dwarfs Ross 1020 (GJ 3779) and LP 819-052 (GJ 1265)}}</ref>
|
|-
|-
|[[Gliese 3779 b]]
|[[Gliese 3779 b]]
Linha 182: Linha 170:
|0.27{{±|0.02}}
|0.27{{±|0.02}}
|3324{{±|51}}
|3324{{±|51}}
|Estrela-mãe também conhecida como Ross 1020<ref name=Luque2018/>
|
|-
|-
|[[HAT-P-11c]]
|[[HAT-P-11c]]
Linha 194: Linha 182:
|0.809{{±|0.020|0.030}}
|0.809{{±|0.020|0.030}}
|4780{{±|50}}
|4780{{±|50}}
|<ref>{{citar periódico | título=HAT-P-11: Discovery of a Second Planet and a Clue to Understanding Exoplanet Obliquities |periódico=The Astronomical Journal | volume=155 |número=6 |em=255 |ano=2018 |último1=Yee |primeiro1=Samuel W. |último2=Petigura |primeiro2=Erik A. |último3=Fulton |primeiro3=Benjamin J. |último4=Knutson |primeiro4=Heather A. |último5=Batygin |primeiro5=Konstantin |último6=Bakos |primeiro6=Gáspár Á. |último7=Hartman |primeiro7=Joel D. |último8=Hirsch |primeiro8=Lea A. |último9=Howard |primeiro9=Andrew W. |último10=Isaacson |primeiro10=Howard |último11=Kosiarek |primeiro11=Molly R. |último12=Sinukoff |primeiro12=Evan |último13=Weiss |primeiro13=Lauren M. |numero-autores=1 | arxiv=1805.09352 | bibcode=2018AJ....155..255Y | bibcode-access=free | doi=10.3847/1538-3881/aabfec | doi-access=free }}</ref>
|
|-
|[[HATS-7b]]
|0.120
|0.563
|3.1853150
|0.04012
|1084
|style="background:#FFFF00"|Trânsito
|838
|0.85
|4985
|
|-
|-
|[[HATS-39b]]
|[[HATS-39b]]
Linha 218: Linha 194:
|1.379{{±|0.040}}
|1.379{{±|0.040}}
|6572{{±|83}}
|6572{{±|83}}
|<ref name=Bento2018>{{citation|arxiv=1804.01623|ano=2018|título=HATS-39b, HATS-40b, HATS-41b, and HATS-42b: Three Inflated Hot Jupiters and a Super-Jupiter Transiting F Stars}}</ref>
|
|-
|-
|[[HATS-40b]]
|[[HATS-40b]]
Linha 230: Linha 206:
|1.561{{±|0.069}}
|1.561{{±|0.069}}
|6460{{±|130}}
|6460{{±|130}}
|<ref name=Bento2018/>
|
|-
|-
|[[HATS-41b]]
|[[HATS-41b]]
Linha 242: Linha 218:
|1.496{{±|0.115|0.078}}
|1.496{{±|0.115|0.078}}
|6424{{±|91}}
|6424{{±|91}}
|<ref name=Bento2018/>
|
|-
|-
|[[HATS-42b]]
|[[HATS-42b]]
Linha 254: Linha 230:
|1.273{{±|0.067}}
|1.273{{±|0.067}}
|6060{{±|120}}
|6060{{±|120}}
|<ref name=Bento2018/>
|
|-
|[[HATS-43b]]
|0.261{{±|0.054}}
|1.180{{±|0.050}}
|4.3888497
|0.04944{{±|0.00046}}
|1003{{±|27}}
|style="background:#FFFF00"|Trânsito
|1194.1{{±|7.4}}
|0.837{{±|0.023}}
|5099{{±|61}}
|
|-
|[[HATS-44b]]
|0.56{{±|0.11}}
|1.067{{±|0.125|0.071}}
|2.7439004
|0.03649{{±|0.00030}}
|1161{{±|34}}
|style="background:#FFFF00"|Trânsito
|1474{{±|11}}
|0.860{{±|0.021}}
|5080{{±|100}}
|
|-
|[[HATS-45b]]
|0.70{{±|0.15}}
|1.286{{±|0.093}}
|4.1876244
|0.05511{{±|0.00069}}
|1518{{±|45}}
|style="background:#FFFF00"|Trânsito
|2575{{±|38}}
|1.272{{±|0.048}}
|6450{{±|110}}
|
|-
|[[HATS-46b]]
|0.173{{±|0.062}}
|0.903{{±|0.058|0.045}}
|4.7423729
|0.05367{{±|0.00053}}
|1054{{±|29}}
|style="background:#FFFF00"|Trânsito
|1500{{±|13}}
|0.917{{±|0.027}}
|5495{{±|69}}
|
|-
|-
|[[HATS-59b]]
|[[HATS-59#Sistema planetário|HATS-59b]]
|0.806{{±|0.069}}
|0.806{{±|0.069}}
|1.126{{±|0.077}}
|1.126{{±|0.077}}
Linha 314: Linha 242:
|1.04{{±|0.04}}
|1.04{{±|0.04}}
|5670{{±|91}}
|5670{{±|91}}
|<ref name=Sarkis2018>{{citation|arxiv=1805.05925|ano=2018|título=HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet Around a Sun-Like Star}}</ref>
|
|-
|-
|[[HATS-59c]]
|[[HATS-59#Sistema planetário|HATS-59c]]
|12.70{{±|0.87}}
|12.70{{±|0.87}}
|
|
Linha 326: Linha 254:
|1.04{{±|0.04}}
|1.04{{±|0.04}}
|5670{{±|91}}
|5670{{±|91}}
|<ref name=Sarkis2018/>
|
|-
|-
|[[HATS-60b]]
|[[HATS-60b]]
Linha 338: Linha 266:
|1.097{{±|0.010|0.016}}
|1.097{{±|0.010|0.016}}
|5688{{±|20}}
|5688{{±|20}}
|<ref name=Hartman2018>{{citation|arxiv=1809.01048|ano=2018|título=HATS-60b - HATS-69b: Ten Transiting Planets From HATSouth}}</ref>
|
|-
|-
|[[HATS-61b]]
|[[HATS-61b]]
Linha 350: Linha 278:
|1.08{{±|0.01}}
|1.08{{±|0.01}}
|5542{{±|21}}
|5542{{±|21}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-62b]]
|[[HATS-62b]]
Linha 362: Linha 290:
|0.90{{±|0.02|0.01}}
|0.90{{±|0.02|0.01}}
|5416{{±|19|13}}
|5416{{±|19|13}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-63b]]
|[[HATS-63b]]
Linha 374: Linha 302:
|0.93{{±|0.02}}
|0.93{{±|0.02}}
|5627{{±|18}}
|5627{{±|18}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-64b]]
|[[HATS-64b]]
Linha 386: Linha 314:
|1.56{{±|0.03}}
|1.56{{±|0.03}}
|6554{{±|27}}
|6554{{±|27}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-65b]]
|[[HATS-65b]]
Linha 398: Linha 326:
|1.26{{±|0.03}}
|1.26{{±|0.03}}
|6277{{±|30}}
|6277{{±|30}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-66b]]
|[[HATS-66b]]
Linha 410: Linha 338:
|1.41{{±|0.02}}
|1.41{{±|0.02}}
|6625{{±|35}}
|6625{{±|35}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-67b]]
|[[HATS-67b]]
Linha 422: Linha 350:
|1.44{{±|0.02}}
|1.44{{±|0.02}}
|6594{{±|33}}
|6594{{±|33}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-68b]]
|[[HATS-68b]]
Linha 434: Linha 362:
|1.35{{±|0.01}}
|1.35{{±|0.01}}
|6147{{±|22}}
|6147{{±|22}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HATS-69b]]
|[[HATS-69b]]
Linha 446: Linha 374:
|0.89{{±|0.01|-0.02}}
|0.89{{±|0.01|-0.02}}
|5137{{±|16}}
|5137{{±|16}}
|<ref name=Hartman2018/>
|
|-
|-
|[[HD 4917 b]]
|[[HD 4917 b]]
Linha 458: Linha 386:
|1.32
|1.32
|4802
|4802
|Dois exoplanetas adicionais no sistema são suspeitos<ref name=Luhn2018/>
|
|-
|-
|[[HD 13167 b]]
|[[HD 13167 b]]
Linha 470: Linha 398:
|1.35
|1.35
|5671
|5671
|<ref name=Luhn2018/><ref name=Livingston2018/>
|
|-
|-
|[[HD 14787 b]]
|[[HD 14787 b]]
Linha 482: Linha 410:
|1.43
|1.43
|4946
|4946
|<ref name=Luhn2018/>
|
|-
|-
|[[HD 18015 b]]
|[[HD 18015 b]]
Linha 494: Linha 422:
|1.49
|1.49
|5603
|5603
|<ref name=Luhn2018/>
|
|-
|-
|[[HD 21749 b]]
|[[HD 23472#Sistema planetário|HD 23472 b]]
|0.073{{±|0.007|0.006}}
|0.05638{{±|0.00444|0.04405}}
|0.254{{±|0.023|0.020}}
|0.179{{±|0.009}}
|17.667{{±|0.142|0.095}}
|36
|0.121{{±|0.001}}
|
|543{{±|18}}
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|127.48{{±|0.06}}
|52.185
|0.67{{±|0.03}}
|
|4684{{±|99}}
|
|<ref name=Trifonov2018>{{citation|arxiv=1812.04501|ano=2018|título=TESS exoplanet candidates validated with HARPS archival data. A massive Neptune around GJ143 and two Neptunes around HD23472}}</ref><ref name=Barros2022>{{citation|arxiv=2209.13345|ano=2022|título=HD 23472: A multi-planetary system with three super-Earths and two potential super-Mercuries}}</ref>
|
|-
|[[HD 23472#Sistema planetário|HD 23472 c]]
|0.05405{{±|0.00337|0.04333}}
|0.167{{±|0.010}}
|29.625{{±|0.224|0.171}}
|0.170{{±|0.001}}
|467{{±|19|18}}
|style="background:#FFFF00"| transit
|127.48{{±|0.06}}
|0.67{{±|0.03}}
|4684{{±|99}}
|<ref name=Trifonov2018/><ref name=Barros2022/>
|-
|-
|[[HD 33142 c]]
|[[HD 33142 c]]
Linha 518: Linha 458:
|1.78{{±|0.31}}
|1.78{{±|0.31}}
|5009{{±|15}}
|5009{{±|15}}
|Detecção de margem<ref name=Luhn2018/>
|
|-
|[[HD 47366 b]]
|1.75
|
|363.3
|1.214
|
|style="background:#00FF00"|Vel. radial
|260
|1.81
|4866
|
|-
|[[HD 47366 c]]
|1.86
|
|684.7
|1.853
|
|style="background:#00FF00"|Vel. radial
|260
|1.81
|4866
|
|-
|-
|[[HD 55696 b]]
|[[HD 55696 b]]
Linha 554: Linha 470:
|1.29{{±|0.20}}
|1.29{{±|0.20}}
|6012
|6012
|<ref name=Ment2018>{{citation|arxiv=1809.01228|ano=2018|título=Radial velocities from the N2K Project: 6 new cold gas giant planets orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810}}</ref>
|
|-
|-
|[[HD 72490 b]]
|[[HD 72490#Sistema planetário|HD 72490 b]]
|1.768{{±|0.080}}
|1.768{{±|0.080}}
|1.218
|1.218
Linha 566: Linha 482:
|1.21
|1.21
|4934
|4934
|<ref name=Luhn2018>{{citation|arxiv=1811.03043|ano=2018|título=Retired A Stars and Their Companions VIII: 15 New Planetary Signals Around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts}}</ref>
|
|-
|-
|[[HD 75784 c]]
|[[HD 72490#Sistema planetário|HD 72490 c]]
|4.5{{±|1.2}}
|4.5{{±|1.2}}
|
|
Linha 578: Linha 494:
|1.26{{±|0.25}}
|1.26{{±|0.25}}
|4867
|4867
|<ref name=Luhn2018/>
|
|-
|-
|[[HD 89345 b]]
|[[HD 89345 b]]
Linha 590: Linha 506:
|1.16
|1.16
|5576
|5576
|<ref>{{citation|arxiv=1803.02858|ano=2018|título=Two warm, low-density sub-Jovian planets orbiting bright stars in K2 campaigns 13 and 14}}</ref> Estrela-mãe também conhecida como K2-234<ref>{{citation|arxiv=1805.01860|ano=2018|título=HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2}}</ref>
|
|-
|-
|[[HD 94834 b]]
|[[HD 94834 b]]
Linha 602: Linha 518:
|1.11
|1.11
|4798
|4798
|<ref name=Luhn2018/>
|
|-
|[[HD 95089 c]]
|3.97{{±|0.33|0.59}}
|
|1860{{±|370|570}}
|
|
|style="background:#00FF00"|Vel. radial
|42.1{{±|0.59}}
|1.58{{±|0.11}}
|5002{{±|44}}
|
|-
|-
|[[HD 98736 b]]
|[[HD 98736 b]]
Linha 626: Linha 530:
|0.92{{±|0.13}}
|0.92{{±|0.13}}
|5271
|5271
|<ref name=Ment2018/>
|
|-
|[[HD 99706 c]]
|5.69{{±|1.43|0.96}}
|
|1278{{±|151|198}}
|
|
|style="background:#00FF00"|Vel. radial
|45.14{{±|0.34}}
|1.70{{±|0.35}}
|4891{{±|35}}
|
|-
|[[HD 102329 c]]
|1.52{{±|0.30|0.25}}
|
|1123{{±|79|53}}
|
|
|style="background:#00FF00"|Vel. radial
|66.97{{±|0.96}}
|3.21{{±|1.28}}
|4745{{±|71}}
|
|-
|-
|[[HD 114783 c]]
|[[HD 114783 c]]
Linha 688: Linha 568:
|
|
|-
|-
|[[HD 148164 b]]
|[[HD 148164#Sistema planetário|HD 148164 b]]
|1.23{{±|0.25}}
|1.23{{±|0.25}}
|
|
Linha 698: Linha 578:
|1.21{{±|0.24}}
|1.21{{±|0.24}}
|6032
|6032
|<ref name=Ment2018/>
|
|-
|-
|[[HD 148164 c]]
|[[HD 148164#Sistema planetário|HD 148164 c]]
|5.16{{±|0.82}}
|5.16{{±|0.82}}
|
|
Linha 710: Linha 590:
|1.21{{±|0.24}}
|1.21{{±|0.24}}
|6032
|6032
|<ref name=Ment2018/>
|
|-
|-
|[[HD 148284 b]]
|[[HD 148284 b]]
Linha 746: Linha 626:
|1.75
|1.75
|5131
|5131
|<ref name=Luhn2018/>
|
|-
|-
|[[HD 202696 b]]
|[[HD 202696 b]]
Linha 782: Linha 662:
|1.12{{±|0.21}}
|1.12{{±|0.21}}
|5780
|5780
|<ref name=Ment2018/>
|
|-
|-
|[[HD 211810 b]]
|[[HD 211810 b]]
Linha 794: Linha 674:
|1.03{{±|0.02}}
|1.03{{±|0.02}}
|5652
|5652
|<ref name=Ment2018/>
|
|-
|-
|[[HD 215152 b]]
|[[HD 215152 b]]
Linha 868: Linha 748:
|
|
|-
|-
|[[K2-141b]]
|[[K2-138b]]
|0.0160{{±|0.0013}}
|0.135{{±|0.004}}
|0.2803226
|0.00716{{±|0.00055|0.00065}}
|2039{{±|87|48}}
|style="background:#FFFF00"|Trânsito
|202.16{{±|0.54}}
|0.708{{±|0.028}}
|4599{{±|79}}
|
|
|0.140
|-
|2.35322
|[[K2-141c]]
|0.03380
|0.023{{±|0|0.023}}
|0.624{{±|0.410|0.250}}
|7.74850
|0.06739{{±|0.00089|0.00091}}
|
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|597
|202.16{{±|0.54}}
|0.93
|0.708{{±|0.028}}
|5378
|4599{{±|79}}
|<ref name=Christiansen2018>{{citar periódico|primeiro1=Jessie L. |último1=Christiansen |primeiro2=Ian J. M. |último2=Crossfield |primeiro3=Geert |último3=Barentsen |primeiro4=Chris J. |último4=Lintott |primeiro5=Thomas |último5=Barclay |primeiro6=Brooke D. |último6=Simmons |primeiro7=Erik |último7=Petigura |primeiro8=Joshua E. |último8=Schlieder |primeiro9=Courtney D. |último9=Dressing |primeiro10=Andrew |último10=Vanderburg |primeiro11=David R. |último11=Ciardi |primeiro12=Campbell |último12=Allen |primeiro13=Adam |último13=McMaster |primeiro14=Grant |último14=Miller |primeiro15=Martin |último15=Veldthuis |primeiro16=Sarah |último16=Allen |primeiro17=Zach |último17=Wolfenbarger |primeiro18=Brian |último18=Cox |primeiro19=Julia |último19=Zemiro |primeiro20=Andrew W. |último20=Howard |primeiro21=John |último21=Livingston |primeiro22=Evan |último22=Sinukoff |primeiro23=Timothy |último23=Catron |primeiro24=Andrew |último24=Grey |primeiro25=Joshua J. E. |último25=Kusch |primeiro26=Ivan |último26=Terentev |primeiro27=Martin |último27=Vales |primeiro28=Martti H. |último28=Kristiansen|data=2018-01-11|título=The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists|periódico=The Astronomical Journal|língua=en|volume=155|número=2|páginas=57|arxiv=1801.03874|doi=10.3847/1538-3881/aa9be0|issn=1538-3881|bibcode=2018AJ....155...57C |s2cid=52971376 }}</ref>
|
|-
|-
|[[HATS-36 b|K2-145b]]
|[[K2-138#Sistema planetário|K2-138c]]
|3.216{{±|0.062}}
|1.235{{±|0.043}}
|4.1752379
|0.05245{{±|0.00043}}
|1356{{±|30}}
|style="background:#FFFF00"|Trânsito
|2862{{±|73}}
|1.222{{±|0.029}}
|6149{{±|76}}
|
|
|0.225
|-
|3.55987
|[[K2-146b]]
|0.04454
|
|0.196{{±|0.021}}
|2.644646
|0.0266{{±|0.0010}}
|
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|597
|259.2{{±|1.5}}
|0.93
|0.358{{±|0.042}}
|5378
|3385{{±|70}}
|<ref name=Christiansen2018/>
|
|-
|-
|[[K2-147b]]
|[[K2-138#Sistema planetário|K2-138d]]
|
|
|0.237
|0.123{{±|0.015|0.013}}
|0.961917
|5.40478
|0.05883
|0.0159{{±|0.0005}}
|
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|597
|296.10{{±|0.90}}
|0.93
|0.583{{±|0.059}}
|5378
|3672{{±|70}}
|<ref name=Christiansen2018/>
|Também conhecido como EPIC 213715787<ref name=Adams2020/>
|-
|-
|[[K2-148b]]
|[[K2-138#Sistema planetário|K2-138e]]
|
|
|0.294
|0.119{{±|0.017|0.016}}
|8.26144
|4.38395{{±|0.00080}}
|0.07807
|0.0454{{±|0.0014}}
|
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|597
|407.4{{±|2.0}}
|0.93
|0.650{{±|0.061}}
|5378
|4079{{±|70}}
|<ref name=Christiansen2018/>
|
|-
|-
|[[K2-148c]]
|[[K2-138#Sistema planetário|K2-138f]]
|
|
|0.251
|0.154{{±|0.021|0.019}}
|12.75759
|6.92260{{±|0.00070}}
|0.10430
|0.0616{{±|0.0019}}
|
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|597
|407.4{{±|2.0}}
|0.93
|0.650{{±|0.061}}
|5378
|4079{{±|70}}
|<ref name=Christiansen2018/>
|
|-
|-
|[[K2-148d]]
|[[K2-141b]]
|0.0160{{±|0.0013}}
|
|0.146{{±|0.021|0.019}}
|0.135{{±|0.004}}
|0.2803226
|9.7579{{±|0.0010}}
|0.0774{{±|0.0024}}
|0.00716{{±|0.00055|0.00065}}
|2039{{±|87|48}}
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|407.4{{±|2.0}}
|202.16{{±|0.54}}
|0.650{{±|0.061}}
|0.708{{±|0.028}}
|4079{{±|70}}
|4599{{±|79}}
|
|
|-
|-
|[[K2-149b]]
|[[K2-141c]]
|0.023{{±|0|0.023}}
|
|0.146{{±|0.018|0.016}}
|0.624{{±|0.410|0.250}}
|7.74850
|11.3320{{±|0.0013}}
|0.0830{{±|0.0027}}
|0.06739{{±|0.00089|0.00091}}
|
|
|style="background:#FFFF00"|Trânsito
|style="background:#FFFF00"|Trânsito
|404.8{{±|1.8}}
|202.16{{±|0.54}}
|0.595{{±|0.059}}
|0.708{{±|0.028}}
|3745{{±|70}}
|4599{{±|79}}
|
|-
|[[K2-150b]]
|
|0.178{{±|0.024|0.019}}
|10.59357{{±|0.00084}}
|0.0727{{±|0.0027}}
|
|style="background:#FFFF00"|Trânsito
|335.2{{±|2.6}}
|0.457{{±|0.051}}
|3499{{±|70}}
|
|-
|[[K2-151b]]
|
|0.120{{±|0.014|0.012}}
|3.835592
|0.0365{{±|0.0014}}
|
|style="background:#FFFF00"|Trânsito
|227.07{{±|0.49}}
|0.440{{±|0.050}}
|3585{{±|70}}
|
|-
|[[K2-152b]]
|
|0.204{{±|0.022|0.021}}
|32.6527{{±|0.0035}}
|0.1716{{±|0.0012}}
|337{{±|3}}
|style="background:#FFFF00"|Trânsito
|354.8{{±|1.3}}
|0.63{{±|0.01}}
|4044{{±|34|35}}
|
|-
|[[K2-153b]]
|
|0.178{{±|0.019|0.016}}
|7.51554
|0.0614{{±|0.0004}}
|497{{±|6}}
|style="background:#FFFF00"|Trânsito
|468.7{{±|3.0}}
|0.55{{±|0.01}}
|3845{{±|37}}
|
|-
|[[K2-154b]]
|
|0.178{{±|0.019|0.010}}
|3.67635
|0.0405{{±|0.0003}}
|715{{±|9|8}}
|style="background:#FFFF00"|Trânsito
|423.5{{±|1.5}}
|0.65{{±|0.02|0.01}}
|4097{{±|40|45}}
|
|-
|[[K2-154c]]
|
|0.185{{±|0.016|0.012}}
|7.95478
|0.0677{{±|0.0005}}
|552{{±|7}}
|style="background:#FFFF00"|Trânsito
|423.5{{±|1.5}}
|0.65{{±|0.02|0.01}}
|4097{{±|40|45}}
|
|
|-
|-
Linha 1 094: Linha 878:
|0.66{{±|0.02|0.01}}
|0.66{{±|0.02|0.01}}
|4597{{±|50}}
|4597{{±|50}}
|<ref name=Adams2020>{{citar periódico|arxiv=2011.11698|título= Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10|ano=2020|último1=Adams|primeiro1=Elisabeth R.|periódico= The Planetary Science Journal|volume= 2|número= 4|página= 152|doi= 10.3847/PSJ/ac0ea0|bibcode= 2021PSJ.....2..152A|s2cid= 227151802|numero-autores=etal}}</ref>
|<ref name=Mayo2018/><ref name=Adams2020>{{citar periódico|arxiv=2011.11698|título= Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10|ano=2020|último1=Adams|primeiro1=Elisabeth R.|periódico= The Planetary Science Journal|volume= 2|número= 4|página= 152|doi= 10.3847/PSJ/ac0ea0|bibcode= 2021PSJ.....2..152A|s2cid= 227151802|numero-autores=etal}}</ref>
|-
|-
|[[K2-157b]]
|[[K2-157b]]
Linha 1 106: Linha 890:
|0.94
|0.94
|5456
|5456
|<ref name=Adams2020/>
|<ref name=Mayo2018/><ref name=Adams2020/>
|-
|-
|[[K2-158b]]
|[[K2-158b]]
Linha 1 118: Linha 902:
|0.92{{±|0.03|0.02}}
|0.92{{±|0.03|0.02}}
|5503{{±|51|48}}
|5503{{±|51|48}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-158c]]
|[[K2-158c]]
Linha 1 130: Linha 914:
|0.92{{±|0.03|0.02}}
|0.92{{±|0.03|0.02}}
|5503{{±|51|48}}
|5503{{±|51|48}}
|<ref name=Livingston2018-06>{{citation|arxiv=1806.11504|ano=2018|título=44 VALIDATED PLANETS FROM K2 CAMPAIGN 10}}</ref>
|
|-
|-
|[[K2-159b]]
|[[K2-159b]]
Linha 1 142: Linha 926:
|0.90{{±|0.02|0.03}}
|0.90{{±|0.02|0.03}}
|5425{{±|44}}
|5425{{±|44}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-160b]]
|[[K2-160b]]
Linha 1 154: Linha 938:
|0.983{{±|0.023|0.025}}
|0.983{{±|0.023|0.025}}
|5649{{±|50}}
|5649{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-161b]]
|[[K2-161b]]
Linha 1 166: Linha 950:
|0.987{{±|0.082|0.060}}
|0.987{{±|0.082|0.060}}
|4972{{±|50}}
|4972{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-162b]]
|[[K2-162b]]
Linha 1 178: Linha 962:
|0.75{{±|0.02}}
|0.75{{±|0.02}}
|4842{{±|49|45}}
|4842{{±|49|45}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-163b]]
|[[K2-163b]]
Linha 1 190: Linha 974:
|0.826{{±|0.019|0.023}}
|0.826{{±|0.019|0.023}}
|4937{{±|50}}
|4937{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-164b]]
|[[K2-164b]]
Linha 1 202: Linha 986:
|1.181{{±|0.093|0.061}}
|1.181{{±|0.093|0.061}}
|5791{{±|50}}
|5791{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-165b]]
|[[K2-165#Sistema planetário|K2-165b]]
|
|
|0.1137{{±|0.0129|0.0087}}
|0.1137{{±|0.0129|0.0087}}
Linha 1 214: Linha 998:
|0.835{{±|0.031|0.030}}
|0.835{{±|0.031|0.030}}
|5185{{±|50}}
|5185{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-165c]]
|[[K2-165#Sistema planetário|K2-165c]]
|
|
|0.1386{{±|0.0187|0.0098}}
|0.1386{{±|0.0187|0.0098}}
Linha 1 226: Linha 1 010:
|0.835{{±|0.031|0.030}}
|0.835{{±|0.031|0.030}}
|5185{{±|50}}
|5185{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-165d]]
|[[K2-165#Sistema planetário|K2-165d]]
|
|
|0.236{{±|0.023|0.013}}
|0.236{{±|0.023|0.013}}
Linha 1 238: Linha 1 022:
|0.835{{±|0.031|0.030}}
|0.835{{±|0.031|0.030}}
|5185{{±|50}}
|5185{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-166b]]
|[[K2-166b]]
Linha 1 250: Linha 1 034:
|1.16{{±|0.05|0.03}}
|1.16{{±|0.05|0.03}}
|5960{{±|52|53}}
|5960{{±|52|53}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-167b]]
|[[K2-167b]]
Linha 1 262: Linha 1 046:
|1.02{{±|0.12|0.09}}
|1.02{{±|0.12|0.09}}
|5908{{±|50}}
|5908{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-168b]]
|[[K2-168b]]
Linha 1 274: Linha 1 058:
|0.907{{±|0.029|0.032}}
|0.907{{±|0.029|0.032}}
|5554{{±|50}}
|5554{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-169b]]
|[[K2-169b]]
Linha 1 286: Linha 1 070:
|0.986{{±|0.028|0.026}}
|0.986{{±|0.028|0.026}}
|5548{{±|50}}
|5548{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-170b]]
|[[K2-170#Sistema planetário|K2-170b]]
|
|
|0.127{{±|0.018|0.012}}
|0.127{{±|0.018|0.012}}
Linha 1 298: Linha 1 082:
|0.964{{±|0.032}}
|0.964{{±|0.032}}
|5748{{±|50}}
|5748{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-170c]]
|[[K2-170#Sistema planetário|K2-170c]]
|
|
|0.161{{±|0.022|0.014}}
|0.161{{±|0.022|0.014}}
Linha 1 310: Linha 1 094:
|0.964{{±|0.032}}
|0.964{{±|0.032}}
|5748{{±|50}}
|5748{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-171b]]
|[[K2-171b]]
Linha 1 322: Linha 1 106:
|0.892{{±|0.060|0.027}}
|0.892{{±|0.060|0.027}}
|5250{{±|50}}
|5250{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-172b]]
|[[K2-172#Sistema planetário|K2-172b]]
|
|
|0.1486{{±|0.014|0.0085}}
|0.1486{{±|0.014|0.0085}}
Linha 1 334: Linha 1 118:
|0.934{{±|0.026|0.027}}
|0.934{{±|0.026|0.027}}
|5569{{±|50}}
|5569{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-172c]]
|[[K2-172#Sistema planetário|K2-172c]]
|
|
|0.286{{±|0.017|0.012}}
|0.286{{±|0.017|0.012}}
Linha 1 346: Linha 1 130:
|0.934{{±|0.026|0.027}}
|0.934{{±|0.026|0.027}}
|5569{{±|50}}
|5569{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-173b]]
|[[K2-173b]]
Linha 1 358: Linha 1 142:
|0.881{{±|0.034|0.036}}
|0.881{{±|0.034|0.036}}
|5580{{±|70}}
|5580{{±|70}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-174b]]
|[[K2-174b]]
Linha 1 370: Linha 1 154:
|0.668{{±|0.022|0.021}}
|0.668{{±|0.022|0.021}}
|4500{{±|50}}
|4500{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-175b]]
|[[K2-175b]]
Linha 1 382: Linha 1 166:
|1.095{{±|0.057|0.039}}
|1.095{{±|0.057|0.039}}
|5909{{±|50}}
|5909{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-176b]]
|[[K2-176b]]
Linha 1 394: Linha 1 178:
|0.939{{±|0.020|0.025}}
|0.939{{±|0.020|0.025}}
|5428{{±|50}}
|5428{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-177b]]
|[[K2-177b]]
Linha 1 406: Linha 1 190:
|1.211{{±|0.032|0.038}}
|1.211{{±|0.032|0.038}}
|6063{{±|50}}
|6063{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-178b]]
|[[K2-178b]]
Linha 1 418: Linha 1 202:
|0.951{{±|0.023|0.027}}
|0.951{{±|0.023|0.027}}
|5525{{±|50}}
|5525{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-179b]]
|[[K2-179b]]
Linha 1 430: Linha 1 214:
|0.824{{±|0.022|0.027}}
|0.824{{±|0.022|0.027}}
|5015{{±|50}}
|5015{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-180b]]
|[[K2-180b]]
Linha 1 442: Linha 1 226:
|0.730{{±|0.020|0.022}}
|0.730{{±|0.020|0.022}}
|5263{{±|50}}
|5263{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-181b]]
|[[K2-181b]]
Linha 1 454: Linha 1 238:
|1.044{{±|0.024|0.029}}
|1.044{{±|0.024|0.029}}
|5609{{±|50}}
|5609{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-182b]]
|[[K2-182b]]
Linha 1 466: Linha 1 250:
|0.847{{±|0.024|0.031}}
|0.847{{±|0.024|0.031}}
|5159{{±|50}}
|5159{{±|50}}
|Confirmado em 2021<ref name=Murphy2021>{{citation|arxiv=2110.05502|ano=2021|título=Another Superdense Sub-Neptune in K2-182 b and Refined Mass Measurements for K2-199 b and C|doi=10.3847/1538-3881/ac2830|último1=Akana Murphy|primeiro1=Joseph M.|último2=Kosiarek|primeiro2=Molly R.|último3=Batalha|primeiro3=Natalie M.|último4=Gonzales|primeiro4=Erica J.|último5=Isaacson|primeiro5=Howard|último6=Petigura|primeiro6=Erik A.|último7=Weiss|primeiro7=Lauren M.|último8=Grunblatt|primeiro8=Samuel K.|último9=Ciardi|primeiro9=David R.|último10=Fulton|primeiro10=Benjamin|último11=Hirsch|primeiro11=Lea A.|último12=Behmard|primeiro12=Aida|último13=Rosenthal|primeiro13=Lee J.|periódico=The Astronomical Journal|volume=162|número=6|página=294|bibcode=2021AJ....162..294A|s2cid=238634110}}</ref>
|<ref name=Mayo2018/><ref name=Livingston2018/> Confirmado em 2021<ref name=Murphy2021>{{citation|arxiv=2110.05502|ano=2021|título=Another Superdense Sub-Neptune in K2-182 b and Refined Mass Measurements for K2-199 b and C|doi=10.3847/1538-3881/ac2830|último1=Akana Murphy|primeiro1=Joseph M.|último2=Kosiarek|primeiro2=Molly R.|último3=Batalha|primeiro3=Natalie M.|último4=Gonzales|primeiro4=Erica J.|último5=Isaacson|primeiro5=Howard|último6=Petigura|primeiro6=Erik A.|último7=Weiss|primeiro7=Lauren M.|último8=Grunblatt|primeiro8=Samuel K.|último9=Ciardi|primeiro9=David R.|último10=Fulton|primeiro10=Benjamin|último11=Hirsch|primeiro11=Lea A.|último12=Behmard|primeiro12=Aida|último13=Rosenthal|primeiro13=Lee J.|periódico=The Astronomical Journal|volume=162|número=6|página=294|bibcode=2021AJ....162..294A|s2cid=238634110}}</ref>
|-
|-
|[[K2-183b]]
|[[K2-183#Sistema planetário|K2-183b]]
|
|
|0.098{{±|0.090}}
|0.098{{±|0.090}}
Linha 1 478: Linha 1 262:
|0.942{{±|0.021|0.025}}
|0.942{{±|0.021|0.025}}
|5482{{±|50}}
|5482{{±|50}}
|<ref name=Adams2020/>
|<ref name=Mayo2018/><ref name=Livingston2018/><ref name=Adams2020/>
|-
|-
|[[K2-183c]]
|[[K2-183#Sistema planetário|K2-183c]]
|
|
|0.224{{±|0.024|0.012}}
|0.224{{±|0.024|0.012}}
Linha 1 490: Linha 1 274:
|0.942{{±|0.021|0.025}}
|0.942{{±|0.021|0.025}}
|5482{{±|50}}
|5482{{±|50}}
|<ref name=Adams2020/>
|<ref name=Mayo2018/><ref name=Livingston2018/><ref name=Adams2020/>
|-
|-
|[[K2-183d]]
|[[K2-183d]]
Linha 1 514: Linha 1 298:
|0.819{{±|0.028|0.030}}
|0.819{{±|0.028|0.030}}
|5252{{±|50}}
|5252{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-185b]]
|[[K2-185b]]
Linha 1 526: Linha 1 310:
|0.976{{±|0.027|0.028}}
|0.976{{±|0.027|0.028}}
|5722{{±|50}}
|5722{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-186b]]
|[[K2-186b]]
Linha 1 538: Linha 1 322:
|1.019{{±|0.023|0.027}}
|1.019{{±|0.023|0.027}}
|5784{{±|50}}
|5784{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-187b]]
|[[K2-187#Sistema planetário|K2-187b]]
|
|
|0.123
|0.123
Linha 1 550: Linha 1 334:
|0.97
|0.97
|5477
|5477
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-187c]]
|[[K2-187#Sistema planetário|K2-187c]]
|
|
|0.152{{±|0.022|0.010}}
|0.152{{±|0.022|0.010}}
Linha 1 562: Linha 1 346:
|0.967{{±|0.025|0.024}}
|0.967{{±|0.025|0.024}}
|5477{{±|50}}
|5477{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-187d]]
|[[K2-187#Sistema planetário|K2-187d]]
|
|
|0.287{{±|0.045|0.022}}
|0.287{{±|0.045|0.022}}
Linha 1 574: Linha 1 358:
|0.967{{±|0.025|0.024}}
|0.967{{±|0.025|0.024}}
|5477{{±|50}}
|5477{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-187e]]
|[[K2-187#Sistema planetário|K2-187e]]
|
|
|0.201{{±|0.019|0.012}}
|0.201{{±|0.019|0.012}}
Linha 1 586: Linha 1 370:
|0.967{{±|0.025|0.024}}
|0.967{{±|0.025|0.024}}
|5477{{±|50}}
|5477{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-188b]]
|[[K2-188#Sistema planetário|K2-188b]]
|
|
|0.112{{±|0.015|0.010}}
|0.112{{±|0.015|0.010}}
Linha 1 598: Linha 1 382:
|1.107{{±|0.031|0.025}}
|1.107{{±|0.031|0.025}}
|5982{{±|50}}
|5982{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-188c]]
|[[K2-188#Sistema planetário|K2-188c]]
|
|
|0.234{{±|0.028|0.016}}
|0.234{{±|0.028|0.016}}
Linha 1 610: Linha 1 394:
|1.107{{±|0.031|0.025}}
|1.107{{±|0.031|0.025}}
|5982{{±|50}}
|5982{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-189b]]
|[[K2-189#Sistema planetário|K2-189b]]
|
|
|0.1349{{±|0.0136|0.0085}}
|0.1349{{±|0.0136|0.0085}}
Linha 1 622: Linha 1 406:
|0.928{{±|0.024|0.027}}
|0.928{{±|0.024|0.027}}
|5503{{±|50}}
|5503{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-189c]]
|[[K2-189#Sistema planetário|K2-189c]]
|
|
|0.222{{±|0.028|0.012}}
|0.222{{±|0.028|0.012}}
Linha 1 634: Linha 1 418:
|0.928{{±|0.024|0.027}}
|0.928{{±|0.024|0.027}}
|5503{{±|50}}
|5503{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-190b]]
|[[K2-190#Sistema planetário|K2-190b]]
|
|
|0.1210{{±|0.0157|0.0091}}
|0.1210{{±|0.0157|0.0091}}
Linha 1 646: Linha 1 430:
|0.905{{±|0.033|0.036}}
|0.905{{±|0.033|0.036}}
|5631{{±|50}}
|5631{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-190c]]
|[[K2-190#Sistema planetário|K2-190c]]
|
|
|0.0975{{±|0.0135|0.0082}}
|0.0975{{±|0.0135|0.0082}}
Linha 1 658: Linha 1 442:
|0.905{{±|0.033|0.036}}
|0.905{{±|0.033|0.036}}
|5631{{±|50}}
|5631{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-191b]]
|[[K2-191b]]
Linha 1 670: Linha 1 454:
|0.901{{±|0.026|0.028}}
|0.901{{±|0.026|0.028}}
|5176{{±|50}}
|5176{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-192b]]
|[[K2-192b]]
Linha 1 682: Linha 1 466:
|0.873{{±|0.024|0.031}}
|0.873{{±|0.024|0.031}}
|5252{{±|50}}
|5252{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-193b]]
|[[K2-193b]]
Linha 1 694: Linha 1 478:
|0.994{{±|0.029|0.027}}
|0.994{{±|0.029|0.027}}
|5623{{±|50}}
|5623{{±|50}}
|<ref name=Mayo2018/> Baixa fidelidade<ref name=Livingston2018/>
|
|-
|-
|[[K2-194b]]
|[[K2-194b]]
Linha 1 706: Linha 1 490:
|1.110{{±|0.046|0.035}}
|1.110{{±|0.046|0.035}}
|5979{{±|52}}
|5979{{±|52}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-195b]]
|[[K2-195#Sistema planetário|K2-195b]]
|
|
|0.262{{±|0.018|0.012}}
|0.262{{±|0.018|0.012}}
Linha 1 718: Linha 1 502:
|0.963{{±|0.028|0.031}}
|0.963{{±|0.028|0.031}}
|5712{{±|50}}
|5712{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-195c]]
|[[K2-195#Sistema planetário|K2-195c]]
|
|
|0.230{{±|0.024|0.013}}
|0.230{{±|0.024|0.013}}
Linha 1 730: Linha 1 514:
|0.963{{±|0.028|0.031}}
|0.963{{±|0.028|0.031}}
|5712{{±|50}}
|5712{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-196b]]
|[[K2-196b]]
Linha 1 742: Linha 1 526:
|1.162{{±|0.075|0.045}}
|1.162{{±|0.075|0.045}}
|6045{{±|50}}
|6045{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-197b]]
|[[K2-197b]]
Linha 1 754: Linha 1 538:
|0.975{{±|0.025|0.029}}
|0.975{{±|0.025|0.029}}
|5675{{±|50}}
|5675{{±|50}}
|<ref name=Mayo2018/> Baixa fidelidade<ref name=Livingston2018/>
|
|-
|-
|[[K2-198b]]
|[[K2-198b]]
Linha 1 766: Linha 1 550:
|0.836{{±|0.029}}
|0.836{{±|0.029}}
|5262{{±|50}}
|5262{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-199b]]
|[[K2-199#Sistema planetário|K2-199b]]
|0.022{{±|0.006}}
|0.022{{±|0.006}}
|0.1679{{±|0.0167|0.0079}}
|0.1679{{±|0.0167|0.0079}}
Linha 1 778: Linha 1 562:
|0.706{{±|0.024|0.023}}
|0.706{{±|0.024|0.023}}
|4681{{±|50}}
|4681{{±|50}}
|<ref name=Murphy2021/>
|<ref name=Mayo2018/><ref name=Livingston2018/><ref name=Murphy2021/>
|-
|-
|[[K2-199c]]
|[[K2-199#Sistema planetário|K2-199c]]
|0.039{{±|0.007}}
|0.039{{±|0.007}}
|0.253{{±|0.015|0.010}}
|0.253{{±|0.015|0.010}}
Linha 1 790: Linha 1 574:
|0.706{{±|0.024|0.023}}
|0.706{{±|0.024|0.023}}
|4681{{±|50}}
|4681{{±|50}}
|<ref name=Murphy2021/>
|<ref name=Mayo2018/><ref name=Livingston2018/><ref name=Murphy2021/>
|-
|-
|[[K2-200b]]
|[[K2-200b]]
Linha 1 802: Linha 1 586:
|0.860{{±|0.023|0.027}}
|0.860{{±|0.023|0.027}}
|5233{{±|50}}
|5233{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-201b]]
|[[K2-201#Sistema planetário|K2-201b]]
|
|
|0.1249{{±|0.0120|0.0069}}
|0.1249{{±|0.0120|0.0069}}
Linha 1 814: Linha 1 598:
|0.956{{±|0.020|0.021}}
|0.956{{±|0.020|0.021}}
|5507{{±|50}}
|5507{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-201c]]
|[[K2-201#Sistema planetário|K2-201c]]
|
|
|0.293{{±|0.036|0.016}}
|0.293{{±|0.036|0.016}}
Linha 1 826: Linha 1 610:
|0.956{{±|0.020|0.021}}
|0.956{{±|0.020|0.021}}
|5507{{±|50}}
|5507{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-202b]]
|[[K2-202b]]
Linha 1 838: Linha 1 622:
|0.971{{±|0.030|0.028}}
|0.971{{±|0.030|0.028}}
|5491{{±|58}}
|5491{{±|58}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-203b]]
|[[K2-203b]]
Linha 1 850: Linha 1 634:
|0.794{{±|0.033|0.028}}
|0.794{{±|0.033|0.028}}
|5000{{±|50}}
|5000{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-204b]]
|[[K2-204b]]
Linha 1 862: Linha 1 646:
|1.009{{±|0.031|0.027}}
|1.009{{±|0.031|0.027}}
|5755{{±|50}}
|5755{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-205b]]
|[[K2-205b]]
Linha 1 874: Linha 1 658:
|0.951{{±|0.038|0.036}}
|0.951{{±|0.038|0.036}}
|5890{{±|50}}
|5890{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-206b]]
|[[K2-206b]]
Linha 1 886: Linha 1 670:
|0.789{{±|0.030|0.028}}
|0.789{{±|0.030|0.028}}
|5043{{±|50}}
|5043{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-207b]]
|[[K2-207b]]
Linha 1 898: Linha 1 682:
|0.942{{±|0.028}}
|0.942{{±|0.028}}
|5522{{±|50}}
|5522{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-208b]]
|[[K2-208b]]
Linha 1 910: Linha 1 694:
|0.925{{±|0.030}}
|0.925{{±|0.030}}
|5582{{±|50}}
|5582{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-209b]]
|[[K2-209b]]
Linha 1 922: Linha 1 706:
|0.745{{±|0.026|0.024}}
|0.745{{±|0.026|0.024}}
|4720{{±|50}}
|4720{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-210b]]
|[[K2-210b]]
Linha 1 934: Linha 1 718:
|0.912{{±|0.023|0.029}}
|0.912{{±|0.023|0.029}}
|5396{{±|50}}
|5396{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-211b]]
|[[K2-211b]]
Linha 1 946: Linha 1 730:
|0.882{{±|0.019|0.027}}
|0.882{{±|0.019|0.027}}
|5221{{±|50}}
|5221{{±|50}}
|Outro planeta descoberto em 2020<ref name=Adams2020/>
|<ref name=Mayo2018/> Outro planeta descoberto em 2020<ref name=Adams2020/>
|-
|-
|[[K2-212b]]
|[[K2-212b]]
Linha 1 958: Linha 1 742:
|0.622{{±|0.020|0.018}}
|0.622{{±|0.020|0.018}}
|4349{{±|50}}
|4349{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-213b]]
|[[K2-213b]]
Linha 1 970: Linha 1 754:
|1.070{{±|0.055|0.038}}
|1.070{{±|0.055|0.038}}
|5794{{±|50}}
|5794{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-214b]]
|[[K2-214b]]
Linha 1 982: Linha 1 766:
|1.022{{±|0.031|0.028}}
|1.022{{±|0.031|0.028}}
|5768{{±|50}}
|5768{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-215b]]
|[[K2-215b]]
Linha 1 994: Linha 1 778:
|1.000{{±|0.026|0.027}}
|1.000{{±|0.026|0.027}}
|5704{{±|50}}
|5704{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-216b]]
|[[K2-216b]]
Linha 2 006: Linha 1 790:
|0.699{{±|0.023}}
|0.699{{±|0.023}}
|4591{{±|50}}
|4591{{±|50}}
|<ref name=Mayo2018/><ref name=Livingston2018/>
|
|-
|-
|[[K2-217b]]
|[[K2-217b]]
Linha 2 018: Linha 1 802:
|1.103{{±|0.046|0.037}}
|1.103{{±|0.046|0.037}}
|5967{{±|50}}
|5967{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-218b]]
|[[K2-218b]]
Linha 2 030: Linha 1 814:
|1.048{{±|0.031|0.028}}
|1.048{{±|0.031|0.028}}
|5757{{±|50}}
|5757{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-219b]]
|[[K2-219#Sistema planetário|K2-219b]]
|
|
|0.120{{±|0.018|0.016}}
|0.120{{±|0.018|0.016}}
Linha 2 042: Linha 1 826:
|1.022{{±|0.034|0.030}}
|1.022{{±|0.034|0.030}}
|5753{{±|50}}
|5753{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-219c]]
|[[K2-219#Sistema planetário|K2-219c]]
|
|
|0.128{{±|0.019|0.017}}
|0.128{{±|0.019|0.017}}
Linha 2 054: Linha 1 838:
|1.022{{±|0.034|0.030}}
|1.022{{±|0.034|0.030}}
|5753{{±|50}}
|5753{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-219d]]
|[[K2-219#Sistema planetário|K2-219d]]
|
|
|0.230{{±|0.032|0.029}}
|0.230{{±|0.032|0.029}}
Linha 2 066: Linha 1 850:
|1.022{{±|0.034|0.030}}
|1.022{{±|0.034|0.030}}
|5753{{±|50}}
|5753{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-220b]]
|[[K2-220b]]
Linha 2 078: Linha 1 862:
|0.960{{±|0.026|0.029}}
|0.960{{±|0.026|0.029}}
|5599{{±|50}}
|5599{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-221b]]
|[[K2-221b]]
Linha 2 090: Linha 1 874:
|1.011{{±|0.024|0.025}}
|1.011{{±|0.024|0.025}}
|5716{{±|50}}
|5716{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-222b]]
|[[K2-222b]]
Linha 2 102: Linha 1 886:
|0.950{{±|0.040|0.036}}
|0.950{{±|0.040|0.036}}
|5934{{±|50}}
|5934{{±|50}}
|<ref>{{citation|arxiv=2111.02608|ano=2021|título=K2-79b and K2-222b: Mass measurements of two small exoplanets with periods beyond 10 days that overlap with periodic magnetic activity signals|último1=Nava|primeiro1=Chantanelle|último2=López-Morales|primeiro2=Mercedes|último3=Mortier|primeiro3=Annelies|último4=Zeng|primeiro4=Li|último5=Giles|primeiro5=Helen A. C.|último6=Bieryla|primeiro6=Allyson|último7=Vanderburg|primeiro7=Andrew|último8=Buchhave|primeiro8=Lars A.|último9=Poretti|primeiro9=Ennio|último10=Saar|primeiro10=Steven H.|último11=Dumusque|primeiro11=Xavier|último12=Latham|primeiro12=David W.|último13=Charbonneau|primeiro13=David|último14=Damasso|primeiro14=Mario|último15=Bonomo|primeiro15=Aldo S.|último16=Lovis|primeiro16=Christophe|autor17=Andrew Collier Cameron|último18=Eastman|primeiro18=Jason D.|último19=Sozzetti|primeiro19=Alessandro|último20=Cosentino|primeiro20=Rosario|último21=Pedani|primeiro21=Marco|último22=Pepe|primeiro22=Francesco|último23=Molinari|primeiro23=Emilio|último24=Sasselov|primeiro24=Dimitar|último25=Mayor|primeiro25=Michel|último26=Stalport|primeiro26=Manu|último27=Malavolta|primeiro27=Luca|último28=Rice|primeiro28=Ken|último29=Watson|primeiro29=Christopher A.|último30=Martinez Fiorenzano|primeiro30=A. F.|periódico=The Astronomical Journal|volume=163|número=2|página=41|doi=10.3847/1538-3881/ac3141|bibcode=2022AJ....163...41N|s2cid=242757805|numero-autores=1}}</ref>
|<ref name=Mayo2018/><ref name=Livingston2018/><ref>{{citation|arxiv=2111.02608|ano=2021|título=K2-79b and K2-222b: Mass measurements of two small exoplanets with periods beyond 10 days that overlap with periodic magnetic activity signals|último1=Nava|primeiro1=Chantanelle|último2=López-Morales|primeiro2=Mercedes|último3=Mortier|primeiro3=Annelies|último4=Zeng|primeiro4=Li|último5=Giles|primeiro5=Helen A. C.|último6=Bieryla|primeiro6=Allyson|último7=Vanderburg|primeiro7=Andrew|último8=Buchhave|primeiro8=Lars A.|último9=Poretti|primeiro9=Ennio|último10=Saar|primeiro10=Steven H.|último11=Dumusque|primeiro11=Xavier|último12=Latham|primeiro12=David W.|último13=Charbonneau|primeiro13=David|último14=Damasso|primeiro14=Mario|último15=Bonomo|primeiro15=Aldo S.|último16=Lovis|primeiro16=Christophe|autor17=Andrew Collier Cameron|último18=Eastman|primeiro18=Jason D.|último19=Sozzetti|primeiro19=Alessandro|último20=Cosentino|primeiro20=Rosario|último21=Pedani|primeiro21=Marco|último22=Pepe|primeiro22=Francesco|último23=Molinari|primeiro23=Emilio|último24=Sasselov|primeiro24=Dimitar|último25=Mayor|primeiro25=Michel|último26=Stalport|primeiro26=Manu|último27=Malavolta|primeiro27=Luca|último28=Rice|primeiro28=Ken|último29=Watson|primeiro29=Christopher A.|último30=Martinez Fiorenzano|primeiro30=A. F.|periódico=The Astronomical Journal|volume=163|número=2|página=41|doi=10.3847/1538-3881/ac3141|bibcode=2022AJ....163...41N|s2cid=242757805|numero-autores=1}}</ref>
|-
|-
|[[K2-223b]]
|[[K2-223#Sistema planetário|K2-223b]]
|
|
|0.0812{{±|0.0088|0.0066}}
|0.0812{{±|0.0088|0.0066}}
Linha 2 114: Linha 1 898:
|1.06{{±|0.02}}
|1.06{{±|0.02}}
|5835{{±|38|40}}
|5835{{±|38|40}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-223c]]
|[[K2-223#Sistema planetário|K2-223c]]
|
|
|0.144{{±|0.010|0.006}}
|0.144{{±|0.010|0.006}}
Linha 2 126: Linha 1 910:
|1.06{{±|0.02}}
|1.06{{±|0.02}}
|5835{{±|38|40}}
|5835{{±|38|40}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-224b]]
|[[K2-224b]]
Linha 2 138: Linha 1 922:
|0.91{{±|0.02}}
|0.91{{±|0.02}}
|5620{{±|42|45}}
|5620{{±|42|45}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-224c]]
|[[K2-224c]]
Linha 2 150: Linha 1 934:
|0.91{{±|0.02}}
|0.91{{±|0.02}}
|5620{{±|42|45}}
|5620{{±|42|45}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-225b]]
|[[K2-225b]]
Linha 2 162: Linha 1 946:
|1.27{{±|0.02|0.04}}
|1.27{{±|0.02|0.04}}
|5742{{±|49|47}}
|5742{{±|49|47}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-226b]]
|[[K2-226b]]
Linha 2 174: Linha 1 958:
|0.88{{±|0.03}}
|0.88{{±|0.03}}
|5424{{±|48|46}}
|5424{{±|48|46}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-227b]]
|[[K2-227b]]
Linha 2 186: Linha 1 970:
|0.951{{±|0.028|0.030}}
|0.951{{±|0.028|0.030}}
|5673{{±|50}}
|5673{{±|50}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-228b]]
|[[K2-228b]]
Linha 2 198: Linha 1 982:
|0.71{{±|0.02}}
|0.71{{±|0.02}}
|4715{{±|48|46}}
|4715{{±|48|46}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-229b]]
|[[K2-229b]]
Linha 2 210: Linha 1 994:
|0.87{{±|0.01}}
|0.87{{±|0.01}}
|5315{{±|25|31}}
|5315{{±|25|31}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-229c]]
|[[K2-229c]]
Linha 2 222: Linha 2 006:
|0.87{{±|0.01}}
|0.87{{±|0.01}}
|5315{{±|25|31}}
|5315{{±|25|31}}
|<ref name=Mayo2018/><ref name=Livingston2018-06/>
|
|-
|-
|[[K2-230b]]
|[[K2-230b]]
Linha 2 234: Linha 2 018:
|1.11{{±|0.02}}
|1.11{{±|0.02}}
|5945{{±|23|25}}
|5945{{±|23|25}}
|<ref name=Mayo2018/>
|
|-
|-
|[[K2-231b]]
|[[K2-231b]]
Linha 2 788: Linha 2 572:
|
|
|-
|-
|[[K2-268b]]
|[[K2-268#Sistema planetário|K2-268b]]
|
|
|0.126{{±|0.012}}
|0.126{{±|0.012}}
Linha 2 798: Linha 2 582:
|0.84{{±|0.02}}
|0.84{{±|0.02}}
|5068{{±|51}}
|5068{{±|51}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-268c]]
|[[K2-268#Sistema planetário|K2-268c]]
|
|
|0.240{{±|0.021}}
|0.240{{±|0.021}}
Linha 2 810: Linha 2 594:
|0.84{{±|0.02}}
|0.84{{±|0.02}}
|5068{{±|51}}
|5068{{±|51}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-269b]]
|[[K2-269b]]
Linha 2 822: Linha 2 606:
|1.16{{±|0.04}}
|1.16{{±|0.04}}
|6209{{±|88}}
|6209{{±|88}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-270b]]
|[[K2-270#Sistema planetário|K2-270b]]
|
|
|0.123{{±|0.010}}
|0.123{{±|0.010}}
Linha 2 834: Linha 2 618:
|0.85{{±|0.02}}
|0.85{{±|0.02}}
|4877{{±|58}}
|4877{{±|58}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-270c]]
|[[K2-270#Sistema planetário|K2-270c]]
|
|
|0.263{{±|0.014}}
|0.263{{±|0.014}}
Linha 2 846: Linha 2 630:
|0.85{{±|0.02}}
|0.85{{±|0.02}}
|4877{{±|58}}
|4877{{±|58}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-271b]]
|[[K2-271b]]
Linha 2 858: Linha 2 642:
|0.83{{±|0.03}}
|0.83{{±|0.03}}
|5644{{±|71}}
|5644{{±|71}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-272b]]
|[[K2-272b]]
Linha 2 870: Linha 2 654:
|0.81{{±|0.04}}
|0.81{{±|0.04}}
|5419{{±|79}}
|5419{{±|79}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-273b]]
|[[K2-273b]]
Linha 2 882: Linha 2 666:
|0.90{{±|0.03}}
|0.90{{±|0.03}}
|5200{{±|67}}
|5200{{±|67}}
|<ref name=Livingston2018/>
|-
|[[K2-274b]]
|
|
|0.196{{±|0.011}}
|14.129714{{±|0.0021022|0.001876}}
|0.1064{{±|0.0009|0.0008}}
|589{{±|9}}
|style="background:#FFFF00"|Trânsito
|1013.0{{±|9.39}}
|0.81{{±|0.02}}
|5065{{±|60}}
|<ref name=Livingston2018/>
|-
|-
|[[K2-275b]]
|[[K2-275#Sistema planetário|K2-275b]]
|
|
|0.200{{±|0.011}}
|0.200{{±|0.011}}
Linha 2 894: Linha 2 690:
|0.79{{±|0.02}}
|0.79{{±|0.02}}
|4812{{±|59}}
|4812{{±|59}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-275c]]
|[[K2-275#Sistema planetário|K2-275c]]
|
|
|0.209{{±|0.009}}
|0.209{{±|0.009}}
Linha 2 906: Linha 2 702:
|0.79{{±|0.02}}
|0.79{{±|0.02}}
|4812{{±|59}}
|4812{{±|59}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-276b]]
|[[K2-276b]]
Linha 2 918: Linha 2 714:
|0.82{{±|0.02}}
|0.82{{±|0.02}}
|5139{{±|62}}
|5139{{±|62}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-277b]]
|[[K2-277b]]
Linha 2 930: Linha 2 726:
|1.02{{±|0.03}}
|1.02{{±|0.03}}
|5741{{±|65}}
|5741{{±|65}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-278b]]
|[[K2-278b]]
Linha 2 942: Linha 2 738:
|1.40{{±|0.08}}
|1.40{{±|0.08}}
|6747{{±|383}}
|6747{{±|383}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-279b]]
|[[K2-279b]]
Linha 2 954: Linha 2 750:
|0.79{{±|0.03}}
|0.79{{±|0.03}}
|5558{{±|70}}
|5558{{±|70}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-280b]]
|[[K2-280b]]
Linha 2 966: Linha 2 762:
|1.11{{±|0.04}}
|1.11{{±|0.04}}
|5742{{±|90}}
|5742{{±|90}}
|<ref>{{citar periódico|arxiv=2007.07939|título=K2-280 b – a low density warm sub-Saturn around a mildly evolved star|ano=2020|doi=10.1093/mnras/staa2077|último1 =Nowak|primeiro1 =Grzegorz|periódico=Monthly Notices of the Royal Astronomical Society|volume=497|número=4|páginas=4423–4435|numero-autores=etal}}</ref><ref>{{citar periódico|arxiv=1810.04074|título=Sixty Validated Planets from K2 Campaigns 5–8|ano=2018|doi=10.3847/1538-3881/aae778|último1 =Livingston|primeiro1 =John H.|numero-autores=etal|periódico=The Astronomical Journal|volume=156|número=6|página=277|bibcode=2018AJ....156..277L|s2cid=119387939}}</ref><ref>{{citar periódico|arxiv=1711.06377|título=Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy|ano=2017|doi=10.3847/1538-3881/aa9b83|último1 =Petigura|primeiro1 =Erik A.|numero-autores=etal|periódico=The Astronomical Journal|volume=155|página=21|s2cid=55674757}}</ref><ref>{{citar periódico|arxiv=1802.05277|título=275 Candidates and 149 Validated Planets Orbiting Bright Stars inK2 Campaigns 0–10|ano=2018|doi=10.3847/1538-3881/aaadff|último1 =Mayo|primeiro1 =Andrew W.|numero-autores=etal|periódico=The Astronomical Journal|volume=155|número=3|página=136|bibcode=2018AJ....155..136M|s2cid=85524387}}</ref>
|<ref name=Livingston2018>{{citar periódico|arxiv=2007.07939|título=K2-280 b – a low density warm sub-Saturn around a mildly evolved star|ano=2020|doi=10.1093/mnras/staa2077|último1=Nowak|primeiro1=Grzegorz|periódico=Monthly Notices of the Royal Astronomical Society|volume=497|número=4|páginas=4423–4435|numero-autores=etal}}</ref><ref>{{citar periódico|arxiv=1810.04074|título=Sixty Validated Planets from K2 Campaigns 5–8|ano=2018|doi=10.3847/1538-3881/aae778|último1=Livingston|primeiro1=John H.|numero-autores=etal|periódico=The Astronomical Journal|volume=156|número=6|página=277|bibcode=2018AJ....156..277L|s2cid=119387939}}</ref><ref>{{citar periódico|arxiv=1711.06377|título=Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy|ano=2017|doi=10.3847/1538-3881/aa9b83|último1=Petigura|primeiro1=Erik A.|numero-autores=etal|periódico=The Astronomical Journal|volume=155|página=21|s2cid=55674757}}</ref><ref name=Mayo2018>{{citar periódico|arxiv=1802.05277|título=275 Candidates and 149 Validated Planets Orbiting Bright Stars inK2 Campaigns 0–10|ano=2018|doi=10.3847/1538-3881/aaadff|último1=Mayo|primeiro1=Andrew W.|numero-autores=etal|periódico=The Astronomical Journal|volume=155|número=3|página=136|bibcode=2018AJ....155..136M|s2cid=85524387}}</ref>
|-
|-
|[[K2-281b]]
|[[K2-281b]]
Linha 2 978: Linha 2 774:
|0.82{{±|0.03}}
|0.82{{±|0.03}}
|4812{{±|72}}
|4812{{±|72}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-282b]]
|[[K2-282b]]
Linha 2 990: Linha 2 786:
|0.95{{±|0.04}}
|0.95{{±|0.04}}
|5523{{±|82}}
|5523{{±|82}}
|Mais dois exoplanetas descobertos em 2019 e 2020<ref name=Adams2020/>
|<ref name=Livingston2018/>Mais dois exoplanetas descobertos em 2019 e 2020<ref name=Adams2020/>
|-
|-
|[[K2-283b]]
|[[K2-283b]]
Linha 3 002: Linha 2 798:
|0.89{{±|0.03}}
|0.89{{±|0.03}}
|5060{{±|70}}
|5060{{±|70}}
|<ref name=Livingston2018/>
|
|-
|-
|[[K2-284b]]
|[[K2-284b]]
Linha 3 650: Linha 3 446:
|1.39{{±|0.14}}
|1.39{{±|0.14}}
|6400{{±|100}}
|6400{{±|100}}
|Nome próprio '''Isli'''
|<ref name=Barkaoui2018/> Nome próprio '''Isli'''
|-
|-
|[[WASP-162b]]
|[[WASP-162b]]
Linha 3 674: Linha 3 470:
|0.97{{±|0.15}}
|0.97{{±|0.15}}
|5500{{±|200}}
|5500{{±|200}}
|<ref name=Barkaoui2018/>
|
|-
|-
|[[WASP-164b]]
|[[WASP-164b]]
Linha 3 710: Linha 3 506:
|1.19{{±|0.06}}
|1.19{{±|0.06}}
|6050{{±|50}}
|6050{{±|50}}
|<ref>{{citation|arxiv=1811.05292|ano=2018|título=WASP-166b: a bloated super-Neptune transiting a V = 9 star}}</ref><ref>{{citation|arxiv=2203.04494|ano=2022|título=The Hot Neptune WASP-166 b with ESPRESSO II: Confirmation of atmospheric sodium}}</ref>
|<ref>{{citation|arxiv=1811.05292|ano=2018|título=WASP-166b: a bloated super-Neptune transiting a V = 9 star}}</ref><ref>{{citation|arxiv=2203.04494|ano=2022|título=The Hot Neptune WASP-166 b with ESPRESSO II: Confirmation of atmospheric sodium}}</ref><ref>{{citation|arxiv=2207.10127|ano=2022|título=The Hot Neptune WASP-166 b with ESPRESSO I: Refining the Planetary Architecture and Stellar Variability}}</ref>
|-
|-
|[[WASP-168b]]
|[[WASP-168b]]
Linha 3 734: Linha 3 530:
|0.93{{±|0.15}}
|0.93{{±|0.15}}
|5600{{±|150}}
|5600{{±|150}}
|<ref name=Barkaoui2018>{{citation|arxiv=1807.06548|ano=2018|título=Discovery of three new transiting hot Jupiters: WASP-161 b, WASP-163 b and WASP-170 b}}</ref>
|
|-
|-
|[[WASP-172b]]
|[[WASP-172b]]
Linha 3 770: Linha 3 566:
|1.30
|1.30
|6400
|6400
|<ref>{{citation|arxiv=1802.00766|ano=2018|título=Discovery of WASP-174b: Doppler tomography of a near-grazing transit}}</ref>
|
|-
|-
|[[Wolf 503b]]
|[[Wolf 503b]]
Linha 3 791: Linha 3 587:
* [[Lista de exoplanetas descobertos entre 2000-2009]] (379)
* [[Lista de exoplanetas descobertos entre 2000-2009]] (379)
* [[Lista de exoplanetas descobertos em 2010]] (108)
* [[Lista de exoplanetas descobertos em 2010]] (108)
* [[Lista de exoplanetas descobertos em 2011]] (177)
* [[Lista de exoplanetas descobertos em 2011]] (178)
* [[Lista de exoplanetas descobertos em 2012]] (148)
* [[Lista de exoplanetas descobertos em 2012]] (148)
* [[Lista de exoplanetas descobertos em 2013]] (151)
* [[Lista de exoplanetas descobertos em 2013]] (151)
* [[Lista de exoplanetas descobertos em 2014]] (878)
* [[Lista de exoplanetas descobertos em 2014]] (878)
* [[Lista de exoplanetas descobertos em 2015]] (149)
* [[Lista de exoplanetas descobertos em 2015]] (151)
* [[Lista de exoplanetas descobertos em 2016]] (1.498)
* [[Lista de exoplanetas descobertos em 2016]] (1.512)
* [[Lista de exoplanetas descobertos em 2017]] (154)
* [[Lista de exoplanetas descobertos em 2017]] (152)
* [[Lista de exoplanetas descobertos em 2018]] (313)
* [[Lista de exoplanetas descobertos em 2018]] (297)
* [[Lista de exoplanetas descobertos em 2019]] (191)
* [[Lista de exoplanetas descobertos em 2019]] (191)
* [[Lista de exoplanetas descobertos em 2020]] (260)
* [[Lista de exoplanetas descobertos em 2020]] (264)
* [[Lista de exoplanetas descobertos em 2021]] (236)
* [[Lista de exoplanetas descobertos em 2021]] (243)
* [[Lista de exoplanetas descobertos em 2022]] (184)
* [[Lista de exoplanetas descobertos em 2022]] (292)
* [[Lista de exoplanetas potencialmente habitáveis]]
* [[Lista de exoplanetas potencialmente habitáveis]]
* [[Lista de nomes próprios de exoplanetas]]
* [[Lista de nomes próprios de exoplanetas]]

Revisão das 01h19min de 7 de novembro de 2022

Esta é uma Lista de exoplanetas descobertos em 2018.[1]

Para exoplanetas detectados apenas pela velocidade radial, o valor da massa é na verdade um limite inferior. (Consulte a massa mínima para obter mais informações)

Nome Massa (MJ) Raio (RJ) Período (dais) Semieixo maior (AU) Temp. (K)[2] Método de descoberta Distância (ly) Massa da estrela-mãe (M☉) Temperatura da estrela-mãe (K) Observações
24 Boötis b 0.91+0.13
−0.10 		30.3506+0.0078
−0.0077 		0.190+0.012
−0.009 		Vel. radial 313.9±2.1 0.99+0.19
−0.13 		4893±15 [3]
40 Eridani Ab 0.0266±0.0015 42.378±0.010 0.2190+0.0073
−0.0078 		Vel. radial 16.426±0.042 0.78±0.08 5072±53 [4]
Barnard's Star b 0.0102±0.0013 0.122+0
−0.122 		232.8+0.38
−0.41 		0.404±0.018 105±3 Vel. radial 6 0.144 3134 [5]
COROT-20c 17±1 1675+19
−17 		2.90±0.07 Vel. radial 2819±80 1.14±0.08 6050±200 Anã marrom (possivelmente)[6]
DE Canum Venaticorum b 12±3 4098.1±131.5 5.75±2.02 Tempo 99.64±0.09 0.51 [7]
Gamma Librae b 1.02±0.14 415.2+1.8
−1.9 		1.24±0.10 Vel. radial 154.7±2.9 1.47±0.20 4822±15 [3]
Gamma Librae c 4.58+0.45
−0.43 		964.6±3.1 2.17±0.10 Vel. radial 154.7±2.9 1.47±0.20 4822±15 [3]
Gliese 15 Ac 0.11 7600 5.4 Vel. radial 11.6 0.38 3567 [8]
Gliese 96 b 0.06186+0.00761
−0.00724 		73.94+0.33
−0.38 		0.291±0.005 Vel. radial 38.929±0.0302 0.60±0.07 3785±62 [9]
Gliese 143 b 0.09637+0.00827
−0.00840 		0.2280839±0.0282262 35.589+0.006
−0.005 		0.1932±0.0002 Trânsito 53.25±0.02 0.76+0.03
−0.02 		[10]
Gliese 1132 c 0.00831±0.00138 8.929±0.010 0.0476±0.0017 300±5 Vel. radial 41.153±0.023 0.181±0.019 3270±140 [11]
Gliese 1265 b 0.023±0.002 3.6511±0.0012 0.026±0.001 Vel. radial 33.45±0.02 0.18±0.02 3236±51 Estrela-mãe também conhecida como LP 819-052[12]
Gliese 3779 b 0.025±0.002 3.0232±0.0013 0.026±0.001 Vel. radial 44.84±0.04 0.27±0.02 3324±51 Estrela-mãe também conhecida como Ross 1020[12]
HAT-P-11c 1.60+0.09
−0.08 		3407+360
−190 		4.13+0.29
−0.16 		Vel. radial 123.31±0.11 0.809+0.020
−0.030 		4780±50 [13]
HATS-39b 0.63±0.13 1.57±0.12 4.5776348 0.06007±0.00058 1645±43 Trânsito 2910±240 1.379±0.040 6572±83 [14]
HATS-40b 1.59±0.24 1.58+0.16
−0.12 		3.2642736 0.04997±0.00074 2101±69 Trânsito 4550±110 1.561±0.069 6460±130 [14]
HATS-41b 9.7±1.6 1.33+0.29
−0.20 		4.193649 0.0583+0.0015
−0.0010 		1710+170
−120 		Trânsito 2457±47 1.496+0.115
−0.078 		6424±91 [14]
HATS-42b 1.88±0.15 1.40+0.25
−0.14 		2.2921020 0.03689±0.00065 1856+105
−75 		Trânsito 2672±35 1.273±0.067 6060±120 [14]
HATS-59b 0.806±0.069 1.126±0.077 5.416081±0.000016 0.06112±0.00076 1128±40 Trânsito 2140±50 1.04±0.04 5670±91 [15]
HATS-59c 12.70±0.87 1422±14 2.504±0.035 175.9±6.4 Vel. radial 2140±50 1.04±0.04 5670±91 [15]
HATS-60b 0.662±0.055 1.153±0.053 3.560829±0.000032 0.04708+0.00015
−0.00023 		1528±11 Trânsito 1609±28 1.097+0.010
−0.016 		5688±20 [16]
HATS-61b 3.40±0.14 1.195±0.067 7.817953±0.000024 0.07908±0.00033 1226.1±7.3 Trânsito 2262±29 1.08±0.01 5542±21 [16]
HATS-62b 0.179+0
−0.179 		1.055±0.025 3.2768837±0.0000033 0.04163+0.00024
−0.00016 		1237±12 Trânsito 1731±34 0.90+0.02
−0.01 		5416+19
−13 		[16]
HATS-63b 0.960±0.120 1.207±0.039 3.0566527±0.0000049 0.04026±0.00028 1398.3±9.0 Trânsito 2070±20 0.93±0.02 5627±18 [16]
HATS-64b 0.960±0.200 1.679±0.081 4.908897±0.000013 0.06562±0.00039 1793±27 Trânsito 3640±140 1.56±0.03 6554±27 [16]
HATS-65b 0.821±0.083 1.501±0.050 3.1051610±0.0000016 0.04497±0.00033 1634±18 Trânsito 1631±41 1.26±0.03 6277±30 [16]
HATS-66b 5.33±0.68 1.411±0.084 3.1414391±0.0000074 0.04714±0.00025 1998±21 Trânsito 5040±130 1.41±0.02 6625±35 [16]
HATS-67b 1.45±0.12 1.685±0.047 1.6091788±0.0000040 0.03032±0.00015 2193±22 Trânsito 3219±80 1.44±0.02 6594±33 [16]
HATS-68b 1.290±0.059 1.232+0.039
−0.029 		3.5862202±0.0000047 0.05071±0.00018 1741±12 Trânsito 2004±34 1.35±0.01 6147±22 [16]
HATS-69b 0.577+0
−0.577 		0.945±0.022 2.2252577±0.0000019 0.03211+0.00014
−0.00019 		1295.7±6.9 Trânsito 1368±11.7 0.89+0.01
−-0.02 		5137±16 [16]
HD 4917 b 1.615±0.092 1.224 400.5±1.7 1.167±0.065 Vel. radial 670.1±8.1 1.32 4802 Dois exoplanetas adicionais no sistema são suspeitos[17]
HD 13167 b 3.31±0.16 1.167 2613±17 4.10±0.34 Vel. radial 487.8±3.5 1.35 5671 [17][18]
HD 14787 b 1.121±0.069 1.250 676.6±8.1 1.70±0.19 Vel. radial 389.9±2.5 1.43 4946 [17]
HD 18015 b 3.18±0.23 1.170 2278±71 3.87±0.32 Vel. radial 405.2±2.6 1.49 5603 [17]
HD 23472 b 0.05638+0.00444
−0.04405 		0.179±0.009 17.667+0.142
−0.095 		0.121±0.001 543±18 Trânsito 127.48±0.06 0.67±0.03 4684±99 [10][19]
HD 23472 c 0.05405+0.00337
−0.04333 		0.167±0.010 29.625+0.224
−0.171 		0.170±0.001 467+19
−18 		transit 127.48±0.06 0.67±0.03 4684±99 [10][19]
HD 33142 c 5.97+1.04
−0.80 		834+29
−24 		Vel. radial 37.34±0.18 1.78±0.31 5009±15 Detecção de margem[17]
HD 55696 b 3.87±0.72 1827±10 3.18±0.18 Vel. radial 255±1 1.29±0.20 6012 [20]
HD 72490 b 1.768±0.080 1.218 858±12 1.88±0.21 Vel. radial 413.5±3.6 1.21 4934 [17]
HD 72490 c 4.5±1.2 3878±261 5.22±0.58 Vel. radial 224±20 1.26±0.25 4867 [17]
HD 89345 b 0.110 0.660 11.81430 0.1066 1089 Trânsito 433.1 1.16 5576 [21] Estrela-mãe também conhecida como K2-234[22]
HD 94834 b 1.26±0.17 1.242 1576±76 2.74±0.18 Vel. radial 321.0±2.1 1.11 4798 [17]
HD 98736 b 2.33±0.78 968.8±2.2 1.864±0.091 Vel. radial 106±0.2 0.92±0.13 5271 [20]
HD 114783 c 0.611+0.056
−0.053 		4319+151
−130 		Vel. radial 66.5±1.3 0.85±0.03 5135±44
HD 116029 c 1.27±0.15 907+30
−29 		Vel. radial 37.92±0.18 0.83±0.24 4819±54
HD 126525 b 0.237±0.002 960.41+6.19
−6.33 		1.837±0.010 Vel. radial 124.1+4.3
−4.6 		0.90±0.01 5638±13
HD 148164 b 1.23±0.25 328.55±0.41 0.9930±0.0660 Vel. radial 252±1.0 1.21±0.24 6032 [20]
HD 148164 c 5.16±0.82 5062±114 6.15±0.50 Vel. radial 252±1.0 1.21±0.24 6032 [20]
HD 148284 b 33.7±5.5 339.331±0.018 0.9740±0.0790 Vel. radial 400±2 1.07±0.26 5572
HD 158996 b 14.0±2.3 820.2±14.0 2.1±0.2 Vel. radial 933±15 1.8±0.3 4069±30
HD 180053 b 2.194±0.064 1.203 213.72±0.47 0.843±0.063 Vel. radial 448.7±2.0 1.75 5131 [17]
HD 202696 b 1.996+0.220
−0.100 		517.8+8.9
−3.9 		1.566+0.016
−0.007 		Vel. radial 618.3±5.2 1.91+0.09
−0.14 		5040+71
−85
HD 202696 c 1.864+0.177
−0.227 		946.6+20.7
−20.9 		2.342+0.034
−0.035 		Vel. radial 618.3±5.2 1.91+0.09
−0.14 		5040+71
−85
HD 203473 b 7.8±1.1 1552.9±3.4 2.73±0.17 Vel. radial 237±1.0 1.12±0.21 5780 [20]
HD 211810 b 0.670±0.440 1558±22 2.656±0.043 Vel. radial 211±0.4 1.03±0.02 5652 [20]
HD 215152 b 0.0057+0.0016
−0.0020 		5.7600+0.0016
−0.0018 		0.05764+0.00074
−0.00076 		Vel. radial 70.48±0.16 0.770±0.015 4935±76 [23]
HD 215152 e 0.0091+0.0033
−0.0047 		25.197+0.048
−0.051 		0.1542±0.0020 Vel. radial 70.48±0.16 0.770±0.015 4935±76 [23]
HD 217850 b 21.6±2.6 3501.3±2.1 4.56±0.24 Vel. radial 215±3 1.03±0.16 5544
HD 238914 b 6.0 4100 5.7 Vel. radial 982 1.47 4769
IC 4651 9122 b 6.3±0.5 734.0±8.1 2.038±0.039 Vel. radial 2870±110 2.1 9000
K2-80d 0.228+0.025
−0.012 		28.8673+0.0051
−0.0046 		0.1778+0.0051
−0.0055 		Trânsito 658.7±5.7 0.90±0.08 5441±249
K2-138b 0.140 2.35322 0.03380 Trânsito 597 0.93 5378 [24]
K2-138c 0.225 3.55987 0.04454 Trânsito 597 0.93 5378 [24]
K2-138d 0.237 5.40478 0.05883 Trânsito 597 0.93 5378 [24]
K2-138e 0.294 8.26144 0.07807 Trânsito 597 0.93 5378 [24]
K2-138f 0.251 12.75759 0.10430 Trânsito 597 0.93 5378 [24]
K2-141b 0.0160±0.0013 0.135±0.004 0.2803226 0.00716+0.00055
−0.00065 		2039+87
−48 		Trânsito 202.16±0.54 0.708±0.028 4599±79
K2-141c 0.023+0
−0.023 		0.624+0.410
−0.250 		7.74850 0.06739+0.00089
−0.00091 		Trânsito 202.16±0.54 0.708±0.028 4599±79
K2-155b 0.015+0.002
−0.001 		0.138+0.018
−0.015 		6.34365 0.0546+0.0013
−0.0014 		708+38
−31 		Trânsito 237.94±0.93 0.65+0.06
−0.03 		4258±150
K2-155c 0.020+0.005
−0.002 		0.174+0.024
−0.020 		13.85402 0.0946+0.0031
−0.0030 		583+52
−35 		Trânsito 237.94±0.93 0.65+0.06
−0.03 		4258±150
K2-155d 0.015+0.005
−0.002 		0.146+0.016
−0.015 		40.6835±0.0031 0.1937+0.0064
−0.0059 		381+47
−25 		Trânsito 237.94±0.93 0.65+0.06
−0.03 		4258±150
K2-156b 0.103+0.009
−0.006 		0.813149 0.0149±0.0001 1347+18
−19 		Trânsito 492.0±3.5 0.66+0.02
−0.01 		4597±50 [25][26]
K2-157b 0.094 0.365257 Trânsito 0.94 5456 [25][26]
K2-158b 0.236+0.014
−0.009 		10.0605+0.0013
−0.0015 		0.0887±0.0008 794±11 Trânsito 647.1±6.7 0.92+0.03
−0.02 		5503+51
−48 		[25]
K2-158c 0.114+0.012
−0.009 		5.9028+0.0019
−0.0023 		0.0622±0.0006 948±13 Trânsito 647.1±6.7 0.92+0.03
−0.02 		5503+51
−48 		[27]
K2-159b 0.202+0.015
−0.010 		12.4221±0.0018 0.1013+0.0008
−0.0009 		684±8 Trânsito 560.4±4.6 0.90+0.02
−0.03 		5425±44 [25]
K2-160b 0.284+0.019
−0.013 		3.705871 0.04660+0.00037
−0.00041 		Trânsito 1038±15 0.983+0.023
−0.025 		5649±50 [25]
K2-161b 0.546+0.146
−0.070 		9.283188 0.0861+0.0018
−0.0023 		Trânsito 3070±160 0.987+0.082
−0.060 		4972±50 [25]
K2-162b 0.128+0.010
−0.006 		9.4589+0.0010
−0.0011 		0.0795±0.0006 631±8 Trânsito 407.3±2.0 0.75±0.02 4842+49
−45 		[25]
K2-163b 0.220+0.023
−0.011 		6.673117 0.06509+0.00050
−0.00060 		Trânsito 684±14 0.826+0.019
−0.023 		4937±50 [25]
K2-164b 0.290+0.046
−0.037 		17.3551+0.0041
−0.0038 		0.1387+0.0036
−0.0025 		Trânsito 1238±25 1.181+0.093
−0.061 		5791±50 [25]
K2-165b 0.1137+0.0129
−0.0087 		2.35499 0.03262±0.00040 Trânsito 440.6±3.9 0.835+0.031
−0.030 		5185±50 [25]
K2-165c 0.1386+0.0187
−0.0098 		4.38275 0.04935±0.00061 Trânsito 440.6±3.9 0.835+0.031
−0.030 		5185±50 [25]
K2-165d 0.236+0.023
−0.013 		14.1014±0.0011 0.1076±0.0013 Trânsito 440.6±3.9 0.835+0.031
−0.030 		5185±50 [25]
K2-166b 0.195+0.018
−0.017 		8.5272±0.0020 0.08583+0.00123
−0.00076 		Trânsito 1577±32 1.16+0.05
−0.03 		5960+52
−53 		[25]
K2-167b 0.252+0.046
−0.040 		9.9775±0.0010 0.0912+0.0036
−0.0029 		Trânsito 264.5±1.5 1.02+0.12
−0.09 		5908±50 [25]
K2-168b 0.191+0.018
−0.012 		15.8540±0.0014 0.1195+0.0013
−0.0014 		Trânsito 801±14 0.907+0.029
−0.032 		5554±50 [25]
K2-169b 0.1136+0.0096
−0.0069 		6.38080 0.06764+0.00063
−0.00061 		Trânsito 774±15 0.986+0.028
−0.026 		5548±50 [25]
K2-170b 0.127+0.018
−0.012 		7.5765+0.0018
−0.0017 		0.07457+0.00083
−0.00086 		Trânsito 1296±21 0.964±0.032 5748±50 [25]
K2-170c 0.161+0.022
−0.014 		12.4000+0.0017
−0.0019 		0.1036+0.0011
−0.0012 		Trânsito 1296±21 0.964±0.032 5748±50 [25]
K2-171b 0.240+0.036
−0.030 		5.6285+0.0017
−0.0015 		0.05960+0.00132
−0.00062 		Trânsito 2010±61 0.892+0.060
−0.027 		5250±50 [25]
K2-172b 0.1486+0.014
−0.0085 		14.3169±0.0014 0.1128+0.0010
−0.0011 		Trânsito 820.3±9.6 0.934+0.026
−0.027 		5569±50 [25]
K2-172c 0.286+0.017
−0.012 		29.6268±0.0016 0.1832+0.0017
−0.0018 		Trânsito 820.3±9.6 0.934+0.026
−0.027 		5569±50 [25]
K2-173b 0.1435+0.0143
−0.0094 		5.86870 0.06105+0.00078
−0.00085} 		Trânsito 750.6±6.4 0.881+0.034
−0.036 		5580±70 [25]
K2-174b 0.2223+0.0157
−0.0087 		19.56274 0.1242±0.0013 Trânsito 326.9±1.2 0.668+0.022
−0.021 		4500±50 [25]
K2-175b 0.182+0.032
−0.024 		9.5260+0.0012
−0.0013 		0.0906+0.0016
−0.0011 		Trânsito 812.2±9.1 1.095+0.057
−0.039 		5909±50 [25]
K2-176b 0.1330+0.0110
−0.0083 		5.32944 0.05846+0.00042
−0.00052 		Trânsito 812±12 0.939+0.020
−0.025 		5428±50 [25]
K2-177b 0.189+0.025
−0.014 		14.1552+0.0032
−0.0030 		0.1221+0.0011
−0.0013 		Trânsito 1628±42 1.211+0.032
−0.038 		6063±50 [25]
K2-178b 0.317+0.018
−0.012 		8.74782 0.08171+0.00066
−0.00081 		Trânsito 704.7±6.0 0.951+0.023
−0.027 		5525±50 [25]
K2-179b 0.224+0.015
−0.011 		5.17219 0.05488+0.00048
−0.00060 		Trânsito 625.7±6.9 0.824+0.022
−0.027 		5015±50 [25]
K2-180b 0.2150+0.0184
−0.0098 		8.86593 0.07550+0.00070
−0.00075 		Trânsito 668.9±5.7 0.730+0.020
−0.022 		5263±50 [25]
K2-181b 0.241+0.028
−0.016 		6.89425 0.07191+0.00055
−0.00067 		Trânsito 1189±17 1.044+0.024
−0.029 		5609±50 [25]
K2-182b 0.063±0.016 0.2469+0.0152
−0.0089 		4.736884 0.05223+0.00048
−0.00064 		Trânsito 507.2±4.1 0.847+0.024
−0.031 		5159±50 [25][18] Confirmado em 2021[28]
K2-183b 0.098±0.090 0.469269 0.011586+0.00010
−0.000087 		Trânsito 1083±14 0.942+0.021
−0.025 		5482±50 [25][18][26]
K2-183c 0.224+0.024
−0.012 		10.79347 0.09371+0.00070
−0.00083 		Trânsito 1083±14 0.942+0.021
−0.025 		5482±50 [25][18][26]
K2-183d 0.227+0.025
−0.013 		22.6295+0.0018
−0.0019 		0.1535+0.0014
−0.0012 		Trânsito 1083±14 0.942+0.021
−0.025 		5482±50 [26]
K2-184b 0.1372+0.0134
−0.0080 		16.99344 0.1210+0.0014
−0.0015 		Trânsito 247.1±1.1 0.819+0.028
−0.030 		5252±50 [25][18]
K2-185b 0.117+0.020
−0.010 		10.6166+0.0016
−0.0018 		0.09378+0.00088
−0.00093 		Trânsito 882±11 0.976+0.027
−0.028 		5722±50 [25]
K2-186b 0.283+0.024
−0.015 		41.4742+0.0033
−0.0043 		0.2359+0.0018
−0.0021 		Trânsito 1089±18 1.019+0.023
−0.027 		5784±50 [25]
K2-187b 0.123 0.773981 Trânsito 0.97 5477 [25][18]
K2-187c 0.152+0.022
−0.010 		2.87179 0.03910+0.00034
−0.00033 		Trânsito 1089±19 0.967+0.025
−0.024 		5477±50 [25][18]
K2-187d 0.287+0.045
−0.022 		7.14908 0.07182+0.00062
−0.00061 		Trânsito 1089±19 0.967+0.025
−0.024 		5477±50 [25][18]
K2-187e 0.201+0.019
−0.012 		13.6083+0.0017
−0.0016 		0.11031+0.00096
−0.00094 		Trânsito 1089±19 0.967+0.025
−0.024 		5477±50 [25][18]
K2-188b 0.112+0.015
−0.010 		1.74298 0.02932+0.000276
−0.000225 		Trânsito 1476±28 1.107+0.031
−0.025 		5982±50 [25][18]
K2-188c 0.234+0.028
−0.016 		7.80760 0.07967+0.00075
−0.00061 		Trânsito 1476±28 1.107+0.031
−0.025 		5982±50 [25][18]
K2-189b 0.1349+0.0136
−0.0085 		5.17630 0.05711+0.00049
−0.00057 		Trânsito 795.2±6.3 0.928+0.024
−0.027 		5503±50 [25][18]
K2-189c 0.222+0.028
−0.012 		6.67934 0.06769+0.00058
−0.00068 		Trânsito 795.2±6.3 0.928+0.024
−0.027 		5503±50 [25][18]
K2-190b 0.1210+0.0157
−0.0091 		10.09886 0.0884+0.0011
−0.0012 		Trânsito 526.5±3.7 0.905+0.033
−0.036 		5631±50 [25]
K2-190c 0.0975+0.0135
−0.0082 		21.5740+0.0057
−0.0043 		0.1467+0.0018
−0.0020 		Trânsito 526.5±3.7 0.905+0.033
−0.036 		5631±50 [25]
K2-191b {{0.141+0.024
−0.012 		2.85865 0.03807+0.00036
−0.00040 		Trânsito 944.5±7.8 0.901+0.026
−0.028 		5176±50 [25]
K2-192b 0.1405+0.0135
−0.0099 		4.16322 0.04840+0.00045
−0.00058 		Trânsito 727.9±5.9 0.873+0.024
−0.031 		5252±50 [25][18]
K2-193b 0.358+0.031
−0.018 		14.78721 0.1177±0.0011 Trânsito 1360±12 0.994+0.029
−0.027 		5623±50 [25] Baixa fidelidade[18]
K2-194b 0.325+0.055
−0.045 		39.7214+0.0057
−0.0056 		0.2359+0.0032
−0.0025 		Trânsito 2090±61 1.110+0.046
−0.035 		5979±52 [25]
K2-195b 0.262+0.018
−0.012 		15.85354 0.1220+0.0012
−0.0014 		Trânsito 1037±14 0.963+0.028
−0.031 		5712±50 [25][18]
K2-195c 0.230+0.024
−0.013 		28.4828+0.0064
−0.0073 		0.1803+0.0018
−0.0020 		Trânsito 1037±14 0.963+0.028
−0.031 		5712±50 [25]
K2-196b 0.321+0.054
−0.045 		48.3242+0.0085
−0.0087 		0.2730+0.0058
−0.0036 		Trânsito 1938±73 1.162+0.075
−0.045 		6045±50 [25]
K2-197b 0.223+0.017
−0.010 		8.35795 0.07992+0.00068
−0.00080 		Trânsito 813.4±7.8 0.975+0.025
−0.029 		5675±50 [25] Baixa fidelidade[18]
K2-198b 0.367+0.023
−0.015 		17.04318 0.1221±0.0014 Trânsito 361.7±2.8 0.836±0.029 5262±50 [25]
K2-199b 0.022±0.006 0.1679+0.0167
−0.0079 		3.225423 0.03804+0.00043
−0.00042 		Trânsito 351.8±2.0 0.706+0.024
−0.023 		4681±50 [25][18][28]
K2-199c 0.039±0.007 0.253+0.015
−0.010 		7.37450 0.06601+0.00075
−0.00074 		Trânsito 351.8±2.0 0.706+0.024
−0.023 		4681±50 [25][18][28]
K2-200b 0.1217+0.0128
−0.0094 		2.84988 0.03741+0.00033
−0.00040 		Trânsito 603.7±6.1 0.860+0.023
−0.027 		5233±50 [25]
K2-201b 0.1249+0.0120
−0.0069 		1.059790 0.02004+0.00014
−0.00015 		Trânsito 649.2±5.4 0.956+0.020
−0.021 		5507±50 [25]
K2-201c 0.293+0.036
−0.016 		22.7799+0.0020
−0.0019 		0.1549+0.0011
−0.0012 		Trânsito 649.2±5.4 0.956+0.020
−0.021 		5507±50 [25]
K2-202b 0.205+0.016
−0.011 		3.40516 0.04387+0.00044
−0.00042 		Trânsito 988.2±8.7 0.971+0.030
−0.028 		5491±58 [25]
K2-203b 0.122+0.025
−0.011 		9.6951±0.0013 0.08238+0.00112
−0.00098 		Trânsito 544.5±5.1 0.794+0.033
−0.028 		5000±50 [25]
K2-204b 0.272+0.039
−0.033 		7.05578 0.07222+0.00074
−0.00066 		Trânsito 1914±58 1.009+0.031
−0.027 		5755±50 [25]
K2-205b 0.178+0.024
−0.021 		26.6723+0.0042
−0.0037 		0.1718+0.0023
−0.0022 		Trânsito 1337±30 0.951+0.038
−0.036 		5890±50 [25]
K2-206b 0.249+0.020
−0.014 		18.2945+0.0017
−0.0016 		0.1256+0.0016
−0.0015 		Trânsito 803±10 0.789+0.030
−0.028 		5043±50 [25]
K2-207b 0.232+0.033
−0.019 		12.4875±0.0012 0.1033±0.0010 Trânsito 1196±18 0.942±0.028 5522±50 [25]
K2-208b 0.150+0.015
−0.011 		4.19095 0.04957+0.00053
−0.00054 		Trânsito 844±10 0.925±0.030 5582±50 [25]
K2-209b 0.0775+0.0094
−0.0056 		2.08062 0.02891+0.00033
−0.00032 		Trânsito 250.05±0.99 0.745+0.026
−0.024 		4720±50 [25]
K2-210b 0.0730+0.0090
−0.0062 		0.570233 0.01305+0.00011
−0.00014 		Trânsito 578.6±6.0 0.912+0.023
−0.029 		5396±50 [25]
K2-211b 0.1226+0.0154
−0.0091 		0.669558 0.01436+0.00011
−0.00015 		Trânsito 895±14 0.882+0.019
−0.027 		5221±50 [25] Outro planeta descoberto em 2020[26]
K2-212b 0.2135+0.0127
−0.0082 		9.79540 0.07648+0.00082
−0.00075 		Trânsito 357.3±3.0 0.622+0.020
−0.018 		4349±50 [25][18]
K2-213b 0.135+0.027
−0.019 		8.1309±0.0018 0.08093+0.00138
−0.00099 		Trânsito 1285±23 1.070+0.055
−0.038 		5794±50 [25]
K2-214b 0.198+0.034
−0.023 		8.59653 0.08273+0.00083
−0.00076 		Trânsito 989±14 1.022+0.031
−0.028 		5768±50 [25][18]
K2-215b 0.189+0.023
−0.014 		8.26965 0.08003+0.00070
−0.00073 		Trânsito 1333±21 1.000+0.026
−0.027 		5704±50 [25]
K2-216b 0.1497+0.0090
−0.0068 		2.174789 0.02916+0.00031
−0.00032 		Trânsito 377.8±2.3 0.699±0.023 4591±50 [25][18]
K2-217b 0.319+0.062
−0.043 		14.07452 0.1179+0.0016
−0.0013 		Trânsito 1259±25 1.103+0.046
−0.037 		5967±50 [25]
K2-218b 0.229+0.025
−0.014 		8.67989 0.08395+0.00082
−0.00075 		Trânsito 1299±32 1.048+0.031
−0.028 		5757±50 [25]
K2-219b 0.120+0.018
−0.016 		3.90129}} 0.04885+0.00054
−0.00048 		Trânsito 1071±16 1.022+0.034
−0.030 		5753±50 [25]
K2-219c 0.128+0.019
−0.017 		6.6677+0.0013
−0.0016 		0.06982+0.00077
−0.00070 		Trânsito 1071±16 1.022+0.034
−0.030 		5753±50 [25]
K2-219d 0.230+0.032
−0.029 		11.13728 0.09830+0.00108
−0.00097 		Trânsito 1071±16 1.022+0.034
−0.030 		5753±50 [25]
K2-220b 0.198+0.023
−0.013 		13.68251 0.11043+0.00099
−0.00112 		Trânsito 766.7±8.9 0.960+0.026
−0.029 		5599±50 [25]
K2-221b 0.1498+0.0149
−0.0085 		2.39909 0.03520+0.00028
−0.00029 		Trânsito 1049±22 1.011+0.024
−0.025 		5716±50 [25]
K2-222b 0.0252±0.0057 0.210±0.007 15.38883 0.1190+0.0016
−0.0015 		Trânsito 331.4±2.0 0.950+0.040
−0.036 		5934±50 [25][18][29]
K2-223b 0.0812+0.0088
−0.0066 		0.505570 0.012664+0.000080
−0.000081 		Trânsito 651.3±8.3 1.06±0.02 5835+38
−40 		[25]
K2-223c 0.144+0.010
−0.006 		4.56417 0.05491±0.00035 Trânsito 651.3±8.3 1.06±0.02 5835+38
−40 		[25]
K2-224b 0.139+0.014
−0.012 		4.47859 0.05422+0.00034
−0.00035 		1002±11 Trânsito 904.8±9.6 0.91±0.02 5620+42
−45 		[25]
K2-224c 0.215+0.014
−0.011 		10.0949+0.0012
−0.0011 		0.08858+0.00065
−0.00066 		764±9 Trânsito 904.8±9.6 0.91±0.02 5620+42
−45 		[25]
K2-225b 0.311+0.023
−0.018 		15.8715+0.0017
−0.0021 		0.13385+0.00140
−0.00072 		902±13 Trânsito 1179±19 1.27+0.02
−0.04 		5742+49
−47 		[25]
K2-226b 0.137+0.012
−0.008 		3.27111 0.04133+0.00047
−0.00048 		1120±16 Trânsito 693±11 0.88±0.03 5424+48
−46 		[25]
K2-227b 0.149+0.109
−0.016 		13.6218+0.0032
−0.0033 		0.1098+0.0011
−0.0012 		Trânsito 613.9±6.7 0.951+0.028
−0.030 		5673±50 [25]
K2-228b 0.108+0.009
−0.005 		2.69837 0.0338±0.0003 914+14
−13 		Trânsito 423±13 0.71±0.02 4715+48
−46 		[25]
K2-229b 0.0082±0.0014 0.102+0.005
−0.003 		0.584249 0.012888±0.00013 1818+14
−15 		Trânsito 335.5±3.5 0.87±0.01 5315+25
−31 		[25]
K2-229c 0.067+0
−0.067 		0.181+0.011
−0.005 		8.32801 0.0769±0.0003 750±6 Trânsito 335.5±3.5 0.87±0.01 5315+25
−31 		[25][27]
K2-230b 0.175+0.016
−0.014 		2.86064 0.0409+0.0003
−0.0002 		1529±22 Trânsito 1791±47 1.11±0.02 5945+23
−25 		[25]
K2-231b 0.22±0.02 13.8419±0.0014 0.1132±0.0011 Trânsito 1057±14 1.01±0.03 5695±50
K2-232b 0.398±0.037 1.000+0.022
−0.020 		11.168459 0.10356+0.00081
−0.00077 		1001±14 Trânsito 427.9±2.5 1.188+0.028
−0.026 		6154±60
K2-233b 0.1247+.0055
−0.0054 		2.46746 0.03317+0.00044
−0.00045 		1040+28
−26 		Trânsito 220.60±0.91 0.800±0.032 4950±100
K2-233c 0.1191+0.0074
−0.0069 		7.06142 0.06687 728+20
−19 		Trânsito 220.60±0.91 0.800±0.032 4950±100
K2-233d 0.236±0.010 24.3662±0.0021 0.1527+0.0020
−0.0021 		482+14
−13 		Trânsito 220.60±0.91 0.800±0.032 4950±100
K2-236b 0.085+0.044
−0.040 		0.546±0.009 19.49213 0.148±0.004 886±17 Trânsito 595.7±4.2 1.18+0.03
−0.04 		6025±100 Primeiro exoplaneta descoberto por cientistas baseados na Índia.
K2-237b 1.60±0.11 1.65+0.07
−0.08 		2.18056 0.037±0.002 1884+37
−36 		Trânsito 1036±23 1.28+0.03
−0.04 		6257±100 Também conhecido como EPIC 229426032 b
K2-238b 0.86+0.13
−0.12 		1.30+0.15
−0.14 		3.20466 0.046± 1587+75
−76 		Trânsito 22000+13000
−50000 		1.19±0.08 5630±78 Também conhecido como EPIC 246067459 b
K2-239b 0.0044±0.0013 0.098±0.009 5.240±0.001 0.0441±0.0008 502+22
−18 		Trânsito 101.48±0.27 0.40±0.01 3420±18
K2-239c 0.0028±0.0009 0.089±0.009 7.775±0.001 0.0576±0.0009 427+24
−19 		Trânsito 101.48±0.27 0.40±0.01 3420±18
K2-239d 0.0041±0.0013 0.098±0.009 10.115±0.001 0.0685±0.0012 399+18
−15 		Trânsito 101.48±0.27 0.40±0.01 3420±18
K2-240b 0.016+0.002
−0.001 		0.18+0.02
−0.01 		6.034±0.001 0.0513±0.0009 586+24
−18 		Trânsito 238.3±1.7 0.58±0.01 3810±17
K2-240c 0.014+0.002
−0.001 		0.16+0.03
−0.01 		20.523±0.001 0.1159±0.0020 389+19
−17 		Trânsito 238.3±1.7 0.58±0.01 3810±17
K2-241b 0.227+0.016
−0.009 		26.8199±0.0025 0.1567+0.0007
−0.0008 		507±5 Trânsito 489.6±3.5 0.71±0.01 5262+43
−39
K2-242b 0.227+0.019
−0.017 		6.51389 0.0494±0.0004 416±8 Trânsito 357.4±2.0 0.38±0.01 3459+65
−38
K2-243b 0.194+0.012
−0.011 		11.5418+0.0027
−0.0022 		0.1087±0.0014 1035+36
−35 		Trânsito 877±11 1.29+0.04
−0.06 		6570+269
−171
K2-243c 0.179+0.013
−0.012 		24.9460+0.0049
−0.0056 		0.1817+0.0022
−0.0024 		801+27
−28 		Trânsito 877±11 1.29+0.04
−0.06 		6570+269
−171
K2-244b 0.156+0.012
−0.009 		21.0688+0.0032
−0.0033 		0.1418+0.0010
−0.0011 		638±7 Trânsito 698.6±7.8 0.86±0.02 5677+38
−39
K2-245b 0.387+0.017
−0.012 		11.89307 0.0959±0.0006 923±14 Trânsito 1507±28 0.83+0.02
−0.01 		5793+66
−52
K2-246b 0.311+0.022
−0.019 		5.76918 0.0602±0.0004 977+19
−18 		Trânsito 2341±89 0.87±0.02 5610+32
−29
K2-247b 0.189+0.017
−0.014 		2.25021 0.0304±0.0004 979+52
−51 		Trânsito 848.1±6.7 0.74±0.03 4667+305
−183
K2-247c 0.195+0.022
−0.021 		6.4942+0.0026
−0.0025 		0.0615±0.0008 688+36
−35 		Trânsito 848.1±6.7 0.74±0.03 4667+305
−183
K2-248b 0.229+0.018
−0.012 		7.1726+0.0015
−0.0014 		0.0699±0.0010 886+19
−18 		Trânsito 1341±16 0.88+0.04
−0.03 		5528+97
−86
K2-249b 0.249+0.024
−0.020 		12.4090+0.0034
−0.0028 		0.1151+0.0030
−0.0031 		1061±66 Trânsito 1726±55 1.32+0.09
−0.12 		6504+329
−419
K2-250b 0.218+0.017
−0.013 		4.01457 0.0459±0.0005 958+14
−13 		Trânsito 1369±21 0.80+0.03
−0.02 		5172+46
−44
K2-251b 0.210+0.023
−0.019 		9.3008+0.0033
−0.0032 		0.0694±0.0005 437±9 Trânsito 481.6±3.4 0.52±0.01 3717+85
−50
K2-252b 0.155+0.015
−0.011 		13.8151+0.0046
−0.0045 		0.1041+0.0008
−0.0007 		639±7 Trânsito 751.3±6.8 0.79+0.02
−0.01 		5152+41
−39
K2-253b 1.130+0.062
−0.054 		4.00167 0.0506+0.0010
−0.0011 		1238+57
−53 		Trânsito 2933±95 1.08+0.05
−0.08 		6027+221
−240
K2-254b 0.145+0.025
−0.021 		4.09639 0.0448±0.0005 791±26 Trânsito 747.8±4.2 0.71+0.02
−0.03 		4629+168
−123
K2-254c 0.195+0.021
−0.016 		12.1184+0.0030
−0.0032 		0.0923±0.0010 551±18 Trânsito 747.8±4.2 0.71+0.02
−0.03 		4629+168
−123
K2-255b 0.259+0.025
−0.010 		1.96417 0.0274±0.0003 1034±17 Trânsito 628.4±5.0 0.71±0.03 4676+63
−61
K2-256b 0.235+0.022
−0.019 		5.5201+0.0024
−0.0028 		0.0578±0.0008 845±28 Trânsito 1871±49 0.84+0.03
−0.04 		5219+179
−136
K2-257b 0.074+0.005
−0.004 		1.60588 0.0216±0.0002 789±14 Trânsito 209.14±0.84 0.52±0.01 3725+80
−46
K2-258b 0.268+0.019
−0.018 		19.0921+0.0058
−0.0063 		0.1490+0.0025
−0.0026 		{831±30 Trânsito 2201±37 1.21+0.05
−0.08 		6351+198
−228
K2-259b 0.207+0.018
−0.015 		15.4804+0.0033
−0.0039 		0.1271+0.0010
−0.0011 		795±13 Trânsito 1374±27 1.14±0.03 6059+62
−76
K2-260b 1.42+0.31
−0.32 		1.552+0.048
−0.057 		2.6266657 0.0404+0.0013
−0.0016 		1957+78
−77 		Trânsito 2206±63 1.39+0.05
−0.06 		6367±250
K2-261b 0.223±0.031 0.850+0.026
−0.022 		11.63344 0.102+0.019
−0.020 		1080+110
−100 		Trânsito 699.9±6.4 1.10+0.01
−0.02 		5537±71
K2-263b 0.0466±0.0098 0.215±0.011 50.818947±0.000094 0.2573±0.0029 470±10 Trânsito 532±4 0.88±0.03 5368±44
K2-264b 0.203+0.018
−0.014 		5.839770+0.000061
−0.000063 		489+12
−13 		Trânsito 609±7 0.47±0.01 3580±70
K2-264c 0.247+0.018
−0.016 		19.663650+0.000303
−0.000306 		326+8
−9 		Trânsito 609±7 0.47±0.01 3580±70
K2-265b 0.0206±0.0026 0.153±0.010 2.369172±0.000089 0.03376±0.00021 Trânsito 454±3 0.912±0.02 5477±27
K2-266b 0.0356+0.0346
−0.0205 		0.29+0.16
−0.12 		0.658524±0.000017 0.01306+0.00020
−0.00021 		1515±18 Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57
K2-266c 0.00091+0.00053
−0.00035 		0.0629+0.0086
−0.0076 		7.8140+0.0019
−0.0016 		0.0679±0.0011 664.5+8.0
−7.7 		Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57
K2-266d 0.0296+0.0091
−0.0063 		0.261+0.012
−0.011 		14.69700+0.00034
−0.00035 		0.1035+0.0016
−0.0017 		538.3+6.5
−6.3 		Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57
K2-266e 0.0261+0.0085
−0.0057 		0.244+0.012
−0.010 		19.4820±0.0012 0.1249+0.0019
−0.0020 		490.1+5.9
−5.7 		Trânsito 251.7+1.95
−1.92 		0.686±0.033 4285+49
−57
K2-267b 3.0+1.1
−1.2 		1.051±0.044 6.180235±0.000014 0.07229+0.00074
−0.00075 		1401±16 Trânsito 1098+27
−26 		1.317+0.041
−0.040 		6202+52
−50
K2-268b 0.126±0.012 2.151894+0.000393
−0.000363 		0.0308±0.0002 1121±14 Trânsito 1081.1±10.27 0.84±0.02 5068±51 [18]
K2-268c 0.240±0.021 9.326841+0.001532
−0.001617 		0.0819±0.0006 688±8 Trânsito 1081.1±10.27 0.84±0.02 5068±51 [18]
K2-269b 0.140±0.011 4.144965+0.000817
−0.000619 		0.0531±0.0006 1429±37 Trânsito 1180.1±47.0 1.16±0.04 6209±88 [18]
K2-270b 0.123±0.010 1.543069+0.000189
−0.000185 		0.0247±0.0002 1203±17 Trânsito 924.75±7.60 0.85±0.02 4877±58 [18]
K2-270c 0.263±0.014 4.400028+0.000169
−0.000178 		0.0497±0.0004 848±12 Trânsito 924.75±7.60 0.85±0.02 4877±58 [18]
K2-271b 0.649±0.021 8.562421±0.000127 0.0770+0.0008
−0.0009 		893±17 Trânsito 1863.9±44.32 0.83±0.03 5644±71 [18]
K2-272b 0.260±0.013 14.453533+0.001328
−0.001360 		0.1081+0.0016
−0.0017 		655±12 Trânsito 1391.3±17.3 0.81±0.04 5419±79 [18]
K2-273b 0.394±0.114 11.716332+0.001172
−0.001198 		0.0974±0.0011 672±11 Trânsito 1013.0±9.39 0.90±0.03 5200±67 [18]
K2-274b 0.196±0.011 14.129714+0.0021022
−0.001876 		0.1064+0.0009
−0.0008 		589±9 Trânsito 1013.0±9.39 0.81±0.02 5065±60 [18]
K2-275b 0.200±0.011 3.280961+0.000112
−0.000107 		0.0400±0.0003 905±13 Trânsito 404.73±2.28 0.79±0.02 4812±59 [18]
K2-275c 0.209±0.009 8.438756+0.000269
−0.000271 		0.0750±0.0005 660±9 Trânsito 404.73±2.28 0.79±0.02 4812±59 [18]
K2-276b 0.336±0.019 18.718269+0.003153
−0.003008 		0.1291±0.0011 583+10
−9 		Trânsito 1597.8±23.9 0.82±0.02 5139±62 [18]
K2-277b 0.185±0.011 6.326763+0.000355
−0.000361 		0.0675±0.0006 958±14 Trânsito 370.29±2.28 1.02±0.03 5741±65 [18]
K2-278b 0.266±0.021 3.334966+0.000701
−0.000859 		0.0488±0.0009 1711±101 Trânsito 2622.7±53.7 1.40±0.08 6747±383 [18]
K2-279b 0.108±0.012 7.122605+0.001647
−0.001601 		0.0670+0.0008
−0.0009 		879±14 Trânsito 599.48±5.15 0.79±0.03 5558±70 [18]
K2-280b 0.684±0.023 19.895202+0.000774
−0.000753 		0.1488+0.0019
−0.0020 		744±15 Trânsito 1294.5±2.38 1.11±0.04 5742±90 [18][30][31][25]
K2-281b 0.730±0.019 8.687721+0.000151
−0.000150 		0.0773±0.0008 665±12 Trânsito 1520.2±23.6 0.82±0.03 4812±72 [18]
K2-282b 0.252±0.012 4.169836+0.000279
−0.000300 		0.0499+0.0006
−0.0007 		1057±20 Trânsito 1638.2±25.3 0.95±0.04 5523±82 [18]Mais dois exoplanetas descobertos em 2019 e 2020[26]
K2-283b 0.314±0.014 1.921036+0.000051
−0.000053 		0.0291±0.0003 1186±20 Trânsito 1331.5±15.7 0.89±0.03 5060±70 [18]
K2-284b 0.248+0.012
−0.011 		4.795069±0.000086 0.04771±0.00025 653+16
−14 		Trânsito 351.0±1.6 0.63±0.01 4140±50
K2-285b 0.03046+0.00381
−0.00431 		0.231±0.005 3.471745+0.000044
−0.000046 		0.03817+0.00095
−0.00092 		1088.9+22.1
−21.9 		Trânsito 508±4 0.83±0.02 4975±95
K2-285c 0.04933+0.00717
−0.00670 		0.315±0.007 7.138048+0.000072
−0.000063 		0.0824±0.0018 741.4±14.5 Trânsito 508±4 0.83±0.02 4975±95
K2-285d 0.020±0.020 0.221±0.005 10.45582+0.00025
−0.00023 		0.1178±0.0029 619.9+12.7
−12.5 		Trânsito 508±4 0.83±0.02 4975±95
K2-285e 0.0337+0
−0.0337 		0.174±0.004 14.76289+0.00065
−0.00061 		0.18041+0.00420
−0.00430 		500.9+10.1
−9.9 		Trânsito 508±4 0.83±0.02 4975±95
K2-286b 0.0214±0.0135 0.1873±0.0178 27.359±0.005 0.1768+0.0175
−0.0205 		347+21
−11 		Trânsito 248.9±0.8 0.64±0.02 3926±100
K2-287b 0.315±0.027 0.847±0.013 14.893291±0.000025 0.1206±0.0008 804+8
−7 		Trânsito 518.7±4.2 1.06±0.02 5695±58
K2-288Bb 0.17±0.03 31.393463+0.000067
−0.000069 		0.164±0.030 226.36±22.30 Trânsito 214.3±2.8 0.33±0.02 3341±276
KELT-21b 3.91+0
−3.91 		1.586+0.039
−0.040 		3.6127647 0.05224+0.00035
−0.00034 		2051+29
−30 		Trânsito 1557±21 1.458+0.029
−0.028 		7598+81
−84
Kepler-411d 0.0478±0.0160 0.2961±0.0093 58.02035±0.00056 0.279±0.004 410±10 Trânsito 500.94±1.57 0.87±0.04
Kepler-730c 0.140±0.012 2.851883380 0.03997+0.00089
−0.00069 		1607+27
−29 		Trânsito 6590+254
−267 		1.05+0.07
−0.05 		5620+55
−59
Kepler-1654b 0.819+0.019
−0.017 		1047.8356+0.0018
−0.0019 		2.026+0.037
−0.035 		206.0+3.7
−3.5 		Trânsito 1884±13 1.011+0.056
−0.052 		5597+95
−93
Kepler-1655b 0.016+0.010
−0.009 		0.1974±0.0073 11.87290396 0.103±0.001 Trânsito 699.9±3.2 1.03±0.04 6148±71 Semelhante a um mini-Netuno[32]
Kepler-1656b 0.153+0.013
−0.012 		0.448±0.047 31.578659 0.197±0.021 651+51
−47 		Trânsito 610±3 1.03±0.04 5731±60
Kepler-1657b 1.93+0.19
−0.21 		0.990+0.060
−0.070 		141.241671±0.000086 0.534+0.012
−0.030 		347±12 Trânsito 3090±80 1.01+0.07
−0.16 		5830±100 Também conhecido como KOI-3680 b em Exoplanet Archive
KMT-2016-BLG-1397Lb 7.00+5.20
−4.30 		5.1+1.5
−1.7 		Microlente 22000+3600
−4200 		0.45+0.33
−0.28
KMT-2016-BLG-1820Lb 4.57+5.03
−2.14 		1.08+0.22
−0.24 		Microlente 20420+3720
−4170 		0.039+0.043
−0.018
KMT-2016-BLG-2142Lb 15.49+24.99
−8.58 		0.830+0.150
−0.200 		Microlente 7010+1010
−1160 		0.0730+0.1170
−0.0400
KPS-1b 1.090+0.086
−0.087 		1.03+0.13
−0.12 		1.706291 0.0269±0.0010 1459±56 Trânsito 863.3±8.5 0.892+0.090
−0.100 		5165±90 Primeiro exoplaneta em trânsito encontrado por um astrônomo amador
LHS 1140 c 0.00569±0.00123 0.1144±0.0021 3.777931±0.000003 0.02675±0.00070 438±9 Trânsito 40.67±1.37 0.18±0.01 3216±39
MOA-2010-BLG-117Lb 0.54±0.10 2369+835
−2717 		2.9+1.6
−0.6 		Microlente 11400±1300 0.58±0.11 4000+450
−350
MOA-2011-BLG-291Lb 0.057+0.107
−0.038 		0.69±0.24 Microlente 14000±4600 0.15+0.27
−0.10
MOA-2015-BLG-337Lb 0.1060+0.4059
−0.0730 		0.24+0.06
−0.09 		Microlente 23000+3600
−3300 		0.00940+0.03590
−0.00650
MOA-2016-BLG-319Lb 0.620+1.160
−0.330 		0.950+0.170
−0.200 		Microlente 22000+3900
−4600 		0.15+0.28
−0.08
NGTS-2b 0.74+0.13
−0.12 		1.595+0.047
−0.045 		4.511164±0.000061 0.0630+0.0024
−0.0030 		1468+45
−42 		Trânsito 1174+27
−25 		1.64+0.19
−0.22 		6478+94
−89
NGTS-3Ab 2.38±0.26 1.48±0.37 1.6753728 0.023+0.007
−0.005 		Trânsito 2480±36 1.017±0.093 5600±150
NGTS-4b 0.0648±0.0094 0.284±0.023 1.3373508±0.0000080 0.019±0.005 1650±400 Trânsito 921.7±5.9 0.75±0.02 5143±100 [33]
OGLE-2011-BLG-0173Lb 0.19+0.18
−0.11 		8 Microlente 20000+4200
−5500 		0.41+0.30
−0.21
OGLE-2013-BLG-1761Lb 2.7+2.5
−1.5 		1.8±0.5 Microlente 23000+3300
−3900 		0.33+0.32
−0.19
OGLE-2014-BLG-1722Lb 0.17+0.16
−0.10 		1512+3715
−1029 		1.9+1.3
−0.8 		Microlente 20900+4200
−5900 		0.40+0.36
−0.24 		3500+1490
−470
OGLE-2014-BLG-1722Lc 0.26+0.27
−0.16 		2283+7021
−1589 		2.5+2.2
−1.1 		Microlente 20900+4200
−5900 		0.40+0.36
−0.24 		3500+1490
−470
OGLE-2016-BLG-1067Lb 0.43 1.7 Microlente 12165.633 0.3
OGLE-2017-BLG-0173Lb 0.0103+0.0121
−0.0063 		4493+3090
−7055 		3.9±1.6 Microlente 15700+4900
−5900 		0.40+0.39
−0.23 		3500+1500
−500
OGLE-2017-BLG-0373Lb 0.40+0.64
−0.26 		2768+3343
−1704 		2.42+0.76
−0.78 		Microlente 19200+4200
−6400 		0.25+0.27
−0.13 		3250+500
−300
OGLE-2017-BLG-0482Lb 0.0283+0.028
−0.014 		1972+1306
−2322 		1.8+0.6
−0.7 		Microlente 18900+5900
−6800 		0.20+0.20
−0.10 		3150+350
−300
OGLE-2017-BLG-1140Lb 1.59+0.35
−0.26 		819+253
−218 		1.02±0.15 Microlente 11300 0.211+0.032
−0.025 		3170+60
−50
OGLE-2017-BLG-1522Lb 0.75+1.26
−0.40 		780+728
−431 		0.59+0.12
−0.11 		Microlente 3200+3000
−1800 		0.045+0.076
−0.024 		1500+1000
−500
OGLE-2017-BLG-1434Lb 0.014±0.002 968±69 1.18±0.10 Microlente 2800±290 0.234±0.026 3220+30
−70 		[34] Exoplaneta confirmado em 2021[35]
Pi Mensae c 0.0152+0.0026
−0.0027 		0.1822±0.0045 6.26790±0.00046 0.06839±0.00050 1169.8+2.8
−4.3 		Trânsito 59.62±0.073 1.094±0.039 6037±45
TCP J05074264+2447555 b 0.0289±0.0208 0.5 Microlente 1200 0.25±0.18
TYC 3318-1333-1 b 3.42±0.35 562.0+4.1
−4.0 		1.414±0.063 Vel. radial 1622±33 1.19±0.14 4776±10
UKIRT-2017-BLG-001Lb 1.28+0.37
−0.44 		3468+2324
−1300 		4.18+0.96
−0.88 		Microlente 20500+5200
−6800 		0.81+0.21
−0.27 		5100+700
−1300
WASP-134b 1.40±0.08 10.1498 0.0956±0.0025 953±22 Trânsito 636±7 0.81±0.04 5700±100 [36]
WASP-134c 0.70±0.07 70.01±0.14 Vel. radial 636±7 0.81±0.04 5700±100 [36]
WASP-137b 0.681±0.054 1.27±0.11 3.9080284±0.0000053 0.0519±0.0018 1601±65 Trânsito 943±13 1.216±0.066 6100±140 [36]
WASP-143b 0.725±0.084 1.234±0.042 3.7788730±0.0000032 0.0490±0.0014 1325±30 Trânsito 1310±20 1.087±0.045 5900±140 [36]
WASP-144b 0.44±0.06 0.85±0.05 2.2783152±0.0000013 0.0316±0.0005 1260±40 Trânsito 1170±34 0.81±0.04 5200±140 [37]
WASP-145Ab 0.89±0.04 0.90±0.40 1.7690381±0.0000008 0.0261±0.0005 1200±60 Trânsito 298±0.8 0.76±0.04 4900±150 [37]
WASP-146b 1.11±0.15 1.228±0.076 3.3969440±0.0000036 0.0451±0.0024 1486±43 Trânsito 1610±90 1.057±0.085 6100±140 [36]
WASP-147b 0.275+0.028
−0.027 		1.115+0.140
−0.093 		4.602730±0.000027 0.0549+0.0012
−0.0013 		1404+69
−43 		Trânsito 1390±46 1.044+0.070
−0.073 		5702±100 [38]
WASP-158b 2.79±0.23 1.07±0.15 3.656333±0.000004 0.0517±0.0018 1590±80 Trânsito 1740±41 1.38±0.14 6350±150 [37]
WASP-159b 0.55±0.08 1.38±0.09 3.840401±0.000007 0.0538±0.0015 1850±50 Trânsito 2382±36 1.41±0.12 6120±140 [37]
WASP-160Bb 0.278+0.044
−0.045 		1.090+0.047
−0.041 		3.7684952±0.0000035 0.0452±0.0012 1119+25
−23 		Trânsito 926±16 9.750±2.280 5298±99 [38]
WASP-161b 2.49±0.21 1.143+0.065
−0.058 		5.4060425±0.0000048 0.0673±0.0023 1557+34
−29 		Trânsito 1130±14 1.39±0.14 6400±100 [39] Nome próprio Isli
WASP-162b 5.2±0.2 1.00±0.05 9.62468±0.00001 0.0871±0.0013 910±20 Trânsito 1023±13 0.95±0.04 5300±100 [37]
WASP-163b 1.87±0.21 1.202±0.097 1.6096884±0.0000015 0.0266±0.0014 1638±68 Trânsito 858±12 0.97±0.15 5500±200 [39]
WASP-164b 2.13+0.12
−0.13 		1.128+0.041
−0.043 		1.7771255±0.0000028 0.02818+0.00065
−0.00072 		1610+58
−53 		Trânsito 1050±23 0.9460+0.0670
−0.0710 		5806+190
−200 		[38]
WASP-165b 0.658+0.097
−0.092 		1.26+0.19
−0.17 		3.465509±0.000023 0.04823+0.00091
−0.00092 		1624+93
−89 		Trânsito 1900±110 1.248+0.072
−0.070 		5599±150 [38]
WASP-166 b 0.101±0.005 0.63±0.03 5.443540±0.000004 0.0641±0.0011 1270±30 Trânsito 368.55 1.19±0.06 6050±50 [40][41][42]
WASP-168b 0.42±0.04 1.5+0.5
−0.3 		4.153658±0.000003 0.0519±0.0008 1340±40 Trânsito 1000±6 1.08±0.05 6000±100 [37]
WASP-170b 1.6±0.2 1.096±0.085 2.34478022±0.00000360 0.0337±0.0018 1422±42 Trânsito 1005±12 0.93±0.15 5600±150 [39]
WASP-172b 0.47±0.10 1.57±0.10 5.477433±0.000007 0.0694±0.0011 1740±60 Trânsito 1780±50 1.49±0.07 6900±140 [37]
WASP-173Ab 3.69±0.18 1.20±0.06 1.38665318±0.00000027 0.0248±0.0006 1880±55 Trânsito 235±5.8 1.05±0.08 5800±140 [37]
WASP-174b 1.3+0
−1.3 		1.3 4.233700 0.0559 1490 Trânsito 1350 1.30 6400 [43]
Wolf 503b 0.020±0.002 0.1811+0.0068
−0.0065 		6.00118+0.00008
−0.00011 		0.0571±0.0020 805±9 Trânsito 145.4±0.3 0.688+0.023
−0.016 		4716±60 [44][45]

Listas específicas de exoplanetas


Referências

  1. ↑ «NASA Exoplanet Archive». exoplanetarchive.ipac.caltech.edu. California Institute of Technology. Consultado em 27 de março de 2018 
  2. ↑ «The Extrasolar Planets Encyclopaedia». Consultado em 20 de janeiro de 2018 
  3. ↑ a b c Takarada, Takuya; et al. (2018). «Planets around the evolved stars 24 Booties and γ Libra: A 30d-period planet and a double giant-planet system in possible 7:3 MMR». Publications of the Astronomical Society of Japan. 70 (4). arXiv:1804.04008Acessível livremente. doi:10.1093/pasj/psy052 
  4. ↑ Ma, Bo; et al. (2018). «The first super-Earth Detection from the High Cadence and High Radial Velocity Precision Dharma Planet Survey». Monthly Notices of the Royal Astronomical Society. 480 (2). 2411 páginas. Bibcode:2018MNRAS.480.2411M. arXiv:1807.07098Acessível livremente. doi:10.1093/mnras/sty1933 
  5. ↑ Ribas, I.; Tuomi, M.; Reiners, Ansgar; Butler, R. P.; et al. (14 de novembro de 2018). «A candidate super-Earth planet orbiting near the snow line of Barnard's star» (PDF). Omega Space Exploration or OSE. Nature. 563 (7731): 365–368. Bibcode:2018Natur.563..365R. ISSN 0028-0836. OCLC 716177853. PMID 30429552. arXiv:1811.05955Acessível livremente. doi:10.1038/s41586-018-0677-y. hdl:2299/21132. Cópia arquivada (PDF) em 26 de março de 2019 
  6. ↑ A 4.6-year period brown-dwarf companion interacting with the hot-Jupiter CoRoT-20 b, 2018, arXiv:1807.01229Acessível livremente 
  7. ↑ DE CVn: An Eclipsing Post-common Envelope Binary with a Circumbinary Disk and a Giant Planet
  8. ↑ Pinamonti, M.; Damasso, M.; Marzari, F.; Sozzetti, A.; Desidera, S.; Maldonado, J.; Scandariato, G.; Affer, L.; Lanza, A. F.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Claudi, R.; Cosentino, R.; Giacobbe, P.; González-Álvarez, E.; González Hernández, J. I.; Gratton, R.; Leto, G.; Malavolta, L.; Martinez Fiorenzano, A.; Micela, G.; Molinari, E.; Pagano, I.; Pedani, M.; Perger, M.; Piotto, G.; Rebolo, R.; Ribas, I.; et al. (2018). «The HADES RV Programme with HARPS-N at TNG. VIII. GJ15A: A multiple wide planetary system sculpted by binary interaction». Astronomy and Astrophysics. 617: A104. Bibcode:2018A&A...617A.104P. arXiv:1804.03476Acessível livremente. doi:10.1051/0004-6361/201732535 
  9. ↑ The SOPHIE search for northern extrasolar planets XIII. Two planets around M-dwarfs Gl617A and Gl96, 2018, arXiv:1806.10958Acessível livremente 
  10. ↑ a b c TESS exoplanet candidates validated with HARPS archival data. A massive Neptune around GJ143 and two Neptunes around HD23472, 2018, arXiv:1812.04501Acessível livremente 
  11. ↑ Radial velocity follow-up of GJ1132 with HARPS. A precise mass for planet 'b' and the discovery of a second planet, 2018, arXiv:1806.03870Acessível livremente 
  12. ↑ a b The CARMENES search for exoplanets around M dwarfs: The warm super-Earths in twin orbits around the mid-type M dwarfs Ross 1020 (GJ 3779) and LP 819-052 (GJ 1265), 2018, arXiv:1810.07572Acessível livremente 
  13. ↑ Yee, Samuel W.; et al. (2018). «HAT-P-11: Discovery of a Second Planet and a Clue to Understanding Exoplanet Obliquities». The Astronomical Journal. 155 (6). 255. Bibcode:2018AJ....155..255YAcessível livremente. arXiv:1805.09352Acessível livremente. doi:10.3847/1538-3881/aabfecAcessível livremente 
  14. ↑ a b c d HATS-39b, HATS-40b, HATS-41b, and HATS-42b: Three Inflated Hot Jupiters and a Super-Jupiter Transiting F Stars, 2018, arXiv:1804.01623Acessível livremente 
  15. ↑ a b HATS-59b,c: A Transiting Hot Jupiter and a Cold Massive Giant Planet Around a Sun-Like Star, 2018, arXiv:1805.05925Acessível livremente 
  16. ↑ a b c d e f g h i j HATS-60b - HATS-69b: Ten Transiting Planets From HATSouth, 2018, arXiv:1809.01048Acessível livremente 
  17. ↑ a b c d e f g h i Retired A Stars and Their Companions VIII: 15 New Planetary Signals Around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts, 2018, arXiv:1811.03043Acessível livremente 
  18. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap Nowak, Grzegorz; et al. (2020). «K2-280 b – a low density warm sub-Saturn around a mildly evolved star». Monthly Notices of the Royal Astronomical Society. 497 (4): 4423–4435. arXiv:2007.07939Acessível livremente. doi:10.1093/mnras/staa2077 
  19. ↑ a b HD 23472: A multi-planetary system with three super-Earths and two potential super-Mercuries, 2022, arXiv:2209.13345Acessível livremente 
  20. ↑ a b c d e f Radial velocities from the N2K Project: 6 new cold gas giant planets orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810, 2018, arXiv:1809.01228Acessível livremente 
  21. ↑ Two warm, low-density sub-Jovian planets orbiting bright stars in K2 campaigns 13 and 14, 2018, arXiv:1803.02858Acessível livremente 
  22. ↑ HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2, 2018, arXiv:1805.01860Acessível livremente 
  23. ↑ a b Delisle, J.-B.; Ségransan, D.; Dumusque, X.; Diaz, R. F.; Bouchy, F.; Lovis, C.; Pepe, F.; Udry, S.; Alonso, R.; Benz, W.; Coffinet, A.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Moutou, C.; Pollacco, D.; Pompei, E.; Queloz, D.; Santos, N. C.; Wyttenbach, A. (2018), «The HARPS search for southern extra-solar planets», Astronomy & Astrophysics, 614: A133, arXiv:1802.04631Acessível livremente, doi:10.1051/0004-6361/201732529 
  24. ↑ a b c d e Christiansen, Jessie L.; Crossfield, Ian J. M.; Barentsen, Geert; Lintott, Chris J.; Barclay, Thomas; Simmons, Brooke D.; Petigura, Erik; Schlieder, Joshua E.; Dressing, Courtney D.; Vanderburg, Andrew; Ciardi, David R.; Allen, Campbell; McMaster, Adam; Miller, Grant; Veldthuis, Martin; Allen, Sarah; Wolfenbarger, Zach; Cox, Brian; Zemiro, Julia; Howard, Andrew W.; Livingston, John; Sinukoff, Evan; Catron, Timothy; Grey, Andrew; Kusch, Joshua J. E.; Terentev, Ivan; Vales, Martin; Kristiansen, Martti H. (11 de janeiro de 2018). «The K2-138 System: A Near-resonant Chain of Five Sub-Neptune Planets Discovered by Citizen Scientists». The Astronomical Journal (em inglês). 155 (2). 57 páginas. Bibcode:2018AJ....155...57C. ISSN 1538-3881. arXiv:1801.03874Acessível livremente. doi:10.3847/1538-3881/aa9be0 
  25. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq Mayo, Andrew W.; et al. (2018). «275 Candidates and 149 Validated Planets Orbiting Bright Stars inK2 Campaigns 0–10». The Astronomical Journal. 155 (3): 136. Bibcode:2018AJ....155..136M. arXiv:1802.05277Acessível livremente. doi:10.3847/1538-3881/aaadff 
  26. ↑ a b c d e f g Adams, Elisabeth R.; et al. (2020). «Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10». The Planetary Science Journal. 2 (4): 152. Bibcode:2021PSJ.....2..152A. arXiv:2011.11698Acessível livremente. doi:10.3847/PSJ/ac0ea0 
  27. ↑ a b 44 VALIDATED PLANETS FROM K2 CAMPAIGN 10, 2018, arXiv:1806.11504Acessível livremente 
  28. ↑ a b c Akana Murphy, Joseph M.; Kosiarek, Molly R.; Batalha, Natalie M.; Gonzales, Erica J.; Isaacson, Howard; Petigura, Erik A.; Weiss, Lauren M.; Grunblatt, Samuel K.; Ciardi, David R.; Fulton, Benjamin; Hirsch, Lea A.; Behmard, Aida; Rosenthal, Lee J. (2021), «Another Superdense Sub-Neptune in K2-182 b and Refined Mass Measurements for K2-199 b and C», The Astronomical Journal, 162 (6): 294, Bibcode:2021AJ....162..294A, arXiv:2110.05502Acessível livremente, doi:10.3847/1538-3881/ac2830 
  29. ↑ Nava, Chantanelle; et al. (2021), «K2-79b and K2-222b: Mass measurements of two small exoplanets with periods beyond 10 days that overlap with periodic magnetic activity signals», The Astronomical Journal, 163 (2): 41, Bibcode:2022AJ....163...41N, arXiv:2111.02608Acessível livremente, doi:10.3847/1538-3881/ac3141 
  30. ↑ Livingston, John H.; et al. (2018). «Sixty Validated Planets from K2 Campaigns 5–8». The Astronomical Journal. 156 (6): 277. Bibcode:2018AJ....156..277L. arXiv:1810.04074Acessível livremente. doi:10.3847/1538-3881/aae778 
  31. ↑ Petigura, Erik A.; et al. (2017). «Planet Candidates from K2 Campaigns 5–8 and Follow-up Optical Spectroscopy». The Astronomical Journal. 155: 21. arXiv:1711.06377Acessível livremente. doi:10.3847/1538-3881/aa9b83 
  32. ↑ NASA. «Discovery alert! An Earth that looks like Neptune». Exoplanet Exploration: Planets Beyond our Solar System. Consultado em 15 de janeiro de 2021 
  33. ↑ West, Richard G.; et al. (2018), «NGTS-4b: A sub-Neptune transiting in the desert», Monthly Notices of the Royal Astronomical Society, 486 (4): 5094–5103, arXiv:1809.00678Acessível livremente, doi:10.1093/mnras/stz1084 
  34. ↑ Udalski, A.; et al. (2018). «OGLE-2017-BLG-1434Lb: Eighth q<1×10-4 Mass-Ratio Microlens Planet Confirms Turnover in Planet Mass-Ratio Function». Acta Astronomica. 68 (1): 1. Bibcode:2018AcA....68....1U. arXiv:1802.02582Acessível livremente. doi:10.32023/0001-5237/68.1.1 
  35. ↑ Blackman, J. W.; Beaulieu, J.-P.; Cole, A. A.; Koshimoto, N.; Vandorou, A.; Bhattacharya, A.; Marquette, J.-B.; Bennett, D. P. (2021). «OGLE-2017-BLG-1434Lb: Confirmation of a Cold Super-Earth Using Keck Adaptive Optics». The Astronomical Journal. 161 (6): 279. Bibcode:2021AJ....161..279B. arXiv:2107.06510Acessível livremente. doi:10.3847/1538-3881/abfda3 
  36. ↑ a b c d e Anderson, D. R.; et al. (2018). «The discovery of WASP-134b, WASP-134c, WASP-137b, WASP-143b and WASP-146b: three hot Jupiters and a pair of warm Jupiters orbiting Solar-type stars». arXiv:1812.09264Acessível livremente [astro-ph.EP] 
  37. ↑ a b c d e f g h Hellier, Coel; et al. (2019). «New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South». Monthly Notices of the Royal Astronomical Society. 482: 1379–1391. arXiv:1803.02224Acessível livremente. doi:10.1093/mnras/sty2741 
  38. ↑ a b c d Lendl, M.; et al. (2019). «WASP-147b, 160Bb, 164b, and 165b: Two hot Saturns and two Jupiters, including two planets with metal-rich hosts». Monthly Notices of the Royal Astronomical Society. 482: 301–312. arXiv:1807.06973Acessível livremente. doi:10.1093/mnras/sty2667 
  39. ↑ a b c Discovery of three new transiting hot Jupiters: WASP-161 b, WASP-163 b and WASP-170 b, 2018, arXiv:1807.06548Acessível livremente 
  40. ↑ WASP-166b: a bloated super-Neptune transiting a V = 9 star, 2018, arXiv:1811.05292Acessível livremente 
  41. ↑ The Hot Neptune WASP-166 b with ESPRESSO II: Confirmation of atmospheric sodium, 2022, arXiv:2203.04494Acessível livremente 
  42. ↑ The Hot Neptune WASP-166 b with ESPRESSO I: Refining the Planetary Architecture and Stellar Variability, 2022, arXiv:2207.10127Acessível livremente 
  43. ↑ Discovery of WASP-174b: Doppler tomography of a near-grazing transit, 2018, arXiv:1802.00766Acessível livremente 
  44. ↑ Peterson, Merrin S.; et al. (2018). «A 2 R ⊕ Planet Orbiting the Bright Nearby K Dwarf Wolf 503». The Astronomical Journal. 156 (5): 188. Bibcode:2018AJ....156..188P. arXiv:1806.03494Acessível livremente. doi:10.3847/1538-3881/aaddfe 
  45. ↑ Polanski, Alex S.; et al. (2021). «Wolf 503 b: Characterization of a Sub-Neptune Orbiting a Metal-poor K Dwarf». The Astronomical Journal. 162 (6): 238. Bibcode:2021AJ....162..238P. arXiv:2107.08092Acessível livremente. doi:10.3847/1538-3881/ac1590 
Obtida de "https://pt.wikipedia.org/w/index.php?title=Lista_de_exoplanetas_descobertos_em_2018&oldid=64693548"