Movatterモバイル変換

List of exoplanets discovered in 2021

From Wikipedia, the free encyclopedia

This is adynamic list and may never be able to satisfy particular standards for completeness. You can help byediting the page to add missing items, with references toreliable sources.

Thislist of exoplanets discovered in 2021 is a list of confirmedexoplanets that were first observed in 2021.For exoplanets detected only byradial velocity, the listed value for mass is a lower limit. SeeMinimum mass for more information.

Name	Mass (`M`_J)	Radius (`R`_J)	Period (days)	Semi-major axis (AU)	Temp. (K)	Discovery method	Distance (ly)	Host star mass (`M`_☉)	Host star temp. (K)	Remarks
2M0437 b	4±1	1.16	1,136,000	115	1,450±50	imaging	417.9±1.5	0.165±0.015	3,100	Gas giant also known as 2MASSJ04372171 b^[1]^[2]^[3]
b Centauri b	10.9±1.6		200000±100000	556±17		imaging	325±10	8±2		Circumbinary planet in unusually massive host star system^[4]
BD+45 0564 b	1.36±0.12		307.88±1.47	0.83±0.04		radial vel.	174±2	0.81±0.07	5,004±50	^[5]
BD+55 0362 b	0.72±0.08		265.59±1.04	0.78±0.05		radial vel.	168±2	0.909±0.099	5,012±78	Additional giant planet is suspected^[5]
BD+60 1417b	15±5	1.31±0.06		1662	1303±74	imaging	146.65±0.09	1.0	4993±124	Young (≈100 million years) host star^[6]
BD+63 1405 b	3.96±0.31		1,198.48±60.79	2.06±0.14		radial vel.	124.4±1.2	0.82±0.08	5,000±53	Extremely eccentric orbit^[5]
Alpha Centauri Ab	0.062-0.157	0.3011-0.6386				imaging	4.37	1.0788	5790	Imaged nearAlpha Centauri A
COCONUTS-2b	6.3^+1.5 _−1.9		400000000	7506⁺⁵²⁰⁵ ₋₂₀₆₀	434±9	imaging	35.6	0.37±0.02	3406±69	Planet also catalogued as WISEPA J075108.79−763449.6,^[7] First identified as a brown dwarf, but revealed to be an exoplanet in 2021.^[8]
EPIC 201427007 b	0.0090	0.134±0.018	0.72091±0.000067			transit	2304±55	0.930	5633±111	^[9]^[10]
EPIC 201595106 b	0.00705	0.116±0.009	0.877214±0.000087			transit	762±9		5820±20	Candidate since 2018;^[9]^[11] also known as K2-360b
EPIC 211314705.01		0.139±0.007	3.793306^+0.000324 _−0.000343		543⁺⁸ ₋₉	transit	300.0±1.7	0.43±0.01	3,669⁺⁸⁸ ₋₈₂	^[12] Two more planets in system are suspected.^[13]
EPIC 211401787.01		0.247^+0.013 _−0.008	13.774798^+0.000028 _−0.000028		969±9	transit	525±5	1.23±0.02	6,232⁺³³ ₋₃₉	^[12] Host star also known as BD+12 1842.
EPIC 211502222.01		0.243^+0.013 _−0.009	22.996591^+0.001848 _−0.001859		673⁺¹² ₋₁₁	transit	694±6	1.10^+0.03 _−0.04	5,994⁺⁹³ ₋₉₁	^[12]
EPIC 211502222.02		0.160^+0.013 _−0.009	9.398977^+0.001506 _−0.001348		909±14	transit	694±6	1.10^+0.03 _−0.04	5,994⁺⁹³ ₋₉₁	^[12]
EPIC 211525753.01		0.201^+0.020 _−0.014	5.7385647^+0.0013939 _−0.0011048	0.0632^+0.0096 _−0.0176	1,066⁺¹⁹⁰ ₋₇₇	transit		0.96^+0.05 _−0.06	5,790⁺¹⁷⁷ ₋₁₄₇	^[14]
EPIC 211537087.01		0.204^+0.013 _−0.011	21.0267366^+0.0036912 _−0.0038993	0.1599^+0.0178 _−0.0306	624⁺⁰ ₋₃₇	transit		0.90^+0.05 _−0.06	5,568⁺¹⁷⁸ ₋₁₅₀	^[14]
EPIC 211579112.01		0.196^+0.017 _−0.014	17.706320±0.000063		266⁺⁵ ₋₈	transit	403±5	0.27^+0.01 _−0.02	3,315⁺¹³⁷ ₋₁₅₂	^[12]
EPIC 211647930.01		0.552^+0.025 _−0.022	14.759287^+0.000243 _−0.000240		826⁺¹⁴ ₋₁₇	transit	1,133±17	1.06±0.04	5,880⁺⁸⁵ ₋₈₂	^[12]
EPIC 211730024.01		0.504^+0.032 _−0.025	5.113981^+0.000061 _−0.000062		1,380⁺³⁴ ₋₃₀	transit	1,226±21	1.36±0.05	6,502⁺¹³² ₋₁₃₀	^[12]
EPIC 211730267.01		0.332^+0.021 _−0.019	16.3488637^+0.0013811 _−0.0014022	0.1450^+0.0136 _−0.0235	735⁺⁸ ₋₃₉	transit		0.98±0.07	5,794⁺²¹⁰ ₋₁₆₉	^[14]
EPIC 211743874.01		0.197^+0.016 _−0.013	12.283211±0.000051		949⁺²¹ ₋₂₆	transit	1,850±60	1.23±0.04	6,222⁺⁹⁶ ₋₉₁	^[12]
EPIC 211763214.01		0.109^+0.008 _−0.005	21.194733^+0.000108 _−0.000107		569⁺¹⁵ ₋₂₂	transit	786±9	0.86^+0.03 _−0.05	5,424⁺¹⁹² ₋₁₄₄	^[12]
EPIC 211770696.01		0.234^+0.017 _−0.013	16.273563^+0.000054 _−0.000053		850⁺¹⁹ ₋₁₈	transit	1,390±30	0.94^+0.04 _−0.03	5,869⁺⁸⁸ ₋₈₁	^[12]
EPIC 211779390.01		0.092^+0.010 _−0.005	3.850614±0.000012		783⁺¹² ₋₁₄	transit	514±2	0.66±0.02	4,558⁺⁹¹ ₋₈₁	^[12]
EPIC 211897691.02		0.171^+0.017 _−0.011	19.507428^+0.000116 _−0.000113		508±12	transit	1,187±17	0.74^+0.04 _−0.03	4,857⁺⁸⁶ ₋₈₄	^[12]
EPIC 211914998.01		0.239^+0.015 _−0.013	11.2510285^+0.0018188 _−0.0017892	0.0863^+0.0079 _−0.0159	888⁺⁰ ₋₄₇	transit		0.93±0.06	5,650⁺¹⁹³ ₋₁₅₂	^[14]
EPIC 211923431.01		0.300^+0.039 _−0.029	29.740451^+0.000169 _−0.000161		606⁺³¹ ₋₃₆	transit	2,460±70	0.93±0.04	5,532±90	^[12]
EPIC 211978988.01		0.287^+0.022 _−0.017	36.552551^+0.000127 _−0.000122		598⁺¹⁶ ₋₁₅	transit	1,390±20	0.98±0.07	5,817⁺⁴⁵ ₋₄₈	^[12]
EPIC 212058012.01		0.181^+0.012 _−0.008	11.561052^+0.000690 _−0.000668		861⁺¹⁴ ₋₁₅	transit	684±6	1.01±0.05	5,920±104	^[12]
EPIC 212072539.01		0.180^+0.009 _−0.006	7.676972^+0.000012 _−0.000012		465±7	transit	545±3	0.49±0.01	3,804⁺⁹³ ₋₇₄	^[12]
EPIC 212072539.02		0.147^+0.015 _−0.007	2.787174±0.000004		653⁺¹⁰ ₋₁₂	transit	545±3	0.49±0.01	3,804⁺⁹³ ₋₇₄	^[12]
EPIC 212081533.01		0.142^+0.009 _−0.004	3.355850^+0.000091 _−0.000093		722⁺⁷ ₋₁₀	transit	245.8	0.51±0.01	4,374⁺³⁸ ₋₃₄	^[12]
EPIC 212088059.01		0.188^+0.018 _−0.008	10.367437^+0.000020 _−0.000019		437⁺⁴ ₋₅	transit	532±3	0.56±0.01	3,779⁺³⁰ ₋₂₆	^[12]
EPIC 212132195.01		0.202^+0.017 _−0.009	26.201446^+0.003331 _−0.003124		450±5	transit	345.5±1.6	0.71±0.02	4,801±49	^[12]
EPIC 212161956.01		0.215^+0.010 _−0.009	7.187257^+0.000020 _−0.000021		640⁺²⁰ ₋₂₁	transit	1055±13	0.66±0.03	4,599⁺¹⁷⁸ ₋₁₅₂	^[12]
EPIC 212204403.01		0.291^+0.020 _−0.010	4.688418^+0.000119 _−0.000117		908⁺¹² ₋₁₁	transit	662±5	0.83^+0.02 _−0.01	5,077⁺⁴⁰ ₋₃₉	^[12]
EPIC 212204403.02		0.238^+0.021 _−0.010	12.550171^+0.001018 _−0.001057		655⁺⁷ ₋₉	transit	662±5	0.83^+0.02 _−0.01	5,077⁺⁴⁰ ₋₃₉	^[12]
EPIC 212420823.01		0.123^+0.009 _−0.006	9.032178±0.000874		518⁺⁵ ₋₄	transit	1,450±20	0.54±0.01	4,385⁺²⁹ ₋₃₁	^[12]
EPIC 212440430.02		0.138^+0.013 _−0.010	4.163873^+0.000022 _−0.000023		1,158⁺²⁹ ₋₃₄	transit	1,620±20	0.98±0.02	5,789⁺⁴⁶ ₋₅₀	^[12]
EPIC 212543933.01		0.227^+0.023 _−0.017	7.806164^+0.000673 _−0.000623		934⁺²⁸ ₋₃₂	transit	1,310±50	1.02±0.02	5,769⁺³⁹ ₋₃₇	^[12]
EPIC 212624936 b	0.00589	0.517^+0.098 _−0.027	0.578657±0.000066			transit			5765±170	^[9] Host star TYC 5557-667-1^[15]
EPIC 212624936 c	0.019	0.214^+0.098 _−0.057	11.811437±0.00016			transit			5765±170	^[9] Host star TYC 5557-667-1^[16]
EPIC 220492298 b	0.00295	0.085±0.018	0.762406±0.00014			transit			5620±31	^[9]^[17]
EPIC 228836835 b	0.00431	0.089±0.027	0.728113±0.00004			transit	491±6		3782±152	^[9]^[18]
EPIC 251319382.01		0.171^+0.012 _−0.006	8.234885^+0.000508 _−0.000475		885⁺¹² ₋₁₄	transit	577±6	0.95±0.02	5,791±81	^[12]
EPIC 251319382.02		0.199^+0.012 _−0.008	14.871387^+0.000916 _−0.000936		727±10	transit	577±6	0.95±0.02	5,791±81	^[12]
EPIC 251319382.03		0.122^+0.009 _−0.006	3.665912^+0.000273 _−0.000295		1,160⁺¹⁶ ₋₁₅	transit	577±6	0.95±0.02	5,791±81	^[12]
EPIC 251554286.01		0.496^+0.020 _−0.018	15.466805^+0.000572 _−0.000565		735⁺¹³ ₋₁₄	transit	883±12	0.87±0.02	5,698±55	^[12]
G 264-12 b	0.0079±0.0009		2.30538±0.00031	0.02279±0.00061	587±16	radial vel.	52.14±0.03	0.297±0.024	3,326±54	^[19]
G 264-12 c	0.0118±0.0015		8.0518±0.0034	0.0525±0.0014	387±11	radial vel.	52.14±0.03	0.297±0.024	3,326±54	^[19]
Gamma Piscium b	1.34^+0.02 _−0.31		555.1^+6.0 _−2.5	1.32^+0.05 _−0.08		radial vel.	138	0.99^+0.17 _−0.13	4742	^[20]
Gliese 146 b	0.0175^+0.0023 _−0.0021		5.09071 ± 0.00026	0.0510^+0.0024 _−0.0026	573⁺⁶³ ₋₆₉	radial vel.	44.37±0.01	0.684±0.013	4,385±21	Host star also known as HD 22496.^[21]
Gliese 367 b	0.0017±0.0002	0.064±0.005	0.321962^+0.000010 _−0.000012	0.0071±0.0002	1745±43	transit	30.695±0.016	0.45±0.011	3522±70	^[22]
Gliese 393 b	0.0054±0.0008		7.02679^+0.00082 _−0.00085	0.05402±0.00072	485±11	radial vel.	22.956±0.008	0.426±0.017	3,579±51	^[19]
Gliese 486 b	0.0089±0.0004	0.117±0.006	1.467119^+0.000031 _−0.000030	0.01734^+0.00026 _−0.00027	701±13	transit	26.344±0.013	0.323±0.015	3,340±54	Planet may have a measurableatmosphere^[23]
Gliese 740 b	0.0093±0.0016		2.37756^+0.00013 _−0.00011	0.029±0.001	829⁺⁴⁰ ₋₅₀	radial vel.	36.21±0.02	0.58±0.06	3,913±21	^[24]
Gliese 9689 b	0.0304±0.0046		18.27±0.01	0.1139±0.0039	453±39	radial vel.	100.10±0.04	0.59±0.06	3,836±69	^[25]
HAT-P-58b	0.372±0.03	1.332±0.043	4.0138379±0.0000024	0.04994±0.00044	1622±18	transit	1690±40	1.031±0.028	6078±48	^[26]
HAT-P-59b	1.540±0.067	1.123±0.013	4.1419771±0.0000012	0.05064±0.00037	1278±7	transit	871±4	1.008±0.022	5678±16	^[26]
HAT-P-60b	0.574±0.038	1.631±0.024	4.7947813±0.0000024	0.06277±0.00017	1772±12	transit	767±7	1.435±0.012	6212±26	^[26]
HAT-P-61b	1.057±0.07	0.899±0.027	1.90231289±0.00000077	0.03010±0.00034	1505±16	transit	1120±20	1.004±0.012	5587±45	^[26]
HAT-P-62b	0.761±0.088	1.073±0.029	2.6453235±0.0000039	0.03772±0.00024	1512±13	transit	1150±20	1.023±0.020	5629±48	^[26]
HAT-P-63b	0.614±0.024	1.119±0.033	3.377728±0.000013	0.04294±0.00035	1237±11	transit	1330±20	0.925±0.023	5400⁺⁵⁵ ₋₃₉	^[26]
HAT-P-64b	0.58^+0.18 _−0.13	1.703±0.07	4.0072320±0.0000017	0.05387±0.00030	1766⁺²² ₋₁₆	transit	2135±20	1.298±0.021	6457⁺⁵⁵ ₋₃₆	^[26]
HATS-74Ab	1.46±0.14	1.032±0.021	1.73185606±0.00000055	0.02384±0.00011	895.1±5.7	transit	952±12	0.601±0.008	3775±54	Host star also known as TOI-737^[27]
HATS-75b	0.491±0.039	0.884±0.013	2.7886556±0.0000011	0.032742^+0.000134 _−0.000099	772.3±2.3	transit	640±4	0.6017^+0.0074 _−0.0055	3812±79	Host star also known as TOI-552^[27]
HATS-76b	2.629±0.089	1.079±0.031	1.9416423±0.0000014	0.02658^+0.00021 _−0.00029	939.8±6.7	transit	1272±19	0.662^+0.016 _−0.021	3990±120	Host star also known as TOI-555^[27]
HATS-77b	1.374^+0.100 _−0.074	1.165±0.021	3.0876262±0.0000016	0.03607±0.00025	828.3±5.9	transit	1440±40	0.655±0.014	4082±69	Host star also known as TOI-730^[27]
HD 360 b	0.75^+0.12 _−0.15		273.1^+1.6 _−0.8	0.98^+0.11 _−0.03		radial vel.	362	1.69^+0.15 _−0.53	4770	^[20]
HD 3765 b	0.173^+0.014 _−0.013		1,211⁺¹⁵ ₋₁₆	2.108^+0.032 _−0.033		radial vel.	78.5±0.1			^[28]
HD 5278 b	0.0245^+0.0047 _−0.0044	0.219±0.004	14.339156^+0.000049 _−0.000047	0.1202±0.0013	943±13	transit	183.1±2.7	1.126^+0.036 _−0.035	6,203±64	Host star also known as TOI-130.^[29]
HD 5278 c	0.0579^+0.0057 _−0.0060		0.2416±0.0027	0.1202±0.0013	943±13	radial vel.	183.1±2.7	1.126^+0.036 _−0.035	6,203±64	Host star also known as TOI-130.^[29]
HD 10975 b	0.45^+0.06 _−0.15		283.8^+12.7 _−0.1	0.95^+0.06 _−0.08		radial vel.	379	1.41^+0.34 _−0.35	4840	^[20]
HD 13808 b	0.0346		14.2	0.11		radial vel.	92.2	0.771±0.022	5,035±50	Candidate since 2011,^[30] confirmed in 2021^[31]
HD 13808 c	0.0315		53.8	0.26		radial vel.	92.2	0.771±0.022	5,035±50	Candidate since 2011,^[30] confirmed in 2021^[31]
HD 19615 b	8.5±0.7		402±2	1.1±0.1		radial vel.	872±7	1.1±0.1	3987±125	Red giant host star^[32]
HD 24040 c	0.201±0.027		515.4^+2.2 _−2.5	1.3±0.021		radial vel.	152.3±0.4	1.14±0.02	5,917±52	^[28]
HD 26161 b	13.5^+8.5 _−3.7		32,000^+21,000 _−10,000	20.4^+7.9 _−4.9		radial vel.	133.6±0.3			Very eccentric orbit, and also red dwarf in the system^[28]
HD 27969 b	4.80^+0.24 _−0.23		654.5^+5.7 _−5.8	1.552^+0.032 _−0.033	261±11	radial vel.		1.16±0.07	5,966±21	^[33]
HD 39474 b	0.42^+0.05 _−0.03	1.008^+0.012 _−0.015	52.97818^+0.00004 _−0.00004	0.30^+0.02 _−0.03	759⁺³⁷ ₋₂₆	transit	372.5±1.1	1.316±0.027	6,394±75	Host star also known as TOI-201^[34]
HD 63935 b	0.0340±0.0057	0.267±0.013	9.058811^+0.000017 _−0.000016		911±27	transit	159.36±0.15	0.933±0.054	5,534±100	^[35]
HD 63935 c	0.0349±0.0076	0.259±0.012	21.4023^+0.00189 _−0.00194		684±21	transit	159.36±0.15	0.933±0.054	5,534±100	^[35]
HD 66428 c	27⁺²² ₋₁₇		39,000^+56,000 _−18,000	23.0^+19.0 _−7.6		radial vel.	174.1±0.7	1.09±0.02	5,773±55	^[28]
HD 68988 c	15.0^+2.8 _−1.5		16,100^+11,000 _−3,500	13.2^+5.3 _−2.0		radial vel.	198.8±0.6	1.16±0.01	5,919±11	Suspected since 2006^[28]
HD 73583 b	0.0315±0.0098	0.253±0.009	6.3980418^+0.0000065 _−0.0000063	0.0601±0.0026	721±21	transit	103.08±0.10	0.71±0.02	4511±110	Host star also known as TOI-560,^[36] planetary helium emission detected.^[37]^[38]
HD 73583 c	0.0302±0.0055	0.212±0.009	18.8797^+0.00088 _−0.00073	0.1236^+0.0053 _−0.0053	503±15	transit	103.08±0.10	0.71±0.02	4511±110	Host star also known as TOI-560^[36]^[38]
HD 79181 b	0.64^+0.06 _−0.16		273.1^+1.3 _−0.4	0.90^+0.07 _−0.08		radial vel.	337	1.28^+0.32 _−0.28	4862	^[20]
HD 80869 b	4.86^+0.65 _−0.29		1711.7^+9.3 _−9.6	2.878^+0.045 _−0.046	203.2^+6.8 _−5.5	radial vel.		1.08±0.05	5,837±15	Very eccentric orbit^[33]
HD 95544 b	6.84±0.31		2172⁺²³ ₋₂₁	3.386^+0.075 _−0.077	156.5^+5.4 _−5.5	radial vel.		1.09±0.07	5,722±15	^[33]
HD 99183 b	0.97^+0.06 _−0.25		310.4^+5.2 _−1.7	1.08^+0.05 _−0.07		radial vel.	355	1.76^+0.31 _−0.30	4886	^[20]
HD 107148 c	0.0626^+0.0097 _−0.0098		18.3267^+0.0022 _−0.0024	0.1406±0.0018		radial vel.	161.4±0.4	1.1±0.1	5,789±36	^[28]
HD 108236 f		0.17406^+0.00482 _−0.00437	29.54255±0.00069	0.1759±0.0037		transit	211	0.853±0.047	5,720.0±50.0	^[39]^[40]
HD 109286 b	2.99±0.15		520.1±2.3	1.259±0.021	259.4±5.5	radial vel.		0.98±0.05	5,694±23	^[33]
HD 103891 b	1.44^+0.06 _−0.05		1919⁺¹⁴ ₋₁₅	3.27^+0.02 _−0.01		radial vel.	179.0±0.4	1.28±0.01	6072±20	^[41]
HD 105779 b	0.64±0.06		2412⁺⁵⁵ ₋₅₂	3.38±0.05		radial vel.	179.7±0.3	0.89±0.01	5792±16	^[41]
HD 110082 b		0.2857±0.0089	10.18271±0.00004	0.113^+0.009 _−0.013		transit	342.8±0.9	1.21±0.06	6,200±100	Orbiting a primary of wide binary system^[42] Host star also known as TOI-1098.
HD 110113 b	0.0143±0.0020	0.183±0.011	2.541^+0.0005 _−0.001	0.035±0.001	1,371±14	transit	346.5±2.3	0.99±0.08	5,730	Radius gap planet, host star also known as TOI-755^[43]
HD 110113 c	0.0330±0.0038		6.744^+0.008 _−0.009	0.068^+0.001 _−0.002	990±10	radial vel.	346.5±2.3	0.99±0.08	5,730	Host star also known as TOI-755.^[43]
HD 115954 b	8.29^+0.75 _−0.58		3700⁺¹⁵⁰⁰ ₋₃₉₀	5.00^+1.3 _−0.36	144.9^+8.1 ₋₁₃	radial vel.		1.18±0.06	5957±26	^[33]
HD 124330 b	0.75±0.06		270.66±1.21	0.86±0.04		radial vel.	198±3	1.15±0.079	5,873±19	Additional giant planet is suspected^[5]
HD 136925 b	0.84^+0.078 _−0.074		4,540⁺¹⁶⁰ ₋₁₄₀	5.13^+0.12 _−0.11		radial vel.	156.2		5715	Additional planet suspected^[28]
HD 137496 b	0.0127±0.0017	0.117±0.005	1.62116±0.00008	0.02732±0.00019	2130⁺³⁰ ₋₂₉	transit	509±6	1.035±0.022	5799±61	^[44]
HD 137496 c	7.66±0.11		479.9^+1.1 _−1.0	1.2163^+0.0087 _−0.0088	370±5	radial vel.	509±6	1.035±0.022	5799±61	^[44]
HD 150010 b	2.4±0.4		562±8	1.1±0.1		radial vel.	473.4±2.1	1.3±0.1	4256±125	Red giant host star^[32]
HD 152843 b	0.0364^+0.0207 _−0.0193	0.304±0.012	11.6264^+0.0022 _−0.0025	0.1053^+0.003 _−0.0031		transit	352.0±1.0	1.15±0.04	6,310±100	^[45]
HD 152843 c	0.0865	0.521±0.013	24.38^+6.23 _−3.4			transit	352.0±1.0	1.15±0.04	6,310±100	^[45]
HD 155193 b	0.75±0.06		352.65±2.58	1.04±0.04		radial vel.	186±6	1.221±0.083	6,239±20	^[5]
HD 156668 c	0.0991^+0.0079 _−0.0077		811.3^+5.2 _−5.3	1.570±0.017		radial vel.	79.34±0.03	0.772±0.020	4,850±88	Additional body in system is suspected^[28]
HD 161178 b	0.57^+0.02 _−0.16		279.3^+1.0 _−0.8	0.85^+0.05 _−0.07		radial vel.	351	1.06^+0.25 _−0.17	4786	^[20]
HD 164922 e	0.0331±0.0031		41.763±0.012	0.2293^+0.0026 _−0.0027		radial vel.	71.69±0.03	0.874±0.012	5,293±32	^[28]
HD 168009 b	0.0300^+0.0038 _−0.0037		15.1479^+0.0035 _−0.0037	0.1192^+0.0017 _−0.0018		radial vel.	75.97±0.03	0.99	5,792±80	^[28]
HD 174205 b	4.2±0.5		582±17	1.7±0.1		radial vel.	769±5	1.8±0.1	4393±125	Red giant host star^[32]
HD 183579 b	0.0620^+0.0126 _−0.0123	0.317^+0.013 _−0.011	17.471278^+0.000058 _−0.000060	0.1334^+0.0062 _−0.0061	769⁺¹⁷ ₋₁₃	transit	186.1±0.8	1.031^+0.025 _−0.026	5,788±44	Host star also known as TOI-1055^[46]^[47]^[48]
HD 191939 e	>0.3531±0.0126		101.12±0.13	0.4007±0.012	390±8	radial vel.	175.1±0.2	0.92	5400	Also suspected brown dwarf on wider orbit^[49]^[50]
HD 207897 b	0.0453±0.0050	0.223±0.007	16.202159^+0.000085 _−0.000083	0.1163^+0.0017 _−0.001	632.2^+8.1 _−7.0	transit	92.15±0.10	0.80^+0.036 _−0.030	5,070⁺⁶⁰ ₋₅₇	^[51]
HD 211403 b	5.54^+0.39 _−0.38		223.8±0.41	0.768±0.013	380±13	radial vel.		1.20±0.06	6,273±44	^[33]
HD 213472 b	3.48^+1.10 _−0.59		16,700^+12,000 _−4,800	13.0^+5.7 _−2.6		radial vel.	210.6			^[28]
HD 219139 b	0.78^+0.05 _−0.20		275.5^+2.3 _−1.0	0.94^+0.06 _−0.07		radial vel.	345	1.46^+0.31 _−0.29	4831	^[20]
HD 331093 b	1.50±0.11		621.62±16.11	1.44±0.07		radial vel.	164.07±0.14	1.030±0.079	5,544±33	^[5]
HIP 5763b	0.51		30.014^+0.1528 _−0.2842	0.170		radial vel.	104.17±0.14	0.72		^[52]
HIP 34222b	0.83		160.0^+2.7 _−2.9	0.492		radial vel.	74.55±0.09	0.62		^[52]
HIP 56640 b	7.1±1.6		2574.9±86.1	3.73±0.08		radial vel.	400.4±1.9	1.04^+0.07 _−0.06	4769±55	Red giant host star also known as HD100939b^[53]^[54]
HIP 86221b	0.71		2.224^+0.0004 _−0.0005	0.031		radial vel.	96±11	0.79		^[52]
HIP 90988 b	2.102^+0.079 _−0.085		455.73816^+2.11413 _−1.88939	1.26±0.01		radial vel.	307.6±1.2	1.30±0.08	4884±58	Gas giant orbiting a red giant host star also known as HD 170707^[55]^[54]^[56]
HIP 97166b	0.0629±0.047	0.245±0.012	10.28891±0.00004	0.089±0.001	757±25	transit	215.54±0.33	0.898±0.054	5,198±100	^[57]
HIP 97166c	9.9±1.8		16.84±0.22	0.124±0.002	642±22	radial vel.	215.54±0.33	0.898±0.054	5,198±100	^[57]
K2-99c	8.4±0.2		522.2±1.4	1.43±0.01	390±6	radial vel.	1980	1.6	5990	^[58]
K2-268d		0.133^+0.013 _−0.006	4.528598^+0.000016 _−0.000015		888⁺¹⁶ ₋₁₅	transit	1,079±10	0.84±0.02	5,106⁺⁷⁰ ₋₆₁	Two more planets were previously known; host star also known as EPIC 211413752.^[12]
K2-268e		0.119^+0.010 _−0.007	6.131243^+0.000032 _−0.000033		801±13	transit	1,079±10	0.84±0.02	5,106⁺⁷⁰ ₋₆₁	Two more planets were previously known; host star also known as EPIC 211413752.^[12]
K2-268f		0.199^+0.013 _−0.008	26.270570^+0.000105 _−0.000109		492⁺⁸ ₋₁₀	transit	1,079±10	0.84±0.02	5,106⁺⁷⁰ ₋₆₁	Two more planets were previously known; host star also known as EPIC 211413752.^[12]
K2-185c		0.213±0.008	52.713494^+0.000155 _−0.000164		477⁺¹⁴ ₋₁₇	transit	882±11	0.96^+0.05 _−0.07	5,788⁺¹⁹⁰ ₋₁₅₇	Host star also known as EPIC 211611158.^[12]
K2-304c		0.203^+0.017 _−0.011	5.213965±0.000442		866⁺²⁷ ₋₃₇	transit	1,380±20	0.83^+0.05 _−0.04	5,171⁺¹⁷² ₋₁₃₀	Host star also known as EPIC 212297394.^[12]
K2-307c		0.207^+0.017 _−0.011	23.228555^+0.000068 _−0.000071		658⁺¹³ ₋₁₄	transit	1,050±20	0.99^+0.03 _−0.04	6,004⁺⁷⁷ ₋₇₈	Host star also known as EPIC 212587672.^[12]
Kepler-129d	8.3^+1.1 _−0.7		2646⁺¹⁴⁰ ₋₉₄	4.0±0.1		radial vel.	1,349±14	1.18	5,770	^[59]
Kepler-1704b	4.15±0.29	1.065^+0.043 _−0.041	988.88113^+0.00091 _−0.00092	2.026^+0.024 _−0.031	253.8^+3.7 _−4.1	transit	2,690±40	1.131^+0.040 _−0.051	5,745⁺⁸⁸ ₋₈₉	Very eccentric orbit (e=0.921),^[60]
KIC 5479689 b	0.5^+0.4 _−0.1		1.701531^+0.000008 _−0.000419			orbital brightness modulation	1,504	0.966^+0.03 _−0.04	5459.1^+90.0 _−85.2	^[61]
KIC 8121913 b	2.1±0.4		3.294601^+0.000013 _−0.00022			orbital brightness modulation	2350	1.456^+0.069 _−0.15	5075.3^+110.2 _−109.4	^[61]
KIC 10068024 b	2.0±0.4		2.073549^+0.000008 _−0.000177			orbital brightness modulation	3,600	1.22^+0.175 _−0.139	6,118.4^+127.2 _−121.2	^[61]
KMT-2016-BLG-2605b	0.8^+1.2 _−0.4			0.68±0.11		microlensing	21,000±3,000	0.065^+0.10 _−0.035		^[62]
KMT-2017-BLG-2509b	2.09^+1.68 _−1.26			2.14^+0.27 _−0.39		microlensing	23,000±3,000	0.46^+0.37 _−0.27		^[63]
KMT-2018-BLG-1025Lb	0.0191^+0.0258 _−0.0104			1.305^+0.194 _−0.227		microlensing	22,000±3,000	0.219^+0.297 _−0.120		Multiple solutions for orbital parameters^[64]
KMT-2018-BLG-1743	0.245^+0.339 _−0.135			1.449^+0.209 _−0.229		microlensing	21,000±3,000	0.193^+0.268 _−0.107		Multiple orbital solutions, binary host star^[65]
KMT-2018-BLG-1976Lb	1.96^+1.23 _−1.12			2.04^+0.72 _−0.83		microlensing	19,000±2,000	0.65^+0.41 _−0.37		^[66]
KMT-2018-BLG-1996Lb	1.22^+0.72 _−0.63			1.97^+0.51 _−0.25		microlensing	19,000±2,000	0.69^+0.40 _−0.38		^[66]
KMT-2018-BLG-1988Lb	0.021^+0.015 _−0.011			2.83^+1.23 _−0.97		microlensing	14000⁺⁶⁰⁰⁰ ₋₅₀₀₀	0.48^+0.33 _−0.25		Multiple solutions for orbital parameters^[67]
KMT-2019-BLG-0371b	7.70^+11.34 _−3.90			0.79^+0.14 _−0.16		microlensing	2,3000^+3,000 _−4,000	0.09^+0.14 _−0.05		Multiple solutions for orbital separation^[68]
KMT-2019-BLG-0253b	0.029^+0.016 _−0.013			3.1^+0.8 _−0.9		microlensing	16,000^+6,000 _−5,000	0.70^+0.34 _−0.31		^[69]
KMT-2019-BLG-1715	2.56^+1.13 _−1.16			3.32^+0.82 _−0.92		microlensing	13,000±3,000	0.61^+0.27 _−0.28		Multiple solutions for orbital separation, also 0.15`M`_☉red dwarf in the system.^[70]
KMT-2020-BLG-0414Lb	0.0032			0.15		microlensing	3,300±300	0.3		Also abrown dwarf with mass 17`M`_J in the system at 15 AU separation^[71]
KMT-2021-BLG-0912Lb	0.022^+0.007 _−0.008			3.03^+3.46 _−2.46		microlensing	22000±3000	0.75^+0.23 _−0.28		Multiple solutions for orbital parameters^[72]
KOI-5Ab	0.179	0.63	5			transit	1,870±70	1.13	5861	Also called TOI-1241b.^[73]^[74]
KOI-984b	0.0544±0.0094	0.384±0.004	4.2881785±0.0000035	0.0504±0.0006	1022⁺³¹ ₋₃₀	transit	749±4	0.928±0.031	5295±150	Another planet in system on poorly constrained orbit^[75]
KOI-4777b		0.046±0.003	0.412000±0.000001	0.0080±0.0003	1180±20	transit	565±4	0.41±0.02	3515±69	^[76]
Lalande 21185 c	0.0568^+0.0091 _−0.0083		3190⁺²⁰⁰ ₋₁₇₀	3.1^+0.13 _−0.11		radial vel.	8.31±0.01	0.390±0.011	3,601±51	^[28]
Lambda Serpentis b	0.0428^+0.0047 _−0.0045		15.5083^+0.0016 _−0.0018	0.1238±0.002		radial vel.	38.87±0.07	1.14	5,884±4	^[28]
LHS 1478 b	0.0073±0.0006	0.111±0.004	1.9495378^+0.0000040 _−0.0000041	0.01848^+0.00061 _−0.0006	595⁺¹⁰ ₋₉	transit	59.40±0.03	0.236±0.012	3,381±54	^[77] Host star also known as TOI-1640 or G 245-61.
LHS 1678 b	0.0002±0.0003	0.062±0.004	0.8602322^+0.0000068 _−0.0000048	0.01251^+0.00059 _−0.00056		transit	64.88±0.03	0.345±0.014	3490±50	^[78]
LHS 1678 c	0.0012^+0.0013 _−0.0008	0.088±0.006	3.694247^+0.0000024 _−0.0000021	0.0331^+0.0016 _−0.0015		transit	64.88±0.03	0.345±0.014	3490±50	^[78]
LTT 1445 Ac	0.0048±0.0006	0.103	3.12390	0.02661^+0.00047 _−0.00049		transit	22.41±0.01	0.256±0.014	3337±150	^[79]
L 98-59 e	0.0094		12.8	0.071	342⁺²⁰ ₋₁₈	radial vel.	34.6	0.32±0.03	3500±150	^[80]
L 98-59 f	0.0078		23.2	0.103	285⁺¹⁸ ₋₁₇	radial vel.	34.6	0.32±0.03	3500±150	Unconfirmed, potentially habitable exoplanet^[80]
NGTS-13b	4.84±0.44	1.142±0.046	4.12	0.0549^+0.0015 _−0.0025	1,605±30	transit	2150	1.30^+0.11 _−0.18	5,819±73	^[81]
NGTS-14Ab	0.092±0.012	0.444±0.030	3.5357173±0.0000069	0.0403±0.0071	1,143±139	transit	1,060	0.898±0.035	5,187±11	^[82]
NGTS-15b	0.751^+0.102 _−0.088	1.10±0.10	3.27623±0.00001	0.0441±0.0046	1,146±47	transit	2,580±60	0.995±0.015	5,600±150	^[83]
NGTS-16b	0.667^+0.157 _−0.129	1.30^+0.13 _−0.12	4.84532±0.00002	0.0523±0.0064	1,177±59	transit	2,910⁺⁹⁵ ₋₇₅	1.002±0.011	5,550±150	^[83]
NGTS-17b	0.764^+0.195 _−0.164	1.24±0.11	3.24253±0.00001	0.0391±0.0043	1,457±50	transit	3,420±90	1.025^+0.015 _−0.014	5,650±100	^[83]
NGTS-18b	0.409^+0.081 _−0.063	1.21±0.18	3.05125±0.00001	0.0448±0.0068	1,381⁺⁵⁵ ₋₅₃	transit	3,610±140	1.003^+0.020 _−0.012	5,610±150	^[83]
OGLE-2014-BLG-0319Lb	0.57^+0.36 _−0.31			3.49^+1.17 _−1.12		microlensing	25000⁺⁴⁰⁰⁰ ₋₉₀₀₀	0.52^+0.33 _−0.29		^[84]
OGLE-2014-BLG-0676Lb	3.68^+0.69 _−1.44			4.53^+1.49 _−2.50		microlensing	8700⁺²⁵⁰⁰ ₋₄₆₀₀	0.73^+0.14 _−0.29		^[85]
OGLE-2017-BLG-1099b	3.02^+2.43 _−1.81			2.73^+0.40 _−0.53		microlensing	24,000±3,000	0.45^+0.36 _−0.27		^[63]
OGLE-2018-BLG-0383L b	0.0201^+0.0173 _−0.0088			1.8±0.2		microlensing	25000±2000	0.10^+0.13 _−0.05		^[86]
OGLE-2018-BLG-0506	0.051^+0.038 _−0.027			3.0^+0.7 _−0.8		microlensing	18,000±5,000	0.63^+0.37 _−0.32		^[69]
OGLE-2018-BLG-0516	0.063^+0.052 _−0.034			2.2^+0.8 _−0.7		microlensing	7,000^+3,000 _−2,000	0.47^+0.38 _−0.25		^[69]
OGLE-2018-BLG-0567Lb	0.32^+0.34 _−0.16			2.72^+0.49 _−0.55		microlensing	23,000±3,000	0.24^+0.16 _−0.13		^[87]
OGLE-2018-BLG-0962Lb	1.37^+0.80 _−0.72			3.57^+0.68 _−1.02		microlensing	21,000^+3,000 _−5,000	0.55^+0.32 _−0.29		^[87]
OGLE-2018-BLG-0977	0.020^+0.016 _−0.012			2.0^+0.6 _−0.5		microlensing	7,000±2,000	0.47^+0.38 _−0.27		^[69]
OGLE-2018-BLG-1428Lb	0.77^+0.77 _−0.53			3.30^+0.59 _−0.83		microlensing	20,000^+3,000 _−5,000	0.43^+0.33 _−0.22		^[88]
OGLE-2019-BLG-0299b	6.22^+3.80 _−3.67			2.80^+0.58 _−0.89		microlensing	19,000±4,000	0.59^+0.36 _−0.35		^[63]
OGLE-2019-BLG-0468Lb	3.43^+1.83 _−1.17			3.29^+4.15 _−2.52		microlensing	14000±3000	0.92^+0.49 _−0.32		Multiple solutions for orbital parameters^[89]
OGLE-2019-BLG-0468Lc	10.22^+5.46 _−3.50			2.77^+3.49 _−2.12		microlensing	14000±3000	0.92^+0.49 _−0.32		Multiple solutions for orbital parameters^[89]
OGLE-2019-BLG-0954Lb	14.2^+9.9 _−7.5			2.65^+0.89 _−1.20		microlensing	12,000^+1,000 _−2,000	0.80^+0.55 _−0.42		^[66]
OGLE-2019-BLG-0960Lb	0.0071±0.0027			1.75±0.55		microlensing	2,900±1000	0.45±0.15		Smallest planet discovered bymicrolensing^[90]
OGLE-2019-BLG-1053Lb	0.0078^+0.0037 _−0.0031			3.4±0.5		microlensing	22,000^+3,000 _−2,000	0.61^+0.29 _−0.24		^[91]
OGLE-2019-BLG-1058	6.836±6.027					microlensing	8,000±5,000			Multiple solutions,rogue planet^[92]
OGLE-2018-BLG-1185b	0.026^+0.025 _−0.015			1.54^+0.18 _−0.22		microlensing	24,000^+2,000 _−3,000	0.37^+0.35 _−0.21		Multiple solutions for planet and star masses.^[93]
OGLE-2019-BLG-1492	0.117^+0.079 _−0.061			2.7±0.9		microlensing	18,000^+6,000 _−7,000	0.68±0.34		^[69]
RR Caeli c	2.7±0.7		14,200±300	9.7±0.9		timing	69.10±0.03	0.18+0.44	3,100+7,540	Circumbinary planet around red and white dwarfs^[94]
TIC 172900988 b	2.84±0.25	1.009±0.043	196.5±7.7			transit	799±9	1.24 and 1.20	6050 and 5983	Circumbinary planet^[95]
TIC 257060897b	0.67±0.03	1.49±0.04	3.660028±0.000006	0.051±0.002	1,762±21	transit	1,655±8	1.32±0.04	6,128±57	^[96]
TOI-178b	0.0047^+0.0012 _−0.0013	0.102±0.006	1.914558±0.000018	0.02607±0.00078	1,040⁺²² ₋₂₁	transit	205.16±0.03	0.650^+0.027 _−0.029	4,316±70	^[97]
TOI-178c	0.015^+0.0017 _−0.0021	0.149^+0.01 _−0.008	3.238450^+0.000020 _−0.000019	0.0370±0.0011	873±18	transit	205.16±0.03	0.650^+0.027 _−0.029	4,316±70	^[97]
TOI-178d	0.0094^+0.0025 _−0.0032	0.229±0.006	6.557700±0.000016	0.0592±0.0018	690±14	transit	205.16±0.03	0.650^+0.027 _−0.029	4,316±70	^[97]
TOI-178e	0.0121^+0.0039 _−0.0029	0.197^+0.007 _−0.008	9.961881±0.000042	0.0783^+0.0023 _−0.0024	600±12	transit	205.16±0.03	0.650^+0.027 _−0.029	4,316±70	^[97]
TOI-178f	0.0242^+0.0052 _−0.0047	0.204±0.009	15.231915^+0.000115 _−0.000095	0.1039±0.0031	521±11	transit	205.16±0.03	0.650^+0.027 _−0.029	4,316±70	^[97]
TOI-178g	0.0123^+0.0041 _−0.0050	0.256^+0.012 _−0.011	20.70950^+0.00014 _−0.00011	0.1275^+0.0038 _−0.0039	470±10	transit	205.16±0.03	0.650^+0.027 _−0.029	4,316±70	^[97]
TOI-220 b	0.0434±0.0031	0.271±0.013	10.695264	0.08911±0.0010	805±21	transit	290±13	0.825±0.028	5,298±65	Additional long-period planet suspected^[98]
TOI-269 b	0.0277±0.0044	0.247±0.011	3.697723^+0.000018 _−0.000017	0.0345±0.0015	531±25	transit	186.01±0.25	0.3917±0.0095	3,514±70	^[99]
TOI-431 b	0.0097±0.0011	0.0014±0.004	0.490047^+0.000010 _−0.000007	0.0113^+0.0002 _−0.0003	1,862±42	transit	106.37±0.03	0.78±0.07	4,850±75	Host star lso known as CD-26 2288 or HIP 26013.^[100]
TOI-431 c	0.0089^+0.0013 _−0.0011		4.8494^+0.0003 _−0.0002	0.0052±0.001	867±20	radial vel.	106.37±0.03	0.78±0.07	4,850±75	Host star also known as CD-26 2288 or HIP 26013.^[100]
TOI-431 d	0.0312±0.0047	0.294±0.008	12.46103±0.00002	0.098±0.002	633±14	transit	106.37±0.03	0.78±0.07	4,850±75	Host star lso known as CD-26 2288 or HIP 26013.^[100]
TOI 451 b		0.1732^+0.0134 _−0.0116	1.858701^+0.000027 _−0.000033	0.0271^+0.0023 _−0.0038	1,524⁺¹⁰⁰ ₋₆₀	transit	405.1±1.3	0.94±0.025	5,550±56	Planets orbiting primary of wide binary system.^[101]^[102] Host star also known asCD-38 1467.
TOI 451 c		0.2741±0.0125	9.192523^+0.000064 _−0.000084	0.0771^+0.0066 _−0.0093	903⁺⁵³ ₋₃₆	transit	405.1±1.3	0.94±0.025	5,550±56	Planets orbiting primary of wide binary system.^[101]^[102] Host star also known asCD-38 1467.
TOI 451 d		0.3598±0.0134	16.364981^+0.000047 _−0.000049	0.1255^+0.0057 _−0.0065	708⁺¹⁵ ₋₁₂	transit	405.1±1.3	0.94±0.025	5,550±56	Planets orbiting primary of wide binary system^[101]^[102] Host star also known asCD-38 1467.
TOI-530b	0.40^+0.09 _−0.10	0.83±0.06	6.387597^+0.000019 _−0.000018	0.052^+0.005 _−0.004	565⁺²⁸ ₋₃₁	transit	482±2	0.53±0.02	3,659±120	^[103]
TOI-532b	0.1935^+0.0305 _−0.0293	0.520±0.017	2.3266508±0.0000030	0.0296±0.00035	867±18	transit	439.1±1.2	0.639±0.023	3927±37	Neptunian desert planet^[104]
TOI-558b	3.61±0.15	1.086^+0.041 _−0.038	14.574071±0.000026	0.1291^+0.0020 _−0.0021	1,061⁺¹³ ₋₁₂	transit	1,312±17	1.349^+0.064 _−0.065	6,466⁺⁹⁵ ₋₉₃	^[105]
TOI-559b	6.01^+0.24 _−0.23	1.091^+0.028 _−0.025	6.9839095±0.0000051	0.0723±0.0013	1,180⁺¹⁸ ₋₁₆	transit	761±7	1.026±0.057	5,925⁺⁸⁵ ₋₇₆	^[105]
TOI-628 b	6.33^+0.29 _−0.31	1.060^+0.041 _−0.034	3.4095675^+0.0000070 _−0.0000069	0.04860^+0.00080 _−0.00094	1,586⁺⁵² ₋₄₀	transit	582	1.311^+0.066 _−0.075	6,250⁺²²⁰ ₋₁₉₀	Host star also known as HD 288842^[106]
TOI-640 b	0.88±0.16	1.771^+0.060 _−0.056	5.0037775±0.0000048	0.06608^+0.00098 _−0.0011	1,749⁺²⁶ ₋₃₀	transit	1,115	1.536^+0.069 _−0.076	6,460⁺¹³⁰ ₋₁₅₀	^[106]
TOI-674b	0.0739±0.0104	0.470±0.016	1.977143±0.000003	0.0231±0.0007	661±14	transit	150.86±0.11	0.442±0.007	3,505⁺²⁸ ₋₃₂	^[107] Possibly steam atmosphere^[108]
TOI-712 b	0.0176	0.183^+0.011 _−0.007	9.531361^+0.000018 _−0.000017	0.07928^+0.00096 _−0.00091	650.0^+6.0 _−5.9	transit	191.2±0.4	0.732^+0.027 _−0.025	4622⁺⁶¹ ₋₅₉	^[109]
TOI-712 c	0.0274	0.241^+0.008 _−0.007	51.69906±0.00017	0.2447^+0.0030 _−0.0028	369.9^+3.4 _−3.3	transit	191.2±0.4	0.732^+0.027 _−0.025	4622⁺⁶¹ ₋₅₉	^[109]
TOI-712 d	0.0236	0.221^+0.008 _−0.007	84.83960^+0.00043 _−0.00040	0.3405^+0.0041 _−0.0039	313.6^+2.9 _−2.8	transit	191.2±0.4	0.732^+0.027 _−0.025	4622⁺⁶¹ ₋₅₉	^[109]
TOI-942 b		0.347^+0.022 _−0.020	4.32421±0.000019	0.04866^+0.00016 _−0.00013		transit	493.9±1.0	0.8220^+0.0079 _−0.0064		^[110]
TOI-942 c		0.417^+0.030 _−0.027	10.156272^+0.000037 _−0.000034	0.08598^+0.00027 _−0.00022		transit	493.9±1.0	0.8220^+0.0079 _−0.0064		^[110]
TOI 1062 b	0.0320±0.0026	0.202±0.008	4.11412^+0.0014 _−0.0015	0.052	1,077⁺¹⁰ ₋₉	transit	268.7±0.2	0.94±0.02	5,328±56	^[111]
TOI 1062 c	0.0294±0.0039		7.978^+0.021 _−0.023	0.080^+0.013 _−0.012	859⁺⁹ ₋₈	radial vel.	268.7±0.2	0.94±0.02	5,328±56	^[111]
TOI-1201 b	0.0198±0.0027	0.216±0.008	2.4919863^+0.0000030 _−0.0000031	0.0287±0.0012	703⁺¹⁵ ₋₁₄	transit	122.77±0.10	0.512±0.020	3,476±51	Belongs to theHyades, also red dwarf in the system.^[112]
TOI 1227 b		0.854^+0.067 _−0.052	27.36397±0.00011	0.0886^+0.0054 _−0.0057		transit	329.3±0.8	0.170±0.015	3,072±74	^[113]
TOI-1231 b	0.0485±0.0104	0.326±0.014	24.245586^+0.000064 _−0.000066	0.1288^+0.0021 _−0.0022	330	transit	89.68±0.04	0.485±0.024	3,553±31	^[114]
TOI-1238b	0.0183±0.0035	0.108±0.010	0.764596^+0.000016 _−0.000013	0.0139±0.0008	1133±167	transit	2030.44±0.20	0.59±0.02	4089±54	^[115]
TOI-1238c	0.0262±0.0059	0.188±0.013	3.294733^+0.000040 _−0.000047	0.037±0.002	695±105	transit	2030.44±0.20	0.59±0.02	4089±54	^[115]
TOI-1259Ab	0.441^+0.049 _−0.047	1.022^+0.030 _−0.037	3.4779780^+0.0000019 _−0.0000017	0.04070^+0.00114 _−0.00110	936	transit	385±1	0.68^+0.1 _−0.01	4,775±100	Alsowhite dwarf on a wide orbit^[116]
TOI-1260 b	0.0271^+0.0043 _−0.0037	0.208^+0.009 _−0.008	3.12748^+0.000047 _−0.000038	0.0366^+0.0022 _−0.0036	860⁺⁴⁷ ₋₃₁	transit	239.5±0.3	0.66±0.01	4,227±85	^[117]
TOI-1260 c	0.0373^+0.0106 _−0.0102	0.252±0.013	7.49325^+0.00015 _−0.00013	0.0656^+0.0039 _−0.0065	643⁺³⁵ ₋₂₃	transit	239.5±0.3	0.66±0.01	4,227±85	^[117]
TOI-1296b	0.298±0.039	1.231±0.031	3.9443715±0.0000058	0.0497^+0.0023 _−0.0028	1,562⁺⁴³ ₋₃₁	transit	1,023±4	1.17±0.14	5,603±47	^[118]
TOI-1298b	0.356±0.032	0.841±0.021	4.537164±0.000012	0.0590±0.0023	1,388±24	transit	1,041±7	1.44±0.10	5,889±43	^[118]
TOI-1333 b	2.37±0.24	1.396^+0.056 _−0.054	4.720219±0.000011	0.0626^+0.0011 _−0.0012	1,679⁺³⁵ ₋₃₄	transit	653	1.464^+0.076 _−0.079	6,274±97	Host star also known as BD+47 3521A.^[106]
TOI-1431 b	3.14^+0.19 _−0.18	1.51±0.06	2.65022±0.00001	0.047±0.002	2,370±100	transit	488±3	1.90^+0.10 _−0.08	7,690⁺⁴⁰⁰ ₋₂₅₀	Also known as MASCARA-5b^[119]^[120]
TOI-1444 b	0.0122±0.0022	0.125±0.006	0.4702694±0.0000044	0.1288^+0.0021 _−0.0022	330	transit	408.9±0.5	0.934±0.038	5,430±90	^[121]
TOI-1478 b	0.847^+0.052 _−0.048	1.061^+0.040 _−0.038	10.180249±0.000015	0.0903^+0.0018 _−0.0013	918±11	transit	498	0.946^+0.059 _−0.041	5,595⁺⁸³ ₋₈₁	^[106]
TOI-1518 b	2.3	1.875±0.053	1.902603±0.000011	0.0389±0.0011	3,237±59	transit	742±6	1.79±0.26	7,300±100	^[12]
TOI-1601 b	0.99±0.11	1.239^+0.046 _−0.039	5.331751±0.000011	0.06864^+0.00079 _−0.00075	1,619⁺²⁴ ₋₂₃	transit	1,096	1.517^+0.053 _−0.049	5,948⁺⁸⁷ ₋₈₉	^[106]
TOI-1634 b	0.0313±0.0030	0.158±0.007	0.9893457±0.0000034	0.01491±0.00015	921±21	transit	114.40±0.08	0.452±0.014	3,472±48	^[122]^[123]
TOI-1685 b	0.0121±0.030	0.131±0.006	0.6691425±0.0000037	0.01156±0.00009	1,052±21	transit	122.68±0.09	0.495±0.019	3,434±51	^[124]^[122] Host star also known as UCAC4 666-026266
TOI-1685 c	0.0290±0.0065		9.025^+0.104 _−0.119		449.1±6.9	radial vel.	122.68±0.09	0.495±0.019	3,434±51	Unconfirmed^[124]
TOI-1749 b	0.060^+0.07 _−0.04	0.124±0.018	2.388821^+0.000057 _−0.000073	0.0291±0.0005	831±18	transit	324.8±0.4	0.58±0.03	3,985±55	^[125]
TOI-1749 c	0.007^+0.018 _−0.005	0.189±0.011	4.489010^+0.000040 _−0.000061	0.0443±0.0008	673±15	transit	324.8±0.4	0.58±0.03	3,985±55	^[125]
TOI-1749 d	0.014^+0.020 _−0.011	0.225±0.013	9.04455±0.00012	0.0707±0.0012	533±12	transit	324.8±0.4	0.58±0.03	3,985±55	^[125]
TOI-1789 b	0.70±0.16	1.40^+0.22 _−0.13	3.208666±0.000016	0.04873^+0.00065 _−0.0016	1,929⁺²⁸ ₋₁₈	transit	729±3	1.499^+0.061 _−0.15	5,984⁺⁵⁵ ₋₅₇	^[126]
TOI-1807 b [it]	0.0071^+0.0015 _−0.0018	0.165±0.004	0.549372±0.000007	0.0135^+0.0013 _−0.0022	1499⁺⁸² ₋₁₂₉	transit	133.88±0.25	0.750^+0.025 _−0.024	4757⁺⁵¹ ₋₅₀	Star is co-moving with TOI-2076^[127]^[128]
TOI-1842b	0.214^+0.040 _−0.038	1.04^+0.06 _−0.05	9.5739^+0.0002 _−0.0001	0.01001±0.0007		transit	729±7	1.46±0.03	6230±50	^[129]
TOI-2076 b		0.293±0.038	10.35566±0.00006	0.0631±0.0027	870±13	transit	136.70±0.23	0.850^+0.025 _−0.026	5187⁺⁵⁴ ₋₅₃	Star is co-moving with TOI-1807^[127]
TOI-2076 c		0.396±0.004	21.01538^+0.00084 _−0.00074	0.0885±0.0038	734±11	transit	136.70±0.23	0.850^+0.025 _−0.026	5187⁺⁵⁴ ₋₅₃	^[130] Star is co-moving with TOI-1807^[127]
TOI-2076 d		0.370±0.006	25.0893±0.01	0.1138^+0.0048 _−0.0049	648±10	transit	136.70±0.23	0.850^+0.025 _−0.026	5187⁺⁵⁴ ₋₅₃	Star is co-moving with TOI-1807^[127]
TOI-2109b	5.02±0.75	1.347±0.047	0.67247414±0.00000028	0.01791±0.00065	3631±69	transit	846±9	1.447^+0.075 _−0.078	6530⁺¹⁶⁰ ₋₁₅₀	^[131]
TOI-2184 b	0.65±0.16	1.017±0.051	6.90683±0.00009			transit	2,515±22	1.53±0.12	5,966±136	^[132]
TOI-2202 b	0.927^+0.047 _−0.048	1.01^+0.522 _−0.080	11.9108^+0.0009 _−0.0009	0.0956^+0.0015 _−0.0016		transit	770±3	0.823^+0.027 _−0.023	5,144±50	^[133]
TOI-2202 c	0.191^+0.033 _−0.030		24.7545^+0.0073 _−0.0078	0.1558^+0.0025 _−0.0026		timing	770±3	0.823^+0.027 _−0.023	5,144±50	^[133]
TOI-2257 b		0.196±0.010	35.189346	0.145±0.003	256⁺⁶¹ ₋₁₇	transit	188.5±0.3	0.33±0.02	3430±130	Habitable zone planet^[134]
TOI-2285b		0.155±0.007	27.26955^+0.00013 _−0.00010	0.1363±0.0010	284±6	transit	138.34±0.14	0.454±0.010	3,491±58	^[135]
TOI-2406b	0.0286^+0.0223 _−0.0126	0.263^+0.015 _−0.014	3.0766896±0.0000065	0.0228±0.0016	447±15	transit	181.4±0.4	0.162±0.008	3,100±75	^[136]
TOI-3362b	5.029^+0.668 _−0.646	1.142^+0.043 _−0.041	18.09547±0.00003	0.153^+0.002 _−0.003		transit	1,198±18	1.445^+0.069 _−0.073	6,532⁺⁸⁸ ₋₈₆	High eccentricity orbit^[137]
Upsilon Leonis b	0.51^+0.06 _−0.26		385.2^+2.8 _−1.3	1.18^+0.11 _−0.32		radial vel.	177.8	1.48^+0.90 _−0.38	4836	^[20]

Former candidate

[edit]

YSES 2 b had been thought to be a planet after the discovery by direct imaging.^[138] Later analysis in 2025 showed that it is a background M-dwarf star instead.^[139]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]

List of exoplanets discovered before 2000 (31)
List of exoplanets discovered between 2000–2009 (375)
List of exoplanets discovered in 2010 (109)
List of exoplanets discovered in 2011 (179)
List of exoplanets discovered in 2012 (149)
List of exoplanets discovered in 2013 (149)
List of exoplanets discovered in 2014 (869)
List of exoplanets discovered in 2015 (144)
List of exoplanets discovered in 2016 (1498)
List of exoplanets discovered in 2017 (152)
List of exoplanets discovered in 2018 (300)
List of exoplanets discovered in 2019 (170)
List of exoplanets discovered in 2020 (247)
List of exoplanets discovered in 2021 (254)
List of exoplanets discovered in 2022 (313)
List of exoplanets discovered in 2023 (307)
List of exoplanets discovered in 2024 (285)
List of exoplanets discovered in 2025 (107)

References

[edit]

^Gaidos, E.; Hirano, T.; Kraus, A. L.; Kuzuhara, M.; Zhang, Z.; Lee, R. A.; Salama, M.; Berger, T. A.; Grunblatt, S. K.; Ansdell, M.; Liu, M. C.; Harakawa, H.; Hodapp, K. W.; Jacobson, S.; Konishi, M.; Kotani, T.; Kudo, T.; Kurokawa, T.; Nishikawa, J.; Omiya, M.; Serizawa, T.; Tamura, M.; Ueda, A.; Vievard, S. (2021)."Zodiacal Exoplanets in Time (ZEIT) XII: A Directly-Imaged Planetary-Mass Companion to a Young Taurus M Dwarf Star".Monthly Notices of the Royal Astronomical Society.512 (1):583–601.arXiv:2110.08655.Bibcode:2022MNRAS.512..583G.doi:10.1093/mnras/stab3069.
^"Astronomers Discover Infant Planet – One of the Youngest Exoplanets Ever Observed". 23 October 2021.Archived from the original on 25 October 2021. Retrieved25 October 2021.
^"2M0437 b - Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved3 December 2023.
^Janson, Markus; Gratton, Raffaele; Rodet, Laetitia; Vigan, Arthur; Bonnefoy, Mickaël; Delorme, Philippe; Mamajek, Eric E.; Reffert, Sabine; Stock, Lukas; Marleau, Gabriel-Dominique; Langlois, Maud; Chauvin, Gaël; Desidera, Silvano; Ringqvist, Simon; Mayer, Lucio; Viswanath, Gayathri; Squicciarini, Vito; Meyer, Michael R.; Samland, Matthias; Petrus, Simon; Helled, Ravit; Kenworthy, Matthew A.; Quanz, Sascha P.; Biller, Beth; Henning, Thomas; Mesa, Dino; Engler, Natalia; Carson, Joseph C. (2021). "A wide-orbit giant planet in the high-mass b Centauri binary system".Nature.600 (7888):231–234.arXiv:2112.04833.Bibcode:2021Natur.600..231J.doi:10.1038/s41586-021-04124-8.PMID 34880428.S2CID 245005994.
^^a ^b ^c ^d ^e ^fDalal, S.; et al. (2021). "The SOPHIE search for northern extrasolar planets".Astronomy & Astrophysics.651: A11.arXiv:2105.09741.Bibcode:2021A&A...651A..11D.doi:10.1051/0004-6361/202140712.S2CID 234790136.
^Faherty, Jacqueline K.; et al. (1 December 2021)."A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9".The Astrophysical Journal.923 (1): 48.arXiv:2112.04678.Bibcode:2021ApJ...923...48F.doi:10.3847/1538-4357/ac2499.ISSN 0004-637X.S2CID 245005964.
^Zhang, Zhoujian; Liu, Michael C.; Claytor, Zachary R.; Best, William M. J.; Dupuy, Trent J.; Siverd, Robert J. (2021), "The Second Discovery from the COCONUTS Program: A Cold Wide-orbit Exoplanet around a Young Field M Dwarf at 10.9 pc",The Astrophysical Journal Letters,916 (2): L11,arXiv:2107.02805,Bibcode:2021ApJ...916L..11Z,doi:10.3847/2041-8213/ac1123,S2CID 236464073
^Kirkpatrick, J. Davy; Cushing, Michael C.; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Mainzer, Amanda K.; Eisenhardt, Peter R.; McLean, Ian S.; Thompson, Maggie A.; Bauer, James M.; Benford, Dominic J.; Bridge, Carrie R.; Lake, Sean E. (1 December 2011). "The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)".The Astrophysical Journal Supplement Series.197 (2): 19.arXiv:1108.4677.Bibcode:2011ApJS..197...19K.doi:10.1088/0067-0049/197/2/19.ISSN 0067-0049.
^^a ^b ^c ^d ^e ^fAdams, Elisabeth R.; et al. (1 August 2021)."Ultra-short-period Planets in K2. III. Neighbors are Common with 13 New Multiplanet Systems and 10 Newly Validated Planets in Campaigns 0–8 and 10".The Planetary Science Journal.2 (4): 152.arXiv:2011.11698.Bibcode:2021PSJ.....2..152A.doi:10.3847/PSJ/ac0ea0.ISSN 2632-3338.
^"Open Exoplanet Catalogue - EPIC 201427007 b".openexoplanetcatalogue.com. Retrieved24 November 2023.
^"Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved24 November 2023.
^^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 ^akDe Leon, J. P.; et al. (2021)."37 New Validated Planets in Overlapping K2 Campaigns".Monthly Notices of the Royal Astronomical Society.508:195–218.arXiv:2108.05621.doi:10.1093/mnras/stab2305.
^Kovacs, Geza (2020). "More planetary candidates from K2 Campaign 5 using TRAN_K2".Astronomy & Astrophysics.643: A169.arXiv:2008.10075.Bibcode:2020A&A...643A.169K.doi:10.1051/0004-6361/202038726.S2CID 221266076.
^^a ^b ^c ^dCastro-González, A.; et al. (2022),"The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18",Monthly Notices of the Royal Astronomical Society,509:1075–1095,arXiv:2109.03346,doi:10.1093/mnras/stab2669
^"Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved24 November 2023.
^"Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved24 November 2023.
^"Exoplanet-catalog – Exoplanet Exploration: Planets Beyond our Solar System".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved24 November 2023.
^"Exoplanet-catalog – Exoplanet Exploration: Planets Beyond our Solar System".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved24 November 2023.
^^a ^b ^cAmado, Pedro J.; Bauer, Florian F.; Rodríguez López, Cristina; Rodríguez, Eloy; Cardona Guillén, C.; Perger, M.; Caballero, José A.; López-González, Maria J.; Muñoz Rodríguez, I.; Pozuelos, F. J.; Sánchez-Rivero, A.; Schlecker, M.; Quirrenbach, Andreas; Ribas, Ignasi; Reiners, Ansgar; Almenara, J.; Astudillo-Defru, N.; Azzaro, M.; Béjar, Victor J. S.; Bohemann, R.; Bonfils, X.; Bouchy, F.; Cifuentes, C.; Cortés-Contreras, M.; Delfosse, Xavier; Dreizler, Stefan; Forveille, Thierry; Hatzes, Artie P.; Henning, Thomas K.; Jeffers, Sandra V.; Kaminski, Adrian; Kürster, Martin; Lafarga, M.; Lodieu, Nicolas; Lovis, C.; Mayor, M.; Montes, David; Morales, Juan Carlos; Morales, Nicolás; Murgas, F.; Ortiz, José L.; Pepe, F.; Perdelwitz, V.; Pollaco, D.; Santos, N. C.; Schöfer, P.; Schweitzer, A.; Ségransan, N. C.; Shan, Y.; Stock, S.; Tal-Or, Lev; Udry, S.; Zapatero-Osorio, María Rosa; Zechmeister, Mathias (28 May 2021). "The CARMENES search for exoplanets around M dwarfs".Astronomy & Astrophysics.650: A188.arXiv:2105.13785.doi:10.1051/0004-6361/202140633.S2CID 235248027.
^^a ^b ^c ^d ^e ^f ^g ^hTeng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro (2021). "Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate".Publications of the Astronomical Society of Japan.74:92–127.arXiv:2112.07169.doi:10.1093/pasj/psab112.
^Lillo-Box, J.; et al. (2021), "HD 22496 b: The first ESPRESSO stand-alone planet discovery",Astronomy & Astrophysics,654: A60,arXiv:2109.00226,Bibcode:2021A&A...654A..60L,doi:10.1051/0004-6361/202141714,S2CID 237371680
^Lam, Kristine W. F.; et al. (2021). "GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star".Science.374 (6572):1271–1275.arXiv:2112.01309.Bibcode:2021Sci...374.1271L.doi:10.1126/science.aay3253.PMID 34855492.S2CID 244799656.
^Trifonov, T.; et al. (2021). "A nearby transiting rocky exoplanet that is suitable for atmospheric investigation".Science.371 (6533):1038–1041.arXiv:2103.04950.Bibcode:2021Sci...371.1038T.doi:10.1126/science.abd7645.PMID 33674491.S2CID 232124642.
^Toledo-Padrón, B.; et al. (2021). "A super-Earth on a close-in orbit around the M1V star GJ 740".Astronomy & Astrophysics.648: A20.arXiv:2102.09441.doi:10.1051/0004-6361/202040099.S2CID 231951695.
^Maldonado, J.; et al. (2021). "HADES RV programme with HARPS-N at TNG".Astronomy & Astrophysics.651: A93.arXiv:2105.06155.Bibcode:2021A&A...651A..93M.doi:10.1051/0004-6361/202141141.S2CID 234482717.
^^a ^b ^c ^d ^e ^f ^gBakos, G. á.; Hartman, J. D.; Bhatti, W.; Csubry, Z.; Penev, K.; Bieryla, A.; Latham, D. W.; Quinn, S.; Buchhave, L. A.; Kovács, G.; Torres, Guillermo; Noyes, R. W.; Falco, E.; Béky, Bence; Szklenár, T. (1 July 2021)."HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars*".The Astronomical Journal.162 (1): 31.arXiv:2007.05528.Bibcode:2021AJ....162....7B.doi:10.3847/1538-3881/abf637.ISSN 0004-6256.
^^a ^b ^c ^dJordán, A.; et al. (2022)."HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs".The Astronomical Journal.163 (3): 125.arXiv:2112.01928.Bibcode:2022AJ....163..125J.doi:10.3847/1538-3881/ac4a77.S2CID 244896205.
^^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^mRosenthal, Lee J.; et al. (2021)."The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades".The Astrophysical Journal Supplement Series.255 (1): 8.arXiv:2105.11583.Bibcode:2021ApJS..255....8R.doi:10.3847/1538-4365/abe23c.S2CID 235186973.
^^a ^bSozzetti, A.; et al. (2021). "A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)".Astronomy & Astrophysics.648: A75.arXiv:2101.12300.Bibcode:2021A&A...648A..75S.doi:10.1051/0004-6361/202040034.S2CID 231728514.
^^a ^bMayor, M.; et al. (2011), "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets",arXiv:1109.2497 [astro-ph.EP]
^^a ^bAhrer, E.; et al. (2021)."The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection".Monthly Notices of the Royal Astronomical Society.503 (1):1248–1263.arXiv:2102.03387.Bibcode:2021MNRAS.503.1248A.doi:10.1093/mnras/stab373.
^^a ^b ^cJeong, G.; Lee, B. C.; Park, M. G.; Bang, T. Y.; Han, I. (2022). "Search for exoplanets around northern circumpolar stars".Astronomy & Astrophysics.662: A12.arXiv:2111.08899.doi:10.1051/0004-6361/202142379.S2CID 244270271.
^^a ^b ^c ^d ^e ^fDemangeon, O. D. S.; et al. (2021), "The SOPHIE search for northern extrasolar planets",Astronomy & Astrophysics,653: A78,arXiv:2107.05089,Bibcode:2021A&A...653A..78D,doi:10.1051/0004-6361/202141079,S2CID 235795175
^Hobson, Melissa J.; et al. (2021)."A Transiting Warm Giant Planet around the Young Active Star TOI-201".The Astronomical Journal.161 (5): 235.arXiv:2103.02685.Bibcode:2021AJ....161..235H.doi:10.3847/1538-3881/abeaa1.S2CID 232110390.
^^a ^bScarsdale, Nicholas; et al. (2021)."TESS-Keck Survey. V. Twin Sub-Neptunes Transiting the Nearby G Star HD 63935".The Astronomical Journal.162 (5): 215.arXiv:2110.06885.Bibcode:2021AJ....162..215S.doi:10.3847/1538-3881/ac18cb.S2CID 238743956.
^^a ^bBarragán, O.; et al. (2022)."The young HD 73583 (TOI-560) planetary system: Two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf".Monthly Notices of the Royal Astronomical Society.514 (2):1606–1627.arXiv:2110.13069.doi:10.1093/mnras/stac638.
^Zhang, Michael; Knutson, Heather A.; Wang, Lile; Dai, Fei; Barragán, Oscar (2022)."Escaping Helium from TOI 560.01, a Young Mini-Neptune".The Astronomical Journal.163 (2): 67.arXiv:2110.13150.Bibcode:2022AJ....163...67Z.doi:10.3847/1538-3881/ac3fa7.S2CID 239885237.
^^a ^bEl Mufti, Mohammed; et al. (1 January 2023)."TOI 560: Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS, and HIRES RVs".The Astronomical Journal.165 (1): 10.arXiv:2112.13448.Bibcode:2023AJ....165...10E.doi:10.3847/1538-3881/ac9834.ISSN 0004-6256.
^"HD 108236 f".Extrasolar Planets Encyclopaedia. 3 December 1995. Retrieved4 January 2021.
^Bonfanti, A.; et al. (2021), "CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii",Astronomy & Astrophysics,646: A157,arXiv:2101.00663,Bibcode:2021A&A...646A.157B,doi:10.1051/0004-6361/202039608,S2CID 230437723
^^a ^bSreenivas, K. R.; Perdelwitz, V.; Tal-Or, L.; Trifonov, T.; Zucker, S.; Mazeh, T. (2022). "Analysis of the public HARPS/ESO spectroscopic archive".Astronomy & Astrophysics.660: A124.arXiv:2112.09029.doi:10.1051/0004-6361/202142612.S2CID 245219286.
^Tofflemire, Benjamin M.; et al. (2021)."TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association".The Astronomical Journal.161 (4): 171.arXiv:2102.06066.Bibcode:2021AJ....161..171T.doi:10.3847/1538-3881/abdf53.S2CID 231879915.
^^a ^bOsborn, H. P.; et al. (2021)."A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113".Monthly Notices of the Royal Astronomical Society.502 (4):4842–4857.arXiv:2101.04745.Bibcode:2021MNRAS.502.4842O.doi:10.1093/mnras/stab182.
^^a ^bAzevedo Silva, T.; et al. (2022). "The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter".Astronomy & Astrophysics.657: A68.arXiv:2111.08764.Bibcode:2022A&A...657A..68A.doi:10.1051/0004-6361/202141520.S2CID 243809625.
^^a ^bEisner, N. L.; et al. (2021)."Planet Hunters TESS III: Two transiting planets around the bright G dwarf HD 152843".Monthly Notices of the Royal Astronomical Society.505 (2):1827–1840.arXiv:2106.04603.doi:10.1093/mnras/stab1253.
^Palatnick, Skyler; et al. (2021)."Validation of HD 183579b Using Archival Radial Velocities: A Warm Neptune Orbiting a Bright Solar Analog".The Astrophysical Journal Letters.909 (1): L6.arXiv:2101.12137.Bibcode:2021ApJ...909L...6P.doi:10.3847/2041-8213/abe0bb.S2CID 231719821.
^Gan, Tianjun; et al. (2021)."HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS".Monthly Notices of the Royal Astronomical Society.507 (2):2220–2240.arXiv:2107.14015.doi:10.1093/mnras/stab2224.
^Bonfanti, A.; et al. (2023). "TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS".Astronomy & Astrophysics.671: L8.arXiv:2302.10664.Bibcode:2023A&A...671L...8B.doi:10.1051/0004-6361/202245607.S2CID 257050671.
^Lubin, Jack; et al. (2022),"TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion",The Astronomical Journal,163 (2): 101,arXiv:2108.02208,Bibcode:2022AJ....163..101L,doi:10.3847/1538-3881/ac3d38,S2CID 236924440
^Orell-Miquel, J. (2023). "HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone".Astronomy & Astrophysics.669: A40.arXiv:2211.00667.Bibcode:2023A&A...669A..40O.doi:10.1051/0004-6361/202244120.S2CID 253197272.
^Heidari, N.; et al. (2022). "HD 207897 b: A dense sub-Neptune transiting a nearby and bright K-type star".Astronomy & Astrophysics.658: A176.arXiv:2110.08597.Bibcode:2022A&A...658A.176H.doi:10.1051/0004-6361/202141429.S2CID 239016573.
^^a ^b ^cParedes, Leonardo A.; Henry, Todd J.; Quinn, Samuel N.; Gies, Douglas R.; Hinojosa-Goñi, Rodrigo; James, Hodari-Sadiki; Jao, Wei-Chun; White, Russel J. (2021)."The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance".The Astronomical Journal.162 (5): 176.arXiv:2111.15028.Bibcode:2021AJ....162..176P.doi:10.3847/1538-3881/ac082a.S2CID 237285778.
^Jones, M. I.; Wittenmyer, R.; Aguilera-Gómez, C.; Soto, M. G.; Torres, P.; Trifonov, T.; Jenkins, J. S.; Zapata, A.; Sarkis, P.; Zakhozhay, O.; Brahm, R.; Ramírez, R.; Santana, F.; Vines, J. I.; Díaz, M. R.; Vučković, M.; Pantoja, B. (2021), "Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS",Astronomy & Astrophysics,646: A131,arXiv:2006.01277,Bibcode:2021A&A...646A.131J,doi:10.1051/0004-6361/202038555,S2CID 219179316
^^a ^bFeng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A.; Bailey, J.; Burt, Jennifer; Carter, B. D.; Crane, Jeffrey D.; Dotti, Francesco Flammini; Holden, Bradford; Ma, Bo; Ogihara, Masahiro; Oppenheimer, Rebecca; O’Toole, S. J.; Shectman, Stephen A.; Wittenmyer, Robert A.; Wang, Sharon X.; Wright, D. J.; Xuan, Yifan (1 September 2022)."3D Selection of 167 Substellar Companions to Nearby Stars".The Astrophysical Journal Supplement Series.262 (1): 21.arXiv:2208.12720.Bibcode:2022ApJS..262...21F.doi:10.3847/1538-4365/ac7e57.ISSN 0067-0049.
^Jones, M. I.; Wittenmyer, R.; Aguilera-Gómez, C.; Soto, M. G.; Torres, P.; Trifonov, T.; Jenkins, J. S.; Zapata, A.; Sarkis, P.; Zakhozhay, O.; Brahm, R.; Ramírez, R.; Santana, F.; Vines, J. I.; Díaz, M. R. (February 2021)."Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS"(PDF).Astronomy & Astrophysics.646: A131.arXiv:2006.01277.Bibcode:2021A&A...646A.131J.doi:10.1051/0004-6361/202038555.ISSN 0004-6361.S2CID 219179316.
^"HIP 90988 b - Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved4 December 2023.
^^a ^bMacDougall, Mason G.; et al. (2021)."The TESS–Keck Survey. VI. Two Eccentric Sub-Neptunes Orbiting HIP-97166".The Astronomical Journal.162 (6): 265.arXiv:2110.05628.Bibcode:2021AJ....162..265M.doi:10.3847/1538-3881/ac295e.S2CID 238634523.
^Smith, A M S.; et al. (2021)."K2-99 revisited: A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant".Monthly Notices of the Royal Astronomical Society.510 (4):5035–5049.arXiv:2111.14660.Bibcode:2022MNRAS.510.5035S.doi:10.1093/mnras/stab3497.
^Zhang, Jingwen; et al. (2021)."Long-period Jovian Tilts the Orbits of Two sub-Neptunes Relative to Stellar Spin Axis in Kepler-129".The Astronomical Journal.162 (3): 89.arXiv:2105.03446.Bibcode:2021AJ....162...89Z.doi:10.3847/1538-3881/ac0634.S2CID 234338914.
^Dalba, Paul A.; et al. (2021),"Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit",The Astronomical Journal,162 (4): 154,arXiv:2107.06901,Bibcode:2021AJ....162..154D,doi:10.3847/1538-3881/ac134b,S2CID 235898945
^^a ^b ^cLillo-Box, J.; et al. (2021), "Follow-up of non-transiting planets detected by Kepler",Astronomy & Astrophysics,654: A9,arXiv:2107.14621,doi:10.1051/0004-6361/202140746,S2CID 236635201
^Ryu, Yoon-Hyun; et al. (2021)."Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605".The Astronomical Journal.162 (3): 96.arXiv:2104.07906.Bibcode:2021AJ....162...96R.doi:10.3847/1538-3881/ac062a.S2CID 233289612.
^^a ^b ^cHan, Cheongho; et al. (2021). "Three faint-source microlensing planets detected via the resonant-caustic channel".Astronomy & Astrophysics.655: A21.arXiv:2109.07068.Bibcode:2021A&A...655A..21H.doi:10.1051/0004-6361/202141517.S2CID 237513708.
^Han, Cheongho; et al. (2021). "KMT-2018-BLG-1025Lb: Microlensing super-Earth planet orbiting a low-mass star".Astronomy & Astrophysics.649: A90.arXiv:2102.01890.Bibcode:2021A&A...649A..90H.doi:10.1051/0004-6361/202039817.S2CID 231786450.
^Han, Cheongho; et al. (2021), "KMT-2018-BLG-1743: Planetary microlensing event occurring on two source stars",Astronomy & Astrophysics,652: A145,arXiv:2107.00155,Bibcode:2021A&A...652A.145H,doi:10.1051/0004-6361/202140923,S2CID 235694685
^^a ^b ^cHan, Cheongho; et al. (2021). "Three microlensing planets with no caustic-crossing features".Astronomy & Astrophysics.650: A89.arXiv:2104.06544.Bibcode:2021A&A...650A..89H.doi:10.1051/0004-6361/202140758.S2CID 233231384.
^Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Youn Kil Jung; Kim, Doeon; Lee, Chung-Uk; Mao, Shude; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Kim, Chun-Hwey (2022). "KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf".Astronomy & Astrophysics.658: A62.arXiv:2111.08955.Bibcode:2022A&A...658A..62H.doi:10.1051/0004-6361/202142077.S2CID 244270928.
^Yun Hak Kim; et al. (2021)."KMT-2019-BLG-0371 and the Limits of Bayesian Analysis".The Astronomical Journal.162 (1): 17.arXiv:2101.12206.Bibcode:2021AJ....162...17K.doi:10.3847/1538-3881/abf930.S2CID 231728667.
^^a ^b ^c ^d ^eHwang, Kyu-Ha; et al. (2021),"Systematic KMTNet Planetary Anomaly Search, Paper II: Five New q<2×10−4 Mass-ratio Planets",The Astronomical Journal,arXiv:2106.06686,doi:10.3847/1538-3881/ac38ad,S2CID 245740102
^Han, Cheongho; et al. (2021)."KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars".The Astronomical Journal.161 (6): 270.arXiv:2104.00293.Bibcode:2021AJ....161..270H.doi:10.3847/1538-3881/abf4d0.S2CID 232478488.
^Zang, Weicheng; et al. (2021), "An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb",Research in Astronomy and Astrophysics,21 (9): 239,arXiv:2103.01896,Bibcode:2021RAA....21..239Z,doi:10.1088/1674-4527/21/9/239,S2CID 232092272
^Han, Cheongho; et al. (2022). "KMT-2021-BLG-0912Lb: A microlensing super Earth around a K-type star".Astronomy & Astrophysics.658: A94.arXiv:2111.04861.Bibcode:2022A&A...658A..94H.doi:10.1051/0004-6361/202142495.S2CID 243860989.
^Hirsch, Lea A.; et al. (2017)."ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST".The Astronomical Journal.153 (3): 117.arXiv:1701.06577.Bibcode:2017AJ....153..117H.doi:10.3847/1538-3881/153/3/117.S2CID 39321033.
^"AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE"(PDF).Archived(PDF) from the original on 15 January 2021. Retrieved18 January 2021.
^Sun, Leilei; Ioannidis, Panagiotis; Gu, Shenghong; Schmitt, Jürgen H. M. M.; Wang, Xiaobin; Kouwenhoven, M. B. N.; Perdelwitz, Volker; Francesco Flammini Dotti; Czesla, Stefan (2022)."A highly mutually inclined compact warm-Jupiter system KOI-984?".Monthly Notices of the Royal Astronomical Society.512 (3):4604–4617.arXiv:2111.09668.doi:10.1093/mnras/stab3367.
^Cañas, Caleb I.;Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A.; Diddams, Scott A.; Endl, Michael; Ford, Eric B.; Halverson, Samuel; Hearty, Fred; Jones, Sinclaire; Kanodia, Shubham; Lin, Andrea S. J.; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Stefánsson, Guđmundur (2022)."A Hot Mars-sized Exoplanet Transiting an M Dwarf".The Astronomical Journal.163 (1): 3.arXiv:2112.03958.Bibcode:2022AJ....163....3C.doi:10.3847/1538-3881/ac3088.S2CID 244954104.
^Soto, M. G.; et al. (2021). "Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b)".Astronomy & Astrophysics.649: A144.arXiv:2102.11640.Bibcode:2021A&A...649A.144S.doi:10.1051/0004-6361/202140618.S2CID 232013854.
^^a ^bSilverstein, Michele L.; et al. (2022)."The LHS 1678 System: Two Earth-sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc".The Astronomical Journal.163 (4): 151.arXiv:2110.12079.Bibcode:2022AJ....163..151S.doi:10.3847/1538-3881/ac32e3.S2CID 239768873.
^Winters, Jennifer G.; Cloutier, Ryan; Medina, Amber A.; Irwin, Jonathan M.; Charbonneau, David; Astudillo-Defru, Nicola; Bonfils, Xavier; Howard, Andrew W.; Isaacson, Howard; Bean, J. L.; Seifahrt, A.; Teske, J. K.; Eastman, Jason D.; Twicken, Joseph D.; Collins, K. A.; Jensen, E. L. N.; Quinn, S. N.; Payne, M. J.; Kristiansen, M. H.; Spencer, A.; Vanderburg, Andrew; Zechmeister, Mathias; Weiss, L. M.; Wang, S. X.; Wang, G.; Udry, Stéphane; Terentev, I. A.; Sturmer, J.; Stefansson, G.; Shectman, Stephen A.; Sefako, R.; Schwengeler, H. M.; Schwarz, R. P.; Scarsdale, N.; Rubenzahl, R. A.; Roy, A.; Rosenthal, L. J.; Robertson, P.; Petigura, Erik A.; Pepe, Francesco; Omohundro, M.; Murphy, J. M. A.; Murgas, Felipe; Movcnik, T.; Montet, B. T.; Mennickent, R.; Mayo, A. W.; Massey, B.; Lubin, J.; Lovis, Christophe; Lewin, P.; Kasper, D.; Kane, S. R.; Jenkins, J. M.; Huber, D.; Horne, K.; Hill, M. L.; Gorrini, P.; Giacalone, S.; Fulton, Benjamin J.; Forveille, Thierry; Figueira, Pedro; Fetherolf, T.; Dressing, Courtney D.; Díaz, Rodrigo F.; Delfosse, Xavier; Dalba, P. A.; Dai, F.; Cortes, C. C.; Crossfield, Ian J. M.; Crane, Jeffrey D.; Conti, D. M.; Collins, K. I.; Chontos, A.; Butler, R. Paul; Brown, P.; Brady, M.; Bouchy, François; Behmard, A.; Beard, C.; Batalha, Natalie M.; Almenara, José M. (2022)."A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds".The Astronomical Journal.163 (4): 168.arXiv:2107.14737.Bibcode:2022AJ....163..168W.doi:10.3847/1538-3881/ac50a9.S2CID 236635391.
^^a ^b"A warm terrestrial planet with half the mass of Venus transiting a nearby star"(PDF).Archived(PDF) from the original on 13 November 2021. Retrieved8 August 2021.
^Grieves, Nolan; et al. (2021). "NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star".Astronomy & Astrophysics.647: A180.arXiv:2101.04245.Bibcode:2021A&A...647A.180G.doi:10.1051/0004-6361/202039586.S2CID 231582818.
^Smith, A. M. S.; et al. (2021). "NGTS-14Ab: A Neptune-sized transiting planet in the desert".Astronomy & Astrophysics.646: A183.arXiv:2101.01470.Bibcode:2021A&A...646A.183S.doi:10.1051/0004-6361/202039712.S2CID 230524042.
^^a ^b ^c ^dTilbrook, Rosanna H.; et al. (2021)."NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey".Monthly Notices of the Royal Astronomical Society.504 (4):6018–6032.arXiv:2103.10302.doi:10.1093/mnras/stab815.
^Miyazaki, Shota; et al. (2022)."OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions".The Astronomical Journal.163 (3): 123.arXiv:2112.14997.Bibcode:2022AJ....163..123M.doi:10.3847/1538-3881/ac4960.S2CID 245634898.
^Xie, Xiao-Jia; Dong, Subo; Shvartzvald, Yossi; Gould, Andrew; Udalski, Andrzej; Beaulieu, Jean-Philippe; Beichman, Charles; Close, Laird Miller; b. Henderson, Calen; r. Males, Jared; Marquette, Jean-Baptiste; m. Morzinski, Katie; r. Gelino, Christopher (2022). "Characterizing microlensing planetary system OGLE-2014-BLG-0676Lb with adaptive optics imaging".Research in Astronomy and Astrophysics.21 (12): 303.arXiv:2112.08030.doi:10.1088/1674-4527/ac2a09.S2CID 244211319.
^Wang(王涵悦), Hanyue; et al. (2022)."Systematic Korea Microlensing Telescope Network planetary anomaly search – III. One wide-orbit planet and two stellar binaries".Monthly Notices of the Royal Astronomical Society.510 (2):1778–1790.arXiv:2112.02414.doi:10.1093/mnras/stab3581.
^^a ^bKil Jung, Youn; et al. (2021)."OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel".The Astronomical Journal.161 (6): 293.arXiv:2102.07338.Bibcode:2021AJ....161..293J.doi:10.3847/1538-3881/abf8bd.S2CID 231924992.
^Kains, N.; et al. (2021). "A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251".Astronomy & Astrophysics.552: A70.arXiv:1303.1184.Bibcode:2013A&A...552A..70K.doi:10.1051/0004-6361/201220626.S2CID 43146154.
^^a ^bHan, Cheongho; et al. (2022). "OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star".Astronomy & Astrophysics.658: A93.arXiv:2111.03755.Bibcode:2022A&A...658A..93H.doi:10.1051/0004-6361/202142327.S2CID 243847948.
^Yee, Jennifer C.; et al. (2021),"OGLE-2019-BLG-0960 Lb: The Smallest Microlensing Planet",The Astronomical Journal,162 (5): 180,arXiv:2101.04696,Bibcode:2021AJ....162..180Y,doi:10.3847/1538-3881/ac1582,S2CID 231592669
^Zang, Weicheng; et al. (2021),"Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet",The Astronomical Journal,162 (4): 163,arXiv:2103.11880,Bibcode:2021AJ....162..163Z,doi:10.3847/1538-3881/ac12d4,S2CID 232307459
^Shin, In-Gu; et al. (2021),"Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058",The Astronomical Journal,162 (6): 267,arXiv:2108.02499,Bibcode:2021AJ....162..267S,doi:10.3847/1538-3881/ac2ba5,S2CID 236924486
^Kondo, Iona; et al. (2021)."OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf".The Astronomical Journal.162 (2): 77.arXiv:2104.02157.Bibcode:2021AJ....162...77K.doi:10.3847/1538-3881/ac00ba.S2CID 233033627.
^Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P.; Sawangwit, U.; Poshyachinda, S.; Reichart, D. E.; Haislip, J. B. (2021),Two circumbinary planets in RR Cae eclipsing binary system,arXiv:2109.09397
^Kostov, Veselin B.; et al. (2021),"TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data",The Astronomical Journal,162 (6): 234,arXiv:2105.08614,Bibcode:2021AJ....162..234K,doi:10.3847/1538-3881/ac223a,S2CID 234762777
^Montalto, M.; Malavolta, L.; Gregorio, J.; Mantovan, G.; Desidera, S.; Piotto, G.; Nascimbeni, V.; Granata, V.; Manthopoulou, E. E.; Claudi, R. (2022)."TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star".Monthly Notices of the Royal Astronomical Society.509 (2):2908–2919.arXiv:2110.00489.doi:10.1093/mnras/stab2923.
^^a ^b ^c ^d ^e ^fLeleu, A.; et al. (2021). "Six transiting planets and a chain of Laplace resonances in TOI-178".Astronomy & Astrophysics.649: A26.arXiv:2101.09260.Bibcode:2021A&A...649A..26L.doi:10.1051/0004-6361/202039767.S2CID 231693292.
^Hoyer, S.; et al. (2021)."TOI-220 b: A warm sub-Neptune discovered by TESS".Monthly Notices of the Royal Astronomical Society.505 (3):3361–3379.arXiv:2105.01944.doi:10.1093/mnras/stab1427.
^Cointepas, M.; et al. (2021). "TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA".Astronomy & Astrophysics.650: A145.arXiv:2104.14782.Bibcode:2021A&A...650A.145C.doi:10.1051/0004-6361/202140328.S2CID 233476660.
^^a ^b ^cOsborn, Ares; et al. (2021)."TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet".Monthly Notices of the Royal Astronomical Society.507 (2):2782–2803.arXiv:2108.02310.doi:10.1093/mnras/stab2313.
^^a ^b ^cNewton, Elisabeth R.; et al. (2021)."TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream".The Astronomical Journal.161 (2): 65.arXiv:2102.06049.Bibcode:2021AJ....161...65N.doi:10.3847/1538-3881/abccc6.S2CID 231879927.
^^a ^b ^cBarragán, Oscar; et al. (2021)."TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution".Research Notes of the American Astronomical Society.5 (3): 51.arXiv:2103.09746.Bibcode:2021RNAAS...5...51B.doi:10.3847/2515-5172/abef70.S2CID 232258104.
^Gan, Tianjun; et al. (2021)."TOI-530b: A giant planet transiting an M dwarf detected by TESS".Monthly Notices of the Royal Astronomical Society.511:83–99.arXiv:2110.04220.doi:10.1093/mnras/stab3708.
^Kanodia, Shubham; et al. (2021), "TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M-dwarf host",The Astronomical Journal,162 (4): 135,arXiv:2107.13670,Bibcode:2021AJ....162..135K,doi:10.3847/1538-3881/ac1940,S2CID 236493328
^^a ^bIkwut-Ukwa, Mma; et al. (2022),"Two Massive Jupiters in Eccentric Orbits from the TESS Full-frame Images",The Astronomical Journal,163 (1): 9,arXiv:2102.02222,Bibcode:2022AJ....163....9I,doi:10.3847/1538-3881/ac2ee1,S2CID 231802379
^^a ^b ^c ^d ^eRodriguez, Joseph E.; et al. (2021)."TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images".The Astronomical Journal.161 (4): 194.arXiv:2101.01726.Bibcode:2021AJ....161..194R.doi:10.3847/1538-3881/abe38a.S2CID 230770138.
^Murgas, F.; et al. (2021), "TOI-674b: An oasis in the desert of exo-Neptunes transiting a nearby M dwarf",Astronomy & Astrophysics,653: A60,arXiv:2106.01246,Bibcode:2021A&A...653A..60M,doi:10.1051/0004-6361/202140718,S2CID 235294286
^Brande, Jonathan; Crossfield, Ian J. M.; Kreidberg, Laura; Oklopčić, Antonija; Polanski, Alex S.; Barman, Travis; Benneke, Björn; Christiansen, Jessie L.; Dragomir, Diana; Foreman-Mackey, Daniel; Fortney, Jonathan J.; Greene, Thomas P.; Howard, Andrew W.; Knutson, Heather A.; Lothringer, Joshua D.; Mikal-Evans, Thomas; Morley, Caroline V. (2022)."A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 B".The Astronomical Journal.164 (5): 197.arXiv:2201.04197.Bibcode:2022AJ....164..197B.doi:10.3847/1538-3881/ac8b7e.S2CID 245877576.
^^a ^b ^cVach, Sydney; et al. (2022)."TOI-712: A System of Adolescent Mini-Neptunes Extending to the Habitable Zone".The Astronomical Journal.164 (2): 71.arXiv:2111.02416.Bibcode:2022AJ....164...71V.doi:10.3847/1538-3881/ac7954.S2CID 242757638.
^^a ^bWirth, Christopher P.; et al. (2021), "TOI-942b: A Prograde Neptune in a ~ 60 Myr Old Multi-transiting System",The Astrophysical Journal Letters,917 (2): L34,arXiv:2106.14968,Bibcode:2021ApJ...917L..34W,doi:10.3847/2041-8213/ac13a9,S2CID 235670113
^^a ^bOtegi, J. F.; et al. (2021), "TESS and HARPS reveal two sub-Neptunes around TOI 1062",Astronomy & Astrophysics,653: A105,arXiv:2105.01945,Bibcode:2021A&A...653A.105O,doi:10.1051/0004-6361/202040247,S2CID 233739805
^Kossakowski, D.; et al. (2021). "TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf".Astronomy & Astrophysics.656: A124.arXiv:2109.09346.Bibcode:2021A&A...656A.124K.doi:10.1051/0004-6361/202141587.S2CID 237571914.
^Mann, Andrew W.; et al. (2022)."TESS Hunt for Young and Maturing Exoplanets (THYME). VI. An 11 Myr Giant Planet Transiting a Very-low-mass Star in Lower Centaurus Crux".The Astronomical Journal.163 (4): 156.arXiv:2110.09531.Bibcode:2022AJ....163..156M.doi:10.3847/1538-3881/ac511d.S2CID 239024522.
^Burt, Jennifer A.; et al. (2021)."TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399".The Astronomical Journal.162 (3): 87.arXiv:2105.08077.Bibcode:2021AJ....162...87B.doi:10.3847/1538-3881/ac0432.S2CID 234763319.
^^a ^bGonzález-Álvarez, E.; et al. (2022). "A multi-planetary system orbiting the early-M dwarf TOI-1238".Astronomy & Astrophysics.658: A138.arXiv:2111.14602.Bibcode:2022A&A...658A.138G.doi:10.1051/0004-6361/202142128.S2CID 244715047.
^Martin, David V.; et al. (2021)."TOI-1259Ab – a gas giant planet with 2.7 per cent deep transits and a bound white dwarf companion".Monthly Notices of the Royal Astronomical Society.507 (3):4132–4148.arXiv:2101.02707.doi:10.1093/mnras/stab2129.
^^a ^bGeorgieva, I. Y.; et al. (2021)."Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260".Monthly Notices of the Royal Astronomical Society.505 (4):4684–4701.arXiv:2104.05653.doi:10.1093/mnras/stab1464.
^^a ^bMoutou, C.; et al. (2021). "TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars".Astronomy & Astrophysics.653: A147.arXiv:2109.09252.Bibcode:2021A&A...653A.147M.doi:10.1051/0004-6361/202141151.S2CID 237571683.
^Brett Christopher Addison; et al. (2021), "TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars",Posters from the Tess Science Conference Ii (Tsc2: 64,arXiv:2104.12078,Bibcode:2021tsc2.confE..64A,doi:10.5281/zenodo.5126266,S2CID 240578462
^Stangret, M.; et al. (2021), "The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions",Astronomy & Astrophysics,654: A73,arXiv:2104.12414,Bibcode:2021A&A...654A..73S,doi:10.1051/0004-6361/202040100,S2CID 233393996
^Dai, Fei; et al. (2021),"TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes",The Astronomical Journal,162 (2): 62,arXiv:2105.08844,Bibcode:2021AJ....162...62D,doi:10.3847/1538-3881/ac02bd,S2CID 234778143
^^a ^bHirano, Teruyuki; et al. (2021),"Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions",The Astronomical Journal,162 (4): 161,arXiv:2103.12760,Bibcode:2021AJ....162..161H,doi:10.3847/1538-3881/ac0fdc,S2CID 232335413
^Cloutier, R.; et al. (2021)."TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley".The Astronomical Journal.162 (2): 79.arXiv:2103.12790.Bibcode:2021AJ....162...79C.doi:10.3847/1538-3881/ac0157.S2CID 232335385.
^^a ^bBluhm, P.; et al. (2021). "An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685".Astronomy & Astrophysics.650: A78.arXiv:2103.01016.Bibcode:2021A&A...650A..78B.doi:10.1051/0004-6361/202140688.S2CID 232092636.
^^a ^b ^cFukui, A.; et al. (2021),"TOI-1749: An M dwarf with a Trio of Planets including a Near-resonant Pair",The Astronomical Journal,162 (4): 167,arXiv:2107.05430,Bibcode:2021AJ....162..167F,doi:10.3847/1538-3881/ac13a5,S2CID 235795469
^Khandelwal, Akanksha; et al. (2021),"Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789",Monthly Notices of the Royal Astronomical Society,arXiv:2106.08660,doi:10.1093/mnras/stab2970
^^a ^b ^c ^dHedges, Christina; et al. (2021)."TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow up".The Astronomical Journal.162 (2): 54.arXiv:2111.01311.Bibcode:2021AJ....162...54H.doi:10.3847/1538-3881/ac06cd.S2CID 235805026.
^Peng, Peifeng; Xiong, Hongyi; Li, He; Li, Felix; Wang, Tianqi (2022),New Parameter Measurements for the Ultra-Short-Period Planet TOI-1807b,arXiv:2210.04162
^Wittenmyer, Robert A.; et al. (2021)."TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant".The Astronomical Journal.163 (2): 82.arXiv:2112.00198.Bibcode:2022AJ....163...82W.doi:10.3847/1538-3881/ac3f39.S2CID 244773259.
^Osborn, H.; et al. (2022). "Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076".Astronomy & Astrophysics.664: A156.arXiv:2203.03194.Bibcode:2022A&A...664A.156O.doi:10.1051/0004-6361/202243065.S2CID 247292643.
^Wong, Ian; et al. (2021)."TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit".The Astronomical Journal.162 (6): 256.arXiv:2111.12074.Bibcode:2021AJ....162..256W.doi:10.3847/1538-3881/ac26bd.S2CID 244488632.
^Saunders, Nicholas; et al. (2022),"TESS Giants Transiting Giants. I.: A Noninflated Hot Jupiter Orbiting a Massive Subgiant",The Astronomical Journal,163 (2): 53,arXiv:2108.02294,Bibcode:2022AJ....163...53S,doi:10.3847/1538-3881/ac38a1,S2CID 236924647
^^a ^bTrifonov, Trifon; et al. (2021),"A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202",The Astronomical Journal,162 (6): 283,arXiv:2108.05323,Bibcode:2021AJ....162..283T,doi:10.3847/1538-3881/ac1bbe,S2CID 236976243
^Schanche, N.; et al. (2022). "TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf".Astronomy & Astrophysics.657: A45.arXiv:2111.01749.Bibcode:2022A&A...657A..45S.doi:10.1051/0004-6361/202142280.S2CID 240419956.
^Fukui, Akihiko; et al. (2021). "TOI-2285b: A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf".Publications of the Astronomical Society of Japan.74:L1 –L8.arXiv:2110.10215.doi:10.1093/pasj/psab106.
^Wells, R. D.; et al. (2021), "A large sub-Neptune transiting the thick-disk M4 V TOI-2406",Astronomy & Astrophysics,653: A97,arXiv:2107.14125,Bibcode:2021A&A...653A..97W,doi:10.1051/0004-6361/202141277,S2CID 236493492
^Dong, Jiayin; et al. (2021),"TOI-3362b: A Proto Hot Jupiter Undergoing High-eccentricity Tidal Migration",The Astrophysical Journal Letters,920 (1): L16,arXiv:2109.03771,Bibcode:2021ApJ...920L..16D,doi:10.3847/2041-8213/ac2600,S2CID 237442300
^Bohn, Alexander J.; et al. (2021). "Discovery of a directly imaged planet to the young solar analog YSES 2".Astronomy & Astrophysics.648: A73.arXiv:2104.08285.Bibcode:2021A&A...648A..73B.doi:10.1051/0004-6361/202140508.S2CID 233296087.
^Kenworthy, Matthew; Stolker, Tomas; Kammerer, Jens; Balmer, William; Vigan, Arthur; Lacour, Sylvestre; Otten, Gilles; Mamajek, Eric; Ginski, Christian; Nowak, Mathias; Martos, Steven; Wang, Jason; Rickman, Emily; Janson, Markus; Bohn, Alexander (14 August 2025)."YSES 2b is a background star. Differential astrometric M-dwarf measurements in time".Astronomy & Astrophysics.arXiv:2509.09504.doi:10.1051/0004-6361/202556170.ISSN 0004-6361.

Exoplanets

Main topics

Sizes
and
types

Terrestrial	Carbon planet Catastrophically evaporating planet Coreless planet Desert planet Dwarf planet Hycean planet Ice planet Iron planet (Super-Mercury) Lava planet Ocean world Mega-Earth Steam world Sub-Earth Super-Earth
Gaseous	Cold Jupiter Eccentric Jupiter Mini-Neptune (Gas dwarf) Helium planet Hot Jupiter Hot Neptune Gas giant Ice giant Neptunian Jupiter analogue Super-Jupiter Super-Neptune Super-puff Ultra-hot Jupiter Ultra-hot Neptune Warm Jupiter
Other types	Blanet Brown dwarf Chthonian planet Circumbinary planet Circumtriple planet Disrupted planet Double planet Ecumenopolis Eyeball planet Giant planet Mesoplanet Planemo Planet/Brown dwarf boundary Planetesimal Protoplanet Pulsar planet Sub-brown dwarf Sub-Neptune Toroidal planet Ultra-cool dwarf Ultra-short period planet (USP)

Formation
and
evolution

Catalogues

Exoplanetary systems

Exoplanets

Discovered exoplanets by year
- before 2000
- 2000–2009
- 2010
- 2011
- 2012
- 2013
- 2014
- 2015
- 2016
- 2017
- 2018
- 2019
- 2020
- 2021
- 2022
- 2023
- 2024
- 2025

Other

v t e 2021 in space
« 2020 2022 »
Space probe and telescope launches	Tiangong space stationTianhe (April 2021) Lucy (Oct 2021) DART /LICIACube (Nov 2021) James Webb Space Telescope (Dec 2021)
Impact events	Winchcombe meteorite
SelectedNEOs	Asteroid close approaches 2021 AV7 (792156) 2020 XR 2016 DV1 2021 DW1 99942 Apophis (231937) 2001 FO32 2021 GW4 2021 PH27 (620094) 2016 AJ193 2021 SG 2021 TP21 2021 UA1 (679648) 2019 XS 3361 Orpheus 1994 WR12 4660 Nereus (163899) 2003 SD220 2018 AH
Exoplanets	Alpha Centauri Ab(unconfirmed) COCONUTS-2b Gliese 486 HD 108236 f HD 110082 b Kepler-1704b KOI-5Ab L 98-59 e f? Lalande 21185 c Lambda Serpentis b LHS 1678 b c NGTS-13b NGTS-14Ab OGLE-2019-BLG-0960Lb PDS 70c circumplanetary disk TIC 172900988 b TOI-178 b c d e f g TOI-755 b c Vega b(unconfirmed) YSES 2 b
Discoveries	QSO J0313−1806 (distant quasar) ID2299 (elliptical galaxy) TIC 168789840 sextuple system V723 Mon black hole candidate 2018 AG37 (TNO)(announced) 2021 DR15 (TNO) ALESS 073.1 (spiral galaxy) PJ352–15 astrophysical jet 2MASS J0348−6022 (rapidly-rotating brown dwarf) ZTF J1901+1458 (massive white dwarf) WISE 1534–1043 (brown dwarf) 1moon of Jupiter (S/2003 J 24) 1moon of Saturn (S/2019 S 1) Andy's object (radio source)
Comets	C/2021 A1 (Leonard) C/2021 J1 (Maury–Attard) (248370) 2005 QN173 8P/Tuttle C/2014 OG₃₉₂ (PanSTARRS) C/2014 UN₂₇₁ (Bernardinelli-Bernstein) C/2021 T4 (Lemmon) P/2021 U3 (Attard–Maury)
Space exploration	Hope Mars mission (Mars orbit insertion: Feb 2021) Mars 2020 (Mars orbit insertion: Feb 2021;Perseverance Mars landing: Feb 2021) Tianwen-1 (Mars orbit insertion: Feb 2021;Zhurong rover Mars landing: May 2021)
Outer space portal Category:2020 in outer space —Category:2021 in outer space —Category:2022 in outer space

Retrieved from "https://en.wikipedia.org/w/index.php?title=List_of_exoplanets_discovered_in_2021&oldid=1320923913"

Categories:

Hidden categories:

[8]ページ先頭