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List of exoplanets discovered in 2022

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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 2022 is a list of confirmedexoplanets that were first reported in 2022.For exoplanets detected only byradial velocity, the listed value for mass is a lower limit. SeeMinimum mass for more information.

On 31 March 2022, K2-2016-BLG-0005Lb was reported to be themost distantexoplanet found byKepler to date.^[1]^[2]

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
29 Cygni b	13.9^+6.1 _−5.1			16.9^+3.4 _−1.9		astrometry + imaging	130.9±0.9	2.14±0.15	8790⁺¹⁵¹³ ₋₁₂₉₂	Host star also known as HIP 99770^[3]
CoRoT-35b	1.10±0.37	1.68±0.11	3.22748±0.00008	0.04290±0.00092	1747±62	transit	3700±200	1.01^+0.07 _−0.06	6390±130	^[4]
CoRoT-36b	0.68^+0.47 _−0.43	1.41±0.14	5.616531±0.000023	0.066±0.007	1567±35	transit	3110±60	1.32±0.09	6730±140	^[4]
EPIC 206317286 c	0.0168±0.098	0.186^+0.015 _−0.014	17.51547^+0.00228 _−0.00296		570	transit		0.832^+0.253 _−0.367	4752±138	^[5]
EPIC 210768568 b		0.088±0.004	3.2141±0.0002	0.0511^+0.0021 _−0.0028		transit	965	1.018±0.131	5711±105	^[6]
EPIC 246078343 b		0.068±0.007	0.8094±0.00003	0.0117^+0.0009 _−0.0012		transit	954	0.808^+0.364 _−0.256	4116±138	^[6]
EPIC 246078343 c		0.110±0.006	5.3301±0.0003	0.0426^+0.0016 _−0.0019		transit	954	0.808^+0.364 _−0.256	4116±138	^[6]
EPIC 246220667 b		0.172±0.006	6.6690±0.0002	0.0552^+0.0017 _−0.0023		transit	835	0.814^+0.363 _−0.251	4343±138	^[6]
EPIC 246220667 c		0.109±0.006	4.3696±0.0001	0.0487^+0.0027 _−0.0031		transit	835	0.814^+0.363 _−0.251	4343±138	^[6]
EPIC 247422570 b		0.189±0.009	5.9382^+0.0006 _−0.0004	0.0586^+0.0032 _−0.0033		transit	2181	0.893^+0.406 _−0.275	5590±138	^[6]
Gaia-1b	1.68±0.11	1.229±0.021	3.052524±0.000017	0.04047±0.00094		transit	1201±7	0.949±0.066	5470±110	First confirmed exoplanet discovered byGaia, along with Gaia-2b^[7]
Gaia-2b	0.817±0.047	1.322±0.013	3.6915224±0.0000039	0.0467±0.0015		transit	676±3	1.000±0.095	5720±84	First confirmed exoplanet discovered byGaia, along with Gaia-1b^[7]
Gliese 514b	0.0164±0.0028		140.43±0.41	0.422^+0.014 _−0.015	202±11	radial vel.	24.850±0.010	0.510±0.051	3714±51	Planetary orbit partially in habitable zone^[8]
Gliese 1002 b	0.0034±0.0004		10.3465±0.027	0.0457±0.0013	230.9±6.7	radial vel.	15.808±0.003	0.120±0.010	3024±52	Planet in habitable zone^[9]
Gliese 1002 c	0.0043±0.0005		21.202±0.013	0.0738±0.0021	181.7±5.2	radial vel.	15.808±0.003	0.120±0.010	3024±52	Planet in habitable zone^[9]
Gliese 3929 b	0.0055±0.0014	0.097±0.004	2.6162745±0.000003	0.0252±0.0005	568±6	transit	51.64±0.02	0.309±0.014	3369±51	Another planet in system is suspected^[10]^[11]
Gliese 3929 c	0.0180±0.0029		15.04±0.03	0.081±0.002	317±3	radial vel.	51.64±0.02	0.309±0.014	3369±51	^[11]
GJ 463 b	3.6±0.4		3448⁺¹¹⁰ ₋₈₈	3.53±0.07		radial vel.	59.91±0.03	0.49±0.02	3540±41	Host star also known as Ross 690^[12]^[13]
GJ 3090 b	0.0105	0.19	2.8531042±0.0000032	0.03165	696	transit	73.21±0.04	0.519±0.013	3556±70	Host star also known as TOI-177^[14]
GJ 3090 c	0.0538		12.734^+0.033 _−0.026	0.08575	421	radial vel.	73.21±0.04	0.519±0.013	3556±70	Host star also known as TOI-177^[14]
HD 3167 e	0.0306±0.0037		102.09^+0.52 _−0.50	0.4048^+0.0077 _−0.0074	375±7	radial vel.	154.59±0.13	0.852^+0.026 _−0.015	5300±73	^[15]
HD 18599 b	0.0758^+0.0223 _−0.0242	0.232±0.012	4.1374354^+0.0000036 _−0.0000037	0.0480±0.0004	935±11	transit	126.02±0.06	0.863±0.020	5145±50	Host star also known as TOI-179, also red dwarf star in the system^[16]^[17]^[18]
HD 20329b	0.0233±0.0034	0.154±0.006	0.926118^+0.000050 _−0.000043	0.0180±0.0003	2141±27	transit	207.7±0.9	0.90±0.05	5596±50	^[19]
HD 22532 b	2.12±0.09		872.6±2.8	1.900±0.004		radial vel.	526±2	1.20±0.05	5067⁺⁵⁹ ₋₂₂	Giant host star^[20]
HD 22946 b		0.154±0.009	4.040301^+0.000023 _−0.000042	0.0528±0.0030	1378±36	transit	205.08±0.16	1.158±0.058	6210⁺¹⁷³ ₋₁₅₈	Host star also known as TOI-411, third transiting planet in system is suspected^[21]
HD 22946 c		0.245±0.013	9.573096^+0.000026 _−0.000023	0.0939±0.0054	1033±27	transit	205.08±0.16	1.158±0.058	6210⁺¹⁷³ ₋₁₅₈	Host star also known as TOI-411, third transiting planet in system is suspected^[21]
HD 23472 d	0.0017±0.0006	0.067±0.005	3.97664^+0.000030 _−0.000044	0.04298^+0.00063 _−0.00065	909⁺³⁵ ₋₃₂	transit	127.48±0.06	0.67±0.03	4684±99	^[22]
HD 23472 e	0.0023±0.0009	0.073±0.006	7.90754±0.00011	0.0680±0.0010	723⁺²⁸ ₋₂₅	transit	127.48±0.06	0.67±0.03	4684±99	^[22]
HD 23472 f	0.0024±0.0013	0.102±0.007	12.1621839^+0.00012 _−0.000099	0.0906±0.0014	630⁺²⁷ ₋₂₃	transit	127.48±0.06	0.67±0.03	4684±99	^[22]
HD 28109 b	0.058^+0.029 _−0.024	0.196±0.009	22.89104^+0.00035 _−0.00036	0.1357±0.0034	881.2±7.5	transit	457.0±0.6	1.26±0.08	6120±50	^[23]
HD 28109 c	0.025^+0.013 _−0.010	0.378±0.010	56.00819^+0.00194 _−0.00202	0.308±0.011	585.2^+8.7 _−8.3	transit	457.0±0.6	1.26±0.08	6120±50	^[23]
HD 28109 d	0.018^+0.009 _−0.007	0.290±0.010	84.25999^+0.00744 _−0.00662	0.411±0.016	506.5^+8.7 _−8.0	transit	457.0±0.6	1.26±0.08	6120±50	^[23]
HD 29399 b	1.57±0.11		892.7±5.9	1.913±0.008		radial vel.	144.2±0.3	1.15±0.04	4845±52	Giant host star^[24]
HD 33142 d	0.89^+0.06 _−0.05		810.2^+3.8 _−4.2	1.955^+0.016 _−0.012		radial vel.	394.3±0.9	1.52±0.03	5025.4^+23.6 _−15.5	Giant host star^[25]
HD 56414 b	0.0944±0.0053	0.331±0.018	29.04992±0.00021	0.229±0.004	1133±30	transit	873±3	1.89±0.11	8500±150	Host star also known as TOI-1228^[26]
HD 64121 b	2.56±0.19		623.0±3.4	1.510±0.006		radial vel.	424.1±1.7	1.18±0.05	5066⁺⁵⁸ ₋₆₀	Giant host star^[20]
HD 69123 b	3.04±0.16		1193.3±7.0	2.482±0.010		radial vel.	245.0±1.3	1.43±0.07	4787⁺²⁸⁰ ₋₅₁	Giant host star^[20]
HD 83443 c	1.5^+0.5 _−0.2		8241⁺¹⁰¹⁹ ₋₅₃₀	8.0±0.8		radial vel.	133.6±0.2	1.00±0.03	5442±17	Eccentric orbit due to hot Jupiter in system^[27]
HD 93963A b		0.121±0.004	1.0391353^+0.0000049 _−0.0000045	0.02085±0.00037	2042±27	transit	268.6±1.3	1.109±0.043	5987±64	Host star also known as TOI-1797^[28]
HD 93963A c		0.288±0.005	3.6451398^+0.0000106 _−0.0000142	0.04813±0.00085	1344±18	transit	268.6±1.3	1.109±0.043	5987±64	Host star also known as TOI-1797^[28]
HD 109833 b		0.258^+0.014 _−0.012	9.188526±0.000026			transit	259.5±0.2	1.08±0.05	5881±50	Young host star also known as TOI-1097^[29]
HD 109833 c		0.231^+0.018 _−0.016	13.900148±0.000057			transit	259.5±0.2	1.08±0.05	5881±50	Young host star also known as TOI-1097^[29]
HD 114082 b	8.0±1.0	1.00±0.03	109.75^+0.40 _−0.37	0.5109^+0.0081 _−0.0083		transit	310.1±0.7	1.47±0.07	6651±35	Young star, eccentric planetary orbit^[30]^[31]
HD 167768 b [zh]	0.85^+0.12 _−0.11		20.6532^+0.0032 _−0.0032	0.1512^+0.0058 _−0.0063	1874	radial vel.	353.5	1.08^+0.14 _−0.12	4830	Host red giant star also known as HR 6840, other planets in system are suspected^[32]
HD 191939 g	0.0425±0.0063		284⁺¹⁰ ₋₈	0.812±0.028	278±6	radial vel.	174.4±0.1	0.81±0.04	5348±100	Habitable zone planet^[33]
HD 191939 f	>2.1		>2200	>3.2	<125		174.4±0.1	0.81±0.04	5348±100	^[33]
HD 199981 b	10.070±2.483		21000±8000	13.048±3.073		radial vel.	66.7±2.4			Host star also known as GJ 9714^[34]
HD 105618 b	0.079±0.008		9.9	0.091±0.004		radial vel.	227.8±0.4			Also brown dwarf in the system^[34]
HD 206893 c	12.3^+1.1 _−1.2	1.46^+0.18 _−0.06	2082	3.53^+0.08 _−0.07	1181.9^+20.6 _−53.9	radial vel.	125.1±2.6	1.24	6486	Some deuterium burning despite its low mass, also another brown dwarf is present in the system^[35]
HD 21019 b [zh]	0.014±0.002		2.56	0.034±0.002		radial vel.	120			Host star also known as GJ 2030^[34]
HD 21019 c [zh]	12.934±2.361		25600±2500	16.752±1.312		radial vel.	120			Host star also known as GJ 2030^[34]
HD 21175 b	0.038±0.010		10.6	0.091±0.004		radial vel.	57.7			Host star also known as GJ 3222, planet on extremely eccentric orbit, also brown dwarf in the system^[34]
HD 260655 b	0.0067±0.0011	0.111±0.002	2.76953±0.00003	0.02933±0.00024	709±4	transit	32.63±0.07	0.439±0.011	3803±10	Host star also known as TOI-4599^[36]
HD 260655 c	0.0097±0.0015	0.137±0.004	5.70588±0.00007	0.04749±0.00039	557±3	transit	32.63±0.07	0.439±0.011	3803±10	Host star also known as TOI-4599^[36]
HIP 34269 b [ja]	0.0052±0.0007	0.103±0.005	0.548177±0.000019	0.01188±0.00040	1617±41	transit	154.81±0.15	0.740±0.017	4440±100	Host star also known as TOI-500^[37]
HIP 34269 c [ja]	0.0146±0.0016		6.6356±0.0040			radial vel.	154.81±0.15	0.740±0.017	4440±100	Host star also known as TOI-500^[37]
HIP 34269 d [ja]	0.1055±0.0033		26.233±0.020			radial vel.	154.81±0.15	0.740±0.017	4440±100	Host star also known as TOI-500^[37]
HIP 34269 e [ja]	0.0376±0.0042		61.30±0.28			radial vel.	154.81±0.15	0.740±0.017	4440±100	Host star also known as TOI-500^[37]
HIP 94235 b		0.268±0.027	7.713057±0.000021	0.07870^+0.00056 _−0.00017	1060±50	transit	191.2±0.4	1.094^+0.024 _−0.007	5991±50	Host star also known as TOI-4399, shares system with a red dwarf^[38]
HR 7321 b	0.30±0.07		285.1^+1.2 _−1.5	0.937±0.003		radial vel.	200.2	1.35^+0.19 _−0.21	4971	Red giant host star also known as HD 184010^[39]
HR 7321 c	0.28^+0.08 _−0.10		483.3^+3.2 _−4.0	1.332^+0.006 _−0.007		radial vel.	200.2	1.35^+0.19 _−0.21	4971	Red giant host star also known as HD 184010^[39]
HR 7321 d	0.46±0.08		837.7^+6.4 _−5.5	1.922^+0.010 _−0.008		radial vel.	200.2	1.35^+0.19 _−0.21	4971	Red giant host star also known as HD 184010^[39]
K2-365 b	0.0272±0.0172	0.259^+0.017 _−0.015	23.448172^+0.00076 _−0.00099		710	transit		0.823^+0.369 _−0.25	5561±138	^[5]
K2-366 b	0.0199±0.0115	0.210^+0.016 _−0.014	15.93703^+0.00079 _−0.00114		770	transit		0.825^+0.366 _−0.255	5601±138	^[5]
K2-367 b	0.0203±0.0126	0.215^+0.020 _−0.017	20.64509^+0.00099 _−0.00137		450	transit		0.756^+0.231 _−0.347	4348±128	^[5]
K2-368 b	0.0073±0.0042	0.118^+0.009 _−0.008	5.02559^+0.00028 _−0.00034		800	transit		0.746^+0.334 _−0.232	4663±138	^[5]
K2-368 c	0.0078±0.0041	0.121^+0.010 _−0.009	9.66018±0.00116		650	transit		0.746^+0.334 _−0.232	4663±138	^[5]
K2-368 d	0.0146±0.0085	0.173^+0.013 _−0.012	20.20108^+0.00235 _−0.00273		500	transit		0.746^+0.334 _−0.232	4663±138	^[5]
K2-369 b	0.0069±0.0040	0.117^+0.009 _−0.008	5.76161^+0.00084 _−0.00071		1080	transit		0.735^+0.334 _−0.224	5682±138	^[5]
K2-370 b	0.0327±0.0207	0.286^+0.020 _−0.048	2.14084^+0.00003 _−0.00004		1420	transit		0.984^+0.428 _−0.303	5377±138	^[5]
K2-371 b	4.7±2.2	1.162^+0.082 _−0.077	3.11490±0.00001		1000	transit		0.958^+0.44 _−0.298	4925±138	^[5]
K2-372 b	0.0289±0.0168	0.262±0.006	9.84407^+0.00056 _−0.00057		870	transit		0.847^+0.101 _−0.088	5479±27	^[5]
K2-373 b	0.0162±0.0089	0.184^+0.013 _−0.012	11.02066^+0.00143 _−0.00136		1130	transit		1.158^+0.499 _−0.349	6138±138	^[5]
K2-374 b	0.0113±0.0058	0.142±0.005	4.52195^+0.00032 _−0.00040		1210	transit		0.731^+0.067 _−0.061	5789±21	^[5]
K2-374 c	0.0179±0.0109	0.197^+0.008 _−0.007	16.43445^+0.00237 _−0.00270		790	transit		0.731^+0.067 _−0.061	5789±21	^[5]
K2-375 b	0.0183±0.0106	0.200^+0.016 _−0.015	14.45389^+0.00477 _−0.00417		1000	transit		1.119^+0.492 _−0.344	5822±138	^[5]
K2-376 b	0.0129±0.0074	0.155^+0.011 _−0.010	5.77647^+0.00026 _−0.00023		1240	transit		0.908^+0.394 _−0.281	5937±138	^[5]
K2-377 b	0.0123±0.0073	0.151^+0.013 _−0.011	12.83223^+0.00155 _−0.00161		530	transit		0.821^+0.371 _−0.258	4200±138	^[5]
K2-378 b	0.0283±0.0173	0.257^+0.024 _−0.020	2.06043^+0.00011 _−0.00007		1130	transit		0.923^+0.425 _−0.291	4823±138	^[5]
K2-379 b	0.0175±0.0104	0.194^+0.032 _−0.017	8.77724^+0.00062 _−0.00061		680	transit		0.856^+0.375 _−0.265	4603±138	^[5]
K2-380 b	0.0250±0.0144	0.243^+0.016 _−0.015	9.40131^+0.00046 _−0.00050		1110	transit		0.993^+0.416 _−0.302	5911±138	^[5]
K2-381 b	0.0040±0.0026	0.095^+0.012 _−0.009	7.93893±0.00059		670	transit		0.754^+0.337 _−0.239	4473±138	^[5]
K2-381 c	0.0158±0.0094	0.178^+0.016 _−0.013	16.03465^+0.00184 _−0.00157		530	transit		0.754^+0.337 _−0.239	4473±138	^[5]
K2-381 d	0.0121±0.0070	0.150^+0.016 _−0.012	26.80302^+0.00277 _−0.00304		440	transit		0.754^+0.337 _−0.239	4473±138	^[5]
K2-382 b	0.0162±0.0101	0.185^+0.013 _−0.011	21.70015^+0.00202 _−0.00191		610	transit		0.922^+0.401 _−0.284	5452±138	^[5]
K2-383 b	0.0102±0.0052	0.139^+0.010 _−0.009	1.86596±0.00001		1270	transit		1.061^+0.459 _−0.327	5129±138	^[5]
K2-384b [ja]	0.0040±0.0026	0.096^+0.020 _−0.005	2.23152^+0.0019 _−0.00032		600	transit		0.330±0.009	3623±138	^[5]
K2-384c [ja]	0.0054±0.0027	0.106^+0.004 _−0.006	4.19476^+0.00030 _−0.00018		480	transit		0.330±0.009	3623±138	^[5]
K2-384d [ja]	0.0085±0.0044	0.124^+0.010 _−0.006	6.67958^+0.00071 _−0.00049		410	transit		0.330±0.009	3623±138	^[5]
K2-384e [ja]	0.0075±0.0042	0.120^+0.012 _−0.007	9.71504^+0.00100 _−0.00073		370	transit		0.330±0.009	3623±138	^[5]
K2-384f [ja]	0.0179±0.0104	0.198^+0.008 _−0.007	13.62749^+0.00034 _−0.00057		330	transit		0.330±0.009	3623±138	^[5]
K2-385 b	0.0100±0.0056	0.137^+0.012 _−0.011	2.38086^+0.00016 _−0.00021		1100	transit	1370±20	0.9270^+0.4120 _−0.2860	4844±138	^[5]
K2-386 b	0.0195±0.0115	0.207^+0.006 _−0.005	7.47322^+0.00037 _−0.00031		1010	transit	1400±30	0.911^+0.088 _−0.083	5749±22	^[5]
K2-387 b	0.1430±0.0996	0.653±0.023	28.73532±0.00099		340	transit	870±12	0.570^+0.051 _−0.048	3572±138	^[5]
K2-388 b	0.0412±0.0263	0.326^+0.029 _−0.020	6.33906^+0.00022 _−0.00018		970	transit	948±13	0.8420^+0.3760 _−0.2590	5367±138	^[5]
K2-389 b	0.0177±0.0103	0.195±0.010	8.58404^+0.00088 _−0.00202		1050	transit	846±9	0.8020^+0.3570 _−0.2460	5782±138	^[5]
K2-389 c	0.0165±0.0085	0.182^+0.013 _−0.012	20.85133^+0.00280 _−0.00298		780	transit	846±9	0.8020^+0.3570 _−0.2460	5782±138	^[5]
K2-390 b	0.0636±0.0390	0.416^+0.027 _−0.030	3.31279±0.00010		1310	transit	1490±18	0.7890^+0.3510 _−0.2390	5558±138	^[5]
K2-391 b	0.0078±0.0053	0.122^+0.025 _−0.016	4.62265^+0.00022 _−0.00025		900	transit	1660±50	0.7570^+0.3410 _−0.2400	5543±138	^[5]
K2-392 b	0.0140±0.0079	0.165^+0.014 _−0.013	15.39872^+0.00242 _−0.00193		840	transit	1330±30	0.8410^+0.3700 _−0.2580	5726±138	^[5]
K2-393 b	0.0199±0.0127	0.210^+0.015 _−0.014	10.41318^+0.00093 _−0.00069		950	transit	867±9	0.8810^+0.3810 _−0.2690	5678±138	^[5]
K2-394 b	0.0123±0.0063	0.151^+0.012 _−0.011	5.09571±0.00011		890	transit	319.7±1.5	0.478^+0.214 _−0.147	4938±138	^[5]
K2-395 b	0.0240±0.0141	0.231^+0.017 _−0.015	4.80335^+0.00035 _−0.00046		910	transit	935±10	0.9520^+0.4210 _−0.2930	5007±138	^[5]
K2-395 c	0.0371±0.0220	0.303^+0.025 _−0.022	8.49128^+0.00033 _−0.00030		750	transit	935±10	0.9520^+0.4210 _−0.2930	5007±138	^[5]
K2-396 b	0.0106±0.0061	0.140^+0.010 _−0.009	0.6736±0.00001		1990	transit	897±9	0.9540^+0.4290 _−0.2930	5236±138	^[5]
K2-396 c	0.0314±0.0189	0.278^+0.015 _−0.010	25.76051^+0.00199 _−0.00188		590	transit	897±9	0.9540^+0.4290 _−0.2930	5236±138	^[5]
K2-397 b	0.0212±0.0127	0.216±0.016	3.57232^+0.00018 _−0.00015		1210	transit	650±5	0.9370^+0.4060 _−0.2850	5387±138	^[5]
K2-398 b	0.0191±0.0112	0.203^+0.010 _−0.009	6.39302^+0.00113 _−0.00075		1240	transit	1980±40	0.9450^+0.0900 _−0.0830	5946±20	^[5]
K2-398 c	0.0736±0.0412	0.455±0.013	18.78783^+0.00087 _−0.00099		870	transit	1980±40	0.9450^+0.0900 _−0.0830	5946±20	^[5]
K2-400 b	0.0051±0.0025	0.103±0.004	3.86505±0.00018		570	transit	203.5±0.8	0.374±0.009	3578±138	^[5]
K2-401 b	0.0183±0.0117	0.201^+0.018 _−0.017	6.29309^+0.00057 _−0.00070		660	transit	655±5	0.8700^+0.3950 _−0.2690	4213±138	^[5]
K2-402 b	0.0245±0.0149	0.239^+0.019 _−0.017	17.27474^+0.00259 _−0.00317		870	transit	1710±60	0.9440^+0.4190 _−0.2900	5716±138	^[5]
K2-403 b	0.0783±0.0515	0.476^+0.031 _−0.034	33.58977±0.00076		580	transit	804±8	0.7840^+0.3400 _−0.2410	5511±138	^[5]
K2-404 b	0.0230±0.0127	0.225±0.007	13.11536^+0.00044 _−0.00060		450	transit	397±2	0.552±0.015	3748±138	^[5]
K2-405 b	0.0586±0.0342	0.407^+0.007 _−0.010	3.43547±0.00003		980	transit	643±7	1.034^+0.459 _−0.314	4927±138	^[5]
K2-406 b	0.063±0.039	0.410^+0.027 _−0.026	22.5494^+0.00137 _−0.00143		720	transit	278±2	0.7980^+0.3390 _−0.2450	5784±138	^[5]
K2-407 b	0.0066±0.0035	0.114^+0.008 _−0.007	4.9419^+0.00066 _−0.00069		1110	transit				^[5]
K2-407 c	0.0078±0.0044	0.121^+0.008 _−0.007	9.22453^+0.00132 _−0.00091		900	transit				^[5]
K2-408 b	0.0122±0.0062	0.149^+0.010 _−0.009	20.97895^+0.00130 _−0.00124		610	transit				^[5]
K2-409 b	0.0212±0.0127	0.221^+0.015 _−0.014	1.90808^+0.00004 _−0.00005		1800	transit				^[5]
K2-2016-BLG-0005Lb	1.1±0.1			4.4^+1.9 _−0.4	4700⁺³³⁰⁰ ₋₇₀₀	microlensing	17000±700	0.58±0.03		^[1]
Kepler-451 c	1.61±0.14		1460±90	2.1±0.2		timing	1340±20	0.48+0.12		^[40]
Kepler-451 d	1.76±0.18		43.0±0.1	0.20±0.03		timing	1340±20	0.48+0.12		^[40]
Kepler-1656 c	0.40±0.09		1919⁺²⁷ ₋₂₄	3.053±0.049		radial vel.		1.03±0.04		^[41]
Kepler-1708b	<4.6	0.8886^+0.0535 _−0.0526	737.11310^+0.00146 _−0.00770	1.64±0.10		transit	5436⁺³³⁴ ₋₂₉₈	1.088±0.072	6157⁺²³¹ ₋₂₀₂	Possibleexomoon host^[42]^[43]
Kepler-1972b [ja]	0.0064±0.0019	0.072±0.004	7.54425±0.00054			transit	923±3	1.12±0.03	5818±27	Very dense planets, additional planet in system suspected^[44]
Kepler-1972c [ja]	0.0066±0.0020	0.078±0.005	11.3295±0.0011			transit	923±3	1.12±0.03	5818±27	Very dense planets, additional planet in system suspected^[44]
KMT-2016-BLG-1105b	0.007^+0.023 _−0.005			2.44^+0.88 _−0.75		microlensing	17000±7000	0.41^+0.25 _−0.21		^[45]
KMT-2017-BLG-0428b	0.018^+0.011 _−0.009			1.81^+0.55 _−0.59		microlensing	18000⁺⁶⁰⁰⁰ ₋₈₀₀₀	0.34^+0.22 _−0.17		^[45]
KMT-2017-BLG-0673Lb	3.67^+2.17 _−2.07			2.34^+0.56 _−0.74		microlensing	17000⁺⁴⁰⁰⁰ ₋₅₀₀₀	0.63^+0.37 _−0.35		^[46]
KMT-2017-BLG-1003b	0.016^+0.017 _−0.009			1.38^+0.39 _−0.32		microlensing	23000±2000	0.32^+0.31 _−0.17		^[45]
KMT-2017-BLG-1194b	0.011±0.006			1.78^+0.45 _−0.46		microlensing	14000±6000	0.41^+0.23 _−0.19		^[45]
KMT-2018-BLG-0030b	1.45^+1.23 _−0.88			4.39^+2.18 _−2.40		microlensing	21000⁺⁴⁰⁰⁰ ₋₆₀₀₀	0.51^+0.43 _−0.31		^[47]
KMT-2018-BLG-0087b	0.23^+0.32 _−0.12			0.87^+0.24 _−0.25		microlensing	23000⁺³⁰⁰⁰ ₋₄₀₀₀	0.10^+0.14 _−0.05		^[47]
KMT-2018-BLG-0247b	2.11^+2.09 _−1.04			2.46^+0.51 _−0.58		microlensing	22000⁺³⁰⁰⁰ ₋₄₀₀₀	0.29^+0.28 _−0.14		^[47]
KMT-2018-BLG-2004b	0.27±\0.12			4.62^+0.80 _−1.10		microlensing	23000⁺³⁰⁰⁰ ₋₄₀₀₀	0.69^+0.32 _−0.31		^[48]
KMT-2018-BLG-2602b	1.15^+0.73 _−0.63			3.81^+2.96 _−2.32		microlensing	14000±6000	0.66^+0.42 _−0.36		^[47]
KMT-2018-BLG-2718b	16.0^+11.7 _−8.0			4.86^+2.97 _−2.55		microlensing	15000⁺¹⁰⁰⁰⁰ ₋₇₀₀₀	0.82^+0.57 _−0.39		^[48]
KMT-2019-BLG-0414Lb	4.57^+3.74 _−2.06			1.16^+0.47 _−0.51		microlensing	14000⁺⁵⁰⁰⁰ ₋₆₀₀₀	0.74^+0.43 _−0.38		^[46]
KMT-2019-BLG-1042Lb	0.19^+0.21 _−0.11			1.7±0.5		microlensing	22000⁺³⁰⁰⁰ ₋₅₀₀₀	0.30^+0.34 _−0.18		^[49]
KMT-2019-BLG-1367b	0.013^+0.008 _−0.007			1.70^+0.50 _−0.56		microlensing	15000⁺⁸⁰⁰⁰ ₋₇₀₀₀	0.25^+0.16 _−0.13		^[45]
KMT-2019-BLG-1552Lb	4.05^+1.73 _−1.85			2.6^+0.6 _−0.8		microlensing	15000⁺⁶⁰⁰⁰ ₋₅₀₀₀	0.79^+0.33 _−0.36		^[49]
KMT-2019-BLG-1806b	0.015±0.005			3.02^+0.70 _−0.73		microlensing	22000⁺²⁰⁰⁰ ₋₇₀₀₀	0.74±0.25		^[45]
KMT-2019-BLG-2974Lb	0.28^+0.29 _−0.18			2.0^+0.8 _−0.7		microlensing	20000⁺⁵⁰⁰⁰ ₋₇₀₀₀	0.47^+0.41 _−0.28		^[49]
KMT-2021-BLG-0171Lb	0.0352^+0.0173 _−0.0142			3.5^+1.3 _−1.0		microlensing	15000⁺⁵⁰⁰⁰ ₋₄₀₀₀	0.78^+0.29 _−0.26		^[50]
KMT-2021-BLG-0240 b	0.40^+0.07 _−0.08			2.5^+2.8 _−1.9		microlensing	23000⁺³⁰⁰⁰ ₋₅₀₀₀	0.47^+0.33 _−0.24		Multiple solutions for orbital separation^[51]
KMT-2021-BLG-0240 c	0.64^+0.25 _−0.24			1.0^+1.1 _−0.8		microlensing	23000⁺³⁰⁰⁰ ₋₅₀₀₀	0.47^+0.33 _−0.24		Multiple solutions for orbital separation^[51]
KMT-2021-BLG-0320Lb	0.10^+0.13 _−0.07			1.54^+0.24 _−0.30		microlensing	23000⁺³⁰⁰⁰ ₋₄₀₀₀	0.32^+0.39 _−0.21		^[52]
KMT-2021-BLG-0748b	0.45^+0.40 _−0.25			2.43±0.67		microlensing	20000⁺³⁰⁰⁰ ₋₄₀₀₀	0.36^+0.32 _−0.20		^[53]
KMT-2021-BLG-0119Lb	5.97^+2.94 _−2.60			3.23^+0.76 _−0.80		microlensing	11000⁺⁶⁰⁰⁰ ₋₄₀₀₀	0.69^+0.34 _−0.30		Multiple orbital solutions^[54]
KMT-2021-BLG-0192Lb	0.19^+0.09 _−0.10			2.07^+0.35 _−0.47		microlensing	22000⁺³⁰⁰⁰ ₋₅₀₀₀	0.55^+0.26 _−0.28		Multiple orbital solutions^[54]
KMT-2021-BLG-0712b	0.12^+0.06 _−0.04			2.22^+0.66 _−0.48		microlensing	10000⁺³⁰⁰⁰ ₋₂₀₀₀	0.22^+0.12 _−0.07		^[55]
KMT-2021-BLG-0909b	1.26^+1.01 _−0.66			1.75±0.42		microlensing	21000⁺³⁰⁰⁰ ₋₅₀₀₀	0.38^+0.30 _−0.20		^[55]
KMT-2021-BLG-1077Lb	0.22^+0.31 _−0.12			1.26^+1.41 _−1.08		microlensing	27000±3000	0.14^+0.19 _−0.07		^[56]
KMT-2021-BLG-1077Lc	0.25^+0.35 _−0.13			0.93^+1.05 _−0.80		microlensing	27000±3000	0.14^+0.19 _−0.07		^[56]
KMT-2021-BLG-1105b	1.30±0.68			3.54±1.06		microlensing	15000±5000	0.63±0.33		^[55]
KMT-2021-BLG-1253b	0.0599^+0.0643 _−0.0319			1.52^+0.57 _−0.41		microlensing	22000⁺³⁰⁰⁰ ₋₄₀₀₀	0.24^+0.26 _−0.13		^[53]
KMT-2021-BLG-1303Lb	0.38^+0.22 _−0.20			2.89^+0.44 _−0.66		microlensing	20000⁺³⁰⁰⁰ ₋₅₀₀₀	0.57^+0.32 _−0.29		Host star also known as MOA-2021-BLG-182^[52]
KMT-2021-BLG-1372b	0.1928±0.1129			2.37±0.77		microlensing	19000⁺⁵⁰⁰⁰ ₋₈₀₀₀	0.42±0.25		^[53]
KMT-2021-BLG-1391b	0.0143±0.0073			2.29^+0.56 _−0.71		microlensing	19000⁺³⁰⁰⁰ ₋₅₀₀₀	0.37±0.19		^[53]
KMT-2021-BLG-1554Lb	0.12^+0.20 _−0.07			0.72^+0.13 _−0.14		microlensing	25000⁺³⁰⁰⁰ ₋₄₀₀₀	0.08^+0.13 _−0.04		^[52]
KMT-2021-BLG-1689Lb	0.145^+0.094 _−0.072			2.5^+0.8 ₋₀₆		microlensing	23000⁺²⁰⁰⁰ ₋₄₀₀₀	0.58^+0.33 _−0.27		^[50]
KMT-2021-BLG-1898 b	0.73^+0.50 _−0.40			1.9^+0.3 _−0.5		microlensing	23000⁺³⁰⁰⁰ ₋₄₀₀₀	0.48^+0.33 _−0.26		Possibly a binary star system^[57]
KMT-2021-BLG-2294Lb	0.07^+0.10 _−0.03			0.94±0.16		microlensing	22000±3000	0.11^+0.17 _−0.06		Multiple orbital solutions^[54]
KMT-2021-BLG-2478b	0.80^+0.56 _−0.35			1.38±0.26		microlensing	8000⁺⁴⁰⁰⁰ ₋₃₀₀₀	0.12^+0.09 _−0.06		^[55]
L 363-38 b	0.0147±0.0014		8.781±0.007	0.048±0.006	330	radial vel.	33.31	0.21	3129	Host star also known asGliese 3049^[58]
MOA-2019-BLG-008L b	30					microlensing	8000±2000	0.8		^[59]
MOA-2020-BLG-135Lb	0.036^+0.060 _−0.021			1.11^+0.23 _−0.20		microlensing	26000±3000	0.23^+0.39 _−0.14		^[60]
MOA-2020-BLG-208Lb	0.217^+0.116 _−0.106			2.88^+0.40 _−0.41		microlensing	25000±3000	0.656^+0.346 _−0.322		^[61]
Mu2 Scorpii b	14.4			290		imaging	474	9.1	21900	^[62]
Mu2 Scorpii c	18.5			21		imaging	474	9.1	21900	^[62]
NGTS-20 b	2.98^+0.16 _−0.15	1.07±0.04	54.18915±0.00015	0.313±0.013	688⁺¹⁴ ₋₁₃	transit	1195±8	1.47±0.09	5980±80	Planet on eccentric orbit, host star also known as TOI-5152^[63]
NGTS-21b	2.36±0.21	1.33±0.03	1.5433897±0.0000016	0.0236±0.0005	1357±15	transit	2090⁺⁹⁰ ₋₈₀	0.72±0.04	4660±41	^[64]
NGTS-23b	0.613±0.097	1.267±0.030	4.0764326±0.0000041	0.0504±0.012	1327⁺¹⁷ ₋₁₆	transit	3230±70	1.01^+0.06 _−0.07	6057±64	^[65]
NGTS-24b	0.52^+0.12 _−0.11	1.214^+0.058 _−0.062	3.4678796±0.0000070	0.0479^+0.0028 _−0.0030	1499⁺⁴¹ ₋₃₆	transit	2360±80	1.26^+0.05 _−0.21	5820⁺⁹³ ₋₈	^[65]
NGTS-25b	0.639^+0.058 _−0.052	1.023^+0.035 _−0.052	2.8230930±0.0000033	0.0388^+0.0014 _−0.002	1101⁺¹⁵ ₋₁₄	transit	2350±30	0.91^+0.03 _−0.04	5321±58	^[65]
OGLE-2016-BLG-1093Lb	0.71±0.12			2.13±0.33		microlensing	26000±2000	0.46±0.08		^[66]
OGLE-2017-BLG-1691Lb	0.046^+0.037 _−0.025			2.41^+0.34 _−0.44		microlensing	24000⁺³⁰⁰⁰ ₋₄₀₀₀	0.45^+0.36 _−0.25		Host star also known as KMT-2017-BLG-0752^[52]
OGLE-2017-BLG-1806b	0.017^+0.015 _−0.009			1.75^+0.46 _−0.47		microlensing	21000⁺³⁰⁰⁰ ₋₅₀₀₀	0.38^+0.34 _−0.20		^[45]
OGLE-2018-BLG-0298Lb	0.14^+0.07 _−0.06			2.86^+0.73 _−0.80		microlensing	21000⁺³⁰⁰⁰ ₋₄₀₀₀	0.69^+0.34 _−0.30		^[47]
OGLE-2018-BLG-0932b	0.89^+0.36 _−0.31			1.75^+0.24 _−0.23		microlensing	22000±3000	0.72^+0.29 _−0.25		^[48]
OGLE-2018-BLG-1119Lb	0.91^+0.66 _−0.52			4.06^+2.14 _−2.58		microlensing	19000⁺⁵⁰⁰⁰ ₋₈₀₀₀	0.48^+0.35 _−0.28		^[47]
OGLE-2018-BLG-1126b	0.056^+0.033 _−0.031			3.23^+1.29 _−1.71		microlensing	19000⁺⁶⁰⁰⁰ ₋₈₀₀₀	0.69^+0.41 _−0.38		^[48]
OGLE-2018-BLG-1212b	0.20^+0.16 _−0.13			1.68^+1.47 _−0.63		microlensing	5100⁺⁴¹⁰⁰ ₋₁₈₀₀	0.16^+0.12 _−0.10		^[48]
OGLE-2018-BLG-1367b	0.95^+0.75 _−0.44			3.63^+1.02 _−0.96		microlensing		0.28^+0.22 _−0.13		Multiple solutions for frojected separation^[48]
OGLE-2018-BLG-1544b	11.2^+6.3 _−5.9			6.21^+1.32 _−2.10		microlensing	21000⁺⁴⁰⁰⁰ ₋₇₀₀₀	0.62^+0.38 _−0.36		Multiple solutions for frojected separation^[48]
OGLE-2018-BLG-1647b	0.97^+1.78 _−0.56			1.36^+0.20 _−0.17		microlensing	26000⁺⁴⁰⁰⁰ ₋₃₀₀₀	0.092^+0.170 _−0.053		^[48]
OGLE-2019-BLG-0362Lb	3.26^+0.83 _−0.58			2.18^+0.58 _−0.72		microlensing	19000±2000	0.42^+0.34 _−0.23		Multiple solutions for planetary parameters^[67]
OGLE-2019-BLG-1470LABc	2.2^+1.8 _−1.3			3.1^+1.2 _−1.1		microlensing	20000±4000	0.55+0.17		Circumbinary planet^[68]
Pi Mensae d	0.0421±0.0042		124.64^+0.48 _−0.52			radial vel.	59.62±0.07	1.11±0.01	6013±18	^[69]
Proxima Centauri d	0.0008±0.0002		5.122^+0.002 _−0.0036	0.02885^+0.00019 _−0.00022	360	radial vel.	4.2465±0.0003	0.1221±0.0022	2900±100	^[70]
PSR J2007+3120 b	0.0072±0.0009		723±8			timing	22000			Pulsar planet, another planet in the system is suspected.^[71]
Ross 508 b	0.0126±0.0019		10.76^+0.01 _−0.02	0.05353^+0.00047 _−0.00051		radial vel.	36.594±0.011	0.1774±0.0045	3071⁺³⁴ ₋₂₂	Host star also known as Gliese 585, planet close to habitable zone.^[72]
TOI-181b	0.127891^+0.013510 _−0.025081	0.631521^+0.007554 _−0.009811	4.532058^+0.000002 _−0.000002	0.055780^+0.005563 _−0.003893	878⁺³² ₋₄₁	transit	314±2	0.781±0.042	4994±50	^[73]
TOI-206 b		0.116±0.004	0.7363104±0.0000003	0.0112±0.0001	910±36	transit	155.9	0.35±0.01	3383±157	^[74]
TOI-277 b	0.0239^+0.0179 _−0.0098	0.237±0.016	3.9940±0.0004	0.0269±0.0011		transit	212.6^+0.6 _−0.3	0.16±0.01	4031⁺²¹ ₋₂₃	^[75]
TOI-500 b		0.104±0.010	0.5481579±0.0000006	0.0128±0.0011	1693±105	transit	154.8	0.88±0.25	4621±50	^[74]
TOI-544 b		0.181±0.009	1.5483510±0.0000015	0.0251 ± 0.0019	1082±47	transit	132.7	0.85±0.20	4369±100	^[74]
TOI-620 b			5.0988179^+0.0000045 _−0.0000046	0.04825^+0.00065 _−0.00066	603.6^+5.5 _−5.3	transit	107.81±0.19	0.577^+0.024 _−0.023	3708⁺⁵⁷ ₋₅₆	^[76]
TOI-778 b	2.76±0.24	1.375±0.045	4.633611±0.000001	0.060±0.003	1561⁺³³ ₋₃₂	transit	530±4	1.428±0.094	6715±128	^[77]
TOI-833 b		0.113±0.006	1.0418777±0.0000324	0.0171±0.0003	1118±49	transit	136.3	0.61±0.03	3920±160	^[74]
TOI-969 b	0.0286±0.0031	0.247±0.033	1.8237305^+0.0000020 _−0.0000021	0.02636±0.00017	941±31	transit	253.8±0.5	0.730±0.037	4550±75	^[78]
TOI-969 c	11.3^+1.1 _−0.9		1700⁺²⁹⁰ ₋₂₈₀	2.52^+0.27 _−0.29	96.4^+6.8 _−5.8	radial vel.	253.8±0.5	0.730±0.037	4550±75	Eccentric orbit^[78]
TOI-1064b	0.0425±0.0055	0.231±0.004	6.443868±0.000025	0.06152^+0.00086 _−0.00089	784±13	transit	224.5±0.2	0.748±0.032	4734±67	^[79]
TOI-1064c	0.0079^+0.0057 _−0.0063	0.237±0.004	12.226574^+0.000046 _−0.000043	0.09429^+0.00132 _−0.00136	634±10	transit	224.5±0.2	0.748±0.032	4734±67	^[79]
TOI-1075 b		0.154±0.007	0.6047328±0.0000032	0.0118±0.0001	1336±56	transit	200.9	0.60±0.02	3921±157	^[74]
TOI-1075 b	0.0313±0.0042	0.160^+0.010 _−0.007	0.6047328±0.0000032	0.01159^+0.00023 _−0.00020	1323±44	transit	200.4^+0.6 _−2.2	0.604±0.030	3875±75	^[80]
TOI-1107b	3.35±0.18	1.30±0.05	4.0782387^+0.0000024 _−0.0000025	0.0561^+0.0024 _−0.0025	1728±27	transit	925±7	1.35±0.08	6311±98	^[81]
TOI-1136 b	0.0095^+0.0022 _−0.0028	0.170^+0.019 _−0.013	4.1728±0.0002			transit	275.8±0.5	1.022±0.027	5770±50	^[82]
TOI-1136 c	0.0189^+0.0041 _−0.0053	0.257±0.005	6.2573±0.0002			transit	275.8±0.5	1.022±0.027	5770±50	^[82]
TOI-1136 d	0.0252^+0.0076 _−0.0060	0.413±0.007	12.5194±0.0004			transit	275.8±0.5	1.022±0.027	5770±50	^[82]
TOI-1136 e	0.0170±0.0031	0.236^+0.006 _−0.008	18.7992^+0.0017 _−0.0015			transit	275.8±0.5	1.022±0.027	5770±50	^[82]
TOI-1136 f	0.0261^+0.0088 _−0.0113	0.346±0.010	26.3162^+0.0017 _−0.0013			transit	275.8±0.5	1.022±0.027	5770±50	^[82]
TOI-1136 g	0.0151^+0.0148 _−0.0104	0.226±0.010	39.5387^+0.0036 _−0.0030			transit	275.8±0.5	1.022±0.027	5770±50	^[82]
TOI-1181 b	1.18±0.14	1.30±0.08	2.103195^+0.000012 _−0.000011		2162	transit	1013±3	1.38^+0.086 _−0.082	6260±100	Subgiant host star^[83]
TOI-1221 b		0.259±0.011	91.68278^+0.00032 _−0.00041	0.404^+0.026 _−0.023	400	transit	447.1±0.7	1.03±0.06	5592±50	^[84]
TOI-1246 b [ja]	0.0255±0.0035	0.269±0.005	4.30744±0.00002	0.049±0.002	955	transit	557.9±1.0	1.12±0.16	5217±50	^[85]
TOI-1246 c [ja]	0.0277±0.0038	0.224±0.007	5.904144±0.000083	0.061±0.002	860	transit	557.9±1.0	1.12±0.16	5217±50	^[85]
TOI-1246 d [ja]	0.0167±0.0053	0.313±0.008	18.65590±0.00048	0.131±0.004	586	transit	557.9±1.0	1.12±0.16	5217±50	^[85]
TOI-1246 e [ja]	0.0466±0.0072	0.338±0.014	37.9216±0.0010	0.211±0.007	462	transit	557.9±1.0	1.12±0.16	5217±50	^[85]
TOI-1260 d	0.0373±0.0245	0.276±0.008	16.608164±0.000083	0.1116±0.0033	499±4	transit	239.5±0.3	0.66±0.01	4227±85	^[86]
TOI-1268 b	0.303±0.026	0.81±0.05	8.1577080±0.0000044	0.072^+0.009 _−0.010	919	transit	359.1±0.4	0.92±0.03	5290±117	^[87]
TOI-1272 b	0.0774±0.0072	0.370±0.019	3.31599±0.00002	0.0412±0.0008	961±32	transit	450.6±1.3	0.851±0.049	4985±121	^[88]
TOI-1272 c	0.0840±0.0098		8.689±0.008	0.0783±0.0014	697±23	radial vel.	450.6±1.3	0.851±0.049	4985±121	^[88]
TOI-1288 b	0.0712^+0.0574 _−0.0304	0.454±0.010	2.69998±0.00015	0.0429±0.0006		transit	375.3^+1.3 _−0.5	1.46±0.06	5307⁺¹⁸ ₋₁₆	^[75]
TOI-1288 c	0.2643±0.0220		443⁺¹¹ ₋₁₃			radial vel.	375.3^+1.3 _−0.5	1.46±0.06	5307⁺¹⁸ ₋₁₆	^[89]
TOI-1411 b		0.121±0.013	1.4520358±0.0000098	0.0230±0.0026	1136±59	transit	106.0	0.59±0.23	4266±100	^[74]
TOI-1422 b	0.0283^+0.0072 _−0.0063	0.354^+0.012 _−0.010	12.9972±0.0006	0.108±0.003	867±17	transit	504.17^+0.12 _−0.09	0.981^+0.062 _−0.065	5840±62	Another planet in the system is suspected.^[90]
TOI-1442 b		0.104±0.005	0.4090677±0.0000003	0.0071±0.0002	1072±54	transit	134.5	0.29±0.02	3330±160	^[74]
TOI-1452 b	0.0152±0.0041	0.149±0.006	11.06201±0.00002	0.061±0.003	326±7	transit	99.51±0.04	0.249±0.008	3185±50	Also a red dwarf on a 97AU separation in the system^[91]
TOI-1468 b	0.0101±0.0008	0.114±0.003	1.8805136^+0.0000024 _−0.0000026		682.2^+7.4 _−6.9	transit	80.64±0.07	0.339±0.011	3496±25	^[92]
TOI-1468 c	0.0209±0.0021	0.184±0.004	15.532482^+0.000034 _−0.000033		337.5^+3.7 _−3.4	transit	80.64±0.07	0.339±0.011	3496±25	^[92]
TOI-1516 b	3.16±0.12	1.36±0.03	2.056014±0.000002		1820	transit	804.6±1.9	1.085^+0.061 _−0.066	6420±100	^[83]
TOI-1669 b	0.0132±0.0085	0.214±0.016	2.7			transit	364.6	1.00±0.05	5542.3±100.0	^[93] Host star also known as BD+82 71, planet suspected since 2020^[94]
TOI-1669 c	0.602±0.078		501±16			radial vel.	364.6	1.00±0.05	5542.3±100.0	^[93] Host star also known as BD+82 71, additional long-period companion is suspected.
TOI-1694 b	0.0979±0.0066	0.461±0.016	3.8			transit	405.7	0.84±0.03	5066±100	^[93] Host star also known as TYC 4108-1434-1, planet suspected since 2020^[94]
TOI-1694 c	0.929±0.037		393.2±4.3			radial vel.	405.7	0.84±0.03	5066±100	^[93] Host star also known as TYC 4108-1434-1
TOI-1670 b	0.04±0.03	0.184^+0.017 _−0.013	10.98462^+0.00046 _−0.00051	0.103±0.002	1062⁺¹⁴ ₋₁₃	transit	540.6^+1.0 _−1.2	1.21±0.02	6170±61	^[95]
TOI-1670 c	0.63^+0.09 _−0.08	0.987±0.025	40.74976^+0.000022 _−0.00021	0.249±0.005	684±9	transit	540.6^+1.0 _−1.2	1.21±0.02	6170±61	^[95]
TOI-1693 b		0.126±0.009	1.7666957±0.0000054	0.0226±0.0004	764±19	transit	100.6	0.49±0.03	3499±70	^[74]
TOI-1695 b	0.0173±0.0031	0.181±0.016	3.1342790±0.0000072	0.033548^+0.000260 _−0.000268	590±90	transit	147.2±0.2	0.51±0.02	3627±31	^[96]^[97]
TOI-1696 b	0.1781	0.276±0.010	2.500311±0.000004	0.0229±0.0002	489±13	transit	210.8±0.5	0.255±0.0066	3185±76	^[98]^[99]
TOI-1710 b	0.0890±0.0148	0.477±0.010	24.283429±0.00043	0.16±0.04	687±50	transit	264.7±0.2	0.984^+0.050 _−0.059	5665±55	^[100]
TOI-1759 b	0.021±0.06	0.279±0.02	18.849975±0.000006	0.1176±0.0013	433±14	transit	130.85±0.05	0.606±0.020	4065±51	^[101]^[102]
TOI-1811 b	0.974^+0.075 _−0.076	1.002^+0.026 _−0.024	3.7130818±0.0000028	0.04393^+0.00058 _−0.00054	961.5±8	transit	418±3	0.819^+0.033 _−0.030	4753⁺⁵⁴ ₋₅₅	^[103]
TOI-1820 b	2.3±0.2	1.12±0.02	4.860700±0.000010	0.069±0.005	1295±11	transit	807±13	1.04±0.13	5734±50	^[104]
TOI-1860 b		0.117±0.005	1.0662107±0.0000014	0.0204±0.0002	1885±28	transit	149.8	0.99±0.03	5752±100	^[74]
TOI-1937 b	2.01^+0.17 _−0.16	1.247^+0.059 _−0.062	0.94667944±0.00000047	0.01932^+0.00035 _−0.00039	2097⁺³⁵ ₋₃₆	transit	1366±6	1.072^+0.059 _−0.064	5814⁺⁹¹ ₋₉₃	^[105]
TOI-2000 b	0.0324±0.0070	0.236±0.010	3.098331^+0.000021 _−0.000019	0.04260^+0.00076 _−0.00067	1475⁺¹²⁰ ₋₁₅₈	transit	566.3±1.0	1.074^+0.059 _−0.050	5607⁺⁸⁶ ₋₈₂	^[106]
TOI-2000 c	0.238±0.012	0.711±0.011	9.1270553±0.0000073	0.0875^+0.0016 _−0.0014	1029⁺⁸⁴ ₋₁₁₁	transit	566.3±1.0	1.074^+0.059 _−0.050	5607⁺⁸⁶ ₋₈₂	^[106]
TOI-2025 b	4.4±0.4	1.120±0.009	8.872086±0.000009	0.089±0.004	1186±11	transit	1106±7	1.32±0.14	5880±53	^[104]
TOI-2025 b	3.51^+0.36 _−0.35	1.118^+0.031 _−0.030	8.8720942^+0.0000080 _−0.0000079	0.0886^+0.0019 _−0.0024	1172⁺¹⁸ ₋₁₇	transit	1095±11	1.176^+0.079 _−0.091	5928⁺⁷⁶ ₋₇₅	^[103]
TOI-2046 b	2.30±0.08	1.44±0.11	1.4971842^+0.0000031 _−0.0000033		1998	transit	940±3	1.153^+0.100 _−0.093	6160±100	Young host star^[83]
TOI-2048 b		0.184±0.018	13.79019^+0.00065 _−0.00084		640±20	transit	379.7±0.5	0.83±0.03	5185±60	Young host star belongs toNGC 3532^[107]
TOI-2081 b	0.0157^+0.0151 _−0.0076	0.182±0.046	10.50534^+0.00007 _−0.00008	0.0752^+0.0047 _−0.0119	488⁺²⁸ ₋₅₂	transit	203.26±0.16	0.540±0.080	3800±100	^[108]
TOI-2136 b	0.0200^+0.0077 _−0.0072	0.196±0.015	7.851928^+0.000018 _−0.000016	0.057±0.006	395⁺²⁴ ₋₂₂	transit	108.82±0.07	0.34±0.02	3342±100	^[109]^[110]
TOI-2145 b	5.35^+0.32 _−0.35	1.103^+0.031 _−0.029	10.261081^+0.000026 _−0.000027	0.1108^+0.0012 _−0.0015	1484⁺¹⁶ ₋₁₄	transit	733±5	1.720^+0.057 _−0.068	6189±67	Host star also known as HIP 86040^[103]
TOI-2152A b	2.83^+0.38 _−0.37	1.281^+0.050 _−0.046	3.3773512^+0.0000060 _−0.0000061	0.05064^+0.00093 _−0.0011	1802⁺⁶⁰ ₋₅₄	transit	988±13	1.516^+0.085 _−0.10	6630⁺³⁰⁰ ₋₂₉₀	Planet orbiting primary of binary star^[103]
TOI-2154 b	0.92^+0.19 _−0.18	1.453^+0.053 _−0.048	3.8240801±0.0000025	0.0513^+0.0011 _−0.0013	1580±27	transit	967±10	1.233^+0.077 _−0.090	6280±160	^[103]
TOI-2180 b	2.755^+0.087 _−0.081	1.010^+0.022 _−0.019	260.79^+0.59 _−0.58	0.828±0.012	348.0^+3.3 _−3.6	transit	379.4±0.8	1.111^+0.047 _−0.046	5695⁺⁵⁸ ₋₆₀	^[111]
TOI-2158 b	0.82±0.08	0.960±0.012	8.60077±0.00003	0.075±0.004	1188±10	transit	652±3	1.12±0.12	5673±50	^[104]
TOI-2193 b	0.94±0.18	1.77	2.1225735±0.0000016	0.03319^+0.00052 _−0.00051	1763⁺²¹ ₋₂₂	transit	1126±3	1.082^+0.052 _−0.049	5974±110	Also 0.54`M`_☉ star in the system^[112]
TOI-2196 b	0.0818±0.0041	0.313±0.013	1.1947268^+0.0000079 _−0.0000093	0.02234±0.00060	1860±20	transit	861±3	1.032±0.038	5634±31	Neptunian desert planet^[113]
TOI-2207 b	0.64^+0.10 _−0.12	0.995^+0.028 _−0.027	8.001968^+0.000024 _−0.000025	0.0854^+0.0015 _−0.0016	1259⁺¹⁶ ₋₁₅	transit	1242±9	1.296^+0.069 _−0.072	6075±110	^[112]
TOI-2260 b		0.145±0.012	0.3524728±0.0000047	0.0097±0.0001	2609±86	transit	331.2	0.99±0.04	5534±100	^[74]
TOI-2236 b	1.58^+0.40 _−0.39	1.282^+0.032 _−0.031	3.5315902±0.0000026	0.05009^+0.00080 _−0.00082	1688⁺¹⁹ ₋₂₁	transit	1149±5	1.343^+0.066 _−0.065	6164±50	^[112]
TOI-2337b	1.60±0.15	0.9±0.1	2.99432±0.00008	0.04467		transit	1780±20	1.325±0.118	4780±100	^[114]
TOI-2364 b	0.225^+0.043 _−0.049	0.768^+0.023 _−0.018	4.0197517±0.0000043	0.04871^+0.00069 _−0.00079	1091⁺¹⁷ ₋₁₄	transit	713±6	0.954^+0.041 _−0.046	5306⁺⁷⁶ ₋₆₈	^[105]
TOI-2411 b		0.150±0.010	0.7826942±0.0000037	0.0144±0.0001	1355±45	transit	194.5	0.65±0.02	4099±123	^[74]
TOI-2421 b	0.333±0.079	0.925^+0.035 _−0.034	4.3474032^+0.0000079 _−0.0000078	0.0543^+0.0021 _−0.0010	1534⁺²⁰ ₋₂₈	transit	1067±7	1.131^+0.130 _−0.064	5577±50	^[112]
TOI-2427 b		0.161±0.011	1.3060011±0.0000102	0.0202±0.0002	1117±46	transit	93.1	0.64±0.02	4072±121	^[74]
TOI-2445 b		0.112±0.007	0.3711281±0.0000005	0.0064±0.0001	1060±54	transit	158.7	0.25±0.01	3333±157	^[74]
TOI-2497 b	5.21±0.52	1.000^+0.040 _−0.038	10.655661±0.000026	0.1167^+0.0018 _−0.0017	1596⁺⁴⁴ ₋₄₁	transit	930±14	1.861^+0.086 _−0.081	7360⁺²⁹⁰ ₋₂₇₀	^[103]
TOI-2567 b	0.201^+0.034 _−0.031	0.975^+0.031 _−0.029	5.983944±0.000013	0.0672^+0.0024 _−0.0012	1352⁺¹⁸ ₋₁₉	transit	1691±8	1.130^+0.130 _−0.059	5650±50	^[112]
TOI-2570 b	0.820^+0.063 _−0.065	1.217^+0.035 _−0.034	2.9887615±0.0000022	0.04145^+0.00081 _−0.00086	1431⁺²⁴ ₋₂₃	transit	1179±6	1.063^+0.063 _−0.065	5765±50	^[112]
TOI-2583 b	0.250^+0.058 _−0.056	1.290^+0.040 _−0.033	4.5207265±0.0000049	0.0571^+0.0010 _−0.0013	1456⁺¹⁹ ₋₁₆	transit	1831±9	1.215^+0.063 _−0.082	5936⁺⁶⁵ ₋₆₈	^[105]
TOI-2587 b	0.218^+0.054 _−0.046	1.077^+0.042 _−0.040	5.456640±0.000011	0.0635^+0.0025 _−0.0013	1445⁺²³ ₋₂₆	transit	1242±10	1.15^+0.14 _−0.07	5760⁺⁸⁰ ₋₇₉	^[105]
TOI-2669b	0.61±0.19	1.76±0.16	6.2034±0.0001			transit	1294±9	1.19±0.16	4800±100	^[114]
TOI-2796 b	0.44^+0.10 _−0.11	1.59	4.8084983^+0.0000057 _−0.0000056	0.0569^+0.0010 _−0.0011	1205⁺¹⁸ ₋₁₇	transit	1150±6	1.063^+0.057 _−0.062	5764⁺⁸¹ ₋₇₈	^[105]
TOI-2803 b	0.975^+0.083 _−0.070	1.616^+0.034 _−0.032	1.96229325±0.00000082	0.03185±0.00052	1893⁺²⁹ ₋₂₈	transit	1635±9	1.118^+0.056 _−0.054	6280⁺⁹⁹ ₋₉₆	^[105]
TOI-2818 b	0.71±0.26	1.363^+0.046 _−0.045	4.0397090^+0.0000024 _−0.0000023	0.0493^+0.0010 _−0.0008	1376⁺²⁶ ₋₂₄	transit	1028±3	0.977^+0.063 _−0.049	5721⁺⁸⁸ ₋₈₃	^[105]
TOI-2842 b	0.370^+0.052 _−0.047	1.146^+0.051 _−0.048	3.5514058^+0.0000077 _−0.0000078	0.0475^+0.0010 _−0.0011	1471⁺²⁹ ₋₂₇	transit	1501±8	1.135^+0.077 _−0.079	5910±100	^[105]
TOI-2977 b	1.68^+0.26 _−0.25	1.174^+0.031 _−0.027	2.3505614±0.0000025	0.03386^+0.00067 _−0.00050	1544±26	transit	1160±30	0.936^+0.057 _−0.041	5691⁺⁹⁴ ₋₉₃	^[105]
TOI-3023 b	0.62^+0.10 _−0.09	1.466^+0.043 _−0.032	3.9014971±0.0000031	0.0505^+0.0015 _−0.0009	1596⁺²⁴ ₋₂₅	transit	1281±5	1.12^+0.11 _−0.06	5760⁺⁸⁵ ₋₈₈	^[105]
TOI-3331 b	2.27±0.16	1.158±0.043	2.0180231^+0.0000043 _−0.0000044	0.03144^+0.00048 _−0.00055	1488⁺³¹ ₋₂₉	transit	733±4	1.016^+0.047 _−0.052	5521±110	Also 0.6`M`_☉ star in the system^[112]
TOI-3364 b	1.67^+0.12 _−0.13	1.091^+0.038 _−0.032	5.8768918±0.0000069	0.0675^+0.0011 _−0.0016	1264⁺²² ₋₂₁	transit	899±3	1.186^+0.059 _−0.083	5706⁺⁹⁵ ₋₉₁	^[105]
TOI-3540 b	1.18±0.14	2.10	3.1199990±0.0000079	0.04289^+0.00092 _−0.00093	1498±22	transit	921±10	1.081^+0.071 _−0.069	5969±50	Also 0.8`M`_☉ star in the system^[112]
TOI-3629 b	0.26±0.02	0.74±0.02	3.936551^+0.000005 _−0.000006	0.043±0.002	690±20	transit	423.1±1.0	0.63±0.02	3870±90	^[115]
TOI-3688 b	0.98^+0.10 _−0.11	1.167^+0.048 _−0.044	3.246075±0.000012	0.04560^+0.00089 _−0.00098	1534⁺²⁹ ₋₂₈	transit	1308±6	1.199^+0.072 _−0.076	5950±100	^[105]
TOI-3693 b	1.02^+0.24 _−0.22	1.124^+0.029 _−0.023	9.088516^+0.000026 _−0.000027	0.0813^+0.0011 _−0.0012	801⁺¹³ ₋₁₂	transit	576±2	0.867^+0.036 _−0.037	5274±50	^[112]
TOI-3714 b	0.70±0.003	1.01±0.03	2.154849±0.000001	0.027±0.001	750±20	transit	367.0^+0.6 _−1.3	0.53±0.02	3660±90	^[115]
TOI-3757 b	0.2684±0.0276	1.07^+0.04 _−0.05	3.4387530^+0.0000039 _−0.0000040	0.03845±0.00043	759±13	transit	579±2	0.64±0.02	3913±56	^[116]
TOI-3807 b	1.04^+0.15 _−0.14	2.00	2.8989727^+0.0000038 _−0.0000039	0.0421^+0.0007 _−0.0011	1646⁺²⁵ ₋₂₄	transit	1399±7	1.181^+0.064 _−0.092	5772⁺⁸⁴ ₋₈₀	^[105]
TOI-3819 b	1.11^+0.18 _−0.20	1.172^+0.036 _−0.035	3.2443141±0.0000055	0.04611^+0.00069 _−0.00096	1633⁺²¹ ₋₁₉	transit	1834±17	1.242^+0.057 _−0.076	5859⁺⁷² ₋₇₁	^[105]
TOI-3884 b	0.0519^+0.0110 _−0.0057	0.563±0.025	4.5445697±0.0000094	0.0354±0.0014	463±12	transit	141.37±0.16	0.2813±0.0067	3269±70	^[117]^[118]
TOI-3912 b	0.406^+0.071 _−0.068	1.274^+0.041 _−0.040	3.4936264±0.0000038	0.0463^+0.0012 _−0.0010	1512±20	transit	1533±9	1.088^+0.086 _−0.070	5725⁺⁶⁹ ₋₆₈	^[105]
TOI-3976 b	0.175^+0.037 _−0.036	1.095^+0.036 _−0.035	6.607662^+0.000016 _−0.000015	0.0743^+0.0013 _−0.0014	1295⁺¹⁶ ₋₁₄	transit	1703±8	1.254^+0.067 _−0.072	5975⁺⁷⁰ ₋₆₉	^[105]
TOI-4087 b	0.73±0.14	1.164^+0.025 _−0.024	3.17748350±0.00000094	0.04469^+0.00048 _−0.00054	1458⁺²⁰ ₋₁₇	transit	1013±4	1.178^+0.039 _−0.042	6060⁺⁷⁴ ₋₆₇	^[105]
TOI-4137 b	1.44^+0.17 _−0.15	1.211^+0.040 _−0.039	3.8016122±0.0000065	0.05222^+0.00089 _−0.00096	1570⁺²⁵ ₋₂₄	transit	1128±7	1.313^+0.068 _−0.071	6134±50	^[112]
TOI-4145 b	0.43±0.13	1.187^+0.032 _−0.031	4.0664428±0.0000058	0.04823^+0.00075 _−0.00079	1074⁺¹⁹ ₋₁₆	transit	668.7±1.3	0.905^+0.043 _−0.044	5281⁺⁸⁶ ₋₇₆	^[105]
TOI-4329b	0.45±0.09	1.50±0.19	2.9223±0.00015			transit	2258±16	1.538±0.049	6000±100	^[114]
TOI-4463 b	0.794^+0.039 _−0.040	1.183^+0.064 _−0.045	2.8807198^+0.0000028 _−0.0000027	0.04036^+0.00074 _−0.00082	1395⁺²⁵ ₋₂₂	transit	579.5±1.8	1.056^+0.059 _−0.063	5640⁺⁸⁹ ₋₈₂	^[105]
TOI-4479 b	0.0261^+0.0252 _−0.0126	0.252±0.057	1.15890^+0.00001 _−0.00002	0.0164^+0.0015 _−0.0029	861⁺⁶⁴ ₋₁₀₃	transit	262.9±0.3	0.452±0.090	3400±100	^[108]
TOI-4562 b	3.29^+1.88 _−0.82	1.072^+0.044 _−0.043	225.11757^+0.00027 _−0.00025	0.771±0.013	349±10	transit	1131±12	1.218^+0.054 _−0.048	6096±32	Highly eccentric orbit^[119]
TOI-4582 b	0.53±0.05	0.94^+0.09 _−0.12	31.034±0.001			transit	1242	1.34±0.06	5190±100	Evolved star, eccentric planetary orbit^[120]
TOI-4791 b	2.31^+0.32 _−0.33	1.110±0.050	4.280880^+0.000022 _−0.000023	0.0555^+0.0011 _−0.0012	1472⁺²⁶ ₋₂₄	transit	1051±6	1.242^+0.072 _−0.077	6058⁺⁹⁹ ₋₉₄	^[105]
TOI-5153 b	3.26^+0.18 _−0.17	1.06±0.04	20.33003±0.00007	0.158±0.006	906±13	transit	1272.336±11	1.24±0.07	6300±80	^[63]
TOI-5174 b	0.07801	0.47667	12.214			transit		1.0±0.125		^[121]^[122]
TOI-5205b	1.08±0.06	1.03±0.03	1.630757±0.000001	0.0199±0.0002	737±15	transit	283.35±0.16	0.392±0.015	3430±54	^[123]
TOI-5542 b	1.32±0.10	1.009^+0.036 _−0.035	75.12375^+0.00019 _−0.00018	0.332±0.016	441⁺⁴⁸ ₋₇₄	transit	1154±12	0.890^+0.056 _−0.031	5700±80	^[124]
Berry 37a	0.69^+0.47 _−0.43	1.41±0.14	5.616531±0.000023	0.066±0.007	961.5±8	transit	20±60	1.32±0.09	4200±140	^[125]
TYC 2187-512-1 b	0.33±0.02		691.90^+8.77 _−8.61	1.22±0.02		radial vel.	50.512±0.016	0.498±0.019	3734±54	^[125]
WASP-132c	0.165±0.009		1.011534±0.000005	0.0182±0.0003		transit	390	0.782±0.034	4714⁺⁸⁷ ₋₈₈	^[126]

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]

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^Teng, Huan-Yu; Sato, Bun'ei; Kunitomo, Masanobu; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Xiao, Guang-Yao; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Shigeru, Ida (2022), "A close-in planet orbiting giant star HD 167768",Publications of the Astronomical Society of Japan,75:169–176,arXiv:2211.06576,doi:10.1093/pasj/psac097
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^^a ^b ^c ^d ^eFeng, 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 (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,S2CID 251864022
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^^a ^bLuque, R.; et al. (2022), "The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc",Astronomy & Astrophysics,664: A199,arXiv:2204.10261,Bibcode:2022A&A...664A.199L,doi:10.1051/0004-6361/202243834,S2CID 248300168
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^^a ^b ^cTeng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Nagasawa, Makiko; Hasegawa, Ryo; Izumiura, Hideyuki; Kambe, Eiji; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru (2022), "A trio of giant planets orbiting evolved star HD 184010",Publications of the Astronomical Society of Japan,74 (6):1309–1328,arXiv:2209.09426,doi:10.1093/pasj/psac070
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^Mistry, Priyashkumar; Pathak, Kamlesh; Lekkas, Georgios; Prasad, Aniket; Bhattarai, Surendra; Maity, Mousam; Beichman, Charles A.; Ciardi, David R.; Evans, Phil; Lucero, Jennifer P. (2023), "VaTEST I: Validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star",Monthly Notices of the Royal Astronomical Society,521:1066–1078,arXiv:2211.07957,doi:10.1093/mnras/stad543
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^^a ^bWilson, Thomas G.; et al. (2022), "A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS",Monthly Notices of the Royal Astronomical Society,511:1043–1071,arXiv:2201.03570,doi:10.1093/mnras/stab3799
^Essack, Zahra; et al. (2023), "TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap",The Astronomical Journal,165 (2): 47,arXiv:2210.14901,Bibcode:2023AJ....165...47E,doi:10.3847/1538-3881/ac9c5b,S2CID 253117166
^Psaridi, A.; et al. (2022), "Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars",Astronomy & Astrophysics,664: A94,arXiv:2205.10854,Bibcode:2022A&A...664A..94P,doi:10.1051/0004-6361/202243454,S2CID 248872705
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^Knudstrup, E.; et al. (2022), "Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion",Monthly Notices of the Royal Astronomical Society,519 (4):5637–5655,arXiv:2211.17035,doi:10.1093/mnras/stac3684
^Naponiello, L.; et al. (2022), "The GAPS programme at TNG. XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422",Astronomy & Astrophysics,A8: 667,arXiv:2207.03293,Bibcode:2022A&A...667A...8N,doi:10.1051/0004-6361/202244079,S2CID 250334523
^Cadieux, Charles; Doyon, René; et al. (27 June 2022)."TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf".The Astronomical Journal. 164:96 (3) (published 12 August 2022): 28pp.arXiv:2208.06333.Bibcode:2022AJ....164...96C.doi:10.3847/1538-3881/ac7cea.
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^^a ^bGiacalone, Steven; et al. (2020), "Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates",The Astronomical Journal,161: 24,arXiv:2002.00691,doi:10.3847/1538-3881/abc6af,S2CID 227141512
^^a ^bTran, Quang H.; et al. (2022), "TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration",The Astronomical Journal,163 (5): 225,arXiv:2203.04334,Bibcode:2022AJ....163..225T,doi:10.3847/1538-3881/ac5c4f,S2CID 247318919
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^Cherubim, Collin; et al. (2023), "TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley",The Astronomical Journal,165 (4): 167,arXiv:2211.06445,Bibcode:2023AJ....165..167C,doi:10.3847/1538-3881/acbdfd,S2CID 256627151
^Mori, Mayuko; et al. (2022), "TOI-1696: A Nearby M4 Dwarf with a 3 R ⊕ Planet in the Neptunian Desert",The Astronomical Journal,163 (6): 298,arXiv:2203.02694,Bibcode:2022AJ....163..298M,doi:10.3847/1538-3881/ac6bf8,S2CID 247291913
^Beard, Corey; et al. (2022), "TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with the Habitable-Zone Planet Finder",The Astronomical Journal,163 (6): 286,arXiv:2204.09063,Bibcode:2022AJ....163..286B,doi:10.3847/1538-3881/ac69ec,S2CID 248266475
^König, P. -C.; et al. (2022), "A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N",Astronomy & Astrophysics,666: A183,arXiv:2204.08984,Bibcode:2022A&A...666A.183K,doi:10.1051/0004-6361/202143002,S2CID 248239823
^Espinoza, Néstor; et al. (2022), "A Transiting, Temperate Mini-Neptune Orbiting the M Dwarf TOI-1759 Unveiled by TESS",The Astronomical Journal,163 (3): 133,arXiv:2202.01240,Bibcode:2022AJ....163..133E,doi:10.3847/1538-3881/ac4af0,S2CID 246485680
^Martioli, E.; et al. (2022), "TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS",Astronomy & Astrophysics,660: A86,arXiv:2202.01259,Bibcode:2022A&A...660A..86M,doi:10.1051/0004-6361/202142540,S2CID 246485686
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^Newton, Elisabeth R.; et al. (2022), "TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet",The Astronomical Journal,164 (3): 115,arXiv:2206.06254,Bibcode:2022AJ....164..115N,doi:10.3847/1538-3881/ac8154,S2CID 249626353
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^Gan, Tianjun; et al. (2022), "TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136",Monthly Notices of the Royal Astronomical Society,514 (3):4120–4139,arXiv:2202.10024,doi:10.1093/mnras/stac1448
^Kawauchi, K.; et al. (2022), "Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf",Astronomy & Astrophysics,666: A4,arXiv:2202.10182,Bibcode:2022A&A...666A...4K,doi:10.1051/0004-6361/202243381,S2CID 247011479
^Dalba, Paul A.; et al. (2022), "The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope",The Astronomical Journal,163 (2): 61,arXiv:2201.04146,Bibcode:2022AJ....163...61D,doi:10.3847/1538-3881/ac415b,S2CID 245877799
^^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^jYee, Samuel W.; et al. (2022), "The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets",The Astronomical Journal,164 (2): 70,arXiv:2205.09728,Bibcode:2022AJ....164...70Y,doi:10.3847/1538-3881/ac73ff,S2CID 248887656
^Persson, Carina M.; et al. (2022), "TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star",Astronomy & Astrophysics,666: A184,arXiv:2208.05797,Bibcode:2022A&A...666A.184P,doi:10.1051/0004-6361/202244118,S2CID 251478602
^^a ^b ^cGrunblatt, Samuel K.; et al. (2022), "TESS Giants Transiting Giants. II. The Hottest Jupiters Orbiting Evolved Stars",The Astronomical Journal,163 (3): 120,arXiv:2201.04140,Bibcode:2022AJ....163..120G,doi:10.3847/1538-3881/ac4972,S2CID 245877793
^^a ^bCañas, Caleb I.; et al. (2022), "TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID",The Astronomical Journal,164 (2): 50,arXiv:2201.09963,Bibcode:2022AJ....164...50C,doi:10.3847/1538-3881/ac7804,S2CID 246275821
^Kanodia, Shubham; et al. (2022), "TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf",The Astronomical Journal,164 (3): 81,arXiv:2203.07178,Bibcode:2022AJ....164...81K,doi:10.3847/1538-3881/ac7c20,S2CID 247446993
^Almenara, J. M.; Bonfils, X.; Forveille, T.; Astudillo-Defru, N.; Ciardi, D. R.; Schwarz, R. P.; Collins, K. A.; Cointepas, M.; Lund, M. B.; Bouchy, F.; Charbonneau, D.; Díaz, R. F.; Delfosse, X.; Kidwell, R. C.; Kunimoto, M.; Latham, D. W.; Lissauer, J. J.; Murgas, F.; Ricker, G.; Seager, S.; Vezie, M.; Watanabe, D. (2022), "TOI-3884 b: A rare 6-RE planet that transits a low-mass star with a giant and likely polar spot",Astronomy & Astrophysics,667: L11,arXiv:2210.10909,Bibcode:2022A&A...667L..11A,doi:10.1051/0004-6361/202244791,S2CID 253018639
^Libby-Roberts, Jessica E.; Schutte, Maria; Hebb, Leslie; Kanodia, Shubham; Canas, Caleb; Stefansson, Gudmundur; Lin, Andrea S. J.;Mahadevan, Suvrath; Parts, Winter; Powers, Luke; Wisniewski, John; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Everett, Mark E.; Gupta, Arvind F.; Halverson, Samuel; Kobulnicky, Henry A.; Kowalski, Adam F.; Larsen, Alexander; Monson, Andrew; Ninan, Joe P.; Parker, Brock A.; Ramsey, Lawrence W.; Robertson, Paul; Schwab, Christian; Swaby, Tera N.; Terrien, Ryan C. (2023),An In-Depth Look at TOI-3884b: a Super-Neptune Transiting a M4 Dwarf with Persistent Star Spot Crossings,arXiv:2302.04757
^Heitzmann, Alexis; et al. (2023), "TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star",The Astronomical Journal,165 (3): 121,arXiv:2208.10854,Bibcode:2023AJ....165..121H,doi:10.3847/1538-3881/acb5a2,S2CID 251741424
^Grunblatt, Samuel K.; Saunders, Nicholas; Chontos, Ashley; Hattori, Soichiro; Veras, Dimitri; Huber, Daniel; Angus, Ruth; Rice, Malena; Breivik, Katelyn; Blunt, Sarah; Giacalone, Steven; Lubin, Jack; Isaacson, Howard; Howard, Andrew W.; Ciardi, David R.; Safonov, Boris S.; Strakhov, Ivan A.; Latham, David W.; Bieryla, Allyson; Ricker, George R.; Jenkins, Jon M.; Tenenbaum, Peter; Shporer, Avi; Morgan, Edward H.; Kostov, Veselin; Osborn, Hugh P.; Dragomir, Diana; Seager, Sara; Vanderspek, Roland K.; Winn, Joshua N. (2023), "TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars",The Astronomical Journal,165 (2): 44,arXiv:2210.17062,Bibcode:2023AJ....165...44G,doi:10.3847/1538-3881/aca670,S2CID 253237700
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^"Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved16 January 2023.
^Kanodia, Shubham; Mahadevan, Suvrath; Libby-Roberts, Jessica; Stefansson, Gudmundur; Canas, Caleb I.; Piette, Anjali A. A.; Boss, Alan; Teske, Johanna; Chambers, John; Zeimann, Greg; Monson, Andrew; Robertson, Paul; Ninan, Joe P.; Lin, Andrea S. J.; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Gupta, Arvind F.; Halverson, Samuel; Hawley, Suzanne; Kobulnicky, Henry A.; Metcalf, Andrew J.; Parker, Brock A.; Powers, Luke; Ramsey, Lawrence W.; Roy, Arpita; Schwab, Christian; Swaby, Tera N.; Terrien, Ryan C.; Wisniewski, John (2023), "TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf",The Astronomical Journal,165 (3): 120,arXiv:2209.11160,Bibcode:2023AJ....165..120K,doi:10.3847/1538-3881/acabce,S2CID 257050897
^Grieves, Nolan; et al. (2022), "An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542",Astronomy & Astrophysics,668: A29,arXiv:2209.14830,Bibcode:2022A&A...668A..29G,doi:10.1051/0004-6361/202244077,S2CID 252595745
^^a ^bQuirrenbach, A.; Passegger, V. M.; Trifonov, T.; Amado, P. J.; Caballero, J. A.; Reiners, A.; Ribas, I.; Aceituno, J.; Bejar, V. J. S.; Chaturvedi, P.; Gonzalez-Cuesta, L.; Henning, T.; Herrero, E.; Kaminski, A.; Kuerster, M.; Lalitha, S.; Lodieu, N.; Lopez-Gonzalez, M. J.; Montes, D.; Palle, E.; Perger, M.; Pollacco, D.; Reffert, S.; Rodriguez, E.; Rodriguez Lopez, C.; Shan, Y.; Tal-Or, L.; Zapatero Osorio, M. R.; Zechmeister, M. (2022), "The CARMENES search for exoplanets around M dwarfs",Astronomy & Astrophysics,663: A48,arXiv:2203.16504,doi:10.1051/0004-6361/202142915,S2CID 247835988
^Hord, Benjamin J.; Colón, Knicole D.; Berger, Travis A.; Kostov, Veselin; Silverstein, Michele L.; Stassun, Keivan G.; Lissauer, Jack J.; Collins, Karen A.; Schwarz, Richard P.; Sefako, Ramotholo; Ziegler, Carl; Briceño, César; Law, Nicholas; Mann, Andrew W.; Ricker, George R.; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Bouma, Luke G.; Falk, Ben; Torres, Guillermo; Twicken, Joseph D.; Vanderburg, Andrew (2022), "The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 B",The Astronomical Journal,164 (1): 13,arXiv:2205.02501,Bibcode:2022AJ....164...13H,doi:10.3847/1538-3881/ac6f57,S2CID 248524687

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

2022 in space

« 2021
2023 »

Space probe launches

CAPSTONE (June 2022)
Danuri (August 2022)
Artemis I (November 2022)
Hakuto-R Mission 1 /Emirates Lunar Mission /Lunar Flashlight (December 2022)

Impact events

SelectedNEOs

Discoveries

2021 LL37 (TNO) 2021 RR205 (TNO) Alcyoneus (galaxy) CEERS-93316 Gaia BH1 GLASS-z12 GNz7q GRB 221009A HD1 (galaxy) J1144–4308 JADES-GS-z13-0 OGLE-2011-BLG-0462 PKS 2131-021 PSR J0901–4046 PSR J0952–0607 Sagittarius A* imaged S4716 SN 2022jli VFTS 243 Webb's First Deep Field (SMACS J0723.3–7327) WD 1054–226 WHL0137-LS ZTF J1813+4251 12moons of Jupiter
Exoplanets	AB Aurigae b CO₂ onWASP-39b Gliese 514 b Gliese 3929 b c Gliese 896 Ab HD 83443 c HD 260655 b c K2-2016-BLG-0005Lb Kepler-451 c d Kepler-1708b and possibleexomoon Kepler-1708b I LP 890-9 b c Mu2 Scorpii b c OGLE-2018-BLG-1119Lb Pi Mensae d Proxima Centauri d TOI-1227 b TOI-1452 b TOI-2180 b

Comets

Space exploration

DART (Dimorphos impact; September 2022)

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