List of exoplanets discovered in 2022 - Meteorite

astro.wikisort.org - Meteorite

This list of exoplanets discovered in 2022 is a list of confirmed exoplanets that were first reported in 2022. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

On 31 March 2022, K2-2016-BLG-0005Lb was reported to be the most distant exoplanet found by Kepler 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
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[3]
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[3]
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[3]
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[4]
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	Possible exomoon host[5][6]
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	[7]
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	[7]
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	[8]
TOI-4329b	0.45±0.09	1.50±0.19	2.9223±0.00015			transit	2258±16	1.538±0.049	6000±100	[8]
TOI-2669b	0.61±0.19	1.76±0.16	6.2034±0.0001			transit	1294±9	1.19±0.16	4800±100	[8]
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	[9]
OGLE-2016-BLG-1093Lb	0.71±0.12			2.13±0.33		microlensing	26000±2000	0.46±0.08		[10]
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	[11]
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	[11]
Kepler-1972 b	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[12]
Kepler-1972 c	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[12]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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	[13]
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[14][15]
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	[16][17]
Kepler-451 c	1.61±0.14		1460±90	2.1±0.2		timing	1340±20	0.48+0.12		[18]
Kepler-451 d	1.76±0.18		43.0±0.1	0.20±0.03		timing	1340±20	0.48+0.12		[18]
KMT-2021-BLG-1391b	0.0143±0.0073			2.29^+0.56 _−0.71		microlensing	19000⁺³⁰⁰⁰ ₋₅₀₀₀	0.37±0.19		[19]
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		[19]
KMT-2021-BLG-1372b	0.1928±0.1129			2.37±0.77		microlensing	19000⁺⁵⁰⁰⁰ ₋₈₀₀₀	0.42±0.25		[19]
KMT-2021-BLG-0748b	0.45^+0.40 _−0.25			2.43±0.67		microlensing	20000⁺³⁰⁰⁰ ₋₄₀₀₀	0.36^+0.32 _−0.20		[19]
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	[20]
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	[21]
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	[22][23]
PSR J2007+3120 b	0.0072±0.0009		723±8			timing	22000			Pulsar planet, another planet in the system is suspected.[24]
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	[25]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
K2-384 b	0.0040±0.0026	0.096^+0.020 _−0.005	2.23152^+0.0019 _−0.00032		600	transit		0.330±0.009	3623±138	[26]
K2-384 c	0.0054±0.0027	0.106^+0.004 _−0.006	4.19476^+0.00030 _−0.00018		480	transit		0.330±0.009	3623±138	[26]
K2-384 d	0.0085±0.0044	0.124^+0.010 _−0.006	6.67958^+0.00071 _−0.00049		410	transit		0.330±0.009	3623±138	[26]
K2-384 e	0.0075±0.0042	0.120^+0.012 _−0.007	9.71504^+0.00100 _−0.00073		370	transit		0.330±0.009	3623±138	[26]
K2-384 f	0.0179±0.0104	0.198^+0.008 _−0.007	13.62749^+0.00034 _−0.00057		330	transit		0.330±0.009	3623±138	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
K2-399 b	0.1015±0.0697	0.540^+0.093 _−0.042	0.75997±0.00001		2780	transit	1680±40	0.783^+0.131 _−0.114	5690±38	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
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	[26]
K2-407 b	0.0066±0.0035	0.114^+0.008 _−0.007	4.9419^+0.00066 _−0.00069		1110	transit				[26]
K2-407 c	0.0078±0.0044	0.121^+0.008 _−0.007	9.22453^+0.00132 _−0.00091		900	transit				[26]
K2-408 b	0.0122±0.0062	0.149^+0.010 _−0.009	20.97895^+0.00130 _−0.00124		610	transit				[26]
K2-409 b	0.0212±0.0127	0.221^+0.015 _−0.014	1.90808^+0.00004 _−0.00005		1800	transit				[26]
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	[26]
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	[27][28]
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	[29]
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	[29]
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	[30]
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	[31]
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		[32]
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		[32]
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]
KMT-2019-BLG-1042Lb	0.19^+0.21 _−0.11			1.7±0.5		microlensing	22000⁺³⁰⁰⁰ ₋₅₀₀₀	0.30^+0.34 _−0.18		[33]
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		[33]
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		[33]
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	[34]
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		[35]
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		[36]
KMT-2018-BLG-2004b	0.27±\0.12			4.62^+0.80 _−1.10		microlensing	23000⁺³⁰⁰⁰ ₋₄₀₀₀	0.69^+0.32 _−0.31		[36]
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		[36]
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[36]
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[36]
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		[36]
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		[36]
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		[36]
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[37]
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[38]
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[39]
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	[40]
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[41]
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[41]
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[42]
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[42]
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[43]
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	[44]
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	[44]
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	[44]
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	[44]
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[45]
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[46]
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[46]
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[46]
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[46]
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	[47]
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	[47]
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	[47]
HIP 63374 B	11±3			30.02±0.12		imaging	176.4±0.3	1.211±0.006		[48]
HIP 60584 B	8±3			16.58±0.15		imaging	99.60±0.12	1.352±0.014		[48]
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[49]
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	[49]
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[49]
WASP-132c	0.165±0.009		1.011534±0.000005	0.0182±0.0003		transit	390	0.782±0.034	4714⁺⁸⁷ ₋₈₈	[50]
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	[51]
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	[51]
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[51]
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[51]
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	[51]
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	[51]
Mu2 Scorpii b	14.4			290		direct imaging	474	9.1	21900	[52]
Mu2 Scorpii c	18.5			21		direct imaging	474	9.1	21900	[52]
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	[53]
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	[53]
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	[53]
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[54]
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	[54]
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	[54]
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	[54]
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	[54]
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	[54]
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[54]
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[54]
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	[54]
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	[54]
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 by Gaia, along with Gaia-2b[55]
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 by Gaia, along with Gaia-1b[55]
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[56]
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		[56]
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[56]
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		[56]
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	[57]
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.[58]
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		[59]
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		[59]
HD 33142 d [ja]	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[60]
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 to NGC 3532[61]
Kepler-1656 c	0.40±0.09		1919⁺²⁷ ₋₂₄	3.053±0.049		radial vel.		1.03±0.04		[62]
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	[63]
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	[63]
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		[64]
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		[64]
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		[64]
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		[64]
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		[64]
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		[64]
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	[65]
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	[65]
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.[66]
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[67]
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	[67]
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		[68]
KMT-2021-BLG-0909b	1.26^+1.01 _−0.66			1.75±0.42		microlensing	21000⁺³⁰⁰⁰ ₋₅₀₀₀	0.38^+0.30 _−0.20		[68]
KMT-2021-BLG-2478b	0.80^+0.56 _−0.35			1.38±0.26		microlensing	8000⁺⁴⁰⁰⁰ ₋₃₀₀₀	0.12^+0.09 _−0.06		[68]
KMT-2021-BLG-1105b	1.30±0.68			3.54±1.06		microlensing	15000±5000	0.63±0.33		[68]
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	[69]
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	[69]
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	[15]
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[70]
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[70]
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[71]
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[71]
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[72]
HD 206893 c [fr]	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 of low mass, also another brown dwarf is present in the system[73]
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[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[75]
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[76]
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	[77]
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	[77]
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[78]
HD 21019 b [zh]	0.014±0.002		2.56	0.034±0.002		radial vel.	120			Host star also known as GJ 2030[79]
HD 21019 c [zh]	12.934±2.361		25600±2500	16.752±1.312		radial vel.	120			Host star also known as GJ 2030[79]
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[79]
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[79]
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[79]
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		[80]
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		[80]
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[81]
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[81]
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[81]
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	[82]
TOI-1669 b	0.0132±0.0085	0.214±0.016	2.7			transit	364.6	1.00±0.05	5542.3±100.0	[83]Host star also known as BD+82 71, planet suspected since 2020[84]
TOI-1669 c	0.602±0.078		501±16			radial vel.	364.6	1.00±0.05	5542.3±100.0	[83]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	[83]Host star also known as TYC 4108-1434-1, planet suspected since 2020[84]
TOI-1694 c	0.929±0.037		393.2±4.3			radial vel.	405.7	0.84±0.03	5066±100	[83]Host star also known as TYC 4108-1434-1
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[85]
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[85]
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[85]
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[86]
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[86]
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	[87]

Specific exoplanet lists

Lists of exoplanets

References

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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, arXiv:2205.02501
Rodriguez, Joseph E.; et al. (2022), Another Shipment of Six Short-Period Giant Planets from TESS, arXiv:2205.05709
Squicciarini, V.; Gratton, R.; Janson, M.; Mamajek, E. E.; Chauvin, G.; Delorme, P.; Langlois, M.; Vigan, A.; Ringqvist, S. C.; Meeus, G.; Reffert, S.; Kenworthy, M.; Meyer, M. R.; Bonnefoy, M.; Bonavita, M.; Mesa, D.; Samland, M.; Desidera, S.; D'Orazi, V.; Engler, N.; Alecian, E.; Miglio, A.; Henning, T.; Quanz, S. P.; Mayer, L.; Flasseur, O.; Marleau, G. D. (2022), A scaled-up planetary system around a supernova progenitor, arXiv:2205.02279
Dransfield, Georgina; et al. (2022), "HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica", Monthly Notices of the Royal Astronomical Society, arXiv:2205.09046, doi:10.1093/mnras/stac1383
Yee, Samuel W.; et al. (2022), The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets, arXiv:2205.09728
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Han, Cheongho; et al. (2022), Four sub-Jovian-mass planets detected by high-cadence microlensing surveys, arXiv:2205.10510
Psaridi, A.; et al. (2022), "Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars", Astronomy & Astrophysics, arXiv:2205.10854, doi:10.1051/0004-6361/202243454, S2CID 248872705
Harakawa, Hiroki; et al. (2022), A Super-Earth Orbiting Near the Inner Edge of the Habitable Zone around the M4.5-dwarf Ross 508, arXiv:2205.11986
Yang, Hongjing; et al. (2022), KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: Two Microlensing Planets in the KMTNet High-cadence Fields with Followup Observations, arXiv:2205.12584
A new third planet and the dynamical architecture of the HD 33142 planetary system, 2022, arXiv:2206.03899
TESS Hunt for Young and Maturing Exoplanets (THYME) VII : Membership, rotation, and lithium in the young cluster Group-X and a new young exoplanet, 2022, arXiv:2206.06254
Kepler-1656b’s Extreme Eccentricity: Signature of a Gentle Giant, 2022, arXiv:2204.00019
A hot sub-Neptune in the desert and a temperate super-Earth around faint M dwarfs Color validation of TOI-4479b and TOI-2081b, 2022, arXiv:2206.10643
Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-Prime-Field Planets, 2022, arXiv:2206.11409
The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272, 2022, arXiv:2206.14327
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, 2022, arXiv:2207.03293
Two long-period transiting exoplanets on eccentric orbits: NGTS-20 b (TOI-5152 b) and TOI-5153 b, 2022, arXiv:2207.03911
Mass Production of 2021 KMTNet Microlensing Planets II, arXiv:2207.07295
Sub-stellar Companions of Intermediate-mass Stars with CoRoT: CoRoT-34b, CoRoT-35b, and CoRoT-36b, 2022, arXiv:2207.08742
The HD 93963 A transiting system: A 1.04 d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS, 2022, arXiv:2207.13920
Atmosphere of the mini-Neptune transiting the bright M dwarf GJ 3090 can be characterized, 2022, arXiv:2207.14121
OGLE-2019-BLG-0362Lb: A SUPER-JOVIAN-MASS PLANET AROUND A LOW-MASS STAR, 2022, arXiv:2208.04230
Direct Discovery of the Inner Exoplanet in the HD 206893 System Evidence for Deuterium Burning in a Planetary Mass Companion, 2022, arXiv:2208.04867
TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star, 2022, arXiv:2208.05797
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. American Astronomical Society (published 12 August 2022). 164:96 (3): 28pp. arXiv:2208.06333. Bibcode:2022AJ....164...96C. doi:10.3847/1538-3881/ac7cea.
HD 56414 b: A Warm Neptune Transiting an A-type Star, 2022, arXiv:2208.06396
TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley, 2022, arXiv:2208.10351
TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field star, 2022, arXiv:2208.10854
3-D selection of 167 sub-stellar companions to nearby stars, 2022, arXiv:2208.12720
KMT-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey, 2022, arXiv:2209.00112
Mass Production of 2021 KMTNet Microlensing Planets III: Analysis of Three Giant Planets, 2022, arXiv:2209.03886
A CHEOPS-enhanced view of the HD3167 system, 2022, arXiv:2209.06937
TESS-Keck Survey XIV: 2 giant exoplanets from the Distant Giants Survey, 2022, arXiv:2209.06958
Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates, 2020, arXiv:2002.00691
A Trio of Giant Planets Orbiting Evolved Star HD 184010, 2022, arXiv:2209.09426
TESS discovery of a super-Earth and two sub-Neptunes orbiting the bright, nearby, Sun-like star HD 22946, 2022, arXiv:2209.09597
TOI-5205b: A Jupiter transiting an M dwarf near the Convective Boundary, 2022, arXiv:2209.11160

Exoplanets

Planet
- Definition
  - IAU
Planetary science

Main topics

Exoplanet
Exoplanet orbital and physical parameters
Methods of detecting exoplanets
Planetary system
Planet-hosting stars

Sizes
and
types

Terrestrial	Carbon planet Coreless planet Desert planet Dwarf planet Ice planet Iron planet Lava planet Ocean world Mega-Earth Sub-Earth Super-Earth
Gaseous	Eccentric Jupiter Mini-Neptune (Gas dwarf) Helium planet Hot Jupiter Hot Neptune Gas giant Ice giant Super-Jupiter Super-Neptune Super-puff Ultra-hot Jupiter Ultra-hot Neptune
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

Accretion
Accretion disk
Asteroid belt
Circumplanetary disk
Circumstellar disc
Circumstellar envelope
Cosmic dust
Debris disk
Detached object
Disrupted planet
Excretion disk
Exozodiacal dust
Extraterrestrial materials
Extraterrestrial sample curation
Giant-impact hypothesis
Gravitational collapse
Hills cloud
Internal structure
Interplanetary dust cloud
Interplanetary medium
Interplanetary space
Interstellar cloud
Interstellar dust
Interstellar medium
Interstellar space
Kuiper belt
List of interstellar and circumstellar molecules
Merging stars
Molecular cloud
Nebular hypothesis
Oort cloud
Outer space
Planetary migration
Planetary system
Planetesimal
Planet formation
Protoplanetary disk
Ring system
Rubble pile
Sample-return mission
Scattered disc
Star formation

Systems

Exocomet
- Interstellar
Exomoon
- Tidally detached
Rogue planet
Orbits
- Retrograde
- Trojan
- Mean-motion resonances
- Titius–Bode law

Host stars

A
B
Binary star
Brown dwarfs
F/Yellow-white dwarfs
G/Yellow dwarfs
Herbig Ae/Be
K/Orange dwarfs
M/Red dwarfs
Pulsar
Red giant
Subdwarf B
Subgiant
T Tauri
White dwarfs
Yellow giants

Detection

Astrometry
Direct imaging
- list
Microlensing
- list
Polarimetry
Timing
- list
Radial velocity
- list
Transit method
- list
Transit-timing variation

Habitability

Astrobiology
Astrooceanography
Circumstellar habitable zone
Earth analog
Extraterrestrial liquid water
Habitability of natural satellites
Habitable exoplanet
Superhabitable planet

Catalogues

Lists

Exoplanetary systems
- Host stars
- Multiplanetary systems
- Stars with proto-planetary discs

Exoplanets
- Discoveries
- Extremes
- Firsts
- Nearest
- Largest
- Heaviest
- Terrestrial candidates
- Kepler
- K2
- Potentially habitable
- Proper names

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

Other

Carl Sagan Institute
Exoplanet naming convention
Exoplanet phase curves
Exoplanetary Circumstellar Environments and Disk Explorer
Extragalactic planet
Fulton gap
Geodynamics of terrestrial exoplanets
Neptunian Desert
Nexus for Exoplanet System Science
Planets in globular clusters
Planets in science fiction
Sudarsky's gas giant classification

Discoveries of exoplanets
Search projects

2022 in space

« 2021

2023 »

Space probe launches

CAPSTONE (June 2022)
Danuri (August 2022)

Impact events

2022 EB5

Selected NEOs

Discoveries

2021 RR205 Alcyoneus (galaxy) CEERS-93316 GLASS-z13 GNz7q HD1 (galaxy) J1144–4308 OGLE-2011-BLG-0462 PKS 2131-021 PSR J0901–4046 PSR J0952–0607 Sagittarius A* imaged S4716 VFTS 243 Webb's First Deep Field (SMACS J0723.3–7327) WD 1054–226 WHL0137-LS
Exoplanets	AB Aurigae b CO₂ on WASP-39b Gliese 514 b Gliese 896 Ab HD 83443 c HD 260655 (b · c) K2-2016-BLG-0005Lb Kepler-451 (c · d) Kepler-1708b and possible exomoon Kepler-1708b I LP 890-9 (b · c) Mu2 Scorpii (b · c) Pi Mensae d Proxima Centauri d TOI-1452 b

Comets

Space exploration

DART (Dimorphos impact; September 2022)

Outer space portal
Category:2021 in space — Category:2022 in space — Category:2023 in space

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