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Esta lista de exoplanetas descobertos em 2022 é uma lista de exoplanetas confirmados que foram relatados pela primeira vez em 2022. Para exoplanetas detectados apenas pela velocidade radial, o valor listado para massa é um limite inferior. Consulte Massa mínima para obter mais informações.

Em 31 de março de 2022, K2-2016-BLG-0005Lb foi relatado como o exoplaneta mais distante encontrado pelo Kepler até o momento.^[1]^[2]

Nome	Massa (`M`_J)	Raio (`R`_J)	Período (dais)	Semieixo maior (AU)	Temp. (K)	Método de descoberta	Distância (ly)	Massa da estrela-mãe (`M`_☉)	Temperatura da estrela-mãe (K)	Observações
HD 22532 b	2.12±0.09		872.6±2.8	1.900±0.004		Vel. radial	526±2	1.20±0.05	5067+59 −22	Estrela-mãe gigante^[3]
HD 64121 b	2.56±0.19		623.0±3.4	1.510±0.006		Vel. radial	424.1±1.7	1.18±0.05	5066+58 −60	Estrela-mãe gigante^[3]
HD 69123 b	3.04±0.16		1193.3±7.0	2.482±0.010		Vel. radial	245.0±1.3	1.43±0.07	4787+280 −51	Estrela-mãe gigante^[3]
HD 29399 b	1.57±0.11		892.7±5.9	1.913±0.008		Vel. radial	144.2±0.3	1.15±0.04	4845±52	Estrela-mãe gigante^[4]
Kepler-1708b	<4.6	0.8886+0.0535 −0.0526	737.11310+0.00146 −0.00770	1.64±0.10		Trânsito	5436+334 −298	1.088±0.072	6157+231 −202	Possível hospedeiro de exolua^[5]^[6]
TOI-1064b	0.0425±0.0055	0.231±0.004	6.443868±0.000025	0.06152+0.00086 −0.00089	784±13	Trânsito	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	Trânsito	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		Trânsito	1780±20	1.325±0.118	4780±100	^[8]
TOI-4329b	0.45±0.09	1.50±0.19	2.9223±0.00015			Trânsito	2258±16	1.538±0.049	6000±100	^[8]
TOI-2669b	0.61±0.19	1.76±0.16	6.2034±0.0001			Trânsito	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	Trânsito	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		Microlente	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	Trânsito	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	Trânsito	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			Trânsito	923±3	1.12±0.03	5818±27	Exoplaneta muito denso, planeta adicional no sistema suspeito^[12]
Kepler-1972 c	0.0066±0.0020	0.078±0.005	11.3295±0.0011			Trânsito	923±3	1.12±0.03	5818±27	Exoplaneta muito denso, planeta adicional no sistema suspeito^[12]
TOI-206 b		0.116±0.004	0.7363104±0.0000003	0.0112±0.0001	910±36	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	51.64±0.02	0.309±0.014	3369±51	Outro exoplaneta no sistema é suspeito^[14]^[15]
TOI-1759 b	0.021±0.06	0.279±0.02	18.849975±0.000006	0.1176±0.0013	433±14	Trânsito	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		Tempo	1340±20	0.48+0.12		^[18]
Kepler-451 d	1.76±0.18		43.0±0.1	0.20±0.03		Tempo	1340±20	0.48+0.12		^[18]
KMT-2021-BLG-1391b	0.0143±0.0073			2.29+0.56 −0.71		Microlente	19000+3000 −5000	0.37±0.19		^[19]
KMT-2021-BLG-1253b	0.0599+0.0643 −0.0319			1.52+0.57 −0.41		Microlente	22000+3000 −4000	0.24+0.26 −0.13		^[19]
KMT-2021-BLG-1372b	0.1928±0.1129			2.37±0.77		Microlente	19000+5000 −8000	0.42±0.25		^[19]
KMT-2021-BLG-0748b	0.45+0.40 −0.25			2.43±0.67		Microlente	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	Vel. radial	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	Trânsito	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	Trânsito	108.82±0.07	0.34±0.02	3342±100	^[22]^[23]
PSR J2007+3120 b	0.0072±0.0009		723±8			Tempo	22000			Planeta pulsar, outro planeta do sistema é suspeito^[24]
Pi Mensae d	0.0421±0.0042		124.64+0.48 −0.52			Vel. radial	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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito		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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito				^[26]
K2-407 c	0.0078±0.0044	0.121+0.008 −0.007	9.22453+0.00132 −0.00091		900	Trânsito				^[26]
K2-408 b	0.0122±0.0062	0.149+0.010 −0.009	20.97895+0.00130 −0.00124		610	Trânsito				^[26]
K2-409 b	0.0212±0.0127	0.221+0.015 −0.014	1.90808+0.00004 −0.00005		1800	Trânsito				^[26]
EPIC 206317286 c	0.0168±0.098	0.186+0.015 −0.014	17.51547+0.00228 −0.00296		570	Trânsito		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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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		Vel. radial	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		Microlente	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		Microlente	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	Microlente	17000±700	0.58±0.03		^[1]
KMT-2019-BLG-1042Lb	0.19+0.21 −0.11			1.7±0.5		Microlente	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		Microlente	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		Microlente	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	Trânsito	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		Microlente	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		Microlente	19000+6000 −8000	0.69+0.41 −0.38		^[36]
KMT-2018-BLG-2004b	0.27±\0.12			4.62+0.80 −1.10		Microlente	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		Microlente	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		Microlente		0.28+0.22 −0.13		Várias soluções para separação congelada^[36]
OGLE-2018-BLG-1544b	11.2+6.3 −5.9			6.21+1.32 −2.10		Microlente	21000+4000 −7000	0.62+0.38 −0.36		Várias soluções para separação congelada^[36]
OGLE-2018-BLG-0932b	0.89+0.36 −0.31			1.75+0.24 −0.23		Microlente	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		Microlente	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		Microlente	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		Vel. radial	133.6±0.2	1.00±0.03	5442±17	Órbita excêntrica devido a um Júpiter quente no sistema^[37]
OGLE-2019-BLG-1470LABc	2.2+1.8 −1.3			3.1+1.2 −1.1		Microlente	20000±4000	0.55+0.17		Planeta circumbinário^[38]
Gliese 514b	0.0164±0.0028		140.43±0.41	0.422+0.014 −0.015	202±11	Vel. radial	24.850±0.010	0.510±0.051	3714±51	Órbita planetária parcialmente em zona habitável^[39]
TOI-1710 b	0.0890±0.0148	0.477±0.010	24.283429±0.00043	0.16±0.04	687±50	Trânsito	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	Trânsito	32.63±0.07	0.439±0.011	3803±10	Estrela-mãe também conhecida como TOI-4599^[41]
HD 260655 c	0.0097±0.0015	0.137±0.004	5.70588±0.00007	0.04749±0.00039	557±3	Trânsito	32.63±0.07	0.439±0.011	3803±10	Estrela-mãe também conhecida como TOI-4599^[41]
KMT-2021-BLG-0240 b	0.40+0.07 −0.08			2.5+2.8 −1.9		Microlente	23000+3000 −5000	0.47+0.33 −0.24		Várias soluções para a separação orbital^[42]
KMT-2021-BLG-0240 c	0.64+0.25 −0.24			1.0+1.1 −0.8		Microlente	23000+3000 −5000	0.47+0.33 −0.24		Várias soluções para a separação orbital^[42]
KMT-2021-BLG-1898 b	0.73+0.50 −0.40			1.9+0.3 −0.5		Microlente	23000+3000 −4000	0.48+0.33 −0.26		Possivelmente um sistema estelar binário^[43]
TOI-1246 b	0.0255±0.0035	0.269±0.005	4.30744±0.00002	0.049±0.002	955	Trânsito	557.9±1.0	1.12±0.16	5217±50	^[44]
TOI-1246 c	0.0277±0.0038	0.224±0.007	5.904144±0.000083	0.061±0.002	860	Trânsito	557.9±1.0	1.12±0.16	5217±50	^[44]
TOI-1246 d	0.0167±0.0053	0.313±0.008	18.65590±0.00048	0.131±0.004	586	Trânsito	557.9±1.0	1.12±0.16	5217±50	^[44]
TOI-1246 e	0.0466±0.0072	0.338±0.014	37.9216±0.0010	0.211±0.007	462	Trânsito	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	Trânsito	191.2±0.4	1.094+0.024 −0.007	5991±50	Estrela-mãe também conhecida como TOI-4399, compartilha sistema com uma anã vermelha^[45]
HIP 34269 b	0.0052±0.0007	0.103±0.005	0.548177±0.000019	0.01188±0.00040	1617±41	Trânsito	154.81±0.15	0.740±0.017	4440±100	Estrela-mãe também conhecida como TOI-500^[46]
HIP 34269 c	0.0146±0.0016		6.6356±0.0040			Vel. radial	154.81±0.15	0.740±0.017	4440±100	Estrela-mãe também conhecida como TOI-500^[46]
HIP 34269 d	0.1055±0.0033		26.233±0.020			Vel. radial	154.81±0.15	0.740±0.017	4440±100	Estrela-mãe também conhecida como TOI-500^[46]
HIP 34269 e	0.0376±0.0042		61.30±0.28			Vel. radial	154.81±0.15	0.740±0.017	4440±100	Estrela-mãe também conhecida como TOI-500^[46]
TOI-1820 b	2.3±0.2	1.12±0.02	4.860700±0.000010	0.069±0.005	1295±11	Trânsito	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	Trânsito	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	Trânsito	652±3	1.12±0.12	5673±50	^[47]
HIP 63374 B	11±3			30.02±0.12		Imagem direta	176.4±0.3	1.211±0.006		^[48]
HIP 60584 B	8±3			16.58±0.15		Imagem direta	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	Trânsito	1013±3	1.38+0.086 −0.082	6260±100	Estrela-mãe subgigante^[49]
TOI-1516 b	3.16±0.12	1.36±0.03	2.056014±0.000002		1820	Trânsito	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	Trânsito	940±3	1.153+0.100 −0.093	6160±100	Estrela-mãe jovem^[49]
WASP-132c	0.165±0.009		1.011534±0.000005	0.0182±0.0003		Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	733±5	1.720+0.057 −0.068	6189±67	Estrela-mãe também conhecida como 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	Trânsito	988±13	1.516+0.085 −0.10	6630+300 −290	Planeta orbitando primário de estrela binária^[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	Trânsito	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	Trânsito	930±14	1.861+0.086 −0.081	7360+290 −270	^[51]
Mu2 Scorpii b	14.4			290		imaging	474	9.1	21900	^[52]
Mu2 Scorpii c	18.5			21		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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	1126±3	1.082+0.052 −0.049	5974±110	Também 0.54`M`_☉ estrela no sistema^[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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	733±4	1.016+0.047 −0.052	5521±110	Também 0.6`M`_☉ estrelas no sistema^[54]
TOI-3540 b	1.18±0.14	2.10	3.1199990±0.0000079	0.04289+0.00092 −0.00093	1498±22	Trânsito	921±10	1.081+0.071 −0.069	5969±50	Também 0.8`M`_☉ estrelas no sistema^[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	Trânsito	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	Trânsito	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		Trânsito	1201±7	0.949±0.066	5470±110	Primeiro exoplaneta confirmado descoberto por Gaia, junto com Gaia-2b^[55]
Gaia-2b	0.817±0.047	1.322±0.013	3.6915224±0.0000039	0.0467±0.0015		Trânsito	676±3	1.000±0.095	5720±84	Primeiro exoplaneta confirmado descoberto por Gaia, junto com Gaia-1b^[55]
OGLE-2017-BLG-1691Lb	0.046+0.037 −0.025			2.41+0.34 −0.44		Microlente	24000+3000 −4000	0.45+0.36 −0.25		Estrela-mãe também conhecida como KMT-2017-BLG-0752^[56]
KMT-2021-BLG-0320Lb	0.10+0.13 −0.07			1.54+0.24 −0.30		Microlente	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		Microlente	20000+3000 −5000	0.57+0.32 −0.29		Estrela-mãe também conhecida como MOA-2021-BLG-182^[56]
KMT-2021-BLG-1554Lb	0.12+0.20 −0.07			0.72+0.13 −0.14		Microlente	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	Trânsito	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		Vel. radial	36.594±0.011	0.1774±0.0045	3071+34 −22	Estrela-mãe também conhecida como Gliese 585, planeta próximo da zona habitável^[58]
KMT-2021-BLG-0171Lb	0.0352+0.0173 −0.0142			3.5+1.3 −1.0		Microlente	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		Microlente	23000+2000 −4000	0.58+0.33 −0.27		^[59]
HD 33142 d	0.89+0.06 −0.05		810.2+3.8 −4.2	1.955+0.016 −0.012		Vel. radial	394.3±0.9	1.52±0.03	5025.4+23.6 −15.5	Estrela-mãe gigante^[60]
TOI-2048 b		0.184±0.018	13.79019+0.00065 −0.00084		640±20	Trânsito	379.7±0.5	0.83±0.03	5185±60	Estrela-mãe jovem pertence a NGC 3532^[61]
Kepler-1656 c	0.40±0.09		1919+27 −24	3.053±0.049		Vel. radial		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	Trânsito	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	Trânsito	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		Microlente	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		Microlente	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		Microlente	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		Microlente	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		Microlente	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		Microlente	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	Trânsito	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	Vel. radial	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	Trânsito	504.17+0.12 −0.09	0.981+0.062 −0.065	5840±62	Outro planeta no sistema é suspeito^[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	Trânsito	1195±8	1.47±0.09	5980±80	Exolaneta em órbita excêntrica, estrela-mãe também conhecida como 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	Trânsito	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		Microlente	10000+3000 −2000	0.22+0.12 −0.07		^[68]
KMT-2021-BLG-0909b	1.26+1.01 −0.66			1.75±0.42		Microlente	21000+3000 −5000	0.38+0.30 −0.20		^[68]
KMT-2021-BLG-2478b	0.80+0.56 −0.35			1.38±0.26		Microlente	8000+4000 −3000	0.12+0.09 −0.06		^[68]
KMT-2021-BLG-1105b	1.30±0.68			3.54±1.06		Microlente	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	Trânsito	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	Trânsito	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	Vel. radial	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	Trânsito	268.6±1.3	1.109±0.043	5987±64	Estrela-mãe também conhecida como TOI-1797^[70]
HD 93963A c		0.288±0.005	3.6451398+0.0000106 −0.0000142	0.04813±0.00085	1344±18	Trânsito	268.6±1.3	1.109±0.043	5987±64	Estrela-mãe também conhecida como TOI-1797^[70]
GJ 3090 b	0.0105	0.19	2.8531042±0.0000032	0.03165	696	Trânsito	73.21±0.04	0.519±0.013	3556±70	Estrela-mãe também conhecida como TOI-177^[71]
GJ 3090 c	0.0538		12.734+0.033 −0.026	0.08575	421	Vel. radial	73.21±0.04	0.519±0.013	3556±70	Estrela-mãe também conhecida como TOI-177^[71]
OGLE-2019-BLG-0362Lb	3.26+0.83 −0.58			2.18+0.58 −0.72		Microlente	19000±2000	0.42+0.34 −0.23		Múltiplas soluções para parâmetros planetários^[72]
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	Vel. radial	125.1±2.6	1.24	6486	Algum deutério queimando apesar de sua baixa massa, também outra anã marrom está presente no sistema^[73]
TOI-2196 b	0.0818±0.0041	0.313±0.013	1.1947268+0.0000079 −0.0000093	0.02234±0.00060	1860±20	Trânsito	861±3	1.032±0.038	5634±31	Deserto Neptuniano desértico^[74]
TOI-1452 b	0.0152±0.0041	0.149±0.006	11.06201±0.00002	0.061±0.003	326±7	Trânsito	99.51±0.04	0.249±0.008	3185±50	Também uma anã vermelha em uma separação de 97 UA no sistema^[75]
HD 56414 b	0.0944±0.0053	0.331±0.018	29.04992±0.00021	0.229±0.004	1133±30	Trânsito	873±3	1.89±0.11	8500±150	Estrela-mãe também conhecida como 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	Trânsito	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	Trânsito	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	Trânsito	1131±12	1.218+0.054 −0.048	6096±32	Órbita altamente excêntrica^[78]
HD 21019 b	0.014±0.002		2.56	0.034±0.002		Vel. radial	120			Estrela-mãe também conhecida como GJ 2030^[79]
HD 21019 c	12.934±2.361		25600±2500	16.752±1.312		Vel. radial	120			Estrela-mãe também conhecida como GJ 2030^[79]
HD 21175 b	0.038±0.010		10.6	0.091±0.004		Vel. radial	57.7			Estrela-mãe também conhecida como GJ 3222, planeta em órbita extremamente excêntrica, também anã marrom no sistema^[79]
HD 199981 b	10.070±2.483		21000±8000	13.048±3.073		Vel. radial	66.7±2.4			Estrela-mãe também conhecida como GJ 9714^[79]
HD 105618 b	0.079±0.008		9.9	0.091±0.004		Vel. radial	227.8±0.4			Também anã marrom no sistema^[79]
KMT-2017-BLG-0673Lb	3.67+2.17 −2.07			2.34+0.56 −0.74		Microlente	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		Microlente	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		Microlente	11000+6000 −4000	0.69+0.34 −0.30		Múltiplas soluções orbitais^[81]
KMT-2021-BLG-0192Lb	0.19+0.09 −0.10			2.07+0.35 −0.47		Microlente	22000+3000 −5000	0.55+0.26 −0.28		Múltiplas soluções orbitais^[81]
KMT-2021-BLG-2294Lb	0.07+0.10 −0.03			0.94±0.16		Microlente	22000±3000	0.11+0.17 −0.06		Múltiplas soluções orbitais^[81]
HD 3167 e	0.0306±0.0037		102.09+0.52 −0.50	0.4048+0.0077 −0.0074	375±7	Vel. radial	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			Trânsito	364.6	1.00±0.05	5542.3±100.0	^[83] Estrela-mãe também conhecida como BD+82 71, planeta suspeito desde 2020^[84]
TOI-1669 c	0.602±0.078		501±16			Vel. radial	364.6	1.00±0.05	5542.3±100.0	^[83] Estrela-mãe também conhecida como BD+82 71, suspeita-se de uma companheira adicional de longo período
TOI-1694 b	0.0979±0.0066	0.461±0.016	3.8			Trânsito	405.7	0.84±0.03	5066±100	^[83] Estrela-mãe também conhecida como TYC 4108-1434-1, exoplaneta suspeito desde 2020^[84]
TOI-1694 c	0.929±0.037		393.2±4.3			Vel. radial	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		Vel. radial	200.2	1.35+0.19 −0.21	4971	Estrela-mãe gigante vermelha também conhecida como HD 184010^[85]
HR 7321 c	0.28+0.08 −0.10		483.3+3.2 −4.0	1.332+0.006 −0.007		Vel. radial	200.2	1.35+0.19 −0.21	4971	Estrela-mãe gigante vermelha também conhecida como HD 184010^[85]
HR 7321 d	0.46±0.08		837.7+6.4 −5.5	1.922+0.010 −0.008		Vel. radial	200.2	1.35+0.19 −0.21	4971	Estrela-mãe gigante vermelha também conhecida como HD 184010^[85]
HD 22946 b		0.154±0.009	4.040301+0.000023 −0.000042	0.0528±0.0030	1378±36	Trânsito	205.08±0.16	1.158±0.058	6210+173 −158	Estrela-mãe também conhecida como TOI-411, terceiro exoplaneta em trânsito no sistema é suspeito^[86]
HD 22946 c		0.245±0.013	9.573096+0.000026 −0.000023	0.0939±0.0054	1033±27	Trânsito	205.08±0.16	1.158±0.058	6210+173 −158	Estrela-mãe também conhecida como TOI-411, terceiro exoplaneta em trânsito no sistema é suspeito^[86]
TOI-5205b	1.08±0.06	1.03±0.03	1.630757±0.000001	0.0199±0.0002	737±15	Trânsito	283.35±0.16	0.392±0.015	3430±54	^[87]
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	Trânsito	127.48±0.06	0.67±0.03	4684±99	^[88]
HD 23472 e	0.0023±0.0009	0.073±0.006	7.90754±0.00011	0.0680±0.0010	723+28 −25	Trânsito	127.48±0.06	0.67±0.03	4684±99	^[88]
HD 23472 f	0.0024±0.0013	0.102±0.007	12.1621839+0.00012 −0.000099	0.0906±0.0014	630+27 −23	Trânsito	127.48±0.06	0.67±0.03	4684±99	^[88]
TOI-1221 b		0.259±0.011	91.68278+0.00032 −0.00041	0.404+0.026 −0.023	400	Trânsito	447.1±0.7	1.03±0.06	5592±50	^[89]
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	Trânsito	566.3±1.0	1.074+0.059 −0.050	5607+86 −82	^[90]
TOI-2000 c	0.238±0.012	0.711±0.011	9.1270553±0.0000073	0.0875+0.0016 −0.0014	1029+84 −111	Trânsito	566.3±1.0	1.074+0.059 −0.050	5607+86 −82	^[90]
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	Trânsito	1154±12	0.890+0.056 −0.031	5700±80	^[91]
NGTS-21b	2.36±0.21	1.33±0.03	1.5433897±0.0000016	0.0236±0.0005	1357±15	Trânsito	2090+90 −80	0.72±0.04	4660±41	^[92]
MOA-2020-BLG-208Lb	0.217+0.116 −0.106			2.88+0.40 −0.41		Microlente	25000±3000	0.656+0.346 −0.322		^[93]
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	Trânsito	126.02±0.06	0.863±0.020	5145±50	Estrela-mãe também conhecida como TOI-179, também estrela anã vermelha no sistema^[94]^[95]^[96]
TOI-969 b	0.0286±0.0031	0.247±0.033	1.8237305+0.0000020 −0.0000021	0.02636±0.00017	941±31	Trânsito	253.8±0.5	0.730±0.037	4550±75	^[97]
TOI-969 c	11.3+1.1 −0.9		1700+290 −280	2.52+0.27 −0.29	96.4+6.8 −5.8	Vel. radial	253.8±0.5	0.730±0.037	4550±75	Órbita excêntrica^[97]
TOI-1136 b	0.0095+0.0022 −0.0028	0.170+0.019 −0.013	4.1728±0.0002			Trânsito	275.8±0.5	1.022±0.027	5770±50	^[98]
TOI-1136 c	0.0189+0.0041 −0.0053	0.257±0.005	6.2573±0.0002			Trânsito	275.8±0.5	1.022±0.027	5770±50	^[98]
TOI-1136 d	0.0252+0.0076 −0.0060	0.413±0.007	12.5194±0.0004			Trânsito	275.8±0.5	1.022±0.027	5770±50	^[98]
TOI-1136 e	0.0170±0.0031	0.236+0.006 −0.008	18.7992+0.0017 −0.0015			Trânsito	275.8±0.5	1.022±0.027	5770±50	^[98]
TOI-1136 f	0.0261+0.0088 −0.0113	0.346±0.010	26.3162+0.0017 −0.0013			Trânsito	275.8±0.5	1.022±0.027	5770±50	^[98]
TOI-1136 g	0.0151+0.0148 −0.0104	0.226±0.010	39.5387+0.0036 −0.0030			Trânsito	275.8±0.5	1.022±0.027	5770±50	^[98]
TOI-3884 b	0.0519+0.0110 −0.0057	0.563±0.025	4.5445697±0.0000094	0.0354±0.0014	463±12	Trânsito	141.37±0.16	0.2813±0.0067	3269±70	^[99]^[100]
EPIC 210768568 b		0.088±0.004	3.2141±0.0002	0.0511+0.0021 −0.0028		Trânsito	965	1.018±0.131	5711±105	^[101]
EPIC 246078343 b		0.068±0.007	0.8094±0.00003	0.0117+0.0009 −0.0012		Trânsito	954	0.808+0.364 −0.256	4116±138	^[101]
EPIC 246078343 c		0.110±0.006	5.3301±0.0003	0.0426+0.0016 −0.0019		Trânsito	954	0.808+0.364 −0.256	4116±138	^[101]
EPIC 246220667 b		0.172±0.006	6.6690±0.0002	0.0552+0.0017 −0.0023		Trânsito	835	0.814+0.363 −0.251	4343±138	^[101]
EPIC 246220667 c		0.109±0.006	4.3696±0.0001	0.0487+0.0027 −0.0031		Trânsito	835	0.814+0.363 −0.251	4343±138	^[101]
EPIC 247422570 b		0.189±0.009	5.9382+0.0006 −0.0004	0.0586+0.0032 −0.0033		Trânsito	2181	0.893+0.406 −0.275	5590±138	^[101]
KMT-2017-BLG-1194b	0.011±0.006			1.78+0.45 −0.46		Microlente	14000±6000	0.41+0.23 −0.19		^[102]
KMT-2017-BLG-0428b	0.018+0.011 −0.009			1.81+0.55 −0.59		Microlente	18000+6000 −8000	0.34+0.22 −0.17		^[102]
KMT-2019-BLG-1806b	0.015±0.005			3.02+0.70 −0.73		Microlente	22000+2000 −7000	0.74±0.25		^[102]
KMT-2017-BLG-1003b	0.016+0.017 −0.009			1.38+0.39 −0.32		Microlente	23000±2000	0.32+0.31 −0.17		^[102]
KMT-2019-BLG-1367b	0.013+0.008 −0.007			1.70+0.50 −0.56		Microlente	15000+8000 −7000	0.25+0.16 −0.13		^[102]
OGLE-2017-BLG-1806b	0.017+0.015 −0.009			1.75+0.46 −0.47		Microlente	21000+3000 −5000	0.38+0.34 −0.20		^[102]
KMT-2016-BLG-1105b	0.007+0.023 −0.005			2.44+0.88 −0.75		Microlente	17000±7000	0.41+0.25 −0.21		^[102]
L 363-38 b	0.0147±0.0014		8.781±0.007	0.048±0.006	330	Vel. radial	33.31	0.21	3129	Estrela-mãe também conhecida como Gliese 3049^[103]
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	Trânsito	200.4+0.6 −2.2	0.604±0.030	3875±75	^[104]
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	Trânsito	1366±6	1.072+0.059 −0.064	5814+91 −93	^[105]
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	Trânsito	713±6	0.954+0.041 −0.046	5306+76 −68	^[105]
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	Trânsito	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	Trânsito	1242±10	1.15+0.14 −0.07	5760+80 −79	^[105]
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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	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	Trânsito	1281±5	1.12+0.11 −0.06	5760+85 −88	^[105]
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	Trânsito	899±3	1.186+0.059 −0.083	5706+95 −91	^[105]
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	Trânsito	1308±6	1.199+0.072 −0.076	5950±100	^[105]
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	Trânsito	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	Trânsito	1834±17	1.242+0.057 −0.076	5859+72 −71	^[105]
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	Trânsito	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	Trânsito	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	Trânsito	1013±4	1.178+0.039 −0.042	6060+74 −67	^[105]
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	Trânsito	668.7±1.3	0.905+0.043 −0.044	5281+86 −76	^[105]
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	Trânsito	579.5±1.8	1.056+0.059 −0.063	5640+89 −82	^[105]
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	Trânsito	1051±6	1.242+0.072 −0.077	6058+99 −94	^[105]
TOI-4582 b	0.53±0.05	0.94+0.09 −0.12	31.034±0.001			Trânsito	1242	1.34±0.06	5190±100	Estrela evoluída, órbita planetária excêntrica^[106]
HD 191939 g	0.0425±0.0063		284+10 −8	0.812±0.028	278±6	Vel. radial	174.4±0.1	0.81±0.04	5348±100	Exoplaneta em zona habitável^[107]
NGTS-23b	0.613±0.097	1.267±0.030	4.0764326±0.0000041	0.0504±0.012	1327+17 −16	Trânsito	3230±70	1.01+0.06 −0.07	6057±64	^[108]
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	Trânsito	2360±80	1.26+0.05 −0.21	5820+93 −8	^[108]
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	Trânsito	2350±30	0.91+0.03 −0.04	5321±58	^[108]
HD 20329b	0.0233±0.0034	0.154±0.006	0.926118+0.000050 −0.000043	0.0180±0.0003	2141±27	Trânsito	207.7±0.9	0.90±0.05	5596±50	^[109]
TOI-1695 b	0.0173±0.0031	0.181±0.016	3.1342790±0.0000072	0.033548+0.000260 −0.000268	590±90	Trânsito	147.2±0.2	0.51±0.02	3627±31	^[110]^[111]
HD 167768 b	0.85+0.12 −0.11		20.6532+0.0032 −0.0032	0.1512+0.0058 −0.0063	1874	Vel. radial	353.5	1.08+0.14 −0.12	4830	Estrela-mãe gigante vermelha também conhecida como HR 8640, outros exoplanetas no sistema são suspeitos^[112]
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	Trânsito	314±2	0.781±0.042	4994±50	^[113]
HD 114082 b	8.0±1.0	1.00±0.03	109.75+0.40 −0.37	0.5109+0.0081 −0.0083		Trânsito	310.1±0.7	1.47±0.07	6651±35	Estrela-mãe jovem, órbita planetária excêntrica^[114]^[115]
TOI-277 b	0.0239+0.0179 −0.0098	0.237±0.016	3.9940±0.0004	0.0269±0.0011		Trânsito	212.6+0.6 −0.3	0.16±0.01	4031+21 −23	^[116]
TOI-1288 b	0.0712+0.0574 −0.0304	0.454±0.010	2.69998±0.00015	0.0429±0.0006		Trânsito	375.3+1.3 −0.5	1.46±0.06	5307+18 −16	^[116]
TOI-1288 c	0.2643±0.0220		443+11 −13			Vel. radial	375.3+1.3 −0.5	1.46±0.06	5307+18 −16	^[117]
29 Cygni b	13.9+6.1 −5.1			16.9+3.4 −1.9		Imagem direta	130.9±0.9	2.14±0.15	8790+1513 −1292	Estrela-mãe também conhecida como HIP 99770^[118]
HD 109833 b		0.258+0.014 −0.012	9.188526±0.000026			Trânsito	259.5±0.2	1.08±0.05	5881±50	Estrela-mãe jovem também conhecida como TOI-1097^[119]
HD 109833 c		0.231+0.018 −0.016	13.900148±0.000057			Trânsito	259.5±0.2	1.08±0.05	5881±50	Estrela-mãe jovem também conhecida como TOI-1097^[119]
TOI-1260 d	0.0373±0.0245	0.276±0.008	16.608164±0.000083	0.1116±0.0033	499±4	Trânsito	239.5±0.3	0.66±0.01	4227±85	^[120]
Gliese 1002 b	0.0034±0.0004		10.3465±0.027	0.0457±0.0013	230.9±6.7	Vel. radial	15.808±0.003	0.120±0.010	3024±52	Exoplaneta em zona habitável^[121]
Gliese 1002 c	0.0043±0.0005		21.202±0.013	0.0738±0.0021	181.7±5.2	Vel. radial	15.808±0.003	0.120±0.010	3024±52	Exoplaneta em zona habitável^[121]
TOI-778 b	2.76±0.24	1.375±0.045	4.633611±0.000001	0.060±0.003	1561+33 −32	Trânsito	530±4	1.428±0.094	6715±128	^[122]
MOA-2019-BLG-008L b	30					Microlente	8000±2000	0.8		^[123]
TOI-5174 b	6998780100000000000♠0.07801	6999476670000000000♠0.47667	7001122140000000000♠12.214			Trânsito		7000100000000000000♠1.0±0.125		^[124]^[125]
GJ 463 b	3.6±0.4		3448+110 −88	3.53±0.07		Vel. radial	59.91±0.03	0.49±0.02	3540±41	Estrela-mãe também conhecida como Ross 690^[126]^[127]

Listas específicas de exoplanetas

Referências

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↑ ^a ^b Leleu, A.; Delisle, J. -B.; Mardling, R.; Udry, S.; Chatel, G.; Alibert, Y.; Eggenberger, P. (2022), «Alleviating the transit timing variation bias in transit surveys», Astronomy & Astrophysics, 661: A141, arXiv:2201.11459, doi:10.1051/0004-6361/202142822
↑ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m Giacalone, Steven; et al. (2022), «Validation of 13 Hot and Potentially Terrestrial TESS Planets», The Astronomical Journal, 163 (2): 99, Bibcode:2022AJ....163...99G, arXiv:2201.12661, doi:10.3847/1538-3881/ac4334
↑ Kemmer, J.; et al. (2022), «Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 B», Astronomy & Astrophysics, 659: A17, Bibcode:2022A&A...659A..17K, arXiv:2202.00970, doi:10.1051/0004-6361/202142653
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↑ 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, Bibcode:2022AJ....163..133E, arXiv:2202.01240, doi:10.3847/1538-3881/ac4af0
↑ 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, Bibcode:2022A&A...660A..86M, arXiv:2202.01259, doi:10.1051/0004-6361/202142540
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↑ Faria, J. P.; et al. (2022), «A candidate short-period sub-Earth orbiting Proxima Centauri», Astronomy & Astrophysics, 658: A115, Bibcode:2022A&A...658A.115F, arXiv:2202.05188, doi:10.1051/0004-6361/202142337
↑ Šubjak, J.; et al. (2022), «TOI-1268b: The youngest hot Saturn-mass transiting exoplanet», Astronomy & Astrophysics, 662: A107, Bibcode:2022A&A...662A.107S, arXiv:2201.13341, doi:10.1051/0004-6361/202142883
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↑ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m ⁿ ^o ^p ^q ^r ^s ^t ^u ^v ^w ^x ^y ^z ^aa ^ab ^ac ^ad ^ae ^af ^ag ^ah ^ai ^aj ^ak ^al ^am ^an ^ao ^ap ^aq ^ar ^as ^at ^au ^av ^aw ^ax ^ay ^az ^ba ^bb ^bc ^bd ^be ^bf ^bg ^bh Christiansen, Jessie L.; et al. (2022), «Scaling K2. V. Statistical Validation of 60 New Exoplanets from K2 Campaigns 2–18», The Astronomical Journal, 163 (6): 244, Bibcode:2022AJ....163..244C, arXiv:2203.02087, doi:10.3847/1538-3881/ac5c4c
↑ 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, Bibcode:2022AJ....163..298M, arXiv:2203.02694, doi:10.3847/1538-3881/ac6bf8
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↑ ^a ^b Tran, 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, Bibcode:2022AJ....163..225T, arXiv:2203.04334, doi:10.3847/1538-3881/ac5c4f
↑ 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, Bibcode:2022AJ....164...81K, arXiv:2203.07178, doi:10.3847/1538-3881/ac7c20
↑ Quirrenbach, 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
↑ ^a ^b Han, Cheongho; et al. (2022), «KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing», Astronomy & Astrophysics, 662: A70, Bibcode:2022A&A...662A..70H, arXiv:2203.16734, doi:10.1051/0004-6361/202243550
↑ ^a ^b ^c Zang, Weicheng; et al. (2022), «Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field», Monthly Notices of the Royal Astronomical Society, 515: 928–939, arXiv:2204.02017, doi:10.1093/mnras/stac1883
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↑ Stela Ishitani Silva; et al. (2022), «MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis», The Astronomical Journal, 164 (3): 118, Bibcode:2022AJ....164..118I, arXiv:2204.03672, doi:10.3847/1538-3881/ac82b8
↑ ^a ^b ^c ^d ^e ^f ^g ^h Gould, Andrew; et al. (2022), «Systematic KMTNet planetary anomaly search», Astronomy & Astrophysics, 664: A13, arXiv:2204.04354, doi:10.1051/0004-6361/202243744
↑ Errico, Adriana; Wittenmyer, Robert A.; Horner, Jonathan; Li, Zhexing; Brandt, G. Mirek; Kane, Stephen R.; Fetherolf, Tara; Holt, Timothy R.; Carter, Brad; Clark, Jake T.; Butler, R. P.; Tinney, C. G.; Ballard, Sarah; Bowler, Brendan P.; Kielkopf, John; Liu, Huigen; Plavchan, Peter P.; Shporer, Avi; Zhang, Hui; Wright, Duncan J.; Addison, Brett C.; Mengel, Matthew W.; Okumura, Jack (2022), «HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit», The Astronomical Journal, 163 (6): 273, Bibcode:2022AJ....163..273E, arXiv:2204.05711, doi:10.3847/1538-3881/ac6589
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↑ ^a ^b Luque, R.; et al. (2022), «The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc», Astronomy & Astrophysics, 664: A199, Bibcode:2022A&A...664A.199L, arXiv:2204.10261, doi:10.1051/0004-6361/202243834
↑ ^a ^b Han, Cheongho; Kim, Doeon; Yang, Hongjing; Gould, Andrew; Youn Kil Jung; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2022), «KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal», Astronomy & Astrophysics, 664: A114, Bibcode:2022A&A...664A.114H, arXiv:2204.11383, doi:10.1051/0004-6361/202243161
↑ Han, Cheongho; Gould, Andrew; Kim, Doeon; Youn Kil Jung; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2022), «KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars», Astronomy & Astrophysics, 663: A145, Bibcode:2022A&A...663A.145H, arXiv:2204.11378, doi:10.1051/0004-6361/202243102
↑ ^a ^b ^c ^d Turtelboom, Emma V.; et al. (2022), «The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI–1246», The Astronomical Journal, 163 (6): 293, Bibcode:2022AJ....163..293T, arXiv:2204.11895, doi:10.3847/1538-3881/ac69e5
↑ Zhou, George; et al. (2022), «A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor Member HIP 94235», The Astronomical Journal, 163 (6): 289, Bibcode:2022AJ....163..289Z, arXiv:2204.11975, doi:10.3847/1538-3881/ac69e3
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↑ ^a ^b ^c 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, 515: 1328–1345, arXiv:2205.09046, doi:10.1093/mnras/stac1383
↑ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j Yee, Samuel W.; et al. (2022), «The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets», The Astronomical Journal, 164 (2): 70, Bibcode:2022AJ....164...70Y, arXiv:2205.09728, doi:10.3847/1538-3881/ac73ff
↑ ^a ^b Panahi, Aviad; Zucker, Shay; Clementini, Gisella; Audard, Marc; Binnenfeld, Avraham; Cusano, Felice; Evans, Dafydd Wyn; Gomel, Roy; Holl, Berry; Ilyin, Ilya; De Fombelle, Grégory Jevardat; Mazeh, Tsevi; Mowlavi, Nami; Nienartowicz, Krzysztof; Rimoldini, Lorenzo; Shahaf, Sahar; Eyer, Laurent (2022). «The detection of transiting exoplanets by Gaia». Astronomy & Astrophysics. 663: A101. Bibcode:2022A&A...663A.101P. arXiv:2205.10197. doi:10.1051/0004-6361/202243497
↑ ^a ^b ^c ^d Han, Cheongho; et al. (2022), «Four sub-Jovian-mass planets detected by high-cadence microlensing surveys», Astronomy & Astrophysics, 664: A33, Bibcode:2022A&A...664A..33H, arXiv:2205.10510, doi:10.1051/0004-6361/202243484
↑ 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, Bibcode:2022A&A...664A..94P, arXiv:2205.10854, doi:10.1051/0004-6361/202243454
↑ Harakawa, Hiroki; et al. (2022), «A super-Earth orbiting near the inner edge of the habitable zone around the M4.5 dwarf Ross 508», Publications of the Astronomical Society of Japan, 74 (4): 904–922, arXiv:2205.11986, doi:10.1093/pasj/psac044
↑ ^a ^b 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», Monthly Notices of the Royal Astronomical Society, 516 (2): 1894–1909, arXiv:2205.12584, doi:10.1093/mnras/stac2023
↑ Trifonov, Trifon; Wollbold, Anna; Kürster, Martin; Eberhardt, Jan; Stock, Stephan; Henning, Thomas; Reffert, Sabine; Butler, R. Paul; Vogt, Steven S.; Reiners, Ansgar; Lee, Man Hoi; Bitsch, Bertram; Zechmeister, Mathias; Rodler, Florian; Perdelwitz, Volker; Tal-Or, Lev; Rybizki, Jan; Heeren, Paul; Gandolfi, Davide; Barragán, Oscar; Zakhozhay, Olga; Sarkis, Paula; Pinto, Marcelo Tala; Kossakowski, Diana; Wolthoff, Vera; Brems, Stefan S.; Passegger, Vera Maria (2022), «A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System», The Astronomical Journal, 164 (4): 156, Bibcode:2022AJ....164..156T, arXiv:2206.03899, doi:10.3847/1538-3881/ac7ce0
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↑ Heitzmann, Alexis; et al. (2023), «TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star», The Astronomical Journal, 165 (3), p. 121, Bibcode:2023AJ....165..121H, arXiv:2208.10854, doi:10.3847/1538-3881/acb5a2
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↑ Bourrier, V.; et al. (2022), «A CHEOPS-enhanced view of the HD 3167 system», Astronomy & Astrophysics, 668: A31, arXiv:2209.06937, doi:10.1051/0004-6361/202243778
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↑ 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), p. 120, Bibcode:2023AJ....165..120K, arXiv:2209.11160, doi:10.3847/1538-3881/acabce
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↑ Mann, Christopher R.; Lafrenière, David; Dragomir, Diana; Quinn, Samuel N.; Tan, Thiam-Guan; Collins, Karen A.; Howell, Steve B.; Ziegler, Carl; Mann, Andrew W.; Stassun, Keivan G.; Kristiansen, Martti H.; Osborn, Hugh; Boyajian, Tabetha; Eisner, Nora; Hellier, Coel; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Seager, S.; Winn, Joshua N.; Jenkins, Jon M.; McLean, Brian; Rowden, Pamela; Torres, Guillermo; Caldwell, Douglas A.; Collins, Kevin I.; Schwarz, Richard P. (2023), «Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star», The Astronomical Journal, 165 (5), p. 217, Bibcode:2023AJ....165..217M, arXiv:2209.13651, doi:10.3847/1538-3881/acc8d4
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↑ Grieves, Nolan; et al. (2022), «An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542», Astronomy & Astrophysics, 668: A29, Bibcode:2022A&A...668A..29G, arXiv:2209.14830, doi:10.1051/0004-6361/202244077
↑ Alves, Douglas R.; et al. (2022), «NGTS-21b: An Inflated Super-Jupiter Orbiting a Metal-poor K dwarf», Monthly Notices of the Royal Astronomical Society, 517 (3): 4447–4457, arXiv:2210.01027, doi:10.1093/mnras/stac2884
↑ Olmschenk, Greg; et al. (2023), «MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert», The Astronomical Journal, 165 (4), p. 175, Bibcode:2023AJ....165..175O, arXiv:2210.02436, doi:10.3847/1538-3881/acbcc8
↑ Desidera, S.; et al. (2022), TOI-179: a young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit, arXiv:2210.07933
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↑ Vines, Jose I.; Jenkins, James S.; Berdiñas, Zaira; Soto, Maritza G.; Díaz, Matías R.; Alves, Douglas R.; Tuomi, Mikko; Wittenmyer, Robert A.; De Leon, Jerome Pitogo; Peña, Pablo; Lissauer, Jack J.; Ballard, Sarah; Bedding, Timothy; Bowler, Brendan P.; Horner, Jonathan; Jones, Hugh R A.; Kane, Stephen R.; Kielkopf, John; Plavchan, Peter; Shporer, Avi; Tinney, C. G.; Wright, Hui Zhang Duncan J.; Addison, Brett; Mengel, Matthew W.; Okumura, Jack; Samadi-Ghadim, Anya (2022), «A dense mini-Neptune orbiting the bright young star HD 18599», Monthly Notices of the Royal Astronomical Society, 518 (2): 2627–2639, arXiv:2210.07945, doi:10.1093/mnras/stac2845
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↑ ^a ^b ^c ^d ^e ^f Dai, Fei; et al. (2023), «TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain», The Astronomical Journal, 165 (2): 33, Bibcode:2023AJ....165...33D, arXiv:2210.09283, doi:10.3847/1538-3881/aca327
↑ 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, Bibcode:2022A&A...667L..11A, arXiv:2210.10909, doi:10.1051/0004-6361/202244791
↑ 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
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[Esmer2022-18] Ekrem Murat Esmer; Baştürk, Özgür; Selim Osman Selam; Aliş, Sinan (2022), «Detection of two additional circumbinary planets around Kepler-451», Monthly Notices of the Royal Astronomical Society, 511 (4): 5207–5216, arXiv:2202.02118, doi:10.1093/mnras/stac357

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[CadieuxHébrard2022-75] Cadieux, Charles; Doyon, René; et al. (27 de junho de 2022). «TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf» (publicado em 12 de agosto de 2022). The Astronomical Journal. 164:96 (3): 28pp. Bibcode:2022AJ....164...96C. arXiv:2208.06333. doi:10.3847/1538-3881/ac7cea

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[Shin2022-81] Shin, In-Gu; et al. (2023), «Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets», The Astronomical Journal, 165 (1): 8, Bibcode:2023AJ....165....8S, arXiv:2209.03886, doi:10.3847/1538-3881/ac9d93

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[Zandt2022-83] Van Zandt, Judah E.; et al. (2023), «TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey», The Astronomical Journal, 165 (2), p. 60, Bibcode:2023AJ....165...60V, arXiv:2209.06958, doi:10.3847/1538-3881/aca6ef

[Ciacalone2020-84] Giacalone, 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

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[Cacciapuoti2022-86] Cacciapuoti, Luca; et al. (2022), «TESS discovery of a super-Earth and two sub-Neptunes orbiting the bright, nearby, Sun-like star HD 22946», Astronomy & Astrophysics, 668: A85, Bibcode:2022A&A...668A..85C, arXiv:2209.09597, doi:10.1051/0004-6361/202243565

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[Barros2022-88] Barros, S. C. C.; et al. (2022), «HD 23472: A multi-planetary system with three super-Earths and two potential super-Mercuries», Astronomy & Astrophysics, 665: A154, Bibcode:2022A&A...665A.154B, arXiv:2209.13345, doi:10.1051/0004-6361/202244293

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[Sha2022-90] Sha, Lizhou; et al. (2023), «TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system», Monthly Notices of the Royal Astronomical Society, arXiv:2209.14396, doi:10.1093/mnras/stad1666

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[Hoyer2022-97] Lillo-Box, J.; et al. (2023), «TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter», Astronomy & Astrophysics, 669, pp. A109, Bibcode:2023A&A...669A.109L, arXiv:2210.08996, doi:10.1051/0004-6361/202243879

[Dai2022-98] ↑ ^a ^b ^c ^d ^e ^f Dai, Fei; et al. (2023), «TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain», The Astronomical Journal, 165 (2): 33, Bibcode:2023AJ....165...33D, arXiv:2210.09283, doi:10.3847/1538-3881/aca327

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[Ser2022-101] ↑ ^a ^b ^c ^d ^e ^f Del Ser, D.; Fors, O.; Del Alcázar, M.; Dyachenko, V.; Horch, E. P.; Tokovinin, A.; Ziegler, C.; Van Belle, G. T.; Clark, C. A.; Hartman, Z. D. (2023), «TFAW survey II: Six newly validated planets and 13 planet candidates from K2», Monthly Notices of the Royal Astronomical Society, 518: 669–690, arXiv:2210.10805, doi:10.1093/mnras/stac3087

[Zang2022-10-102] ↑ ^a ^b ^c ^d ^e ^f ^g Zang, Weicheng; et al. (2023), «Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10−4 Planets from the First 4 yr Survey», The Astronomical Journal, 165 (3), p. 103, Bibcode:2023AJ....165..103Z, arXiv:2210.12344, doi:10.3847/1538-3881/acb34b

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[Yee2022-10-105] ↑ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m ⁿ ^o ^p ^q ^r ^s ^t Yee, Samuel W.; et al. (2023), «The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets», The Astrophysical Journal Supplement Series, 265 (1), p. 1, Bibcode:2023ApJS..265....1Y, arXiv:2210.15473, doi:10.3847/1538-4365/aca286

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Lista de exoplanetas descobertos em 2022

Listas específicas de exoplanetas

Referências