List of exoplanets discovered in 2022

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This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

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.

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

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

List of exoplanets discovered before 2000 (31)
List of exoplanets discovered between 2000–2009 (377)
List of exoplanets discovered in 2010 (109)
List of exoplanets discovered in 2011 (179)
List of exoplanets discovered in 2012 (149)
List of exoplanets discovered in 2013 (151)
List of exoplanets discovered in 2014 (870)
List of exoplanets discovered in 2015 (149)
List of exoplanets discovered in 2016 (1497)
List of exoplanets discovered in 2017 (158)
List of exoplanets discovered in 2018 (303)
List of exoplanets discovered in 2019 (172)
List of exoplanets discovered in 2020 (249)
List of exoplanets discovered in 2021 (257)
List of exoplanets discovered in 2022 (313)
List of exoplanets discovered in 2023 (307)
List of exoplanets discovered in 2024 (281)

References

^ Specht, D.; et al. (2023). "Kepler K2Campaign 9 – II. First space-based discovery of an exoplanet using microlensing". Monthly Notices of the Royal Astronomical Society. 520 (4): 6350–6366. arXiv:2203.16959. doi:10.1093/mnras/stad212.
Starr, Michelle (4 April 2022). "The Most Distant Exoplanet Ever Found by Kepler Is... Surprisingly Familiar". ScienceAlert. Retrieved 4 April 2022.
Currie, Thayne; et al. (2023), "Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star", Science, 380 (6641): 198–203, arXiv:2212.00034, Bibcode:2023Sci...380..198C, doi:10.1126/science.abo6192, PMID 37053312, S2CID 258108042
^ Sebastian, D.; Guenther, E. W.; Deleuil, M.; Dorsch, M.; Heber, U.; Heuser, C.; Gandolfi, D.; Grziwa, S.; Deeg, H. J.; Alonso, R.; Bouchy, F.; Csizmadia, Sz; Cusano, F.; Fridlund, M.; Geier, S.; Irrgang, A.; Korth, J.; Nespral, D.; Rauer, H.; Tal-Or, L. (2022), "Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT–34b, CoRoT–35b, and CoRoT–36b", Monthly Notices of the Royal Astronomical Society, 516: 636–655, arXiv:2207.08742, doi:10.1093/mnras/stac2131
^ 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, arXiv:2203.02087, Bibcode:2022AJ....163..244C, doi:10.3847/1538-3881/ac5c4c, S2CID 247244871
^ 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
^ 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. arXiv:2205.10197. Bibcode:2022A&A...663A.101P. doi:10.1051/0004-6361/202243497. S2CID 248965147.
Damasso, M.; et al. (2022), "A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514", Astronomy & Astrophysics, 666: A187, arXiv:2204.06376, doi:10.1051/0004-6361/202243522, S2CID 248157318
^ Suárez Mascareño, A.; et al. (2022), "Two temperate Earth-mass planets orbiting the nearby star GJ 1002", Astronomy & Astrophysics, 670: A5, arXiv:2212.07332, doi:10.1051/0004-6361/202244991, S2CID 254353639
Kemmer, J.; et al. (2022), "Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 B", Astronomy & Astrophysics, 659: A17, arXiv:2202.00970, Bibcode:2022A&A...659A..17K, doi:10.1051/0004-6361/202142653, S2CID 246473345
^ Beard, Corey; et al. (2022), "GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion", The Astrophysical Journal, 936 (1): 55, arXiv:2207.10672, Bibcode:2022ApJ...936...55B, doi:10.3847/1538-4357/ac8480, S2CID 251018402
A Jupiter Analog Orbiting The Nearby M Dwarf GJ 463
Sozzetti, A. (2023), "A dynamical mass for GJ 463 b: A massive super-Jupiter companion beyond the snow line of a nearby M dwarf", Astronomy & Astrophysics, 670: L17, arXiv:2302.00413, Bibcode:2023A&A...670L..17S, doi:10.1051/0004-6361/202245454, S2CID 256253670
^ Almenara, J. M.; et al. (2022), "GJ 3090 b: One of the most favourable mini-Neptune for atmospheric characterisation", Astronomy & Astrophysics, 665: A91, arXiv:2207.14121, Bibcode:2022A&A...665A..91A, doi:10.1051/0004-6361/202243975, S2CID 252367299
Bourrier, V.; et al. (2022), "A CHEOPS-enhanced view of the HD 3167 system", Astronomy & Astrophysics, 668: A31, arXiv:2209.06937, Bibcode:2022A&A...668A..31B, doi:10.1051/0004-6361/202243778, S2CID 251861892
Desidera, S.; et al. (2023), "TOI-179: A young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit", Astronomy & Astrophysics, 675: A158, arXiv:2210.07933, Bibcode:2023A&A...675A.158D, doi:10.1051/0004-6361/202244611, S2CID 252907692
de Leon, Jerome P.; et al. (2023), "A sub-Neptune transiting the young field star HD 18599 at 40 pc", Monthly Notices of the Royal Astronomical Society, 522: 750–766, arXiv:2210.08179, doi:10.1093/mnras/stad894
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
Murgas, F.; et al. (2022), "HD 20329b: An ultra-short-period planet around a solar-type star found by TESS", Astronomy & Astrophysics, 668: A158, arXiv:2211.02547, Bibcode:2022A&A...668A.158M, doi:10.1051/0004-6361/202244459, S2CID 253370507
^ Ottoni, G.; Udry, S.; Ségransan, D.; et al. (2022). "CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars". Astronomy & Astrophysics. 657: A87. arXiv:2201.01528. Bibcode:2022A&A...657A..87O. doi:10.1051/0004-6361/202040078. ISSN 0004-6361. S2CID 245440163.
^ 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, arXiv:2209.09597, Bibcode:2022A&A...668A..85C, doi:10.1051/0004-6361/202243565, S2CID 252383725
^ 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, arXiv:2209.13345, Bibcode:2022A&A...665A.154B, doi:10.1051/0004-6361/202244293, S2CID 251463803
^ 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
Pezzotti, C.; Ottoni, G.; Buldgen, G.; et al. (22 April 2021). "Coralie radial-velocity search for companions around evolved stars (CASCADES). III. A new Jupiter host-star: in-depth analysis of HD29399 using TESS data". Astronomy & Astrophysics. 657. EDP Sciences: A89. arXiv:2201.01553. doi:10.1051/0004-6361/202040080. ISSN 0004-6361. S2CID 242974999.
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, arXiv:2206.03899, Bibcode:2022AJ....164..156T, doi:10.3847/1538-3881/ac7ce0, S2CID 249461702
Giacalone, Steven; Dressing, Courtney D.; Muñoz, A. García; Hooton, Matthew J.; Stassun, Keivan G.; Quinn, Samuel N.; Zhou, George; Ziegler, Carl; Vanderspek, Roland; Latham, David W.; Seager, S.; Winn, Joshua N.; Jenkins, Jon M.; Briceño, César; Huang, Chelsea X.; Rodriguez, David R.; Shporer, Avi; Mann, Andrew W.; Watanabe, David; Wohler, Bill (2022), "HD 56414 b: A Warm Neptune Transiting an A-type Star", The Astrophysical Journal Letters, 935 (1): L10, arXiv:2208.06396, Bibcode:2022ApJ...935L..10G, doi:10.3847/2041-8213/ac80f4, S2CID 251538927
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, arXiv:2204.05711, Bibcode:2022AJ....163..273E, doi:10.3847/1538-3881/ac6589, S2CID 248118529
^ Serrano, L. M.; et al. (2022), "The HD 93963 a transiting system: A 1.04 d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS", Astronomy & Astrophysics, 667: A1, arXiv:2207.13920, Bibcode:2022A&A...667A...1S, doi:10.1051/0004-6361/202243093, S2CID 250709574
^ Choi, Gong jun; Yanagida, Tsutomu T.; Yokozaki, Norimi (2022), "The upper bound of the second Higgs boson mass in minimal gauge mediation with the gravitino warm dark matter", Journal of High Energy Physics, 2021 (4), arXiv:2012.03266, doi:10.1007/JHEP04(2021)024, S2CID 227340010
Zakhozhay, O.; Launhardt, R.; Trifonov, T.; Kürster, M.; Reffert, S.; Henning, Th.; Brahm, R.; Vinés, J.; Marleau, G. -D.; Patel, J. (2022), "Radial velocity survey for planets around young stars (RVSPY)", Astronomy & Astrophysics, 667: L14, arXiv:2211.08294, doi:10.1051/0004-6361/202244747, S2CID 235028524
Engler, N.; et al. (2023), "The high-albedo, low polarization disk around HD 114082 that harbors a Jupiter-sized transiting planet", Astronomy & Astrophysics, 672: A1, arXiv:2211.11767, doi:10.1051/0004-6361/202244380, S2CID 256215468
Teng, Huan-Yu; Sato, Bun'ei; Kunitomo, Masanobu; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Xiao, Guang-Yao; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Shigeru, Ida (2022), "A close-in planet orbiting giant star HD 167768", Publications of the Astronomical Society of Japan, 75: 169–176, arXiv:2211.06576, doi:10.1093/pasj/psac097
^ Orell-Miquel, J.; Nowak, G.; Murgas, F.; Palle, E.; Morello, G.; Luque, R.; Badenas-Agusti, M.; Ribas, I.; Lafarga, M.; Espinoza, N.; Morales, J. C.; Zechmeister, M.; Alqasim, A.; Cochran, W. D.; Gandolfi, D.; Goffo, E.; Kabáth, P.; Korth, J.; Livingston, J.; Lam, K. W. F.; Muresan, A.; Persson, C. M.; Van Eylen, V. (2023). "HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone". Astronomy & Astrophysics. 669: A40. arXiv:2211.00667. Bibcode:2023A&A...669A..40O. doi:10.1051/0004-6361/202244120. S2CID 253197272.
^ Feng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A.; Bailey, J.; Burt, Jennifer; Carter, B. D.; Crane, Jeffrey D.; Dotti, Francesco Flammini; Holden, Bradford; Ma, Bo; Ogihara, Masahiro; Oppenheimer, Rebecca; o'Toole, S. J.; Shectman, Stephen A.; Wittenmyer, Robert A.; Wang, Sharon X.; Wright, D. J.; Xuan, Yifan (2022), "3D Selection of 167 Substellar Companions to Nearby Stars", The Astrophysical Journal Supplement Series, 262 (1): 21, arXiv:2208.12720, Bibcode:2022ApJS..262...21F, doi:10.3847/1538-4365/ac7e57, S2CID 251864022
Hinkley, S.; et al. (2023), "Direct discovery of the inner exoplanet in the HD 206893 system", Astronomy & Astrophysics, 671: L5, arXiv:2208.04867, Bibcode:2023A&A...671L...5H, doi:10.1051/0004-6361/202244727, S2CID 251442869
^ Luque, R.; et al. (2022), "The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc", Astronomy & Astrophysics, 664: A199, arXiv:2204.10261, Bibcode:2022A&A...664A.199L, doi:10.1051/0004-6361/202243834, S2CID 248300168
^ Serrano, Luisa Maria; et al. (2022), "A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system", Nature Astronomy, 6 (6): 736–750, arXiv:2204.13573, Bibcode:2022NatAs...6..736S, doi:10.1038/s41550-022-01641-y, S2CID 248426734
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, arXiv:2204.11975, Bibcode:2022AJ....163..289Z, doi:10.3847/1538-3881/ac69e3, S2CID 248392044
^ Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Nagasawa, Makiko; Hasegawa, Ryo; Izumiura, Hideyuki; Kambe, Eiji; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru (2022), "A trio of giant planets orbiting evolved star HD 184010", Publications of the Astronomical Society of Japan, 74 (6): 1309–1328, arXiv:2209.09426, doi:10.1093/pasj/psac070
^ 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, Bibcode:2022MNRAS.511.5207E, doi:10.1093/mnras/stac357
Angelo, Isabel; Naoz, Smadar; Petigura, Erik; MacDougall, Mason; Stephan, Alexander P.; Isaacson, Howard; Howard, Andrew W. (2022), "Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant", The Astronomical Journal, 163 (5): 227, arXiv:2204.00019, Bibcode:2022AJ....163..227A, doi:10.3847/1538-3881/ac6094, S2CID 247922620
Kipping, David; Bryson, Steve; et al. (13 January 2022). "An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i". Nature. 6 (3): 367–380. arXiv:2201.04643. Bibcode:2022NatAs...6..367K. doi:10.1038/s41550-021-01539-1. PMC 8938273. PMID 35399159.
"Kepler-1708". NASA Exoplanet Archive. Retrieved 13 January 2022.
^ 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, S2CID 246294682
^ 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): 103, arXiv:2210.12344, Bibcode:2023AJ....165..103Z, doi:10.3847/1538-3881/acb34b, S2CID 253098604
^ Han, Cheongho; Lee, Chung-Uk; Gould, Andrew; Youn Kil Jung; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Kim, Doeon; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; 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-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey", Astronomy & Astrophysics, 666: A132, arXiv:2209.00112, Bibcode:2022A&A...666A.132H, doi:10.1051/0004-6361/202244438, S2CID 251979813
^ Youn Kil Jung; et al. (2022), "Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets", The Astronomical Journal, 164 (6): 262, arXiv:2206.11409, Bibcode:2022AJ....164..262J, doi:10.3847/1538-3881/ac9c5c, S2CID 249953591
^ Gould, Andrew; et al. (2022), "Systematic KMTNet planetary anomaly search", Astronomy & Astrophysics, 664: A13, arXiv:2204.04354, doi:10.1051/0004-6361/202243744, S2CID 248085003
^ 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
^ 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
^ 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, arXiv:2204.11383, Bibcode:2022A&A...664A.114H, doi:10.1051/0004-6361/202243161, S2CID 248377479
^ Han, Cheongho; et al. (2022), "Four sub-Jovian-mass planets detected by high-cadence microlensing surveys", Astronomy & Astrophysics, 664: A33, arXiv:2205.10510, Bibcode:2022A&A...664A..33H, doi:10.1051/0004-6361/202243484, S2CID 248986310
^ Ryu, Yoon-Hyun; Youn Kil Jung; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, %Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard (2022), "Mass Production of 2021 KMTNet Microlensing Planets I", The Astronomical Journal, 164 (5): 180, arXiv:2202.03022, Bibcode:2022AJ....164..180R, doi:10.3847/1538-3881/ac8d6c, S2CID 246634000
^ 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, arXiv:2209.03886, Bibcode:2023AJ....165....8S, doi:10.3847/1538-3881/ac9d93, S2CID 254407196
^ Ryu, Yoon-Hyun; Shin, In-Gu; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Youn Kil Jung; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, %Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W. (2023), "Mass Production of 2021 KMTNet Microlensing Planets II", The Astronomical Journal, 165 (3): 83, arXiv:2207.07295, Bibcode:2023AJ....165...83R, doi:10.3847/1538-3881/acab6b, S2CID 256544515
^ Han, Cheongho; et al. (2022), "KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing", Astronomy & Astrophysics, 662: A70, arXiv:2203.16734, Bibcode:2022A&A...662A..70H, doi:10.1051/0004-6361/202243550, S2CID 247839227
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, arXiv:2204.11378, Bibcode:2022A&A...663A.145H, doi:10.1051/0004-6361/202243102, S2CID 248377122
Sartori, Lia F.; Lovis, Christophe; Delisle, Jean-Baptiste; Lendl, Monika; Cugno, Gabriele; Boehle, Anna; Dannert, Felix; Krenn, Andrea; Gubler, Jonas L.; Quanz, Sascha P. (2023), "L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star", Astronomy & Astrophysics, 670: A42, arXiv:2210.12710, Bibcode:2023A&A...670A..42S, doi:10.1051/0004-6361/202244347, S2CID 253098575
Bachelet, E.; et al. (2022), "MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary", The Astronomical Journal, 164 (3): 75, arXiv:2205.07522, Bibcode:2022AJ....164...75B, doi:10.3847/1538-3881/ac78ed, S2CID 248810881
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, arXiv:2204.03672, Bibcode:2022AJ....164..118I, doi:10.3847/1538-3881/ac82b8, S2CID 248069150
Olmschenk, Greg; et al. (2023), "MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert", The Astronomical Journal, 165 (4): 175, arXiv:2210.02436, Bibcode:2023AJ....165..175O, doi:10.3847/1538-3881/acbcc8, S2CID 252715812
^ 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", Astronomy & Astrophysics, 664: A9, arXiv:2205.02279, Bibcode:2022A&A...664A...9S, doi:10.1051/0004-6361/202243675, S2CID 248524983
^ Ulmer-Moll, S.; et al. (2022), "Two long-period transiting exoplanets on eccentric orbits: NGTS-20 b (TOI-5152 b) and TOI-5153 B", Astronomy & Astrophysics, 666: A46, arXiv:2207.03911, Bibcode:2022A&A...666A..46U, doi:10.1051/0004-6361/202243583, S2CID 250408027
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
^ Jackson, David G.; et al. (2022), "The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey", Monthly Notices of the Royal Astronomical Society, 518 (4): 4845–4860, arXiv:2211.01044, doi:10.1093/mnras/stac3192
Shin, In-Gu; et al. (2022), "OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge", The Astronomical Journal, 163 (6): 254, arXiv:2201.04312, Bibcode:2022AJ....163..254S, doi:10.3847/1538-3881/ac6513, S2CID 245877628
Chung, Sun-Ju; et al. (2022), "OGLE-2019-BLG-0362Lb: A SUPER-JOVIAN-MASS PLANET AROUND a LOW-MASS STAR", Journal of the Korean Astronomical Society, 55 (4): 123, arXiv:2208.04230, Bibcode:2022JKAS...55..123C, doi:10.5303/JKAS.2022.55.4.123, S2CID 251402706
Kuang, Renkun; et al. (2022), "OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system?", Monthly Notices of the Royal Astronomical Society, 516 (2): 1704–1720, arXiv:2204.05606, doi:10.1093/mnras/stac2315
Hatzes, Artie P.; et al. (2022), "A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit", The Astronomical Journal, 163 (5): 223, arXiv:2203.01018, Bibcode:2022AJ....163..223H, doi:10.3847/1538-3881/ac5dcb, S2CID 247218413
Faria, J. P.; et al. (2022), "A candidate short-period sub-Earth orbiting Proxima Centauri", Astronomy & Astrophysics, 658: A115, arXiv:2202.05188, Bibcode:2022A&A...658A.115F, doi:10.1051/0004-6361/202142337, S2CID 246706321
Niţu, Iuliana C.; Keith, Michael J.; Stappers, Ben W.; Lyne, Andrew G.; Mickaliger, Mitchell B. (2022), "A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme", Monthly Notices of the Royal Astronomical Society, 512 (2): 2446–2459, arXiv:2203.01136, doi:10.1093/mnras/stac593
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
Mistry, Priyashkumar; Pathak, Kamlesh; Lekkas, Georgios; Prasad, Aniket; Bhattarai, Surendra; Maity, Mousam; Beichman, Charles A.; Ciardi, David R.; Evans, Phil; Lucero, Jennifer P. (2023), "VaTEST I: Validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star", Monthly Notices of the Royal Astronomical Society, 521: 1066–1078, arXiv:2211.07957, doi:10.1093/mnras/stad543
^ Giacalone, Steven; et al. (2022), "Validation of 13 Hot and Potentially Terrestrial TESS Planets", The Astronomical Journal, 163 (2): 99, arXiv:2201.12661, Bibcode:2022AJ....163...99G, doi:10.3847/1538-3881/ac4334, S2CID 246386453
^ Magliano, Christian; Covone, Giovanni; Dobal, Richa; Cacciapuoti, Luca; Tonietti, Luca; Giacalone, Steven; Vines, Jose I.; Inno, Laura; Jenkins, James S.; Lissauer, Jack J.; Bieryla, Allyson; Oliva, Fabrizio; Pagano, Isabella; Kostov, Veselin; Ziegler, Carl; Ciardi, David R.; Gonzales, Erica J.; Dressing, Courtney D.; Buchhave, Lars A.; Howell, Steve B.; Matson, Rachel A.; Matthews, Elisabeth; Rotundi, Alessandra; Alves, Douglas; Fiscale, Stefano; Ienco, Riccardo M.; Pena, Pablo; Gallo, Francesco; Muscari Tomajoli, Maria T. (2022), "A systematic validation of hot Neptunes in TESS data", Monthly Notices of the Royal Astronomical Society, 519: 1562–1577, arXiv:2211.08490, doi:10.1093/mnras/stac3404
Reefe, Michael A.; et al. (2022), "A Close-in Puffy Neptune with Hidden Friends: The Enigma of TOI 620", The Astronomical Journal, 163 (6): 269, arXiv:2204.03108, Bibcode:2022AJ....163..269R, doi:10.3847/1538-3881/ac658b, S2CID 248006000
Clark, Jake; et al. (2023), "Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778", The Astronomical Journal, 165 (5): 207, arXiv:2212.08242, Bibcode:2023AJ....165..207C, doi:10.3847/1538-3881/acc3a0, S2CID 254823145
^ 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: A109, arXiv:2210.08996, Bibcode:2023A&A...669A.109L, doi:10.1051/0004-6361/202243879, S2CID 252917906
^ Wilson, Thomas G.; et al. (2022), "A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS", Monthly Notices of the Royal Astronomical Society, 511: 1043–1071, arXiv:2201.03570, doi:10.1093/mnras/stab3799
Essack, Zahra; et al. (2023), "TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap", The Astronomical Journal, 165 (2): 47, arXiv:2210.14901, Bibcode:2023AJ....165...47E, doi:10.3847/1538-3881/ac9c5b, S2CID 253117166
Psaridi, A.; et al. (2022), "Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars", Astronomy & Astrophysics, 664: A94, arXiv:2205.10854, Bibcode:2022A&A...664A..94P, doi:10.1051/0004-6361/202243454, S2CID 248872705
^ 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, arXiv:2210.09283, Bibcode:2023AJ....165...33D, doi:10.3847/1538-3881/aca327, S2CID 252918416
^ Kabáth, Petr; et al. (2022), "TOI-2046b, TOI-1181b and TOI-1516b, three new hot Jupiters from TESS: Planets orbiting a young star, a subgiant and a normal star", Monthly Notices of the Royal Astronomical Society, 513 (4): 5955–5972, arXiv:2205.01860, doi:10.1093/mnras/stac1254
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): 217, arXiv:2209.13651, Bibcode:2023AJ....165..217M, doi:10.3847/1538-3881/acc8d4, S2CID 252568279
^ 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, arXiv:2204.11895, Bibcode:2022AJ....163..293T, doi:10.3847/1538-3881/ac69e5, S2CID 248392257
Lam, Kristine W F.; et al. (2022), "Discovery of TOI-1260d and the characterisation of the multi-planet system", Monthly Notices of the Royal Astronomical Society, 519: 1437–1451, arXiv:2212.04307, doi:10.1093/mnras/stac3639
Šubjak, J.; et al. (2022), "TOI-1268b: The youngest hot Saturn-mass transiting exoplanet", Astronomy & Astrophysics, 662: A107, arXiv:2201.13341, Bibcode:2022A&A...662A.107S, doi:10.1051/0004-6361/202142883, S2CID 246430777
^ MacDougall, Mason G.; et al. (2022), "The TESS–Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-mass Outer Companion around TOI-1272", The Astronomical Journal, 164 (3): 97, arXiv:2206.14327, Bibcode:2022AJ....164...97M, doi:10.3847/1538-3881/ac7ce1, S2CID 250113765
Knudstrup, E.; et al. (2022), "Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion", Monthly Notices of the Royal Astronomical Society, 519 (4): 5637–5655, arXiv:2211.17035, doi:10.1093/mnras/stac3684
Naponiello, L.; et al. (2022), "The GAPS programme at TNG. XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422", Astronomy & Astrophysics, A8: 667, arXiv:2207.03293, Bibcode:2022A&A...667A...8N, doi:10.1051/0004-6361/202244079, S2CID 250334523
Cadieux, Charles; Doyon, René; et al. (27 June 2022). "TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf". The Astronomical Journal. 164:96 (3) (published 12 August 2022): 28pp. arXiv:2208.06333. Bibcode:2022AJ....164...96C. doi:10.3847/1538-3881/ac7cea.
^ Chaturvedi, P.; et al. (2022), "TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley", Astronomy & Astrophysics, 666: A155, arXiv:2208.10351, Bibcode:2022A&A...666A.155C, doi:10.1051/0004-6361/202244056, S2CID 251718760
^ Van Zandt, Judah E.; et al. (2023), "TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey", The Astronomical Journal, 165 (2): 60, arXiv:2209.06958, Bibcode:2023AJ....165...60V, doi:10.3847/1538-3881/aca6ef, S2CID 252280288
^ 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, S2CID 227141512
^ 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, arXiv:2203.04334, Bibcode:2022AJ....163..225T, doi:10.3847/1538-3881/ac5c4f, S2CID 247318919
Kiefer, F.; et al. (2023), "A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS", Astronomy & Astrophysics, 670: A136, arXiv:2211.06205, Bibcode:2023A&A...670A.136K, doi:10.1051/0004-6361/202245129, S2CID 253498974
Cherubim, Collin; et al. (2023), "TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley", The Astronomical Journal, 165 (4): 167, arXiv:2211.06445, Bibcode:2023AJ....165..167C, doi:10.3847/1538-3881/acbdfd, S2CID 256627151
Mori, Mayuko; et al. (2022), "TOI-1696: A Nearby M4 Dwarf with a 3 R ⊕ Planet in the Neptunian Desert", The Astronomical Journal, 163 (6): 298, arXiv:2203.02694, Bibcode:2022AJ....163..298M, doi:10.3847/1538-3881/ac6bf8, S2CID 247291913
Beard, Corey; et al. (2022), "TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with the Habitable-Zone Planet Finder", The Astronomical Journal, 163 (6): 286, arXiv:2204.09063, Bibcode:2022AJ....163..286B, doi:10.3847/1538-3881/ac69ec, S2CID 248266475
König, P. -C.; et al. (2022), "A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N", Astronomy & Astrophysics, 666: A183, arXiv:2204.08984, Bibcode:2022A&A...666A.183K, doi:10.1051/0004-6361/202143002, S2CID 248239823
Espinoza, Néstor; et al. (2022), "A Transiting, Temperate Mini-Neptune Orbiting the M Dwarf TOI-1759 Unveiled by TESS", The Astronomical Journal, 163 (3): 133, arXiv:2202.01240, Bibcode:2022AJ....163..133E, doi:10.3847/1538-3881/ac4af0, S2CID 246485680
Martioli, E.; et al. (2022), "TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS", Astronomy & Astrophysics, 660: A86, arXiv:2202.01259, Bibcode:2022A&A...660A..86M, doi:10.1051/0004-6361/202142540, S2CID 246485686
^ Rodriguez, Joseph E.; et al. (2023), "Another shipment of six short-period giant planets from TESS", Monthly Notices of the Royal Astronomical Society, 521 (2): 2765–2785, arXiv:2205.05709, doi:10.1093/mnras/stad595
^ Knudstrup, E.; et al. (2022), "Confirmation and characterisation of three giant planets detected by TESS from the FIES/NOT and Tull/Mc Donald spectrographs", Astronomy & Astrophysics, 667: A22, arXiv:2204.13956, Bibcode:2022A&A...667A..22K, doi:10.1051/0004-6361/202243656, S2CID 251083570
^ 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): 1, arXiv:2210.15473, Bibcode:2023ApJS..265....1Y, doi:10.3847/1538-4365/aca286, S2CID 253157404
^ 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, 524: 1113–1138, arXiv:2209.14396, doi:10.1093/mnras/stad1666
Newton, Elisabeth R.; et al. (2022), "TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet", The Astronomical Journal, 164 (3): 115, arXiv:2206.06254, Bibcode:2022AJ....164..115N, doi:10.3847/1538-3881/ac8154, S2CID 249626353
^ Esparza-Borges, E.; et al. (2022), "A hot sub-Neptune in the desert and a temperate super-Earth around faint M dwarfs", Astronomy & Astrophysics, 666: A10, arXiv:2206.10643, doi:10.1051/0004-6361/202243731, S2CID 249926978
Gan, Tianjun; et al. (2022), "TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136", Monthly Notices of the Royal Astronomical Society, 514 (3): 4120–4139, arXiv:2202.10024, doi:10.1093/mnras/stac1448
Kawauchi, K.; et al. (2022), "Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf", Astronomy & Astrophysics, 666: A4, arXiv:2202.10182, Bibcode:2022A&A...666A...4K, doi:10.1051/0004-6361/202243381, S2CID 247011479
Dalba, Paul A.; et al. (2022), "The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope", The Astronomical Journal, 163 (2): 61, arXiv:2201.04146, Bibcode:2022AJ....163...61D, doi:10.3847/1538-3881/ac415b, S2CID 245877799
^ Yee, Samuel W.; et al. (2022), "The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets", The Astronomical Journal, 164 (2): 70, arXiv:2205.09728, Bibcode:2022AJ....164...70Y, doi:10.3847/1538-3881/ac73ff, S2CID 248887656
Persson, Carina M.; et al. (2022), "TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star", Astronomy & Astrophysics, 666: A184, arXiv:2208.05797, Bibcode:2022A&A...666A.184P, doi:10.1051/0004-6361/202244118, S2CID 251478602
^ Grunblatt, Samuel K.; et al. (2022), "TESS Giants Transiting Giants. II. The Hottest Jupiters Orbiting Evolved Stars", The Astronomical Journal, 163 (3): 120, arXiv:2201.04140, Bibcode:2022AJ....163..120G, doi:10.3847/1538-3881/ac4972, S2CID 245877793
^ Cañas, Caleb I.; et al. (2022), "TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID", The Astronomical Journal, 164 (2): 50, arXiv:2201.09963, Bibcode:2022AJ....164...50C, doi:10.3847/1538-3881/ac7804, S2CID 246275821
Kanodia, Shubham; et al. (2022), "TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf", The Astronomical Journal, 164 (3): 81, arXiv:2203.07178, Bibcode:2022AJ....164...81K, doi:10.3847/1538-3881/ac7c20, S2CID 247446993
Almenara, J. M.; Bonfils, X.; Forveille, T.; Astudillo-Defru, N.; Ciardi, D. R.; Schwarz, R. P.; Collins, K. A.; Cointepas, M.; Lund, M. B.; Bouchy, F.; Charbonneau, D.; Díaz, R. F.; Delfosse, X.; Kidwell, R. C.; Kunimoto, M.; Latham, D. W.; Lissauer, J. J.; Murgas, F.; Ricker, G.; Seager, S.; Vezie, M.; Watanabe, D. (2022), "TOI-3884 b: A rare 6-RE planet that transits a low-mass star with a giant and likely polar spot", Astronomy & Astrophysics, 667: L11, arXiv:2210.10909, Bibcode:2022A&A...667L..11A, doi:10.1051/0004-6361/202244791, S2CID 253018639
Libby-Roberts, Jessica E.; Schutte, Maria; Hebb, Leslie; Kanodia, Shubham; Canas, Caleb; Stefansson, Gudmundur; Lin, Andrea S. J.; Mahadevan, Suvrath; Parts, Winter; Powers, Luke; Wisniewski, John; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Everett, Mark E.; Gupta, Arvind F.; Halverson, Samuel; Kobulnicky, Henry A.; Kowalski, Adam F.; Larsen, Alexander; Monson, Andrew; Ninan, Joe P.; Parker, Brock A.; Ramsey, Lawrence W.; Robertson, Paul; Schwab, Christian; Swaby, Tera N.; Terrien, Ryan C. (2023), An In-Depth Look at TOI-3884b: a Super-Neptune Transiting a M4 Dwarf with Persistent Star Spot Crossings, arXiv:2302.04757
Heitzmann, Alexis; et al. (2023), "TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star", The Astronomical Journal, 165 (3): 121, arXiv:2208.10854, Bibcode:2023AJ....165..121H, doi:10.3847/1538-3881/acb5a2, S2CID 251741424
Grunblatt, Samuel K.; Saunders, Nicholas; Chontos, Ashley; Hattori, Soichiro; Veras, Dimitri; Huber, Daniel; Angus, Ruth; Rice, Malena; Breivik, Katelyn; Blunt, Sarah; Giacalone, Steven; Lubin, Jack; Isaacson, Howard; Howard, Andrew W.; Ciardi, David R.; Safonov, Boris S.; Strakhov, Ivan A.; Latham, David W.; Bieryla, Allyson; Ricker, George R.; Jenkins, Jon M.; Tenenbaum, Peter; Shporer, Avi; Morgan, Edward H.; Kostov, Veselin; Osborn, Hugh P.; Dragomir, Diana; Seager, Sara; Vanderspek, Roland K.; Winn, Joshua N. (2023), "TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars", The Astronomical Journal, 165 (2): 44, arXiv:2210.17062, Bibcode:2023AJ....165...44G, doi:10.3847/1538-3881/aca670, S2CID 253237700
"The Extrasolar Planet Encyclopaedia — TOI-5174 b". Extrasolar Planets Encyclopaedia. 3 December 1995. Retrieved 16 January 2023.
"Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 16 January 2023.
Kanodia, Shubham; Mahadevan, Suvrath; Libby-Roberts, Jessica; Stefansson, Gudmundur; Canas, Caleb I.; Piette, Anjali A. A.; Boss, Alan; Teske, Johanna; Chambers, John; Zeimann, Greg; Monson, Andrew; Robertson, Paul; Ninan, Joe P.; Lin, Andrea S. J.; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Gupta, Arvind F.; Halverson, Samuel; Hawley, Suzanne; Kobulnicky, Henry A.; Metcalf, Andrew J.; Parker, Brock A.; Powers, Luke; Ramsey, Lawrence W.; Roy, Arpita; Schwab, Christian; Swaby, Tera N.; Terrien, Ryan C.; Wisniewski, John (2023), "TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf", The Astronomical Journal, 165 (3): 120, arXiv:2209.11160, Bibcode:2023AJ....165..120K, doi:10.3847/1538-3881/acabce, S2CID 257050897
Grieves, Nolan; et al. (2022), "An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542", Astronomy & Astrophysics, 668: A29, arXiv:2209.14830, Bibcode:2022A&A...668A..29G, doi:10.1051/0004-6361/202244077, S2CID 252595745
^ 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, S2CID 247835988
Hord, Benjamin J.; Colón, Knicole D.; Berger, Travis A.; Kostov, Veselin; Silverstein, Michele L.; Stassun, Keivan G.; Lissauer, Jack J.; Collins, Karen A.; Schwarz, Richard P.; Sefako, Ramotholo; Ziegler, Carl; Briceño, César; Law, Nicholas; Mann, Andrew W.; Ricker, George R.; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Bouma, Luke G.; Falk, Ben; Torres, Guillermo; Twicken, Joseph D.; Vanderburg, Andrew (2022), "The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 B", The Astronomical Journal, 164 (1): 13, arXiv:2205.02501, Bibcode:2022AJ....164...13H, doi:10.3847/1538-3881/ac6f57, S2CID 248524687

Exoplanets

Main topics

Sizes
and
types

Terrestrial	Carbon planet Coreless planet Desert planet Dwarf planet Hycean planet Ice planet Iron planet (Super-Mercury) 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

Catalogues

Exoplanetary systems

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
- 2023
- 2024

Other

2022 in space

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Space probe launches

CAPSTONE (June 2022)
Danuri (August 2022)
Artemis I (November 2022)
- ArgoMoon
- EQUULEUS
- LunaH-Map
- Lunar IceCube
- NEA Scout
- OMOTENASHI
- LunIR
Hakuto-R Mission 1 / Emirates Lunar Mission / Lunar Flashlight (December 2022)

Impact events

Selected NEOs

Discoveries

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

Comets

Space exploration

DART (Dimorphos impact; September 2022)

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