List of exoplanets discovered in 2025

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

Thislist of exoplanets discovered in 2025 is a list of confirmedexoplanets that were first reported in 2025.For exoplanets detected only byradial velocity, the listed value for mass is a lower limit. SeeMinimum mass for more information.

Name	Mass (`M`_J)	Radius (`R`_J)	Period (days)	Semi-major axis (AU)	Temp. (K)	Discovery method	Distance (ly)	Host star mass (`M`_☉)	Host star temp. (K)	Remarks
AB Pictoris c	2.5–9			3–5		astrometry + radial vel.	163	0.90±0.10	5188±50	^[1]
AT2021uey b	1.34^+0.45 _−0.50		4,170^+2,910 _−1,710	4.01^+1.68 _−1.34		microlensing	3,390^+2,410 _−1,440	0.49^+0.16 _−0.18	3,680⁺³⁰⁷ ₋₂₀₄	^[2]
Barnard's Star c	0.00105		4.12	0.0274±0.0004		radial vel.	5.96	0.162	3,195	^[3]
Barnard's Star d	0.00083		2.34	0.0188±0.0003		radial vel.
Barnard's Star e	0.00061		6.74	0.0381±0.0005		radial vel.
BEBOP-3b	0.558^+0.051 _−0.048		547.0^+6.2 _−7.6	1.444±0.017		radial vel.	385.13±0.58^[4]	1.3445^[a]	6,033^[b]	Acircumbinary planet.^[5]
BD+05 4868 Ab	0.000063	0.028	1.27187	0.0208±0.0003	1,820±45	transit	142.4±0.1	0.70±0.02	4,596⁺⁶⁵ ₋₆₄	A disintegrating planet with a comet-like tail.^[6]
Cha 1107-7626	8.0±2.0	2.8			1800	imaging	636			Free-floating object of planetary mass. Could also be a sub-brown dwarf.^[7]
G 192-15 b	0.00324±0.00057		2.27476^+0.00026 _−0.00028	0.01723^+0.00038 _−0.00039	453.6^+8.8 _−8.5	radial vel.	31.09±0.022	0.132±0.009		Also known as GJ 3380 b.^[8]
G 192-15 c	0.0450^+0.0050 _−0.0047		1,219⁺¹³ ₋₁₁	1.137^+0.026 _−0.027	55.9±1.1	radial vel.	31.09±0.022	0.132±0.009		Also known as GJ 3380 c.^[8]
G 261-6 b	0.00431^+0.00072 _−0.00069		5.4536^+0.0031 _−0.0032	0.02971^+0.00087 _−0.00093	322.3^+9.9 _−9.7	radial vel.	34.66±0.021	0.118±0.011		^[8]
G 268-110 b	0.00478±0.00079		1.432630^+0.000072 _−0.000076	0.01283^+0.00028 _−0.00029	534⁺¹² ₋₁₁	radial vel.	31.86	0.137±0.009		^[8]
Gliese 251 c	0.01207		53.647±0.044	0.196±0.014		radial vel.	18.21	0.360±0.015	3342±24	Potentially habitable.^[9]
Gliese 410 b	0.0249±0.0038		6.02	0.0531±0.0007		radial vel.	38.9	0.55±0.02	3,842±31	Two additional planets in the same system are suspected.^[10]
Gliese 536 c	0.01853±0.0022		32.76	0.1617±0.003	290	radial vel.	32.71	0.52±0.05	3685±68	^[11]
GJ 2126 b	1.3^+0.2 _−0.1		272.7	0.71±0.03		radial vel.	124.3±0.4	0.65^+0.09 _−0.07	4,159±130	^[12]
GJ 3998 d	0.0191^+0.00315 _−0.00302		41.78±0.05	0.189±0.006		radial vel.	58.056±2.283	0.52±0.05	3726±68	^[13]
HD 87816 b	6.74		484	1.618±0.0003		radial vel.	434.4	2.41±0.1	4,989±46	Host star also known as R Velorum.^[14]
HD 87816 c	12.2		7,596⁺¹¹⁴⁰ ₋₅₃₅	10.14^+1.0 _−0.5		radial vel.	434.4	2.41±0.1	4,989±46	Host star also known as R Velorum.^[14]
HD 94890 b	2.13		824	2.07±0.001		radial vel.	201.2	1.74±0.20	4,867±38	Host star also known as iota Antliae.^[14]
HD 94890 c	8.9		2492	4.33±0.02		radial vel.	201.2	1.74±0.20	4,867±38	Host star also known as iota Antliae.^[14]
HD 102888 b	5.69		252	1.05±0.001		radial vel.	412.6	2.42±0.06	4,990±39	^[14]
HD 135344 Ab	10.0^+1.4 _−1.9	1.45^+0.06 _−0.03		16.5^+2.8 _−2.0	1,585⁺⁸² ₋₇₃	imaging	440	1.5	9,540±100	^[15]
HD 143811 (AB)b	5.6±1.1			63.88	1042	imaging	446.4	2.5	6,575±325	Acircumbinary planet.^[16]
HD 224018 b	0.0129±0.0025	0.0812^+0.0036 _−0.033	10.64	0.0952±0.002	968	transit	346.0±0.7	1.013^+0.069 _−0.061	5,784±60	^[17]
HD 224018 c	0.0327^+0.0041 _−0.0035	0.2159^+0.0062 _−0.0071	36.58	0.217±0.005	641	transit
HD 224018 d	0.0132^+0.0057 _−0.0050	0.214±0.009	138.1	0.53^+0.06 _−0.02	411	transit
HD 224018 e	0.475^+0.041 _−0.044		9129±2499	8.6^+1.5 _−1.6	102	radial vel.
J042705.86+261520.3	4.5					imaging	522			Part of aJuMBO along with J042705.86+261520.3 b .^[18]
J042705.86+261520.3 b	3.9					imaging	522			Part of aJuMBO along with J042705.86+261520.3.^[18]
J041546.22+280811.4	6.0					imaging	–			Free-floating object of planetary mass. Could also be a sub-brown dwarf.^[18]
K2-157c	0.0969		25.9	0.165±0.0018	587	radial vel.	946.5	0.89 ± 0.029	5,334 ± 64	^[19]
K2-157d	0.0733		66.5	0.309±0.0038	429	radial vel.	946.5	0.89 ± 0.029	5,334 ± 64	^[19]
Kepler-139 f	0.113±0.0315		355±2			radial vel. + timing	1,289.78±13.89	1.08	5,594±100	^[20]
Kepler-279 e	0.176^+0.0189 _−0.0154	0.310±0.0482	~98.35			transit	3,487.26±74.07	1.10^+0.16 _−0.13	6,363±259	^[21]
Kepler-289 e	0.0547^+0.00409 _−0.00377	0.286^+0.00437 _−0.00259	~330			transit	2,283.09±45.66	1.08±0.02	5,990±38	^[21]
Kepler-725 c	0.031		207.5	0.674±0.002		timing	2474±45	0.91	5,293±122	Partially in habitable zone.^[22]
KMT-2017-BLG-2197Lb	8.84^+8.3 _−4.9			15.9^+2.1 _−2.7		microlensing	25,400^+3,300 _−4,300	0.36^+0.34 _−0.2		^[23]
KMT-2019-BLG-0578Lb	1.2^+1.2 _−0.6			1.2±0.2 or 2.0±0.3		microlensing	23,810^+2,280 _−2,610	0.28^+0.28 _−0.14		^[24]
KMT-2021-BLG-0736Lb	0.0661^+0.0409 _−0.0315			4.0^+0.9 _−0.8		microlensing	22,830^+2,610 _−4,890	0.60^+0.37 _−0.29		^[24]
KMT-2022-BLG-1790Lb	1.73^+0.95 _−0.9			5.25^+0.75 _−1.0		microlensing	21,100^+3,000 _−4,200	0.58^+0.32 _−0.3		^[23]
KMT-2022-BLG-1818Lb	1.5+0.6 −0.3			1.5+0.3 −0.2		microlensing	9460+2280 −1300	0.3+0.12 −0.06		^[25]
KMT-2022-BLG-1818Lc	0.35+0.24 −0.17			0.4±0.1		microlensing	9460+2280 −1300	0.3+0.12 −0.06		^[25]
KMT-2022-BLG-2076Lb	0.88±0.46			5.67±1.58		microlensing	18,200^+4,100 _−5,000	0.67±0.35		^[23]
KMT-2023-BLG-0119Lb	0.2634^+0.16822 _−0.14396			3.14^+1.32 _−1.33 or 4.01^+1.69 _−1.70		microlensing	10,240^+5,510 _−5,540	0.71^+0.45 _−0.39		^[26]
KMT-2023-BLG-1896Lb	0.0515^+0.03087 _−0.02656			2.86^+1.12 _−1.02 or 4.62^+1.81 _−1.94		microlensing	17,900^+7,000 _−7,500	0.72^+0.43 _−0.37		^[26]
KMT-2023-BLG-2209Lb	0.80±0.38			5.31^+0.95 _−1.1		microlensing	18,200^+5,000 _−5,700	0.73±0.35		^[23]
KMT-2024-BLG-0404L b	0.0544^+0.0802 _−0.0277			0.34±0.05		microlensing	23,510^+3,030 _−3,160	0.09^+0.133 _−0.046		Also a brown dwarf exists in the system^[27]
KMT-2024-BLG-1209Lb	2.64^+1.57 _−1.16			2.51^+1.50 _−1.10		microlensing	12,800^+6,600 _−4,600	0.77^+0.46 _−0.34		^[28]
KOBE-1 b	0.0277±0.0024		8.54	0.07±0.0004	594	radial vel.	77.89±0.04	0.629±0.017	4,135±36	^[29]
KOBE-1 c	0.039±0.0035		29.67	0.161±0.001	392	radial vel.	77.89±0.04	0.629±0.017	4,135±36	^[29]
KOI-134 b		1.08±0.2	67.59	0.358	588	transit	3780	1.17	6154±26	^[30]
KOI-134 c	0.22 ± 0.01		33.5			timing	3780	1.17	6154±26	^[30]
L 98-59 f	0.00934		23.07	0.1053±0.0024		radial vel.	34.6	0.32±0.03	3,415±135	Potentially habitable^[31]
MOA-2022-BLG-033Lb	0.0382^+0.0296 _−0.0197			2.15^+1.17 _−0.75 or 2.31^+1.27 _−0.81		microlensing	6,000^+3,260 _−2,640	0.51^+0.39 _−0.26		^[26]
MOA-2022-BLG-091Lb	3.59^+2.00 _−1.67			2.67^+1.45 _−1.24 to 3.63^+1.30 _−1.31		microlensing	13,900^+4,960 _−4,990	0.75^+0.42 _−0.35		^[28]
MP Muscae b	5.0			1 – 3		astrometry + disk kinematics	319.3	1.3±0.08	5000	^[32]
OGLE-2016-BLG-0007 b	0.00415^+0.0028 _−0.0022			10.1^+3.8 _−3.4		microlensing	14,020⁺³⁵⁹⁰ ₋₄₅₇₀	0.6^+0.4 _−0.3		^[33]
OGLE-2023-BLG-0524	0.0293 or 0.182^[c]					microlensing	–			Free-floating object of planetary mass.^[34]
o005 s41280	8.4	2.3			2,162	imaging	17,300			Free-floating object of planetary mass. Could also be a sub-brown dwarf.^[35]
o006 s00089	11.5	1.2			955	imaging	6,520			Free-floating object of planetary mass. Could also be a sub-brown dwarf.^[35]
Ross 176 b	0.01438±0.0028	0.1642±0.0071	5.00663±0.00008	0.0464±0.001	682	transit	151.7	0.58±0.02	4,061±70	^[36]
TIC 88785435 b		0.449±0.019	10.508843	0.08432±0.00068	635±16	transit	398.2±0.8	0.724±0.017	3,998±95	^[37]
TOI-201 c	14.2±2.0	0.99±0.017	2,800⁺³⁶⁰ ₋₂₁₀	4.28^+0.36 _−0.2		timing + transit	372.5	1.316±0.027	6,394±75	^[38]
TOI-333 b	0.0632±0.0076	0.3801±0.0098	3.785250±0.000006	0.049±0.001	1445	transit	1132	1.2±0.1	6,241±73	^[39]
TOI-512 b	0.01123^+0.00167 _−0.00173	0.1374±0.0089	7.18886^+0.000069 _−0.000077		1,009±29	transit	219.16±0.14	0.74±0.03	5,277±67	^[40]
TOI-771 c	0.00903		7.61	0.046±0.002	365	radial vel.	82.45	0.22±0.024	3,201±100	^[41]
TOI-1117 b	0.028±0.003	0.219^+0.012 _−0.011	2.22816±0.00001	0.0330±0.0002	1,538±21	transit	546.64±2.94	0.97±0.02	5,635±62	^[42]
TOI-1117 c	0.0276^+0.0037 _−0.0038		4.579±0.004	0.0534±0.0003	1,210±16	radial vel.
TOI-1117 d	0.0337±0.0050		8.665±0.011	0.0817±0.0006	978±13	radial vel.
TOI-1453 Ab	0.00390^+0.00208 _−0.00204	0.105^+0.00526 _−0.00500	4.3135225^+0.0000118 _−0.0000092			transit	257.288±0.209	0.715±0.035	4,975±68	^[43]
TOI-1453 Ac	0.00928^+0.00261 _−0.00264	0.198±0.00848	6.5886982			transit	257.288±0.209	0.715±0.035	4,975±68	^[43]
TOI-1846 b	0.01385^+0.00503 _−0.00315	0.15987^+0.00580 _−0.00607	3.931	0.03646^+0.00072 _−0.00074	568.1^+6.1 _−5.9	transit	154.09±0.11	0.40±0.02	3,568±44	^[44]
TOI-2005 b	<6.4	1.07^+0.06 _−0.11	17.305904^+0.000023 _−0.000020	0.16±0.02		transit	1,072.08^+15.00 _−13.70	1.59^+0.016 _−0.017	7,130±150	^[45]
TOI-2015 c	0.02803^+0.001196 _−0.001259		5.582796^+0.000042 _−0.000041	0.041232±0.000004	448±3	timing	154.34±0.16	0.3041^+0.0353 _−0.0312	3,297⁺¹⁴ ₋₂₈	^[46] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection.^[47]
TOI-2076 e		0.12089^+0.00901 _−0.00874	3.0223445±0.0000033	0.0385^+0.0021 _−0.0049	1138	transit	136.7	0.849^+0.027 _−0.026	5,200±100	^[48]
TOI-2407 b		0.380±0.023	2.703	0.033±0.001	705±12	transit	300.06	0.548±0.016	3,530±100	^[49]
TOI-2427 c	0.02033		5.15±0.01	0.05±0.01		radial vel.	92.95	0.64±0.02	4,072±121	^[50]
TOI-2431 b	0.020±0.004	0.137±0.003	0.224196	0.0063±0.0001	2,063±30	transit	117	0.661^+0.021 _−0.024	4,109⁺²⁸ ₋₂₇	Has one of the shortest orbital periods of any exoplanet. In just 31 million years the planet will have been destroyed.^[51]
TOI-2449 b	0.7±0.04	1.0±0.01	106.1447	0.45±0.01	400	transit	505.5	1.079^+0.045 _−0.048	6,021±62	Also known as NGTS-36 b.^[52]
TOI-2969 b	1.16±0.04	1.1±0.08	1.8237146±0.0000002	0.0261±0.0002	1186	transit	530.0	0.71±0.02	4738±100	^[53]
TOI-2989 b	3.0±0.2	1.12±0.05	3.122832±0.000001	0.0384±0.0003	1000	transit	635.7	0.77±0.02	4672±170	^[53]
TOI-3493 b	0.0282^+0.00368 _−0.00377	0.287±0.00714	8.1594667^+0.0000016 _−0.0000017		1,102⁺²⁰ ₋₁₄	transit	315.59±0.65	1.023±0.041	5,844±42	^[54]
TOI-3495 b		0.3631	8.413073±0.000055		902	transit	562.2	1.42±0.17	6,400±230	^[55]
TOI-4507 b	<0.094	0.7333±0.0071	104.61595±0.00004	0.449±0.003		transit	580.6	1.15±0.07	6,235±100	^[56]
TOI-5108 b	0.101±0.0157	0.589±0.00892	6.753	0.073±0.004	1,180±40	transit	427.6±2.0	1.10±0.03	5,808±40	^[57]
TOI-5143 c		1.45^+0.18 _−0.12	5.2097118^+0.0000032 _−0.0000039	0.05602^+0.00082 _−0.00079		transit	582.42±1.97	0.864^+0.040 _−0.033	5,183±125	^[58]
TOI-5300 b	0.6±0.1	0.88±0.08	2.262196±0.000003	0.0295±0.0003	1043	transit	530.6	0.67±0.02	4610±207	^[53]
TOI-5573 b	0.35±0.06	0.87±0.04	8.79759±0.00001	0.0712±0.0008	528	transit	606.0	0.619±0.023	3,790±59	^[59]
TOI-5786 b	0.230±0.0283	0.762±0.0116	12.779	0.114±0.007	1,040±40	transit	632.1±1.6	1.23^+0.04 _−0.03	6,235±50	^[57]
TOI-5795 b	0.0744^+0.0129 _−0.0145	0.5014±0.0098	6.140632±0.000005	0.064±0.002	1137	transit	526.7	0.901^+0.055 _−0.037	5,715±55	^[60]
TOI-5800 b	0.030±0.006	0.218±0.026	2.6279	0.0345±0.0014	1,108±20	transit	139.4±0.1	0.778^+0.037 _−0.032	4,850±78	^[61]
TOI-5817 b	0.03241^+0.00441 _−0.00409	0.275±0.012	15.61	0.1223±0.0060	950⁺²¹ ₋₁₈	transit	262.0±0.5	0.970^+0.072 _−0.055	5,770±50	^[61]
TOI-6038 Ab	0.247^+0.030 _−0.031	0.572^+0.018 _−0.014	5.82673	0.0690^+0.0012 _−0.0011	1,439⁺²⁵ ₋₂₄	transit	577.9±2.0	1.291^+0.066 _−0.060	6,110±100	The host star is part of a binary system with a K-type companion.^[62]
TOI-6054 b	0.039±0.0053	0.2364±0.0134	7.501	0.0763±0.0048	1,360⁺³⁵ ₋₃₁	transit	256.7±0.4	1.107±0.040	6,047±50	^[63]
TOI-6054 c	0.0289±0.006	0.250±0.016	12.564	0.1077±0.0067	1,144⁺²⁹ ₋₂₆	transit	256.7±0.4	1.107±0.040	6,047±50	^[63]
TOI-6478 b	0.0311	0.411±0.021	34.005019±0.000025	0.1136±0.0060	204.4±4.9	transit	125.93±0.33	0.230±0.007	3,230±75	^[64]
TOI-6695 b	0.21	0.85±0.02	80.4	0.402±0.002	599	transit	922	1.338	6,400	^[65]
TOI-6695 c	1.45		242	0.838±0.005	415	radial vel.	922	1.338	6,400	^[65]
TOI-6894 b	0.168±0.022	0.855±0.022	3.371	0.02604±0.00045	417.9±8.6	transit	237.96±0.95	0.207±0.011	3007±58	^[66]
TOI-7149 b	0.705±0.075	1.180±0.045	2.652	0.026±0.00076	593±21	transit	415.0±2.4	0.344±0.030	3,363±59	^[67]
TOI-7166 b		0.1793±0.0054	12.920636±0.000001	0.06191±0.00044	249	transit	114.9	0.19±0.004	3,099±51	^[68]
WASP-154 b	0.626±0.129	0.96±0.06	3.811678±0.000001	0.044±0.003	994±63	transit	702.87±6.40	0.80±0.05	4,774±133	^[69]
WASP-188 Ab	1.443^+0.296 _−0.298	1.322±0.051	5.748916±0.000003	0.072±0.003	1,666±70	transit	2,202.47±31.55	1.50±0.09	6,850±125	^[69]
WASP-195 b	0.104^+0.03 _−0.031	0.92±0.05	5.051928±0.000004	0.063±0.003	1,522±71	transit	1,581.38±16.60	1.30±0.08	6,300±125	^[69]
WASP-197 b	1.269±0.254	1.289±0.049	5.167228±0.000003	0.065±0.002	1,665±67	transit	1,577.54±40.08	1.36±0.08	6,050±100	^[69]
WISPIT 2 b	5.3±1.0	1.6±0.2		15.0		imaging	435	1.08^+0.06 _−0.17	4,400±50	^[70]^[71]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]

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

Notes

[edit]

^Sum of masses of the system
^Temperature of component A
^The mass of planet depends on its location, which is either galactic disk or galactic bulge

References

[edit]

^Lagrange, A.-M.; Kiefer, F.; Rubini, P.; Squicciarini, V.; Chomez, A.; Milli, J.; Zurlo, A.; Bouvier, J.; Delorme, P. (17 January 2025). "Searching for substellar companion candidates with Gaia. III. Search for companions to members of young associations".arXiv:2501.10488 [astro-ph.EP].
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^.arXiv:2511.13832.{{cite arXiv}}:Missing or empty|title= (help)CS1 maint: missing class (link) A bot will complete this citation soon.Click here to jump the queue
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Exoplanets

Main topics

Sizes
and
types

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