List of exoplanets discovered in 2026

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by editing the page to add missing items, with references to reliable sources.

This list of exoplanets discovered in 2026 is a list of confirmed exoplanets and exoplanet candidates that were first reported in 2026. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information. For exoplanets detected only by direct imaging or microlensing without a determined orbit, the listed value for semi-major axis is the projected separation.

Name	Mass (MJ)	Radius (RJ)	Period (days)	Semi-major axis (AU)	Temp. (K)	Discovery method	Planet status	Distance (ly)	Host star mass (M☉)	Host star temp. (K)	Remarks
AB Aurigae d	20			65	550	imaging	Candidate	508.6	2.4	25	Candidate into planet. [1]
DMPP-2c	0.1629+0.0171 −0.0173	0.737	3.168+0.355 −0.002	0.04789+0.00327 −0.00049		radial vel.	Confirmed	443	1.41±0.04	6,500±100	[2]
DMPP-2d	0.2888+0.0192 −0.0230	1.03	16.491+0.067 −0.053	0.1432+0.0012 −0.0013		radial vel.	Confirmed				[2]
DMPP-6b	0.0182+0.0030 −0.0025	0.203	7.6027+0.0261 −0.0016	0.00779+0.0016 −0.0012		radial vel.	Confirmed	178	1.079±0.045		[2]
DMPP-6c	0.0424+0.0050 −0.0062	0.334	36.441+0.077 −0.070	0.2206+0.0033 −0.0039		radial vel.	Confirmed				[2]
DMPP-7b	0.1932+0.0136 −0.0128	0.815	4.984+0.069 −0.061	0.05873+0.00086 −0.00089		radial vel.	Confirmed	333	1.09±0.04		[2]
DMPP-8b	0.2551±0.0223	0.96	62.915+0.041 −0.033	0.3098+0.0098 −0.0108		radial vel.	Confirmed	248	0.99±0.04		[2]
DMPP-9b	0.0454+0.0081 −0.0074	0.347	12.733+0.584 −0.524	0.1097+0.0041 −0.0037		radial vel.	Confirmed	359	1.10±0.04		[2]
DO Tauri b	2.8±0.6		21.14±0.2	10.12±0.01		radial vel.	Candidate	1451.8	10.54±0.07	3450±50	Candidate into planet. [3]
GJ 523 b	0.0739±0.0104	0.2275±0.0134	17.745740±0.000045	0.1226±0.0015	538±13	transit	Confirmed	86.8	0.781±0.029		[4]
GJ 887 d	0.0192±0.0044		50.77±0.05	0.212+0.007 −0.008	241+10 −9	radial vel.	Confirmed	10.724	0.495±0.049	3,688±86	A super-Earth located in the habitable zone [5]
GJ 887 e	0.0046±0.0006		4.4249±0.0001	0.0417+0.0014 −0.0015	544+21 −20	radial vel.	Confirmed				[5]
GJ 887 f	~≥0.00157		~2.21661±0.0001	~0.0263	~685	radial.vel	Candidate				Candidate into planet. [5]
GJ 1137 c	0.0161±0.0022		9.6412+0.0012 −0.0011	0.0835±0.0008		radial vel.	Confirmed	92.83	0.836+0.023 −0.025	5,033.8+85.7 −77.2	[6]
GJ 3090 c	0.031±0.004	0.28	15.9407±0.0058	0.0997±0.0008	407.2±7.4	radial vel.	Confirmed	73.24	0.519±0.013	3,707±32	[7]
GJ 3410	~6.8			~11.8	~261±9	imaging	Candidate	159	10.95	16943±68	Candidate into planet.Orbits a white dwarf. [8]
GJ 4274 b	0.0093+0.0017 −0.0016	0.1394	1.6339±0.0001	0.0153±0.0008		radial vel.	Confirmed	23.595	0.18±0.03	3,228±19	[9]
GJ 4274 c	0.0264+0.0053 −0.0049	0.252	69.57+0.32 −1.14	0.186±0.010		radial vel.	Confirmed
HD 2134 b			32.3			radial vel.	Candidate	233	1.01±0.128	5672±129	Candidate into planet. [10]
HD 48265 c	4.45+0.75 −0.37	1.15	10418+2451 −1412	10.4+1.6 −1.0		astrometry + radial vel.	Confirmed	296.2	1.38±0.06	5,805±34	[11]
HD 50554 c	0.01148±0.00425	0.117±0.005	5.969362	0.066+0.009 −0.018		transit	Confirmed	101.34	1.04±0.05	5,968±96	[12]
HD 50554 d	0.0211±0.0116	0.126+0.013 −0.008	28.06940	0.168+0.028 −0.065		transit	Confirmed
HD 68475 b	5.16+0.53 −0.47	1.15	7832+463 −323	7.27+0.39 −0.36		astrometry + radial vel.	Confirmed	108.7	0.83±0.10	5,022±113	[11]
HD 100508 b	1.20+0.30 −0.18	1.22	5681±42	6.11+0.25 −0.28		astrometry + radial vel.	Confirmed	106.9	0.94±0.12	5,419±112	[11]
HD 114386 c	0.37±0.03	1.2	444.00+0.93 −0.88	1.05±0.04		radial vel.	Confirmed	91.26	0.80±0.03	4,895±62	[11]
HD 137010 b		0.0946±0.0054	355.0+200.0 −59.0	0.88+0.3 −0.1	205.0±25.0	transit	Candidate	146.3	0.726±0.017	4,770±90	сandidate Earth-sized planet at the edge of the habitable zone [13]
HD 164604 c	9.5±1.2 or [a] 7.6±1.0	1.12	5387+120 −127	5.556+0.093 −0.100		astrometry + radial vel.	Confirmed	128.5	0.77±0.02	4,663±31	[14]
HD 176986 d	0.0213±0.0029	0.222	61.376+0.051 −0.049	0.28149±0.0024	363±10	radial vel.	Confirmed	90.93	0.789±0.019	4,931±77	[15]
KMT-2016-BLG-1337Lb	0.54±0.30	1.01	3945	3.97+0.60 −0.92		microlensing	Confirmed	22570+3392 −5251	0.54±0.30 0.40±0.22		A circumbinary planet. [16]
KMT-2020-BLG-0202Lb	12.28+7.37 −5.43	1.1	3470	4.17+1.29 −1.28		microlensing	Confirmed	12518+3879 −3847	0.81+0.49 −0.36		[17]
KMT-2021-BLG-0852Lb	0.49+0.17 −0.17			7.78+0.89 −1.11		microlensing	Confirmed	23581+2707 −3359	0.75+0.26 −0.27		[18]
KMT-2022-BLG-1551Lb	2.96+1.71 −1.53	1.17	1717	2.29+0.30 −0.44		microlensing	Confirmed	22494+2999 −4336	0.54+0.31 −0.28		[17]
KMT-2023-BLG-0164Lb	0.047+0.026 −0.019			1.33+0.39 −0.25		microlensing	Confirmed	3390+1663 −880	0.32+0.21 −0.13		[19]
KMT-2023-BLG-0466Lb	3.25+2.59 −2.03	1.17	2411	2.68+0.45 −0.63		microlensing	Confirmed	22168+3716 −5216	0.44+0.36 −0.27		[17]
KMT-2023-BLG-1286Lb	0.062+0.058 −0.035			2.02±0.60		microlensing	Confirmed	20049+3227 −4401	0.31+0.29 −0.18		[19]
KMT-2023-BLG-1746Lb	0.0070+0.0048 −0.0021			1.06+0.55 −0.17		microlensing	Confirmed	25363±3064	0.11+0.08 −0.03		[19]
KMT-2024-BLG-0792L	0.219+0.075 −0.046					microlensing	Candidate	9948+1892 −1402			candidate rogue planet [20]
KMT-2024-BLG-2005Lb	0.16+0.24 −0.09			1.12+0.15 −0.15		microlensing	Confirmed	25179+3262 −3457	0.12+0.17 −0.06		[18]
KMT-2024-BLG-3237L	0.212+0.325 −0.134					microlensing	Candidate	23940+3131 −6882			candidate rogue planet [21]
KMT-2025-BLG-0121Lb	7.77+4.08 −4.04	1.13	2484	3.05+0.46 −0.66		microlensing	Confirmed	20212+3032 −4400	0.61±0.32		[17]
KMT-2025-BLG-0481Lb	0.59+0.85 −0.34			2.18+0.31 −0.39		microlensing	Confirmed	26027+3686 −4697	0.22+0.31 −0.13		[18]
KMT-2025-BLG-0811Lb	0.02199±0.01466			2.47±0.57		microlensing	Confirmed	22799+2772 −3457	0.49+0.32 −0.23		[22]
KMT-2025-BLG-1616Lb	0.1332+0.1278 −0.0694			1.6+0.2 −0.3		microlensing	Confirmed	24462+2283 −3262	0.26+0.25 −0.14		[23]
KOINTREAU-3b	3.4±0.7	1.17	3609839	342±4		imaging	Confirmed	450		3,920±70	[24]
KOINTREAU-4b	11.5+1.2 −1.6 or [b] 14.8+1.2 −0.9	1.09		182±2		imaging	Confirmed	463			[24]
LHS 1903 b	0.01032±0.0013	0.1233±0.0041	2.1555098	0.02656+0.00055 −0.00058	796±20	transit	Confirmed	116.3	0.538+0.039 −0.030	3,664±70	[25]
LHS 1903 c	0.01432+0.0023 −0.0022	0.1825+0.0070 −0.0066	6.226185	0.05387+0.00112 −0.00117	559±14	transit	Confirmed
LHS 1903 d	0.01875±0.0036	0.2230+0.0070 −0.0069	12.566287	0.08604+0.00178 −0.00186	442±11	transit	Confirmed
LHS 1903 e	0.01822+0.0050 −0.0051	0.1545+0.0053 −0.0052	29.31773	0.15135+0.00314 −0.00338	333+9 −8	transit	Confirmed
MP mus g	~0.003+0.028 −0.0028			~60		imaging	Candidate	319.3	1.3±0.08	5000	Candidate into planet. [26]
TIC 259230140 b		~0.5692±0.0348	~14.31708±0.00016			transit	Candidate	904.8		7500-10000	Candidate into planet.Also known as HD 130599. [27]
TIC 65910228 b	4.78+0.40 −0.37	1.081±0.047	180.52791	0.695±0.036	458±11	transit	Confirmed	864	1.46±0.09	6,310±129	Planet also known as NGTS-38 b. [28] [29]
TIC 87422071 b	1.29+0.10 −0.11	0.969+0.087 −0.084	11.364929	0.106±0.005	1,110±33	transit	Confirmed	1302	1.239+0.070 −0.080	6,150±178	Star also known as TOI-6752. [30]
TIC 147027702 b	1.09+0.07 −0.13	0.975+0.065 −0.064	44.40523	0.274+0.014 −0.013	863+26 −27	transit	Confirmed	1490	1.406+0.074 −0.086	6,410±183	[30]
TIC 245076932 b	0.51+0.04 −0.05	0.970±0.048	21.613890	0.157±0.007	845±25	transit	Confirmed	1026	1.117±0.063	6,130±178	[30]
TOI-237 c		0.1076±0.0031	1.74486147	0.0160+0.0005 −0.0006	515+11 −8	transit	Confirmed	124.86	0.1698+0.0385 −0.0350	3,226+47 −48	[31]
TOI-883 b	0.123±0.012	0.604±0.028	10.057716	0.0898±0.0023	1,086±19	transit	Confirmed	336	0.956+0.054 −0.051	5,697±80	[32]
TOI-899 b	0.213±0.024	0.991±0.044	12.846185	0.1063±0.0026	1,040±19	transit	Confirmed	1004	0.972+0.054 −0.053	5,696±80	[32]
TOI-1080 b	0.0055+0.0039 −0.0018 [c]	0.1071±0.0052	3.9652482	0.0272+0.0015 −0.0016	368+12 −10	transit	Confirmed	83.36	0.1667±0.0041	3,065±50	[33]
TOI-1232 b	0.964±0.06	0.975±0.05	14.256±0.001	0.117±0.001		transit	Confirmed	1068	1.05±0.133	5818±134.1	[34]
TOI-1232 c	0.18±0.02		30.356±0.01	0.194±0.002		radial vel.	Confirmed
TOI-1243 b	0.0242±0.0047	0.2079±0.0107	4.65948	0.0437±0.0001	450	transit	Confirmed	140.6	0.515±0.027	3,515±79	[35]
TOI-2133 b	0.026+0.010 −0.008 [c]	0.211±0.008	3.8266472	0.0410±0.0015	798±12	transit	Confirmed	245.3	0.644±0.019	4,250±45	[36]
TOI-3862 b	0.1688+0.0087 −0.0090	0.493±0.016	1.55745774	0.02539+0.00064 −0.00068	1,539	transit	Confirmed	801.2	0.90±0.07	5,300±50	[37]
TOI-4336 A c	0.114	0.1039+0.0054 −0.0052	7.587270	0.0481±0.0027	378±12	transit	Confirmed	73.23	0.2853+0.0438 −0.0356	3,369+51 −57	[31]
TOI-4495 b	0.024+0.004 −0.05	0.221+0.012 −0.008	2.56699	0.03957±0.00047	1735	transit	Confirmed	801.2	1.247±0.045	6,210±70	[38]
TOI-4529 b	0.0154	0.1579±0.008	5.87958	0.04997±0.0008	511	transit	Confirmed	92.6	0.482±0.023	3,697±71	[35]
TOI-4552 b	0.00576±0.0016	0.099±0.0036	0.30110032±0.00000014	0.0056255±0.0000003	1122	transit	Confirmed	89.3	0.2619±0.0063	3,258±115	[39]
TOI-4616 b	0.00708±0.00236	0.1088	1.55382±0.00001	0.0150±0.00001 [d]	525	transit	Confirmed	91.9	0.1881±0.0094	3,150±75	[40]
TOI-5734 b	0.0286±0.0082	0.187±0.011	6.1841876	0.05921±0.00024	688±23	transit	Confirmed	100.1	0.724±0.009	4,750±100	[36] [41]
TOI-5788 b	0.0117±0.0030	0.1365±0.0067	6.340758	0.0640±0.0011		transit	Confirmed	318.2	0.87±0.04	5,615±25	[42]
TOI-5788 c	0.0201±0.0038	0.2025±0.0036	16.213358	0.1197±0.0020		transit	Confirmed
TOI-6692 b	0.620+0.080 −0.065	1.042+0.050 −0.049	131.125±0.012	0.512+0.014 −0.012	467.0+9.3 −9.5	transit	Confirmed	1013	1.047+0.089 −0.071	5,890+170 −180	[43]
TOI-5938 b	0.049+0.025 −0.022 [c]	0.341±0.010	2.2604240	0.0308±0.0010	1077+16 −15	transit	Confirmed	371.9	0.744±0.016	4,650±50	[36]
TOI-6716 b	0.00287	0.0874±0.0062	4.71859	0.032±0.003	369	transit	Confirmed	61.6	0.223±0.011	3,110±80	[44]
TOI-7009 b	0.047+0.023 −0.021 [c]	0.331±0.013	2.3206612	0.0287±0.0010	872+11 −10	transit	Confirmed	600.5	0.583±0.014	4,080±25	[36]
TOI-7169 b	0.41±0.014v	1.475±0.029	3.4373125			transit	Confirmed		0.885 ±0.01	1,477	Orbits a metal-poor star. [45] [46]
TOI-7384 b	0.039	0.3176±0.0187	6.23403	0.0439±0.004	378	transit	Confirmed	218	0.318±0.016	3,185±75	[44]

Specific exoplanet lists

Lists of exoplanets

• List of directly imaged exoplanets
• List of exoplanet extremes
• List of exoplanet firsts
• List of exoplanets discovered by the Kepler space telescope
• List of exoplanets observed during Kepler's K2 mission
• List of exoplanets discovered by the TESS mission
• List of extrasolar candidates for liquid water
• List of terrestrial exoplanet candidates for atmosphere detection
• List of hottest exoplanets
• List of coldest exoplanets
• List of multiplanetary systems
• List of circumbinary planets
• List of nearest exoplanets
• List of nearest terrestrial exoplanet candidates
• List of potentially habitable exoplanets
• List of proper names of exoplanets
• List of largest exoplanets
• List of smallest exoplanets
• List of transiting exoplanets
• List of exoplanets and planetary debris around giant stars
• List of exoplanets and planetary debris around white dwarfs
• List of extrasolar planetary collisions

Lists of exoplanets by year of discovery

• 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 (169)
• List of exoplanets discovered in 2020 (256)
• List of exoplanets discovered in 2021 (254)
• List of exoplanets discovered in 2022 (313)
• List of exoplanets discovered in 2023 (304)
• List of exoplanets discovered in 2024 (284)
• List of exoplanets discovered in 2025 (138)
• List of exoplanets discovered in 2026 (79)

Notes

1. Mass determination depends on whether the orbit is prograde or retrograde.
2. Mass determination depends on whether the star is an Ophiuchus or Upper Scorpius association member.
3. Estimated using theoretical mass–radius relations.
4. Converted from orbital period.

References

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2. Standing, Matthew R.; Barnes, John R.; et al. (2026). "The Dispersed Matter Planet Project Sample - Detection limits, Occurrence Rates and New Planets". Monthly Notices of the Royal Astronomical Society. stag370 (3) stag370. arXiv: 2602.18207 . Bibcode:2026MNRAS.tmp..387S. doi: 10.1093/mnras/stag370 .
3. Donati, J.-F.; Cristofari, P.I.; et al. (27 February 2026). "Monitoring the magnetospherie accretion of the classical T Tauri star DO Tau with SPIRou". arXiv: 2602.24078 [astro-ph.EP].
4. Kroft, Maxwell A.; Beatty, Thomas G.; Salzer, Joseph M.; Zwicker, Claire; Becker, Juliette; Dou, Jingyao; et al. (25 March 2026). "GJ 523b is a Massive, 170 Myr-old Mega-Earth, Likely on a Polar Orbit". Astronomical Journal. forthcoming. arXiv: 2603.24682 .
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6. Stoeva, Denitza; Stefanov, Atanas K.; et al. (March 2026). "Long-period magnetic activity in the K dwarf GJ 1137 and a new super-Earth on a 9-day orbit". Astronomy & Astrophysics . arXiv: 2603.04919 . doi:10.1051/0004-6361/202557806.
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8. Poulsen, Sabrina; Debes, John; et al. (26 January 2026). "The MIRI Excess around Degenerates (MEAD) Survey II: A Probable Planet detected via IR Excess around WD 0644+025". The Astronomical Journal. 171 (3): 183. arXiv: 2601.18965 . Bibcode:2026AJ....171..183P. doi: 10.3847/1538-3881/ae3c0e .
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11. Wu, Yiyun; Xiao, Guang-Yao; Butler, R. Paul; Feng, Fabo; Shectman, Stephen A.; Crane, Jeffrey D.; Teske, Johanna K.; Wang, Sharon X.; Beletsky, Yuri; Burt, Jennifer A.; Daylan, Tansu; Diaz, Matias; Dragomir, Diana; Flowers, Erin; Jenkins, Sydney; Kanodia, Shubham; Nandakumar, Sangeetha; Rice, Malena; Shporer, Avi; Yee, Sam; Zhou, George; Lin, Zitao (2026). "Detection of four cold Jupiters through combined analyses of radial velocity and astrometry data". The Astronomical Journal. 171 (3): 189. arXiv: 2601.11280 . Bibcode:2026AJ....171..189W. doi: 10.3847/1538-3881/ae40f5 .
12. Liu, Quanyi (刘权毅); Zhu, Wei (祝伟); Gan, Tianjun (干天君); Dai, Fei (戴飞) (11 February 2026). "TESS planets in known radial velocity cold Jupiter systems: Hot super Earth occurrence is enhanced by cold Jupiters". arXiv: 2602.11017 [astro-ph.EP].
13. Venner, Alexander; Vanderburg, Andrew; Huang, Chelsea X.; Dholakia, Shishir; Schwengeler, Hans Martin; Howell, Steve B.; Wittenmyer, Robert A.; Kristiansen, Martti H.; Omohundro, Mark; Terentev, Ivan A. (1 February 2026). "A Cool Earth-sized Planet Candidate Transiting a Tenth Magnitude K-dwarf From K2". The Astrophysical Journal Letters. 997 (2): L38. arXiv: 2601.19870 . Bibcode:2026ApJ...997L..38V. doi: 10.3847/2041-8213/adf06f . ISSN   2041-8205.
14. Xiao, Guang-Yao (肖光耀); Feng, Fabo (冯发波); Butler, R. Paul; Teske, Johanna K.; Shectman, Stephen A.; Crane, Jeffrey D.; Wang, Sharon X. (王雪凇) (11 February 2026). "HD 164604 c: a second giant planet on a 15-yr orbit and the constraint of the planet-planet mutual inclination". arXiv: 2602.10919 [astro-ph.EP].
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