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List of exoplanets discovered in 2025

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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 2025 is a list of confirmed exoplanets that were first reported in 2025. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name Mass (MJ) Radius (RJ) 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 velocity 5.96 0.162 3,195 [3]
Barnard's Star d 0.00083 2.34 0.0188±0.0003 radial velocity
Barnard's Star e 0.00061 6.74 0.0381±0.0005 radial velocity
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.[4]
GJ 2126 b 1.3+0.2
−0.1 		272.7 0.71±0.03 radial velocity 124.3±0.4 0.65+0.09
−0.07 		4,159±130 [5]
GJ 3998 d 0.0191+0.00315
−0.00302 		41.78±0.05 0.189±0.006 radial velocity 58.056±2.283 0.52±0.05 3726±68 [6]
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 		[7]
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 		[7]
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 		[8]
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 		[8]
KOBE-1 b 0.0277±0.0024 8.54 0.07±0.0004 594 radial velocity 77.89±0.04 0.629±0.017 4,135±36 [9]
KOBE-1 c 0.039±0.0035 29.67 0.161±0.001 392 radial velocity
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 		[8]
o005 s41280 8.4 2.3 2,162 imaging 17,300 Free-floating object of planetary mass. Could also be a brown dwarf.[10]
o006 s00089 11.5 1.2 955 imaging 6,520 Free-floating object of planetary mass. Could also be a brown dwarf.[10]
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 [11]
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 [12]
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 4975±68 [13]
TOI-1453 Ac 0.00928+0.00261
−0.00264 		0.198±0.00848 6.5886982 transit
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 [14]
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 		[15] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection.[16]
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 [17]
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 		5183±125 [18]
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 [17]
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.[19]
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 [20]
TOI-6054 c 0.0289±0.006 0.250±0.016 12.564 0.1077±0.0067 1,144+29
−26 		transit

Specific exoplanet lists

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Lists of exoplanets

Lists of exoplanets by year of discovery

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References

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  1. ^ 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.
  2. ^ Ban, M.; et al. (45) (31 March 2025). "AT2021uey: A planetary microlensing event outside the Galactic bulge". arXiv:2503.22331.
  3. ^ Basant, Ritvik; Luque, Rafael; et al. (March 2025). "Four Sub-Earth Planets Orbiting Barnard's Star from MAROON-X and ESPRESSO". The Astrophysical Journal Letters. 982: L1. arXiv:2503.08095. doi:10.3847/2041-8213/adb8d5.
  4. ^ Hon, Marc; Rappaport, Saul; Shporer, Avi; Vanderburg, Andrew; Collins, Karen A.; Watkins, Cristilyn N.; Schwarz, Richard P.; Barkaoui, Khalid; Yee, Samuel W. (9 January 2025). "A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star". arXiv:2501.05431 [astro-ph.EP].
  5. ^ Schorr, A.; Binnenfeld, A.; Zucker, S. (31 January 2025). "GJ 2126 b: A highly eccentric Jovian exoplanet". Astronomy & Astrophysics. 694: A210. arXiv:2502.11139. Bibcode:2025A&A...694A.210S. doi:10.1051/0004-6361/202452563. ISSN 0004-6361.
  6. ^ Stefanov, A. K.; Suárez Mascareño, A.; González Hernández, J. I.; Nari, N.; Rebolo, R.; Affer, L.; Micela, G.; Ribas, I.; Sozzetti, A.; Perger, M.; Pinamonti, M.; Damasso, M.; Maldonado, J.; González Álvarez, E.; Scandariato, G. (11 March 2025). "HADES RV Programme with HARPS-N at TNG XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system". Astronomy and Astrophysics. 695. doi:10.1051/0004-6361/202452630. Retrieved 13 March 2025.
  7. ^ a b Yang, Hongjing; Yee, Jennifer C.; Zhang, Jiyuan; Lee, Chung-Uk; Kim, Dong-Jin; Bond, Ian A.; Udalski, Andrzej; Hwang, Kyu-Ha; Zang, Weicheng; Qian, Qiyue; Gould, Andrew; Mao, Shude (26 March 2025). "Systematic Reanalysis of KMTNet Microlensing Events, Paper II: Two New Planets in Giant-Source Events". arXiv:2503.19471.
  8. ^ a b c Han, Cheongho; Bond, Ian A.; Jung, Youn Kil; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun (4 January 2025). "MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals". Astronomy and Astrophysics. 694: A90. arXiv:2501.02193. Bibcode:2025A&A...694A..90H. doi:10.1051/0004-6361/202452027.
  9. ^ Balsalobre-Ruza, O.; Lillo-Box, J.; Silva, A. M.; Grouffal, S.; Aceituno, J.; Castro-González, A.; Cifuentes, C.; Standing, M. R.; Faria, J. P. (3 February 2025), "KOBE-1: The first planetary system from the KOBE survey", Astronomy & Astrophysics, 694: A15, arXiv:2502.01249, doi:10.1051/0004-6361/202452631
  10. ^ a b Tu, Zhijun; Wang, Shu; Chen, Xiaodian; Liu, Jifeng (2025). "Three Brown Dwarfs Masquerading as High-Redshift Galaxies in JWST Observations". The Astrophysical Journal. 980 (2): 230. arXiv:2501.16648. Bibcode:2025ApJ...980..230T. doi:10.3847/1538-4357/adaf9f.
  11. ^ Vach, Sydney; et al. (1 February 2025). "A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS". arXiv:2502.00576 [astro-ph.EP].
  12. ^ Rodrigues, J.; et al. (20 February 2025). "TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO". arXiv:2502.14472 [astro-ph.EP].
  13. ^ Stalport, M.; Mortier, A.; Cretignier, M.; Egger, J. A.; Malavolta, L.; Latham, D. W.; Collins, K. A.; Watkins, C. N.; Murgas, F.; Buchhave, L. A.; López-Morales, M.; Udry, S.; Quinn, S. N.; Silva, A. M.; Andreuzzi, G.; Baker, D.; Boschin, W.; Ciardi, D. R.; Damasso, M.; Di Fabrizio, L.; Dumusque, X.; Fukui, A.; Haywood, R.; Howell, S. B.; Jenkins, J. M.; Leleu, A.; Lewin, P.; Lillo-Box, J.; Martínez-Fiorenzano, A. F.; Narita, N.; Pedani, M.; Pinamonti, M.; Poretti, E.; Schwarz, R. P.; Seager, S.; Sozzetti, A.; Ting, E. B.; Vanderburg, A.; Winn, J. N.; Ziegler, C. (10 March 2025). "TESS and HARPS-N unveil two planets transiting TOI-1453". arXiv:2503.07529 [astro-ph.EP].
  14. ^ Bieryla, Allyson; et al. (39) (27 March 2025). "TOI-2005b: An Eccentric Warm Jupiter in Spin-Orbit Alignment". arXiv:2503.20069.
  15. ^ Barkaoui, K.; et al. (10 February 2025). "TOI-2015b: a sub-Neptune in strong gravitational interaction with an outer non-transiting planet". arXiv:2502.07074 [astro-ph.EP].
  16. ^ Jones, Sinclaire E.; et al. (9 May 2024). "TOI-2015b: A Warm Neptune with Transit Timing Variations Orbiting an Active mid M Dwarf". arXiv:2310.11775 [astro-ph.EP].
  17. ^ a b Thomas, Luis; et al. (47) (7 January 2025). "TOI-5108 b and TOI 5786 b: Two transiting sub-Saturns detected and characterized with TESS, MaHPS, and SOPHIE". Astronomy & Astrophysics. 694: A143. arXiv:2501.03803. Bibcode:2025A&A...694A.143T. doi:10.1051/0004-6361/202451676.
  18. ^ Radzom, Brandon T.; Dong, Jiayin; Rice, Malena; Wang, Xian-Yu; Hixenbaugh, Kyle; Zhou, George; Huang, Chelsea X.; Wang, Songhu (3 March 2025). "Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems". The Astronomical Journal. 169 (3): 189. arXiv:2503.03745. Bibcode:2025AJ....169..189R. doi:10.3847/1538-3881/ad9dd5.
  19. ^ Baliwal, Sanjay; Sharma, Rishikesh; Chakraborty, Abhijit; Nikitha, K. J.; Castro-González, A.; Bhaskar, Hareesh G.; Khandelwal, Akanksha; Latham, David W.; Bieryla, Allyson (4 January 2025). "TOI-6038 A b: A dense sub-Saturn in the transition regime between the Neptunian ridge and savanna". The Astronomical Journal. 169 (3): 147. arXiv:2501.02272. Bibcode:2025AJ....169..147B. doi:10.3847/1538-3881/ada959.
  20. ^ Kroft, Maxwell; Beatty, Thomas G.; Crossfield, Ian J. M.; Livesey, Joseph R.; Becker, Juliette; Luhn, Jacob K.; Robertson, Paul; Bieryla, Allyson; Ciardi, David R. (15 January 2025). "A Pair of Dynamically Interacting Sub-Neptunes Around TOI-6054". arXiv:2501.09095 [astro-ph.EP].
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