Jump to content

List of exoplanets discovered in 2025: Difference between revisions

Edit links
From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
Citation bot (talk | contribs)
Bots
5,735,754 edits
Altered template type. Add: pages, issue, volume, bibcode, class, date, display-authors, authors 1-30. | Use this bot. Report bugs. | Suggested by Headbomb | Category:Articles with missing Cite arXiv inputs | #UCB_Category 9/12
correct spelling
Tags: Reverted Mobile edit Mobile web edit
Line 44: Line 44:
|<ref name=Lagrange-2025-01-17>{{Cite arXiv |last1=Lagrange |first1=A.-M. |last2=Kiefer |first2=F. |last3=Rubini |first3=P. |last4=Squicciarini |first4=V. |last5=Chomez |first5=A. |last6=Milli |first6=J. |last7=Zurlo |first7=A. |last8=Bouvier|first8=J. |last9=Delorme |first9=P. |title=Searching for substellar companion candidates with Gaia. III. Search for companions to members of young associations |date=2025-01-17 |class=astro-ph.EP |eprint=2501.10488 }}</ref>
|<ref name=Lagrange-2025-01-17>{{Cite arXiv |last1=Lagrange |first1=A.-M. |last2=Kiefer |first2=F. |last3=Rubini |first3=P. |last4=Squicciarini |first4=V. |last5=Chomez |first5=A. |last6=Milli |first6=J. |last7=Zurlo |first7=A. |last8=Bouvier|first8=J. |last9=Delorme |first9=P. |title=Searching for substellar companion candidates with Gaia. III. Search for companions to members of young associations |date=2025-01-17 |class=astro-ph.EP |eprint=2501.10488 }}</ref>
|-
|-
|AT2021uey b
|AT2021ueyl b
|1.34{{±|0.45|0.50}}
|1.34{{±|0.45|0.50}}
|
|

Revision as of 01:08, 11 July 2025

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]
AT2021ueyl 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
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] A circumbinary 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]
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 velocity 31.09±0.022 0.132±0.009 Also known as GJ 3380 b.[7]
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 velocity Also known as GJ 3380 c.[7]
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 velocity 34.66±0.021 0.118±0.011 [7]
G 268-110 b 0.00478±0.00079 1.432630+0.000072
−0.000076 		0.01283+0.00028
−0.00029 		534+12
−11 		radial velocity 31.86 0.137±0.009 [7]
Gliese 410 b 0.0249±0.0038 6.02 0.0531±0.0007 radial velocity 38.9 0.55±0.02 3,842±31 Two additional planets in the same system are suspected.[8]
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 [9]
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 [10]
HD 87816 b 6.74 484 1.618±0.0003 radial velocity 434.4 2.41±0.1 4,989±46 Host star also known as R Velorum.[11]
HD 87816 c 12.2 7,596+1140
−535 		10.14+1.0
−0.5 		radial velocity
HD 94890 b 2.13 824 2.07±0.001 radial velocity 201.2 1.74±0.20 4,867±38 Host star also known as iota Antliae.[11]
HD 94890 c 8.9 2492 4.33±0.02 radial velocity
HD 102888 b 5.69 252 1.05±0.001 radial velocity 412.6 2.42±0.06 4,990±39 [11]
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 [12]
K2-157c 0.0969 25.9 0.165±0.0018 587 radial velocity 946.5 0.89 ± 0.029 5,334 ± 64 [13]
K2-157d 0.0733 66.5 0.309±0.0038 429 radial velocity
Kepler-139 f 0.113±0.0315 355±2 radial velocity 1,289.78±13.89 1.08 5,594±100 [14]
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 [15]
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 [15]
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 		[16]
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 		[16]
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 		[17]
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 		[17]
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 		[18]
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 [19]
KOBE-1 c 0.039±0.0035 29.67 0.161±0.001 392 radial velocity
KOI-134 b 1.08±0.2 67.59 0.358 588 transit 3780 1.17 6154±26 [20]
KOI-134 c 0.22 ± 0.01 33.5 timing
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 		[17]
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 		[18]
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 		[21]
o005 s41280 8.4 2.3 2,162 imaging 17,300 Free-floating object of planetary mass. Could also be a brown dwarf.[22]
o006 s00089 11.5 1.2 955 imaging 6,520 Free-floating object of planetary mass. Could also be a brown dwarf.[22]
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 [23]
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 [24]
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 [25]
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 [26]
TOI-1453 Ac 0.00928+0.00261
−0.00264 		0.198±0.00848 6.5886982 transit
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 [27]
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 [28]
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 		[29] Already suspected on discovery of TOI-2015 b in 2023 based on observed TTVs but without clear detection.[30]
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 [31]
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 [32]
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 [33]
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 [34]
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 [33]
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 [35]
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 [35]
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.[36]
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 [37]
TOI-6054 c 0.0289±0.006 0.250±0.016 12.564 0.1077±0.0067 1,144+29
−26 		transit
TOI-6478 b 0.0311 0.411±0.021 34.005019±0.000025 0.1136±0.0060 204.4±4.9 radial velocity 125.93±0.33 0.230±0.007 3,230±75 [38]
TOI-6695 b 0.21 0.85±0.02 80.4 0.402±0.002 599 transit 922 1.338 6,400 [39]
TOI-6695 c 1.45 242 0.838±0.005 415 radial velocity
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 [40]
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 [41]
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 [42]
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 [41]
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 [41]
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 [41]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery


Notes

  1. ^ Sum of masses of the system
  2. ^ Temperature of component A

References

  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 [astro-ph.EP].
  2. ^ Ban, M.; et al. (45) (31 March 2025). "AT2021uey: A planetary microlensing event outside the Galactic bulge". Astronomy & Astrophysics. 697: A57. arXiv:2503.22331. Bibcode:2025A&A...697A..57B. doi:10.1051/0004-6361/202554236.
  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 (1): L1. arXiv:2503.08095. Bibcode:2025ApJ...982L...1B. doi:10.3847/2041-8213/adb8d5.
  4. ^ "PPM 6653". SIMBAD. Centre de données astronomiques de Strasbourg.
  5. ^ Baycroft, Thomas A. last2=Santerne; Triaud, Amaury H. M. J.; Heidari, Neda; Sebastian, Daniel; Davis, Yasmin T.; Correia, Alexandre C. M.; Sairam, Lalitha; Freckelton, Alix V. (17 June 2025). "BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit". arXiv:2506.14615 [astro-ph.EP]. {{cite arXiv}}: |first2= missing |last2= (help); Missing pipe in: |first1= (help)CS1 maint: numeric names: authors list (link)
  6. ^ 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". The Astrophysical Journal. 984 (1): L3. arXiv:2501.05431. Bibcode:2025ApJ...984L...3H. doi:10.3847/2041-8213/adbf21.
  7. ^ a b c d Kaminski, A.; Sabotta, S.; Kemmer, J.; Chaturvedi, P.; Burn, R.; Morales, J. C.; Caballero, J. A.; Ribas, I.; Reiners, A.; Quirrenbach, A.; Amado, P. J.; Béjar, V. J. S.; Dreizler, S.; Guenther, E. W.; Hatzes, A. P.; Henning, Th.; Kürster, M.; Montes, D.; Nagel, E.; Pallé, E.; Pinter, V.; Reffert, S.; Schlecker, M.; Shan, Y.; Trifonov, T.; Zapatero Osorio, M. R.; Zechmeister, M. (8 April 2025). "The CARMENES search for exoplanets around M dwarfs". Astronomy & Astrophysics. 696: A101. arXiv:2504.03364. doi:10.1051/0004-6361/202453381.
  8. ^ Carmona, A.; Delfosse, X.; et al. (4 April 2025). "Characterizing planetary systems with SPIRou: Detection of a sub-Neptune in a 6 day period orbit around the M dwarf Gl 410". arXiv:2504.03572 [astro-ph.EP].
  9. ^ 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.
  10. ^ 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. arXiv:2503.08405. Bibcode:2025A&A...695A..62S. doi:10.1051/0004-6361/202452630. Retrieved 13 March 2025.
  11. ^ a b c Fontanet, E.; Udry, S. (May 2025). "CORALIE radial-velocity search for companions around evolved stars (CASCADES) IV: New planetary systems around HD 87816, HD 94890, and HD 102888 and an update on HD 121056". arXiv:2505.14317 [astro-ph.EP].
  12. ^ Stolker, T.; et al. (2025). "Direct imaging discovery of a young giant planet orbiting on Solar System scales". arXiv:2507.06206 [astro-ph.EP].
  13. ^ Castro-González, A.; et al. (2025). "Two neighbours to the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna". arXiv:2504.20999 [astro-ph.EP].
  14. ^ Lammers, Caleb; Winn, Joshua N. (17 April 2025). "Discovery and Dynamics of the Nontransiting Planet Kepler-139f". The Astrophysical Journal. 984 (2): L39. arXiv:2504.13160. Bibcode:2025ApJ...984L..39L. doi:10.3847/2041-8213/adce01.
  15. ^ a b Ofir, Aviv; Yoffe, Gideon; Aharonson, Oded (21 January 2025). "Planetary Mass Determinations from a Simplified Photodynamical Model—Application to the Complete Kepler Dataset". The Astronomical Journal. 169 (2): 90. arXiv:2410.11401. Bibcode:2025AJ....169...90O. doi:10.3847/1538-3881/ad91a7.
  16. ^ 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. II. Two New Planets in Giant-source Events". The Astronomical Journal. 169 (6): 295. arXiv:2503.19471. Bibcode:2025AJ....169..295Y. doi:10.3847/1538-3881/adc73e.
  17. ^ 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.
  18. ^ a b Han, Cheongho; Lee, Chung-Uk; Udalski, Andrzej; Bond, Ian A.; Yang, Hongjing; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Jung, Youn Kil (29 May 2025), MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals, arXiv:2505.22951
  19. ^ 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
  20. ^ Nabbie, Emma; Huang, Chelsea X.; Korth, Judith; Parviainen, Hannu; Wang, Su; Venner, Alexander; Wittenmyer, Robert; Bieryla, Allyson; Latham, David W.; Li, Gongjie; Lin, Douglas N. C.; Zhou, George (27 June 2025). "A high mutual inclination system around KOI-134 revealed by transit timing variations". Nature Astronomy: 1–9. arXiv:2507.02238. Bibcode:2025NatAs.tmp..136N. doi:10.1038/s41550-025-02594-8. ISSN 2397-3366.{{cite journal}}: CS1 maint: bibcode (link)
  21. ^ Weicheng, Zang; Youn Kil, Jung (2025). "Microlensing events indicate that super-Earth exoplanets are common in Jupiter-like orbits". Science. 388 (6745): 400–404. arXiv:2504.20158. Bibcode:2025Sci...388..400Z. doi:10.1126/science.adn6088. PMID 40273242.
  22. ^ 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.
  23. ^ 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].
  24. ^ Rodrigues, J.; et al. (20 February 2025). "TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO". Astronomy and Astrophysics. 695: A237. arXiv:2502.14472. Bibcode:2025A&A...695A.237R. doi:10.1051/0004-6361/202452887.
  25. ^ Lockley, Isobel S.; Armstrong, David J.; Fernández, Jorge Fernández; Millholland, Sarah; Knierim, Henrik; Mena, Elisa Delgado; Sousa, Sergio; Collins, Karen A.; Watkins, Cristilyn N.; Howell, Steve B.; Adibekyan, Vardan; Helled, Ravit; Ziegler, Carl; Bayliss, Daniel; Briceño, César (June 2025). "The TOI-1117 Multi-planetary System: 3 sub-Neptunes, 1 in both the Neptunian Desert and Radius Valley". Monthly Notices of the Royal Astronomical Society. 541 (2): 919–938. arXiv:2506.05521. Bibcode:2025MNRAS.tmp..926L. doi:10.1093/mnras/staf939. ISSN 0035-8711.{{cite journal}}: CS1 maint: bibcode (link)
  26. ^ 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. A super-Earth and one of the lowest mass sub-Neptunes". Astronomy & Astrophysics. 696. arXiv:2503.07529. Bibcode:2025A&A...696A..86S. doi:10.1051/0004-6361/202452969.
  27. ^ Soubkiou, Abderahmane; Barkaoui, Khalid; Benkhaldoun, Zouhair; Ghachoui, Mourad; Chouqar, Jamila; Rackham, Benjamin V.; Burgasser, Adam; Softich, Emma; Pallé, Enric (23 June 2025). "TOI-1846b: A super-Earth in the radius valley orbiting a nearby M dwarf". Monthly Notices of the Royal Astronomical Society. arXiv:2506.18550. Bibcode:2025MNRAS.tmp..978S. doi:10.1093/mnras/staf1030.{{cite journal}}: CS1 maint: bibcode (link)
  28. ^ Bieryla, Allyson; et al. (39) (27 March 2025). "TOI-2005b: An Eccentric Warm Jupiter in Spin-orbit Alignment". The Astronomical Journal. 169 (5): 273. arXiv:2503.20069. Bibcode:2025AJ....169..273B. doi:10.3847/1538-3881/adc441.
  29. ^ Barkaoui, K.; et al. (10 February 2025). "TOI-2015b: a sub-Neptune in strong gravitational interaction with an outer non-transiting planet". Astronomy and Astrophysics. 695: A281. arXiv:2502.07074. Bibcode:2025A&A...695A.281B. doi:10.1051/0004-6361/202452916.
  30. ^ 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].
  31. ^ Janó Muñoz, C.; Hooton, M. J.; Pedersen, P. P.; Barkaoui, K.; Rackham, B. V.; Burgasser, A. J.; Pozuelos, F. J.; Stassun, K. G.; Queloz, D.; Triaud, A. H. M. J.; Ziegler, C.; Almenara, J. M.; Timmermans, M.; Bonfils, X.; Collins, K. A. (June 2025). "TOI-2407 b: a warm Neptune in the desert". Monthly Notices of the Royal Astronomical Society. 541: 630–641. arXiv:2506.05521. Bibcode:2025MNRAS.tmp..932M. doi:10.1093/mnras/staf946. ISSN 0035-8711.{{cite journal}}: CS1 maint: bibcode (link)
  32. ^ Chaturvedi, P.; Goffo, E.; Gandolfi, D.; Persson, C. M.; Hatzes, A. P.; Nowak, G.; Bonfanti, A.; Bieryla, A.; Cochran, W. D.; Collins, K. A.; Fajardo-Acosta, S. B.; Howell, S. B.; Jenkins, J. M.; Korth, J.; Livingston, J.; Pallé, E.; Quinn, S. N.; Schwarz, R. P.; Seager, S.; Shporer, A.; Stassun, K. G.; Striegel, S.; Van Eylen, V.; Watkins, C. N.; Winn, J. N.; Ziegler, C. (17 April 2025). "TOI-3493 b: A planet with a Neptune-like density transiting a bright G0-type star". Astronomy and Astrophysics. 697: A169. arXiv:2504.12884. Bibcode:2025A&A...697A.169C. doi:10.1051/0004-6361/202453511.
  33. ^ 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.
  34. ^ 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.
  35. ^ a b Naponiello, L.; Vissapragada, S.; Bonomo, A. S.; Steinmeyer, M.-L.; Filomeno, S.; D'Orazi, V.; Dorn, C.; Sozzetti, A.; Mancini, L. (15 May 2025). "The Hot-Neptune Initiative (HONEI) I. Two hot sub-Neptunes on a close-in, eccentric orbit (TOI-5800 b) and a farther-out, circular orbit (TOI-5817 b)". arXiv:2505.10123 [astro-ph.EP].
  36. ^ 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.
  37. ^ 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].
  38. ^ Scott, Madison G.; Triaud, Amaury H. M. J.; Barkaoui, Khalid; Sebastian, Daniel; Burgasser, Adam J.; Collins, Karen A.; Dransfield, Georgina; Hellier, Coel; Howell, Steve B.; Piette, Anjali A. A.; Rackham, Benjamin V.; Stassun, Keivan G.; Stokholm, Amalie; Timmermans, Mathilde; Watkins, Cristilyn N.; Fausnaugh, Michael; Fukui, Akihiko; Jenkins, Jon M.; Narita, Norio; Ricker, George; Softich, Emma; Schwarz, Richard P.; Seager, Sara; Shporer, Avi; Theissen, Christopher; Twicken, Joseph D.; Winn, Joshua N.; Watanabe, David (9 April 2025). "TOI-6478 b: a cold under-dense Neptune transiting a fully convective M dwarf from the thick disc". Monthly Notices of the Royal Astronomical Society. 540 (2): 1909–1927. arXiv:2504.06848. Bibcode:2025MNRAS.540.1909S. doi:10.1093/mnras/staf684.
  39. ^ Eberhardt, Jan; Trifonov, Trifon (2025). "TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey". The Astronomical Journal. 169 (6): 298. arXiv:2504.20999. Bibcode:2025AJ....169..298E. doi:10.3847/1538-3881/adc44e.
  40. ^ Bryant, Edward M.; Jordán, Andrés; Hartman, Joel D.; Bayliss, Daniel; Sedaghati, Elyar; Barkaoui, Khalid; Chouqar, Jamila; Pozuelos, Francisco J.; Thorngren, Daniel P.; Timmermans, Mathilde; Almenara, Jose Manuel; Chilingarian, Igor V.; Collins, Karen A.; Gan, Tianjun; Howell, Steve B. (June 2025). "A transiting giant planet in orbit around a 0.2-solar-mass host star". Nature Astronomy. arXiv:2506.07931. Bibcode:2025NatAs.tmp..129B. doi:10.1038/s41550-025-02552-4. ISSN 2397-3366.{{cite journal}}: CS1 maint: bibcode (link)
  41. ^ a b c d Schanche, N.; et al. (55) (10 April 2025). "A Swarm of WASP Planets: Nine giant planets identified by the WASP survey". The Astronomical Journal. 169 (6): 334. arXiv:2504.08091. Bibcode:2025AJ....169..334S. doi:10.3847/1538-3881/adccc6.
  42. ^ Kanodia, Shubham; Cañas, Caleb I.; Mahadevan, Suvrath; Lin, Andrea S. J.; Kobulnicky, Henry A.; Karfs, Ian; Birkholz, Alexina; Gupta, Arvind; Everett, Mark (2025). "Searching for GEMS: TOI-7149~b an Inflated Giant Planet causing a 12% Transit of a Fully Convective M-dwarf". arXiv:2506.17861 [astro-ph.EP].
Retrieved from "https://en.wikipedia.org/w/index.php?title=List_of_exoplanets_discovered_in_2025&oldid=1299888936"