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List of exoplanets discovered in 2024

From Wikipedia, the free encyclopedia

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 2024 is a list of confirmed exoplanets that were first reported in 2024. 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
BD-14 3065 b 12.11+0.95
−0.91 		1.926±0.094 4.3 0.0646±0.0026 1957±28 transit 1847.4[1][a] 1.4±0.06 6985±90 Located in a triple star system. It orbits the primary component of the system (BD-14 3065 A), a subgiant star.[2] Also known as TOI-4987 b
CI Tauri c 3.6±0.3 25.2±1.8 0.17 radial vel. 522.6±1.3 0.9±0.02 4250±50 [3]Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu.[4][3]
Gliese 341 b 0.00227±0.00044 0.0821±0.045 7.577 540 transit 33.9 0.506 3745 [5]Also known as TOI-741 b
HD 77946 b 0.02637±0.00415 0.24133+0.00767
−0.0071 		6.527 0.072±0.0012 1248+40
−38 		transit 322.7±1 1.17±0.06 6046.0±50.0 [6]Also known as TOI-1778 b
HD 104067 c 0.0415 13.8992+0.0047
−0.0037 		0.1058±0.0013 radial vel. 66.34±0.03 0.82±0.03 4952±100 [7]Another planet in the system is suspected.
HD 134606 e 0.00726+0.00113
−0.0011 		4.32 0.0527±0.0012 radial vel. 87.4±0.068 1.046+0.07
−0.059 		5576+86
−85 		[8]
HD 134606 f 0.01737+0.00232
−0.00229 		26.915 0.1784±0.004 radial vel. 87.4±0.068 1.046+0.07
−0.059 		5576+86
−85 		[8]
HD 63433 d 0.09573±0.0141 4.21 0.0503±0.0027 1040±40 transit 71.7 0.99±0.03 5688±28 [9]Hot Earth-sized exoplanet
HS Piscium b 1.44+0.56
−0.44 		3.986 0.0435±0.0017 radial vel. 122.79+0.12
−0.14 		0.69±0.07 4203±116 [10]
KMT-2016-BLG-2321Lb 3.58±1.22 3.58±0.81 microlensing 11,670±3980 0.73±0.28 [11]
KMT-2023-BLG-0416Lb 6.15+3.03
−3.2 		3.73+0.56
−0.8 		microlensing 20,640+3100
−4400 		0.61+0.3
−0.32 		[12]The mass of the planet can be as low as 0.042+0.021
−0.022 MJ
KMT-2023-BLG-0469Lb 0.124+0.092
−0.067 		2.37±0.9 microlensing 23,050+3260
−3910 		0.47±0.36 [13]
KMT-2023-BLG-0735Lb 0.12±0.07 2.75±1 microlensing 20,830+3910
−3260 		0.61±0.34 [13]
KMT-2023-BLG-1454Lb 0.63+0.71
−0.34 		1.18+0.17
−0.18 		microlensing 23,540+3460
−3590 		0.17+0.19
−0.09 		[12]Estimates of the planet's mass varies between 0.3+0.34
−0.16 MJ and 0.77+0.87
−0.42 MJ
KMT-2023-BLG-1642Lb 1.08+1.53
−0.58 		1.41+0.22
−0.27 		microlensing 22,750+3550
−4370 		0.17+0.24
−0.09 		[12]
LHS 1678 d 0.00289+0.00208
−0.00107 		0.08752±0.0062 4.965 0.04+0.0018
−0.0017 		transit 65 0.345±0.014 3490±50 [14]
M62H b 2.83 0.133 0.004908 timing 21,500[15] 1.4 Pulsar planet located in the globular cluster Messier 62.[16]
MOA-2016-BLG-526Lb 6.93±0.75 2.07±0.35 microlensing [11]
MOA-2022-BLG-563Lb 0.4+0.31
−0.25 		2.25±0.25 microlensing 21,290+3650
−5220 		0.48+0.36
−0.3 		[13]
OGLE-2016-BLG-1598Lb 5.91±1.74 2.5±0.88 microlensing 19,270±5670 0.55±0.32 [11]
NGTS-30 b 0.96 0.93 98.3 0.408 390 transit 762.5 0.94 5455 [17] Also known as TOI-4862 b
OGLE-2016-BLG-1800Lb 2.59±1.46 1.88±0.51 microlensing 21,100±3360 0.41±0.22 [11]
OGLE-2017-BLG-0640Lb 1.62+1.64
−0.94 		1.14±0.38 microlensing 21,600+3550
−4730 		0.32+0.32
−0.18 		[18]
OGLE-2017-BLG-1237Lb 3.8+2.49
−1.99 		2.53+0.5
−0.64 		microlensing 19,660+3060
−4990 		0.46+0.3
−0.24 		[18]
OGLE-2017-BLG-1275Lb 5.9±2.2 1.19±0.36 microlensing 25,070±2930 0.63±0.23 [18]Another solution suggests a larger semi-major axis, of 2.09±0.63 AU
OGLE-2023-BLG-0836Lb 4.36+2.35
−2.2 		3.7+1
−1.2 		microlensing 16,690+4430
−5250 		[b] [19]The planet is located in a binary star system, and is likely to be orbiting both stars in the system.
S1429 b 1.8±0.2 77.51±0.2 0.384±0.4 683±9 radial vel. 2836±26 1.26±0.04 6000±40 [20]Located in the open cluster Messier 67
Teegarden's Star d 0.00258±0.00053 26.13 0.0791 ±0.0027 159±3 radial vel. 12.5 0.097±0.01 3034±45 Orbits beyond the habitable zone of its star. Another planet in the system is suspected.[21]
TIC 4672985 b 12.74±1.01 1.026+0.065
−0.067 		69.05 0.33±0.019 517.2+11.3
−11.2 		transit 1.01±0.03 5757+72
−65 		[22]
TIC 139270665 b 0.463 0.645 23.624 0.163 700 transit 486 1.035 5844 [23]
TOI-238 c 0.0211±0.0035 0.1945±0.0161 8.466 0.0749±0.0013 696±15 transit 261.328±0.312 0.79±0.022 5059±89 [24]
TOI-815 b 0.0239±0.0047 0.2622±0.0044 11.197 0.0903+0.0018
−0.0019 		686+13
−14 		transit 193.76±0.15 0.776±0.036 4869±77 [25] The host star is part of a binary star system with a red dwarf companion
TOI-815 c 0.0739±0.00755 0.2337+0.0089
−0.008 		34.976 0.193±0.004 469±9 transit 193.76±0.15 0.776±0.036 4869±77 [25] The host star is part of a binary star system with a red dwarf companion
TOI-1135 b 0.062+0.033
−0.031 		0.805±0.02 5.13±0.27 0.082±0.003 1198.9±21.3 transit 371.4±0.5 1.125±0.032 6122±25 [26]
TOI-1173 A b 0.08213±0.00598 0.723±0.015 7.064 0.0702±0.0012 863.9±9.8 transit 0.911+0.028
−0.03 		5350±340 [27]Low-density planet
TOI-1194 b 0.456+0.055
−0.051 		0.947+0.035
−0.033 		5.963 0.0674±0.001 1391+38
−37 		transit 802.44+35.05
−36.27 		1.057+0.050
−0.049 		5769+49
−50 		[28] The host star has also a low-mass star companion with a mass of 96.5±1.5 MJ
TOI-1199 b 0.239±0.02 0.938±0.025 3.671 0.04988+ 1486±20 transit 805±2.6 1.23±0.07 5710±40 [29]
TOI-1273 b 0.222±0.015 0.99±0.2 4.631 0.0549±0.001 1211±15 transit 574±1.3 1.06±0.06 5690±40 [29]
TOI-1347 b 0.0349±0.0038 0.161±0.009 0.847 1400±40 transit 480.8±2 0.913±0.033 5464±100 [30] Ultra-short period planet
TOI-1347 c 0.0088±0.0072 0.143±0.009 4.842 1000±25 transit 480.8±2 0.913±0.033 5464±100 [30]
TOI-1386 b 0.148+0.019
−0.018 		0.54+0.018
−0.016 		25.838 0.1732+0.0027
−0.0033 		676.4+10
−8.3 		transit 478.8±2.2 1.038+0.05
−0.058 		5793+76
−73 		[31]
TOI-1386 c 0.309±0.038 227.6+4.6
−4 		0.739+0.015
−0.016 		327.4+5.3
−4.6 		radial vel. 478.8±2.2 1.038+0.05
−0.058 		5793+76
−73 		[31]
TOI-1751 b 0.0538±0.0101 0.2489±0.0259 37.468 0.2115±0.0024 820 transit 370.3±0.3 1.15±0.17 6116±22 [32]The host star is metal-poor ([Fe/H] = –0.40 dex)
TOI-1855 b 1.133±0.096 1.65+0.37
−0.62 		1.364 0.02398+0.00037
−0.00036 		1700±20 transit + radial vel. 576.3±4.6 0.987+0.058
−0.045 		5359+89
−83 		[33]
TOI-2107 b 0.83±0.11 1.211±0.035 2.454 0.0315+0.0006
−0.00067 		1397±20 transit + radial vel. 767.4+6.2
−5.9 		0.961+0.049
−0.054 		5627+94
−93 		[33]
TOI-2266 b 0.1374±0.008 2.326 0.02±0.002 550±47 transit 168.6±0.2 0.23±0.02 3240±160 [34]
TOI-2368 b 0.65±0.18 0.967+0.06
−0.03 		5.175 0.05649±0.001 1000+44
−30 		transit 685±3.9 0.897+0.048
−0.049 		5360+230
−170 		[33]
TOI-2373 b 9.3±0.2 0.93±0.02 13.337 0.112±0.001 860±10 transit 1617±33 1.041+0.032
−0.028 		5651±180 [35]
TOI-2416 b 3+0.1
−0.09 		0.88±0.02 8.275 0.0831±0.0007 1080±10 transit 1767±261 1.118+0.029
−0.027 		5808±80 [35]
TOI-2524 b 0.64±0.04 1+0.02
−0.03 		7.186 0.073±0.0007 1100±20 transit 1399±36 1.007+0.032
−0.029 		5831±80 [35]
TOI-2529 b 2.34±0.2 1.03±0.05 64.5949±0.0003 0.327±0.02 636±15.7 transit 965.8+14
−13.7 		1.11+0.02
−0.02 		5802+60
−52 		[22]
TOI-3321 b 0.554±0.076 1.39+0.07
−0.06 		3.652 0.047±0.001 1616±30 transit 928+10.8
−10.4 		1.041+0.084
−0.068 		5850±140 [33]
TOI-3894 b 0.85±0.15 1.36±0.05 4.335 0.0543±0.0014 1519±22 transit 1343+12.7
−12.4 		1.138+0.089
−0.075 		6000±110 [33]
TOI-3919 b 3.88±0.023 1.1±0.05 7.433 0.0795±0.0016 1200±15 transit 1973+28.7
−28.4 		1.208+0.067
−0.07 		6100±110 [33]
TOI-4153 b 1.15±0.38 1.438±0.045 4.617 0.06311+0.00084
−0.00096 		1670+30
−40 		transit 1366±11.4 1.572+0.064
−0.071 		6860+150
−180 		[33]
TOI-4438 b 0.017±0.0035 0.2248±0.0116 7.44 0.0534±0.009 400±50 transit 98 0.368±0.021 3422±81 [36]
TOI-5232 b 2.34±0.16 1.14+0.05
−0.045 		4.097 0.0599±0.001 1772+40
−45 		transit 1985+28
−27 		1.389+0.068
−0.075 		6500+180
−190 		[33]
TOI-5301 b 3.65±0.4 1.18+0.08
−0.07 		5.859 0.0726+0.0013
−0.0024 		1655±40 transit 1914+59
−55 		1.483+0.081
−0.14 		6240±160 [33]
V808 Aurigae b [ru] 6.8±0.7 4109±362 timing 698±13 0.9±0.1 [37]The planet's host star is a polar. The mass value for the planet is only a minimum mass.
Wolf 327 b 0.00796±0.00145 0.1106±0.0054 0.573 0.01 996±22 transit 92.9 0.405±0.019 3542±70 [38] Ultra-short period planet

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Transcription

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery


References

  1. ^ "BD-14 3065". SIMBAD. Centre de données astronomiques de Strasbourg.
  2. ^ Šubjak, Ján; Latham, David W.; Quinn, Samuel N.; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Brahm, Rafael; Guenther, Eike; Janík, Jan (18 March 2024). "BD-14 3065b (TOI-4987b): from giant planet to brown dwarf: evidence for deuterium burning in old age?". arXiv:2403.12311 [astro-ph.EP].
  3. ^ a b "CI Tau | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 29 March 2024.
  4. ^ Martin, Pierre-Yves (2024). "Planet Cl Tau c". exoplanet.eu. Retrieved 29 March 2024.
  5. ^ Kirk, James; Stevenson, Kevin B.; Fu, Guangwei; Lustig-Yaeger, Jacob; Moran, Sarah E.; Peacock, Sarah; Alam, Munazza K.; Batalha, Natasha E.; Bennett, Katherine A. (11 January 2024), "JWST/NIRCam Transmission Spectroscopy of the Nearby Sub-Earth GJ 341b", The Astronomical Journal, 167 (3): 90, arXiv:2401.06043, Bibcode:2024AJ....167...90K, doi:10.3847/1538-3881/ad19df
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  9. ^ Capistrant, Benjamin K.; Soares-Furtado, Melinda; Vanderburg, Andrew; Jankowski, Alyssa; Mann, Andrew W.; Ross, Gabrielle; Srdoc, Gregor; Hinkel, Natalie R.; Becker, Juliette (9 January 2024), "TESS Hunt for Young and Maturing Exoplanets (THYME) XI: An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400Myr Ursa Major Moving Group", The Astronomical Journal, 167 (2): 54, arXiv:2401.04785, Bibcode:2024AJ....167...54C, doi:10.3847/1538-3881/ad1039
  10. ^ Tran, Quang H.; Bowler, Brendan P.; Cochran, William D.; Halverson, Samuel; Mahadevan, Suvrath; Ninan, Joe P.; Robertson, Paul; Stefánsson, Guðmundur; Terrien, Ryan C. (4 March 2024). "The Epoch of Giant Planet Migration Planet Search Program. II. A Young Hot Jupiter Candidate around the AB Dor Member HS Psc". The Astronomical Journal. 167 (5): 193. arXiv:2403.02378. Bibcode:2024AJ....167..193T. doi:10.3847/1538-3881/ad2eaf.
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  13. ^ a b c Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun (20 January 2024). "MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planets". arXiv:2401.11329 [astro-ph.EP].
  14. ^ Silverstein, Michele L.; Barclay, Thomas; Schlieder, Joshua E.; Collins, Karen A.; Schwarz, Richard P.; Hord, Benjamin J.; Rowe, Jason F.; Kruse, Ethan; Astudillo-Defru, Nicola (29 February 2024). "Validation of a Third Planet in the LHS 1678 System". arXiv:2403.00110 [astro-ph.EP].
  15. ^ Oliveira, R. A. P.; Ortolani, S.; Barbuy, B.; Kerber, L. O.; Maia, F. F. S.; Bica, E.; Cassisi, S.; Souza, S. O.; Pérez-Villegas, A. (January 2022). "Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters". Astronomy & Astrophysics. 657: A123. arXiv:2110.13943. Bibcode:2022A&A...657A.123O. doi:10.1051/0004-6361/202141596. ISSN 0004-6361.
  16. ^ Vleeschower, L.; Corongiu, A.; Stappers, B. W.; Freire, P. C. C.; Ridolfi, A.; Abbate, F.; Ransom, S. M.; Possenti, A.; Padmanabh, P. V.; Balakrishnan, V.; Kramer, M.; Krishnan, V. Venkatraman; Zhang, L.; Bailes, M.; Barr, E. D. (1 March 2024). "Discoveries and timing of pulsars in M62". Monthly Notices of the Royal Astronomical Society. arXiv:2403.12137. Bibcode:2024MNRAS.tmp..838V. doi:10.1093/mnras/stae816. ISSN 0035-8711.{{cite journal}}: CS1 maint: bibcode (link)
  17. ^ Battley, M. P.; Collins, K. A.; Ulmer-Moll, S.; Quinn, S. N.; Lendl, M.; Gill, S.; Brahm, R.; Hobson, M. J.; Osborn, H. P. (3 April 2024), NGTS-30 b/TOI-4862 b: An 1 Gyr old 98-day transiting warm Jupiter, arXiv:2404.02974
  18. ^ a b c Ryu, Yoon-Hyun; Udalski, Andrzej; Yee, Jennifer C.; Zang, Weicheng; Shvartzvald, Yossi; Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil; Shin, In-Gu; Yang, Hongjing; Cha, Sang-Mok; Kim, Dong-Jin (1 March 2024). "Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets". The Astronomical Journal. 167 (3): 88. arXiv:2307.13359. Bibcode:2024AJ....167...88R. doi:10.3847/1538-3881/ad1888. ISSN 0004-6256.
  19. ^ Han, Cheongho; Udalski, Andrzej; Jung, Youn Kil; Gould, Andrew; Kim, Doeon; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk (12 February 2024). "OGLE-2023-BLG-0836L: The sixth microlensing planet in a binary stellar system". arXiv:2402.08116 [astro-ph.EP].
  20. ^ Thomas, Luis; Saglia, Roberto; Pasquini, Luca; Brucalassi, Anna; Bonifacio, Piercarlo; de Medeiros, José Renan; Leão, Izan de Castro; Martins, Bruno Leonardo Canto; Ruh, Henrik Lukas (5 March 2024). "Search for giant planets in M67 V: a warm Jupiter orbiting the turn-off star S1429". arXiv:2403.02911 [astro-ph.EP].
  21. ^ Dreizler, S.; Luque, R.; Ribas, I.; Koseleva, V.; Ruh, H. L.; Nagel, E.; Pozuelos, F. J.; Zechmeister, M.; Reiners, A. (1 February 2024). "Teegarden's Star revisited: A nearby planetary system with at least three planets". arXiv:2402.00923 [astro-ph.EP].
  22. ^ a b Jones, Matias I.; Reinarz, Yared; Brahm, Rafael; Pinto, Marcelo Tala; Eberhardt, Jan; Rojas, Felipe; Triaud, Amaury H. M. J.; Gupta, Arvind F.; Ziegler, Carl (17 January 2024). "A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS". Astronomy and Astrophysics. 683: A192. arXiv:2401.09657. Bibcode:2024A&A...683A.192J. doi:10.1051/0004-6361/202348147.
  23. ^ Peluso, Daniel O’Conner; Dalba, Paul A.; Wright, Duncan; Esposito, Thomas M.; Sgro, Lauren A.; Weaver, Ian C.; Marchis, Franck; Dragomir, Diana; Villanueva, Steven; Fulton, Benjamin; Isaacson, Howard; Gupta, Arvind F.; Jacobs, Thomas Lee; LaCourse, Daryll M.; Gagliano, Robert (March 2024). "Confirming the Warm and Dense Sub-Saturn TIC 139270665 b with the Automated Planet Finder and Unistellar Citizen Science Network". The Astronomical Journal. 167 (4): 170. Bibcode:2024AJ....167..170P. doi:10.3847/1538-3881/ad2772. ISSN 1538-3881.
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  1. ^ Derived from a parallax of 1.7646 mas
  2. ^ The planet is located in a two-star system, with masses of 0.78+0.38
    −0.36     M☉     and 0.56+0.3
    −0.28     M☉    . There is a large chance that it is orbiting both stars in the system, so the "host star mass" would be 0.78+0.38
    −0.36     M☉     + 0.56+0.3
    −0.28     M☉    . However, there is a small chance that is orbiting only one of the stars in the system.
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