List of exoplanets discovered in 2024

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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 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.

Contents

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 b12.11+0.95
−0.91		1.926±0.0944.30.0646±0.00261957±28transit1847.4 [1] [lower-alpha 1] 1.4±0.066985±90Located 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±0.325.2±1.80.17radial vel.522.6±1.30.9±0.024250±50 [3] Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu. [4] [3]
Gliese 341 b0.00227±0.000440.0821±0.0457.577540transit33.90.5063745 [5] Also known as TOI-741 b
HD 77946 b0.02637±0.004150.24133+0.00767
−0.0071		6.5270.072±0.00121248+40
−38		transit322.7±11.17±0.066046.0±50.0 [6] Also known as TOI-1778 b
HD 104067 c 0.041513.8992+0.0047
−0.0037		0.1058±0.0013radial vel.66.34±0.030.82±0.034952±100 [7] Another planet in the system is suspected.
HD 134606 e 0.00726+0.00113
−0.0011		4.320.0527±0.0012radial vel.87.4±0.0681.046+0.07
−0.059		5576+86
−85		 [8]
HD 134606 f 0.01737+0.00232
−0.00229		26.9150.1784±0.004radial vel.87.4±0.0681.046+0.07
−0.059		5576+86
−85		 [8]
HD 63433 d 0.09573±0.01414.210.0503±0.00271040±40transit71.70.99±0.035688±28 [9] Hot Earth-sized exoplanet
HS Piscium b 1.44+0.56
−0.44		3.9860.0435±0.0017radial vel.122.79+0.12
−0.14		0.69±0.074203±116 [10]
KMT-2016-BLG-2321Lb3.58±1.223.58±0.81microlensing11,670±39800.73±0.28 [11]
KMT-2023-BLG-0416Lb6.15+3.03
−3.2		3.73+0.56
−0.8		microlensing20,640+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-0469Lb0.124+0.092
−0.067		2.37±0.9microlensing23,050+3260
−3910		0.47±0.36 [13]
KMT-2023-BLG-0735Lb0.12±0.072.75±1microlensing20,830+3910
−3260		0.61±0.34 [13]
KMT-2023-BLG-1454Lb0.63+0.71
−0.34		1.18+0.17
−0.18		microlensing23,540+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-1642Lb1.08+1.53
−0.58		1.41+0.22
−0.27		microlensing22,750+3550
−4370		0.17+0.24
−0.09		 [12]
LHS 1678 d 0.00289+0.00208
−0.00107		0.08752±0.00624.9650.04+0.0018
−0.0017		transit650.345±0.0143490±50 [14]
M62H b 2.830.1330.004908timing21,500 [15] 1.4 Pulsar planet located in the globular cluster Messier 62. [16]
MOA-2016-BLG-526Lb6.93±0.752.07±0.35microlensing [11]
MOA-2022-BLG-563Lb0.4+0.31
−0.25		2.25±0.25microlensing21,290+3650
−5220		0.48+0.36
−0.3		 [13]
OGLE-2016-BLG-1598Lb5.91±1.742.5±0.88microlensing19,270±56700.55±0.32 [11]
NGTS-30 b0.960.9398.30.408390transit762.50.945455 [17] Also known as TOI-4862 b
OGLE-2016-BLG-1800Lb2.59±1.461.88±0.51microlensing21,100±33600.41±0.22 [11]
OGLE-2017-BLG-0640Lb1.62+1.64
−0.94		1.14±0.38microlensing21,600+3550
−4730		0.32+0.32
−0.18		 [18]
OGLE-2017-BLG-1237Lb3.8+2.49
−1.99		2.53+0.5
−0.64		microlensing19,660+3060
−4990		0.46+0.3
−0.24		 [18]
OGLE-2017-BLG-1275Lb5.9±2.21.19±0.36microlensing25,070±29300.63±0.23 [18] Another solution suggests a larger semi-major axis, of 2.09±0.63 AU
OGLE-2023-BLG-0836Lb4.36+2.35
−2.2		3.7+1
−1.2		microlensing16,690+4430
−5250		 [lower-alpha 2] [19] The planet is located in a binary star system, and is likely to be orbiting both stars in the system.
S1429 b1.8±0.277.51±0.20.384±0.4683±9radial vel.2836±261.26±0.046000±40 [20] Located in the open cluster Messier 67
Teegarden's Star d 0.00258±0.0005326.130.0791 ±0.0027159±3radial vel.12.50.097±0.013034±45Orbits beyond the habitable zone of its star. Another planet in the system is suspected. [21]
TIC 4672985 b12.74±1.011.026+0.065
−0.067		69.050.33±0.019517.2+11.3
−11.2		transit1.01±0.035757+72
−65		 [22]
TIC 139270665 b0.4630.64523.6240.163700transit4861.0355844 [23]
TOI-238 c0.0211±0.00350.1945±0.01618.4660.0749±0.0013696±15transit261.328±0.3120.79±0.0225059±89 [24]
TOI-815 b0.0239±0.00470.2622±0.004411.1970.0903+0.0018
−0.0019		686+13
−14		transit193.76±0.150.776±0.0364869±77 [25] The host star is part of a binary star system with a red dwarf companion
TOI-815 c0.0739±0.007550.2337+0.0089
−0.008		34.9760.193±0.004469±9transit193.76±0.150.776±0.0364869±77 [25] The host star is part of a binary star system with a red dwarf companion
TOI-1135 b0.062+0.033
−0.031		0.805±0.025.13±0.270.082±0.0031198.9±21.3transit371.4±0.51.125±0.0326122±25 [26]
TOI-1173 A b 0.08213±0.005980.723±0.0157.0640.0702±0.0012863.9±9.8transit0.911+0.028
−0.03		5350±340 [27] Low-density planet
TOI-1194 b0.456+0.055
−0.051		0.947+0.035
−0.033		5.9630.0674±0.0011391+38
−37		transit802.44+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 b0.239±0.020.938±0.0253.6710.04988+1486±20transit805±2.61.23±0.075710±40 [29]
TOI-1273 b0.222±0.0150.99±0.24.6310.0549±0.0011211±15transit574±1.31.06±0.065690±40 [29]
TOI-1347 b 0.0349±0.00380.161±0.0090.8471400±40transit480.8±20.913±0.0335464±100 [30] Ultra-short period planet
TOI-1347 c 0.0088±0.00720.143±0.0094.8421000±25transit480.8±20.913±0.0335464±100 [30]
TOI-1386 b0.148+0.019
−0.018		0.54+0.018
−0.016		25.8380.1732+0.0027
−0.0033		676.4+10
−8.3		transit478.8±2.21.038+0.05
−0.058		5793+76
−73		 [31]
TOI-1386 c0.309±0.038227.6+4.6
−4		0.739+0.015
−0.016		327.4+5.3
−4.6		radial vel.478.8±2.21.038+0.05
−0.058		5793+76
−73		 [31]
TOI-1751 b0.0538±0.01010.2489±0.025937.4680.2115±0.0024820transit370.3±0.31.15±0.176116±22 [32] The host star is metal-poor ([Fe/H] = –0.40 dex)
TOI-1855 b1.133±0.0961.65+0.37
−0.62		1.3640.02398+0.00037
−0.00036		1700±20transit + radial vel.576.3±4.60.987+0.058
−0.045		5359+89
−83		 [33]
TOI-2107 b0.83±0.111.211±0.0352.4540.0315+0.0006
−0.00067		1397±20transit + radial vel.767.4+6.2
−5.9		0.961+0.049
−0.054		5627+94
−93		 [33]
TOI-2266 b0.1374±0.0082.3260.02±0.002550±47transit168.6±0.20.23±0.023240±160 [34]
TOI-2368 b0.65±0.180.967+0.06
−0.03		5.1750.05649±0.0011000+44
−30		transit685±3.90.897+0.048
−0.049		5360+230
−170		 [33]
TOI-2373 b9.3±0.20.93±0.0213.3370.112±0.001860±10transit1617±331.041+0.032
−0.028		5651±180 [35]
TOI-2416 b3+0.1
−0.09		0.88±0.028.2750.0831±0.00071080±10transit1767±2611.118+0.029
−0.027		5808±80 [35]
TOI-2524 b0.64±0.041+0.02
−0.03		7.1860.073±0.00071100±20transit1399±361.007+0.032
−0.029		5831±80 [35]
TOI-2529 b2.34±0.21.03±0.0564.5949±0.00030.327±0.02636±15.7transit965.8+14
−13.7		1.11+0.02
−0.02		5802+60
−52		 [22]
TOI-3321 b0.554±0.0761.39+0.07
−0.06		3.6520.047±0.0011616±30transit928+10.8
−10.4		1.041+0.084
−0.068		5850±140 [33]
TOI-3894 b0.85±0.151.36±0.054.3350.0543±0.00141519±22transit1343+12.7
−12.4		1.138+0.089
−0.075		6000±110 [33]
TOI-3919 b3.88±0.0231.1±0.057.4330.0795±0.00161200±15transit1973+28.7
−28.4		1.208+0.067
−0.07		6100±110 [33]
TOI-4153 b1.15±0.381.438±0.0454.6170.06311+0.00084
−0.00096		1670+30
−40		transit1366±11.41.572+0.064
−0.071		6860+150
−180		 [33]
TOI-4436 b0.189116.3370.0872+0.0013
−0.0014		308±9transit73.150.331±0.0153298+75
−73		 [36] Located in a triple hierarchical stellar system
TOI-4438 b0.017±0.00350.2248±0.01167.440.0534±0.009400±50transit980.368±0.0213422±81 [37]
TOI-5232 b2.34±0.161.14+0.05
−0.045		4.0970.0599±0.0011772+40
−45		transit1985+28
−27		1.389+0.068
−0.075		6500+180
−190		 [33]
TOI-5301 b3.65±0.41.18+0.08
−0.07		5.8590.0726+0.0013
−0.0024		1655±40transit1914+59
−55		1.483+0.081
−0.14		6240±160 [33]
V808 Aurigae b  [ ru ]6.8±0.74109±362timing698±130.9±0.1 [38] The planet's host star is a polar. The mass value for the planet is only a minimum mass.
Wolf 327 b 0.00796±0.001450.1106±0.00540.5730.01996±22transit92.90.405±0.0193542±70 [39] Ultra-short period planet

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

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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. 1 2 "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
  6. ↑ Palethorpe, L.; John, A. Anna; Mortier, A.; Davoult, J.; Wilson, T. G.; Rice, K.; Cameron, A. C.; Alibert, Y.; Buchhave, L. A. (7 March 2024). "Confronting compositional confusion through the characterisation of the sub-Neptune orbiting HD 77946". Monthly Notices of the Royal Astronomical Society. 529 (4): 3323. arXiv: 2403.04464 . Bibcode:2024MNRAS.529.3323P. doi:10.1093/mnras/stae707.
  7. ↑ Kane, Stephen R.; Fetherolf, Tara; Li, Zhexing; Polanski, Alex S.; Howard, Andrew W.; Isaacson, Howard; Močnik, Teo; Welter, Sadie G. (25 March 2024). "A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World". arXiv: 2403.17062 [astro-ph.EP].
  8. 1 2 Li, Zhexing; Kane, Stephen R.; Brandt, Timothy D.; Fetherolf, Tara; Robertson, Paul; Zhao, Jinglin; Dalba, Paul A.; Wittenmyer, Robert A.; Butler, R. Paul (30 January 2024), "Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System", The Astronomical Journal, 167 (4): 155, arXiv: 2401.17415 , Bibcode:2024AJ....167..155L, doi: 10.3847/1538-3881/ad2461
  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 .
  11. 1 2 3 4 Shin, In-Gu; Yee, Jennifer C.; Zang, Weicheng; Han, Cheongho; Yang, Hongjing; Gould, Andrew; Lee, Chung-Uk; Udalski, Andrzej; Sumi, Takahiro (8 January 2024), "Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Sub-Prime Field Planets", arXiv: 2401.04256 [astro-ph.EP]
  12. 1 2 3 Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil (16 January 2024). "KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals". Astronomy and Astrophysics. 683: A187. arXiv: 2401.08904 . Bibcode:2024A&A...683A.187H. doi:10.1051/0004-6361/202348245.
  13. 1 2 3 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. 530 (2): 1436–1456. 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. 1 2 3 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". Astronomy and Astrophysics. 684. arXiv: 2402.00923 . Bibcode:2024A&A...684A.117D. doi:10.1051/0004-6361/202348033.
  22. 1 2 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.
  24. ↑ Mascareño, A. Suárez; Passegger, V. M.; Hernández, J. I. González; Armstrong, D. J.; Nielsen, L. D.; Lovis, C.; Lavie, B.; Sousa, S. G.; Silva, A. M. (6 February 2024). "TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238". arXiv: 2402.04113 [astro-ph.EP].
  25. 1 2 Psaridi, Angelica; Osborn, Hugh; Bouchy, François; Lendl, Monika; Parc, Léna; Billot, Nicolas; Broeg, Christopher; Sousa, Sérgio G.; Adibekyan, Vardan (30 January 2024). "Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815". arXiv: 2401.15709 [astro-ph.EP].
  26. ↑ Mallorquín, M.; Lodieu, N.; Béjar, V. J. S.; Osorio, M. R. Zapatero; Sanz-Forcada, J.; Alarcon, M. R.; Tabernero, H. M.; Nagel, E.; Collins, K. A. (27 February 2024). "TOI-1135 b: A young hot Saturn-size planet orbiting a solar-type star". arXiv: 2402.17448 [astro-ph.EP].
  27. ↑ Jhon Yana Galarza; Ferreira, Thiago; Lorenzo-Oliveira, Diego; Simon, Joshua D.; Reggiani, Henrique; Piro, Anthony L.; McWilliam, Andrew; Netto, Yuri; Valio, Adriana; Ciardi, David R. (2024). "TOI-1173 A $b$: The First Inflated Super-Neptune in a Wide Binary System". arXiv: 2403.06240v1 [astro-ph.EP].
  28. ↑ Wang, Jia-Qi; Jiang, Xiao-Jun; Zheng, Jie; Kellermann, Hanna; Riffeser, Arno; Wang, Liang; Collins, Karen A.; Bieryla, Allyson; Buchhave, Lars A. (20 October 2023). "Confirmation of a Sub-Saturn-size transiting exoplanet orbiting a G dwarf: TOI-1194 b and a very low mass companion star: TOI-1251 B from TESS". arXiv: 2310.12458 [astro-ph.EP].
  29. 1 2 Bell, J. Serrano; Díaz, R. F.; Hébrard, G.; Martioli, E.; Heidari, N.; Sousa, S.; Boisse, I.; Almenara, J. M.; Alonso-Santiago, J. (12 February 2024). "TOI-1199 b and TOI-1273 b: Two new transiting hot Saturns detected and characterized with SOPHIE and TESS". Astronomy & Astrophysics. 684: A6. arXiv: 2402.07861 . Bibcode:2024A&A...684A...6S. doi:10.1051/0004-6361/202348288.
  30. 1 2 Rubenzahl, Ryan A.; Dai, Fei; Howard, Andrew W.; Lissauer, Jack J.; Van Zandt, Judah; Beard, Corey; Giacalone, Steven; Murphy, Joseph M. Akana; Chontos, Ashley (12 February 2024). "The TESS-Keck Survey. XII. A Dense 1.8 R🜨 Ultra-Short-Period Planet Possibly Clinging to a High-Mean-Molecular-Weight Atmosphere After the First Gyr". arXiv: 2402.07451 [astro-ph.EP].
  31. 1 2 Hill, Michelle L.; Kane, Stephen R.; Dalba, Paul A.; MacDougall, Mason; Fetherolf, Tara; Li, Zhexing; Pidhorodetska, Daria; Batalha, Natalie M.; Crossfield, Ian J. M. (5 February 2024), "The TESS–Keck Survey. XIX. A Warm Transiting Sub-Saturn-mass Planet and a Nontransiting Saturn-mass Planet Orbiting a Solar Analog", The Astronomical Journal, 167 (4): 151, arXiv: 2402.03498 , Bibcode:2024AJ....167..151H, doi: 10.3847/1538-3881/ad2765
  32. ↑ Desai, Anmol; Turtelboom, Emma V.; Harada, Caleb K.; Dressing, Courtney D.; Rice, David R.; Murphy, Joseph M. Akana; Brinkman, Casey L.; Chontos, Ashley; Crossfield, Ian J. M. (11 February 2024). "The TESS-Keck Survey. XVIII. A sub-Neptune and spurious long-period signal in the TOI-1751 system". The Astronomical Journal. 167 (5): 194. arXiv: 2402.07110 . Bibcode:2024AJ....167..194D. doi: 10.3847/1538-3881/ad29ee .
  33. 1 2 3 4 5 6 7 8 9 Schulte, Jack; Rodriguez, Joseph E.; Bieryla, Allyson; Quinn, Samuel N.; Collins, Karen A.; Yee, Samuel W.; Nine, Andrew C.; Soares-Furtado, Melinda; Latham, David W. (11 January 2024), "Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission", arXiv: 2401.05923 [astro-ph.EP]
  34. ↑ Parviainen, Hannu; Murgas, Felipe; Esparza-Borges, Emma; Peláez-Torres, A.; Palle, Enric; Luque, Rafael; Zapatero-Osorio, M. R.; Korth, Judith; Fukui, Akihiko (22 January 2024). "TOI-2266 b: a keystone super-Earth at the edge of the M dwarf radius valley". Astronomy and Astrophysics. 683: A170. arXiv: 2401.11879 . Bibcode:2024A&A...683A.170P. doi:10.1051/0004-6361/202347431.
  35. 1 2 3 Eberhardt, Jan; Hobson, Melissa J.; Henning, Thomas; Trifonov, Trifon; Brahm, Rafael; Espinoza, Nestor; Jordán, Andrés; Thorngren, Daniel; Burn, Remo; Rojas, Felipe I.; Sarkis, Paula; Schlecker, Martin; Pinto, Marcelo Tala; Barkaoui, Khalid; Schwarz, Richard P. (27 February 2024). "Three Warm Jupiters around Solar-analog stars detected with TESS". The Astronomical Journal. 166 (6): 271. arXiv: 2402.17592 . doi: 10.3847/1538-3881/ad06bc . ISSN   0004-6256.
  36. ↑ Timmermans, M.; Dransfield, G.; Gillon, M.; Triaud, A. H. M. J.; Rackham, B. V.; Aganze, C.; Barkaoui, K.; Briceño, C.; Burgasser, A. J. (19 April 2024), TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system , retrieved 22 April 2024
  37. ↑ Martin, Pierre-Yves (2024). "Planet TOI-4438 b". exoplanet.eu. Retrieved 6 March 2024.
  38. ↑ Leichty, McKenna; Garnavich, Peter; Littlefield, Colin; Schwope, Axel D.; Kurpas, Jan; Mason, Paul A.; Beuermann, Klaus (26 February 2024). "An Eccentric Planet Orbiting the Polar V808 Aurigae". arXiv: 2402.16959 [astro-ph.SR].
  39. ↑ Murgas, F.; Pallé, E.; Orell-Miquel, J.; Carleo, I.; Peña-Moñino, L.; Pérez-Torres, M.; Watkins, C. N.; Jeffers, S. V.; Azzaro, M. (22 January 2024). "Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs". Astronomy and Astrophysics. 684: A83. arXiv: 2401.12150 . Bibcode:2024A&A...684A..83M. doi:10.1051/0004-6361/202348813.
  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.