List of exoplanets discovered in 2024

Last updated

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
2MASS J05581644-4501559 b6–121043imaging94.50.259±0.02 [1] 3218±158 [1] [2]
BD-14 3065 b12.11+0.95
0.91
1.926±0.0944.30.0646±0.00261957±28transit1847.4 [3] [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. [4] 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 [5] Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu. [6] [5]
Gliese 341 b0.00227±0.000440.0821±0.0457.577540transit33.90.5063745 [7] Also known as TOI-741 b
HD 63433 d 0.09573±0.01414.210.0503±0.00271040±40transit71.70.99±0.035688±28 [8] Hot Earth-sized exoplanet
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 [9] 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 [10]
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
[11]
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
[11]
HIP 39017 b 23.6+9.1
7.4
0.8730681+18627.8
9496.5
22.1+8.0
4.9
imaging214.9±0.31.52+0.28
0.26
7201+142
112
[12]
[13] May be a brown dwarf. Estimated of the mass vary from 13.8 MJ to 30+31
−12
 MJ
.
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 [14]
KMT-2016-BLG-2321Lb3.58±1.223.58±0.81microlensing11,670±39800.73±0.28 [15]
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
[16] 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 [17]
KMT-2023-BLG-0735Lb0.12±0.072.75±1microlensing20,830+3910
3260
0.61±0.34 [17]
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
[16] 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
[16]
LHS 1678 d 0.00289+0.00208
0.00107
0.08752±0.00624.9650.04+0.0018
0.0017
transit650.345±0.0143490±50 [18]
M62H b 2.830.1330.004908timing21,500 [19] 1.4 Pulsar planet located in the globular cluster Messier 62. [20]
MOA-2016-BLG-526Lb6.93±0.752.07±0.35microlensing22,4900.4 [15]
MOA-2022-BLG-563Lb0.4+0.31
0.25
2.25±0.25microlensing21,290+3650
5220
0.48+0.36
0.3
[17]
OGLE-2016-BLG-1598Lb5.91±1.742.5±0.88microlensing19,270±56700.55±0.32 [15]
NGTS-26 b0.29+0.07
0.06
1.33+0.06
0.05
4.520.0490+0.0038
0.0032
1331+85
72
transit3610±1000.96+0.04
0.03
5550±100Highly inflated planet (density = 0.153 g/cm3) [21]
NGTS-27 b0.593+0.095
0.072
1.396+0.038
0.035
3.370.0446+0.0026
0.0036
1783+104
88
transit3185±551.07±0.065700±80 [21]
NGTS-30 b 0.960.9398.30.408390transit762.50.945455 [22] Also known as TOI-4862 b
OGLE-2016-BLG-1800Lb2.59±1.461.88±0.51microlensing21,100±33600.41±0.22 [15]
OGLE-2017-BLG-0640Lb1.62+1.64
0.94
1.14±0.38microlensing21,600+3550
4730
0.32+0.32
0.18
[23]
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
[23]
OGLE-2017-BLG-1275Lb5.9±2.21.19±0.36microlensing25,070±29300.63±0.23 [23] 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] [24] 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 [25] 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. [26]
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
[27]
TIC 139270665 b0.4630.64523.6240.163700transit6181.035+0.052
0.062
5844+84
82
[28] [29]
TIC 139270665 c4.89+0.66
0.37
1010+780
220
2+0.93
0.31
200+18
35
radial vel.6181.035+0.052
0.062
5844+84
82
[29]
TOI-238 c0.0211±0.00350.1945±0.01618.4660.0749±0.0013696±15transit261.328±0.3120.79±0.0225059±89 [30]
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 [31] 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 [31] 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 [32]
TOI-1173 Ab0.08213±0.005980.723±0.0157.0640.0702±0.0012863.9±9.8transit0.911+0.028
0.03
5350±340 [33] Low-density planet located in a wide binary system
TOI-1199 b0.239±0.020.938±0.0253.6710.04988±0.00091486±20transit805±2.61.23±0.075710±40 [34]
TOI-1273 b0.222±0.0150.99±0.24.6310.0549±0.0011211±15transit574±1.31.06±0.065690±40 [34]
TOI-1347 b 0.0349±0.00380.161±0.0090.8471400±40transit480.8±20.913±0.0335464±100 [35] Ultra-short period planet
TOI-1347 c 0.0088±0.00720.143±0.0094.8421000±25transit480.8±20.913±0.0335464±100 [35]
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
[36]
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
[36]
TOI-1751 b0.0538±0.01010.2489±0.025937.4680.2115±0.0024820transit370.3±0.31.15±0.176116±22 [37] 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
[38]
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
[38]
TOI-2266 b0.1374±0.0082.3260.02±0.002550±47transit168.6±0.20.23±0.023240±160 [39]
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
[38]
TOI-2373 b9.3±0.20.93±0.0213.3370.112±0.001860±10transit1617±331.041+0.032
0.028
5651±180 [40]
TOI-2416 b3+0.1
0.09
0.88±0.028.2750.0831±0.00071080±10transit1767±2611.118+0.029
0.027
5808±80 [40]
TOI-2524 b0.64±0.041+0.02
0.03
7.1860.073±0.00071100±20transit1399±361.007+0.032
0.029
5831±80 [40]
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
[27]
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 [38]
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 [38]
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 [38]
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
[38]
TOI-4436 b0.189116.3370.0872+0.0013
0.0014
308±9transit73.150.331±0.0153298+75
73
[41] 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 [42]
TOI-4633 c 0.15+0.087
0.075
0.285+0.018
0.017
271.940.847±0.061290transit310.4±0.781.05±0.06 or 1.1±0.06 [lower-alpha 3] 5600±50 or 5800±50 [lower-alpha 3] Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron. [43]
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
[38]
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 [38]
V808 Aurigae b  [ ru ]6.8±0.74109±362timing698±130.9±0.1 [44] The planet's host star is a polar. The mass value for the planet is only a minimum mass.
VHS J183135.58-551355.9 7±11.42+0.04
0.03
1085±60imaging180.6±17.9Free-floating planet [45]
Wolf 327 b0.00796±0.001450.1106±0.00540.5730.01996±22transit92.90.405±0.0193542±70 [46] Ultra-short period planet

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

Related Research Articles

OGLE-2005-BLG-071L is a distant, magnitude 19.5 galactic bulge star located in the constellation Scorpius, approximately 11,000 light years away from the Solar System. The star is probably a red dwarf with a mass 43% of that of the Sun.

<span class="mw-page-title-main">Planet Hunters</span> Citizen science project to find exoplanets

Planet Hunters is a citizen science project to find exoplanets using human eyes. It does this by having users analyze data from the NASA Kepler space telescope and the NASA Transiting Exoplanet Survey Satellite. It was launched by a team led by Debra Fischer at Yale University, as part of the Zooniverse project.

TOI-700 is a red dwarf 101.4 light-years away from Earth located in the Dorado constellation that hosts TOI-700 d, the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).

<span class="mw-page-title-main">TOI-700 d</span> Goldilocks terrestrial planet orbiting TOI-700

TOI-700 d is a near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the red dwarf TOI-700, the outermost planet within the system. It is located roughly 101.4 light-years (31.1 pc) away from Earth in the constellation of Dorado. The exoplanet is the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite (TESS).

LTT 3780, also known as TOI-732 or LP 729-54, is the brighter component of a wide visual binary star system in the constellation Hydra. This star is host to a pair of orbiting exoplanets. Based on parallax measurements, it is located at a distance of 72 light years from the Sun. LTT 3780 has an apparent visual magnitude of 13.07, requiring a telescope to view.

L 98-59 is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.608 parsecs, as measured by Gaia.

TESS Hunt for Young and Maturing Exoplanets (THYME) is an exoplanet search project. The researchers of the THYME collaboration are mainly from the United States and search for young exoplanets using data from the Transiting Exoplanet Survey Satellite (TESS). The new discoveries should help to understand the early evolution of exoplanets. As of March 2023 the collaboration produced 9 papers announcing the discovery of exoplanets.

The TESS-Keck Survey or TKS is an exoplanet search project that uses the Keck I and the Automated Planet Finder (APF) to conduct ground-based follow-up of planet candidates discovered by the Transiting Exoplanet Survey Satellite. The TKS aims to measure the mass for about 100 exoplanets and has been awarded some of the largest time allocations in the histories of Keck I and APF. The program has four main science themes:

  1. the bulk compositions of small planets
  2. dynamical temperatures and system architectures
  3. a larger, more refined sample for future atmospheric studies
  4. planets orbiting evolved stars
<span class="mw-page-title-main">TOI-2180 b</span> Jovian-sized exoplanet orbiting TOI-2180

TOI-2180 b is a giant exoplanet orbiting the G-type star TOI-2180, also known as HD 238894. It was discovered with the help of the Transiting Exoplanet Survey Satellite and is currently the exoplanet with the longest orbital period TESS was able to uncover. TOI-2180 b orbits its host star every 260.16 days.

HD 63433 c is a mini-Neptune exoplanet orbiting the Sun-like star HD 63433. It is the outermost planet in its planetary system, being located 0.1448 astronomical units (21,660,000 km) from its star, and completing one orbit every 21 days. Despite being the outermost planet in the system, it is still located close to its star, meaning that its temperature is hot, being estimated between 267 and 406 °C. HD 63433 c is about 2.7 times larger than Earth and 15.5 times more massive, but still smaller and less massive than Neptune. In 2022, a study showed that its atmosphere, made up of hydrogen, is being evaporated by the strong radiation from its star, causing it to slowly turn into a super-Earth planet.

References

  1. 1 2 "VizieR".
  2. Marocco, Federico; Kirkpatrick, J. Davy; Schneider, Adam C.; Meisner, Aaron M.; Popinchalk, Mark; Gelino, Christopher R.; Faherty, Jacqueline K.; Burgasser, Adam J.; Caselden, Dan (22 April 2024), Thirteen New M Dwarf + T Dwarf Pairs Identified with WISE/NEOWISE, arXiv: 2404.14324 , retrieved 3 May 2024
  3. "BD-14 3065". SIMBAD . Centre de données astronomiques de Strasbourg.
  4. 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].
  5. 1 2 "CI Tau | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 29 March 2024.
  6. Martin, Pierre-Yves (2024). "Planet Cl Tau c". exoplanet.eu. Retrieved 29 March 2024.
  7. 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
  8. 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
  9. 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.
  10. 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". The Astronomical Journal. 167 (5): 239. arXiv: 2403.17062 . Bibcode:2024AJ....167..239K. doi: 10.3847/1538-3881/ad3820 .
  11. 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
  12. "HIP 39017 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 26 April 2024.
  13. Tobin, Taylor L.; Currie, Thayne; Li, Yiting; Chilcote, Jeffrey; Brandt, Timothy D.; Lacy, Brianna; Kuzuhara, Masayuki; Vincent, Maria; El Morsy, Mona; Deo, Vincent; Williams, Jonathan P.; Guyon, Olivier; Lozi, Julien; Vievard, Sebastien; Skaf, Nour; Ahn, Kyohoon; Groff, Tyler; Kasdin, N. Jeremy; Uyama, Taichi; Tamura, Motohide; Gibbs, Aidan; Lewis, Briley L.; Bowens-Rubin, Rachel; Salama, Maïssa; An, Qier; Chen, Minghan (9 April 2024). "Direct-imaging Discovery of a Substellar Companion Orbiting the Accelerating Variable Star HIP 39017". The Astronomical Journal. 167 (5): 205. arXiv: 2403.04000 . Bibcode:2024AJ....167..205T. doi: 10.3847/1538-3881/ad3077 .
  14. 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 .
  15. 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]
  16. 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.
  17. 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].
  18. 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].
  19. 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.
  20. 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.530.1436V. doi:10.1093/mnras/stae816. ISSN   0035-8711.
  21. 1 2 https://www.aanda.org/articles/aa/pdf/forth/aa47162-23.pdf
  22. 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
  23. 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.
  24. 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].
  25. 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].
  26. 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.
  27. 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.
  28. 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.
  29. 1 2 "TIC 139270665 Overview". NASA Exoplanet Archive . Retrieved 10 May 2024.
  30. 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].
  31. 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].
  32. 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].
  33. 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].
  34. 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.
  35. 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].
  36. 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
  37. 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 .
  38. 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]
  39. 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.
  40. 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.
  41. 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, arXiv: 2404.12722
  42. Martin, Pierre-Yves (2024). "Planet TOI-4438 b". exoplanet.eu. Retrieved 6 March 2024.
  43. Eisner, Nora L.; Grunblatt, Samuel K.; Barragán, Oscar; Faridani, Thea H.; Lintott, Chris; Aigrain, Suzanne; Johnston, Cole; Mason, Ian R.; Stassun, Keivan G.; Bedell, Megan; Boyle, Andrew W.; Ciardi, David R.; Clark, Catherine A.; Hebrard, Guillaume; Hogg, David W. (1 May 2024). "Planet Hunters TESS V: a planetary system around a binary star, including a mini-Neptune in the habitable zone". The Astronomical Journal. 167 (5): 241. arXiv: 2404.18997 . doi: 10.3847/1538-3881/ad1d5c . ISSN   0004-6256.
  44. 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].
  45. Bickle, Thomas P.; Schneider, Adam C.; Gagné, Jonathan; Faherty, Jacqueline K.; Rothermich, Austin; Vos, Johanna M.; Suárez, Genaro; Kirkpatrick, J. Davy; Meisner, Aaron M. (6 May 2024), Discovery of the Remarkably Red L/T Transition Object VHS J183135.58-551355.9, doi:10.48550/arXiv.2405.03849 , retrieved 9 May 2024
  46. 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.
  3. 1 2 It is not known which of the stars the planet orbits.