List_of_exoplanets_discovered_in_2024

List of exoplanets discovered in 2024

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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.

More information Name, Mass (MJ) ...

Name	Mass (`M`_J)	Radius (`R`_J)	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]^{[lower-alpha 1]}	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
HIP 39017 b	23.6^+9.1 _−7.4	0.87	30681^+18627.8 _−9496.5	22.1^+8.0 _−4.9		imaging	214.9±0.3	1.52^+0.28 _−0.26	7201⁺¹⁴² ₋₁₁₂^[10]	^[11] May be a brown dwarf. Estimated of the mass vary from 13.8 M_J to 30+31 −12 M_J.
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	^[12]
KMT-2016-BLG-2321Lb	3.58±1.22			3.58±0.81		microlensing	11,670±3980	0.73±0.28		^[13]
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		^[14]The mass of the planet can be as low as 0.042+0.021 −0.022 M_J
KMT-2023-BLG-0469Lb	0.124^+0.092 _−0.067			2.37±0.9		microlensing	23,050⁺³²⁶⁰ ₋₃₉₁₀	0.47±0.36		^[15]
KMT-2023-BLG-0735Lb	0.12±0.07			2.75±1		microlensing	20,830⁺³⁹¹⁰ ₋₃₂₆₀	0.61±0.34		^[15]
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		^[14]Estimates of the planet's mass varies between 0.3+0.34 −0.16 M_J and 0.77+0.87 −0.42 M_J
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		^[14]
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	^[16]
M62H b	2.83		0.133	0.004908		timing	21,500^[17]	1.4		Pulsar planet located in the globular cluster Messier 62.^[18]
MOA-2016-BLG-526Lb	6.93±0.75			2.07±0.35		microlensing				^[13]
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		^[15]
OGLE-2016-BLG-1598Lb	5.91±1.74			2.5±0.88		microlensing	19,270±5670	0.55±0.32		^[13]
NGTS-26 b	0.29^+0.07 _−0.06	1.33^+0.06 _−0.05	4.52	0.0490^+0.0038 _−0.0032	1331⁺⁸⁵ ₋₇₂	transit	3610±100	0.96^+0.04 _−0.03	5550±100	Highly inflated planet (density = 0.153 g/cm³)^[19]
NGTS-27 b	0.593^+0.095 _−0.072	1.396^+0.038 _−0.035	3.37	0.0446^+0.0026 _−0.0036	1783⁺¹⁰⁴ ₋₈₈	transit	3185±55	1.07±0.06	5700±80	^[19]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	^[20] 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		^[13]
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		^[21]
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		^[21]
OGLE-2017-BLG-1275Lb	5.9±2.2			1.19±0.36		microlensing	25,070±2930	0.63±0.23		^[21]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	^{[lower-alpha 2]}		^[22]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	^[23]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.^[24]
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	^[25]
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	486	1.035	5844	^[26]
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	^[27]
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	^[28] 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	^[28] 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	^[29]
TOI-1173 Ab	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	^[30]Low-density planet located in a wide binary system
TOI-1199 b	0.239±0.02	0.938±0.025	3.671	0.04988±0.0009	1486±20	transit	805±2.6	1.23±0.07	5710±40	^[31]
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	^[31]
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	^[32] 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	^[32]
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	^[33]
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	^[33]
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	^[34]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	^[35]
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	^[35]
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	^[36]
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	^[35]
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	^[37]
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	^[37]
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	^[37]
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	^[25]
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	^[35]
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	^[35]
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	^[35]
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	^[35]
TOI-4436 b		0.1891	16.337	0.0872^+0.0013 _−0.0014	308±9	transit	73.15	0.331±0.015	3298⁺⁷⁵ ₋₇₃	^[38]Located in a triple hierarchical stellar system
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	^[39]
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	^[35]
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	^[35]
V808 Aurigae b [ru]	6.8±0.7		4109±362			timing	698±13	0.9±0.1		^[40]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	^[41] Ultra-short period planet

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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].
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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.
[25]
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.
[26]
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.
[27]
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].
[28]
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].
[29]
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].
[30]
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].
[31]
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.
[32]
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].
[33]
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
[34]
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.
[35]
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]
[36]
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.
[37]
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.
[38]
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
[39]
Martin, Pierre-Yves (2024). "Planet TOI-4438 b". exoplanet.eu. Retrieved 6 March 2024.
[40]
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].
[41]
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.

Derived from a parallax of 1.7646 mas
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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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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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

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Martin, Pierre-Yves (2024). "Planet TOI-4438 b". exoplanet.eu. Retrieved 6 March 2024.

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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].

[43] [41]
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.

[2] Derived from a parallax of 1.7646 mas

[23] 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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List_of_exoplanets_discovered_in_2024

List of exoplanets discovered in 2024

Specific exoplanet lists

Lists of exoplanets by year of discovery

References

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