List of exoplanets discovered in 2024

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
2MASS J05581644-4501559 b	6–12			1043		imaging	94.5	0.259±0.02 [1]	3218±158 [1]	[2]
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 [3] [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. [4] 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	[5] Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu. [6] [5]
Gaia20eae b	6			0.062		disc thermal instability	9226+3130 −2021 [7]	1.15	4330±300 [7]	[8]
Gliese 12 b	0.002769+0.00123 −0.0008	0.0892±0.0089 [lower-alpha 2]	12.7	0.066±0.002	315±5	transit	39.65	0.241±0.006	3253±55	[9]
Gliese 341 b	0.00227±0.00044	0.0821±0.045	7.577		540	transit	33.9	0.506	3745	[10] Also known as TOI-741 b
HD 63433 d		0.09573±0.0141	4.21	0.0503±0.0027	1040±40	transit	71.7	0.99±0.03	5688±28	[11] Hot Earth-sized exoplanet
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	[12] 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	[13]
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	[14]
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	[14]
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 [15]	[16] 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		3.986	0.0435±0.0017		radial vel.	122.79+0.12 −0.14	0.69±0.07	4203±116	[17]
KMT-2016-BLG-2321Lb	3.58±1.22			3.58±0.81		microlensing	11,670±3980	0.73±0.28		[18]
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		[19] 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		[20]
KMT-2023-BLG-0735Lb	0.12±0.07			2.75±1		microlensing	20,830+3910 −3260	0.61±0.34		[20]
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		[19] 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		[19]
KMT-2023-BLG-1866Lb	0.00828+0.00132 −0.00214			2.63+0.37 −0.34		microlensing	20,240+2840 −1100	0.51+0.08 −0.13		Super-Earth planet detected by microlensing [21]
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	[22]
M62H b	>2.47 or 2.83	>0.653 or >0.683 [lower-alpha 3] [lower-alpha 4]	0.133	0.004908		timing	21,500 [23]	1.4		Pulsar planet located in the globular cluster Messier 62. [24]
MOA-2016-BLG-526Lb	6.93±0.75			2.07±0.35		microlensing	22,490	0.4		[18]
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		[20]
OGLE-2016-BLG-1598Lb	5.91±1.74			2.5±0.88		microlensing	19,270±5670	0.55±0.32		[18]
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) [25]
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	[25]
NGTS-29 b	0.393	0.857	69.33	0.347	414	transit	487±1	1.034±0.032	5730±80	[26]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	[27] 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		[18]
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		[28]
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		[28]
OGLE-2017-BLG-1275Lb	5.9±2.2			1.19±0.36		microlensing	25,070±2930	0.63±0.23		[28] 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 5]		[29] 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	[30] Located in the open cluster Messier 67
SPECULOOS-3 b		0.08716	0.719	0.00733	553	transit	57.9	0.1	2800	Ultra-short period planet [31]
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. [32]
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	823.4 [33] [lower-alpha 1]	1.01±0.03	5757+72 −65	[34]
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	618	1.035+0.052 −0.062	5844+84 −82	[35] [36]
TIC 139270665 c	4.89+0.66 −0.37		1010+780 −220	2+0.93 −0.31	200+18 −35	radial vel.	618	1.035+0.052 −0.062	5844+84 −82	[36]
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	[37]
TOI-782 b	<0.06	0.244±0.008	8.024	0.0578±0.0018	398±6–435±6 [lower-alpha 6]	transit	170.2±0.2	0.397±0.01	3370+29 −32	[38]
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	[39] 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	[39] 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	[40]
TOI-1173 Ab	0.08213±0.00598	0.723±0.015	7.064	0.0702±0.0012	863.9±9.8	transit	430.85 [41] [lower-alpha 1]	0.911+0.028 −0.03	5350±340	[42] 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	[43]
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	[43]
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	[44] 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	[44]
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	[45]
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	[45]
TOI-1448 b	<0.0613	0.245±0.006	8.112	0.0567±0.0015	389±5–426±6 [lower-alpha 6]	transit	240±0.3	0.372±0.009	3412+28 −32	[38]
TOI-1450 Ab	0.00396±0.0004	0.1±0.004	2.04		722±35	transit	73.2±0.1	0.48±0.24	3437±86	Located in a binary star system. It is the second-lowest mass transiting planet with a high-precision mass measurement. [46]
TOI-1450 Ac	0.0048±0.0006		5.07		533±26	radial vel.	73.2±0.1	0.48±0.24	3437±86	Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab [46]
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	[47] The host star is metal-poor ([Fe/H] = –0.40 dex)
TOI-1824 b	0.0582±0.01	0.2346±0.0133	22.8	0.149±0.003	577±19	transit	192.3	0.85±0.05	5180±110	High-density planet, situated in the small group of "superdense sub-Neptunes". TOI-1824 has also a red dwarf companion star named TIC 142387022. [48]
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	[49]
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	[49]
TOI-2120 b	<0.02139	0.1893±0.0056	5.8	0.0377±0.0013	351±6–384±6 [lower-alpha 6]	transit	104.9	0.211±0.005	3131±30	[38]
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	[50]
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	[49]
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	[51]
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	[51]
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	[51]
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	[34]
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	[49]
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	[49]
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	[49]
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	[49]
TOI-4336A b	0.017+0.013 −0.007	0.1891	16.337	0.0872+0.0013 −0.0014	308±9	transit	73.15	0.331±0.015	3298+75 −73	[52] 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	[53]
TOI-4633 c	0.15+0.087 −0.075	0.285+0.018 −0.017	271.94	0.847±0.061	290	transit	310.4±0.78	1.05±0.06 or 1.1±0.06 [lower-alpha 7]	5600±50 or 5800±50 [lower-alpha 7]	Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron. [54]
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	[49]
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	[49]
TOI-5720 b	0.0041+0.0029 −0.0015	0.0972±0.0062	1.434	0.0183±0.0003	708±19	transit	116.9±0.1	0.383±0.019	3325±75	[55]
TOI-6008 b	0.00346+0.0023 −0.0011	0.0919±0.0045	0.858	0.0108±0.0002	707±19	transit	75.05±0.03	0.23±0.011	3075±75	Ultra-short period planet [55]
TOI-6086 b	0.00346+0.00362 −0.00176	0.1053±0.0062	1.389	0.0154±0.0002	634±16	transit	102.6	0.254±0.013	3200±75	[55]
V808 Aurigae b  [ ru ]	6.8±0.7		4109±362			timing	698±13	0.9±0.1		[56] 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±1	1.42+0.04 −0.03			1085±60	imaging	180.6±17.9			Free-floating planet [57]
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	[58] Ultra-short period planet

Specific exoplanet lists

Lists of exoplanets

• List of directly imaged exoplanets
• List of exoplanet extremes
• List of exoplanet firsts
• List of exoplanets discovered by the Kepler space telescope
• List of exoplanets observed during Kepler's K2 mission
• List of extrasolar candidates for liquid water
• List of hottest exoplanets
• List of coolest exoplanets
• List of multiplanetary systems
• List of nearest exoplanets
• List of nearest terrestrial exoplanet candidates
• List of potentially habitable exoplanets
• List of proper names of exoplanets
• List of smallest exoplanets
• List of transiting exoplanets

Lists of exoplanets by year of discovery

• List of exoplanets discovered before 2000 (31)
• List of exoplanets discovered between 2000–2009 (378)
• List of exoplanets discovered in 2010 (109)
• List of exoplanets discovered in 2011 (178)
• List of exoplanets discovered in 2012 (149)
• List of exoplanets discovered in 2013 (151)
• List of exoplanets discovered in 2014 (870)
• List of exoplanets discovered in 2015 (150)
• List of exoplanets discovered in 2016 (1513)
• List of exoplanets discovered in 2017 (158)
• List of exoplanets discovered in 2018 (306)
• List of exoplanets discovered in 2019 (172)
• List of exoplanets discovered in 2020 (253)
• List of exoplanets discovered in 2021 (257)
• List of exoplanets discovered in 2022 (313)
• List of exoplanets discovered in 2023 (297)
• List of exoplanets discovered in 2024 (81)

Notes

1. Distance calculated from parallax
2. The radius is the same as that of the Earth, with an uncertainty of 10%
3. Radius calculated with mass and lower limit in density in the equation d=(1.89813*10^(30)*m)/((4/3)*π*r³), where d is density (in g/cm³), m is the mass (in M_J and r is the radius (in centimeters). Should be divided by 7.1492×10⁹ to convert from centimeters to R_J
4. First value use the minimum mass (2.47 M_J), while the second values use the median mass (2.83 M_J). Since the density (11 g/cm³) is only a lower limit, the radius is also a lower limit.
5. 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.
6. Assuming albedos of 0.3 and 0 respectively.
7. It is not known which of the stars the planet orbits.

References

1. "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
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. "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. Cruz-Sáenz de Miera, Fernando; Kóspál, Ágnes; Ábrahám, Péter; Park, Sunkyung; Nagy, Zsófia; Siwak, Michał; Kun, Mária; Fiorellino, Eleonora; Szabó, Zsófia Marianna; Antoniucci, Simone; Giannini, Teresa; Nisini, Brunella; Szabados, László; Kriskovics, Levente; Ordasi, András (1 March 2022). "Recurrent Strong Outbursts of an EXor-like Young Eruptive Star Gaia20eae". The Astrophysical Journal. 927 (1): 125. arXiv: 2112.04140 . Bibcode:2022ApJ...927..125C. doi: 10.3847/1538-4357/ac477f . ISSN   0004-637X.
8. Nayakshin, Sergei; de Miera, Fernando Cruz Sáenz; Kóspál, Ágnes (27 April 2024). "The youngest of hot jupiters in action: episodic accretion outbursts in Gaia20eae". Monthly Notices of the Royal Astronomical Society: Letters. 532: L27–L32. arXiv: 2405.09904 . doi:10.1093/mnrasl/slae034. ISSN   1745-3925.
9. Dholakia, Shishir; Palethorpe, Larissa; Venner, Alexander; Mortier, Annelies; Wilson, Thomas G.; Huang, Chelsea X.; Rice, Ken; Van Eylen, Vincent; Nabbie, Emma (21 May 2024), Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPS, arXiv: 2405.13118
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