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
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 238 b		0.05049±0.0012	1.74	0.02123^+0.00016 _−0.00017	758⁺¹⁶ ₋₁₅	transit	49.6	0.419±0.01	3485±140	Mars-sized exoplanet, one of the smallest exoplanets currently known^[10]
Gliese 341 b	0.00227±0.00044	0.0821±0.045	7.577		540	transit	33.9	0.506	3745	^[11]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	^[12]Hot Earth-sized exoplanet
HD 77344 b	0.00939^+0.00787 _−0.00599	0.2573^+0.0073 _−0.0064	15.6	0.131	911±7	transit	114.7	1.2±0.02	6220±64	The temperature can be as high as 1,066 K if the planet is tidally locked. Another planet in the system (HD 77344 c) is suspected. It has a minimum mass of 116.3 `M`_E and an orbital period of 66 days^[13]
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	^[14]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	^[15]
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	^[16]
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	^[16]
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^[17]	^[18] 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	^[19]
KMT-2016-BLG-2321Lb	3.58±1.22			3.58±0.81		microlensing	11,670±3980	0.73±0.28		^[20]
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		^[21]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		^[22]
KMT-2023-BLG-0735Lb	0.12±0.07			2.75±1		microlensing	20,830⁺³⁹¹⁰ ₋₃₂₆₀	0.61±0.34		^[22]
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		^[21]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		^[21]
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^[23]
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	^[24]
M62H b	2.83	<0.683 ^{[lower-alpha 3]}^{[lower-alpha 4]}	0.133	0.004908		timing	21,500^[25]	1.4		Pulsar planet located in the globular cluster Messier 62.^[26]
MOA-2016-BLG-526Lb	6.93±0.75			2.07±0.35		microlensing	22,490	0.4		^[20]
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		^[22]
OGLE-2016-BLG-1598Lb	5.91±1.74			2.5±0.88		microlensing	19,270±5670	0.55±0.32		^[20]
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)^[27]
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	^[27]
NGTS-29 b	0.393	0.857	69.33	0.347	414	transit	487±1	1.034±0.032	5730±80	^[28]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	^[29] 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		^[20]
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		^[30]
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		^[30]
OGLE-2017-BLG-1275Lb	5.9±2.2			1.19±0.36		microlensing	25,070±2930	0.63±0.23		^[30]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]}		^[31]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	^[32]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^[33]
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.^[34]
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^[35]^{[lower-alpha 1]}	1.01±0.03	5757⁺⁷² ₋₆₅	^[36]
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	618	1.035^+0.052 _−0.062	5844⁺⁸⁴ ₋₈₂	^[37]^[38]
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	^[38]
TIC 393818343 b	4.34±0.15	1.087^+0.023 _−0.021	16.25	0.129±0.002	805.5^+9.6 _−9.4	transit	306.3±1.1	1.082^+0.055 _−0.056	5756⁺⁵⁷ ₋₆₆	Highly eccentricit orbit (e=0.6058)^[39] Also known as TOI-6883 b^[40]
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	^[41]
TOI-260 b	0.0104	0.1311	13.47	0.09		transit	66			Host star also known as HIP 1532^[42]
TOI-329 b	0.1271		5.71	0.064		transit	927.1	0.98	5560	Radius of the host star is significantly larger compared to mass (1.61 `R`_☉)^[43]
TOI-480 b	0.0654		6.866			transit	177.8	1.2	6,212	^[44]
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	^[45]
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	^[46] 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	^[46] 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	^[47]
TOI-1173 Ab	0.08213±0.00598	0.723±0.015	7.064	0.0702±0.0012	863.9±9.8	transit	430.85^[48]^{[lower-alpha 1]}	0.911^+0.028 _−0.03	5350±340	^[49]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	^[50]
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	^[50]
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	^[51] 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	^[51]
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	^[52]
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	^[52]
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	^[45]
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.^[53]
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 ^[53]
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	^[54]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.^[55]
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	^[56]
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	^[56]
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	^[45]
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	^[57]
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	^[56]
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	^[58]
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	^[58]
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	^[58]
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	^[36]
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	^[56]
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	^[56]
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	^[56]
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	^[56]
TOI-4336 Ab	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	^[59]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	^[60]
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.^[61]
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	^[56]
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	^[56]
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	^[62]
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^[62]
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	^[62]
V808 Aurigae b [ru]	6.8±0.7		4109±362			timing	698±13	0.9±0.1		^[63]The planet's host star is a polar. The mass value for the planet is only a minimum mass.
VHS J183135.58-551355.9	6.5±1.5	1.42^+0.04 _−0.03			1085±60	imaging	180.6±17.9			Free-floating planet^[64]
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	^[65] Ultra-short period planet

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[distp-4] Distance calculated from parallax

[10] The radius is the same as that of the Earth, with an uncertainty of 10%

[Radius1-27] 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

[28] Since the density is only a lower limit, the radius is an upper limit.

[35] 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.

[Albedo1-50] Assuming albedos of 0.3 and 0 respectively.

[A-67] It is not known which of the stars the planet orbits.

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"VizieR".

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[3] [3]
"BD-14 3065". SIMBAD. Centre de données astronomiques de Strasbourg.

[5] [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].

[:11-6] [5]
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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

Notes

References

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