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List of exoplanets discovered in 2024

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This is adynamic list and may never be able to satisfy particular standards for completeness. You can help byediting the page to add missing items, with references toreliable sources.

Thislist of exoplanets discovered in 2024 is a list of confirmedexoplanets that were first reported in 2024. For exoplanets detected only byradial velocity, the listed value for mass is a lower limit. SeeMinimum mass for more information.

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
20 Leonis Minoris b	0.02882^+0.00173 _−0.00176		31.15	0.1916±0.0007		radial vel.	48.64±0.07	0.967±0.01	5610±46	^[1]
82 G. Eridani d	0.01831±0.00179		647.6^+2.5 _−2.7	1.354±0.007		radial vel.	19.7	0.813^+0.018 _−0.012	5490±70	Orbiting within the habitable zone of its host star.^[2]^[3]
2MASS J05581644–4501559 b	6–12			1043		imaging	94.5	0.259±0.02^[4]	3218±158^[4]	^[5]
Barnard's Star b	0.00116±0.00016		3.153	0.0229	~400	radial vel.	5.9629±0.0004	0.162±0.007	3195±28	The closest exoplanet around a solitary star. Also located in the second closest star system to the Sun, afterAlpha Centauri.^[6] Not to be confused with the disproved planetBarnard's Star b of 2018, which shared the same name.
BD+00 444b	0.0151±0.0035	0.2108±0.0059	15.669	0.105±0.025	519±6	transit	77.99±0.036	0.642±0.026	4375±65	^[7]
BD-10 47 b	0.0133±0.005	0.1529±0.0007	13.476	0.0943±0.0016	493±12	transit	65.89	0.616±0.032	4026±14	Also known as TOI-260 b^[8]
BD-14 3065 b	12.11^+0.95 _−0.91	1.926±0.094	4.3	0.0646±0.0026	3520±130	transit	1847.4^[9]^[a]	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. Also known as TOI-4987 b^[10]
BX Trianguli b	7.5		3923	4.5		timing	192±7	0.858 (combined)	3735 + 3359	^[11]^[12]
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	Highly eccentric orbit(e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu.^[13]^[14]
CWISE J054129.32–745021.5 b	1.8			6576		imaging	111			Orbits a young red dwarf.^[5]
Gaia-4 b	11.8^+0.73 _−0.66		571.3^+1.4 _−1.3			astrometry + radial vel.	239.2±0.4	0.644^+0.025 _−0.023	4034±77	^[15]
Gaia20eae b	6			0.062		episodic accretion outbursts	9226⁺³¹³⁰ ₋₂₀₂₁^[16]	1.15	4330±300^[16]	^[17]
Gaia22dkvLb	0.15 to 5.67^+0.39 _−0.38		219⁺⁴⁷ ₋₂₉ to964+99 −106	0.48^+0.01 _−0.07 to 2.08^+0.16 _−0.18		microlensing	3097±130 to 5477⁺³²⁶ ₋₃₉₁	0.219^+0.056 _−0.039 to 1.3^+0.04 _−0.05		^[18]
Gliese 12 b	0.002769^+0.00123 _−0.0008	0.0892±0.0089^[b]	12.7	0.066±0.002	315±5	transit	39.65	0.241±0.006	3253±55	^[19]
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^[20]
Gliese 341 b	0.00227±0.00044	0.0821±0.045	7.577		540	transit	33.9	0.506	3745	Also known as TOI-741 b^[21]
Gliese 900 b	10.5		460,000,000^[22]	12,000		imaging	68^[23]	1.08 (combined)	3976^[24]	Located in a three-star system.^[25] It has the longest orbital time of any exoplanet so far at 1.26 million years.^[22]
Gliese 1289 b	0.01655^+0.002958 _−0.003052		111.74	0.27±0.01	150	radial vel.	28.88	0.21±0.02	3296±30	^[26]
Gliese 4256 b	0.00453±0.00044	0.0962±0.0058	0.238	0.0054^[27]	1340±60	transit	66.46±0.03	0.353±0.015	3421±70	An ultra-short period planet orbiting close to the host star'sRoche limit. It is expected to undergotidal disruption in the next hundred million years. Also known as TOI-6255 b^[28]
HD 21520 b	0.02486^+0.01007 _−0.00944	0.2409±0.008	25.13	0.1726±0.0071	637⁺¹³ ₋₁₂	transit	258	1.09±0.07	5871±62	^[29]
HD 28185 c	5.68^+0.44 _−0.36		9224⁺³³² ₋₂₂₃	8.54^+0.21 _−0.14		astrometry + radial vel.	127.8±0.1	0.974±0.018	5602±36	Already known to exist in 2022, but was found to be an exoplanet—as opposed to a brown dwarf, in 2024.^[30]^[31]
HD 48948 b	0.0154±0.000661		7.34013±0.00040	0.0652±0.0005	715±10	radial vel.	54.915±0.0228	0.686^+0.020 _−0.013	4593±60	^[32]
HD 48948 c	0.0229±0.00220		37.920^+0.026 _−0.024	0.1951±0.0016	413±6	radial vel.				^[32]
HD 48948 d	0.0333±0.00315		150.95^+0.45 _−0.41	0.4894±0.0042	262±4	radial vel.				ClosestSuper Earth inhabitable zone around a K-dwarf star.^[32]
HD 57625 b	8.43^+1.10 _−0.91		4843⁺³⁰⁶ ₋₁₆₇	5.70^+0.14 _−0.13		radial vel. + astrometry	144.3	1.040^+0.078 _−0.080	5962±43	True mass revealed usingastrometry.^[33]
HD 63433 d		0.09573±0.0141	4.21	0.0503±0.0027	1040±40	transit	71.7	0.99±0.03	5688±28	Hot Earth-sized exoplanet^[34]
HD 73344 b	0.00939^+0.00787 _−0.00599	0.2573^+0.0073 _−0.0064	15.6	0.131	911±7	transit	114.7^+0.1 _−0.0^[35]	1.20±0.02^[35]	6028±110^[35]	The dayside temperature can be as high as 1,066 K if the planet is tidally locked.^[36]
HD 73344 c	0.367^+0.022 _−0.021		65.936	0.3388^+0.0042 _−0.0043	562±4^[36]	radial vel.				^[35]
HD 73344 d	2.55^+0.56 _−0.46		5746⁺¹²⁰ ₋₁₅₀	6.70^+0.25 _−0.26		radial vel.				True mass revealed usingastrometry.^[35]
HD 75898 c	8.49^+0.65 _−0.63		6717±40	7.39±0.05		astrometry + radial vel.	263	1.295±0.015	6122±52	^[37]^[38]
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	Also known as TOI-1778 b^[39]
HD 101581 b		0.0877	4.47			transit	41.7	0.740±0.087	4675±53	Host star is the brightest star with multiple known transiting Earth-size exoplanets. Another transiting planet in the system is suspected.^[40]
HD 101581 c		0.0925	6.21			transit	41.7	0.740±0.087	4675±53	Host star is the brightest star with multiple known transiting Earth-size exoplanets. Another transiting planet in the system is suspected.^[40]
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	^[41]
HD 111520 b	≥1		1,285,900	≥200		disk kinematics	352.6±0.7	1.350±0.215^[42]	6542±131^[42]	^[43]
HD 115587 b	0.7	0.49	372			transit	356.2±0.5	1.248±0.190	6324±129	^[44]^[45]
HD 118203 c	11.1^+1.3 ₋₁		5070	6.2±0.2	146±3	astrometry + radial vel.	300±0.5	1.353±0.006	5872±20	^[46]
HD 128717 b	12.8		1089.2	2.18		astrometry	240±0.5	1.17^+0.06 _−0.16	6158±115	^[47]^[48]
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	^[49]
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	^[49]
HD 148193 Ab	0.0894±0.0135	0.7476±0.017	20.38	0.1577		transit	626±3	1.261±0.183	6351±119	The host star is orbited by two red dwarfs 157 and 1950 AU away.^[50] Also known as TOI-1836 Ab
HD 148193 Ac	0.025	0.232^+0.01972 _−0.01285	1.773	0.03089±0.0005	2007.6^+35.85 ₋₂₉	transit	626±3	1.261±0.183	6351±119	Also known as TOI-1836 Ac^[51]
HD 156141 b	0.0305±0.0060	0.211±0.005	21.269	0.154±0.003	694.1^+11.2 _−11.0	transit	237.726^+0.390 _−0.389	1.09^+0.034 _−0.033	5814±137	Also known as TOI-1742 b.^[52]
HD 222237 b	5.19±0.58		14,890⁺²¹²⁰ ₋₁₆₄₃	10.8^+1.1 _−1.0		astrometry + radial vel.	37.31±0.0	0.76±0.09	4751±139	^[53]
HD 278878 b	0.6963±0.0242	0.9225±0.0571	8.71	0.08258		transit	520.8±4.9	0.989±0.126	5597±147	^[54]
HIP 11696 b	4 to 16			2.5 to 28		astrometry	160.8	1.40±0.07	6298^[55]	^[56]
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^[57]	May be a brown dwarf. Estimates of the mass vary from13.8 M_J to30+31 −12 M_J.^[58]
HIP 47110 b	3 to 10			3 to 30		astrometry	126.2	0.98±0.05	4529^[55]	^[56]
HIP 67522 c		0.731^+0.055 _−0.057	14.335	0.1235	915⁺²² ₋₁₉	transit	414^[59]	1.2±0.05^[59]	5675±75^[59]	^[60]
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	^[61]
IRAS 04125+2902 b	0.3	0.955	8.83			transit	520^[62]	0.7	3720^[63]	^[64] The youngest transiting exoplanet discovered to date.^[65]
Kepler-51e	0.01572		260			timing	2610±50	1.04	6018	Assuming the 2:1resonance solution, which is the best-fit one, Kepler-51e has a mass of about 5`M`_🜨 and a period of 260 days.^[66]
Kepler-158d		0.038±0.004	0.645088±0.000002			transit	1028±7	0.656^+0.073 _−0.049	4895.97	^[67]
Kepler-879c		0.04±0.01	0.646716±0.000003			transit	2618⁺³⁶ ₋₃₅	0.974^+0.127 _−0.104	5456.75	^[67]
Kepler-963c		0.05±0.02	0.919783±0.000003			transit	2516⁺⁴² ₋₄₀	0.821^+0.120 _−0.065	5169.47	^[67]
Kepler-1489c		0.045±0.007	0.680741±0.000004			transit	4185⁺¹¹⁸ ₋₁₁₁	0.977^+0.050 _−0.062	5565.53	^[67]
Kepler-2003b		0.06±0.01	0.941967±0.000003			transit	3054⁺⁸⁵ ₋₈₁	0.859^+0.126 _−0.065	5050.28	Also known as KOI-4978 b.^[67]
K2-360 c	0.0479±0.0024		9.797±0.030	0.0883±0.0016	912±18	radial vel.	762.59±19.05	0.958±0.048	5679⁺⁶⁰ ₋₃₉	^[68]
K2-419 Ab	0.617±0.047	0.941±0.034	20.358	0.1208^+0.0016 _−0.0017	377±11	transit	860±8	0.562±0.024	3711±88	^[69]
KMT-2016-BLG-2321Lb	3.58±1.22			3.58±0.81		microlensing	11,670±3980	0.73±0.28		^[70]
KMT-2017-BLG-0849Lb	0.0201^+0.0245 _−0.0097			2.73^+0.68 _−0.62		microlensing	23,540⁺²⁶⁷⁰ ₋₃₂₂₀	0.19^+0.23 _−0.09		^[71]
KMT-2017-BLG-1057Lb	0.0739^+0.0472 _−0.0378			2.36^+0.69 _−0.62		microlensing	21,190⁺²⁶⁴⁰ ₋₅₂₈₀	0.57^+0.37 _−0.29		^[71]
KMT-2017-BLG-2331Lb	0.538^+0.431 _−0.277			2.14^+0.48 _−0.42		microlensing	26,180⁺²⁷⁴⁰ ₋₃₄₂₀	0.4^+0.32 _−0.21		^[71]
KMT-2020-BLG-0157Lb	10.71^+6.17 _−5.61			11.54^+1.61 _−2.25		microlensing	21,744⁺³⁰³² ₋₄₂₃₈	0.58^+0.33 _−0.30		^[72]
KMT-2021-BLG-2609Lb	0.032^+0.044 _−0.018 or 0.112^+0.152 _−0.061			2.30^+0.32 _−0.36		microlensing	24,380⁺³⁴²⁰ ₋₃₈₁₀	0.20^+0.27 _−0.11		^[73]
KMT-2022-BLG-0303Lb	0.513^+0.410 _−0.275			4.81^+0.65 _−0.76		microlensing	21,400⁺²⁹⁰⁰ ₋₃₄₀₀	0.368^+0.294 _−0.197		^[73]
KMT-2022-BLG-0732Lb	1.12±0.65			4.11^+0.74 _−1.14		microlensing	21,712⁺³⁸⁷⁹ ₋₆₀₀₀	0.54±0.31		^[72]
KMT-2022-BLG-1787Lb	6.64^+4.98 _−3.64			6.3^+0.75 _−1.08		microlensing	24,613⁺²⁹⁰¹ ₋₄₀₃₈	0.42^+0.32 _−0.23		^[72]
KMT-2022-BLG-1852Lb	4.98^+5.42 _−2.94			5.03^+0.72 _−0.92		microlensing	20,440⁺²⁹³⁴ ₋₃₇₄₉	0.32^+0.34 _−0.19		^[72]
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		The mass of the planet can be as low as0.042+0.021 −0.022 M_J.^[74]
KMT-2023-BLG-0469Lb	0.124^+0.092 _−0.067			2.37±0.9		microlensing	23,050⁺³²⁶⁰ ₋₃₉₁₀	0.47±0.36		^[75]
KMT-2023-BLG-0735Lb	0.12±0.07			2.75±1		microlensing	20,830⁺³⁹¹⁰ ₋₃₂₆₀	0.61±0.34		^[75]
KMT-2023-BLG-1431Lb	0.0428^+0.0261 _−0.0217			2.3±0.5 or 3.2^+0.7 _−0.8		microlensing	22,500⁺²⁶¹⁰ ₋₅₅₄₀	0.57^+0.33 _−0.29		^[76]
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		Estimates of the planet's mass varies between0.3+0.34 −0.16 M_J and0.77+0.87 −0.42 M_J^[74]
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		^[74]
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.^[77]
KMT-2023-BLG-2669	0.02517					microlensing				Candidaterogue planet. Might have a mass ranging from sub-Neptune to Saturn-mass, depending on its distance.^[78]
KMT-2024-BLG-1044L	0.0244^+0.0378 _−0.0127 or 0.0430^+0.0479 _−0.0211					microlensing	21,900⁺³²⁰⁰ ₋₃₄₀₀ or 23,300±3100	0.069^+0.080 _−0.036 or 0.131^+0.146 _−0.064		Host star is either abrown dwarf or ared dwarf.^[79]
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	^[80]
M62H b	2.83	<0.683^[c]^[d]	0.133	0.004908		timing	21,500^[81]	1.4		Pulsar planet located in the globular clusterMessier 62.^[82] Second shortest orbit of any confirmed exoplanet afterPSR J1719-1438 b.^[83]
MOA-2011-BLG-262Lb	0.056634			0.98^+0.56 _−0.20		microlensing	22830	0.193 ± 0.029	3300	Once considered as eitherexomoon or exoplanet, the latter scenario was confirmed in 2024 based on observations of the host star by theKeck telescope. Has the highesttransverse velocity of541.3±65.75 km/s.^[84]
MOA-2016-BLG-526Lb	6.93±0.75			2.07±0.35		microlensing	22,490	0.4		^[70]
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		^[75]
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)^[85]
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	^[85]
NGTS-29 b	0.393	0.857	69.33	0.347	414	transit	487±1	1.034±0.032	5730±80	^[86]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	Also known as TOI-4862 b^[87]
NGTS-31 b	1.12±0.12	1.61±0.16	4.162734±0.000004	0.064±0.008	1410±20	transit	2780⁺³²³ ₋₃₂₆	0.96^+0.11 _−0.05	5710±70	^[88]
NGTS-32 b	0.57±0.05	1.42±0.03	3.31211±0.00002	0.044±0.001	1750±20	transit	2760⁺³³ ₋₂₃	1.07^+0.06 _−0.04	5680±60	^[88]
NGTS-33 b	3.6±0.3	1.64±0.07	2.828	0.048±0.02	1991±21	transit	1430±23	1.60±0.11	7437±72	^[89]
OGLE-2014-BLG-0221Lb	4.35^+1.65 _−1.91			3.76^+0.96 _−1.07		microlensing	12,000⁺³⁶⁹⁰ ₋₃₇₈₀	0.69^+0.26 _−0.30		^[90]
OGLE-2015-BLG-1609Lb	0.0059^+0.0122 _−0.0031 to^+0.24 _−0.90					microlensing	10,100⁺⁸⁵⁰⁰ ₋₆₈₀₀	0.025^+0.050 _−0.012 to 0.17^+0.63 _−0.12		^[91]
OGLE-2016-BLG-1598Lb	5.91±1.74			2.5±0.88		microlensing	19,270±5670	0.55±0.32		^[70]
OGLE-2016-BLG-1800Lb	2.59±1.46			1.88±0.51		microlensing	21,100±3360	0.41±0.22		^[70]
OGLE-2017-BLG-0364Lb	0.0642^+0.106 _−0.034 to 0.805^+0.554 _−0.437			1.27^+0.49 _−0.3		microlensing	22,300 to 29,300	0.1^+0.16 _−0.05 to 0.55^+0.38 _−0.3		^[71] Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassingSWEEPS-04/11.^[83]
OGLE-2017-BLG-0380Lb A	10.5					microlensing	6,980			A pair ofrogue planets.^[92]
OGLE-2017-BLG-0380Lb B	3.08					microlensing	6,980			A pair ofrogue planets.^[92]
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		^[93]
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		^[93]
OGLE-2017-BLG-1275Lb	5.9±2.2			1.19±0.36		microlensing	25,070±2930	0.63±0.23		Another solution suggests a larger semi-major axis, of2.09±0.63 AU.^[93]
OGLE-2023-BLG-0836Lb	4.36^+2.35 _−2.2			3.7⁺¹ _−1.2		microlensing	16,690⁺⁴⁴³⁰ ₋₅₂₅₀	^[e]		The planet is located in a binary star system, and is likely to be orbiting both stars in the system.^[94]
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	Located in the open clusterMessier 67.^[95]
SPECULOOS-3 b		0.08716	0.719	0.00733	553	transit	57.9	0.1	2800	Ultra-short period planet^[96]
Struve 2398 Ab	0.00875±0.0011	0.107–0.178	11.2201±0.0051	0.068±0.001		radial vel.	11.4	0.330±0.008	3470±31	^[97]
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.^[98]
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^[99]^[a]	1.01±0.03	5757⁺⁷² ₋₆₅	^[100]
TIC 46432937 b	3.2±0.11	1.188±0.03	1.44	0.1951±0.0051	872±14	transit	295.5±0.3	0.563±0.029	3572±57	^[101]
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	618	1.035^+0.052 _−0.062	5844⁺⁸⁴ ₋₈₂	^[102]^[103]
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	^[103]
TIC 241249530 b	4.98^+0.16 _−0.18	1.19±0.04	165.772			transit	1058±12^[45]	1.271^+0.061 _−0.068	6139±103^[45]	A planet on a highly-eccentric (e=0.94) and retrograde orbit.^[104]
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 eccentric orbit (e=0.6058)^[105] Also known asTOI-6883 b^[106]
TIC 393818343 c	0.357±0.132	0.792±0.018	7.8458±0.0023	0.079±0.011	1027.2089± 0.3717	transit	306.3±1.1	1.082^+0.055 _−0.056	5756⁺⁵⁷ ₋₆₆	^[107]
TIC 434398831 b		0.3131^+0.0196 _−0.0187	3.6855	0.04641±0.00017	1250±11	transit	698±6	0.992^+0.014 _−0.018	5638±50	Young exoplanet located in the Theia 116association.^[108]
TIC 434398831 c		0.5023^+0.0259 _−0.025	6.21	0.06572±0.00024	1050±10	transit	698±6	0.992^+0.014 _−0.018	5638±50	Young exoplanet located in the Theia 116association.^[108]
TOI-128 b		0.198	4.94	0.054	1345	transit	222.5±0.2^[109]	0.85	6086	^[110]
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	^[111]
TOI-261 b		0.271	3.36	0.035	1722	transit	370.6±0.9^[112]	0.50	5890	^[110]
TOI-286 b	0.01425±0.00245	0.1267±0.0089	4.512	0.0503±0.001	979±31	transit	193	0.832±0.049	5152±12	There are three available models to explain the disagreement between the radial velocity and transit measurements.^[f]^[8]
TOI-286 c	0.01171±0.00698	0.1677±0.0107	39.36	0.213±0.004	475±15	transit	193	0.832±0.049	5152±12	^[8]
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`_☉)^[113]
TOI-406 b	0.00654^+0.00072 _−0.00069	0.1178±0.0107	3.307	0.0322±0.0013	584±22	transit	101±0.7	0.408^+0.046 _−0.042	3392±44	^[114]
TOI-406 c	0.02067±0.003	0.1846±0.0143	13.18	0.0809±0.003	368±14	transit	101±0.7	0.408^+0.046 _−0.042	3392±44	^[114]
TOI-429 b	0.8	0.8056±0.0196	338			transit	391.5±0.5	0.99±0.06	5245⁺²⁵ ₋₆₇	^[115]^[116]^[117]
TOI-480 b	0.0654		6.866			transit	177.8	1.2	6212	^[118]
TOI-588 b		1.459±0.036	39.4718^[119]		1015	transit	502.9±3.2	2.69^+0.34 _−0.36	10,416⁺²⁵⁴ ₋₂₂₀	^[119]^[120]
TOI-603 b	0.1495±0.0431	0.7075±0.018	16.18	0.1281		transit	671.3±5.15	1.072±0.136	5901±130	^[121]
TOI-654 b		0.211	1.53	0.021	749	transit	188.7±0.18^[122]	0.53	3433	^[110]
TOI-663 b	0.0140±0.00204	0.203±0.00892	2.599	0.0295±0.0011	674±30	transit	209.490±0.587	0.514±0.012	3681±70	^[123]
TOI-663 c	0.0115±0.00305	0.202±0.00892	4.696	0.0437±0.0016	553±24	transit
TOI-663 d	<0.0164	0.171±0.0116	7.103	0.0576^+0.0021 _−0.0022	482±21	transit
TOI-694 b		1.146±0.056	48.05^[119]		479.8	transit	730.2^+4.1 _−4.0	1.042^+0.063 _−0.038	5355⁺⁷⁴ ₋₁₄₀	^[119]^[124]
TOI-710 b		1.66±1.10	72.08^[119]			transit	514±2	1.71^+0.39 _−0.19	7458⁺¹⁴⁶ ₋₁₂₃	^[119]^[125]
TOI-757 b	0.033±0.007	0.223±0.001	17.468	0.122±0.002	641±10	transit	196.9⁺¹ _−0.7	0.8±0.04	5278±63	^[126]
TOI-762 Ab	0.251±0.042	0.744±0.017	3.472	0.03418	555±6	transit	322±0.7	0.442±0.025	3266±36	Located in a binary star system.^[101]
TOI-782 b	<0.06	0.244±0.008	8.024	0.0578±0.0018	398±6–435±6^[g]	transit	170.2±0.2	0.397±0.01	3370⁺²⁹ ₋₃₂	^[127]
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	The host star is part of a binary star system with a red dwarf companion^[128]
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
TOI-880 b		0.248	2.57	0.034	1163	transit	197.5±0.2^[129]	0.81	4935	^[110]
TOI-907 b		0.858	4.58	0.055	1847	transit	989.9±5.0^[130]	1.07	6272	^[110]
TOI-1011 b	0.01271±0.00186	0.1294±0.0045	2.47	0.0346		transit	170.8±0.1^[131]	0.92±0.03	5475±84	^[132]
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	^[133]
TOI-1173 Ab	0.08213±0.00598	0.723±0.015	7.064	0.0702±0.0012	863.9±9.8	transit	430.85^[134]^[a]	0.911^+0.028 _−0.03	5350±340	Low-density planet located in a wide binary system.^[135]
TOI-1184 b	0.021±0.007	0.215^+0.009 _−0.013	5.748	0.056±0.001	715.5^+13.7 _−14.1	transit	191.110±0.254	0.73^+0.024 _−0.025	4616±104	^[52]
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	^[136]
TOI-1224 b		0.1877^+0.0084 _−0.0081	4.178	0.0355^+0.0017 _−0.0034	541⁺²⁶ ₋₁₄	transit	121.5	0.4±0.01	3326±66	Located in theMELANGE-5 association, which is200 Myr old. The host star may be binary.^[137]
TOI-1224 c		0.2573±0.0087	17.945			transit	121.5	0.4±0.01	3326±66
TOI-1248 b	0.0862^+0.0113 _−0.0110	0.607^+0.0104 _−0.0107	4.360	0.051±0.001	952.1^+13.5 _−14.3	transit	550.340^+1.963 _−1.947	0.90±0.03	5205±120	^[52]
TOI-1249 b	0.0374^+0.0164 _−0.0160	0.2918^+0.0274 _−0.0167	13.079	0.109±0.002	727⁺¹² ₋₁₁	transit	455.0^+1.8 _−1.7	0.952^+0.167 _−0.082	5453⁺⁷⁶ ₋₁₆₀	^[138]
TOI-1266 d	0.01158^+0.00330 _−0.00349		32.5	0.1513±0.0024	288±5	radial vel. + timing	117.4±0.1	0.437±0.021	3563±77	^[139]
TOI-1269 b	0.020±0.009	0.2142^+0.0134 _−0.0066	4.253	0.0496^+0.0009 _−0.0010	1005⁺¹⁵ ₋₁₄	transit	561.4±2.3	0.969^+0.154 _−0.104	5517⁺¹⁰⁷ ₋₁₄₃	^[140]
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	^[136]
TOI-1279 b	0.0334±0.0079	0.237^+0.0123 _−0.0095	9.61419±0.00004	0.085±0.002	759^+11.8 _−11.7	transit	349.167^+0.933 _−0.926	0.88±0.03	5457±127	^[52]
TOI-1294 b	0.1957±0.016	0.8199±0.0277	3.915	0.0489		transit	1052±7	1.02±0.13	5714±126	^[141]
TOI-1294 c	0.467±0.053		160.1±2.5	0.581		radial vel.	1052±7	1.02±0.13	5714±126	^[142]
TOI-1295 b	1.42±0.08	1.40±0.08	3.197	0.047±0.002	2360±50	transit	1265±16	1.38±0.08	6280±50	^[143]
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	Ultra-short period planet^[144]
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	^[144]
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	^[145]
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	^[145]
TOI-1408 c	0.0239±0.0006	0.1981±0.0054	2.1664±0.0001	0.3587±0.0008		timing	435.6±0.7	1.31±0.01	6117±31	^[146]
TOI-1410 b		0.262	1.22	0.020	1396	transit	236.7±0.2^[147]	0.72	4635	^[110]
TOI-1437 b	0.0302^+0.0123 _−0.0104	0.200^+0.021 _−0.020	18.841	0.140^+0.018 _−0.017	794±14^[148]	transit + radial vel.	336	1.10±0.10	6008±113	^[149]
TOI-1439 b	0.121±0.018	0.379^+0.021 _−0.015	27.644	0.192±0.004	748.4^+10.9 _−13.1	transit	751.158^+7.691 _−7.537	1.24	5857±60	^[150]
TOI-1443 b	<0.0944	0.2055^+0.0113 _−0.0090	23.541	0.147±0.003	521⁺¹⁴ ₋₁₂	transit	279.9±0.7	0.89^+0.14 _−0.09	5236⁺¹¹¹ ₋₁₄₀	^[151]
TOI-1448 b	<0.0613	0.245±0.006	8.112	0.0567±0.0015	389±5–426±6^[g]	transit	240±0.3	0.372±0.009	3412⁺²⁸ ₋₃₂	^[127]
TOI-1450 Ab	0.00396±0.0004	0.1±0.004	2.04		722±35	transit	73.2±0.1	0.48±0.024	3437±86	Located in a binary star system. It is the second-lowest mass transiting planet with a high-precision mass measurement.^[152]
TOI-1450 Ac	0.0048±0.0006		5.07		533±26	radial vel.	73.2±0.1	0.48±0.024	3437±86	Located in a binary system, its true mass could be similar to the minimum mass assumingcoplanarity with TOI-1450 Ab.^[152]
TOI-1451 b	0.0478±0.0088	0.233^+0.0120 _−0.0092	16.538	0.127±0.003	723.3^+12.4 _−12.2	transit	299.856^+0.710 _−0.707	1.00^+0.04 _−0.03	5800±139	^[52]
TOI-1472 b	0.0519±0.0160	0.371^+0.0140 _−0.0113	6.36381±0.00091	0.065±0.001	811.1^+11.2 _−10.8	transit	397.389^+4.341 _−4.250	0.92±0.02	5103⁺¹¹⁹ ₋₁₄₄	^[52]
TOI-1669 b	<0.0409	0.2049^+0.0091 _−0.0080	2.68	0.0376±0.0007	1285⁺²² ₋₂₁	transit	362.9±1.2	1.00±0.05	5542±100	^[153]
TOI-1683 b		0.236	3.06	0.037	929	transit	166.2±0.2^[154]	0.69	4402	^[110]
TOI-1691 b	0.0459^+0.0170 _−0.0167	0.3181^+0.0096 _−0.0078	16.737	0.126±0.003	703⁺¹³ ₋₁₂	transit	363.5±1.2	1.031^+0.159 _−0.127	5759⁺²⁰⁹ ₋₁₆₅	^[155]
TOI-1723 b		0.2937^+0.0127 _−0.0114	13.72641±0.00046	0.114±0.002	783⁺¹⁵ ₋₁₄	transit	328.5±1.0	1.035^+0.147 _−0.107	5777⁺¹⁴⁹ ₋₁₀₁	^[156]
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	The host star ismetal-poor([Fe/H] = –0.40dex).^[157]
TOI-1753 b	0.0522±0.0164	0.221^+0.009 _−0.007	5.385	0.059±0.001	1005.4^+18.3 _−17.6	transit	739.302^+8.907 _−8.699	0.95±0.03	5620±134	^[52]
TOI-1758 b		0.3174^+0.0203 _−0.0127	20.705	0.138±0.003	551⁺⁹ ₋₈	transit	315.1±1.1	0.88^+0.12 _−0.09	5169⁺⁹⁵ ₋₁₄₈	^[158]
TOI-1775 b	0.302±0.047	0.718^+0.0128 _−0.0114	10.241	0.080±0.002	707.9^+8.6 _−8.3	transit	486.736^+3.108 _−3.072	0.92^+0.01 _−0.02	5283±116	^[52]
TOI-1776 b		0.1085^+0.0080 _−0.0069	2.8	0.0378^+0.0007 _−0.0008	1269±21	transit	146	1.02^+0.11 _−0.14	5724±105	^[159]
TOI-1798 b		0.126	0.44	0.011	2122	transit	369.147^+1.008 _−1.005	0.86	5165	^[110]
TOI-1798 c	0.018^+0.003 _−0.002	0.125^+0.006 _−0.005	0.438	0.0107±0.0002	1935.8^+25.2 _−25.9	transit	369.147^+1.008 _−1.005	0.86	5165	^[52]
TOI-1799 b	0.013^+0.005 _−0.006	0.1269^+0.0932 _−0.0880	7.085738±0.000083	0.071±0.001	923⁺¹⁵ ₋₁₄	transit	203	1.01^+0.14 _−0.12	5690⁺¹²¹ ₋₁₂₄	^[160]
TOI-1803 b	0.03241±0.00787	0.267±0.007	6.293287±0.000028	0.060±0.001	747±11	transit	388.3	0.756^+0.050 _−0.042	4687±65	^[161]
TOI-1803 c	0.01794±0.00944	0.3738^+0.0223 _−0.0267	12.885776±0.000036	0.097±0.002	561±10	transit	388.3	0.756^+0.050 _−0.042	4687±65	^[161]
TOI-1806 b		0.304	15.15	0.088	337	transit	180.7±0.2^[162]	0.39	3272	^[110]
TOI-1823 b	0.212^+0.025 _−0.026	0.673^+0.030 _−0.022	38.80±0.01	0.212±0.004	423.6^+10.4 _−8.7	transit	233.677^+0.375 _−0.374	0.84±0.03	4926±113	^[52]
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 "overdense sub-Neptunes". TOI-1824 has also a red dwarf companion named TIC 142387022.^[163]
TOI-1828 b	0.1841±0.012	0.769±0.017	9.09	0.0859		transit	1208±8	1.04±0.13	5809±127	^[164]
TOI-1855 b	1.133±0.096	1.65^+0.52 _−0.37	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	^[165]
TOI-1883 b		0.4953±0.0460	4.506		524.9	transit	376±3	0.492±0.02	3477±157	^[166]^[167]
TOI-1885 b	1.624±0.103	1.219±0.037	6.544060±0.000006			transit	1826.773^+21.464 _−20.982		6527±98	^[150]
TOI-1898 b	0.4059^+0.0220 _−0.0252	0.838^+0.021 _−0.028	45.52	0.269±0.005	674.5^+11.6 _−11.8	transit	259.7±1.4	1.24^+0.22 _−0.16	6304⁺¹³⁹ ₋₁₄₄	^[168]
TOI-2019 b	0.109±0.0132	0.505±0.0250	15.3444±0.0055			transit	645.812^+2.684 _−2.665		5590	^[150]
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	^[165]
TOI-2120 b	<0.02139	0.1893±0.0056	5.8	0.0377±0.0013	351±6–384±6^[g]	transit	104.9	0.211±0.005	3131±30	^[127]
TOI-2128 b	0.014±0.006	0.186^+0.008 _−0.007	16.341	0.127±0.003	780.5^+14.8 _−14.4	transit	119.2±0.1	1.1^+0.15 _−0.12	5991⁺¹¹⁴ ₋₉₀	^[169]
TOI-2264 b		0.3726±0.0355	55.08^[119]		373.1	transit	617.2^+7.1 _−6.9	1.164^+0.146 _−0.168	6140⁺¹²⁹ ₋₁₂₈	^[119]^[170]
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	^[171]
TOI-2274 b			2.679		771	transit	159.9±0.2	0.612±0.02	3943±157	^[172]^[167]
TOI-2286 b		0.3343±0.0606	179.4		434.7	transit	761.6^+3.4 _−3.3	1.487^+0.322 _−0.209	6863⁺¹⁴⁷ ₋₂₇₇	^[119]^[173]
TOI-2295 b	0.875^+0.042 _−0.041	1.47^+0.85 _−0.53	30.03	0.1992^+0.0039 _−0.0041	747±24	transit	409.36^+0.52 _−0.46	1.168^+0.070 _−0.071	5730±140	Radius in unconstrained due to the planet's grazing transit.^[174]
TOI-2295 c	5.61^+0.23 _−0.24		966.5^+4.3 _−4.2	2.018^+0.040 _−0.042	234.9±7.6	radial vel.	409.36^+0.52 _−0.46	1.168^+0.070 _−0.071	5730±140	^[174]
TOI-2328 b	0.16±0.02	0.89±0.04	17.102	0.127^+0.005 _−0.006	842⁺²⁰ ₋₂₁	transit	746.6±4.9	0.95±0.06	5525⁺¹⁴⁷ ₋₁₄₄	^[175]
TOI-2368 b	0.65±0.18	0.967^+0.036 _−0.031	5.175	0.05649±0.001	1000⁺⁴⁴ ₋₃₀	transit	685±3.9	0.897^+0.048 _−0.049	5360⁺²³⁰ ₋₁₇₀	^[165]
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	^[176]
TOI-2374 b	0.1782^+0.011 _−0.0134	0.6075±0.0268	4.314	0.0471	<885±22	transit	439±3	0.75±0.01	4802±97	^[177]
TOI-2379 b	5.76±0.20	1.046±0.023	5.4693827±0.0000023	0.05263±0.00091	624±12	transit	689.5±3.6	0.645±0.033	3707±58	^[178]
TOI-2384 b	1.966±0.059	1.025±0.021	2.13570304±0.00000038	0.02793±0.00023	889.7±5.0	transit	609.9±4.9	0.635±0.016	3943±14	^[178]
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	^[176]
TOI-2420 b	0.927^+0.085 _−0.079	1.340^+0.074 _−0.072	5.8426	0.0684^+0.0067 _−0.0059	1571.6^+60.8 ₋₆₄	transit	1450^[a]	1.158±0.098		^[179]
TOI-2458 b	0.04188^+0.00311 _−0.00302	0.252^+0.018 _−0.016	3.73659^+0.00044 _−0.00047	0.0482^+0.0025 _−0.0027	1509⁺⁴¹ ₋₃₅	transit	368.42^+1.76 _−1.74	1.05±0.03	6005±50	Also known as HD 34562 b.^[180]
TOI-2458 c	0.03216^+0.00538 _−0.00598		16.553^+0.059 _−0.061	0.129±0.002		radial vel.	368.42^+1.76 _−1.74	1.05±0.03	6005±50	^[180]
TOI-2477 b		1.156±0.403	34.78^[119]			transit	1181.4^+16.8 _−16.3	1.73^+0.40 _−0.21	7505⁺¹⁹² ₋₂₂₂	^[119]^[181]
TOI-2485 b	2.412^+0.088 _−0.087	1.083±0.045	11.235	0.1093^+0.0055 _−0.0057	1134⁺²⁷ ₋₂₅	transit	1296^[a]	1.163±0.053		^[179]
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	^[176]
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	^[100]
TOI-2537 b	1.307^+0.091 _−0.088	1.004^+0.059 _−0.061	94.1022±0.0011	0.3715^+0.0077 _−0.0080	338±14	transit	594.97^+3.42 _−3.03	0.771±0.049	4870±150	^[174]
TOI-2537 c	7.23^+0.52 _−0.45		1920⁺²³⁰ ₋₁₄₀	2.78^+0.22 _−0.15	123.1^+6.3 _−6.7	radial vel.	594.97^+3.42 _−3.03	0.771±0.049	4870±150	^[174]
TOI-2580 b	0.63±0.08	1.55±0.05	3.397750±0.000002	0.048±0.003	2410±60	transit	1236±16	1.33±0.08	6120±30	^[143]
TOI-2714 b	0.717^+0.104 _−0.101	1.224^+0.0625 _−0.0598	2.499	0.036±0.002	1603±65	transit	1930±16	1.07±0.06	5665±115	^[182]
TOI-2768 b		0.2688±0.0313	1.508		855	transit	255.8±0.6	0.63^+0.06 _−0.10	4008⁺¹²⁴ ₋₁₃₇	^[183]^[167]
TOI-2981 b	2.007±0.104	1.1955±0.0375	3.602	0.048±0.002	1358±39	transit	1741±16	1.03±0.06	5940±75	^[182]
TOI-3071 b	0.2146±0.011	0.6388^+0.0509 _−0.0455	1.267	0.0249	<2155±40	transit	1582±29	1.29±0.02	6177±62	^[177]
TOI-3261 b	0.0953±0.0076	0.3408^+0.0375 _−0.0312	0.883	0.01714	1722⁺²⁶ ₋₁₈	transit	972.3^+2.3 _−3.1	0.861^+0.02 _−0.03	4995±47	Ultra-hot Neptune^[184]
TOI-3321 b	0.554±0.076	1.388^+0.070 _−0.064	3.652	0.047±0.001	1616±30	transit	928^+10.8 _−10.4	1.041^+0.084 _−0.068	5850±140	^[165]
TOI-3353 b		0.238	4.67	0.060	1264	transit	257.1±0.2^[185]	1.33	6365	^[110]
TOI-3568 b	0.083±0.003	0.473±0.024	4.42	0.0485±0.0004	899±12	transit	645±2	0.78±0.02	4969±45	^[186]
TOI-3837 b	0.59±0.06	0.96±0.05	11.889	0.098±0.005	1182⁺³⁰ ₋₃₁	transit	1000.3±18.9	0.89±0.05	5905⁺¹⁵⁷ ₋₁₅₅	^[175]
TOI-3894 b	0.85±0.15	1.358^+0.054 _−0.052	4.335	0.0543±0.0014	1519±22	transit	1343^+12.7 _−12.4	1.138^+0.089 _−0.075	6000±110	^[165]
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	^[165]
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	^[165]
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	Located in a triple hierarchical stellar system.^[187]
TOI-4356 b		0.321±0.198	289.92^[119]			transit	668.6±3.8	1.48^+0.32 _−0.19	6855⁺¹⁴⁰ ₋₁₂₇	^[119]^[188]
TOI-4364 b		0.1793^+0.0089 _−0.0082	5.424	0.04753^+0.00053 _−0.00054	488±4	transit	142.9±0.1	0.487^+0.017 _−0.016	3528⁺³³ ₋₂₀	Located in theHyades.^[189]
TOI-4379 b	1.113±0.071	1.489±0.079	3.254			transit	2013⁺³⁸ ₋₃₉	1.372^+0.037 _−0.105	6020±100	^[190]
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	^[191]
TOI-4443 b		0.153	1.85	0.030	1639	transit	183.0^[192]	1.05	5834	^[110]
TOI-4468 b		1.0197±0.0517	2.77			transit	1224.7±8.2	0.82	4975±122	^[193]
TOI-4468 c		0.296±0.023	7.01			transit	1224.7±8.2	0.82	4975±122	^[194]
TOI-4495 b		0.324	5.18	0.062	1383	transit	431.2^[195]	1.17	6156	^[110]
TOI-4504 b	0.03272±0.00283	0.240±0.017	2.426	0.03392±0.00068		transit	1117.43±5.57	0.89^+0.06 _−0.04	5315±60	^[196]
TOI-4504 c	3.77±0.18	0.9897±0.0092	82.97213±0.00013	0.3546^+0.0073 _−0.0077		transit + radial vel.
TOI-4504 d	1.417±0.065		40.5634^+0.0365 _−0.0368	0.2219^+0.0041 _−0.0043		timing
TOI-4527 b		0.0812	0.40	0.008	1363	transit	59.03^[197]	0.48	3702	^[110]
TOI-4562 c	5.77^+0.37 _−0.56		3990⁺²⁰¹ ₋₁₉₂	5.219±0.002		timing	1131±12^[198]	1.218^+0.054 _−0.048^[198]	6096±32^[198]	^[199]
TOI-4602 b		0.227	3.98	0.051	1380	transit		1.12	6012	^[110]
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^[h]	5600±50 or 5800±50^[h]	Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are atperiastron.^[200]
TOI-4914 b	0.714±0.041	1.1482±0.0321	10.6	0.098±0.003	894±20	transit	951±5	1.03±0.06	5805±62	^[182]
TOI-4994 b	0.280^+0.037 _−0.034	0.762^+0.030 _−0.027	21.491984±0.000023	0.1515^+0.0032 _−0.0031	717.6^+9.7 ₋₁₀	transit	1079±8	1.005^+0.064 _−0.061	5640±110	^[201]
TOI-5005 b	0.103±0.018	0.558±0.021	6.309	0.06614±0.0045	1040±20	transit	685±2	0.97±0.02	5749±61	^[202]
TOI-5027 b	2.01±0.13	0.99^+0.07 _−0.12	10.244	0.093±0.004	1056⁺²³ ₋₂₄	transit	659.5±4.9	1.02±0.05	5909⁺¹⁴⁵ ₋₁₄₄	^[175]
TOI-5076 b	0.0503±0.00629	0.285±0.00892	23.445±0.001		615±20	transit	270.057±0.326	0.80±0.07	5070±143	^[203]
TOI-5082 b		0.227	4.24	0.051	1165	transit		1.00	5670	^[110]
TOI-5110 b	2.90±0.13	1.069^+0.054 _−0.052	30.159	0.2157^+0.0042 _−0.0044	976⁺³³ ₋₃₂	transit	1170.64^+5.12 _−9.65	1.469^+0.089 _−0.088	6160±150	^[174]
TOI-5218 b	0.799^+0.393 _−0.359	0.879±0.034	4.291	0.0469±0.0006	783±21	transit	1243±11	0.739±0.03	4230±88	^[69]
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	^[165]
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	^[165]
TOI-5319 b		0.33427±0.0551	4.079		695	transit	199.4±0.7	0.5±0.1	3580⁺¹⁰⁷ ₋₁₄₁	^[204]^[167]
TOI-5388 b		0.169	2.59	0.024	601	transit	60.40^[205]	0.29	3495	^[110]
TOI-5575 b		0.8459±0.0255	32.07^[119]		195	transit	184.9±0.6	0.21±0.02	3176±157	^[119]^[206]
TOI-5616 b	0.802^+0.371 _−0.384	0.961^+0.048 _−0.042	2.003	0.0272±0.0003	939±27	transit	1249±14	0.666±0.025	3996±88	^[69]
TOI-5634 Ab	0.576^+0.406 _−0.346	0.923^+0.056 _−0.050	2.2035	0.0272±0.0003	837±34	transit	1051⁺²⁰ ₋₁₈	0.556±0.022	3896±88	^[69]
TOI-5688 Ab	0.390^+0.074 _−0.077	0.920^+0.053 _−0.062	2.948	0.03379^+0.00046 _−0.00045	742±18	transit	735.8^+4.2 _−4.9	0.60±0.02	3713±59	^[207]
TOI-5713 b	0.0135^+0.0053 _−0.0035	0.1579^+0.0152 _−0.0125	10.44	0.06008±0.00046	347±3	transit	133.7^[a]	0.265±0.006	3228±41	^[208]
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	^[209]
TOI-5723 b		1.146±0.068	56.88^[119]			transit	1878⁺²² ₋₂₁	1.01^+0.12 _−0.15	5695⁺¹¹⁰ ₋₁₇₀	^[119]^[210]
TOI-5731 b		0.401±0.046	90.1			transit	358.2±0.8	0.697^+0.088 _−0.077	4448⁺⁹² ₋₁₂₃	^[119]^[211]
TOI-5975 b		0.7536±0.0422	186.52^[119]			transit	1141^+7.1 _−7.0	1.335^+0.260 _−0.188	6508⁺⁸³ ₋₁₆₃	^[119]^[212]
TOI-6002 b	0.0119^+0.005 _−0.0031	0.1454^+0.0107 _−0.017	10.905	0.05722±0.00044	321⁺⁷ ₋₅	transit	104.6^[a]	0.21	3241⁺⁸⁰ ₋₆₀	^[208]
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^[209]
TOI-6016 b	1.17±0.09	1.22±0.03	4.023687±0.000003	0.055±0.002	1890±40	transit	1190±13	1.31±0.08	6110±50	^[143]
TOI-6029 b	1.635±0.032	1.284±0.098	5.7987±0.0004			transit	1946⁺³⁷ ₋₃₆	1.548^+0.027 _−0.085	6223±100	^[190]
TOI-6034 b	0.798±0.075	1.063±0.042	2.576	0.02949^+0.00043 _−0.00044	714±21	transit	385	0.514^+0.025 _−0.022	3635±88	^[69]
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	^[209]
TOI-6130 b	1.05±0.06	1.28±0.03	2.392679±0.000002	0.036±0.002	1750±40	transit	721±10	1.16±0.07	5940±50	^[143]
TOI-6303 b	7.84±0.31	1.034^+0.054 _−0.057	9.4852360±0.0000162	0.07610±0.00100	541±14	transit	495.17±1.37	0.644±0.024	3977±59	^[213]
TOI-6324 b	0.0041±0.0006	0.0937	0.28			transit	67.02±0.05	0.272±0.020	3358±160	^[115]
TOI-6330 b	10±0.32	0.972^+0.033 _−0.031	6.8500246±0.0000033	0.05763^+0.00073 _−0.00077	495±14	transit	468.07±1.79	0.531±0.021	3539±59	^[213]
TOI-6383 Ab	1.04±0.094	1.008^+0.036 _−0.033	1.791	0.02292±0.00037	745±23	transit	561^+3.0 _−2.7	0.458±0.011	3444±88	^[214]
TOI-6651 b	0.1919^+0.0239 _−0.0249	0.4541^+0.0241 _−0.0232	5.057	0.06330^+0.00078 _−0.00072	1493⁺¹⁴ ₋₁₅	transit	690±3^[215]^[a]	1.323^+0.050 _−0.045	5940±110	^[216]
TOI-6628 b	0.75±0.06	0.98±0.05	18.184	0.133±0.007	836⁺²² ₋₂₃	transit	1028±27	0.97±0.06	5463⁺¹⁴³ ₋₁₄₂	^[175]
TOI-7041 b	0.36±0.16	1.02±0.03	9.691±0.006			transit	1431±10	1.12±0.02	4640±10	^[217]
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^[218]
WASP-132d	5.16±0.52		1816.6±44.4	2.71±0.12	107⁺¹¹ ₋₁₈	radial vel.	401.53±1.86	0.789±0.039	4686±99	^[219]
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	Ultra-short period planet^[220]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]

List of exoplanets discovered before 2000 (31)
List of exoplanets discovered between 2000–2009 (375)
List of exoplanets discovered in 2010 (109)
List of exoplanets discovered in 2011 (179)
List of exoplanets discovered in 2012 (149)
List of exoplanets discovered in 2013 (149)
List of exoplanets discovered in 2014 (869)
List of exoplanets discovered in 2015 (144)
List of exoplanets discovered in 2016 (1498)
List of exoplanets discovered in 2017 (152)
List of exoplanets discovered in 2018 (300)
List of exoplanets discovered in 2019 (170)
List of exoplanets discovered in 2020 (247)
List of exoplanets discovered in 2021 (254)
List of exoplanets discovered in 2022 (313)
List of exoplanets discovered in 2023 (307)
List of exoplanets discovered in 2024 (285)
List of exoplanets discovered in 2025 (107)

Notes

[edit]

^^a ^b ^c ^d ^e ^f ^g ^hDistance calculated from parallax
^The radius is the same as that of the Earth, with an uncertainty of 10%
^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 (inM_J and r is the radius (in centimeters). Should be divided by7.1492×10⁹ to convert from centimeters toR_J
^Since the density is only a lower limit, the radius is an upper limit.
^The planet is located in a two-star system, with masses of0.78+0.38
−0.36 M_☉ and0.56+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 be0.78+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.
^The transit observations of TOI-286 indicate periodic transit signals of 4.5 and 39.4 days. While this, radial velocity measurements with ESPRESSO do not immediately show evidence for periodic signals at either periods.
^^a ^b ^cAssumingalbedos of 0.3 and 0 respectively.
^^a ^bIt is not known which of the stars the planet orbits.

References

[edit]

^Gupta, Arvind F.; Luhn, Jacob K.; Wright, Jason T.; Mahadevan, Suvrath; Robertson, Paul; Krolikowski, Daniel M.; Ford, Eric B.; Cañas, Caleb I.; Halverson, Samuel (2025)."The NEID Earth Twin Survey. I. Confirmation of a 31-day planet orbiting HD 86728".The Astronomical Journal.169 (1): 1.arXiv:2409.12315.Bibcode:2025AJ....169....1G.doi:10.3847/1538-3881/ad89bf.
^"The Extrasolar Planet Encyclopaedia — 82 Eri d".Extrasolar Planets Encyclopaedia.Paris Observatory.
^Nari, N.; Dumusque, X.; Hara, N. C.; Mascareño, A. Suárez; Cretignier, M.; Hernández, J. I. González; Stefanov, A. K.; Passegger, V. M.; Rebolo, R.; Pepe, F.; Santos, N. C.; Cristiani, S.; Faria, J. P.; Figueira, P.; Sozzetti, A. (4 November 2024). "Revisiting the multi-planetary system of the nearby star HD 20794. Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarf".Astronomy & Astrophysics.arXiv:2501.17092.doi:10.1051/0004-6361/202451769.ISSN 0004-6361.
^^a ^b"VizieR".
^^a ^bMarocco, 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".The Astrophysical Journal.967 (2): 147.arXiv:2404.14324.Bibcode:2024ApJ...967..147M.doi:10.3847/1538-4357/ad3f1d.
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^Zingales, T.; Malavolta, L.; Borsato, L.; Turrini, D.; Bonfanti, A.; Polychroni, D.; Mantovan, G.; Nardiello, D.; Nascimbeni, V. (2025). "A joint effort to discover and characterize two resonant mini Neptunes around TOI-1803 with TESS, HARPS-N and CHEOPS".Astronomy and Astrophysics.695: A273.arXiv:2412.05423.Bibcode:2025A&A...695A.273Z.doi:10.1051/0004-6361/202451180.
^"TOI-1806".SIMBAD.Centre de données astronomiques de Strasbourg.
^Lange, Sarah; Murphy, Joseph M. Akana; Batalha, Natalie M.; Crossfield, Ian J. M.; Dressing, Courtney D.; Fulton, Benjamin; Howard, Andrew W.; Huber, Daniel; Isaacson, Howard; Kane, Stephen R.; Petigura, Erik A.; Robertson, Paul; Weiss, Lauren M.; Behmard, Aida; Beard, Corey (23 May 2024)."The TESS-Keck Survey. VII. A Superdense Sub-Neptune Orbiting TOI-1824*".The Astronomical Journal.167 (6): 282.Bibcode:2024AJ....167..282L.doi:10.3847/1538-3881/ad34d9.ISSN 1538-3881.
^"The Extrasolar Planet Encyclopaedia — TOI-1828 b".Extrasolar Planets Encyclopaedia.Paris Observatory.
^^a ^b ^c ^d ^e ^f ^g ^h ⁱSchulte, 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",The Astronomical Journal,168 (1): 32,arXiv:2401.05923,Bibcode:2024AJ....168...32S,doi:10.3847/1538-3881/ad4a57
^"TOI-1883 Overview".NASA Exoplanet Archive.
^^a ^b ^c ^dPeláez-Torres, A.; Esparza-Borges, E.; Pallé, E.; Parviainen, H.; Murgas, F.; Morello, G.; Zapatero-Osorio, M. R.; Korth, J.; Narita, N.; Fukui, A.; Carleo, I.; Luque, R.; García, N. Abreu; Barkaoui, K.; Boyle, A. (1 October 2024)."Validation of up to seven TESS planet candidates through multi-colour transit photometry using MuSCAT2 data".Astronomy & Astrophysics.690: A62.arXiv:2409.07400.Bibcode:2024A&A...690A..62P.doi:10.1051/0004-6361/202347251.ISSN 0004-6361.
^"TOI-1898 Overview".NASA Exoplanet Archive.
^"TOI-2128 Overview".NASA Exoplanet Archive.
^"TOI-2264 Overview".NASA Exoplanet Archive.
^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.
^"TOI-2274 Overview".NASA Exoplanet Archive.
^"TOI-2286 Overview".NASA Exoplanet Archive.
^^a ^b ^c ^dHeidari, N.; H'ebrard, G.; Martioli, E.; Eastman, J. D.; Jackson, J. M.; Delfosse, X.; Jord'an, A.; Correia, A. C. M.; Sousa, S. (2025), "Characterization of seven transiting systems including four warm Jupiters from SOPHIE and TESS",Astronomy and Astrophysics,694: A36,arXiv:2412.08527,Bibcode:2025A&A...694A..36H,doi:10.1051/0004-6361/202451519
^^a ^b ^c ^dPinto, Marcelo Tala; Jordán, Andrés; Acuña, Lorena; Jones, Matías; Brahm, Rafael; Reinarz, Yared; Eberhardt, Jan; Espinoza, Néstor; Henning, Thomas (2025). "Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328".Astronomy and Astrophysics.694: A268.arXiv:2412.02069.Bibcode:2025A&A...694A.268T.doi:10.1051/0004-6361/202452517.
^^a ^b ^cEberhardt, 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.
^^a ^bHacker, Alejandro; et al. (43) (8 June 2024)."TOI-2374 b and TOI-3071 b: two metal-rich sub-Saturns well within the Neptunian desert".Monthly Notices of the Royal Astronomical Society.532 (2):1612–1634.arXiv:2406.12996.doi:10.1093/mnras/stae1420.
^^a ^bBryant, Edward M.; et al. (34) (29 August 2024)."TOI-2379 b and TOI-2384 b: two super-Jupiter mass planets transiting low-mass host stars".Monthly Notices of the Royal Astronomical Society.533 (4):3893–3906.arXiv:2409.01239.doi:10.1093/mnras/stae2034. Retrieved28 September 2024.
^^a ^bCarleo, Ilaria; Barrágan, Oscar; Persson, Carina M.; Fridlund, Malcolm; Lam, Kristine W. F.; Messina, Sergio; Gandolfi, Davide; Smith, Alexis M. S.; Johnson, Marshall C. (10 August 2024). "Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b".Astronomy and Astrophysics.690: A18.arXiv:2408.05612.Bibcode:2024A&A...690A..18C.doi:10.1051/0004-6361/202451313.
^^a ^bŠubjak, Ján; et al. (36) (2025). "TOI-2458 b: A mini-Neptune consistent with in situ hot Jupiter formation".Astronomy and Astrophysics.693: A235.arXiv:2409.17532.Bibcode:2025A&A...693A.235S.doi:10.1051/0004-6361/202451057.
^"TOI-2477 Overview".NASA Exoplanet Archive.
^^a ^b ^cMantovan, G.; Wilson, T. G.; Borsato, L.; Zingales, T.; Biazzo, K.; Nardiello, D.; Malavolta, L.; Desidera, S.; Marzari, F. (11 September 2024). "The inflated, eccentric warm Jupiter TOI-4914 b orbiting a metal-poor star, and the hot Jupiters TOI-2714 b and TOI-2981 B".Astronomy & Astrophysics.691: A67.arXiv:2409.07520.Bibcode:2024A&A...691A..67M.doi:10.1051/0004-6361/202451841.
^"TOI-2768 Overview".NASA Exoplanet Archive.
^Nabbie, Emma; et al. (2024). "Surviving in the Hot Neptune Desert: The Discovery of the Ultra-Hot Neptune TOI-3261b".arXiv:2407.04225v1 [astro-ph.EP].
^"TOI-3353".SIMBAD.Centre de données astronomiques de Strasbourg.
^Martioli, E.; Petrucci, R. P.; Jofre, E.; Hebrard, G.; Ghezzi, L.; Chew, Y. Gomez Maqueo; Diaz, R. F.; Perottoni, H. D.; Garcia, L. H. (5 September 2024). "TOI-3568 b: a super-Neptune in the sub-Jovian desert".Astronomy and Astrophysics.690: A312.arXiv:2409.03704.Bibcode:2024A&A...690A.312M.doi:10.1051/0004-6361/202450334.
^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".Astronomy & Astrophysics.687: A48.arXiv:2404.12722.Bibcode:2024A&A...687A..48T.doi:10.1051/0004-6361/202347981.
^"TOI-4356 Overview".NASA Exoplanet Archive.
^Distler, Adam; Soares-Furtado, Melinda; Vanderburg, Andrew; Schulte, Jack; Becker, Juliette; Mann, Andrew W.; Howell, Steve B.; Kraus, Adam L.; Barkaoui, Khalid (16 October 2024)."TESS Hunt for Young and Maturing Exoplanets (THYME) XII: A Young Mini-Neptune on the Upper Edge of the Radius Valley in the Hyades Cluster".The Astronomical Journal.169 (3): 166.arXiv:2410.11990.Bibcode:2025AJ....169..166D.doi:10.3847/1538-3881/ada26a.
^^a ^bSaunders, Nicholas; Grunblatt, Samuel K.; Chontos, Ashley; Dai, Fei; Huber, Daniel; Zhang, Jingwen; Stefansson, Gudmundur; van Saders, Jennifer L.; Winn, Joshua N.; Hey, Daniel; Howard, Andrew W.; Fulton, Benjamin; Isaacson, Howard; Beard, Corey; Giacalone, Steven (1 August 2024)."TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence".The Astronomical Journal.168 (2): 81.arXiv:2407.21650.Bibcode:2024AJ....168...81S.doi:10.3847/1538-3881/ad543b.ISSN 0004-6256.
^Martin, Pierre-Yves (2024)."Planet TOI-4438 b".exoplanet.eu. Retrieved6 March 2024.
^"The Extrasolar Planet Encyclopaedia — TOI-4443 b.".Extrasolar Planets Encyclopaedia. 2025.
^"The Extrasolar Planet Encyclopaedia — TOI-4468 b".Extrasolar Planets Encyclopaedia.Paris Observatory. Retrieved31 December 2024.
^"The Extrasolar Planet Encyclopaedia — TOI-4468 c".Extrasolar Planets Encyclopaedia.Paris Observatory. Retrieved31 December 2024.
^"The Extrasolar Planet Encyclopaedia — TOI-4495 b.".Extrasolar Planets Encyclopaedia. 2025.
^Vítková, Michaela; Brahm, Rafael; Trifonov, Trifon; Kabáth, Petr; Jordán, Andrés; Henning, Thomas; Hobson, Melissa J.; Eberhardt, Jan; Pinto, Marcelo Tala (2025)."TOI-4504: Exceptionally large Transit Timing Variations induced by two resonant warm gas giants in a three planet system".The Astrophysical Journal.978 (2): L22.arXiv:2412.05609.Bibcode:2025ApJ...978L..22V.doi:10.3847/2041-8213/ad9a53.
^"The Extrasolar Planet Encyclopaedia — TOI-4527 b.".Extrasolar Planets Encyclopaedia. 2025.
^^a ^b ^cHeitzmann, Alexis; Zhou, George; Quinn, Samuel N.; Huang, Chelsea X.; Dong, Jiayin; Bouma, Luke G.; Dawson, Rebekah I.; Marsden, Stephen C.; Wright, Duncan; Petit, Pascal; Collins, Karen A.; Barkaoui, Khalid; Wittenmyer, Robert A.; Gillen, Edward; Brahm, Rafael (1 March 2023)."TOI-4562 b: A highly eccentric temperate Jupiter analog orbiting a young field star".The Astronomical Journal.165 (3): 121.arXiv:2208.10854.Bibcode:2023AJ....165..121H.doi:10.3847/1538-3881/acb5a2.ISSN 0004-6256.
^Fermiano, V.; Saito, R. K.; Ivanov, V. D.; Caceres, C.; Almeida, L. A.; Aires, J.; Beamin, J. C.; Minniti, D.; Ferreira, T. (10 September 2024). "The young exoplanetary system TOI-4562: Confirming the presence of a third body in the system".Astronomy and Astrophysics.690: L7.arXiv:2409.06924.Bibcode:2024A&A...690L...7F.doi:10.1051/0004-6361/202451935.
^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.Bibcode:2024AJ....167..241E.doi:10.3847/1538-3881/ad1d5c.ISSN 0004-6256.
^Romy Rodriguez Martinez; et al. (2024)."Discovery and Characterization of an Eccentric, Warm Saturn Transiting the Solar Analog TOI-4994".The Astronomical Journal.169 (2): 72.arXiv:2412.02769.Bibcode:2025AJ....169...72R.doi:10.3847/1538-3881/ad9b90.
^Castro-González, A.; Lillo-Box, J.; Armstrong, D. J.; Acuña, L.; Aguichine, A.; Bourrier, V.; Gandhi, S.; Sousa, S. G.; Delgado-Mena, E. (26 September 2024). "TOI-5005 b: A super-Neptune in the savanna near the ridge".Astronomy & Astrophysics.691: A233.arXiv:2409.18129.Bibcode:2024A&A...691A.233C.doi:10.1051/0004-6361/202451656.
^Montalto, M.; et al. (39) (29 May 2024). "The GAPS programme at TNG. LVII. TOI-5076b: A warm sub-Neptune planet orbiting a thin-to-thick-disk transition star in a wide binary system".Astronomy and Astrophysics.687.arXiv:2405.18950.Bibcode:2024A&A...687A.226M.doi:10.1051/0004-6361/202349082.
^"TOI-5319 Overview".NASA Exoplanet Archive.
^"The Extrasolar Planet Encyclopaedia — TOI-5388 b.".Extrasolar Planets Encyclopaedia. 2025.
^"TOI-5575 Overview".NASA Exoplanet Archive.
^Reji, Varghese; Kanodia, Shubham; Ninan, Joe; Cañas, Caleb I.; Libby-Roberts, Jessica; Lin, Andrea S. J.; Gupta, Arvind F.; Sewaby, Tera N.; Larsen, Alexander (4 September 2024)."Searching for GEMS: TOI-5688 A b, a low-density giant orbiting a high-metallicity early M-dwarf".The Astronomical Journal.169 (3): 187.arXiv:2409.01371.Bibcode:2025AJ....169..187R.doi:10.3847/1538-3881/ada7ea.
^^a ^bGhachoui, M.; Rackham, B. V.; Dévora-Pajares, M.; Chouqar, J.; Timmermans, M.; Kaltenegger, L.; Sebastian, D.; Pozuelos, F. J.; Eastman, J. D. (1 August 2024). "TESS discovery of two super-Earths orbiting the M-dwarf stars TOI-6002 and TOI-5713 near the radius valley".Astronomy & Astrophysics.690: A263.arXiv:2408.00709.Bibcode:2024A&A...690A.263G.doi:10.1051/0004-6361/202451120.
^^a ^b ^cBarkaoui, K.; Schwarz, R. P.; Narita, N.; Mistry, P.; Magliano, C.; Hirano, T.; Maity, M.; Burgasser, A. J.; Rackham, B. V. (10 May 2024). "Three short-period Earth-sized planets around M dwarfs discovered by TESS: TOI-5720b, TOI-6008b and TOI-6086b".Astronomy and Astrophysics.687: A264.arXiv:2405.06350.Bibcode:2024A&A...687A.264B.doi:10.1051/0004-6361/202349127.
^"TOI-5723 Overview".NASA Exoplanet Archive.
^"TOI-5731 Overview".NASA Exoplanet Archive.
^"TOI-5975 Overview".NASA Exoplanet Archive.
^^a ^bHotnisky, Andrew; Kanodia, Shubham; Libby-Roberts, Jessica; Mahadevan, Suvrath; Canas, Caleb I.; Gupta, Arvind F.; Han, Te; Kobulnicky, Henry A.; Larsen, Alexander (12 November 2024). "Searching for GEMS: Two Super-Jupiters around M-dwarfs -- Signatures of Instability or Accretion?".arXiv:2411.08159 [astro-ph.EP].
^Bernabò, Lia Marta; Kanodia, Shubham; Canas, Caleb I.; Cochran, William D.; Csizmadia, Szilárd; Mahadevan, Suvrath; Stefánsson, Gudhmundur; Gupta, Arvind F.; Monson, Andrew (25 September 2024)."Searching for GEMS: TOI-6383Ab, a giant planet transiting an M3-dwarf star in a binary system".The Astronomical Journal.168 (6): 273.arXiv:2409.16889.Bibcode:2024AJ....168..273B.doi:10.3847/1538-3881/ad7fe8.
^"TIC 174328045".SIMBAD.Centre de données astronomiques de Strasbourg.
^Baliwal, Sanjay; Sharma, Rishikesh; Chakraborty, Abhijit; Khandelwal, Akanksha; Nikitha, K. J.; Safonov, Boris S.; Strakhov, Ivan A.; Montalto, Marco; Eastman, Jason D. (30 August 2024). "Discovery and characterization of a dense sub-Saturn TOI-6651b".Astronomy & Astrophysics.691: A12.arXiv:2408.17179.Bibcode:2024A&A...691A..12B.doi:10.1051/0004-6361/202450934.
^Saunders, Nicholas; Grunblatt, Samuel K.; Huber, Daniel; Ong, J. M. Joel; Schlaufman, Kevin C.; Hey, Daniel; Li, Yaguang; Butler, R. P.; Crane, Jeffrey D. (14 October 2024)."TESS Giants Transiting Giants. VII. A Hot Saturn Orbiting an Oscillating Red Giant Star".The Astronomical Journal.169 (2): 75.arXiv:2410.11037.Bibcode:2025AJ....169...75S.doi:10.3847/1538-3881/ad9a87.
^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".The Astronomical Journal.168 (2): 66.arXiv:2405.03849.Bibcode:2024AJ....168...66B.doi:10.3847/1538-3881/ad4b16.
^Grieves, N.; Bouchy, F.; Armstrong, D. J.; Akinsanmi, B.; Psaridi, A.; Ulmer-Moll, S.; Frensch, Y. G. C.; Helled, R.; Muller, S. (2025). "Discovery of a cold giant planet and mass measurement of a hot super-Earth in the multi-planetary system WASP-132".Astronomy & Astrophysics.693: A144.arXiv:2406.15986v1.Bibcode:2025A&A...693A.144G.doi:10.1051/0004-6361/202348177.
^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.

Exoplanets

Main topics

Sizes
and
types

Terrestrial	Carbon planet Catastrophically evaporating planet Coreless planet Desert planet Dwarf planet Hycean planet Ice planet Iron planet (Super-Mercury) Lava planet Ocean world Mega-Earth Steam world Sub-Earth Super-Earth
Gaseous	Cold Jupiter Eccentric Jupiter Mini-Neptune (Gas dwarf) Helium planet Hot Jupiter Hot Neptune Gas giant Ice giant Neptunian Jupiter analogue Super-Jupiter Super-Neptune Super-puff Ultra-hot Jupiter Ultra-hot Neptune Warm Jupiter
Other types	Blanet Brown dwarf Chthonian planet Circumbinary planet Circumtriple planet Disrupted planet Double planet Ecumenopolis Eyeball planet Giant planet Mesoplanet Planemo Planet/Brown dwarf boundary Planetesimal Protoplanet Pulsar planet Sub-brown dwarf Sub-Neptune Toroidal planet Ultra-cool dwarf Ultra-short period planet (USP)

Formation
and
evolution

Catalogues

Exoplanetary systems

Exoplanets

Discovered exoplanets by year
- before 2000
- 2000–2009
- 2010
- 2011
- 2012
- 2013
- 2014
- 2015
- 2016
- 2017
- 2018
- 2019
- 2020
- 2021
- 2022
- 2023
- 2024
- 2025

Other

2024 in space

« 2023
2025 »

Space probe launches

Peregrine Mission One (January)
XPoSat
Einstein Probe (January)
DRO A/B (March)
Chang'e 6 (Sample return from lunar far side, May-June)
IM-1 /EagleCam
Queqiao 2 /Tiandu-1 and 2 (March)
Chang'e 6 /ICUBE-Q (May)
Space Variable Objects Monitor (June)
Hera /Milani /Juventas (October)
Europa Clipper (October)
PROBA-3 (December)

Impact events

SelectedNEOs

Discoveries

QSO J0529-4351
1moon of Uranus (S/2023 U 1)
2moons of Neptune (S/2002 N 5,S/2021 N 1)
Gaia BH3
JADES-GS-z14-0
Porphyrion (radio galaxy)
2019 UO14 (First confirmed Saturnian trojan)
Little red dots
- The Cliff
Cheyava Falls

Exoplanets	82 G. Eridani d Barnard's Star b BX Trianguli b Gliese 12 b Gliese 341 b Gliese 900 b HD 48948#Planetary system b c d HD 73344 b c d HD 101581 b c HD 63433 d IRAS 04125+2902 b Kepler-51e LHS 1678 d SPECULOOS-3 b Struve 2398 Ab Teegarden's Star d TOI-6883 b WASP-132d

Comets

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