List of exoplanets discovered in 2024

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 (`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, after Alpha Centauri.^[6] Not to be confused with the disproved planet Barnard'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	0.51±0.02 (combined)	3735±100	^[11]
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.^[12]^[13]
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	^[14]
Gaia20eae b	6			0.062		disk thermal instability	9226⁺³¹³⁰ ₋₂₀₂₁^[15]	1.15	4330±300^[15]	First object detected by this method^[16]
Gaia22dkvLb	0.15 to 5.67^+0.39 _−0.38		219⁺⁴⁷ ₋₂₉ to 964+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		^[17]
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	^[18]
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^[19]
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^[20]
Gliese 900 b	10.5		460,000,000^[21]	12,000		imaging	68^[22]	1.08 (combined)	3976^[23]	Located in a three-star system.^[24] It has the longest orbital time of any exoplanet so far at 1.4 million years.^[25]
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	0.0107^[c]	1340±60	transit	66.46±0.03	0.353±0.015	3421±70	An ultra-short period planet orbiting close to the host star's Roche limit. It is expected to undergo tidal disruption in the next hundred million years. Also known as TOI-6255 b^[27]
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	^[28]
HD 28185 c	6.0±0.6		9088.5^+474.5 _−401.5	8.50^+0.29 _−0.26		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.^[29]
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	^[30]
HD 48948 c	0.0229±0.00220		37.920^+0.026 _−0.024	0.1951±0.0016	413±6	radial vel.				^[30]
HD 48948 d	0.0333±0.00315		150.95^+0.45 _−0.41	0.4894±0.0042	262±4	radial vel.				Closest Super Earth in habitable zone around a K-dwarf star.^[30]
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^[31]
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^[32]	1.20±0.02^[32]	6028±110^[32]	The dayside temperature can be as high as 1,066 K if the planet is tidally locked.^[33]
HD 73344 c	0.367^+0.022 _−0.021		65.936	0.3388^+0.0042 _−0.0043	562±4^[33]	radial vel.				^[32]
HD 73344 d	2.55^+0.56 _−0.46		5746⁺¹²⁰ ₋₁₅₀	6.70^+0.25 _−0.26		radial vel.				True mass revealed using astrometry.^[32]
HD 75898 c	8.49±0.65		6717±40	7.39±0.05		astrometry + radial vel.	263	1.28±0.13	6021±50	^[34]
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^[35]
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	^[36]
HD 111520 b	≥1		1,285,900	≥200		disk kinematics	352.6±0.7	1.350±0.215^[37]	6542±131^[37]	^[38]
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	^[39]
HD 128717 b	12.8		1089.2	2.18		astrometry	240±0.5	1.17^+0.06 _−0.16	6158±115	^[40]^[41]
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	^[42]
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	^[42]
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.^[43] 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^[44]
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.^[45]
HD 222237 b	5.19±0.58		14,890⁺²¹²⁰ ₋₁₆₄₃	10.8^+1.1 _−1.0		astrometry	37.31±0.0	0.76±0.09	4751±139	^[46]
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	^[47]
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^[48]	May be a brown dwarf. Estimates of the mass vary from 13.8 M_J to 30+31 −12 M_J.^[49]
HIP 67522 c		0.731^+0.055 _−0.057	14.335	0.1235	915⁺²² ₋₁₉	transit	414^[50]	1.2±0.05^[50]	5675±75^[50]	^[51]
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	^[52]
IRAS 04125+2902 b	0.3	0.955	8.83			transit	520^[53]	0.7	3720^[54]	^[55] The youngest transiting exoplanet discovered to date.^[56]
Kepler-51e	0.01572		260			timing	2610±50	1.04	6018	Assuming the 2:1 resonance solution, which is the best-fit one, Kepler-51e has a mass of about 5 `M`_E and a period of 260 days.^[57]
Kepler-158d		0.038±0.004	0.645088±0.000002			transit	1028±7	0.656^+0.073 _−0.049	4895.97	^[58]
Kepler-879c		0.04±0.01	0.646716±0.000003			transit	2618⁺³⁶ ₋₃₅	0.974^+0.127 _−0.104	5456.75	^[58]
Kepler-963c		0.05±0.02	0.919783±0.000003			transit	2516⁺⁴² ₋₄₀	0.821^+0.120 _−0.065	5169.47	^[58]
Kepler-1489c		0.045±0.007	0.680741±0.000004			transit	4185⁺¹¹⁸ ₋₁₁₁	0.977^+0.050 _−0.062	5565.53	^[58]
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.^[58]
K2-360 b	0.02413±0.00236	0.01435±0.00072	0.87724±0.00004	0.0177±0.0003	2038±39	transit	762.59±19.05	0.958±0.048	5679⁺⁶⁰ ₋₃₉	Ultra-dense super-Earth.^[59]
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	^[59]
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	^[60]
KMT-2016-BLG-2321Lb	3.58±1.22			3.58±0.81		microlensing	11,670±3980	0.73±0.28		^[61]
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		^[62]
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		^[62]
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		^[62]
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		^[63]
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		^[64]
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		^[64]
KMT-2022-BLG-0732Lb	1.12±0.65			4.11^+0.74 _−1.14		microlensing	21,712⁺³⁸⁷⁹ ₋₆₀₀₀	0.54±0.31		^[63]
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		^[63]
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		^[63]
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 as 0.042+0.021 −0.022 M_J.^[65]
KMT-2023-BLG-0469Lb	0.124^+0.092 _−0.067			2.37±0.9		microlensing	23,050⁺³²⁶⁰ ₋₃₉₁₀	0.47±0.36		^[66]
KMT-2023-BLG-0735Lb	0.12±0.07			2.75±1		microlensing	20,830⁺³⁹¹⁰ ₋₃₂₆₀	0.61±0.34		^[66]
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		^[67]
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 between 0.3+0.34 −0.16 M_J and 0.77+0.87 −0.42 M_J^[65]
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		^[65]
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.^[68]
KMT-2023-BLG-2669	0.02517					microlensing				Candidate rogue planet. Might have a mass ranging from sub-Neptune to Saturn-mass, depending on its distance.^[69]
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 a brown dwarf or a red dwarf.^[70]
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	^[71]
M62H b	2.83	<0.683 ^[d]^[e]	0.133	0.004908		timing	21,500^[72]	1.4		Pulsar planet located in the globular cluster Messier 62.^[73] Second shortest orbit of any confirmed exoplanet after PSR J1719-1438 b.^[74]
MOA-2016-BLG-526Lb	6.93±0.75			2.07±0.35		microlensing	22,490	0.4		^[61]
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		^[66]
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)^[75]
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	^[75]
NGTS-29 b	0.393	0.857	69.33	0.347	414	transit	487±1	1.034±0.032	5730±80	^[76]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	Also known as TOI-4862 b^[77]
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	^[78]
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		^[79]
OGLE-2016-BLG-1598Lb	5.91±1.74			2.5±0.88		microlensing	19,270±5670	0.55±0.32		^[61]
OGLE-2016-BLG-1800Lb	2.59±1.46			1.88±0.51		microlensing	21,100±3360	0.41±0.22		^[61]
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		^[62] Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassing SWEEPS-04/11.^[74]
OGLE-2017-BLG-0380Lb A	10.5					microlensing	6,980			A pair of rogue planets.^[80]
OGLE-2017-BLG-0380Lb B	3.08					microlensing	6,980			A pair of rogue planets.^[80]
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		^[81]
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		^[81]
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, of 2.09±0.63 AU.^[81]
OGLE-2023-BLG-0836Lb	4.36^+2.35 _−2.2			3.7⁺¹ _−1.2		microlensing	16,690⁺⁴⁴³⁰ ₋₅₂₅₀	^[f]		The planet is located in a binary star system, and is likely to be orbiting both stars in the system.^[82]
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 cluster Messier 67.^[83]
SGR 1935+2154 b	0.0318 – 0.0573	0.125 – 0.223	238 or 398	0.85 or 1.19		x-ray bursts	21,500^[84]–28,400	1.4		Has a highly-eccentric orbit (0.992) and is tidally disrupted.^[85]
SPECULOOS-3 b		0.08716	0.719	0.00733	553	transit	57.9	0.1	2800	Ultra-short period planet^[86]
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	^[87]
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.^[88]
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^[89]^[a]	1.01±0.03	5757⁺⁷² ₋₆₅	^[90]
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	^[91]
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	618	1.035^+0.052 _−0.062	5844⁺⁸⁴ ₋₈₂	^[92]^[93]
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	^[93]
TIC 241249530 b	4.98^+0.16 _−0.18	1.19±0.04	165.772			transit		1.271^+0.061 _−0.068		A planet on a highly-eccentric (e=0.94) and retrograde orbit.^[94]
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)^[95] Also known as TOI-6883 b^[96]
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	^[97]
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 116 association.^[98]
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 116 association.^[98]
TOI-128 b		0.198	4.94	0.054	1345	transit		0.85	6086	^[99]
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	^[100]
TOI-261 b		0.271	3.36	0.035	1722	transit		0.50	5890	^[99]
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.^[g]^[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`_☉)^[101]
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	^[102]
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	^[102]
TOI-480 b	0.0654		6.866			transit	177.8	1.2	6,212	^[103]
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	^[104]
TOI-654 b		0.211	1.53	0.021	749	transit		0.53	3433	^[99]
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	^[105]
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-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	^[106]
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.^[91]
TOI-782 b	<0.06	0.244±0.008	8.024	0.0578±0.0018	398±6–435±6^[h]	transit	170.2±0.2	0.397±0.01	3370⁺²⁹ ₋₃₂	^[107]
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^[108]
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		0.81	4935	^[99]
TOI-907 b		0.858	4.58	0.055	1847	transit		1.07	6272	^[99]
TOI-1011 b	0.01271±0.00186	0.1294±0.0045	2.47	0.0346		transit		0.92±0.03	5475±84	^[109]
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	^[110]
TOI-1173 Ab	0.08213±0.00598	0.723±0.015	7.064	0.0702±0.0012	863.9±9.8	transit	430.85^[111]^[a]	0.911^+0.028 _−0.03	5350±340	Low-density planet located in a wide binary system.^[112]
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	^[45]
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	^[113]
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 the MELANGE-5 association, which is 200 Myr old. The host star may be binary.^[114]
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	^[45]
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	^[115]
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	^[116]
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	^[117]
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	^[113]
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	^[45]
TOI-1294 b	0.1957±0.016	0.8199±0.0277	3.915	0.0489		transit	1052±7	1.02±0.13	5714±126	^[118]
TOI-1294 c	0.467±0.053		160.1±2.5	0.581		radial vel.	1052±7	1.02±0.13	5714±126	^[119]
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^[120]
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	^[120]
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	^[121]
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	^[121]
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	^[122]
TOI-1410 b		0.262	1.22	0.020	1396	transit		0.72	4635	^[99]
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^[123]	transit + radial vel.	336	1.10±0.10	6008±113	^[124]
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	^[125]
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	^[126]
TOI-1448 b	<0.0613	0.245±0.006	8.112	0.0567±0.0015	389±5–426±6^[h]	transit	240±0.3	0.372±0.009	3412⁺²⁸ ₋₃₂	^[107]
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.^[127]
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 assuming coplanarity with TOI-1450 Ab.^[127]
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	^[45]
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	^[45]
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	^[128]
TOI-1683 b		0.236	3.06	0.037	929	transit		0.69	4402	^[99]
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	^[129]
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	^[130]
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 is metal-poor ([Fe/H] = –0.40 dex).^[131]
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	^[45]
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	^[132]
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	^[45]
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	^[133]
TOI-1798 b		0.126	0.44	0.011	2122	transit	369.147^+1.008 _−1.005	0.86	5165	^[99]
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	^[45]
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	^[134]
TOI-1806 b		0.304	15.15	0.088	337	transit		0.39	3272	^[99]
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	^[45]
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.^[135]
TOI-1828 b	0.1841±0.012	0.769±0.017	9.09	0.0859		transit	1208±8	1.04±0.13	5809±127	^[136]
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	^[137]
TOI-1883 b		0.4953±0.0460	4.506		524.9	transit	376±3	0.492±0.02	3477±157	^[138]^[139]
TOI-1885 b	1.624±0.103	1.219±0.037	6.544060±0.000006			transit	1826.773^+21.464 _−20.982		6527±98	^[125]
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	^[140]
TOI-2019 b	0.109±0.0132	0.505±0.0250	15.3444±0.0055			transit	645.812^+2.684 _−2.665		5590	^[125]
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	^[137]
TOI-2120 b	<0.02139	0.1893±0.0056	5.8	0.0377±0.0013	351±6–384±6^[h]	transit	104.9	0.211±0.005	3131±30	^[107]
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	^[141]
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	^[142]
TOI-2274 b			2.679		771	transit	159.9±0.2	0.612±0.02	3943±157	^[143]^[139]
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	^[137]
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	^[144]
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	^[145]
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	^[146]
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	^[146]
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	^[144]
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		^[147]
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		^[147]
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	^[144]
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	^[90]
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	^[148]
TOI-2768 b		0.2688±0.0313	1.508		855	transit	255.8±0.6	0.63^+0.06 _−0.10	4008⁺¹²⁴ ₋₁₃₇	^[149]^[139]
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	^[148]
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	^[145]
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^[150]
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	^[137]
TOI-3353 b		0.238	4.67	0.060	1264	transit		1.33	6365	^[99]
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	^[151]
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	^[137]
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	^[137]
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	^[137]
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.^[152]
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 the Hyades.^[153]
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	^[154]
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	^[155]
TOI-4443 b		0.153	1.85	0.030	1639	transit		1.05	5834	^[99]
TOI-4495 b		0.324	5.18	0.062	1383	transit		1.17	6156	^[99]
TOI-4527 b		0.0812	0.40	0.008	1363	transit		0.48	3702	^[99]
TOI-4562 c	5.77^+0.37 _−0.56		3990⁺²⁰¹ ₋₁₉₂	5.219±0.002		timing	1131±12^[156]	1.218^+0.054 _−0.048^[156]	6096±32^[156]	^[157]
TOI-4602 b		0.227	3.98	0.051	1380	transit		1.12	6012	^[99]
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^[i]	5600±50 or 5800±50 ^[i]	Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron.^[158]
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	^[148]
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	^[159]
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	^[160]
TOI-5082 b		0.227	4.24	0.051	1165	transit		1.00	5670	^[99]
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	^[60]
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	^[137]
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	^[137]
TOI-5319 b		0.33427±0.0551	4.079		695	transit	199.4±0.7	0.5±0.1	3580⁺¹⁰⁷ ₋₁₄₁	^[161]^[139]
TOI-5388 b		0.169	2.59	0.024	601	transit		0.29	3495	^[99]
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	^[60]
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	^[60]
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	^[162]
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	^[163]
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	^[164]
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	^[163]
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^[164]
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	^[154]
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	^[60]
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	^[164]
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	^[165]
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^[166]^[a]	1.323^+0.050 _−0.045	5940±110	^[167]
TOI-7041 b	0.36±0.16	1.02±0.03	9.691±0.006			transit	1431±10	1.12±0.02	4640±10	^[168]
V808 Aurigae b [ru]	6.8±0.7		4109±362			timing	698±13	0.9±0.1		The planet's host star is a polar. The mass value for the planet is only a minimum mass.^[169]
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^[170]
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	^[171]
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^[172]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

List of exoplanets discovered before 2000 (31)
List of exoplanets discovered between 2000–2009 (377)
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 (151)
List of exoplanets discovered in 2014 (870)
List of exoplanets discovered in 2015 (149)
List of exoplanets discovered in 2016 (1497)
List of exoplanets discovered in 2017 (158)
List of exoplanets discovered in 2018 (303)
List of exoplanets discovered in 2019 (172)
List of exoplanets discovered in 2020 (249)
List of exoplanets discovered in 2021 (257)
List of exoplanets discovered in 2022 (313)
List of exoplanets discovered in 2023 (307)
List of exoplanets discovered in 2024 (239)

Notes

^ ^a ^b ^c ^d ^e ^f ^g ^h Distance calculated from parallax
^ The radius is the same as that of the Earth, with an uncertainty of 10%
^ Calculated using a/R⋆ (ratio between Semi-major axis and host star radius)
^ 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
^ 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 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.
^ 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 ^c Assuming albedos of 0.3 and 0 respectively.
^ ^a ^b It is not known which of the stars the planet orbits.

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[distp-10] ^ ^a ^b ^c ^d ^e ^f ^g ^h Distance calculated from parallax

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

[a-r0-29] Calculated using a/R⋆ (ratio between Semi-major axis and host star radius)

[Radius1-75] 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

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

[87] 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.

[107] 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.

[Albedo1-114] Assuming albedos of 0.3 and 0 respectively.

[A-166] It is not known which of the stars the planet orbits.

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[:15-4] "VizieR".

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