List of exoplanets discovered in 2024

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

This list of exoplanets discovered in 2024 is a list of confirmed exoplanets that were first reported in 2024. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name	Mass (MJ)	Radius (RJ)	Period (days)	Semi-major axis (AU)	Temp. (K)	Discovery method	Distance (ly)	Host star mass (M☉)	Host star temp. (K)	Remarks
2MASS J05581644-4501559 b	6–12			1043		imaging	94.5	0.259±0.02 [1]	3218±158 [1]	[2]
BD-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 [3]
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 [4] [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. Also known as TOI-4987 b [5]
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. [6] [7]
Gaia20eae b	6			0.062		disc thermal instability	9226+3130 −2021 [8]	1.15	4330±300 [8]	First object detected by this method [9]
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	[10]
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 [11]
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 [12]
Gliese 900 b	10.5		500,000,000 [13]	12,000		imaging	68 [13]	1.08 (combined)	3976 [14]	Located in a three-star system. [15] It has the longest orbital time of any exoplanet so far at 1.4 million years. [16]
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	Another planet candidate around Gliese 3378 (a similar red dwarf) was reported. [17]
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	[18]
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	[19]
HD 48948 c	0.0229±0.00220		37.920+0.026 −0.024	0.1951±0.0016	413±6	radial vel.				[19]
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. [19]
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 [20]
HD 73344 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 ME and an orbital period of 66 days. [21]
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 [22]
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	[23]
HD 118203 c	11.1+1.3 −1		5070	6.2±0.2	146±3	radial vel.	300±0.5	1.353±0.006	5872±20	[24]
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	[25]
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	[25]
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. [26]
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	[27]
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 [28]	May be a brown dwarf. Estimates of the mass vary from 13.8 MJ to 30+31 −12 MJ. [29]
HIP 67522 c		0.731+0.055 −0.057	14.335	0.1235	915+22 −19	transit	414 [30]	1.2±0.05 [30]	5675±75 [30]	[31]
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	[32]
KMT-2016-BLG-2321Lb	3.58±1.22			3.58±0.81		microlensing	11,670±3980	0.73±0.28		[33]
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		[34]
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		[34]
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		[34]
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		[35]
KMT-2022-BLG-0732Lb	1.12±0.65			4.11+0.74 −1.14		microlensing	21,712+3879 −6000	0.54±0.31		[35]
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		[35]
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		[35]
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 MJ. [36]
KMT-2023-BLG-0469Lb	0.124+0.092 −0.067			2.37±0.9		microlensing	23,050+3260 −3910	0.47±0.36		[37]
KMT-2023-BLG-0735Lb	0.12±0.07			2.75±1		microlensing	20,830+3910 −3260	0.61±0.34		[37]
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		[38]
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 MJ and 0.77+0.87 −0.42 MJ [36]
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		[36]
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. [39]
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. [40]
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	[41]
M62H b	2.83	<0.683 [lower-alpha 3] [lower-alpha 4]	0.133	0.004908		timing	21,500 [42]	1.4		Pulsar planet located in the globular cluster Messier 62. [43] Second shortest orbit of any exoplanet after PSR J1719-1438 b. [44]
MOA-2016-BLG-526Lb	6.93±0.75			2.07±0.35		microlensing	22,490	0.4		[33]
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		[37]
OGLE-2016-BLG-1598Lb	5.91±1.74			2.5±0.88		microlensing	19,270±5670	0.55±0.32		[33]
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) [45]
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	[45]
NGTS-29 b	0.393	0.857	69.33	0.347	414	transit	487±1	1.034±0.032	5730±80	[46]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	Also known as TOI-4862 b [47]
OGLE-2016-BLG-1800Lb	2.59±1.46			1.88±0.51		microlensing	21,100±3360	0.41±0.22		[33]
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		[48]
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		[34] Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassing SWEEPS-04/11. [44]
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		[48]
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. [48]
OGLE-2023-BLG-0836Lb	4.36+2.35 −2.2			3.7+1 −1.2		microlensing	16,690+4430 −5250	[lower-alpha 5]		The planet is located in a binary star system, and is likely to be orbiting both stars in the system. [49]
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. [50]
SPECULOOS-3 b		0.08716	0.719	0.00733	553	transit	57.9	0.1	2800	Ultra-short period planet [51]
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. [52]
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 [53] [lower-alpha 1]	1.01±0.03	5757+72 −65	[54]
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	[55]
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	618	1.035+0.052 −0.062	5844+84 −82	[56] [57]
TIC 139270665 c	4.89+0.66 −0.37		1010+780 −220	2+0.93 −0.31	200+18 −35	radial vel.				[57]
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) [58] Also known as TOI-6883 b [59]
TOI-128 b		0.198	4.94	0.054	1345	transit		0.85	6086	[60]
TOI-201 b	0.42+0.05 −0.03	1.008+0.012 −0.015	52.978	0.3+0.02 −0.03	759+37 −26	transit	373	1.316±0.027	6394±75	[61]
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	[62]
TOI-261 b		0.271	3.36	0.035	1722	transit		0.50	5890	[60]
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. [lower-alpha 6] [3]
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	[3]
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☉) [63]
TOI-406 b		0.175	13.18	0.086	344	transit		0.48	3349	[60]
TOI-480 b	0.0654		6.866			transit	177.8	1.2	6,212	[64]
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	[65]
TOI-654 b		0.211	1.53	0.021	749	transit		0.53	3433	[60]
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	[66]
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-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. [55]
TOI-782 b	<0.06	0.244±0.008	8.024	0.0578±0.0018	398±6–435±6 [lower-alpha 7]	transit	170.2±0.2	0.397±0.01	3370+29 −32	[67]
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 [68]
TOI-815 c	0.0739±0.00755	0.2337+0.0089 −0.008	34.976	0.193±0.004	469±9	transit
TOI-880 b		0.248	2.57	0.034	1163	transit		0.81	4935	[60]
TOI-907 b		0.858	4.58	0.055	1847	transit		1.07	6272	[60]
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	[69]
TOI-1173 Ab	0.08213±0.00598	0.723±0.015	7.064	0.0702±0.0012	863.9±9.8	transit	430.85 [70] [lower-alpha 1]	0.911+0.028 −0.03	5350±340	Low-density planet located in a wide binary system. [71]
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	[72]
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. [73]
TOI-1224 c		0.2573±0.0087	17.945			transit
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	[72]
TOI-1294 b	0.1957±0.016	0.8199±0.0277	3.915	0.0489		transit	1052±7	1.02±0.13	5714±126	[74]
TOI-1294 c	0.467±0.053		160.1±2.5	0.581		radial vel.	1052±7	1.02±0.13	5714±126	[75]
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 [76]
TOI-1347 c	0.0088±0.0072	0.143±0.009	4.842		1000±25	transit				[76]
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	[77]
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	[77]
TOI-1410 b		0.262	1.22	0.020	1396	transit		0.72	4635	[60]
TOI-1448 b	<0.0613	0.245±0.006	8.112	0.0567±0.0015	389±5–426±6 [lower-alpha 7]	transit	240±0.3	0.372±0.009	3412+28 −32	[67]
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. [78]
TOI-1450 Ac	0.0048±0.0006		5.07		533±26	radial vel.				Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab. [78]
TOI-1683 b		0.236	3.06	0.037	929	transit		0.69	4402	[60]
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). [79]
TOI-1798 b		0.126	0.44	0.011	2122	transit		0.86	5165	[60]
TOI-1806 b		0.304	15.15	0.088	337	transit		0.39	3272	[60]
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. [80]
TOI-1828 b	0.1841±0.012	0.769±0.017	9.09	0.0859		transit	1208±8	1.04±0.13	5809±127	[81]
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	[82]
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	[82]
TOI-2120 b	<0.02139	0.1893±0.0056	5.8	0.0377±0.0013	351±6–384±6 [lower-alpha 7]	transit	104.9	0.211±0.005	3131±30	[67]
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	[83]
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	[82]
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	[84]
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	[85]
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	[84]
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	[84]
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	[54]
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	[85]
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 [86]
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	[82]
TOI-3353 b		0.238	4.67	0.060	1264	transit		1.33	6365	[60]
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	[82]
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	[82]
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	[82]
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. [87]
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	[88]
TOI-4443 b		0.153	1.85	0.030	1639	transit		1.05	5834	[60]
TOI-4495 b		0.324	5.18	0.062	1383	transit		1.17	6156	[60]
TOI-4527 b		0.0812	0.40	0.008	1363	transit		0.48	3702	[60]
TOI-4602 b		0.227	3.98	0.051	1380	transit		1.12	6012	[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 8]	5600±50 or 5800±50 [lower-alpha 8]	Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron. [89]
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	[90]
TOI-5082 b		0.227	4.24	0.051	1165	transit		1.00	5670	[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	[82]
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	[82]
TOI-5388 b		0.169	2.59	0.024	601	transit		0.29	3495	[60]
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	[91]
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 [91]
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	[91]
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. [92]
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 [93]
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 [94]

Specific exoplanet lists

Lists of exoplanets

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

Lists of exoplanets by year of discovery

• List of exoplanets discovered before 2000 (31)
• List of exoplanets discovered between 2000–2009 (377)
• List of exoplanets discovered in 2010 (109)
• List of exoplanets discovered in 2011 (178)
• List of exoplanets discovered in 2012 (149)
• List of exoplanets discovered in 2013 (151)
• List of exoplanets discovered in 2014 (870)
• List of exoplanets discovered in 2015 (150)
• List of exoplanets discovered in 2016 (1497)
• List of exoplanets discovered in 2017 (158)
• List of exoplanets discovered in 2018 (305)
• List of exoplanets discovered in 2019 (172)
• List of exoplanets discovered in 2020 (253)
• List of exoplanets discovered in 2021 (257)
• List of exoplanets discovered in 2022 (313)
• List of exoplanets discovered in 2023 (298)
• List of exoplanets discovered in 2024 (142)

Notes

1. Distance calculated from parallax
2. The radius is the same as that of the Earth, with an uncertainty of 10%
3. Radius calculated with mass and lower limit in density in the equation d=(1.89813*10^(30)*m)/((4/3)*π*r³), where d is density (in g/cm³), m is the mass (in M_J and r is the radius (in centimeters). Should be divided by 7.1492×10⁹ to convert from centimeters to R_J
4. Since the density is only a lower limit, the radius is an upper limit.
5. The planet is located in a two-star system, with masses of 0.78+0.38
   −0.36 M_☉ and 0.56+0.3
   −0.28 M_☉. There is a large chance that it is orbiting both stars in the system, so the "host star mass" would be 0.78+0.38
   −0.36 M_☉ + 0.56+0.3
   −0.28 M_☉. However, there is a small chance that is orbiting only one of the stars in the system.
6. The transit observations of TOI-286 indicate periodic transit signals of 4.5 abd 39.4 days. While this, radial velocity measurements with ESPRESSO do not immediately show evidence for periodic signals at either periods.
7. Assuming albedos of 0.3 and 0 respectively.
8. It is not known which of the stars the planet orbits.

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