List of exoplanets discovered in 2024 explained

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 !data-sort-type="number"	Mass !data-sort-type="number"	Radius !data-sort-type="number"	Period (days) !data-sort-type="number"	Semi-major axis (AU) !data-sort-type="number"	Temp. (K) !Discovery method	data-sort-type="number"	Distance (ly) !data-sort-type="number"	Host star mass !data-sort-type="number"	Host star temp. (K) !Remarks	radial vel. FFFF00"	transit FF6CDA"	imaging 0099FF"	microlensing FF7519"	timing 909090"	astrometry 00c9c2"	orbital brightness modulation -->
2MASS J05581644-4501559 b	6–12			1043		imaging	94.5	0.259^[1]	3218
BD-10 47 b	0.0133	0.1529	13.476	0.0943	493	transit	65.89	0.616	4026	Also known as TOI-260 b^[2]
BD-14 3065 b	12.11	1.926	4.3	0.0646	1957	transit	1847.4^[3]	1.4	6985	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^[4]
CI Tauri c	3.6		25.2	0.17		radial vel.	522.6	0.9	4250	Highly eccentric orbit . Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu.^[5] ^[6]
Gaia20eae b	6			0.062		disc thermal instability	9226^[7]	1.15	4330	First object detected by this method^[8]
Gaia22dkvLb	0.15 to 5.67		219 to	0.48 to 2.08		microlensing	3097 to 5477	0.219 to 1.3		^[9]
Gliese 12 b	0.002769	0.0892	12.7	0.066	315	transit	39.65	0.241	3253
Gliese 238 b		0.05049	1.74	0.02123	758	transit	49.6	0.419	3485	Mars-sized exoplanet, one of the smallest exoplanets currently known^[10]
Gliese 341 b	0.00227	0.0821	7.577		540	transit	33.9	0.506	3745	Also known as TOI-741 b^[11]
Gliese 900 b	10.5		500,000,000	12,000		imaging	68^[12]	1.08 (combined)	3976^[13]	Located in a three-star system.^[14] It has the longest orbital time of any exoplanet so far at 1.4 million years.
Gliese 1289 b	0.01655		111.74	0.27	150	radial vel.	28.88	0.21	3296	^[15]
Gliese 4256 b	0.00453	0.0962	0.238	0.0107	1340	transit	66.46	0.353	3421	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^[16]
HD 21520 b	0.02486	0.2409	25.13	0.1726	637	transit	258	1.09	5871	^[17]
HD 48948 b	0.0154		7.34013	0.0652	715	radial vel.	54.915	0.686	4593	^[18]
HD 48948 c	0.0229		37.920	0.1951	413	radial vel.
HD 48948 d	0.0333		150.95	0.4894	262	radial vel.				Closest Super Earth in habitable zone around a K-dwarf star.
HD 63433 d		0.09573	4.21	0.0503	1040	transit	71.7	0.99	5688	^[19]
HD 73344 b	0.00939	0.2573	15.6	0.131	911	transit	114.7	1.2	6220	The dayside temperature can be as high as 1,066K if the planet is tidally locked. Another planet in the system (HD 73344 c) is suspected. The later has a minimum mass of and an orbital period of 66 days.^[20]
HD 75898 c	8.49		6717	7.39		astrometry and radial vel.	263	1.28	6021	^[21]
HD 77946 b	0.02637	0.24133	6.527	0.072	1248	transit	322.7	1.17	6046.0	Also known as TOI-1778 b^[22]
HD 104067 c	0.0415		13.8992	0.1058		radial vel.	66.34	0.82	4952	^[23]
	11.1		5070	6.2	146	radial vel.	300	1.353	5872	^[24]
HD 128717 b	12.8		1089.2	2.18		astrometry	240	1.17	6158	^[25]
HD 134606 e	0.00726		4.32	0.0527		radial vel.	87.4	1.046	5576
HD 134606 f	0.01737		26.915	0.1784		radial vel.	87.4	1.046	5576
HD 148193 Ab	0.0894	0.7476	20.38	0.1577		transit	626	1.261	6351	The host star is orbited by two red dwarfs 157 and 1950 AU away.^[26] Also known as TOI-1836 Ab
HD 148193 Ac	0.025	0.232	1.773	0.03089	2007.6	transit				Also known as TOI-1836 Ac^[27]
HD 156141 b	0.0305	0.211	21.269	0.154	694.1	transit	237.726	1.09	5814	Also known as TOI-1742 b.
HD 278878 b	0.6963	0.9225	8.71	0.08258		transit	520.8	0.989	5597	^[28]
HIP 39017 b	23.6	0.87	30681	22.1		imaging	214.9	1.52	7201^[29]	May be a brown dwarf. Estimates of the mass vary from to .^[30]
HIP 67522 c		0.731	14.335	0.1235	915	transit	414^[31]	1.2	5675	^[32]
HS Piscium b	1.44		3.986	0.0435		radial vel.	122.79	0.69	4203	^[33]
KMT-2016-BLG-2321Lb	3.58			3.58		microlensing	11,670	0.73
KMT-2017-BLG-0849Lb	0.0201			2.73		microlensing	23,540	0.19
KMT-2017-BLG-1057Lb	0.0739			2.36		microlensing	21,190	0.57		^[34]
KMT-2017-BLG-2331Lb	0.538			2.14		microlensing	26,180	0.4
KMT-2020-BLG-0157Lb	10.71			11.54		microlensing	21,744	0.58		^[35]
KMT-2021-BLG-2609Lb	0.032 or 0.112			2.30		microlensing	24,380	0.20		^[36]
KMT-2022-BLG-0303Lb	0.513			4.81		microlensing	21,400	0.368
KMT-2022-BLG-0732Lb	1.12			4.11		microlensing	21,712	0.54
KMT-2022-BLG-1787Lb	6.64			6.3		microlensing	24,613	0.42
KMT-2022-BLG-1852Lb	4.98			5.03		microlensing	20,440	0.32
KMT-2023-BLG-0416Lb	6.15			3.73		microlensing	20,640	0.61		The mass of the planet can be as low as .^[37]
KMT-2023-BLG-0469Lb	0.124			2.37		microlensing	23,050	0.47		^[38]
KMT-2023-BLG-0735Lb	0.12			2.75		microlensing	20,830	0.61
KMT-2023-BLG-1431Lb	0.0428			2.3 or 3.2		microlensing	22,500	0.57		^[39]
KMT-2023-BLG-1454Lb	0.63			1.18		microlensing	23,540	0.17		Estimates of the planet's mass varies between and
KMT-2023-BLG-1642Lb	1.08			1.41		microlensing	22,750	0.17
KMT-2023-BLG-1866Lb	0.00828			2.63		microlensing	20,240	0.51		Super-Earth planet detected by microlensing.^[40]
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.^[41]
LHS 1678 d	0.00289	0.08752	4.965	0.04		transit	65	0.345	3490	^[42]
M62H b	2.83		0.133	0.004908		timing	21,500^[43]	1.4		Pulsar planet located in the globular cluster Messier 62.^[44] Second shortest orbit of any confirmed exoplanet after PSR J1719-1438 b.^[45]
MOA-2016-BLG-526Lb	6.93			2.07		microlensing	22,490	0.4		^[46]
MOA-2022-BLG-563Lb	0.4			2.25		microlensing	21,290	0.48
NGTS-26 b	0.29	1.33	4.52	0.0490	1331	transit	3610	0.96	5550	Highly inflated planet ^[47]
NGTS-27 b	0.593	1.396	3.37	0.0446	1783	transit	3185	1.07	5700
NGTS-29 b	0.393	0.857	69.33	0.347	414	transit	487	1.034	5730	^[48]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	Also known as TOI-4862 b
OGLE-2014-BLG-0221Lb	4.35			3.76		microlensing	12,000	0.69		^[49]
	5.91			2.5		microlensing	19,270	0.55
OGLE-2016-BLG-1800Lb	2.59			1.88		microlensing	21,100	0.41
OGLE-2017-BLG-0640Lb	1.62			1.14		microlensing	21,600	0.32		^[50]
OGLE-2017-BLG-0364Lb	0.0642 to 0.805			1.27		microlensing	22,300 to 29,300	0.1 to 0.55		Assuming the largest distance, it would be the most distant confirmed exoplanet, surpassing SWEEPS-04/11.
OGLE-2017-BLG-1237Lb	3.8			2.53		microlensing	19,660	0.46
OGLE-2017-BLG-1275Lb	5.9			1.19		microlensing	25,070	0.63		Another solution suggests a larger semi-major axis, of .
OGLE-2023-BLG-0836Lb	4.36			3.7		microlensing	16,690			The planet is located in a binary star system, and is likely to be orbiting both stars in the system.^[51]
S1429 b	1.8		77.51	0.384	683	radial vel.	2836	1.26	6000	Located in the open cluster Messier 67.^[52]
SPECULOOS-3 b		0.08716	0.719	0.00733	553	transit	57.9	0.1	2800	Ultra-short period planet^[53]
Teegarden's Star d	0.00258		26.13	0.0791	159	radial vel.	12.5	0.097	3034	Orbits beyond the habitable zone of its star. Another planet in the system is suspected.^[54]
TIC 4672985 b	12.74	1.026	69.05	0.33	517.2	transit	823.4^[55]	1.01	5757
TIC 46432937 b	3.2	1.188	1.44	0.1951	872	transit	295.5	0.563	3572
TIC 139270665 b	0.463	0.645	23.624	0.163	700	transit	618	1.035	5844	^[56] ^[57]
TIC 139270665 c	4.89		1010	2	200	radial vel.
TIC 241249530 b	4.98	1.19	165.772			transit		1.271		A planet on a highly-eccentric and retrograde orbit.^[58]
TIC 393818343 b	4.34	1.087	16.25	0.129	805.5	transit	306.3	1.082	5756	Highly eccentric orbit Also known as TOI-6883 b^[59]
TIC 434398831 b		0.3131	3.6855	0.04641	1250	transit	698	0.992	5638	Young exoplanet located in the Theia 116 association.^[60]
TIC 434398831 c		0.5023	6.21	0.06572	1050	transit
TOI-128 b		0.198	4.94	0.054	1345	transit		0.85	6086	^[61]
TOI-201 b	0.42	1.008	52.978	0.3	759	transit	373	1.316	6394	^[62]
TOI-238 c	0.0211	0.1945	8.466	0.0749	696	transit	261.328	0.79	5059	^[63]
TOI-261 b		0.271	3.36	0.035	1722	transit		0.50	5890
TOI-286 b	0.01425	0.1267	4.512	0.0503	979	transit	193	0.832	5152	There are three available models to explain the disagreement between the radial velocity and transit measurements.
TOI-286 c	0.01171	0.1677	39.36	0.213	475	transit	193	0.832	5152
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 ^[64]
TOI-406 b		0.175	13.18	0.086	344	transit		0.48	3349
TOI-480 b	0.0654		6.866			transit	177.8	1.2	6,212	^[65]
TOI-603 b	0.1495	0.7075	16.18	0.1281		transit	671.3	1.072	5901	^[66]
TOI-654 b		0.211	1.53	0.021	749	transit		0.53	3433
TOI-663 b	0.0140	0.203	2.599	0.0295	674	transit	209.490	0.514	3681	^[67]
TOI-663 c	0.0115	0.202	4.696	0.0437	553	transit
TOI-663 d	<0.0164	0.171	7.103	0.0576	482	transit
TOI-757 b	0.033	0.223	17.468	0.122	641	transit	196.9	0.8	5278	^[68]
TOI-762 Ab	0.251	0.744	3.472	0.03418	555	transit	322	0.442	3266	Located in a binary star system.^[69]
TOI-782 b		0.244	8.024	0.0578	398–435	transit	170.2	0.397	3370
TOI-815 b	0.0239	0.2622	11.197	0.0903	686	transit	193.76	0.776	4869	The host star is part of a binary star system with a red dwarf companion^[70]
TOI-815 c	0.0739	0.2337	34.976	0.193	469	transit
TOI-880 b		0.248	2.57	0.034	1163	transit		0.81	4935
TOI-907 b		0.858	4.58	0.055	1847	transit		1.07	6272
TOI-1135 b	0.062	0.805	5.13	0.082	1198.9	transit	371.4	1.125	6122	^[71]
TOI-1173 Ab	0.08213	0.723	7.064	0.0702	863.9	transit	430.85^[72]	0.911	5350	Low-density planet located in a wide binary system.^[73]
TOI-1184 b	0.021	0.215	5.748	0.056	715.5	transit	191.110	0.73	4616	^[74]
TOI-1199 b	0.239	0.938	3.671	0.04988	1486	transit	805	1.23	5710	^[75]
TOI-1224 b		0.1877	4.178	0.0355	541	transit	121.5	0.4	3326	Located in the MELANGE-5 association, which is old. The host star may be binary.^[76]
TOI-1224 c		0.2573	17.945			transit
TOI-1248 b	0.0862	0.607	4.360	0.051	952.1	transit	550.340	0.90	5205
TOI-1273 b	0.222	0.99	4.631	0.0549	1211	transit	574	1.06	5690
TOI-1279 b	0.0334	0.237	9.61419	0.085	759	transit	349.167	0.88	5457
TOI-1294 b	0.1957	0.8199	3.915	0.0489		transit	1052	1.02	5714	^[77]
TOI-1294 c	0.467		160.1	0.581		radial vel.	1052	1.02	5714	^[78]
TOI-1347 b	0.0349	0.161	0.847		1400	transit	480.8	0.913	5464	Ultra-short period planet^[79]
TOI-1347 c	0.0088	0.143	4.842		1000	transit
TOI-1386 b	0.148	0.54	25.838	0.1732	676.4	transit	478.8	1.038	5793
TOI-1386 c	0.309		227.6	0.739	327.4	radial vel.	478.8	1.038	5793
TOI-1408 c	0.0239	0.1981	2.1664	0.3587		timing	435.6	1.31	6117	^[80]
TOI-1410 b		0.262	1.22	0.020	1396	transit		0.72	4635
TOI-1439 b	0.121	0.379	27.644	0.192	748.4	transit	751.158	1.24	5857	^[81]
TOI-1448 b		0.245	8.112	0.0567	389–426	transit	240	0.372	3412
TOI-1450 Ab	0.00396	0.1	2.04		722	transit	73.2	0.48	3437	Located in a binary star system. It is the second-lowest mass transiting planet with a high-precision mass measurement.
TOI-1450 Ac	0.0048		5.07		533	radial vel.				Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab.
TOI-1451 b	0.0478	0.233	16.538	0.127	723.3	transit	299.856	1.00	5800
TOI-1472 b	0.0519	0.371	6.36381	0.065	811.1	transit	397.389	0.92	5103
TOI-1683 b		0.236	3.06	0.037	929	transit		0.69	4402
TOI-1751 b	0.0538	0.2489	37.468	0.2115	820	transit	370.3	1.15	6116	The host star is metal-poor .^[82]
TOI-1753 b	0.0522	0.221	5.385	0.059	1005.4	transit	739.302	0.95	5620
TOI-1775 b	0.302	0.718	10.241	0.080	707.9	transit	486.736	0.92	5283
TOI-1798 b		0.126	0.44	0.011	2122	transit	369.147	0.86	5165
TOI-1798 c	0.018	0.125	0.438	0.0107	1935.8	transit	369.147	0.86	5165
TOI-1806 b		0.304	15.15	0.088	337	transit		0.39	3272
TOI-1823 b	0.212	0.673	38.80	0.212	423.6	transit	233.677	0.84	4926
TOI-1824 b	0.0582	0.2346	22.8	0.149	577	transit	192.3	0.85	5180	High-density planet, situated in the small group of "overdense sub-Neptunes". TOI-1824 has also a red dwarf companion named TIC 142387022.^[83]
TOI-1828 b	0.1841	0.769	9.09	0.0859		transit	1208	1.04	5809	^[84]
TOI-1855 b	1.133	1.65	1.364	0.02398	1700	transit + radial vel.	576.3	0.987	5359	^[85]
TOI-1885 b	1.624	1.219	6.544060			transit	1826.773		6527
TOI-1898 b	0.4059	0.838	45.52	0.269	674.5	transit	259.7	1.24	6304
TOI-2019 b	0.109	0.505	15.3444			transit	645.812		5590
TOI-2107 b	0.83	1.211	2.454	0.0315	1397	transit + radial vel.	767.4	0.961	5627
TOI-2120 b		0.1893	5.8	0.0377	351–384	transit	104.9	0.211	3131
TOI-2128 b	0.014	0.186	16.341	0.127	780.5	transit	119.2	1.1	5991
TOI-2266 b		0.1374	2.326	0.02	550	transit	168.6	0.23	3240	^[86]
TOI-2368 b	0.65	0.967	5.175	0.05649	1000	transit	685	0.897	5360
TOI-2373 b	9.3	0.93	13.337	0.112	860	transit	1617	1.041	5651	^[87]
TOI-2374 b	0.1782	0.6075	4.314	0.0471		transit	439	0.75	4802	^[88]
TOI-2416 b	3	0.88	8.275	0.0831	1080	transit	1767	1.118	5808
TOI-2420 b	0.927	1.340	5.8426	0.0684	1571.6	transit	1450	1.158		^[89]
TOI-2485 b	2.412	1.083	11.235	0.1093	1134	transit	1296	1.163
TOI-2524 b	0.64	1	7.186	0.073	1100	transit	1399	1.007	5831
TOI-2529 b	2.34	1.03	64.5949	0.327	636	transit	965.8	1.11	5802	^[90]
TOI-3071 b	0.2146	0.6388	1.267	0.0249		transit	1582	1.29	6177
TOI-3261 b	0.0953	0.3408	0.883	0.01714	1722	transit	972.3	0.861	4995	Ultra-hot Neptune^[91]
TOI-3321 b	0.554	1.39	3.652	0.047	1616	transit	928	1.041	5850
TOI-3353 b		0.238	4.67	0.060	1264	transit		1.33	6365
TOI-3894 b	0.85	1.36	4.335	0.0543	1519	transit	1343	1.138	6000
TOI-3919 b	3.88	1.1	7.433	0.0795	1200	transit	1973	1.208	6100
TOI-4153 b	1.15	1.438	4.617	0.06311	1670	transit	1366	1.572	6860
TOI-4336 Ab	0.017	0.1891	16.337	0.0872	308	transit	73.15	0.331	3298	Located in a triple hierarchical stellar system.
TOI-4379 b	1.113	1.489	3.254	9.15		transit	2013	1.372	6020
TOI-4438 b	0.017	0.2248	7.44	0.0534	400	transit	98	0.368	3422	^[92]
TOI-4443 b		0.153	1.85	0.030	1639	transit		1.05	5834
TOI-4495 b		0.324	5.18	0.062	1383	transit		1.17	6156
TOI-4527 b		0.0812	0.40	0.008	1363	transit		0.48	3702
TOI-4602 b		0.227	3.98	0.051	1380	transit		1.12	6012
TOI-4633 c	0.15	0.285	271.94	0.847	290	transit	310.4	1.05 or 1.1	5600 or 5800	Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron.^[93]
TOI-5076 b	0.0503	0.285	23.445		615	transit	270.057	0.80	5070	^[94]
TOI-5082 b		0.227	4.24	0.051	1165	transit		1.00	5670
TOI-5232 b	2.34	1.14	4.097	0.0599	1772	transit	1985	1.389	6500
TOI-5301 b	3.65	1.18	5.859	0.0726	1655	transit	1914	1.483	6240
TOI-5388 b		0.169	2.59	0.024	601	transit		0.29	3495
TOI-5713 b	0.0135	0.1579	10.44	0.06008	347	transit	133.7	0.265	3228
TOI-5720 b	0.0041	0.0972	1.434	0.0183	708	transit	116.9	0.383	3325
TOI-6002 b	0.0119	0.1454	10.905	0.05722	321	transit	104.6	0.21	3241	^[95]
TOI-6008 b	0.00346	0.0919	0.858	0.0108	707	transit	75.05	0.23	3075	Ultra-short period planet
TOI-6029 b	1.635	1.284	5.7987	16.76		transit	1946	1.548	6223	^[96]
TOI-6086 b	0.00346	0.1053	1.389	0.0154	634	transit	102.6	0.254	3200
	6.8		4109			timing	698	0.9		The planet's host star is a polar. The mass value for the planet is only a minimum mass.^[97]
VHS J183135.58-551355.9	6.5	1.42			1085	imaging	180.6			Free-floating planet
Wolf 327 b	0.00796	0.1106	0.573	0.01	996	transit	92.9	0.405	3542	Ultra-short period planet^[98]

Notes

1. Web site: VizieR .
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3. BD-14 3065.
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6. Web site: CI Tau NASA Exoplanet Archive . 2024-03-29 . exoplanetarchive.ipac.caltech.edu.
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12. GJ 900 (ABC)b. 9120.
13. June 18, 2024.
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21. HD 75898 c. 10288. August 1, 2024.
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25. HD 128717 b. 8996.
26. HD 148193 Ab. 9627.
27. TOI-1836 Ac. 10269.
28. TOI-1605 b. 9625.
29. Web site: HIP 39017 NASA Exoplanet Archive . 2024-04-26 . exoplanetarchive.ipac.caltech.edu.
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64. TOI-329 b. 9092. May 28, 2024.
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66. TOI-603 b. 9622.
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77. TOI-1294 b. 9623.
78. TOI-1294 c. 9624.
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84. TOI-1828 b. 9626.
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