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 -->
20 Leonis Minoris b	0.02882		31.15	0.1916		radial vel.	48.64	0.967	5610
82 G. Eridani d	0.01831		647.6	1.354		radial vel.	19.7	0.813	5490	Orbiting within the habitable zone of its host star.^[1] ^[2]
2MASS J05581644–4501559 b	6–12			1043		imaging	94.5	0.259^[3]	3218
Barnard's Star b	0.00116		3.153	0.0229	~400	radial vel.	5.9629	0.162	3195	The closest exoplanet around a solitary star. Also located in the second closest star system to the Sun, after Alpha Centauri.^[4] Not to be confused with the disproved planet Barnard's Star b of 2018, which shared the same name.
BD+00 444b	0.0151	0.2108	15.669	0.105	519	transit	77.99	0.642	4375	^[5]
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^[6]
BD-14 3065 b	12.11	1.926	4.3	0.0646	3520	transit	1847.4^[7]	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^[8]
BX Trianguli b	7.5		3923	4.5		timing	192	0.51 (combined)	3735	^[9]
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.^[10] ^[11]
CWISE J054129.32–745021.5 b	1.8			6576		imaging	111			Orbits a young red dwarf.
Gaia-4 b	11.8		571.3			astrometry + radial vel.	239.2	0.644	4034
Gaia20eae b	6			0.062		disk thermal instability	9226^[12]	1.15	4330	First object detected by this method^[13]
Gaia22dkvLb	0.15 to 5.67		219 to	0.48 to 2.08		microlensing	3097 to 5477	0.219 to 1.3		^[14]
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^[15]
Gliese 341 b	0.00227	0.0821	7.577		540	transit	33.9	0.506	3745	Also known as TOI-741 b^[16]
Gliese 900 b	10.5		460,000,000^[17]	12,000		imaging	68^[18]	1.08 (combined)	3976^[19]	Located in a three-star system.^[20] 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	^[21]
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^[22]
HD 21520 b	0.02486	0.2409	25.13	0.1726	637	transit	258	1.09	5871	^[23]
HD 28185 c	6.0		9088.5	8.50		astrometry + radial vel.	127.8	0.974	5602	Already known to exist in 2022, but was found to be an exoplanetas opposed to a brown dwarf, in 2024.^[24]
HD 48948 b	0.0154		7.34013	0.0652	715	radial vel.	54.915	0.686	4593	^[25]
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	^[26]
HD 73344 b	0.00939	0.2573	15.6	0.131	911	transit	114.7	1.20	6028	The dayside temperature can be as high as 1,066K if the planet is tidally locked.^[27]
HD 73344 c	0.367		65.936	0.3388	562	radial vel.				^[28]
HD 73344 d	2.55		5746	6.70		radial vel.				True mass revealed using astrometry.
HD 75898 c	8.49		6717	7.39		astrometry + radial vel.	263	1.28	6021	^[29]
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^[30]
HD 104067 c	0.0415		13.8992	0.1058		radial vel.	66.34	0.82	4952	^[31]
HD 111520 b			1,285,900			disk kinematics	352.6	1.350^[32]	6542
	11.1		5070	6.2	146	astrometry + radial vel.	300	1.353	5872	^[33]
HD 128717 b	12.8		1089.2	2.18		astrometry	240	1.17	6158	^[34]
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.^[35] Also known as TOI-1836 Ab
HD 148193 Ac	0.025	0.232	1.773	0.03089	2007.6	transit	626	1.261	6351	Also known as TOI-1836 Ac^[36]
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 222237 b	5.19		14,890	10.8		astrometry	37.31	0.76	4751	^[37]
HD 278878 b	0.6963	0.9225	8.71	0.08258		transit	520.8	0.989	5597	^[38]
HIP 39017 b	23.6	0.87	30681	22.1		imaging	214.9	1.52	7201^[39]	May be a brown dwarf. Estimates of the mass vary from to .^[40]
HIP 67522 c		0.731	14.335	0.1235	915	transit	414^[41]	1.2	5675	^[42]
HS Piscium b	1.44		3.986	0.0435		radial vel.	122.79	0.69	4203	^[43]
IRAS 04125+2902 b	0.3	0.955	8.83			transit	520^[44]	0.7	3720^[45]	^[46] The youngest transiting exoplanet discovered to date.^[47]
Kepler-51e	0.01572		260			timing	2610	1.04	6018	Assuming the 2:1 resonance solution, which is the best-fit one, Kepler-51e has a mass of about 5 and a period of 260 days.^[48]
Kepler-158d		0.038	0.645088			transit	1028	0.656	4895.97	^[49]
Kepler-879c		0.04	0.646716			transit	2618	0.974	5456.75
Kepler-963c		0.05	0.919783			transit	2516	0.821	5169.47
Kepler-1489c		0.045	0.680741			transit	4185	0.977	5565.53
Kepler-2003b		0.06	0.941967			transit	3054	0.859	5050.28	Also known as KOI-4978 b.
K2-360 b	0.02413	0.01435	0.87724	0.0177	2038	transit	762.59	0.958	5679	Ultra-dense super-Earth.^[50]
K2-360 c	0.0479		9.797	0.0883	912	radial vel.	762.59	0.958	5679
K2-419 Ab	0.617	0.941	20.358	0.1208	377	transit	860	0.562	3711
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		^[51]
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		^[52]
KMT-2021-BLG-2609Lb	0.032 or 0.112			2.30		microlensing	24,380	0.20		^[53]
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 .^[54]
KMT-2023-BLG-0469Lb	0.124			2.37		microlensing	23,050	0.47		^[55]
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		^[56]
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.^[57]
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.^[58]
KMT-2024-BLG-1044L	0.0244 or 0.0430					microlensing	21,900 or 23,300	0.069 or 0.131		Host star is either a brown dwarf or a red dwarf.^[59]
LHS 1678 d	0.00289	0.08752	4.965	0.04		transit	65	0.345	3490	^[60]
M62H b	2.83		0.133	0.004908		timing	21,500^[61]	1.4		Pulsar planet located in the globular cluster Messier 62.^[62] Second shortest orbit of any confirmed exoplanet after PSR J1719-1438 b.^[63]
MOA-2016-BLG-526Lb	6.93			2.07		microlensing	22,490	0.4		^[64]
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 ^[65]
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	^[66]
NGTS-30 b	0.96	0.93	98.3	0.408	390	transit	762.5	0.94	5455	Also known as TOI-4862 b
NGTS-33 b	3.6	1.64	2.828	0.048	1991	transit	1430	1.60	7437
OGLE-2014-BLG-0221Lb	4.35			3.76		microlensing	12,000	0.69		^[67]
	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-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-0380Lb A	10.5					microlensing	6,980			A pair of rogue planets.^[68]
OGLE-2017-BLG-0380Lb B	3.08					microlensing	6,980			A pair of rogue planets.^[68]
OGLE-2017-BLG-0640Lb	1.62			1.14		microlensing	21,600	0.32		^[69]
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.^[70]
S1429 b	1.8		77.51	0.384	683	radial vel.	2836	1.26	6000	Located in the open cluster Messier 67.^[71]
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^[72] –28,400	1.4		Has a highly-eccentric orbit (0.992) and is tidally disrupted.^[73]
SPECULOOS-3 b		0.08716	0.719	0.00733	553	transit	57.9	0.1	2800	Ultra-short period planet^[74]
Struve 2398 Ab	0.00875	0.107–0.178	11.2201	0.068		radial vel.	11.4	0.330	3470	^[75]
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.^[76]
TIC 4672985 b	12.74	1.026	69.05	0.33	517.2	transit	823.4^[77]	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	^[78] ^[79]
TIC 139270665 c	4.89		1010	2	200	radial vel.	618	1.035	5844
TIC 241249530 b	4.98	1.19	165.772			transit		1.271		A planet on a highly-eccentric and retrograde orbit.^[80]
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^[81]
TIC 393818343 c	0.357	0.792	7.8458	0.079	1027.2089	transit	306.3	1.082	5756	^[82]
TIC 434398831 b		0.3131	3.6855	0.04641	1250	transit	698	0.992	5638	Young exoplanet located in the Theia 116 association.^[83]
TIC 434398831 c		0.5023	6.21	0.06572	1050	transit	698	0.992	5638	Young exoplanet located in the Theia 116 association.^[83]
TOI-128 b		0.198	4.94	0.054	1345	transit		0.85	6086	^[84]
TOI-238 c	0.0211	0.1945	8.466	0.0749	696	transit	261.328	0.79	5059	^[85]
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 ^[86]
TOI-406 b	0.00654	0.1178	3.307	0.0322	584	transit	101	0.408	3392	^[87]
TOI-406 c	0.02067	0.1846	13.18	0.0809	368	transit	101	0.408	3392
TOI-480 b	0.0654		6.866			transit	177.8	1.2	6,212	^[88]
TOI-603 b	0.1495	0.7075	16.18	0.1281		transit	671.3	1.072	5901	^[89]
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	^[90]
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	^[91]
TOI-762 Ab	0.251	0.744	3.472	0.03418	555	transit	322	0.442	3266	Located in a binary star system.^[92]
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^[93]
TOI-815 c	0.0739	0.2337	34.976	0.193	469	transit	193.76	0.776	4869
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-1011 b	0.01271	0.1294	2.47	0.0346		transit		0.92	5475
TOI-1135 b	0.062	0.805	5.13	0.082	1198.9	transit	371.4	1.125	6122	^[94]
TOI-1173 Ab	0.08213	0.723	7.064	0.0702	863.9	transit	430.85^[95]	0.911	5350	Low-density planet located in a wide binary system.^[96]
TOI-1184 b	0.021	0.215	5.748	0.056	715.5	transit	191.110	0.73	4616	^[97]
TOI-1199 b	0.239	0.938	3.671	0.04988	1486	transit	805	1.23	5710	^[98]
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.^[99]
TOI-1224 c		0.2573	17.945			transit	121.5	0.4	3326
TOI-1248 b	0.0862	0.607	4.360	0.051	952.1	transit	550.340	0.90	5205
TOI-1249 b	0.0374	0.2918	13.079	0.109	727	transit	455.0	0.952	5453
TOI-1266 d	0.01158		32.5	0.1513	288	radial vel. + timing	117.4	0.437	3563	^[100]
TOI-1269 b	0.020	0.2142	4.253	0.0496	1005	transit	561.4	0.969	5517
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	^[101]
TOI-1294 c	0.467		160.1	0.581		radial vel.	1052	1.02	5714	^[102]
TOI-1347 b	0.0349	0.161	0.847		1400	transit	480.8	0.913	5464	Ultra-short period planet^[103]
TOI-1347 c	0.0088	0.143	4.842		1000	transit	480.8	0.913	5464
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	^[104]
TOI-1410 b		0.262	1.22	0.020	1396	transit		0.72	4635
TOI-1437 b	0.0302	0.200	18.841	0.140	794	transit + radial vel.	336	1.10	6008	^[105]
TOI-1439 b	0.121	0.379	27.644	0.192	748.4	transit	751.158	1.24	5857	^[106]
TOI-1443 b	<0.0944	0.2055	23.541	0.147	521	transit	279.9	0.89	5236
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.	73.2	0.48	3437	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-1669 b	<0.0409	0.2049	2.68	0.0376	1285	transit	362.9	1.00	5542
TOI-1683 b		0.236	3.06	0.037	929	transit		0.69	4402
TOI-1691 b	0.0459	0.3181	16.737	0.126	703	transit	363.5	1.031	5759
TOI-1723 b		0.2937	13.72641	0.114	783	transit	328.5	1.035	5777
TOI-1751 b	0.0538	0.2489	37.468	0.2115	820	transit	370.3	1.15	6116	The host star is metal-poor .^[107]
TOI-1753 b	0.0522	0.221	5.385	0.059	1005.4	transit	739.302	0.95	5620
TOI-1758 b		0.3174	20.705	0.138	551	transit	315.1	0.88	5169
TOI-1775 b	0.302	0.718	10.241	0.080	707.9	transit	486.736	0.92	5283
TOI-1776 b		0.1085	2.8	0.0378	1269	transit	146	1.02	5724
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-1799 b	0.013	0.1269	7.085738	0.071	923	transit[\|203 \|1.01{{+-\|0.14\|0.12}} \|5690{{+-\|121\|124}} \|<ref>{{cite Exoplanet Archive\|TOI-1799}}</ref> \|- \|TOI-1806 b \| \|0.304 \|15.15 \|0.088 \|337 \| style="background:#FFFF00"\|transit \| \|0.39 \|3272 \|<ref name=":21"/> \|- \|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}} \| style="background:#FFFF00"\|transit \|233.677{{±\|0.375\|0.374}} \|0.84{{±\|0.03}} \|4926{{±\|113}} \|<ref name=":26"/> \|- \|[[TOI-1824 b]]\|0.0582\|0.2346\|22.8\|0.149\|577\|style="background:#FFFF00" \|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.^[108] \|-\|TOI-1828 b\|0.1841\|0.769\|9.09\|0.0859\|\|style="background:#FFFF00"\|transit\|1208\|1.04\|5809\|^[109] \|-\|TOI-1855 b\|1.133\|1.65\|1.364\|0.02398\|1700\| style="background:#FFFF00"\|transit + radial vel.\|576.3\|0.987\|5359\|^[110] \|-\|TOI-1883 b\|\|0.4953\|4.506\|\|524.9\|style="background:#FFFF00"\|transit\|376\|0.492\|3477\|^[111] \|-\|TOI-1885 b\|1.624\|1.219\|6.544060\|\|\|style="background:#FFFF00"\|transit\|1826.773\|\|6527\|\|-\|TOI-1898 b\|0.4059\|0.838\|45.52\|0.269\|674.5\|style="background:#FFFF00"\|transit\|259.7\|1.24\|6304\|\|-\|TOI-2019 b\|0.109\|0.505\|15.3444\|\|\|style="background:#FFFF00"\|transit\|645.812\|\|5590\|\|-\|TOI-2107 b\|0.83\|1.211\|2.454\|0.0315\|1397\|style="background:#FFFF00"\|transit + radial vel.\|767.4\|0.961\|5627\|\|-\|TOI-2120 b\|\|0.1893\|5.8\|0.0377\|351–384\|style="background:#FFFF00"\|transit\|104.9\|0.211\|3131\|\|-\|TOI-2128 b\|0.014\|0.186\|16.341\|0.127\|780.5\|style="background:#FFFF00"\|transit\|119.2\|1.1\|5991\|\|-\|TOI-2266 b\|\|0.1374\|2.326\|0.02\|550\|style="background:#FFFF00"\|transit\|168.6\|0.23\|3240\|^[112] \|-\|TOI-2274 b\|\|\|2.679\|\|771\|style="background:#FFFF00"\|transit\|159.9\|0.612\|3943\|\|-\|TOI-2368 b\|0.65\|0.967\|5.175\|0.05649\|1000\|style="background:#FFFF00"\|transit\|685\|0.897\|5360\|\|-\|TOI-2373 b\|9.3\|0.93\|13.337\|0.112\|860\|style="background:#FFFF00"\|transit\|1617\|1.041\|5651\|^[113] \|-\|TOI-2374 b\|0.1782\|0.6075\|4.314\|0.0471\|\|style="background:#FFFF00"\|transit\|439\|0.75\|4802\|^[114] \|-\|TOI-2379 b\|5.76\|1.046\|5.4693827\|0.05263\|624\|style="background:#FFFF00"\|transit\|689.5\|0.645\|3707\|^[115] \|-\|TOI-2384 b\|1.966\|1.025\|2.13570304\|0.02793\|889.7\|style="background:#FFFF00"\|transit\|609.9\|0.635\|3943\|\|-\|TOI-2416 b\|3\|0.88\|8.275\|0.0831\|1080\|style="background:#FFFF00"\|transit\|1767\|1.118\|5808\|\|-\|TOI-2420 b\|0.927\|1.340\|5.8426\|0.0684\|1571.6\|style="background:#FFFF00"\|transit\|1450\|1.158\|\|^[116] \|-\|TOI-2485 b\|2.412\|1.083\|11.235\|0.1093\|1134\|style="background:#FFFF00"\|transit\|1296\|1.163\|\|\|-\|TOI-2524 b\|0.64\|1\|7.186\|0.073\|1100\|style="background:#FFFF00"\|transit\|1399\|1.007\|5831\|\|-\|TOI-2529 b\|2.34\|1.03\|64.5949\|0.327\|636\|style="background:#FFFF00"\|transit\|965.8\|1.11\|5802\|^[117] \|-\|TOI-2714 b\|0.717\|1.224\|2.499\|0.036\|1603\|style="background:#FFFF00"\|transit\|1930\|1.07\|5665\|\|-\|TOI-2768 b\|\|0.2688\|1.508\|\|855\|style="background:#FFFF00"\|transit\|255.8\|0.63\|4008\|\|-\|TOI-2981 b\|2.007\|1.1955\|3.602\|0.048\|1358\|style="background:#FFFF00"\|transit\|1741\|1.03\|5940\|^[118] \|-\|TOI-3071 b\|0.2146\|0.6388\|1.267\|0.0249\|\|style="background:#FFFF00"\|transit\|1582\|1.29\|6177\|\|-\|TOI-3261 b\|0.0953\|0.3408\|0.883\|0.01714\|1722\|style="background:#FFFF00"\|transit\|972.3\|0.861\|4995\|Ultra-hot Neptune^[119] \|-\|TOI-3321 b\|0.554\|1.388\|3.652\|0.047\|1616\|style="background:#FFFF00"\|transit\|928\|1.041\|5850\|\|-\|TOI-3353 b\|\|0.238\|4.67\|0.060\|1264\| style="background:#FFFF00"\|transit\|\|1.33\|6365\|\|-\|TOI-3568 b\|0.083\|0.473\|4.42\|0.0485\|899\|style="background:#FFFF00"\|transit\|645\|0.78\|4969\|^[120] \|-\|TOI-3894 b\|0.85\|1.358\|4.335\|0.0543\|1519\|style="background:#FFFF00"\|transit\|1343\|1.138\|6000\|\|-\|TOI-3919 b\|3.88\|1.1\|7.433\|0.0795\|1200\|style="background:#FFFF00"\|transit\|1973\|1.208\|6100\|\|-\|TOI-4153 b\|1.15\|1.438\|4.617\|0.06311\|1670\|style="background:#FFFF00"\|transit\|1366\|1.572\|6860\|\|-\|TOI-4336 Ab\|0.017\|0.1891\|16.337\|0.0872\|308\|style="background:#FFFF00"\|transit\|73.15\|0.331\|3298\|Located in a triple hierarchical stellar system.\|-\|TOI-4364 b\|\|0.1793\|5.424\|0.04753\|488\|style="background:#FFFF00"\|transit\|142.9\|0.487\|3528\|Located in the Hyades.^[121] \|-\|TOI-4379 b\|1.113\|1.489\|3.254\|\|\|style="background:#FFFF00"\|transit\|2013\|1.372\|6020\|\|-\|TOI-4438 b\|0.017\|0.2248\|7.44\|0.0534\|400\|style="background:#FFFF00"\|transit\|98\|0.368\|3422\|^[122] \|-\|TOI-4443 b\|\|0.153\|1.85\|0.030\|1639\| style="background:#FFFF00"\|transit\|\|1.05\|5834\|\|-\|TOI-4495 b\|\|0.324\|5.18\|0.062\|1383\| style="background:#FFFF00"\|transit\|\|1.17\|6156\|\|-\|TOI-4527 b\|\|0.0812\|0.40\|0.008\|1363\| style="background:#FFFF00"\|transit\|\|0.48\|3702\|\|-\|TOI-4562 c\|5.77\|\|3990\|5.219\|\|style="background:#FF7519"\|timing\|1131^[123] \|1.218\|6096\|^[124] \|-\|TOI-4602 b\|\|0.227\|3.98\|0.051\|1380\| style="background:#FFFF00"\|transit\|\|1.12\|6012\|\|-\|TOI-4633 c\|0.15\|0.285\|271.94\|0.847\|290\|style="background:#FFFF00"\|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.^[125] \|-\|TOI-4914 b\|0.714\|1.1482\|10.6\|0.098\|894\|style="background:#FFFF00"\|transit\|951\|1.03\|5805\|\|-\|TOI-5005 b\|0.103\|0.558\|6.309\|0.06614\|1040\|style="background:#FFFF00"\|transit\|685\|0.97\|5749\|\|-\|TOI-5076 b\|0.0503\|0.285\|23.445\|\|615\| style="background:#FFFF00"\|transit\|270.057\|0.80\|5070\|^[126] \|-\|TOI-5082 b\|\|0.227\|4.24\|0.051\|1165\| style="background:#FFFF00"\|transit\|\|1.00\|5670\|\|-\|TOI-5218 b\|0.799\|0.879\|4.291\|0.0469\|783\| style="background:#FFFF00"\|transit\|1243\|0.739\|4230\|\|-\|TOI-5232 b\|2.34\|1.14\|4.097\|0.0599\|1772\|style="background:#FFFF00"\|transit\|1985\|1.389\|6500\|\|-\|TOI-5301 b\|3.65\|1.18\|5.859\|0.0726\|1655\|style="background:#FFFF00"\|transit\|1914\|1.483\|6240\|\|-\|TOI-5319 b\|\|0.33427\|4.079\|\|695\|style="background:#FFFF00"\|transit\|199.4\|0.5\|3580\|\|-\|TOI-5388 b\|\|0.169\|2.59\|0.024\|601\| style="background:#FFFF00"\|transit\|\|0.29\|3495\|\|-\|TOI-5616 b\|0.802\|0.961\|2.003\|0.0272\|939\| style="background:#FFFF00"\|transit\|1249\|0.666\|3996\|^[127] \|-\|TOI-5634 Ab\|0.576\|0.923\|2.2035\|0.0272\|837\|style="background:#FFFF00"\|transit\|1051\|0.556\|3896\|\|-\|TOI-5688 Ab\|0.390\|0.920\|2.948\|0.03379\|742\|style="background:#FFFF00"\|transit\|735.8\|0.60\|3713\|^[128] \|-\|TOI-5713 b\|0.0135\|0.1579\|10.44\|0.06008\|347\|style="background:#FFFF00"\|transit\|133.7\|0.265\|3228\|\|-\|TOI-5720 b\|0.0041\|0.0972\|1.434\|0.0183\|708\|style="background:#FFFF00"\|transit\|116.9\|0.383\|3325\|\|-\|TOI-6002 b\|0.0119\|0.1454\|10.905\|0.05722\|321\|style="background:#FFFF00"\|transit\|104.6\|0.21\|3241\|^[129] \|-\|TOI-6008 b\|0.00346\|0.0919\|0.858\|0.0108\|707\|style="background:#FFFF00"\|transit\|75.05\|0.23\|3075\|Ultra-short period planet\|-\|TOI-6029 b\|1.635\|1.284\|5.7987\|\|\|style="background:#FFFF00"\|transit\|1946\|1.548\|6223\|^[130] \|-\|TOI-6034 b\|0.798\|1.063\|2.576\|0.02949\|714\|style="background:#FFFF00"\|transit\|385\|0.514\|3635\|\|-\|TOI-6086 b\|0.00346\|0.1053\|1.389\|0.0154\|634\|style="background:#FFFF00"\|transit\|102.6\|0.254\|3200\|\|-\|TOI-6383 Ab\|1.04\|1.008\|1.791\|0.02292\|745\|style="background:#FFFF00"\|transit\|561\|0.458\|3444\|^[131] \|-\|TOI-6651 b\|0.1919\|0.4541\|5.057\|0.06330\|1493\|style="background:#FFFF00"\|transit\|690^[132] \|1.323\|5940\|^[133] \|-\|TOI-7041 b\|0.36\|1.02\|9.691\|\|\|style="background:#FFFF00"\|transit\|1431\|1.12\|4640\|^[134] \|-\|\|6.8\|\|4109\|\|\|style="background:#FF7519"\|timing\|698\|0.9\|\|The planet's host star is a polar. The mass value for the planet is only a minimum mass.^[135] \|-\|VHS J183135.58-551355.9\|6.5\|1.42\|colspan="2"\|\|1085\|style="background:#FF6CDA" \|imaging\|180.6\|colspan="2"\|\|Free-floating planet\|-\|WASP-132d\|5.16\|\|1816.6\|2.71\|107\|style="background:#00FF00"\|radial vel.\|401.53\|0.789\|4686\|\|-\|Wolf 327 b\|0.00796\|0.1106\|0.573\|0.01\|996\|style="background:#FFFF00"\|transit\|92.9\|0.405\|3542\|Ultra-short period planet^[136] \|} References

Notes and References

82 Eri d. 888.
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GJ 900 (ABC)b. 9120.
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HD 75898 c. 10288. August 1, 2024.
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2407.11706v1 . Maciejewski . G. . Niedzielski . A. . Gozdziewski . K. . Wolszczan . A. . Villaver . E. . Fernandez . M. . Adamow . M. . Sierzputowska . J. . Tracking Advanced Planetary Systems (TAPAS) with HARPS-N VIII. A wide-orbit planetary companion in the hot-Jupiter system HD 118203 . 2024 . astro-ph.EP .
HD 128717 b. 8996.
HD 148193 Ab. 9627.
TOI-1836 Ac. 10269.
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TOI-1605 b. 9625.
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TOI-329 b. 9092. May 28, 2024.
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TOI-480 b. 9094. May 28, 2024.
TOI-603 b. 9622.
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TOI-1294 b. 9623.
TOI-1294 c. 9624.
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Bryant. Edward M.. 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. 10.1093/mnras/stae2034 . free . 28 September 2024.
Carleo . Ilaria . Mass determination of two Jupiter-sized planets orbiting slightly evolved stars: TOI-2420 b and TOI-2485 b . 2024-08-10 . 2408.05612 . Barrágan . Oscar . Persson . Carina M. . Fridlund . Malcolm . Lam . Kristine W. F. . Messina . Sergio . Gandolfi . Davide . Smith . Alexis M. S. . Johnson . Marshall C.. Astronomy and Astrophysics . 690 . A18 . 10.1051/0004-6361/202451313 . 2024A&A...690A..18C .
Jones . Matias I. . A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS . 2024-01-17 . 2401.09657 . Reinarz . Yared . Brahm . Rafael . Pinto . Marcelo Tala . Eberhardt . Jan . Rojas . Felipe . Triaud . Amaury H. M. J. . Gupta . Arvind F. . Ziegler . Carl. Astronomy and Astrophysics . 683 . A192 . 10.1051/0004-6361/202348147 . 2024A&A...683A.192J .
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Montalto. M.. 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 . 10.1051/0004-6361/202349082 . 2405.18950. 2024A&A...687A.226M .
Kanodia . Shubham . Searching for GEMS: Characterizing Six Giant Planets around Cool Dwarfs . 2408.14694 . August 26, 2024 . Gupta . Arvind F. . Canas . Caleb I. . Bernabo . Lia Marta . Reji . Varghese . Han . Te . Brady . Madison . Seifahrt . Andreas . Cochran . William D.. astro-ph.EP .
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TIC 174328045.
Baliwal . Sanjay . Sharma . Rishikesh . Chakraborty . Abhijit . Khandelwal . Akanksha . Nikitha . K. J. . Safonov . Boris S. . Strakhov . Ivan A. . Montalto . Marco . Eastman . Jason D. . 2024-08-30 . Discovery and characterization of a dense sub-Saturn TOI-6651b . Astronomy & Astrophysics . 691 . A12 . 10.1051/0004-6361/202450934 . 2408.17179 .
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