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List of exoplanets discovered by the TESS mission

Last updated February 27, 2026

The list of exoplanets detected by the Transiting Exoplanet Survey Satellite (TESS) contains bodies with a wide variety of properties, with significant ranges in orbital distances, masses, radii, composition, habitability, and host star type. As of 17 September 2025, the TESS Mission has detected 8,361 planets and confirmed 693 planets, including hot Jupiters, super-Earths, circumbinary planets, and planets located in the circumstellar habitable zones of their host stars.^[1] TESS has detected over 7,668 unconfirmed planet candidates.

Table

Name	Mass (`M`_J)	Radius (`R`_J)	Period (days)	Semi-major axis (AU)	Temp. (K)	Discovery method	Distance (ly)	Host star	Host star mass (`M`_☉)	Host star temp. (K)	Year of Discovery	Remarks
Earth (for reference)								Sun			–	^[2]
TESS Object of Interest (TOI)
TOI 122 b	0.028^+0.029 _−0.010	0.243±0.016	5.078030±0.000015	0.0392±0.0007	471	transit	202.9±0.7	TOI-122	0.312±0.007	3403±100	2020	^[3]
TOI-125 b	0.0299±0.00277	0.2432±0.00669	4.65382±0.00033	0.05186^+0.00086 _−0.00077	1037±11	transit	363.3382±1.435088	TOI-125	0.859^+0.044 _−0.038	5320±39	2019	^[4]
TOI-125 c	0.02086±0.00311	0.24614±0.009	9.15059^+0.0007 _−0.00082	0.814±0.0013	827.8±8.6	transit	363.3382±1.435088		0.859^+0.044 _−0.038	5320±39		^[4]
TOI-125 d	0.0428±0.0038	0.2614±0.0152	19.98^+0.005 _−0.0056	0.05186^+0.00086 _−0.00077	638.1±6.6	transit	363.3382±1.435088		0.859^+0.044 _−0.038	5320±39		^[5]^[4]
TOI-132 b	0.07048^+0.00598 _−0.00604	0.305±0.012	2.1097019^+0.000012 _−0.000011	0.026^+0.002 _−0.003	1395⁺⁵² ₋₇₂	transit	536.43±89.11	TOI-132	0.970±0.06	5397±46	2020	^[6]
TOI-150 b	1.75^+0.14 _−0.17	1.38±0.04	5.857342^+0.000065 _−0.000066	0.0583^+0.0013 _−0.0018	1493⁺²⁹ ₋₃₂	transit	1095.89±6.52	TO-150	1.25^+0.07 _−0.12	6003⁺¹⁰⁴ ₋₉₈	2019	^[7]
TOI-157 b	1.18±0.13	1.29±0.02	2.0845435±0.0000023	0.03138^+0.00025 _−0.00020	1588⁺²¹ ₋₂₀	transit	1171	TOI-157	0.948^+0.023 _−0.018	5404⁺⁷⁰ ₋₆₇	2020	^[4]
TOI-163b	1.22	1.489	4.231306	0.0580	1669	transit	1359	TOI-163	1.44	6495	2019	^[7]
TOI-172b	5.42^+0.22 _−0.20	0.965^+0.032 _−0.029	9.47725^+0.00064 _−0.00079	0.0914±0.0017		transit	1097.418	TOI-172	1.128^+0.065 _−0.061	5645±50	2019	^[8]
TOI-175b	0.00126^+0.00050 _−0.00048	0.0642^+0.0046 _−0.0035	2.2531136^+0.0000012 _−0.0000015	0.02191^+0.00080 _−0.00084	627⁺³³ ₋₃₆	transit	34.636±0.010	L 98-59	0.273±0.030	3415±135	2019	^[9]To date, it is the lowest mass planet confirmed, or measured, using the radial velocity technique.^[10] Host star also known as L 98-59.^[11]
GJ 3090 b (TOI-177 b)	0.0105	0.19	2.8531042±0.0000032	0.03165	696	transit	73.21±0.04	TOI-177	0.519±0.013	3556±70	2022	^[12]
HD 21749 b (TOI-186 b)	0.073^+0.007 _−0.006	0.254^+0.023 _−0.020	35.61253^+0.00060 _−0.00062	0.1915^+0.0058 _−0.0063	422⁺¹⁵ ₋₁₄	transit	53.261±0.023	HD 21749	0.73±0.07	4640±100	2019	^[13]
HD 21749 c (TOI-186 c)	<0.0116	0.0796^+0.0057 _−0.0052	7.78993^+0.00051 _−0.00044	0.0695^+0.0021 _−0.0023	701⁺²⁵ ₋₂₃	transit	53.261±0.023	HD 21749	0.73±0.07	4640±100	2019	^[13]
DS Tucanae Ab (TOI-200 b)		0.509±0.015	8.138268±0.000011		850	transit	143.89±0.22	DS Tucanae	1.01±0.06	5428±80	2019	^[14]
TOI-201 c	14.2±2.0	0.99±0.017	2,800⁺³⁶⁰ ₋₂₁₀	4.28^+0.36 _−0.2		timing + transit	372.5	TOI-201	1.316±0.027	6,394±75	2025	^[15]
TOI-216 b	0.059±0.002	0.714^+0.268 _−0.179	17.1607	0.1293^+0.0067 _−0.0051	628⁺¹³ ₋₁₁	transit	583±3	TOI-216	0.77	5026±125	2019	Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years^[16]^[17]^[18]
TOI-216 c	0.56±0.02	0.902±0.018	34.525528	0.2069^+0.0107 _−0.0082	497⁺¹⁰ ₋₈	transit	583±3	TOI-216	0.77	5026±125	2019
TOI-237 c		0.1076±0.0031	1.74486147	0.0160+0.0005 −0.0006	515+11 −8	transit	124.86	TOI-237	0.1698+0.0385 −0.0350	3226+47 −48	2026	^[19]
TOI-333 b	0.0632±0.0076	0.3801±0.0098	3.785250±0.000006	0.049±0.001	1445	transit	1132	TOI-333	1.2±0.1	6,241±73	2025	^[20]
Gliese 238 b (TOI-486 b)		0.05049±0.0012	1.74	0.02123^+0.00016 _−0.00017	758⁺¹⁶ ₋₁₅	transit	49.6	Gliese 238	0.419±0.01	3485±140	2024	Mars-sized exoplanet, one of the smallest exoplanets currently known^[21]
TOI-270b	0.0050	0.1112	3.360080	0.0306	528	transit	73.23	TOI-270	0.40	3386	2019	^[22]^[23]
TOI-270c	0.0193	0.216	5.660172	0.0472	424	transit	73.23		0.40	3386		^[22]^[23]
TOI-270d	0.0150	0.190	11.38014	0.0733	340	transit	73.23		0.40	3386		^[22]^[23]Hydrogen and steam atmosphere^[24]
NGTS-6b (TOI-448 b)	1.339	1.326	0.8820590	0.01677		transit	1010	NGTS-6	0.77	4730	2019	^[25]
GJ 3473 b (TOI-488 b)	0.0059±0.0009	0.113^+0.0045 _−0.0044	1.1980035^+0.0000018 _−0.0000019	0.01589±0.00062	773⁺¹⁶ ₋₁₅	transit	89.29±0.13	GJ 3473	0.360±0.016	3347±54	2020	Potentially rocky world, larger than Earth, also called TOI-488 b^[26]
GJ 3473 c (TOI-488 c)	0.0233^+0.0029 _−0.0027	0.235	15.509±0.033	0.0876^+0.0035 _−0.0034	329.1^+6.6 _−6.4	radial vel.	89.29±0.13	GJ 3473	0.360±0.016	3347±54	2020	Neptune-like ice giant also called TOI-488 c^[26]^[27]^[28]
TOI-512 b	0.01123^+0.00167 _−0.00173	0.1374±0.0089	7.18886^+0.000069 _−0.000077		1,009±29	transit	219.16±0.14	TOi-512	0.74±0.03	5,277±67	2025	^[29]
TOI-561 b	0.0050±0.0011	0.127±0.006	0.446578±0.000017	0.01055±0.00008		transit	279.2±1.6	TOI-561	0.785±0.018	5455⁺⁶⁵ ₋₄₇	2020	^[30]^[31]
TOI-561 c	0.017±0.003	0.257±0.009	10.779±0.004	0.08809±0.0007		transit	279.2±1.6		0.785±0.018	5455⁺⁶⁵ ₋₄₇		^[30]^[31]
TOI-561 d	0.038±0.004	0.226±0.011	25.62±0.04	0.1569±0.0012		transit	279.2±1.6		0.785±0.018	5455⁺⁶⁵ ₋₄₇		^[30]^[31]
TOI-561 e	0.050±0.007	0.238±0.010	77.23±0.39	0.3274^+0.0028 _−0.0027		transit	279.2±1.6		0.785±0.018	5455⁺⁶⁵ ₋₄₇		^[30]
TOI-564b	1.463^+0.10 _−0.096	1.02^+0.71 _−0.29	1.651144±0.000018	0.02734^+0.00061 _−0.00053	1714⁺²⁰ ₋₂₁	transit	643.8±5.9	TOI-564	0.998^+0.068 _−0.057	5640⁺³⁴ ₋₃₇	2019	^[32]
TOI-700 b	0.00406^+0.003 _−0.00116	0.0901^+0.00839 _−0.00776	9.97701^+0.00024 _−0.00028	0.0637^+0.0064 _−0.006		transit	101.5	TOI-700	0.416±0.01	3480±135	2020	^[33]
TOI-700 c	0.0249^+0.0085 _−0.0057	0.2346^+0.0214 _−0.0205	16.051998^+0.000089 _−0.000092	0.0925^+0.0088 _−0.0083		transit	101.5		0.416±0.01	3480±135		^[33]
TOI-700 d	0.00711^+0.0022 _−0.00164	0.1062±0.0098	37.426^+0.0007 _−0.001	0.163±0.015	295±55	transit	101.5		0.416±0.01	3480±135		First "Earth sized" discovered by TESS ^[33]^[34]
TOI-771 c	0.00903		7.61	0.046±0.002	365	radial vel.	82.45	TOI-771	0.22±0.024	3,201±100	2025	^[35]
TOI-905b	0.667^+0.042 _−0.041	1.171^+0.052 _−0.051	3.739494±0.000038	0.04666^+0.00096 _−0.0011	1192⁺³⁹ ₋₃₆	transit	489.9^+23.5 _−22.5	TOI-905	0.968^+0.061 _−0.068	5570⁺¹⁵⁰ ₋₁₄₀	2019	^[32]
TOI-1117 b	0.028±0.003	0.219^+0.012 _−0.011	2.22816±0.00001	0.0330±0.0002	1,538±21	transit	546.64±2.94	TOI-1117	0.97±0.02	5,635±62	2025	^[36]
TOI-1117 c	0.0276^+0.0037 _−0.0038		4.579±0.004	0.0534±0.0003	1,210±16	radial vel.
TOI-1117 d	0.0337±0.0050		8.665±0.011	0.0817±0.0006	978±13	radial vel.
TOI-1243 b	0.0242±0.0047	0.2079±0.0107	4.65948	0.0437±0.0001	450	transit	140.6	TOI-1243	0.515±0.027	3,515±79	2026	^[37]
TOI-3862 b	0.1688+0.0087 −0.0090	0.493±0.016	1.55745774	0.02539+0.00064 −0.00068	1539	transit	801.2	TOI-3861	0.90±0.07	5300±50	2026	^[38]
TOI-4336 Ac		0.1039+0.0054 −0.0052	7.587270	0.0481±0.0027	378±12	transit	73.23	TOI-4336	0.2853+0.0438 −0.0356	3369+51 −57	2026	^[19]
TOI-4495 b	0.024+0.004 −0.05	0.221+0.012 −0.008	2.56699	0.03957±0.00047	1735	transit	801.2	TOI-4495	1.247±0.045	6210±70	2026	^[39]
TOI-4529 b	0.0154	0.1579±0.008	5.87958	0.04997±0.0008	511	transit	92.6	TOI-4529	0.482±0.023	3,697±71	2026	^[37]
BD-14 3065 b (TOI-4987 b)	12.11^+0.95 _−0.91	1.926±0.094	4.3	0.0646±0.0026	3520±130	transit	1847.4^[40]^[a]	BD-14 3065	1.4±0.06	6985±90	2024	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^[41]
TOI-5788 b	0.0117±0.0030	0.1365±0.0067	6.340758	0.0640±0.0011		transit	318.2	TOI-5788	0.87±0.04	5615±25	2026	^[42]
TOI-5788 c	0.0201±0.0038	0.2025±0.0036	16.213358	0.1197±0.0020		transit	318.2	TOI-5788	0.87±0.04	5615±25	2026	^[42]
Gliese 12 b (TOI-6251 b)	0.002769^+0.00123 _−0.0008	0.0892±0.0089^[b]	12.7	0.066±0.002	315±5	transit	39.65	Gliese 12	0.241±0.006	3253±55	2024	^[43]
HD 101581 b (TOI-6276 b)		0.0877	4.47			transit	41.7	HD 101581	0.740±0.087	4675±53	2024	Host star is the brightest star with multiple known transiting Earth-size exoplanets. Another transiting planet in the system is suspected.^[44]
HD 101581 c (TOI-6276 c)		0.0925	6.21			transit	41.7	HD 101581	0.740±0.087	4675±53	2024
TOI-6716 b		0.0874±0.0062	4.71859	0.032±0.003	369	transit	61.6	TOI-6716	0.223±0.011	3,110±80	2026	^[45]
TOI-7384 b		0.3176±0.0187	6.23403	0.0439±0.004	378	transit	218	TOI-7384	0.318±0.016	3,185±75	2026	^[45]
TESS Input Catalog (TIC)
TIC 237913194b	1.942^+0.092 _−0.091	1.117^+0.054 _−0.047	15.168865±0.000018	0.1207±0.0037	974	transit	1009±6	TIC 237913194	1.026^+0.057 _−0.055	5788±80	2020	Very eccentric orbit^[46]
BD+05 4868 Ab (TIC 466376085 b)	0.000063	0.028	1.27187	0.0208±0.0003	1,820±45	transit	142.4±0.1	BD+05 4868	0.70±0.02	4,596⁺⁶⁵ ₋₆₄	2025	A disintegrating planet with a comet-like tail.^[47]
TIC 88785435 b		0.449±0.019	10.508843	0.08432±0.00068	635±16	transit	398.2±0.8	TIC 88785435	0.724±0.017	3,998±95	2025	^[48]

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Notes

↑
↑ The radius is the same as that of the Earth, with an uncertainty of 10%

Reference

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1 2 3 "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は？". sorae. 2019-07-30. Retrieved 2021-01-08.
1 2 3 Van Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), "Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley", Monthly Notices of the Royal Astronomical Society stab2143, arXiv: 2101.01593 , doi: 10.1093/mnras/stab2143
↑ Mikal-Evans, Thomas; Madhusudhan, Nikku; Dittmann, Jason; Guenther, Maximilian N.; Welbanks, Luis; Vincent Van Eylen; Crossfield, Ian J. M.; Daylan, Tansu; Kreidberg, Laura (2023), "Hubble Space Telescope Transmission Spectroscopy for the Temperate Sub-Neptune TOI-270 d: A Possible Hydrogen-rich Atmosphere Containing Water Vapor", The Astronomical Journal, 165 (3): 84, arXiv: 2211.15576 , Bibcode:2023AJ....165...84M, doi: 10.3847/1538-3881/aca90b , S2CID 254044155
↑ Vines, Jose I.; et al. (2019), "NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf", Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv: 1904.07997 , doi: 10.1093/mnras/stz2349
1 2 Kemmer, J.; et al. (2020), "Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488)", Astronomy & Astrophysics, 642: A236, arXiv: 2009.10432 , Bibcode:2020A&A...642A.236K, doi:10.1051/0004-6361/202038967, S2CID 221836679
↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. 22 October 2020. Retrieved 2023-11-25.
↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. 14 February 2020. Retrieved 2023-11-25.
↑ Rodrigues, J.; et al. (2025-02-20). "TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO". Astronomy and Astrophysics. 695: A237. arXiv: 2502.14472 . Bibcode:2025A&A...695A.237R. doi:10.1051/0004-6361/202452887.
1 2 3 4 Lacedelli, G.; et al. (2021), "An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561", Monthly Notices of the Royal Astronomical Society, 501 (3): 4148–4166, arXiv: 2009.02332 , doi: 10.1093/mnras/staa3728
1 2 3 Weiss, Lauren M.; et al. (2021), "The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561", The Astronomical Journal, 161 (2): 56, arXiv: 2009.03071 , Bibcode:2021AJ....161...56W, doi: 10.3847/1538-3881/abd409 , S2CID 229279232
1 2 Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160 (5): 229. arXiv: 1912.10186 . Bibcode:2020AJ....160..229D. doi: 10.3847/1538-3881/aba49d . hdl:1721.1/134083. S2CID 209444463.
1 2 3 Gilbert, Emily A.; Barclay, Thomas; Schlieder, Joshua E.; Quintana, Elisa V.; Hord, Benjamin J.; Kostov, Veselin B.; Lopez, Eric D.; Rowe, Jason F.; Hoffman, Kelsey; Walkowicz, Lucianne M.; Silverstein, Michele L.; Rodriguez, Joseph E.; Vanderburg, Andrew; Suissa, Gabrielle; Airapetian, Vladimir S.; Clement, Matthew S.; Raymond, Sean N.; Mann, Andrew W.; Kruse, Ethan; Lissauer, Jack J.; Colón, Knicole D.; Ravi kumar Kopparapu; Kreidberg, Laura; Zieba, Sebastian; Collins, Karen A.; Quinn, Samuel N.; Howell, Steve B.; Ziegler, Carl; Eliot Halley Vrijmoet; et al. (2020). "The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System". The Astronomical Journal. 160 (3): 116. arXiv: 2001.00952 . Bibcode:2020AJ....160..116G. doi: 10.3847/1538-3881/aba4b2 . S2CID 209862554.
↑ Suissa, Gabrielle; Wolf, Eric T.; Ravi kumar Kopparapu; Villanueva, Geronimo L.; Fauchez, Thomas; Mandell, Avi M.; Arney, Giada; Gilbert, Emily A.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Lopez, Eric; Rodriguez, Joseph E.; Vanderburg, Andrew (2020). "The First Habitable-zone Earth-sized Planet from TESS. III. Climate States and Characterization Prospects for TOI-700 D". The Astronomical Journal. 160 (3): 118. arXiv: 2001.00955 . Bibcode:2020AJ....160..118S. doi: 10.3847/1538-3881/aba4b4 . S2CID 209862275.
↑ Lacedelli, G.; Pallé, E.; Davis, Y. T.; Luque, R.; Morello, G.; Tabernero, H. M.; Zapatero Osorio, M. R.; Pozuelos, F. J.; Jankowski, D.; Nowak, G.; Murgas, F.; Orell-Miquel, J.; Akana Murphy, J. M.; Barkaoui, K.; Charbonneau, D.; Dransfield, G.; Ducrot, E.; Geraldía-González, S.; Irwin, J.; Jehin, E.; Osborne, H. L. M.; Pedersen, P. P.; Rackham, B. V.; Scott, M. G.; Timmermans, M.; Triaud, A.; Van Eylen, V. (2025). "A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771". Astronomy & Astrophysics. 698: A223. arXiv: 2504.18223 . Bibcode:2025A&A...698A.223L. doi:10.1051/0004-6361/202554161.
↑ Lockley, Isobel S.; Armstrong, David J.; Fernández, Jorge Fernández; Millholland, Sarah; Knierim, Henrik; Mena, Elisa Delgado; Sousa, Sergio; Collins, Karen A.; Watkins, Cristilyn N.; Howell, Steve B.; Adibekyan, Vardan; Helled, Ravit; Ziegler, Carl; Bayliss, Daniel; Briceño, César (June 2025). "The TOI-1117 Multi-planetary System: 3 sub-Neptunes, 1 in both the Neptunian Desert and Radius Valley". Monthly Notices of the Royal Astronomical Society. 541 (2): 919–938. arXiv: 2506.05521 . Bibcode:2025MNRAS.541..919L. doi: 10.1093/mnras/staf939 . ISSN 0035-8711.
1 2 Poultourtzidis, E.; et al. (2026). "Characterization of two new transiting sub-Neptunes and a terrestrial planet around M-dwarf hosts". arXiv: 2601.07414 [astro-ph.EP].
↑ Carleo, Ilaria; Castro-González, Amadeo; Pallé, Enric; et al. (2026-01-15). "TOI-3862 b: A dense super-Neptune deep in the hot Neptune desert". arXiv: 2601.10450v1 [astro-ph.EP].
↑ Wang, Mu-Tian; Dai, Fei; Liu, Hui-Gen; et al. (2026-01-06). "TOI-4495: A Pair of Aligned, Near-Resonant Sub-Neptunes that Likely Experienced Overstable Migration". arXiv: 2601.02665v1 [astro-ph.EP].
↑ "BD-14 3065". SIMBAD . Centre de données astronomiques de Strasbourg.
↑ Šubjak, Ján; Latham, David W.; Quinn, Samuel N.; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Brahm, Rafael; Guenther, Eike; Janík, Jan (2024-03-18). "Evolution of BD-14 3065b (TOI-4987b) from giant planet to brown dwarf as possible evidence of deuterium burning at old stellar ages". Astronomy & Astrophysics. 688: A120. arXiv: 2403.12311 . Bibcode:2024A&A...688A.120S. doi:10.1051/0004-6361/202349028.
↑ Lakeland, Ben S.; Mortier, A.; Haywood, R. D.; et al. (2026-01-20). "Discovery and characterisation of two exoplanets orbiting the metal-poor, solar-type star TOI-5788 with TESS, CHEOPS, and HARPS-N". Monthly Notices of the Royal Astronomical Society stag158. arXiv: 2601.14045v1 . Bibcode:2026MNRAS.tmp..146L. doi: 10.1093/mnras/stag158 .{{cite journal}}: CS1 maint: bibcode (link)
↑ Dholakia, Shishir; Palethorpe, Larissa; Venner, Alexander; Mortier, Annelies; Wilson, Thomas G.; Huang, Chelsea X.; Rice, Ken; Van Eylen, Vincent; Nabbie, Emma (2024-05-21). "Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPS". Monthly Notices of the Royal Astronomical Society. 531 (1): 1276. arXiv: 2405.13118 . Bibcode:2024MNRAS.531.1276D. doi: 10.1093/mnras/stae1152 .
↑ Kunimoto, Michelle; Lin, Zifan; Millholland, Sarah; Venner, Alexander; Hinkel, Natalie R.; Shporer, Avi; Vanderburg, Andrew; Bailey, Jeremy; Brahm, Rafael (December 2024), "Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581", The Astronomical Journal, 169 (1): 47, arXiv: 2412.08863 , Bibcode:2025AJ....169...47K, doi: 10.3847/1538-3881/ad9266
1 2 Scott, Madison G.; et al. (2026). "Two temperate Earth- and Neptune-sized planets orbiting fully convective M dwarfs". Monthly Notices of the Royal Astronomical Society stag070. arXiv: 2601.05799 . Bibcode:2026MNRAS.tmp...63S. doi: 10.1093/mnras/stag070 .{{cite journal}}: CS1 maint: bibcode (link)
↑ Schlecker, Martin; et al. (2020), "A Highly Eccentric Warm Jupiter Orbiting TIC 237913194", The Astronomical Journal, 160 (6): 275, arXiv: 2010.03570 , Bibcode:2020AJ....160..275S, doi: 10.3847/1538-3881/abbe03 , S2CID 222208966
↑ Hon, Marc; Rappaport, Saul; Shporer, Avi; Vanderburg, Andrew; Collins, Karen A.; Watkins, Cristilyn N.; Schwarz, Richard P.; Barkaoui, Khalid; Yee, Samuel W. (2025-01-09). "A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star". The Astrophysical Journal. 984 (1): L3. arXiv: 2501.05431 . Bibcode:2025ApJ...984L...3H. doi: 10.3847/2041-8213/adbf21 .
↑ Vach, Sydney; et al. (2025-02-01). "A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS". The Astronomical Journal. 170 (2): 131. arXiv: 2502.00576 . Bibcode:2025AJ....170..131V. doi: 10.3847/1538-3881/ade67f .

External links

List of TOIs at IPAC's ExoFOP

This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
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蚂蚁超级镜像烟雨镜像程序批量镜像网站干扰字符镜像时间因子转换镜像

[distp-41] ↑

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

[1] "Exoplanet and Candidate Statistics". exoplanetarchive.ipac.caltech.edu. Retrieved 2025-09-24.

[2] NASA. "Jupiter Fact Sheet". NASA. Archived from the original on 2011-09-26. Retrieved 2013-03-31.

[Waalkes2020-3] Waalkes, William C.; et al. (2021), "TOI 122b and TOI 237b: Two Small Warm Planets Orbiting Inactive M Dwarfs Found by TESS", The Astronomical Journal, 161 (1): 13, arXiv: 2010.15905 , Bibcode:2021AJ....161...13W, doi: 10.3847/1538-3881/abc3b9 , S2CID 226221997

[Nielsen2019-4] 1 2 3 4 Nielsen, L. D.; Gandolfi, D.; Armstrong, D. J.; Jenkins, J. S.; Fridlund, M.; Santos, N. C.; Dai, F.; Adibekyan, V.; Luque, R.; Steffen, J. H.; Esposito, M.; Meru, F.; Sabotta, S.; Bolmont, E.; Kossakowski, D.; Otegi, J. F.; Murgas, F.; Stalport, M.; Rodler, F.; Díaz, M. R.; Kurtovic, N. T.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Allart, R.; Almenara, J. M.; et al. (2020). "Mass determinations of the three mini-Neptunes transiting TOI-125". Monthly Notices of the Royal Astronomical Society. 492 (4): 5399. arXiv: 2001.08834 . Bibcode:2020MNRAS.492.5399N. doi: 10.1093/mnras/staa197 .

[5] "exoplanet.eu toi-125_d". Extrasolar Planets Encyclopaedia .^{[ dead link ]}

[6] TOI-132 b

[Kossakowski2019-7] 1 2 Kossakowski, Diana; et al. (2019), "TOI-150b and TOI-163b: Two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ", Monthly Notices of the Royal Astronomical Society, 490: 1094–1110, arXiv: 1906.09866 , doi: 10.1093/mnras/stz2433

[8] Rodriguez, Joseph E.; et al. (2019), "An Eccentric Massive Jupiter Orbiting a Subgiant on a 9.5-day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images", The Astronomical Journal, 157 (5): 191, arXiv: 1901.09950 , Bibcode:2019AJ....157..191R, doi: 10.3847/1538-3881/ab11d9 , S2CID 119314505

[9] Kostov, Veselin B.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Colón, Knicole D.; Brande, Jonathan; Collins, Karen A.; Feinstein, Adina D.; Hadden, Samuel; Kane, Stephen R.; Kreidberg, Laura; Kruse, Ethan; Lam, Christopher; Matthews, Elisabeth; Montet, Benjamin T. (2019-06-27). "The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf". The Astronomical Journal. 158 (1): 32. arXiv: 1903.08017 . Bibcode:2019AJ....158...32K. doi: 10.3847/1538-3881/ab2459 . ISSN 1538-3881.

[DemangeonZapatero_Osorio2021-10] Demangeon, O. D. S.; Zapatero Osorio, M. R.; Alibert, Y.; Barros, S. C. C.; Adibekyan, V.; Tabernero, H. M.; Antoniadis-Karnavas, A.; Camacho, J. D.; al, et (2021). "Warm terrestrial planet with half the mass of Venus transiting a nearby star" (PDF). Astronomy & Astrophysics. 653: A41. arXiv: 2108.03323 . Bibcode:2021A&A...653A..41D. doi:10.1051/0004-6361/202140728. S2CID 236957385.

[11] "Planet L 98-59 b". Extrasolar Planets Encyclopaedia . 1995. Retrieved 6 August 2021.

[Almenara2022-12] Almenara, J. M.; et al. (2022), "GJ 3090 b: One of the most favourable mini-Neptune for atmospheric characterisation", Astronomy & Astrophysics, 665: A91, arXiv: 2207.14121 , Bibcode:2022A&A...665A..91A, doi:10.1051/0004-6361/202243975, S2CID 252367299

[Dragomir2019-13] 1 2 Dragomir, Diana; et al. (2019), "TESS Delivers Its First Earth-sized Planet and a Warm Sub-Neptune", The Astrophysical Journal, 875 (2): L7, arXiv: 1901.00051 , Bibcode:2019ApJ...875L...7D, doi: 10.3847/2041-8213/ab12ed , S2CID 129945503

[14] Benatti, S.; Nardiello, D.; Malavolta, L.; Desidera, S.; Borsato, L.; Nascimbeni, V.; Damasso, M.; D'Orazi, V.; Mesa, D.; Messina, S.; Esposito, M.; Bignamini, A.; Claudi, R.; Covino, E.; Lovis, C.; Sabotta, S. (October 2019). "A possibly inflated planet around the bright young star DS Tucanae A". Astronomy & Astrophysics. 630: A81. arXiv: 1904.01591 . Bibcode:2019A&A...630A..81B. doi:10.1051/0004-6361/201935598. ISSN 0004-6361. S2CID 102486551.

[15] Maciejewski, Gracjan; Łoboda, Weronika (2025). "A Transiting Giant on a 7.7 yr Orbit Revealed by Transit Timing Variations in the TOI-201 System". The Astrophysical Journal Letters. 988 (2): L63. arXiv: 2507.11504 . Bibcode:2025ApJ...988L..63M. doi: 10.3847/2041-8213/adefe5 .

[Kipping2019-16] Teachey, Alex; Jansen, Tiffany; Bakos, Gaspar; Torres, Guillermo; Hartman, Joel; Nesvorný, David; Kipping, David (2019). "A resonant pair of warm giant planets revealed by TESS". Monthly Notices of the Royal Astronomical Society. 486 (4): 4980–4986. arXiv: 1902.03900 . doi: 10.1093/mnras/stz1141 .

[Dawson2019-17] Dawson, Rebekah I.; et al. (2019). "TOI-216b and TOI-216 c: Two Warm, Large Exoplanets in or Slightly Wide of the 2:1 Orbital Resonance". The Astronomical Journal. 158 (2): 65. arXiv: 1904.11852 . Bibcode:2019AJ....158...65D. doi: 10.3847/1538-3881/ab24ba . S2CID 135466349.

[Dawson2021-18] Dawson, Rebekah I.; Huang, Chelsea X.; Brahm, Rafael; Collins, Karen A.; Hobson, Melissa J.; Jordán, Andrés; Dong, Jiayin; Korth, Judith; Trifonov, Trifon; Abe, Lyu; Agabi, Abdelkrim; Bruni, Ivan; Butler, R. Paul; Barbieri, Mauro; Collins, Kevin I.; Conti, Dennis M.; Crane, Jeffrey D.; Crouzet, Nicolas; Dransfield, Georgina; Evans, Phil; Espinoza, Néstor; Gan, Tianjun; Guillot, Tristan; Henning, Thomas; Lissauer, Jack J.; Jensen, Eric L. N.; Sainte, Wenceslas Marie; Mékarnia, Djamel; Myers, Gordon; et al. (2021), "Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b", The Astronomical Journal, 161 (4): 161, arXiv: 2102.06754 , Bibcode:2021AJ....161..161D, doi: 10.3847/1538-3881/abd8d0 , S2CID 231924886

[Timmermans-19] 1 2 Timmermans, M.; et al. (2026-01-29). "Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs". arXiv: 2601.21774 [astro-ph.EP].

[20] Alves, Douglas R.; et al. (2026). "TOI-333b: A Neptune-desert planet around an F7V star". Astronomy & Astrophysics. 705: A210. arXiv: 2511.13832 . Bibcode:2026A&A...705A.210A. doi:10.1051/0004-6361/202557014.

[21] Tey, Evan; Shporer, Avi; Lin, Zifan; Stassun, Keivan G.; Lissauer, Jack J.; Hellier, Coel; Collins, Karen A.; Collins, Kevin I.; Wingham, Geof; Relles, Howard M.; Mallia, Franco; Isopi, Giovanni; Kielkopf, John F.; Conti, Dennis M.; Schwarz, Richard P. (2024-05-24). "GJ 238 b: A 0.57 Earth Radius Planet Orbiting an M2.5 Dwarf Star at 15.2 pc". The Astronomical Journal. 167 (6): 283. arXiv: 2407.18199 . Bibcode:2024AJ....167..283T. doi: 10.3847/1538-3881/ad3df1 . ISSN 0004-6256.

[sorae-22] 1 2 3 "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は？". sorae. 2019-07-30. Retrieved 2021-01-08.

[Eylen2021-23] 1 2 3 Van Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), "Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley", Monthly Notices of the Royal Astronomical Society stab2143, arXiv: 2101.01593 , doi: 10.1093/mnras/stab2143

[24] Mikal-Evans, Thomas; Madhusudhan, Nikku; Dittmann, Jason; Guenther, Maximilian N.; Welbanks, Luis; Vincent Van Eylen; Crossfield, Ian J. M.; Daylan, Tansu; Kreidberg, Laura (2023), "Hubble Space Telescope Transmission Spectroscopy for the Temperate Sub-Neptune TOI-270 d: A Possible Hydrogen-rich Atmosphere Containing Water Vapor", The Astronomical Journal, 165 (3): 84, arXiv: 2211.15576 , Bibcode:2023AJ....165...84M, doi: 10.3847/1538-3881/aca90b , S2CID 254044155

[25] Vines, Jose I.; et al. (2019), "NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf", Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv: 1904.07997 , doi: 10.1093/mnras/stz2349

[Kemmer2020-26] 1 2 Kemmer, J.; et al. (2020), "Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488)", Astronomy & Astrophysics, 642: A236, arXiv: 2009.10432 , Bibcode:2020A&A...642A.236K, doi:10.1051/0004-6361/202038967, S2CID 221836679

[27] "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. 22 October 2020. Retrieved 2023-11-25.

[28] "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. 14 February 2020. Retrieved 2023-11-25.

[29] Rodrigues, J.; et al. (2025-02-20). "TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO". Astronomy and Astrophysics. 695: A237. arXiv: 2502.14472 . Bibcode:2025A&A...695A.237R. doi:10.1051/0004-6361/202452887.

[Lacedelli2020-30] 1 2 3 4 Lacedelli, G.; et al. (2021), "An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561", Monthly Notices of the Royal Astronomical Society, 501 (3): 4148–4166, arXiv: 2009.02332 , doi: 10.1093/mnras/staa3728

[Weiss2020-31] 1 2 3 Weiss, Lauren M.; et al. (2021), "The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561", The Astronomical Journal, 161 (2): 56, arXiv: 2009.03071 , Bibcode:2021AJ....161...56W, doi: 10.3847/1538-3881/abd409 , S2CID 229279232

[:0-32] 1 2 Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160 (5): 229. arXiv: 1912.10186 . Bibcode:2020AJ....160..229D. doi: 10.3847/1538-3881/aba49d . hdl:1721.1/134083. S2CID 209444463.

[Gilbert2020-33] 1 2 3 Gilbert, Emily A.; Barclay, Thomas; Schlieder, Joshua E.; Quintana, Elisa V.; Hord, Benjamin J.; Kostov, Veselin B.; Lopez, Eric D.; Rowe, Jason F.; Hoffman, Kelsey; Walkowicz, Lucianne M.; Silverstein, Michele L.; Rodriguez, Joseph E.; Vanderburg, Andrew; Suissa, Gabrielle; Airapetian, Vladimir S.; Clement, Matthew S.; Raymond, Sean N.; Mann, Andrew W.; Kruse, Ethan; Lissauer, Jack J.; Colón, Knicole D.; Ravi kumar Kopparapu; Kreidberg, Laura; Zieba, Sebastian; Collins, Karen A.; Quinn, Samuel N.; Howell, Steve B.; Ziegler, Carl; Eliot Halley Vrijmoet; et al. (2020). "The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System". The Astronomical Journal. 160 (3): 116. arXiv: 2001.00952 . Bibcode:2020AJ....160..116G. doi: 10.3847/1538-3881/aba4b2 . S2CID 209862554.

[34] Suissa, Gabrielle; Wolf, Eric T.; Ravi kumar Kopparapu; Villanueva, Geronimo L.; Fauchez, Thomas; Mandell, Avi M.; Arney, Giada; Gilbert, Emily A.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Lopez, Eric; Rodriguez, Joseph E.; Vanderburg, Andrew (2020). "The First Habitable-zone Earth-sized Planet from TESS. III. Climate States and Characterization Prospects for TOI-700 D". The Astronomical Journal. 160 (3): 118. arXiv: 2001.00955 . Bibcode:2020AJ....160..118S. doi: 10.3847/1538-3881/aba4b4 . S2CID 209862275.

[35] Lacedelli, G.; Pallé, E.; Davis, Y. T.; Luque, R.; Morello, G.; Tabernero, H. M.; Zapatero Osorio, M. R.; Pozuelos, F. J.; Jankowski, D.; Nowak, G.; Murgas, F.; Orell-Miquel, J.; Akana Murphy, J. M.; Barkaoui, K.; Charbonneau, D.; Dransfield, G.; Ducrot, E.; Geraldía-González, S.; Irwin, J.; Jehin, E.; Osborne, H. L. M.; Pedersen, P. P.; Rackham, B. V.; Scott, M. G.; Timmermans, M.; Triaud, A.; Van Eylen, V. (2025). "A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771". Astronomy & Astrophysics. 698: A223. arXiv: 2504.18223 . Bibcode:2025A&A...698A.223L. doi:10.1051/0004-6361/202554161.

[Lockley-2025-06-36] Lockley, Isobel S.; Armstrong, David J.; Fernández, Jorge Fernández; Millholland, Sarah; Knierim, Henrik; Mena, Elisa Delgado; Sousa, Sergio; Collins, Karen A.; Watkins, Cristilyn N.; Howell, Steve B.; Adibekyan, Vardan; Helled, Ravit; Ziegler, Carl; Bayliss, Daniel; Briceño, César (June 2025). "The TOI-1117 Multi-planetary System: 3 sub-Neptunes, 1 in both the Neptunian Desert and Radius Valley". Monthly Notices of the Royal Astronomical Society. 541 (2): 919–938. arXiv: 2506.05521 . Bibcode:2025MNRAS.541..919L. doi: 10.1093/mnras/staf939 . ISSN 0035-8711.

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