List of exoplanets discovered by the TESS mission
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 (MJ) | Radius (RJ) | 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 | 0.73±0.07 | 4640±100 | [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 | 0.77 | 5026±125 | |||
| 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 | 0.360±0.016 | 3347±54 | 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 | |||||||
| 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 | 0.740±0.087 | 4675±53 | ||||||
| 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] | |
See also
- Lists of exoplanets
- List of exoplanets discovered in 2018
- List of exoplanets discovered in 2019
- List of exoplanets discovered in 2020
- List of exoplanets discovered in 2021
- List of exoplanets discovered in 2022
- List of exoplanets discovered in 2023
- List of exoplanets discovered in 2024
- List of exoplanets discovered in 2025
- List of exoplanets discovered in 2026
- List of exoplanets discovered by the Kepler space telescope
- Exoplanet
Notes
Reference
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{{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
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External links
- List of TOIs at IPAC's ExoFOP