Transiting brown dwarfs at a glance
This is a table of the known transiting brown dwarf population as of September 2023 (white dwarf host stars to be added). This table is sorted by the mass of the brown dwarf in ascending order. Additional details for each system are linked at the buttons below. A recent citable publication including this table is here.
| Brown dwarf name | Mass (MJ) | Radius (RJ) | Period (Days) | Eccentricity | Host star Teff (K) | RA/DEC | Reference |
|---|---|---|---|---|---|---|---|
| HATS-70b | 12.9 ± 1.8 | 1.38 ± 0.08 | 1.9 | < 0.18 | 7930 ± 820 | 109.104, -31.244 | Zhou et al. 2019 |
| TOI-1278b | 18.5 ± 0.5 | 1.09 ± 0.24 | 14.5 | < 0.02 | 3799 ± 42 | 320.478, +35.648 | Artigau et al. 2021 |
| Kepler-39b | 19.0 ± 1.3 | 1.07 ± 0.03 | 21.1 | 0.07 ± 0.03 | 6290 ± 120 | 296.960, +46.034 | Bouchy et al. 2011 |
| GPX-1b | 19.7 ± 1.6 | 1.47 ± 0.10 | 1.7 | 0.0 | 7000 ± 200 | 38.369, +56.025 | Benni et al. 2020 |
| CoRoT-3b | 22.5 ± 1.0 | 1.06 ± 0.07 | 4.3 | < 0.04 | 6740 ± 150 | 292.055, +0.121 | Deleuli et al. 2008 |
| KELT-1b | 27.9 ± 1.0 | 1.13 ± 0.03 | 1.2 | < 0.01 | 6519 ± 47 | 0.362, +39.383 | Siverd et al. 2012 |
| NLTT 41135b | 33.7 ± 2.8 | 1.13 ± 0.27 | 2.9 | < 0.02 | 3230 ± 130 | 236.518, +4.690 | Irwin et al. 2010 |
| WASP-128b | 37.2 ± 0.9 | 0.94 ± 0.02 | 2.2 | < 0.01 | 5950 ± 50 | 172.858, -41.689 | Hodžić et al. 2018 |
| CWW 89Ab | 39.2 ± 1.1 | 0.94 ± 0.02 | 5.3 | 0.19 ± 0.01 | 5755 ± 49 | 289.391, -16.871 | Nowak et al. 2017 |
| KOI-205b | 40.2 ± 1.8 | 0.81 ± 0.02 | 11.7 | < 0.02 | 5289 ± 86 | 295.496, +42.537 | Díaz et al. 2013 |
| TOI-1406b | 46.0 ± 2.7 | 0.86 ± 0.03 | 10.6 | < 0.04 | 6290 ± 100 | 82.127, -48.409 | Carmichael et al. 2020 |
| EPIC 212036875b | 52.3 ± 1.9 | 0.87 ± 0.02 | 5.2 | 0.13 ± 0.01 | 6238 ± 60 | 134.690, +20.868 | Carmichael et al. 2019 |
| TOI-503b | 53.7 ± 1.2 | 1.34 ± 0.26 | 3.7 | 0.0 | 7650 ± 160 | 124.320, +12.601 | Ŝubjak et al. 2019 |
| TOI-852b | 53.7 ± 1.4 | 0.83 ± 0.04 | 4.9 | < 0.01 | 5768 ± 84 | 24.740, -7.280 | Carmichael et al. 2021 |
| AD 3116b | 54.6 ± 6.9 | 0.95 ± 0.07 | 2.0 | 0.14 ± 0.05 | 3165 ± 53 | 130.664, +19.414 | Gillen et al. 2017 |
| CoRoT-33b | 59.0 ± 1.8 | 1.10 ± 0.53 | 5.8 | 0.07 ± 0.01 | 5225 ± 80 | 279.641, +5.624 | Csizmadia et al. 2015 |
| RIK 72b | 59.2 ± 6.8 | 3.10 ± 0.31 | 97.8 | 0.15 ± 0.01 | 3349 ± 142 | 240.913, -18.858 | David et al. 2019 |
| TOI-811b | 59.9 ± 8.6 | 1.26 ± 0.06 | 25.2 | 0.51 ± 0.08 | 6107 ± 77 | 88.030, -32.925 | Carmichael et al. 2021 |
| WASP-30b | 60.8 ± 3.3 | 0.78 ± 0.04 | 4.2 | < 0.01 | 6130 ± 120 | 358.408, -10.118 | Triaud et al. 2013 |
| TOI-263b | 61.6 ± 4.0 | 0.91 ± 0.07 | 0.56 | < 0.02 | 3471 ± 33 | 37.108, -25.097 | Palle et al. 2021 |
| LHS 6343c | 62.9 ± 2.3 | 0.83 ± 0.02 | 12.7 | 0.06 ± 0.03 | 3750 ± 125 | 287.559, +46.957 | Johnson et al. 2011 |
| TOI-569b | 63.8 ± 1.0 | 0.75 ± 0.02 | 6.6 | < 0.01 | 5705 ± 76 | 115.102, -42.154 | Carmichael et al. 2020 |
| CoRoT-15b | 64.0 ± 5.0 | 0.94 ± 0.12 | 3.1 | < 0.08 | 6340 ± 190 | 97.115, +6.186 | Bouchy et al. 2011 |
| TOI-1982b | 65.8 ± 2.8 | 1.08 ± 0.04 | 17.2 | 0.27 ± 0.01 | 6325 ± 110 | 207.585, -23.383 | Psaridi et al. 2022 |
| KOI-415b | 66.9 ± 3.6 | 0.82 ± 0.02 | 166.8 | 0.70 ± 0.01 | 5840 ± 80 | 293.306, +41.606 | Moutou et al. 2013 |
| TOI-2119b | 67.0 ± 2.0 | 1.11 ± 0.03 | 7.2 | 0.34 ± 0.01 | 3553 ± 67 | 244.430, +26.304 | Cañas et al. 2022 |
| TOI-629b | 67.0 ± 3.0 | 1.11 ± 0.05 | 8.7 | 0.30 ± 0.01 | 9100 ± 200 | 95.828, +0.883 | Psaridi et al. 2022 |
| TOI-2543b | 67.6 ± 3.5 | 0.95 ± 0.09 | 7.5 | 0.01 ± 0.01 | 6060 ± 82 | 136.597, +3.567 | Psaridi et al. 2022 |
| TOI-588b | 68.0 ± 7.4 | 1.58 ± 0.07 | 39.5 | 0.56 ± 0.03 | 10400 ± 800 | 104.750, -47.023 | Vowell et al. 2023 |
| LP 261-75b | 68.1 ± 2.1 | 0.90 ± 0.02 | 1.9 | < 0.01 | 3100 ± 50 | 147.768, +35.968 | Irwin et al. 2018 |
| EPIC 201702477b | 68.1 ± 2.7 | 0.86 ± 0.05 | 40.7 | 0.28 ± 0.01 | 5602 ± 64 | 175.240, +3.681 | Bayliss et al. 2017 |
| NGTS-19b | 69.5 ± 5.7 | 1.03 ± 0.06 | 17.8 | 0.37 ± 0.01 | 4500 ± 110 | 229.131, -25.705 | Acton et al. 2021 |
| TOI-2336b | 69.9 ± 2.3 | 1.05 ± 0.04 | 7.71 | 0.01 ± 0.03 | 6433 ± 84 | 230.230, -33.692 | Lin et al. 2023 |
| CoRoT-34b | 71.4 ± 8.9 | 1.09 ± 0.17 | 2.1 | 0.0 | 7820 ± 160 | 102.8708, -3.8175 | Sebastian et al. 2022 |
| NGTS-7Ab | 75.5 ± 13.7 | 1.38 ± 0.14 | 0.7 | 0.0 | 3359 ± 106 | 352.521, -38.969 | Jackman et al. 2019 |
| TOI-148b | 77.1 ± 5.8 | 0.81 ± 0.06 | 4.9 | < 0.01 | 5990 ± 140 | 338.320, -38.159 | Grieves et al. 2021 |
| TOI-2521b | 77.5 ± 3.3 | 1.01 ± 0.04 | 5.56 | < 0.04 | 5625 ± 74 | 93.529, -8.062 | Lin et al. 2023 |
| Kepler-503b | 78.6 ± 3.1 | 0.96 ± 0.06 | 7.26 | 0.03 ± 0.01 | 5670 ± 110 | 290.636, +38.708 | Cañas et al. 2018 |
| ZTF J2020+5033 | 80.1 ± 1.6 | 1.05 ± 0.02 | 0.079 | 0.0 | 2856 ± 6 | 305.014, +50.560 | El-Badry et al. 2023 |
| KOI-189b | 80.4 ± 2.5 | 0.99 ± 0.02 | 30.4 | 0.27 ± 0.01 | 4973 ± 84 | 284.879, +49.267 | Díaz et al. 2014 |
| TOI-587b | 81.1 ± 7.1 | 1.35 ± 0.07 | 8.0 | 0.04 ± 0.01 | 9800 ± 200 | 130.395, -22.194 | Grieves et al. 2021 |
| TOI-746b | 82.2 ± 4.9 | 0.95 ± 0.09 | 11.0 | 0.20 ± 0.01 | 5690 ± 140 | 99.620, -67.648 | Grieves et al. 2021 |