 An image of HATS-36 taken using the Kepler Space Telescope | |
| Discovery[1] | |
|---|---|
| Discovery date | June 12, 2017 |
| Transit | |
| Designations | |
| K2-145 b or EPIC 215969174b | |
| Orbital characteristics[2] | |
| 0.0529 (± 0.0011) AU | |
| Eccentricity | 0.105 ± 0.028 |
| 4.17524 (± 2.1×10−6) day | |
| Inclination | 87.57 (± 0.36)° |
| Star | HATS-36 |
| Physical characteristics | |
| 1.235 ± 0.043 RJ | |
| Mass | 2.79 ± 0.40 MJ |
HATS-36b is a gas giant exoplanet that orbits an F-type star. Its mass is 3.216 Jupiters, it takes 4.2 days to complete one orbit of its star, and is 0.05425 AU from it. It was discovered on June 12, 2017 and was announced in 2018.[3][4] Its discoverers were 23, namely Daniel Bayliss, Joel Hartman, George Zhou, Gaspar Á. Bakos, Andrew Vanderburg, J. Bento, L. Mancini, S. Ciceri, Rafael Brahm, Andres Jordán, N. Espinoza, M. Rabus, T. G. Tan, K. Penev, W. Bhatti, M. de Val-Borro, V. Suc, Z. Csubry, Th. Henning, P. Sarkis, J. Lázár, I. Papp, P. Sári.[5]
- ^ Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á.; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S.; Brahm, R.; Jordán, A.; Espinoza, N.; Rabus, M.; Tan, T. G.; Penev, K.; Bhatti, W.; de Val-Borro, M.; Suc, V.; Csubry, Z.; Henning, Th.; Sarkis, P.; Lázár, J.; Papp, I.; Sári, P. (2017). "HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program". The Astronomical Journal. 155 (3): 119. arXiv:1706.03858. doi:10.3847/1538-3881/aaa8e6. S2CID 119383417.
- ^ "The Extrasolar Planet Encyclopaedia — HATS-36 b". Extrasolar Planets Encyclopaedia.
- ^ "HATS-36 b | New World Atlas - Exoplanet Exploration: Planets Beyond our Solar System". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2018-07-05.
- ^ "HAT-36 b". www.exoplanetkyoto.org. Retrieved 2018-07-05.
- ^ Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S.; Brahm, R. (2017-06-12). "HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program". The Astronomical Journal. 155 (3): 119. arXiv:1706.03858. doi:10.3847/1538-3881/aaa8e6. S2CID 119383417.