TOI-1431 b
In this article, TOI-1431 b will be addressed from various perspectives, with the aim of delving into its importance, incidence and relevance today. Along these lines, different aspects related to TOI-1431 b will be analyzed, focusing on its evolution over time, its impact on society and its influence in different areas. Likewise, relevant data, studies and reflections will be presented that will allow the reader to obtain a comprehensive and enriching vision about TOI-1431 b. From its origins to its current situation, through its implications in the cultural, social, political or economic sphere, this article aims to shed light on TOI-1431 b and generate a space for reflection and debate around this very transcendental topic.
| Discovery | |
|---|---|
| Discovered by | TESS, MASCARA |
| Discovery date | 2021 |
| Transit | |
| Orbital characteristics | |
| 0.046 | |
| Eccentricity | 0 |
| 2.7 d | |
| Inclination | 80.4 |
| Star | TOI-1431 |
| Physical characteristics | |
| 1.49 RJ | |
| Mass | 3.12 MJ |
| Temperature | 2700±2600 K |
TOI-1431 b, also known as MASCARA-5b, is an ultra-hot Jupiter exoplanet orbiting TOI-1431 in the constellation of Cepheus. It has an orbital period of 2.7 days.[1] Its dayside temperature is 2,700 K (2,427 °C), making it hotter than 40% of stars in our galaxy.[2] The nightside temperature is 2,600 K (2,300 °C).[3][4][5]
References
- ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2023-09-05.
- ^ "Scientists uncover a 'hellish' planet so hot it could vaporize most metals". CNET. April 27, 2021. Retrieved April 27, 2021.
- ^ "'Hellish' new planet discovered". University of Southern Queensland. April 27, 2021. Retrieved April 27, 2021.
- ^ Brett Christopher Addison; et al. (2021), "TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars", Posters from the Tess Science Conference Ii (Tsc2: 64, arXiv:2104.12078, Bibcode:2021tsc2.confE..64A, doi:10.5281/zenodo.5126266, S2CID 240578462
- ^ Stangret, M.; et al. (2021), "The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions", Astronomy & Astrophysics, 654: A73, arXiv:2104.12414, Bibcode:2021A&A...654A..73S, doi:10.1051/0004-6361/202040100, S2CID 233393996
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