astro.wikisort.org - MeteoriteKepler-56c is a hot Jupiter[2] (a class of exoplanets) orbiting the star Kepler-56, located in the constellation Cygnus. It was discovered by the Kepler telescope in October 2013. It orbits its parent star only 0.17 AU (16 million mi; 25 million km) away, and at its distance it completes an orbit once every 21.4 days.[1] Its orbit is significantly misaligned with its parent star's equator.[1]
Hot Jupiter orbiting Kepler-56
Kepler-56c A diagram of the planetary system of Kepler-56 |
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Discovered by | Daniel Huber et al.[1] |
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Discovery date | 16 October 2013 |
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Detection method | Transit method |
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Semi-major axis | 0.1652 ± 0.0059 AU (24,710,000 ± 880,000 km)[1] |
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Orbital period (sidereal) | 21.40239+0.00059 −0.00062[1] d |
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Star | Kepler-56 |
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Mean radius | 9.80 ± 0.46[1] REarth |
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Mass | 181+21 −19[1] MEarth |
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Mean density | 1.06+0.14 −0.13 g cm−3 |
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Both Kepler-56b and Kepler-56c will be devoured by their parent star in about 130 and 155 million years.[3] Further research shows that it will have its atmosphere boiled away by intense heat from the star, and it will be stretched by the strengthening stellar tides.[3]
References
- Huber, D.; et al. (2013). "Stellar Spin-Orbit Misalignment in a Multiplanet System". Science. 342 (6156): 331–4. arXiv:1310.4503. Bibcode:2013Sci...342..331H. doi:10.1126/science.1242066. PMID 24136961. S2CID 1056370.
- Huber, Daniel; Carter, Joshua A.; Barbieri, Mauro; Miglio, Andrea; Deck, Katherine M.; Fabrycky, Daniel C.; Montet, Benjamin T.; Buchhave, Lars A.; Chaplin, William J.; Hekker, Saskia; Montalbán, Josefina (2013-10-18). "Stellar Spin-Orbit Misalignment in a Multiplanet System". Science. 342 (6156): 331–334. doi:10.1126/science.1242066.
- Charles Poladian (2014-06-03). "Cosmic Snack: Planets Kepler-56b And Kepler-56c Will Be Swallowed Whole By Host Star". International Business Times. Retrieved 7 August 2017.
External links
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