CoRoT-8: Difference between revisions
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{{AFC comment|1=See [[WP:NASTCRIT]] for guidelines on the notability of astronomical objects. Furthermore, please provide a different link to the journal that study was published in, which does not use Arxiv, per [[WP:ArXiv]]. [[User:ARandomName123|ARandomName123]] ([[User talk:ARandomName123|talk]])<sup><span style="color:Green"><small>Ping me!</small></span></sup> 21:26, 23 August 2023 (UTC)}} |
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{{Short description|Star in Aquila }} |
{{Short description|Star in Aquila }} |
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CoRoT-8 is a star in the [[constellation Aquila]] at a distance of about 1239 light-years from us. At least one planet revolves around a star. |
CoRoT-8 is a star in the [[constellation Aquila]] at a distance of about 1239 light-years from us. At least one planet revolves around a star. |
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== References == |
== References == |
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Revision as of 21:26, 23 August 2023
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Comment: See WP:NASTCRIT for guidelines on the notability of astronomical objects. Furthermore, please provide a different link to the journal that study was published in, which does not use Arxiv, per WP:ArXiv. ARandomName123 (talk)Ping me! 21:26, 23 August 2023 (UTC)
CoRoT-8 is a star in the constellation Aquila at a distance of about 1239 light-years from us. At least one planet revolves around a star.
Characteristics
CoRoT-8 is an orange dwarf which has 0.88 solar masses and 0.77 solar radius. [1]. By astronomical standards, this is already a rather young star compared to the Sun: its age is about 3 billion years. It got its name in honor of the CoRoT space telescope, with the help of which her planetary companion was discovered.
Planetary system
In 2010, a group of astronomers working within the CoRoT program announced the discovery of the planet CoRoT-8b in this system. It is a hot gas giant, similar in mass and size to Saturn. The planet orbits at a distance of about 0.06 AU. e. from the parent star, while making a complete revolution in 6.21 days.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.218 ± 0.034 MJ | 0.0636 ± 0.0014 | 6.212445 ± 0.000007 | 0.19 | — | — |
References
- ^ P. Bordé, F. Bouchy, M. Deleuil, J. Cabrera, L. Jorda, C. Lovis, S. Csizmadia, S. Aigrain, J. M. Almenara, R. Alonso, M. Auvergne, A. Baglin, P. Barge, W. Benz, A. S. Bonomo, H. Bruntt, L. Carone, S. Carpano, H. Deeg, R. Dvorak, A. Erikson, S. Ferraz-Mello, M. Fridlund, D. Gandolfi, J.-C. Gazzano, M. Gillon, E. Guenther, T. Guillot, P. Guterman, A. Hatzes, M. Havel, G. Hébrard, H. Lammer, A. Léger, M. Mayor, T. Mazeh, C. Moutou, M. Pätzold, F. Pepe, M. Ollivier, D. Queloz, H. Rauer, D. Rouan, B. Samuel, A. Santerne, J.Schneider, B. Tingley, S. Udry, J. Weingrill, G. Wuchterl (2010-08-02). "Transiting exoplanets from the CoRoT space mission. XI. CoRoT-8b: a hot and dense sub-Saturn around a K1 dwarf". Arxiv.org. Archived from the original on 2017-03-05. Retrieved 2010-08-12.
{{cite web}}: CS1 maint: multiple names: authors list (link)
