Kepler-395c
Kepler-395c is a potentially habitable exoplanet 616 light-years away in the constellation of Cygnus.[2]
Discovery | |
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Discovered by | Jason F. Rowe et al.[1] |
Discovery site | Kepler |
Discovery date | February 26, 2014 |
Transit method | |
Orbital characteristics | |
34.989262[1] d | |
JD 2454977.22265[1] | |
Star | Kepler-395 |
Physical characteristics | |
Mean radius | 1.32[1] R🜨 |
Mean density | 2.7856 g/cm3 (0.10064 lb/cu in)[1] |
Habitability and Properties
It orbits an M-type star. It's radius is 1.32 ± 0.09 times that of Earth.[1] It orbits at 0.177 AU[3] with an orbital period of 34.9893 days.[1] Because of its proximity to its star, it's likely to be tidally locked, meaning one side always facing the star, and one side always facing away. This means one side is blistering hot, and one side is bitter cold. However, in between those hostile zones, there would be a sliver of habitability. If it has a thick enough atmosphere, the sliver may even be global.
Earth | Kepler-395c |
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See also
References
- Rowe, Jason F.; et al. (2014). "Validation of Kepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-planet Systems". The Astrophysical Journal. 784 (1): 20. arXiv:1402.6534. Bibcode:2014ApJ...784...45R. doi:10.1088/0004-637X/784/1/45. S2CID 119118620. 45.
- Muirhead, Philip S; Becker, Juliette; Feiden, Gregory A; Rojas-Ayala, Bárbara; Vanderburg, Andrew; Price, Ellen M; Thorp, Rachel; Law, Nicholas M; Riddle, Reed; Baranec, Christoph; Hamren, Katherine; Schlawin, Everett; Covey, Kevin R; Johnson, John Asher; Lloyd, James P (2014). "Characterizing the Cool KOIs. VI. H- and K-band Spectra of Kepler M Dwarf Planet-Candidate Hosts". The Astrophysical Journal Supplement Series. 213 (1): 5. arXiv:1406.2718. Bibcode:2014ApJS..213....5M. doi:10.1088/0067-0049/213/1/5. S2CID 12296808.
- "Kepler-395 c". exoplanets.nasa.gov. Retrieved 26 December 2020.
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