astro.wikisort.org - Meteorite

Search / Calendar

Kepler-395c is a potentially habitable[citation needed] exoplanet 616 light-years away in the constellation of Cygnus.[2]

Kepler-395c
Discovery
Discovered byJason F. Rowe et al.[1]
Discovery siteKepler
Discovery dateFebruary 26, 2014
Detection method
Transit method
Orbital characteristics
Orbital period (sidereal)
34.989262[1] d
Time of periastron
JD 2454977.22265[1]
StarKepler-395
Physical characteristics
Mean radius
1.32[1] REarth
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.[citation needed]

    Size comparison
    Earth Kepler-395c

    See also



    References


    1. 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. 45.
    2. 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: 5. arXiv:1406.2718. Bibcode:2014ApJS..213....5M. doi:10.1088/0067-0049/213/1/5.
    3. "Kepler-395 c". exoplanets.nasa.gov. Retrieved 26 December 2020.

    This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it.

    • v
    • t
    • e

    На других языках

    - [en] Kepler-395c

    [es] Kepler-395c

    Kepler-395c, también denominado KOI-2650.01, es un exoplaneta confirmado descubierto en 2012 por el telescopio espacial Kepler, siendo el primer planeta encontrado en torno al sistema Kepler-395 (posteriormente se descubrió un segundo, KOI-2650.02).[1] Las primeras observaciones indicaron un posible carácter habitable del mismo, pero quedó descartado como análogo terrestre tras comprobar que su estrella es mayor de lo previsto (suponiendo una temperatura superficial para el planeta considerablemente mayor).


    Текст в блоке "Читать" взят с сайта "Википедия" и доступен по лицензии Creative Commons Attribution-ShareAlike; в отдельных случаях могут действовать дополнительные условия.

    Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.

    2019-2025
    WikiSort.org - проект по пересортировке и дополнению контента Википедии