Kepler-395c
Potential goldilocks Super-Earth orbiting Kepler-395
Kepler-395c is a potentially habitable[citation needed] exoplanet 616 light-years away in the constellation of Cygnus.[2]
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]
| Earth | Kepler-395c |
|---|---|
 |  |
See also
- Kepler-186e
- Kepler-186f
- Kepler-438b
- Kepler-442b
- Kepler-296e
- Kepler-62e
- Kepler-69c
- Kepler-395b
References
- ^ a b c d e f g 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.
- v
- t
- e
Exoplanets
and
types
and
evolution
- Accretion
- Accretion disk
- Asteroid belt
- Circumplanetary disk
- Circumstellar disc
- Circumstellar envelope
- Cosmic dust
- Debris disk
- Detached object
- Disrupted planet
- Excretion disk
- Exozodiacal dust
- Extraterrestrial materials
- Extraterrestrial sample curation
- Giant-impact hypothesis
- Gravitational collapse
- Hills cloud
- Internal structure
- Interplanetary dust cloud
- Interplanetary medium
- Interplanetary space
- Interstellar cloud
- Interstellar dust
- Interstellar medium
- Interstellar space
- Kuiper belt
- List of interstellar and circumstellar molecules
- Merging stars
- Molecular cloud
- Nebular hypothesis
- Oort cloud
- Outer space
- Planetary migration
- Planetary system
- Planetesimal
- Planet formation
- Protoplanetary disk
- Ring system
- Rubble pile
- Sample-return mission
- Scattered disc
- Star formation
- Astrobiology
- Astrooceanography
- Circumstellar habitable zone
- Earth analog
- Extraterrestrial liquid water
- Galactic habitable zone
- Habitability of binary star systems
- Habitability of F-type main-sequence star systems
- Habitability of K-type main-sequence star systems
- Habitability of natural satellites
- Habitability of neutron star systems
- Habitability of red dwarf systems
- Habitability of yellow dwarf systems
- Habitable zone for complex life
- List of potentially habitable exoplanets
- Tholin
- Superhabitable planet
- Exoplanetary systems
- Exoplanets
- Discoveries
- Extremes
- Firsts
- Nearest
- Largest
- Heaviest
- Terrestrial candidates
- Kepler
- 1–500
- 501–1000
- 1001–1500
- 1501–2000
- K2
- Potentially habitable
- Proper names
- Carl Sagan Institute
- Exoplanet naming convention
- Exoplanet phase curves
- Exoplanetary Circumstellar Environments and Disk Explorer
- Extragalactic planet
- Extrasolar planets in fiction
- Geodynamics of terrestrial exoplanets
- Neptunian desert
- Nexus for Exoplanet System Science
- Planets in globular clusters
- Small planet radius gap
- Sudarsky's gas giant classification
Portals:
Astronomy
Biology
 | This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |
- v
- t
- e
