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Kepler-283c 
Summary
Kepler-283c is an exoplanet orbiting the K-type star Kepler-283 every 93 days in the circumstellar habitable zone, discovered by the Kepler space telescope in 2014.[4]
| Discovery | |
|---|---|
| Discovery site | Kepler Space Observatory |
| Discovery date | 2014 |
| Transit | |
| Orbital characteristics | |
| 0.336144±2.93e-06[1] AU | |
| Eccentricity | 0 |
| 92.750106±0.001214 d | |
| Inclination | 88.43±0.846 |
| Star | Kepler-283 |
| Physical characteristics | |
Mean radius | 1.82 R🜨 |
| ≙9.11 hr[2] | |
| Temperature | 238.5 K (−34.6 °C; −30.4 °F) [3] |
Characteristics edit
Mass, radius and temperature edit
It has a surface equilibrium temperature of 238.5 K (−34.6 °C; −30.4 °F).[3] Its radius is 1.82 R🜨. Its orbit is circular with an eccentricity of 0.
Host star edit
The planet orbits a late orange dwarf star called Kepler-283, spectral type K7V, about 1,596 light years from Earth in the constellation of Cygnus.[5]
Orbit edit
The planet orbits its star every 93 days, at a distance of around 0.336 AU
References edit
- ^ "HEC: Exoplanets Calculator - Planetary Habitability Laboratory @ UPR Arecibo". phl.upr.edu. Archived from the original on 2017-08-24. Retrieved 2015-08-27.
- ^ Hall, C.; Stancil, P. C.; Terry, J. P.; Ellison, C. K. (2023). "A New Definition of Exoplanet Habitability: Introducing the Photosynthetic Habitable Zone". The Astrophysical Journal Letters. 948 (2): L26. arXiv:2301.13836. Bibcode:2023ApJ...948L..26H. doi:10.3847/2041-8213/acccfb.Table 2
- ^ a b "K01298.02". exoplanetarchive.ipac.caltech.edu.
- ^ "Kepler-283 c". exoplanetarchive.ipac.caltech.edu.
- ^ "SIMBAD Query Result: Kepler-283 -- Rotating Variable". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 1 February 2023.