Kepler-445c
Kepler-445c is an exoplanet orbiting the red dwarf star Kepler-445 every 5 days in the inner edge of the star's circumstellar habitable zone.[3] PHL does not consider this planet potentially habitable.[4]
| Discovery | |
|---|---|
| Discovery site | Kepler Space Observatory |
| Discovery date | 2015 |
| Transit | |
| Orbital characteristics | |
| 0.033427 AU (5,000,600 km) | |
| Eccentricity | 0 |
| 4.871229±0.000011 d | |
| Inclination | 89.91 |
| Star | Kepler-445 |
| Physical characteristics | |
Mean radius | 2.72+0.44 −0.43 REarth[1] |
| Temperature | 362 K (89 °C; 192 °F) [2] |
Physical features
With a radius of 2.72 times that of Earth, it is likely a mini-Neptune with a gaseous composition. Assuming that Kepler-445c instead has the same density as Earth, it would have a mass of 15.9 MEarth, according to the PHL exoplanet density calculator.
| Earth | Kepler-445c |
|---|---|
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References
- Mann, Andrew W.; Dupuy, Trent; Muirhead, Philip S.; Johnson, Marshall C.; Liu, Michael C.; Ansdell, Megan; Dalba, Paul A.; Swift, Jonathan J.; Hadden, Sam (2017), "THE GOLD STANDARD: ACCURATE STELLAR AND PLANETARY PARAMETERS FOR EIGHT Kepler M DWARF SYSTEMS ENABLED BY PARALLAXES", The Astronomical Journal, 153 (6): 267, arXiv:1705.01545, doi:10.3847/1538-3881/aa7140, S2CID 119325474
- "Kepler Objects of Interest".
- "Kepler-445".
- "The Habitable Exoplanets Catalog - Planetary Habitability Laboratory @ UPR Arecibo".
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