|Extrasolar planet||List of extrasolar planets|
|Right ascension||(α)||18h 52m 51.06019s|
|Declination||(δ)||+45° 20′ 59.507″|
|Mass||(m)||0.69 (± 0.02) M☉|
|Radius||(r)||0.64 (± 0.02) R☉|
|Temperature||(T)||4925 (± 70) K|
|Metallicity||[Fe/H]||-0.37 (± 0.04)|
|Age||7 (± 4) Gyr|
|Radius||(r)||1.61 (± 0.05) R⊕|
|Stellar flux||(F⊙)||1.2 ± 0.2 ⊕|
|Semimajor axis||(a)||0.427 AU|
|Orbital period||(P)||122.3874 d|
|Discovery date||18 April 2013|
|Discoverer(s)||Borucki et al.|
|Discovery method||Transit (Kepler Mission)|
|Other detection methods||Transit timing variation|
|Discovery site||Kepler Space Observatory|
|Discovery status||Published refereed article|
Kepler-62e is a super-Earth exoplanet (extrasolar planet) discovered in orbit around the star Kepler-62, the second outermost of five such planets discovered by NASA's Kepler spacecraft. Kepler-62e is located about 1,200 ly (370 pc) from Earth in the constellation of Lyra. The exoplanet was found using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured. Kepler-62e is most likely a terrestrial planet in the inner part of its host star's habitable zone and has an Earth Similarity Index of 0.83.
Given the planet's age (7 ± 4 billion years), stellar flux (1.2 ± 0.2 times Earth's) and radius (1.61 ± 0.05 times Earth's), a rocky (silicate-iron) composition with the addition of a possibly substantial amount of water is considered plausible. A modeling study accepted in The Astrophysical Journal suggests it is likely that a great majority of planets in Kepler-62e's size range are completely covered by ocean.
Kepler-62e orbits its host star every 122 days and is roughly 60 percent larger than Earth.
- "Kepler Input Catalog search result". Space Telescope Science Institute. Retrieved 2013-04-18.
- Borucki, William J.; et al. (18 April 2013). "Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone". Science Express 340 (6132): 587. arXiv:1304.7387. Bibcode:2013Sci...340..587B. doi:10.1126/science.1234702. Retrieved 18 April 2013.
- PHL's Exoplanets Catalog - Planetary Habitability Laboratory @ UPR Arecibo
- Kepler-62e: Super-Earth and Possible Water World
- 3 Potentially Habitable 'Super-Earths' Explained (Infographic)
- "Water worlds surface: Planets covered by global ocean with no land in sight". Harvard Gazette. 2013-04-18. Retrieved 2013-04-19.
- Kaltenegger, L.; Sasselov, D.; Rugheimer, S. (2013-04-18 [preprint]). "Water Planets in the Habitable Zone: Atmospheric Chemistry, Observable Features, and the case of Kepler-62e and −62f". The Astrophysical Journal 1304: 5058. arXiv:1304.5058. Bibcode:2013arXiv1304.5058K.
- Super-Earths: Two Earth-like planets that could host life discovered. Indian Express. April 20, 2013
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