Discovery | |
---|---|
Discovered by | Kepler spacecraft |
Discovery date | May 12, 2016 |
transit | |
Orbital characteristics | |
0.2896 AU (43,320,000 km)[nb 1] | |
Eccentricity | ~0 |
86.829[1] d | |
Inclination | ~89.5 |
Star | Kepler-1229 (KOI-2418) |
Physical characteristics | |
1.40+0.11 −0.13[2][nb 2] R🜨 | |
Mass | ~2.7[3] ME |
Temperature | 213 K (−60 °C; −76 °F) |
Kepler-1229b[1] (also known by its Kepler Object of Interest designation KOI-2418.01) is a confirmed super-Earth exoplanet, likely rocky, orbiting within the habitable zone of the red dwarf Kepler-1229, located about 870 light years (267 parsecs) from Earth in the constellation of Cygnus.[4][2] It was discovered in 2016 by the Kepler space telescope.[5] The exoplanet was found by using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured.
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