Kepler-61b
Kepler-61b (also known by its Kepler Object of Interest designation KOI-1361.01) is a super-Earth exoplanet orbiting within parts of the habitable zone of the K-type main-sequence star Kepler-61. It is located about 1,100 light-years (338 parsecs) from Earth in the constellation of Cygnus. It was discovered in 2013 using the transit method, in which the dimming effect that a planet causes as it crosses in front of its star is measured, by NASA's Kepler spacecraft.
Discovery | |
---|---|
Discovered by | Kepler spacecraft |
Discovery date | 24 April 2013 |
Transit | |
Orbital characteristics | |
0.26 AU (39,000,000 km) | |
Eccentricity | <0.25 |
59.87756 d | |
Inclination | >89.80 |
Star | Kepler-61 (KOI-1361) |
Physical characteristics | |
Mean radius | 2.15 ± 0.13 R🜨 |
Mass | 6.65 ME |
Temperature | 273 K (0 °C; 32 °F) |
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