Kepler-69
Kepler-69 (KOI-172, 2MASS J19330262+4452080, KIC 8692861) is a G-type main-sequence star similar to the Sun in the constellation Cygnus, located about 2,430 ly (750 pc) from Earth. On April 18, 2013 it was announced that the star has two planets. Although initial estimates indicated that the terrestrial planet Kepler-69c might be within the star's habitable zone, further analysis showed that the planet very likely is interior to the habitable zone and is far more analogous to Venus than to Earth and thus completely inhospitable.
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Kepler-69
Kepler-69 (KOI-172, 2MASS J19330262+4452080, KIC 8692861) is a G-type main-sequence star similar to the Sun in the constellation Cygnus, located about 2,430 ly (750 pc) from Earth. On April 18, 2013 it was announced that the star has two planets. Although initial estimates indicated that the terrestrial planet Kepler-69c might be within the star's habitable zone, further analysis showed that the planet very likely is interior to the habitable zone and is far more analogous to Venus than to Earth and thus completely inhospitable.
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Kepler-69 (KOI-172, 2MASS J193 ...... thus completely inhospitable.
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Comparison of Planet Sizes - Kepler-69c, Kepler-62e, Kepler-62f, and Earth.
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Comparison of the Kepler-69 System and the Solar System
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Kepler-69c, a Super-Earth-size exoplanet orbiting Kepler-69, a star like the Sun.
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G4V
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NASA Ames/JPL-Caltech
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Kepler-69
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J2000
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Kepler-69
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Simbad
KOI-172
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Kepler-69c - a Venus-like exoplanet orbiting a Sun-like star
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Kepler-69 (KOI-172, 2MASS J193 ...... thus completely inhospitable.
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Kepler-69
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Kepler-69
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