
Kepler-767 b
Also written Kepler-767b, Kepler 767b, Kepler 767 b
- Mass
- 35.70 × Earth
- Radius
- 6.64 × Earth
- Gravity
- 0.81 g
- Surface (est.)
- 478 K
- Year
- 162 days
- From Earth
- 7,339 ly
- Mass
- 35.70 × Earth
- Radius
- 6.64 × Earth
- Gravity
- 0.81 g
- Surface (est.)
- 478 K
- Year
- 162 days
- From Earth
- 7,339 ly
Kepler-767 system
- Type
- G-type (Yellow (Sun-like))
- Temperature
- 5,694 K
- Radius
- 0.94 ☉
- Mass
- 0.96 ☉
- Planets
- 1
- Luminosity
- 2.99 ☉
Published by the NASA Exoplanet Archive. This world’s temperature and habitability score are computed from this star’s measured luminosity, not from a stand-in for its class.
Kepler-767 b0.59 AUYou are here36 M⊕Star and planets drawn to scale: the star is 15 times as wide as Kepler-767 b, so only its edge is in view. Orbits spaced as in the star system view.
Kepler-767 b, from the NASA Exoplanet Archive (found 2016). Measured: 35.7 Earth masses, 0.587 AU, a 5694 K G-type star. Composition inferred from a measured bulk density of 0.12x Earth's, which only hydrogen and helium can explain, with an assumed 24-hour day — rotation cannot be measured for exoplanets. Note: TerraForge comes out at 478 K against the archive's 366 K, because it models stars by spectral class, and Kepler-767 is not an average G-type.
Surface. No solid surface - thick gaseous envelope with possible rocky core deep within
Hydrogen and helium dominated with trace methane and ammonia
Hydrogen-rich atmosphere typical of gas giants


