Astronomy:Kepler-1649b
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Short description: Venus-like exoplanet orbiting Kepler-1649
Discovery | |
---|---|
Discovered by | Kepler spacecraft |
Discovery date | 15 April 2020 |
Transit | |
Orbital characteristics | |
0.0514 ± 0.0028 AU | |
Orbital period | 8.689099 ± 0.000025 d |
Inclination | 89.150 |
Star | Kepler-1649 |
Physical characteristics | |
Mean radius | 1.017 ± 0.051 R⊕ |
Mass | 1.03 M⊕ |
Kepler-1649b is a Venus-like exoplanet orbiting Kepler-1649. [1]
Host star
Kepler-1649 is a type-M red dwarf star estimated to be roughly ¼ the radius of the Sun [2] with only two confirmed planets in its orbit, the other being Kepler-1649c.[3] Kepler-1649c is similar to Earth from our own solar system in two ways: both Kepler-1649c and Earth have orbits roughly twice the radius of the previous known planets (Kepler-1649b and Venus respectively), and they are of similar size.
Orbit
Kepler-1649b takes only 8.6 Earth days to orbit Kepler-1649.
References
- ↑ "Exoplanet-catalog". https://exoplanets.nasa.gov/exoplanet-catalog/3489/Kepler-1649-b/.
- ↑ McDonald, Rebecca (April 15, 2020). "Dedicated Team of Scientists Discover Habitable-Zone Earth-Size Planet in Kepler Data". https://www.seti.org/press-release/dedicated-team-scientists-discover-habitable-zone-earth-size-planet-kepler-data.
- ↑ "Exoplanet-catalog". https://exoplanets.nasa.gov/exoplanet-catalog/3489/Kepler-1649-b/.
Original source: https://en.wikipedia.org/wiki/Kepler-1649b.
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