Kepler-20b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | Kepler-20 (KOI-070) | |
Constellation | Lyra | |
Right ascension | (α) | 19h 10m 47.5235s[1] |
Declination | (δ) | +42° 20′ 19.299″[1] |
Apparent magnitude | (mV) | 12.51 |
Distance | ±6 929[1] ly (±2 285[1] pc) | |
Mass | (m) | ±0.035 0.912 M☉ |
Radius | (r) | +0.06 −0.095 0.944 R☉ |
Temperature | (T) | ±93 5466 K |
Metallicity | [Fe/H] | ±0.04 0.02 |
Age | +4.7 −2.7 8.8 Gyr | |
Physical characteristics | ||
Mass | (m) | +1.41 −1.44 9.7[2] M⊕ |
Radius | (r) | +0.066 −0.034 1.868R⊕ |
Density | (ρ) | +2.0 −2.7 8.2g cm−3 |
Temperature | (T) | 1014 |
Orbital elements | ||
Semi-major axis | (a) | 37 0.045AU |
Eccentricity | (e) | <0.32 |
Orbital period | (P) | 1219 3.696d |
Inclination | (i) | +0.36 −0.31° 86.50 |
Discovery information | ||
Discovery date | 20 December 2011 | |
Discoverer(s) | Kepler team | |
Discovery method | Transit (Kepler Mission) | |
Other detection methods | Radial velocity | |
Discovery status | Conference announcement |
Kepler-20b is an exoplanet orbiting Kepler-20. It is classified as a Super-Earth, as it has a radius and mass greater than that of Earth. At about 1.87 R⊕, it would most likely be a Mini-Neptune, but its high mass of 9.7 M⊕ implies that it is an iron-rich rocky world. Along with the other four planets in the system, Kepler-20b was announced on 20 December 2011.
References
- 1 2 3 4 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia Data Release 2 Vizier catalog entry
- ↑ https://arxiv.org/abs/1608.06836 A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system
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