Alpha Centauri Bc
Exoplanet | List of exoplanets
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Parent star | ||||||
Star | Alpha Centauri B | |||||
Constellation | Centaurus | |||||
Right ascension | (α) | 14h 39m 35.0803s | ||||
Declination | (δ) | -60° 50′ 13.761″ | ||||
Apparent magnitude | (mV) | +1.33 | ||||
Distance | 4.366 ± 0.007 ly (1.339 ± 0.002 pc) | |||||
Spectral type | K1 V | |||||
Mass | (m) | 0.907 M☉ | ||||
Radius | (r) | 0.865 R☉ | ||||
Temperature | (T) | 5260 K | ||||
Metallicity | [Fe/H] | 160% | ||||
Age | 6 ± 1 Gyr | |||||
Physical characteristics | ||||||
Radius | (r) | 0.92±0.06[1] R⊕ | ||||
Orbital elements | ||||||
Semi-major axis | (a) | 0.10[1] AU | ||||
Eccentricity | (e) | <0.24[1] | ||||
Orbital period | (P) | 12.4[1] d | ||||
Discovery information | ||||||
Discovery date | 2013 | |||||
Discoverer(s) | Demory et al.[1] | |||||
Discovery method | Transit[1] | |||||
Discovery status | Unconfirmed |
Alpha Centauri Bc is a suspected exoplanet orbiting Alpha Centauri B, part of Alpha Centauri system, the closest system to our own. It is located about 4.4 light-years away and is not in the habitable zone. It was first announced in 2013, and was the second proposed exoplanet in the system, after Alpha Centauri Bb. It would have an orbital period of approximately 12 Earth days, longer than that of Bb, now proven to not exist, and far smaller than that of Mercury.[1][2]
References
- 1 2 3 4 5 6 7 LePage, Andrew (March 28, 2015). "Has Another Planet Been Found Orbiting Alpha Centauri B?". Drew ex Machina. Retrieved September 5, 2015.
- ↑ Aron, Jacob (March 28, 2015). "Twin Earths may lurk in our nearest star system". New Scientist. Reed Business Information, Ltd. Retrieved September 5, 2015.
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