![]() Schematic: Orbits of Proxima Centauri d, Proxima Centauri b and Proxima Centauri c around Proxima Centauri | |
Discovery[1] | |
---|---|
Discovered by | Damasso et al. |
Discovery site | HARPS |
Discovery date | January 2020 |
Radial velocity | |
Orbital characteristics | |
1.489±0.049 AU[2] | |
Eccentricity | 0.04±0.01[3] |
1928±20 d[3] | |
Inclination | 133±1[3] |
331±1[3] | |
−4±4[3] | |
2456202±21[3] | |
Semi-amplitude | 1.1±0.2[3] |
Star | Proxima Centauri |
Physical characteristics | |
Mass | 7±1 M🜨[3] |
Temperature | 39 K (−234.2 °C; −389.5 °F)[1] |
Proxima Centauri c (also called Proxima c[2] or Alpha Centauri Cc) is a controversial exoplanet candidate, claimed to be orbiting the red dwarf star Proxima Centauri, which is the closest star to the Sun and part of a triple star system.[4]
Damasso2020
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Kervella2020
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BenedictMcArthur2020
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Artigau2022
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