Proxima Centauri c
| Schematic: Orbits of Proxima Centauri d, Proxima Centauri b and Proxima Centauri c around Proxima Centauri | |
| Discovery | |
|---|---|
| Discovered by | Damasso et al. | 
| Discovery site | HARPS | 
| Discovery date | January 2020 | 
| Radial velocity | |
| Orbital characteristics | |
| 1.489±0.049 AU | |
| Eccentricity | 0.04±0.01 | 
| 1928±20 d | |
| Inclination | 133±1 | 
| 331±1 | |
| −4±4 | |
| 2456202±21 | |
| Semi-amplitude | 1.1±0.2 | 
| Star | Proxima Centauri | 
| Physical characteristics | |
| Mass | 7±1 ME | 
| Temperature | 39 K (−234.2 °C; −389.5 °F) | 
Proxima Centauri c (also called Proxima c 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.