![]() Artistic depiction of Proxima Centauri d, with Proxima Centauri and Alpha Centauri A & B visible in the background | |
Discovery[1] | |
---|---|
Discovery site | VLT-ESPRESSO |
Discovery date | 2020 |
Radial velocity | |
Orbital characteristics[1] | |
0.02885+0.00019 −0.00022 AU | |
Eccentricity | 0.04+0.15 −0.04 |
5.122+0.002 −0.0036 d | |
Semi-amplitude | 0.39±0.07 m/s |
Star | Proxima Centauri |
Physical characteristics[1] | |
~0.81±0.08 R🜨 (predicted) | |
Mass | ≥0.26±0.05 M🜨 |
Temperature | 360 K (87 °C; 188 °F) |
Proxima Centauri d (also called Proxima d) is a candidate[2][1] exoplanet orbiting the red dwarf star Proxima Centauri, the closest star to the Sun and part of the Alpha Centauri triple star system. Together with two other planets[a] in the Proxima Centauri system, it is the closest known exoplanet to the Solar System, located approximately 4.2 light-years (1.3 parsecs; 40 trillion kilometres; 25 trillion miles) away in the constellation of Centaurus. The first signs of the exoplanet emerged as a weak 5.15-day signal in radial velocity data taken from the Very Large Telescope during a 2020 study on Proxima b's mass. This signal was formally proposed to be a candidate exoplanet by Faria et al. in a follow-up paper published in February 2022.[4][1]
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Artigau2022
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