![]() 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 | February 2022 |
Radial velocity | |
Orbital characteristics[2] | |
0.02881±0.00017 AU | |
Eccentricity | 0 (assumed) |
5.12338±0.00035 d | |
Semi-amplitude | 0.392±0.057 m/s |
Star | Proxima Centauri |
Physical characteristics | |
~0.81±0.08 R🜨[1] (predicted) | |
Mass | ≥0.260±0.038 M🜨[2] |
Temperature | 360 K (87 °C; 188 °F)[1] |
Proxima Centauri d (also called Proxima d) is a confirmed[2] 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 one or 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.[4] This signal was formally proposed to be a candidate exoplanet by Faria et al. in a follow-up paper published in February 2022,[1] and was independently confirmed in 2025.[2]
Faria2022
was invoked but never defined (see the help page).
SuárezMascareño2025
was invoked but never defined (see the help page).
Artigau2022
was invoked but never defined (see the help page).
SuarezMascareno2020
was invoked but never defined (see the help page).
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