Proxima Centauri d

Proxima Centauri d
Artistic depiction of Proxima Centauri d, with Proxima Centauri and Alpha Centauri A & B visible in the background
Discovery[1]
Discovery siteVLT-ESPRESSO
Discovery dateFebruary 2022
Radial velocity
Orbital characteristics[2]
0.02881±0.00017 AU
Eccentricity0 (assumed)
5.12338±0.00035 d
Semi-amplitude0.392±0.057 m/s
StarProxima Centauri
Physical characteristics
~0.81±0.08 R🜨[1] (predicted)
Mass≥0.260±0.038 M🜨[2]
Temperature360 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]

  1. ^ a b c d Cite error: The named reference Faria2022 was invoked but never defined (see the help page).
  2. ^ a b c d Cite error: The named reference SuárezMascareño2025 was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference Artigau2022 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference SuarezMascareno2020 was invoked but never defined (see the help page).


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