Proxima Centauri d
.jpg) 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🜨 | |
| 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]
Proxima d is a sub-Earth at least one-quarter of the mass of Earth (or twice the mass of Mars), orbiting at roughly 0.029 AU (4.3 million km; 2.7 million mi) every 5.1 days.[4] It is the least massive and innermost known planet of the Proxima Centauri system. It is the least massive exoplanet detected with the radial velocity method as of 2022[update]. Its proximity to the star and short orbital period of 5.1 days suggest that it is likely tidally locked due to strong tidal forces. Although Proxima d orbits too close to its star to have a habitable equilibrium temperature (which likely reaches 360 K (87 °C; 188 °F)[1] from about 190% of Earth's irradiation—assuming an Earth-like reflectivity, it is theoretically possible that Proxima d possesses polar regions with habitable temperatures.
Proxima d is considered a candidate exoplanet by its discoverers and the NASA Exoplanet Archive, because it has not been independently confirmed by more than one observatory.[1][2] However, some astronomers regard Proxima d as confirmed because it could be detected via different methods of measuring the same radial velocity data from which Proxima d was discovered.[3] As of 2022, Proxima d has been detected by the ESPRESSO spectrograph on the Very Large Telescope,[1]: 9 and also at a 2σ level (which does not constitute confirmation) by the HARPS spectrograph at the La Silla Observatory.[3]
See also
[edit]Notes
[edit]- ^ Proxima Centauri c's radial velocity signature was disputed in a 2022 study, which instead attributed its detection to potential bias in data processing methods, thereby leaving its existence as disputed.[3]
References
[edit]- ^ a b c d e f g h Faria, J. P.; Suárez Mascareño, A.; et al. (4 January 2022). "A candidate short-period sub-Earth orbiting Proxima Centauri" (PDF). Astronomy & Astrophysics. 658. European Southern Observatory: 17. arXiv:2202.05188. Bibcode:2022A&A...658A.115F. doi:10.1051/0004-6361/202142337.
- ^ a b "alf Cen Overview". NASA Exoplanet Archive. NASA. Retrieved 24 September 2024.
- ^ a b c Artigau, Étienne; Cadieux, Charles; Cook, Neil J.; Doyon, René; Vandal, Thomas; et al. (September 2022). "Line-by-line Velocity Measurements: an Outlier-resistant Method for Precision Velocimetry". The Astronomical Journal. 164 (3): 18. arXiv:2207.13524. Bibcode:2022AJ....164...84A. doi:10.3847/1538-3881/ac7ce6. 84.
- ^ a b Suárez Mascareño, A.; Faria, J. P.; et al. (11 May 2020). "Revisiting Proxima with ESPRESSO". Astronomy & Astrophysics. 639: 24. arXiv:2005.12114. Bibcode:2020A&A...639A..77S. doi:10.1051/0004-6361/202037745. ISSN 0004-6361.
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