Schematic: Orbits of Proxima Centauri d, Proxima Centauri b and Proxima Centauri c around Proxima Centauri
Discovery[1]
Discovered by
Damasso et al.
Discovery site
HARPS
Discovery date
January 2020
Detection method
Radial velocity
Orbital characteristics
Semi-major axis
1.489±0.049 AU[2]
Eccentricity
0.04±0.01[3]
Orbital period (sidereal)
1928±20 d[3]
Inclination
133±1[3]
Longitude of ascending node
331±1[3]
Longitude of periastron
−4±4[3]
Time of periastron
2456202±21[3]
Semi-amplitude
1.1±0.2[3]
Star
Proxima Centauri
Physical characteristics
Mass
7±1ME[3]
Temperature
39 K (−234.2 °C; −389.5 °F)[1]
Proxima Centauri c (also called Proxima c[2] or Alpha Centauri Cc) is a controversial[4] 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. It is located approximately 4.2 light-years (1.3 parsecs; 40 trillion kilometres; 25 trillion miles) from Earth in the constellation of Centaurus, making it, Proxima b, and Proxima d the closest known exoplanets to the Solar System.
Proxima Centauri c is a super-Earth or mini-Neptune about 7 times as massive as Earth, orbiting at roughly 1.49 AU (223 million km; 139 million mi) every 1,928 days (5.28 yr).[3] Due to its large mass and its distance from Proxima Centauri, the exoplanet is uninhabitable, with an equilibrium temperature of approximately 39 K (−234.2 °C; −389.5 °F).[1] The planet is not transiting its parent star from the point of view of an Earth-based observer.[5]
The planet was first reported by Italian astrophysicist Mario Damasso and his colleagues in April 2019. Damasso's team had noticed minor movements of Proxima Centauri in the radial velocity data from the ESO's HARPS instrument, indicating a possible second planet orbiting Proxima Centauri.[6] The discovery was published in January 2020.[1] In June 2020, the planet's existence was initially confirmed using Hubble astrometry data from c. 1995, allowing its inclination and true mass to be determined.[3][7] Also in June 2020, a possible directly imaged counterpart of Proxima c was detected in the infrared with SPHERE, but the authors admit that they "did not obtain a clear detection".[8] If their candidate source is in fact Proxima Centauri c, it is too bright for a planet of its mass and age, implying that the planet may have a ring system with a radius of around 5 RJ.[8]
However, a 2022 study questioned the planetary nature of the observed radial velocity signal corresponding to Proxima c, attributing it to systematic effects.[4] If this is the case, it is unclear why astrometric observations detected what appeared to be a similar planetary signature.
^ abcdCite error: The named reference Damasso2020 was invoked but never defined (see the help page).
^ abCite error: The named reference Kervella2020 was invoked but never defined (see the help page).
^ abcdefghijCite error: The named reference BenedictMcArthur2020 was invoked but never defined (see the help page).
^ abCite error: The named reference Artigau2022 was invoked but never defined (see the help page).
^Gilbert, Emily A.; Barclay, Thomas; Kruse, Ethan; Quintana, Elisa V.; Walkowicz, Lucianne M. (2021), "No Transits of Proxima Centauri Planets in High-Cadence TESS Data", Frontiers in Astronomy and Space Sciences, 8: 190, arXiv:2110.10702, Bibcode:2021FrASS...8..190G, doi:10.3389/fspas.2021.769371
^Cite error: The named reference SA-20190412 was invoked but never defined (see the help page).
^Benedict, Fritz (June 2, 2020). "Texas astronomer uses 25 year-old Hubble data to confirm planet Proxima Centauri c". McDonald Observatory. University of Texas.
^ abCite error: The named reference Gratton2020 was invoked but never defined (see the help page).
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