The Alpha Centauri system as a whole has two confirmed planets, both of them around Proxima Centauri. While other planets have been claimed to exist around all of the stars, none of the discoveries have been confirmed.
Planets of Alpha Centauri A In 2021, a candidate planet named Candidate 1 (or C1) was detected around Alpha Centauri A, thought to orbit at approximately with a period of about one year, and to have a mass between that of Neptune and one-half that of Saturn, though it may be a dust disk or an artefact. The possibility of C1 being a background star has been ruled out. If this candidate is confirmed, the temporary name C1 will most likely be replaced with the scientific designation Alpha Centauri Ab in accordance with current naming conventions. GO Cycle 1 observations are planned for the
James Webb Space Telescope (JWST) to search for planets around Alpha Centauri A, as well as observations of
Epsilon Muscae. The coronographic observations, which occurred on July 26 and 27, 2023, were failures, though there are follow-up observations in March 2024. Pre-launch estimates predicted that JWST will be able to find planets with a radius of 5 at . Multiple observations every 3–6 months could push the limit down to 3 . Post-launch estimates based on observations of
HIP 65426 b find that JWST will be able to find planets even closer to Alpha Centauri A and could find a 5 planet at . Candidate 1 has an estimated radius between If it is an exoplanet, it should have a mass between 90 and 150
Earth masses, a radius between 1.0 and 1.1 and a temperature of . A search for
transits of planet Bb was conducted with the
Hubble Space Telescope from 2013 to 2014. This search detected one potential transit-like event, which could be associated with a different planet with a radius around . This planet would most likely orbit Alpha Centauri B with an orbital period of 20.4 days or less, with only a 5% chance of it having a longer orbit. The median of the likely orbits is 12.4 days. Its orbit would likely have an eccentricity of 0.24 or less. It could have lakes of molten lava and would be far too close to Alpha Centauri B to harbour
life. If confirmed, this planet might be called . However, the name has not been used in the literature, as it is not a claimed discovery.
Planets of Proxima Centauri Proxima Centauri b or Alpha Centauri Cb is a terrestrial planet discovered in 2016 by astronomers at the
European Southern Observatory (ESO). It has an estimated
minimum mass of 1.17 (
Earth masses) and orbits approximately 0.049
AU from Proxima Centauri, placing it in the star's
habitable zone. It has a mass of roughly 7 and orbits about from Proxima Centauri with a period of . In June 2020, a possible direct imaging detection of the planet hinted at the presence of a large ring system. However, a 2022 study disputed the existence of this planet. , evidence for Proxima c remains inconclusive; observations with the
NIRPS spectrograph were unable to confirm it, but found hints of a lower-amplitude signal with a similar period.
Hypothetical planets Additional planets may exist in the Alpha Centauri system, either orbiting Alpha Centauri A or Alpha Centauri B individually, or in large orbits around Alpha Centauri AB. Because both stars are fairly similar to the Sun (in age and
metallicity, for example), astronomers have been especially interested in making detailed searches for planets in the Alpha Centauri system. Several established planet-hunting teams have used various
radial velocity or star
transit methods in their searches around these two bright stars. Bodies around Alpha Centauri A would be able to orbit at slightly farther distances due to its stronger gravity. In addition, the lack of any brown dwarfs or gas giants in close orbits around Alpha Centauri make the likelihood of terrestrial planets greater than otherwise. A 2016 estimate placed the probability of finding an Earth-like planet around Alpha Centauri at roughly 75%. The observational thresholds for planet detection in the habitable zones by the radial velocity method are currently (2017) estimated to be about for Alpha Centauri A, for Alpha Centauri B, and for
Proxima Centauri. Early computer-generated models of planetary formation predicted the existence of
terrestrial planets around
both Alpha Centauri A and B, Despite these difficulties, given the similarities to the Sun in
spectral types, star type, age and probable stability of the orbits, it has been suggested that this stellar system could hold one of the best possibilities for harbouring
extraterrestrial life on a potential planet. In the
Solar System, it was once thought that
Jupiter and
Saturn were probably crucial in perturbing
comets into the inner Solar System, providing the inner planets with a source of water and various other ices. However, since isotope measurements of the
deuterium to
hydrogen (D/H) ratio in comets
Halley,
Hyakutake,
Hale–Bopp, 2002T7, and Tuttle yield values approximately twice that of Earth's oceanic water, more recent models and research predict that less than 10% of Earth's water was supplied from comets. In the system, Proxima Centauri may have influenced the planetary disk as the system was forming, enriching the area around Alpha Centauri with volatile materials. This would be discounted if, for example, happened to have
gas giants orbiting (or vice versa), or if and B themselves were able to perturb comets into each other's inner systems, as Jupiter and Saturn presumably have done in the Solar System. For the slightly less luminous and cooler , the habitable zone is between about 0.7 and . The S.I.M. mission, however, was cancelled due to financial issues in 2010.
Circumstellar discs Based on observations between 2007 and 2012, a study found a slight excess of emissions in the 24
μm (mid/far-infrared) band surrounding , which may be interpreted as evidence for a sparse
circumstellar disc or dense
interplanetary dust. == View from this system ==