A terrestrial planet candidate in a temperate orbit around Proxima Centauri
Guillem Anglada-Escud\'e, Pedro J. Amado, John Barnes, Zaira M., Berdi\~nas, R. Paul Butler, Gavin A. L. Coleman, Ignacio de la Cueva, Stefan, Dreizler, Michael Endl, Benjamin Giesers, Sandra V. Jeffers, James S., Jenkins, Hugh R. A. Jones, Marcin Kiraga, Martin K\"urster

TL;DR
This paper reports the discovery of a small, Earth-mass planet orbiting Proxima Centauri within the habitable temperature zone, based on new observational data.
Contribution
It presents the detection of a terrestrial planet candidate around Proxima Centauri, a nearby red dwarf, with specific orbital and physical characteristics.
Findings
Detected a planet with minimum mass of 1.3 Earth masses
Orbital period of approximately 11.2 days
Orbital semi-major axis of about 0.05 AU
Abstract
At a distance of 1.295 parsecs, the red-dwarf Proxima Centauri ( Centauri C, GL 551, HIP 70890, or simply Proxima) is the Sun's closest stellar neighbor and one of the best studied low-mass stars. It has an effective temperature of only 3050 K, a luminosity of 0.1 per cent solar, a measured radius of 0.14 R and a mass of about 12 per cent the mass of the Sun. Although Proxima is considered a moderately active star, its rotation period is 83 days, and its quiescent activity levels and X-ray luminosity are comparable to the Sun's. New observations reveal the presence of a small planet orbiting Proxima with a minimum mass of 1.3~Earth masses and an orbital period of 11.2 days. Its orbital semi-major axis is AU, with an equilibrium temperature in the range where water could be liquid on its surface.
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