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arxiv: 1609.03449 · v1 · pith:PLR7SOQGnew · submitted 2016-09-12 · 🌌 astro-ph.EP

A terrestrial planet candidate in a temperate orbit around Proxima Centauri

classification 🌌 astro-ph.EP
keywords proximacentaurimasscentdaysluminosityorbitalperiod
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At a distance of 1.295 parsecs, the red-dwarf Proxima Centauri ($\alpha$ 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 $\sim$ 3050 K, a luminosity of $\sim$0.1 per cent solar, a measured radius of 0.14 R$_\odot$ 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 $\sim$ 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 $\sim$11.2 days. Its orbital semi-major axis is $\sim0.05$ AU, with an equilibrium temperature in the range where water could be liquid on its surface.

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Cited by 1 Pith paper

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  1. Star-planet interaction in the Proxima system

    astro-ph.EP 2026-05 unverdicted novelty 7.0

    Spectroscopic monitoring detects phase-locked flares to Proxima d and flare-intensity modulation by Proxima b, producing a -16 G polar field estimate for the inner planet via Poynting-flux modeling.