| Literature DB >> 27558064 |
Guillem Anglada-Escudé1, Pedro J Amado2, John Barnes3, Zaira M Berdiñas2, R Paul Butler4, Gavin A L Coleman1, Ignacio de la Cueva5, Stefan Dreizler6, Michael Endl7, Benjamin Giesers6, Sandra V Jeffers6, James S Jenkins8, Hugh R A Jones9, Marcin Kiraga10, Martin Kürster11, Marίa J López-González2, Christopher J Marvin6, Nicolás Morales2, Julien Morin12, Richard P Nelson1, José L Ortiz2, Aviv Ofir13, Sijme-Jan Paardekooper1, Ansgar Reiners6, Eloy Rodríguez2, Cristina Rodrίguez-López2, Luis F Sarmiento6, John P Strachan1, Yiannis Tsapras14, Mikko Tuomi9, Mathias Zechmeister6.
Abstract
At a distance of 1.295 parsecs, the red dwarf Proxima Centauri (α Centauri C, GL 551, HIP 70890 or simply Proxima) is the Sun's closest stellar neighbour and one of the best-studied low-mass stars. It has an effective temperature of only around 3,050 kelvin, a luminosity of 0.15 per cent of that of the Sun, a measured radius of 14 per cent of the radius of the Sun and a mass of about 12 per cent of the mass of the Sun. Although Proxima is considered a moderately active star, its rotation period is about 83 days (ref. 3) and its quiescent activity levels and X-ray luminosity are comparable to those of the Sun. Here we report observations that reveal the presence of a small planet with a minimum mass of about 1.3 Earth masses orbiting Proxima with a period of approximately 11.2 days at a semi-major-axis distance of around 0.05 astronomical units. Its equilibrium temperature is within the range where water could be liquid on its surface.Entities:
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Year: 2016 PMID: 27558064 DOI: 10.1038/nature19106
Source DB: PubMed Journal: Nature ISSN: 0028-0836 Impact factor: 49.962