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$0.1 per cent solar, a
measured radius of 0.14 R$_ødot$ 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.
Description
A terrestrial planet candidate in a temperate orbit around Proxima
Centauri
cite arxiv:1609.03449Comment: Version accepted for publication by Nature (unedited, July 7th, 2016), figures inserted in text for easier read. Article body : 10 pages, 3 figures, 1 table. Methods section : 23 pages, 9 figures, 1 table. IMPORTANT NOTE : Acknowledgment to IAA/CSIC researchers Javier Pascual Granado and Rafael Garrido added for useful discussions and feedback on the mathematical properties of time-series
%0 Generic
%1 angladaescude2016terrestrial
%A Anglada-Escudé, Guillem
%A Amado, Pedro J.
%A Barnes, John
%A Berdiñas, Zaira M.
%A Butler, R. Paul
%A Coleman, Gavin A. L.
%A de la Cueva, Ignacio
%A Dreizler, Stefan
%A Endl, Michael
%A Giesers, Benjamin
%A Jeffers, Sandra V.
%A Jenkins, James S.
%A Jones, Hugh R. A.
%A Kiraga, Marcin
%A Kürster, Martin
%A López-González, María J.
%A Marvin, Christopher J.
%A Morales, Nicolás
%A Morin, Julien
%A Nelson, Richard P.
%A Ortiz, José L.
%A Ofir, Aviv
%A Paardekooper, Sijme-Jan
%A Reiners, Ansgar
%A Rodríguez, Eloy
%A Rodríguez-López, Cristina
%A Sarmiento, Luis F.
%A Strachan, John P.
%A Tsapras, Yiannis
%A Tuomi, Mikko
%A Zechmeister, Mathias
%D 2016
%K exoplanet mdwarf
%R 10.1038/nature19106
%T A terrestrial planet candidate in a temperate orbit around Proxima
Centauri
%U http://arxiv.org/abs/1609.03449
%X 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$0.1 per cent solar, a
measured radius of 0.14 R$_ødot$ 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.
@misc{angladaescude2016terrestrial,
abstract = {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.},
added-at = {2016-09-13T17:41:09.000+0200},
author = {Anglada-Escudé, Guillem and Amado, Pedro J. and Barnes, John and Berdiñas, Zaira M. and Butler, R. Paul and Coleman, Gavin A. L. and de la Cueva, Ignacio and Dreizler, Stefan and Endl, Michael and Giesers, Benjamin and Jeffers, Sandra V. and Jenkins, James S. and Jones, Hugh R. A. and Kiraga, Marcin and Kürster, Martin and López-González, María J. and Marvin, Christopher J. and Morales, Nicolás and Morin, Julien and Nelson, Richard P. and Ortiz, José L. and Ofir, Aviv and Paardekooper, Sijme-Jan and Reiners, Ansgar and Rodríguez, Eloy and Rodríguez-López, Cristina and Sarmiento, Luis F. and Strachan, John P. and Tsapras, Yiannis and Tuomi, Mikko and Zechmeister, Mathias},
biburl = {https://www.bibsonomy.org/bibtex/26de620ddb2e6befabd354bf131c88db8/superjenwinters},
description = {A terrestrial planet candidate in a temperate orbit around Proxima
Centauri},
doi = {10.1038/nature19106},
interhash = {5a062b686ce7318a0a54a7916b5fb4a3},
intrahash = {6de620ddb2e6befabd354bf131c88db8},
keywords = {exoplanet mdwarf},
note = {cite arxiv:1609.03449Comment: Version accepted for publication by Nature (unedited, July 7th, 2016), figures inserted in text for easier read. Article body : 10 pages, 3 figures, 1 table. Methods section : 23 pages, 9 figures, 1 table. IMPORTANT NOTE : Acknowledgment to IAA/CSIC researchers Javier Pascual Granado and Rafael Garrido added for useful discussions and feedback on the mathematical properties of time-series},
timestamp = {2016-09-13T17:41:09.000+0200},
title = {A terrestrial planet candidate in a temperate orbit around Proxima
Centauri},
url = {http://arxiv.org/abs/1609.03449},
year = 2016
}