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A terrestrial planet candidate in a temperate orbit around Proxima Centauri

  • Guillem Anglada-Escude
  • , Pedro J. Amado
  • , John Barnes
  • , Zaira M. Berdinas
  • , Paul Butler
  • , Gavin A. L. Coleman
  • , Ignacio de la Cueva
  • , Stefan Dreizler
  • , Michael Endl
  • , Benjamin Giesers
  • , Sandra V. Jeffers
  • , James S. Jenkins
  • , Hugh Jones
  • , Marcin Kiraga
  • , Martin Kurster
  • , Maria J. Lopez-Gonzalez
  • , Christopher J. Marvin
  • , Nicolas Morales
  • , Julien Morin
  • , Richard P. Nelson
  • Jose L. Ortiz, Aviv Ofir, Sijme-Jan Paardekooper, Ansgar Reiners, Eloy Rodriguez, Cristina Rodriguez-Lopez, Luis F. Sarmiento, John P. Strachan, Yiannis Tsapras, Mikko Tuomi, Mathias Zechmeister

Research output: Contribution to journalArticlepeer-review

878 Citations (Scopus)
281 Downloads (Pure)

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 and its quiescent activity levels and X-ray luminosity4 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.
Original languageEnglish
Pages (from-to)437-440
JournalNature
Volume536
Early online date24 Aug 2016
DOIs
Publication statusPublished - 25 Aug 2016

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