A terrestrial planet candidate in a temperate orbit around Proxima Centauri

@article{AngladaEscud2016ATP,
  title={A terrestrial planet candidate in a temperate orbit around Proxima Centauri},
  author={G. Anglada-Escud{\'e} and P. Amado and J. Barnes and Z. Berdi{\~n}as and R. Butler and G. Coleman and I. Cueva and S. Dreizler and M. Endl and B. Giesers and S. Jeffers and J. Jenkins and H. Jones and M. Kiraga and M. K{\"u}rster and M. L{\'o}pez-Gonz{\'a}lez and C. Marvin and N. Morales and J. Morin and R. Nelson and J. Ortiz and A. Ofir and S. Paardekooper and A. Reiners and E. Rodr{\'i}guez and Cristina Rodrίguez-L{\'o}pez and L. F. Sarmiento and J. Strachan and Y. Tsapras and M. Tuomi and M. Zechmeister},
  journal={Nature},
  year={2016},
  volume={536},
  pages={437-440}
}
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… Expand

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