A temperate rocky super-Earth transiting a nearby cool star

@article{Dittmann2017ATR,
  title={A temperate rocky super-Earth transiting a nearby cool star},
  author={J. Dittmann and J. Irwin and D. Charbonneau and X. Bonfils and N. Astudillo-Defru and R. Haywood and Z. Berta-Thompson and E. Newton and Joseph E. Rodriguez and J. Winters and T. Tan and J. Almenara and F. Bouchy and X. Delfosse and T. Forveille and C. Lovis and F. Murgas and F. Pepe and N. Santos and S. Udry and A. W{\"u}nsche and G. Esquerdo and D. Latham and C. Dressing},
  journal={Nature},
  year={2017},
  volume={544},
  pages={333-336}
}
M dwarf stars, which have masses less than 60 per cent that of the Sun, make up 75 per cent of the population of the stars in the Galaxy. The atmospheres of orbiting Earth-sized planets are observationally accessible via transmission spectroscopy when the planets pass in front of these stars. Statistical results suggest that the nearest transiting Earth-sized planet in the liquid-water, habitable zone of an M dwarf star is probably around 10.5 parsecs away. A temperate planet has been… Expand
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