Nature Communications (Apr 2016)

Hot super-Earths stripped by their host stars

  • M. S. Lundkvist,
  • H. Kjeldsen,
  • S. Albrecht,
  • G. R. Davies,
  • S. Basu,
  • D. Huber,
  • A. B. Justesen,
  • C. Karoff,
  • V. Silva Aguirre,
  • V. Van Eylen,
  • C. Vang,
  • T. Arentoft,
  • T. Barclay,
  • T. R. Bedding,
  • T. L. Campante,
  • W. J. Chaplin,
  • J. Christensen-Dalsgaard,
  • Y. P. Elsworth,
  • R. L. Gilliland,
  • R. Handberg,
  • S. Hekker,
  • S. D. Kawaler,
  • M. N. Lund,
  • T. S. Metcalfe,
  • A. Miglio,
  • J. F. Rowe,
  • D. Stello,
  • B. Tingley,
  • T. R. White

DOI
https://doi.org/10.1038/ncomms11201
Journal volume & issue
Vol. 7, no. 1
pp. 1 – 8

Abstract

Read online

Theory predicts a deficit of super-Earth sized planets, which orbit close to their host star. Here, Lundkvist et al. use data from the NASA Kepler mission to show that this deficit is also seen in observations, thereby providing new insight into exoplanetary systems.