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Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1

  • Michaël Gillon
  • , Amaury H.M.J. Triaud
  • , Brice Olivier Demory
  • , Emmanuël Jehin
  • , Eric Agol
  • , Katherine M. Deck
  • , Susan M. Lederer
  • , Julien De Wit
  • , Artem Burdanov
  • , James G. Ingalls
  • , Emeline Bolmont
  • , Jeremy Leconte
  • , Sean N. Raymond
  • , Franck Selsis
  • , Martin Turbet
  • , Khalid Barkaoui
  • , Adam Burgasser
  • , Matthew R. Burleigh
  • , Sean J. Carey
  • , Aleksander Chaushev
  • Chris M. Copperwheat, Laetitia Delrez, Catarina S. Fernandes, Daniel L. Holdsworth, Enrico J. Kotze, Valérie Van Grootel, Yaseen Almleaky, Zouhair Benkhaldoun, Pierre Magain, Didier Queloz
  • University of Liège
  • Institute of Astronomy
  • University of Bern
  • University of Cambridge
  • University of Washington
  • NASA Astrobiology Institute's Virtual Planetary Laboratory
  • California Institute of Technology
  • NASA Johnson Space Center
  • Massachusetts Institute of Technology
  • Spitzer Science Center
  • University of Namur
  • Universite Paris-Saclay
  • Univ. Bordeaux
  • Cadi Ayyad University
  • University of California at San Diego
  • University of Leicester
  • Liverpool John Moores University
  • Lancashire Polytechnic
  • South African Astronomical Observatory
  • Faculty of Sciences, King Abdulaziz University
  • King Abdullah Centre for Crescent Observations and Astronomy
  • Université de Genève

Research output: Contribution to journalArticlepeer-review

Abstract

One aim of modern astronomy is to detect temperate, Earth-like exoplanets that are well suited for atmospheric characterization. Recently, three Earth-sized planets were detected that transit (that is, pass in front of) a star with a mass just eight per cent that of the Sun, located 12 parsecs away. The transiting configuration of these planets, combined with the Jupiter-like size of their host star - named TRAPPIST-1 - makes possible in-depth studies of their atmospheric properties with present-day and future astronomical facilities. Here we report the results of a photometric monitoring campaign of that star from the ground and space. Our observations reveal that at least seven planets with sizes and masses similar to those of Earth revolve around TRAPPIST-1. The six inner planets form a near-resonant chain, such that their orbital periods (1.51, 2.42, 4.04, 6.06, 9.1 and 12.35 days) are near-ratios of small integers. This architecture suggests that the planets formed farther from the star and migrated inwards. Moreover, the seven planets have equilibrium temperatures low enough to make possible the presence of liquid water on their surfaces.

Original languageEnglish
Pages (from-to)456-460
Number of pages5
JournalNature
Volume542
Issue number7642
DOIs
Publication statusPublished - 22 Feb 2017

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