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Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3

  • Michaël Gillon
  • , Peter P. Pedersen
  • , Benjamin V. Rackham
  • , Georgina Dransfield
  • , Elsa Ducrot
  • , Khalid Barkaoui
  • , Artem Y. Burdanov
  • , Urs Schroffenegger
  • , Yilen Gómez Maqueo Chew
  • , Susan M. Lederer
  • , Roi Alonso
  • , Adam J. Burgasser
  • , Steve B. Howell
  • , Norio Narita
  • , Julien de Wit
  • , Brice Olivier Demory
  • , Didier Queloz
  • , Amaury H.M.J. Triaud
  • , Laetitia Delrez
  • , Emmanuël Jehin
  • Matthew J. Hooton, Lionel J. Garcia, Clàudia Jano Muñoz, Catriona A. Murray, Francisco J. Pozuelos, Daniel Sebastian, Mathilde Timmermans, Samantha J. Thompson, Sebastián Zúñiga-Fernández, Jesús Aceituno, Christian Aganze, Pedro J. Amado, Thomas Baycroft, Zouhair Benkhaldoun, David Berardo, Emeline Bolmont, Catherine A. Clark, Yasmin T. Davis, Fatemeh Davoudi, Zoë L. de Beurs, Jerome P. de Leon, Masahiro Ikoma, Kai Ikuta, Keisuke Isogai, Izuru Fukuda, Akihiko Fukui, Roman Gerasimov, Mourad Ghachoui, Maximilian N. Günther, Samantha Hasler, Yuya Hayashi, Kevin Heng, Renyu Hu, Taiki Kagetani, Yugo Kawai, Kiyoe Kawauchi, Daniel Kitzmann, Daniel D.B. Koll, Monika Lendl, John H. Livingston, Xintong Lyu, Erik A. Meier Valdés, Mayuko Mori, James J. McCormac, Felipe Murgas, Prajwal Niraula, Enric Pallé, Ilse Plauchu-Frayn, Rafael Rebolo, Laurence Sabin, Yannick Schackey, Nicole Schanche, Franck Selsis, Alfredo Sota, Manu Stalport, Matthew R. Standing, Keivan G. Stassun, Motohide Tamura, Yuka Terada, Christopher A. Theissen, Martin Turbet, Valérie Van Grootel, Roberto Varas, Noriharu Watanabe, Francis Zong Lang
  • University of Liège
  • University of Cambridge
  • ETH Zurich
  • Massachusetts Institute of Technology
  • Massachusetts Institute of Technology
  • University of Birmingham
  • CNRS
  • Instituto de Astrofisica de Canarias
  • University of Bern
  • Universidad Nacional Autónoma de México
  • NASA Johnson Space Center
  • Research Unit; CIBERNED and Universidad de La Laguna
  • University of California, San Diego
  • NASA Ames Research Center
  • University of Tokyo
  • Astrobiology Center
  • KU Leuven
  • Flatiron Institute
  • University of Colorado Boulder
  • Instituto de Astrofísica de Andalucía-CSIC
  • Centro Astronómico Hispano en Andalucia
  • Stanford University
  • Cadi Ayyad University
  • University of Geneva
  • California Institute of Technology
  • California Institute of Technology
  • National Astronomical Observatory
  • The Graduate University for Advanced Studies
  • Kyoto University
  • University of Notre Dame
  • ESTEC - European Space Research and Technology Centre
  • Universität München
  • California Institute of Technology
  • Ritsumeikan University Biwako-Kusatsu Campus
  • Tsinghua University
  • University of Warwick
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Laboratoire d'Astrophysique de Bordeaux
  • ESAC campus
  • Vanderbilt University

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them, TRAPPIST-1, has so far been found to host a transiting planetary system. In this context, we present the SPECULOOS project’s detection of an Earth-sized planet in a 17 h orbit around an ultracool dwarf of M6.5 spectral type located 16.8 pc away. The planet’s high irradiation (16 times that of Earth) combined with the infrared luminosity and Jupiter-like size of its host star make it one of the most promising rocky exoplanet targets for detailed emission spectroscopy characterization with JWST. Indeed, our sensitivity study shows that just ten secondary eclipse observations with the Mid-InfraRed Instrument/Low-Resolution Spectrometer on board JWST should provide strong constraints on its atmospheric composition and/or surface mineralogy.

langue originaleAnglais
Pages (de - à)865-878
Nombre de pages14
journalNature Astronomy
Volume8
Numéro de publication7
Les DOIs
étatPublié - 1 juil. 2024

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