Author
Listed:
- Brice-Olivier Demory
(Astrophysics Group, Cavendish Laboratory)
- Michael Gillon
(Institut d’Astrophysique et de Géophysique, Université of Liège)
- Julien de Wit
(Atmospheric and Planetary Sciences, Massachusetts Institute of Technology)
- Nikku Madhusudhan
(Institute of Astronomy, University of Cambridge)
- Emeline Bolmont
(NaXys, University of Namur)
- Kevin Heng
(University of Bern, Center for Space and Habitability)
- Tiffany Kataria
(Astrophysics Group, School of Physics, University of Exeter)
- Nikole Lewis
(Space Telescope Science Institute)
- Renyu Hu
(Jet Propulsion Laboratory, California Institute of Technology
California Institute of Technology)
- Jessica Krick
(Spitzer Science Center, MS 220-6, California Institute of Technology)
- Vlada Stamenković
(Jet Propulsion Laboratory, California Institute of Technology
California Institute of Technology)
- Björn Benneke
(California Institute of Technology)
- Stephen Kane
(San Francisco State University)
- Didier Queloz
(Astrophysics Group, Cavendish Laboratory)
Abstract
A longitudinal thermal brightness map of the super-Earth exoplanet 55 Cancri e reveals strong day–night temperature contrast, indicating inefficient heat redistribution consistent with 55 Cancri e either being devoid of atmosphere or having an optically thick atmosphere with heat recirculation confined to the planetary dayside.
Suggested Citation
Brice-Olivier Demory & Michael Gillon & Julien de Wit & Nikku Madhusudhan & Emeline Bolmont & Kevin Heng & Tiffany Kataria & Nikole Lewis & Renyu Hu & Jessica Krick & Vlada Stamenković & Björn Benneke, 2016.
"A map of the large day–night temperature gradient of a super-Earth exoplanet,"
Nature, Nature, vol. 532(7598), pages 207-209, April.
Handle:
RePEc:nat:nature:v:532:y:2016:i:7598:d:10.1038_nature17169
DOI: 10.1038/nature17169
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