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A high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b

Author

Listed:
  • Nikku Madhusudhan

    (Massachusetts Institute of Technology
    Present address: Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA.)

  • Joseph Harrington

    (Planetary Sciences Group, University of Central Florida)

  • Kevin B. Stevenson

    (Planetary Sciences Group, University of Central Florida)

  • Sarah Nymeyer

    (Planetary Sciences Group, University of Central Florida)

  • Christopher J. Campo

    (Planetary Sciences Group, University of Central Florida)

  • Peter J. Wheatley

    (University of Warwick)

  • Drake Deming

    (NASA’s Goddard Space Flight Center)

  • Jasmina Blecic

    (Planetary Sciences Group, University of Central Florida)

  • Ryan A. Hardy

    (Planetary Sciences Group, University of Central Florida)

  • Nate B. Lust

    (Planetary Sciences Group, University of Central Florida)

  • David R. Anderson

    (Astrophysics Group, Keele University)

  • Andrew Collier-Cameron

    (School of Physics and Astronomy, University of St Andrews)

  • Christopher B. T. Britt

    (Planetary Sciences Group, University of Central Florida)

  • William C. Bowman

    (Planetary Sciences Group, University of Central Florida)

  • Leslie Hebb

    (Vanderbilt University)

  • Coel Hellier

    (Astrophysics Group, Keele University)

  • Pierre F. L. Maxted

    (Astrophysics Group, Keele University)

  • Don Pollacco

    (Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University, University Road)

  • Richard G. West

    (University of Leicester)

Abstract

A carbon-rich exoplanet The transiting 'hot Jupiter' WASP-12b orbits a star slightly hotter than the Sun in a circular orbit at a distance of only 0.023 astronomical units (AU), making it one of the hottest exoplanets known. An analysis of dayside multi-wavelength photometry of WASP-12b reveals a carbon-rich atmosphere abundant in carbon monoxide. Compared with model predictions, the atmosphere is depleted in water vapour and enhanced in methane content by two orders of magnitude. In addition, the absence of a strong thermal inversion or a prominent stratosphere challenges existing theories about the atmospheres of such exoplanets.

Suggested Citation

  • Nikku Madhusudhan & Joseph Harrington & Kevin B. Stevenson & Sarah Nymeyer & Christopher J. Campo & Peter J. Wheatley & Drake Deming & Jasmina Blecic & Ryan A. Hardy & Nate B. Lust & David R. Anderson, 2011. "A high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b," Nature, Nature, vol. 469(7328), pages 64-67, January.
  • Handle: RePEc:nat:nature:v:469:y:2011:i:7328:d:10.1038_nature09602
    DOI: 10.1038/nature09602
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