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Detection of titanium oxide in the atmosphere of a hot Jupiter

Author

Listed:
  • Elyar Sedaghati

    (European Southern Observatory
    Deutsches Zentrum für Luft- und Raumfahrt
    Zentrum für Astronomie und Astrophysik, TU Berlin)

  • Henri M. J. Boffin

    (European Southern Observatory)

  • Ryan J. MacDonald

    (Institute of Astronomy, University of Cambridge)

  • Siddharth Gandhi

    (Institute of Astronomy, University of Cambridge)

  • Nikku Madhusudhan

    (Institute of Astronomy, University of Cambridge)

  • Neale P. Gibson

    (Astrophysics Research Centre, School of Mathematics and Physics, Queens University Belfast)

  • Mahmoudreza Oshagh

    (Institut für Astrophysik, Georg-August Universität Göttingen
    Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas)

  • Antonio Claret

    (Instituto de Astrofísica de Andalucía, CSIC)

  • Heike Rauer

    (Deutsches Zentrum für Luft- und Raumfahrt
    Zentrum für Astronomie und Astrophysik, TU Berlin)

Abstract

Titanium oxide, water, sodium and a strongly scattering haze have been detected in the atmosphere of the hot Jupiter exoplanet WASP-19b.

Suggested Citation

  • Elyar Sedaghati & Henri M. J. Boffin & Ryan J. MacDonald & Siddharth Gandhi & Nikku Madhusudhan & Neale P. Gibson & Mahmoudreza Oshagh & Antonio Claret & Heike Rauer, 2017. "Detection of titanium oxide in the atmosphere of a hot Jupiter," Nature, Nature, vol. 549(7671), pages 238-241, September.
  • Handle: RePEc:nat:nature:v:549:y:2017:i:7671:d:10.1038_nature23651
    DOI: 10.1038/nature23651
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