Detection of titanium oxide in the atmosphere of a hot Jupiter

Elyar Sedaghati (), Henri M. J. Boffin, Ryan J. MacDonald, Siddharth Gandhi, Nikku Madhusudhan, Neale P. Gibson, Mahmoudreza Oshagh, Antonio Claret and Heike Rauer
Additional contact information
Elyar Sedaghati: European Southern Observatory
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
Antonio Claret: Instituto de Astrofísica de Andalucía, CSIC
Heike Rauer: Deutsches Zentrum für Luft- und Raumfahrt

Nature, 2017, vol. 549, issue 7671, 238-241

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

Date: 2017
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DOI: 10.1038/nature23651

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