A ground-based near-infrared emission spectrum of the exoplanet HD 189733b View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2010-02

AUTHORS

Mark R. Swain, Pieter Deroo, Caitlin A. Griffith, Giovanna Tinetti, Azam Thatte, Gautam Vasisht, Pin Chen, Jeroen Bouwman, Ian J. Crossfield, Daniel Angerhausen, Cristina Afonso, Thomas Henning

ABSTRACT

Exoplanet atmospheresSpace-based infrared spectroscopy has successfully identified various molecules — H2O, CH4, CO2 and CO — in the atmospheres of 'hot Jupiter' extrasolar planets. Swain et al. now report ground-based observations of the dayside emission spectrum of the hot Jupiter HD 189733b at near-infrared wavelengths not available to space-based telescopes. They find a bright emission feature at ∼3.25 μm which is unexpected and difficult to explain using current models that assume local thermodynamic equilibrium conditions. Fluorescence emission from methane, similar to that seen in the atmospheres of Solar System planets, seems a likely explanation. This work suggests that atmospheric chemistry on exoplanets is more complex than was thought, and opens the field of exoplanet molecular spectroscopy to ground-based telescopes. More... »

PAGES

637-639

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/nature08775

DOI

http://dx.doi.org/10.1038/nature08775

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1025359473

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/20130645


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