Title

A Spectrum Of An Extrasolar Planet

Abstract

Of the over 200 known extrasolar planets, 14 exhibit transits in front of their parent stars as seen from Earth. Spectroscopic observations of the transiting planets can probe the physical conditions of their atmospheres. One such technique can be used to derive the planetary spectrum by subtracting the stellar spectrum measured during eclipse (planet hidden behind star) from the combined-light spectrum measured outside eclipse (star + planet). Although several attempts have been made from Earth-based observatories, no spectrum has yet been measured for any of the established extrasolar planets. Here we report a measurement of the infrared spectrum (7.5-13.2 μm) of the transiting extrasolar planet HD 209458b. Our observations reveal a hot thermal continuum for the planetary spectrum, with an approximately constant ratio to the stellar flux over this wavelength range. Superposed on this continuum is a broad emission peak centred near 9.65 μm that we attribute to emission by silicate clouds. We also find a narrow, unidentified emission feature at 7.78 νm. Models of these 'hot Jupiter' planets predict a flux peak near 10 μm, where thermal emission from the deep atmosphere emerges relatively unimpeded by water absorption, but models dominated by water fit the observed spectrum poorly.

Publication Date

2-22-2007

Publication Title

Nature

Volume

445

Issue

7130

Number of Pages

892-895

Document Type

Article

Personal Identifier

scopus

DOI Link

https://doi.org/10.1038/nature05636

Socpus ID

33847238401 (Scopus)

Source API URL

https://api.elsevier.com/content/abstract/scopus_id/33847238401

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