A Spitzer Spectrum of the Transiting Exoplanet HD 189733b

Details A Spitzer Spectrum of the Transiting Exoplanet HD 189733b A Spitzer Spectrum of the Transiting Exoplanet HD 189733b

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop30473g&link_type=abstract

Spitzer Proposal ID #30473

Physics

Scientific paper

We propose to obtain a 7-15 micron IRS spectrum of the newly discovered, transiting extrasolar giant planet HD 189733b. The flux contrast is sufficiently high, and the parent star sufficiently nearby, that differential spectroscopy should yield a moderate signal-to-noise ratio spectrum in a relatively short amount of time. This would represent an enormous leap in our capabilities, ushering in a new era of detailed, quantitative spectral studies of nearby exoplanets.

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