Exploring the thermal emission of two new transiting planets from the WASP survey

Details Exploring the thermal emission of two new transiting planets from the WASP survey Exploring the thermal emission of two new transiting planets from the WASP survey

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sptz.prop..282w&link_type=abstract

Spitzer Proposal ID #282

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Scientific paper

We are shortly to announce the discovery of two transiting extra-solar planets from the Wide Angle Search for Planets (WASP) survey. One is expected to be the hottest of all hot Jupiters observable by Spitzer. The other may have suffered significant mass loss. Here we propose to use the unique capability of Spitzer to detect the thermal emission of both planets using secondary eclipse observations. We will measure their temperatures, and test planetary atmosphere models in a new high temperature regime. We will also search for modified molecular abundances that might result from mass loss. These observations will also inform the planning of a more comprehensive follow up programme of these important new planets in Cycle-4.

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