Warm Spitzer Studies of the Atmospheres of Kepler-Detected Exoplanets

Computer Science – Performance

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Scientific paper

I present results from an ongoing project to use the Spitzer Space Telescope to gather near-infrared photometric measurements of the atmospheres of transiting extrasolar planets detecting by the Kepler Mission. I will first briefly review the instrumental performance of the Warm Spitzer mission for exoplanet measurements. I will then describe the atmospheric studies of the highly-irradiated transiting hot-Jupiters Kepler-5b and Kepler-6b. Spitzer studies of these objects are valuable since our near-infrared observations are complemented by constraints on the geometric albedo in the optical from the Kepler Mission photometry. By combining secondary eclipse measurements of the reflected starlight in the optical with estimates of the thermal emission in the near-infrared, we are able to constrain the energy budget of these planets and compare such constraints to those for the Solar system giant planets.

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