An Upper Limit on the Albedo of HD 209458b: Direct Imaging Photometry with the MOST Satellite

Details An Upper Limit on the Albedo of HD 209458b: Direct Imaging Photometry with the MOST Satellite An Upper Limit on the Albedo of HD 209458b: Direct Imaging Photometry with the MOST Satellite

2006-03-16

arxiv.org/abs/astro-ph/0603410v1

Astrophys.J.646:1241-1251,2006

Astronomy and Astrophysics

Astrophysics

29 pages, 9 figures. Accepted for publication in the Astrophysical Journal (July 2006, v645n1)

Scientific paper

10.1086/504252

We present space-based photometry of the transiting exoplanetary system HD 209458 obtained with the MOST (Microvariablity and Oscillations of STars) satellite, spanning 14 days and covering 4 transits and 4 secondary eclipses. The HD 209458 photometry was obtained in MOST's lower-precision Direct Imaging mode, which is used for targets in the brightness range $6.5 < V < 13$. We describe the photometric reduction techniques for this mode of observing, in particular the corrections for stray Earthshine. We do not detect the secondary eclipse in the MOST data, to a limit in depth of 0.053 mmag (1 \sigma). We set a 1 \sigma upper limit on the planet-star flux ratio of 4.88 x 10^-5 corresponding to a geometric albedo upper limit in the MOST bandpass (400 to 700 nm) of 0.25. The corresponding numbers at the 3 \sigma level are 1.34 x 10^-4 and 0.68 respectively. HD 209458b is half as bright as Jupiter in the MOST bandpass. This low geometric albedo value is an important constraint for theoretical models of the HD209458b atmosphere, in particular ruling out the presence of reflective clouds. A second MOST campaign on HD 209458 is expected to be sensitive to an exoplanet albedo as low as 0.13 (1 sigma), if the star does not become more intrinsically variable in the meantime.

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