A New 24 micron Phase Curve for upsilon Andromedae b

Details A New 24 micron Phase Curve for upsilon Andromedae b A New 24 micron Phase Curve for upsilon Andromedae b

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dps....42.5209c&link_type=abstract

American Astronomical Society, DPS meeting #42, #52.09; Bulletin of the American Astronomical Society, Vol. 42, p.1071

Astronomy and Astrophysics

Astronomy

Scientific paper

We report the detection of 24 um variations from the planet-hosting τπσιλον Andromedae system consistent with the orbital periodicity of the system's innermost planet, τπσιλον And b. Fitting a simple model with two hemispheres of constant surface brightness to our observations gives a peak-to-valley phase curve amplitude of 0.00130 times the mean system flux. Assuming a planetary radius of 1.3 RJup , this corresponds to a planetary temperature contrast of >900 K and an orbital inclination of >25 deg. We further report the largest phase offset yet observed for an extrasolar planet: the flux maximum occurs 80 deg before phase 0.5. Such a large phase offset is difficult to reconcile with most current atmospheric circulation models. We improve on earlier observations of this system in several important ways: (1) observations of a flux calibrator star demonstrate the MIPS detector is stable to 104 on long timescales, (2) we note that the background light varies systematically due to spacecraft operations, precluding use of this background as a flux calibrator (stellar flux measured above the background is not similarly affected), and (3) we calibrate for flux variability correlated with motion of the star on the MIPS detector. A reanalysis of our earlier observations of this system is consistent with our new result.

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