1. Search for rings and satellites around the exoplanet CoRoT-9b using Spitzer photometry
- Author
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Etangs, A. Lecavelier des, Hébrard, G., Blandin, S., Cassier, J., Deeg, H. J., Bonomo, A. S., Bouchy, F., Désert, J. -M., Ehrenreich, D., Deleuil, M., Díaz, R. F., and Moutou, C.
- Subjects
Astrophysics - Earth and Planetary Astrophysics - Abstract
Using Spitzer photometry at 4.5 microns, we search for rings and satellites around the long period transiting planet CoRoT-9b. We observed two transits in 2010 and 2011. From their non-detection, we derive upper limits on the plausible physical characteristics of these objects in the planet environment. We show that a satellite larger than about 2.5 Earth radii is excluded at 3-$\sigma$ for a wide range of elongations at the two epochs of observations. Combining the two observations, we conclude that rings are excluded for a wide variety of sizes and inclination. We find that for a ring extending up to the Roche limit, its inclination angle from the edge-on configuration as seen from the Earth must be lower than 13{\deg} in the case of silicate composition and lower than 3{\deg} in the case of material with water ice density., Comment: Accepted for publication in A&A
- Published
- 2017
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