Volume 420, Number 3, June IV 2004
|Page(s)||1153 - 1162|
|Section||Planets and planetary systems|
|Published online||04 June 2004|
The detectability of extrasolar planet surroundings
I. Reflected-light photometry of unresolved rings
Observatoire de Haute-Provence, CNRS, 04870 Saint-Michel-l'Observatoire, France
2 Observatoire de Paris-Meudon, 92195 Meudon Cedex, France e-mail: Jean.Schneider@obspm.fr
Corresponding author: L. Arnold, email@example.com
Accepted: 9 March 2004
It is expected that the next generation of high-contrast imaging instruments will deliver the first unresolved image of an extrasolar planet. The emitted thermal infrared light from the planet should show no phase effect assuming the planet is in thermal equilibrium. But the reflected visible light will vary with phase angle. Here we study the photometric variation of the reflected light with orbital phase of a ringed extrasolar planet. We show that a ring around an extrasolar planet, both obviously unresolved, can be detected by its specific photometric signature. A simple quantitative model is discussed, taking into account the basic optical and geometrical properties of the ringed planet.
Key words: planetary systems / planets: rings
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.