An extrasolar planet sculpts the famous debris dish around Fomalhaut; probably ma ny other debris disks contain planets that we could locate if only we could better recognize their signatures in the dust that surrounds them. But the interaction between planets and debris disks involves both orbital resonances and collisions among grains and rocks in the disks --- difficult processes to model simultanemus]y. I will describe new 3-D models of debris disk dynamics that incorporate both collisions and resonant trapping of dust for the first time, allowing us to decode debris disk images and read the signatures of the planets they contain.
Reading the Signatures of Extrasolar Planets in Debris Disks
Satellite Workshop: Dynamics of Outer Planetary Systems ; 2009 ; Edinburgh, Scotland, United Kingdom
2009-11-09
Conference paper
No indication
English
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