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SUMMARY:How Jupiter's gas-driven migration shaped the inner Solar System -
  Sean Raymond (CNRS\, Bordeaux)
DTSTART:20111114T160000Z
DTEND:20111114T170000Z
UID:TALK32549@talks.cam.ac.uk
CONTACT:Henrik Latter
DESCRIPTION:I will present a new model for the evolution of the Solar Syst
 em -- called\nthe Grand Tack -- that invokes a large scale\, inward-then-o
 utward migration\nof Jupiter in the gaseous protoplanetary disk.  This mod
 el is able to\nreproduce both the terrestrial planets and the asteroid bel
 t.  I will also\nshow how Uranus and Neptune's growth can\, in some circum
 stances\, be\naccelerated by the gas giants' outward migration.\n
LOCATION:MR14\,  Centre for Mathematical Sciences\, Wilberforce Road\, Cam
 bridge
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