last update at July 22, 2010

Goal:
Planet formation theories have been stimulated by observations of
protoplanetary disks, exoplanets, debris disks, and Saturnian
ring. In particular, the diversity of extrasolar planets forces
theorists to change and generalize the model for formation of the
solar system. Here we summarize the observational constrains, review
the current status, and discuss the future perspectives of theories
for planet formation.
Topics (invited speakers):
Scientific Organizing Committee:
Eiichiro Kokubo (National Astronomical Observatory Japan) Kees Dullemond (Max Planck Institute for Astronomy) Tristan Guillot (Observatoire de la Cote d'Azur) Greg Laughlin (Univ. of California, Santa Cruz) Frédéric Masset (Laboratoire AIM, CEA/DSM - CNRS) Local Organizing Committee (ishigaki2010 @ geo.titech.ac.jp)
Eiichiro Kokubo, Takeshi Miyaji (National Astronomical Observatory Japan) Sponsorship:
Global COE program "From the Earth to Earths" (Tokyo Institute of Technology/Univ. of Tokyo)
National Astronomical Observatory Japan Ishigaki city |