Session 25. Planet and Satellite Origins I: Disks, Nebulae and Giant Planets

Oral, Chairs: A. P. Boss and J. J. Lissaurer, Thursday, September 4, 2003, 1:30-3:20pm, DeAnza I-II

25.01 The Formation of a Planet in the Eye of a Hurricane -- A Three Phase Model for Planet Formation

H. Klahr (MPI fuer Astronomie), P. Bodenheimer (UCO/Lick Observatory)

25.02 A Simplified Model for Rossby Wave Instabilities in Protoplanetary Disks

G.R. Stewart (Univ. of Colorado)

25.03 Hydrodynamic Instability and Enhanced Transport in Protoplanetary Nebulae

D.T. Richard (NASA Ames)

25.04 Protoplanetary Nebula Evolution using the Beta Viscosity Model

S. S. Davis (NASA Ames Research Center)

25.05 Hydrodynamical Shear Instability in Accretion Disks?

I. Mosqueira (NASA Ames/SETI Institute), S. Kassinos (Univ. of Cyprus/Stanford Univ.), K. Shariff, J. N. Cuzzi (NASA Ames)

25.06 Small Core for Jupiter using the Core Instability Model

O. Hubickyj, P. Bodenheimer (UCO/Lick Obs. @ UCSC), J. Lissauer (NASA Ames Research Center)

25.07 Planetary Accretion: Beyond the ``Isolation Mass”

S. J. Weidenschilling, D. R. Davis (Planetary Science Institute)

25.08 Jupiter's formation: early or late?

T. Guillot (Observatoire de la Côte d'Azur), R. Hueso (E.T.S. Ing. Industriales y Telecom)

25.09 A Gas-poor Planetesimal Feeding Model for the Formation of Giant Planet Satellite Systems: Disk Size and Formation Timescale

P. R. Estrada (NASA Ames), I. Mosqueira (NASA Ames/SETI Institute)

25.10 Rapid Formation of Giant Planets in Binary Star Systems

A. P. Boss (Carnegie Institution)

25.11 Angular Momentum Constraints on Planet Migration.

W. R. Ward (Southwest Research Institute)