San Francisco / Paris / Princeton / Berlin / Amsterdam / Toronto / /
Company
Hamiltonian Systems / GM / /
Country
France / United States / Canada / /
Currency
pence / / /
Facility
Institute of Tectonics / University of Toronto / Canadian Institute / University of California / /
IndustryTerm
orbital energy / gas surface density / gas surface densities / ruby chips / gas envelope / negative energy / solar metal abundance / planetesimal removes energy / positive energy / energy / metal / gas interior / stainless steel bolts / planetesimal energy / gas disk / energy transfer / gas giant / /
Organization
University of Toronto / Toronto / Canadian Institute for Theoretical Astrophysics / Institute of Tectonics / Berkeley Geochronology Center / Canadian Institute for Advanced Research / Institut de Physique / University of California / Santa Cruz / African Union / Earth Sciences Department / Natural Sciences and Engineering Research Council of Canada / Astronomical Society of the Pacific / Princeton Univ. / /
Person
G. Burki / S. Gilder / R. P. Butler / T. Mazeh / Jonathan Glen / Fe / G. W. Marcy / /
Position
Mayor / Sc Mp / Mp / order Mp / MJ Mp / Butler / Astrophys / candidate / M. Mayor / Butler / /
ProvinceOrState
New Jersey / Maryland / Delaware / California / Ontario / /
REPORTS Migrating Planets N. Murray,* B. Hansen, M. Holman, S. Tremaine A planet orbiting in a disk of planetesimals can experience an instability in which it migrates to smaller orbital radii. Resonant interactions bet