Gravitational Interactions Between Protoplanets and Planetismal Disks of Equal Mass
B. D. Lindsay, K. W. Orr, T. W. Hyde, L. Barge
Abstract
Numerical simulations show that planetesimal systems with unevenly distributed masses may actually be more stable than those where all the bodies are of roughly equal size.
Create a lesson
Related papers
Solar Magnetic Configuration Control over Radiation Belt Electrons
Ahmad Lalti, Jonathan Rae, Clare Watt et al.
Statistical Models of Ionospheric Variability and Irregularities in the Topside Ionosphere Based on the Swarm Satellite Data
Daria Kotova, Alan Wood, Eelco Doornbos et al.
A quiet STEVE disturbs navigation satellites' signals in the Antarctic
Daria Kotova, Luca Spogli, Yaqi Jin et al.
Empirical Relationship for Geomagnetically Induced Currents (GIC) and Solar Wind Conditions
Dean Thomas, Lucy A. Wilkerson, Robert S. Weigel et al.
Comprehensive solar eruption analyses enabled by the tools of the SOLER project
Nina Dresing, Jan Gieseler, Markus Baumgartner-Steinleitner et al.
Evolution of lunar wake potentials: structure, energy conversion, and their imprints on velocity distributions
Xin An, Vassilis Angelopoulos, Jasper S. Halekas et al.