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Evolution of Orbital Eccentricity of a Protoplanet
1999The evolution of the orbital eccentricity of a planet due to tidal interaction with a protoplanetary disk is modeled. It is found that the eccentricity of the planet tends to increase when the mass of the planet is large enough to make a gap in the disk, i.e., is larger than about a Saturn mass.
openaire +1 more source
Scattering of Planetesimals by a Protoplanet: Slowing Down of Runaway Growth
Icarus, 1993Shigeru Ida, Junichiro Makino
exaly
Protoplanet Vesta and HED Meteorites
2022Harry Y. McSween, Richard P. Binzel
openaire +1 more source
Distribution of Planetesimals around a Protoplanet in the Nebula Gas
Icarus, 1997, Shigeru Ida
exaly
Kinematic Evidence for an Embedded Protoplanet in a Circumstellar Disk
Astrophysical Journal Letters, 2018C Pinte, F Menard, Gaspard Duchêne
exaly
N-Body simulation of gravitational interaction between planetesimals and a protoplanet
Icarus, 1992Shigeru Ida, Junichiro Makino
exaly

