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4 papers · 2 filters
Unconvergence of Very Large Scale GI Simulations
Natsuki Hosono, Masaki Iwasawa, Ataru Tanikawa +3
The giant impact (GI) is one of the most important hypotheses both in planetary science and geoscience, since it is related to the origin of the Moon and also the initial condition…
Constraints on the size and dynamics of the J1407b ring system
Steven Rieder, Matthew A. Kenworthy
Context. J1407 (1SWASP J140747.93-394542.6 in full) is a young star in the Scorpius-Centaurus OB association that underwent a series of complex eclipses over 56 days in 2007. To ex…
The Giant Impact Simulations with Density Independent Smoothed Particle Hydrodynamics
Natsuki Hosono, Takayuki R. Saitoh, Junichiro Makino +2
At present, the giant impact (GI) is the most widely accepted model for the origin of the Moon. Most of the numerical simulations of GI have been carried out with the smoothed part…
Global High-resolution -body Simulation of Planet Formation I. Planetesimal Driven Migration
Junko Kominami, Hiroshi Daisaka, Junichiro Makino +1
We investigated whether outward Planetesimal Driven Migration (PDM) takes place or not in simulations when the self gravity of planetesimals is included. We performed -body simu…