2 papers
astro-ph.EP2026
Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact
Keiya Murashima, Takanori Sasaki
The obliquity of Uranus is widely attributed to a giant impact that ejected material and formed a debris disk, which subsequently coalesced into its regular satellites.…
astro-ph.EP2024
Modifications of SPH towards three-dimensional simulations of an icy moon with internal ocean
Keiya Murashima, Natsuki Hosono, Takayuki R. Saitoh +1
There are some traces of the existence of internal ocean in some icy moons, such as the vapor plumes of Europa and Enceladus. This implies a region of liquid water beneath the surf…