Collisional Stripping and Disruption of Super-Earths
Robert A. Marcus, Sarah T. Stewart, Dimitar Sasselov, Lars Hernquist

TL;DR
This paper uses hydrodynamics simulations to study high-velocity collisions between super-Earths, revealing how such impacts can lead to planetary disruption, compositional changes, and different collision regimes during planet formation.
Contribution
It provides new criteria for catastrophic disruption, transition energy, and a scaling law for compositional changes in super-Earth collisions.
Findings
Disruption occurs at high velocities, small impact parameters, or small projectile mass.
Derived criteria for catastrophic disruption and transition energy.
Established a scaling law for compositional changes due to mantle stripping.
Abstract
The final stage of planet formation is dominated by collisions between planetary embryos. The dynamics of this stage determine the orbital configuration and the mass and composition of planets in the system. In the solar system, late giant impacts have been proposed for Mercury, Earth, Mars, and Pluto. In the case of Mercury, this giant impact may have significantly altered the bulk composition of the planet. Here we present the results of smoothed particle hydrodynamics simulations of high-velocity (up to ~5 v_esc) collisions between 1 and 10 M_Earth planets of initially terrestrial composition to investigate the end stages of formation of extrasolar super-Earths. As found in previous simulations of collisions between smaller bodies, when collision energies exceed simple merging, giant impacts are divided into two regimes: (1) disruption and (2) hit-and-run (a grazing inelastic…
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