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Disruption and reaccretion of midsized moons during an outer solar system Late Heavy Bombardment

  • Author(s): Movshovitz, N.
  • Nimmo, F.
  • Korycansky, D. G
  • Asphaug, E.
  • Owen, J. M
  • et al.
Abstract

We investigate the problem of satellite survival during a hypothetical late heavy bombardment in the outer solar system, as predicted by the Nice Model (Tsiganis, Gomes, Morbidelli, & Levison 2005, Nature 435). Using a Monte-Carlo approach we calculate, for satellites of Jupiter, Saturn, and Uranus, the probability of experiencing a catastrophic collision during the LHB. We find that Mimas, Enceladus, Tethys, and Miranda experience at least one catastrophic impact in every simulation. Because re-accretion is expected to be rapid, these bodies will have emerged as scrambled mixtures of rock and ice. Tidal heating may have subsequently modified the latter three, but in the nominal LHB model Mimas should be a largely undifferentiated, homo geneous body. A differentiated Mimas would imply either that this body formed late, or that the Nice model requires significant modification.

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