The growth of embryos considering SPH-collision studies

Elke Pilat-Lohinger, Thomas Maindl, David Bancelin, Christoph Schäfer

Publications: Contribution to bookContribution to proceedings

Abstract

To get more realistic results for terrestrial planet formation we combine N-body simulations with SPH collision studies. In this context we show the mass-loss and water-loss for Moon- and Mars-size bodies after collision where we consider various impact angles which have been determined in N-body simulations.
Original languageEnglish
Title of host publicationEPSC-DPS Joint Meeting 2019
Volume13
Publication statusPublished - Sep 2019

Austrian Fields of Science 2012

  • 103003 Astronomy
  • 103004 Astrophysics

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