The growth of embryos considering SPH-collision studies

Author(s)
Elke Pilat-Lohinger, Thomas Maindl, David Bancelin, Christoph Schäfer
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.

Organisation(s)
Department of Astrophysics
External organisation(s)
Eberhard Karls Universität Tübingen
Volume
13
Publication date
09-2019
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Portal url
https://ucrisportal.univie.ac.at/en/publications/7c99db3b-854e-4295-bc12-01241a7a3a10