The growth of embryos considering SPH-collision studies

Autor(en)
Elke Pilat-Lohinger, Thomas Maindl, David Bancelin, Christoph Schäfer
Abstrakt

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(en)
Institut für Astrophysik
Externe Organisation(en)
Eberhard Karls Universität Tübingen
Band
13
Publikationsdatum
09-2019
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/7c99db3b-854e-4295-bc12-01241a7a3a10