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 language | English |
---|---|
Title of host publication | EPSC-DPS Joint Meeting 2019 |
Volume | 13 |
Publication status | Published - Sep 2019 |
Austrian Fields of Science 2012
- 103003 Astronomy
- 103004 Astrophysics