Reconstruction of Callisto's Valhalla basin using n-body and SPH simulations
- Autor(en)
- Philip Winter, Thomas Maindl, Christoph Schäfer, Mattia Galiazzo
- Abstrakt
We present results of n-body and smooth particle hydrodynamics (SPH) simulations, exploring the crater formation process of the Valhalla crater located on the Jovian Moon Callisto. We compute typical impact velocities and impact angles which we then use as input for the SPH simulations to reconstruct the actual crater formation. Using a three-layered Callisto model with a subsurface ocean, we find significant connections between the crater formation process and the interaction with the subsurface ocean. We also investigate the properties of the projectile and numerical effects of low-resolution projectiles in the context of SPH.
- Organisation(en)
- Institut für Astrophysik
- Externe Organisation(en)
- Eberhard Karls Universität Tübingen
- Publikationsdatum
- 09-2017
- ÖFOS 2012
- 103003 Astronomie, 103004 Astrophysik
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/4b70a4fe-c8be-4aa5-adac-9a9ca6703d6a