Water transport and water loss by collisions during planet formation
- Autor(en)
- Thomas Maindl, Christoph Schäfer, Nader Haghighipour, David Bancelin, Christoph Burger, Rudolf Dvorak
- Abstrakt
We present results of collision simulations pertaining to water loss covering body masses ranging from a small planetary embryo to the mass of Earth. We find that for most realistic combinations of object masses, collision velocities, and impact angles a considerable amount of water is lost, which may significantly change the water inventory of formed terrestrial planets. Also, there is indication that beyond the 'usual' parameters characterizing a collision (velocity expressed in units of the mutual escape velocity and impact angle), water loss depends on factors like absolute mass, the projectile-target mass ratio, and to a certain extent the water distribution inside the objects.
- Organisation(en)
- Institut für Astrophysik
- Externe Organisation(en)
- Eberhard Karls Universität Tübingen, University of Hawaii
- Publikationsdatum
- 09-2017
- ÖFOS 2012
- 103004 Astrophysik, 103003 Astronomie
- Link zum Portal
- https://ucrisportal.univie.ac.at/de/publications/e20c82b6-32ca-4af0-b40f-0b2a01b2cc71