A detailed numerical analysis of asymmetrical density distribution in Saturn's F ring during an encounter with Prometheus
Saturn's rings, reminiscent of an early Solar system present a unique opportunity to investigate experimentally some mechanisms thought to be responsible for planet and planetesimal formation in protoplanetary discs. Here, we extended the comparison of our numerical models of Prometheus encount...
Saved in:
| Main Authors: | , |
|---|---|
| Format: | Default Article |
| Published: |
2014
|
| Subjects: | |
| Online Access: | https://hdl.handle.net/2134/14525 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|