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NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity
- Source :
- Icarus, 219, 737 (2012)
- Publication Year :
- 2012
-
Abstract
- We show that the existence of prograde equatorial satellites is consistent with a collisional tilting scenario for Uranus. In fact, if the planet was surrounded by a proto-satellite disk at the time of the tilting and a massive ring of material was temporarily placed inside the Roche radius of the planet by the collision, the proto-satellite disk would have started to precess incoherently around the equator of the planet, up to a distance greater than that of Oberon. Collisional damping would then have collapsed it into a thin equatorial disk, from which the satellites eventually formed. The fact that the orbits of the satellites are prograde requires Uranus to have had a non-negligible initial obliquity (comparable to that of Neptune) before it was finally tilted to 98 degrees.
- Subjects :
- Astrophysics - Earth and Planetary Astrophysics
Subjects
Details
- Database :
- arXiv
- Journal :
- Icarus, 219, 737 (2012)
- Publication Type :
- Report
- Accession number :
- edsarx.1208.4685
- Document Type :
- Working Paper
- Full Text :
- https://doi.org/10.1016/j.icarus.2012.03.025