Explaining why the uranian satellites have equatorial prograde orbits despite the large planetary obliquity
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°.
Additional Information
© 2012 Elsevier Inc. Received 16 November 2011; Revised 23 March 2012; Accepted 27 March 2012; Available online 3 April 2012.Attached Files
Submitted - 1208.4685.pdf
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Additional details
- Eprint ID
- 32354
- DOI
- 10.1016/j.icarus.2012.03.025
- Resolver ID
- CaltechAUTHORS:20120711-122936061
- Created
-
2012-07-11Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences