کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1773603 | 1021140 | 2012 | 4 صفحه PDF | دانلود رایگان |
![عکس صفحه اول مقاله: Explaining why the uranian satellites have equatorial prograde orbits despite the large planetary obliquity Explaining why the uranian satellites have equatorial prograde orbits despite the large planetary obliquity](/preview/png/1773603.png)
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°.
Journal: Icarus - Volume 219, Issue 2, June 2012, Pages 737–740