Constraints to Uranus' Great Collision. IV. The Origin of Prospero
Gabriela Parisi (IAR-LaPlata), Giovanni Carraro (ESO-Santiago),, Michele Maris (OATS), Adrian Brunini (LaPlata)

TL;DR
This paper investigates whether Uranus's large obliquity resulted from a great collision and explores the origin of its irregular moon Prospero, analyzing capture mechanisms and their plausibility within planetary formation scenarios.
Contribution
It provides a detailed analysis of the collision hypothesis for Uranus's obliquity and evaluates potential formation mechanisms for Prospero, considering various timing and capture scenarios.
Findings
Prospero could not have existed during the collision event.
Capture of Prospero after the collision is dynamically challenging.
The collision hypothesis for Uranus's obliquity remains uncertain.
Abstract
It is widely accepted that the large obliquity of Uranus is the result of a great tangential collision (GC) with an Earth size proto-planet at the end of the accretion. We attempt to constraint the GC scenario as the cause of Uranus' obliquity as well as on the mechanisms able to give origin to the Uranian irregulars. Different capture mechanisms for irregulars operate at different stages on the giant planets formation process. The mechanisms able to capture the uranian irregulars before and after the GC are analysed. Assuming that they were captured before the GC, we calculate the orbital transfer of the nine irregulars by the impulse imparted by the GC. If their orbital transfer results dynamically implausible, they should have originated after the GC. We investigate and discuss the dissipative mechanisms able to operate later. In particular Prospero could not exist at the time of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstro and Planetary Science · Historical Astronomy and Related Studies
