Size distribution of particles in Saturn's rings, missed moonlets and misinterpretation of Chariklo rings
Nick Gorkavyi

TL;DR
This paper critiques existing models of particle size distribution in Saturn's rings and Chariklo's rings, highlighting their limitations in explaining moonlets and ring boundaries, and suggests the need for more comprehensive physical mechanisms.
Contribution
The paper provides a critical analysis of previous models, emphasizing the importance of self-gravitation and differential rotation effects, and questions the applicability of current models to moonlets and proto-satellite disks.
Findings
Existing models do not account for moonlets and ring boundaries.
Self-gravitation and differential rotation are key effects missing in current models.
Current models are inadequate for explaining Chariklo's rings as proto-satellite disks.
Abstract
Brilliantov et al. (PNAS, 2015) propose a model for the size distribution ~R^-3 for small particles with radius R and ~exp(-(R/Rc)^3) for large particles, where Rc=5.5 m. In 1989 Longaretti found analytically ~R^-3 for small particles and R^-6 for large ones (2). The law R^-6 also describes moonlets with size ~ 0.1-1 km. Cut-off law from Brilliantov et al. model does not describe moonlets and requires new mechanism for the origin of ~ 1 km size bodies. This model does not take into account the key effects of self-gravitation of large particles and differential rotation of the rings. Longaretti used a more accurate model of destruction of particles: "A relative increase of the erosion/destruction rate of the large particles must take place, because these particles have relative velocities of collision larger than the dispersion velocity, due to the differential Keplerian motion". The new…
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 · Space Exploration and Technology · Planetary Science and Exploration
