A Simplified Model for the Forced Libration of Icy Moons with Subsurface Oceans: Application to Enceladus and Mimas
In this work, we investigate a minimalist model capable of accurately replicating the forced librations of an icy moon with a subsurface ocean.
The model holds potential to predict the presence of a subsurface ocean through analysis of longitudinal librations.
We demonstrate that a two-layered model, with a prestressed icy crust and a fixed mantle cavity, can effectively model the librational behavior of icy moons. The proposed model is applied to model the longitudinal libration of Enceladus and Mimas, two medium-sized icy moons of Saturn.
Yeva Gevorgyan
Comments: 7 pages, 12 figures, submitted to MNRAS
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2405.03350 [astro-ph.EP] (or arXiv:2405.03350v1 [astro-ph.EP] for this version)
Submission history
From: Yeva Gevorgyan
[v1] Mon, 6 May 2024 11:01:54 UTC (1,674 KB)
https://arxiv.org/abs/2405.03350
Astrobiology,