How does salinity shape ocean circulation and ice geometry on Enceladus and other icy satellites?
Wanying Kang, Tushar Mittal, Suyash Bire, Jean-Michel Campin, and John, Marshall

TL;DR
This study explores how salinity influences ocean circulation and ice shell geometry on Enceladus, revealing that intermediate salinity levels lead to reduced overturning and better ice thickness regulation, impacting habitability assessments.
Contribution
It demonstrates how salinity and heat partitioning affect ocean dynamics and ice geometry, providing new insights into the conditions necessary for observed ice features on icy satellites.
Findings
Intermediate salinity reduces ocean overturning.
Heat convergence towards the equator maintains ice thickness.
Core heat sources conflict with observed ice dissipation requirements.
Abstract
Of profound astrobiological interest, Enceladus appears to have a global subsurface ocean that is salty, indicating water-rock reaction at present or in the past, important for its habitability. Here, we investigate how salinity and the partition of heat production between the silicate core and the ice shell affect ocean dynamics and the associated heat transport -- a key factor that determines the equilibrium ice shell geometry. Assuming steady state conditions, we show that the meridional overturning circulation of the ocean, driven by heat and salt exchange with the ice, has opposing signs at very low and very high salinities. Regardless of these differing circulations, heat and freshwater converge towards the equator, where the ice is thick, acting to homogenize thickness variations. In order to maintain the observed ice thickness variation, the polar-amplified ice dissipation needs…
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Taxonomy
TopicsAstro and Planetary Science · Spacecraft and Cryogenic Technologies · Methane Hydrates and Related Phenomena
