Resonant stratification in Titan's global ocean
Abstract
Titan's ice shell floats on top of a global ocean revealed by the large tidal Love number registered by Cassini. The Cassini observation exceeds the predicted by one order of magnitude in the absence of an ocean, and is 3- away from the predicted if the ocean is pure water resting on top of a rigid ocean floor. Previous studies demonstrate that an ocean heavily enriched in salts (salinity g/kg) can explain the 3- signal in . Here we revisit previous interpretations of Titan's large using simple physical arguments and propose a new interpretation based on the dynamic tidal response of a stably stratified ocean in resonance with eccentricity tides raised by Saturn. Our models include inertial effects from a full consideration of the Coriolis force and the radial stratification of the ocean, typically neglected or approximated elsewhere. The stratification of the ocean emerges from a salinity profile where salt concentration linearly increases with depth. We find multiple salinity profiles that lead to the required by Cassini. In contrast with previous interpretations that neglect stratification, resonant stratification reduces the bulk salinity required by observations by an order of magnitude, reaching a salinity for Titan's ocean that is compatible with that of Earth's oceans and close to Enceladus' plumes. Consequently, no special process is required to enrich Titan's ocean to a high salinity as previously suggested.
Keywords
Cite
@article{arxiv.2312.05723,
title = {Resonant stratification in Titan's global ocean},
author = {Benjamin Idini and Francis Nimmo},
journal= {arXiv preprint arXiv:2312.05723},
year = {2023}
}
Comments
29 pages, 8 figures, accepted to PSJ