English

Resonant stratification in Titan's global ocean

Earth and Planetary Astrophysics 2023-12-12 v1 Fluid Dynamics

Abstract

Titan's ice shell floats on top of a global ocean revealed by the large tidal Love number k2=0.616±0.067k_2 = 0.616\pm0.067 registered by Cassini. The Cassini observation exceeds the predicted k2k_2 by one order of magnitude in the absence of an ocean, and is 3-σ\sigma away from the predicted k2k_2 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 S200S\gtrsim200 g/kg) can explain the 3-σ\sigma signal in k2k_2. Here we revisit previous interpretations of Titan's large k2k_2 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 k2k_2 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

R2 v1 2026-06-28T13:46:06.231Z