Titan

Titan's Dynamic Love Number Implies Stably-Stratified Ocean

By Keith Cowing
astro-ph.EP
May 12, 2019
Filed under
Titan's Dynamic Love Number Implies Stably-Stratified Ocean
Titan
NASA

The dynamic quadrupole Love number of Titan measured by Cassini is k2,obs=0.616±0.067, strongly indicating a global subsurface ocean.

However, the theoretical Love number due to equilibrium tides is at most kmax2,eq≈0.48 in the absence of an ice shell on top of the ocean. In reality, there is an outer ice shell of thickness 100km, reducing the equilibrium-tide Love number to k2,eq≈0.42. Therefore, other types of tidal response, like dynamic tides, may be also present in Titan. We propose that the ocean is stably stratified. As a result, there exist standing ocean waves (gravity modes) with eigen-frequencies close to the tidal frequency. Such a gravity mode (g-mode) is resonantly excited. It bends the outer ice shell radially and thus enhances the dynamic Love number by k2,g. In order for k2,g to account for the discrepancy between k2,eq and k2,obs, the Brunt-Vaisala frequency in the ocean is required to be 3.3×10−4rads−1.

It is compatible with the volatile-rich model for Titan that was proposed to explain the methane-rich atmosphere. The three components of the tidal potential with azimuthal degrees, m=−2,0,2, correspond to the three components of the quadrupole Love number, k2,−2, k2,0 and k2,2. They can excite retrograde, axisymmetric and prograde g-modes equally in the absence of rotation.

However, Coriolis force induced by Titan’s rotation breaks the symmetry among these modes. Most likely, only one of the Love-number components is significantly enhanced by a g-mode, while the other two are still attributed to equilibrium tides. This prediction is testable by observation. If confirmed, the smaller components of the Love number can be used to constrain the thickness of the outer ice shell.

Jing Luan
(Submitted on 9 May 2019)
Comments: Comments are welcome. Submit to Icarus
Subjects: Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:1905.03802 [astro-ph.EP] (or arXiv:1905.03802v1 [astro-ph.EP] for this version)
Submission history
From: Jing Luan
[v1] Thu, 9 May 2019 18:06:34 UTC (232 KB)
https://arxiv.org/abs/1905.03802
Astrobiology

Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻