Vertical compositional variations of liquid hydrocarbons in Titan’s alkanofers

¹ Université de Reims Champagne Ardenne, CNRS, GSMA UMR CNRS 7331, 51097 Reims, France
e-mail: daniel.cordier@univ-reims.fr
² NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA
³ Engineering Management of Additional Recovery, Mexican Petroleum Institute, Eje Central Lázaro Cárdenas Norte 152, 07730 Mexico City, Mexico

Received: 11 March 2021
Accepted: 22 June 2021

Abstract

Context. According to clues left by the Cassini mission, Titan, one of the two Solar System bodies with a hydrologic cycle, may harbor liquid hydrocarbon-based analogs of our terrestrial aquifers, referred to as “alkanofers”.

Aims. On the Earth, petroleum and natural gas reservoirs show a vertical gradient in chemical composition, established over geological timescales. In this work, we aim to investigate the conditions under which Titan’s processes could lead to similar situations.

Methods. We built numerical models including barodiffusion and thermodiffusion (Soret’s effect) in N₂+CH₄+C₂H₆ liquid mixtures, which are relevant for Titan’s possible alkanofers. Our main assumption is the existence of reservoirs of liquids trapped in a porous matrix with low permeability.

Results. Due to the small size of the molecule, nitrogen seems to be more sensitive to gravity than ethane, even if the latter has a slightly larger mass. This behavior, noticed for an isothermal crust, is reinforced by the presence of a geothermal gradient. Vertical composition gradients, formed over timescales of between a fraction of a mega-year to several tens of mega-years, are not influenced by molecular diffusion coefficients. We find that ethane does not accumulate at the bottom of the alkanofers under diffusion, leaving the question of why ethane is not observed on Titan’s surface unresolved. If the alkanofer liquid was in contact with water-ice, we checked that N₂ did not, in general, impede the clathration of C₂H₆, except in some layers. Interestingly, we found that noble gases could easily accumulate at the bottom of an alkanofer.