Hydrocarbon lakes on Titan: Distribution and interaction with a porous regolith

210Citations
Citations of this article
95Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Synthetic Aperture Radar (SAR) images of Titan's north polar region reveal quasi-circular to complex features which are interpreted to be liquid hydrocarbon lakes. We investigate methane transport in Titan's hydrologic cycle using the global distribution of lake features. As of May 2007, the SAR data set covers ∼22% of the surface and indicates multiple lake morphologies which are correlated across the polar region. Lakes are limited to latitudes above 55°N and vary from <10 to more than 100,000 km2. The size and location of lakes provide constraints on parameters associated with subsurface transport. Using porous media properties inferred from Huygens probe observations, timescales for flow into and out of observed lakes are shown to be in the tens of years, similar to seasonal cycles. Derived timescales are compared to the time between collocated SAR observations in order to consider the role of subsurface transport in Titan's hydrologic cycle. Copyright 2008 by the American Geophysical Union.

Cite

CITATION STYLE

APA

Hayes, A., Aharonson, O., Callahan, P., Elachi, C., Gim, Y., Kirk, R., … Wall, S. (2008). Hydrocarbon lakes on Titan: Distribution and interaction with a porous regolith. Geophysical Research Letters, 35(9). https://doi.org/10.1029/2008GL033409

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free