Physics
Scientific paper
Feb 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012georl..3904201c&link_type=abstract
Geophysical Research Letters, Volume 39, Issue 4, CiteID L04201
Physics
Mineralogy And Petrology: Reactions And Phase Equilibria (1012, 8412), Planetary Sciences: Comets And Small Bodies: Ices, Planetary Sciences: Solar System Objects: Titan
Scientific paper
Titan's shape is characterized by a difference between the long equatorial radius and the polar radius that is several hundred meters larger than that predicted by the flattening due to its spin rate. The North polar region is covered by large mare filled with hydrocarbons, including ethane. Moreover global circulation models predict ethane precipitation on the polar areas. This study shows that the shape of Titan can be explained by the subsidence associated with the substitution of methane with ethane-rich liquids percolating into the crust which, as suggested by evolution models, may be composed of methane clathrate hydrates. Such substitutions have been observed in laboratory experiments. This process would provide an additional methane source as required for sustaining the presence of this constituent in Titan's atmosphere through its history. A 270 m subsidence of the polar caps is explained by the circulation of 1.5 to 6 × 1018 kg of ethane in the top three kilometers of an initially methane-clathrate crust. This process would have operated during the last 300-1200 Myr at the present ethane production rate.
Choukroun Mathieu
Sotin Ch.
No associations
LandOfFree
Is Titan's shape caused by its meteorology and carbon cycle? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Is Titan's shape caused by its meteorology and carbon cycle?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Is Titan's shape caused by its meteorology and carbon cycle? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1838881