Discovery of lake-effect clouds on Titan

Details Discovery of lake-effect clouds on Titan Discovery of lake-effect clouds on Titan

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufm.p12a..03b&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #P12A-03

Mathematics

Logic

0343 Planetary Atmospheres (5210, 5405, 5704), 3307 Boundary Layer Processes, 3346 Planetary Meteorology (5445, 5739), 6281 Titan

Scientific paper

Images from instruments on Cassini as well as from telescopes on the ground reveal the presence of sporadic small-scale cloud activity in the cold late-winter north polar of Saturn's large moon Titan. These clouds lie underneath the previously discovered uniform polar cloud attributed to a quiescent ethane cloud at ~40 km and appear confined to the same latitudes as those of the largest known hydrocarbon lakes at the north pole of Titan. The physical properties of these clouds suggest that they are due to methane convection and condensation. Such convection has not been predicted for the cold winter pole, but can be caused by a process in many ways analogous to terrestrial lake-effect clouds. The lakes on Titan are a key connection between the surface and the meteorological cycle.

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