Discovery of lake-effect clouds on Titan

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 region of Saturn's large moon Titan. These clouds lie underneath the previously discovered uniform polar cloud attributed to...

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Bibliographic Details
Published in:Geophysical Research Letters
Main Authors: Brown, M. E., Schaller, E. L., Roe, H. G., Chen, C., Roberts, J., Brown, R. H., Baines, K. H., Clark, R. N.
Format: Article in Journal/Newspaper
Language:English
Published: American Geophysical Union 2009
Subjects:
Online Access:https://authors.library.caltech.edu/13341/
https://authors.library.caltech.edu/13341/1/BROgrl09.pdf
https://authors.library.caltech.edu/13341/3/0809.1841.pdf
https://resolver.caltech.edu/CaltechAUTHORS:BROgrl09
Description
Summary: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 region of Saturn's large moon Titan. These clouds lie underneath the previously discovered uniform polar cloud attributed to a quiescent ethane cloud at similar to 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 could be caused by a process in some ways analogous to terrestrial lake-effect clouds. The lakes on Titan could be a key connection between the surface and the meteorological cycle.