Evidence for a Polar Ethane Cloud on Titan

Spectra from Cassini’s Visual and Infrared Mapping Spectrometer reveal the presence of a vast tropospheric cloud on Titan at latitudes 51- to 68- north and all longitudes observed (10- to 190- west). The derived characteristics indicate that this cloud is composed of ethane and forms as a result of...

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Bibliographic Details
Published in:Science
Main Authors: Griffith, C. A., Penteado, P., Rannou, P., Brown, R., Boudon, V., Baines, K. H., Clark, R., Drossart, P., Buratti, B., Nicholson, P., McKay, C. P., Coustenis, A., Negrao, A., Jaumann, R.
Format: Other Non-Article Part of Journal/Newspaper
Language:unknown
Published: 2006
Subjects:
Planetengeologie
North Pole
Online Access:http://elib.dlr.de/45050/
Description
Summary:Spectra from Cassini’s Visual and Infrared Mapping Spectrometer reveal the presence of a vast tropospheric cloud on Titan at latitudes 51- to 68- north and all longitudes observed (10- to 190- west). The derived characteristics indicate that this cloud is composed of ethane and forms as a result of stratospheric subsidence and the particularly cool conditions near the moon’s north pole. Preferential condensation of ethane, perhaps as ice, at Titan’s poles during the winters may partially explain the lack of liquid ethane oceans on Titan’s surface at middle and lower latitudes.

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