J. Bow J. Schwartz R. H. Brown J.M. Soderblom A. G. Hayes G. Vixie Stéphane Le Mouélic S. Rodriguez Christophe Sotin R. Jaumann K. Stephan L.A. Soderblom Roger N. Clark B. J. Buratti K. H. Baines P. D. Nicholson J. W. Barnes 2011 <p><span>We report the discovery of organic sedimentary deposits at the bottom of dry lakebeds near Titan’s north pole in observations from the&nbsp;</span><i>Cassini</i><span>&nbsp;Visual and Infrared Mapping&nbsp;<a title="Learn more about Spectrometer from ScienceDirect's AI-generated Topic Pages" href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/spectrometer" data-mce-href="https://www.sciencedirect.com/topics/earth-and-planetary-sciences/spectrometer">Spectrometer</a>&nbsp;(VIMS). We show evidence that the deposits are evaporitic, making Titan just the third known planetary body with evaporitic processes after Earth and Mars, and is the first that uses a solvent other than water.</span></p> application/pdf 10.1016/j.icarus.2011.08.022 en Elsevier Organic sedimentary deposits in Titan's dry lakebeds: Probable evaporite article