Title of article
A geological characterization of Ligeia Mare in the northern polar region of Titan
Author/Authors
Wasiak، نويسنده , , F.C. and Androes، نويسنده , , Ian D. and Blackburn، نويسنده , , D.G. and Tullis، نويسنده , , J.A. and Dixon، نويسنده , , J. and Chevrier، نويسنده , , V.F.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2013
Pages
7
From page
141
To page
147
Abstract
Ligeia Mare, the second largest sea on Titan, resides in an endorheic basin dominated by seas in the northeastern polar region. Ligeiaʹs shoreline morphology resembles terrestrial man-made reservoirs where water is dammed and valleys are flooded. Here we describe the mare and surrounding geologically diverse terrain including rugged highlands and lowlands, incised valleys, and smooth plains. Observations include active processes evidenced by drainage flow directions, areal extent of rivers and river valleys, sediment volume estimates, and varied drainage patterns. Headward erosion has carved valley and ridge systems in the flanks of the highlands, while the more distal highland plateau is mostly uncut by rivers or extensive erosion and contains smaller lakes, lakebeds, and mottled terrain.
Keywords
Titan , Saturn satellites , Satellites Surfaces , Titan surface
Journal title
PLANETARY AND SPACE SCIENCE
Serial Year
2013
Journal title
PLANETARY AND SPACE SCIENCE
Record number
2315396
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