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Barlow et al. 2001
Barlow, N.G., Koroshetz, J. and Dohm, J.M. (2001). Variations in the onset diameter for Martian layered ejecta morphologies and their implications for subsurface volatile reservoirs. Geophysical Research Letters 28: doi: 10.1029/2000GL012804. issn: 0094-8276.

We investigated regional variations in the onset diameter of craters displaying a single layer ejecta morphology within ¿30¿ latitude using Viking imagery. Our results generally agree with those of previous studies which show onset diameters of 5 to 6 km in the equatorial region, but we have identified localized regions with unusually small onset diameters. The largest region is located in Solis and Thaumasia Planae. The 3--5 km onset diameter range in this area indicates a near-surface ice-rich reservoir (depth ~110 m). This unusual concentration of near-surface ice may have resulted from magmatic-driven uplifts associated with the Tharsis rise, which modified parts of a regional aquifer/drainage basin system and resulted in the transfer and concentration of subsurface volatiles in this region. ¿ 2001 American Geophysical Union

BACKGROUND DATA FILES

Abstract

Keywords
Planetology, Solid Surface Planets, Impact phenomena (includes cratering), Planetology, Solid Surface Planets, Remote sensing, Planetology, Solid Surface Planets, Tectonics, Planetology, Solar System Objects, Mars
Journal
Geophysical Research Letters
http://www.agu.org/journals/gl/
Publisher
American Geophysical Union
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