Ng. Barlow et al., Variations in the onset diameter for Martian layered ejecta morphologies and their implications for subsurface volatile reservoirs, GEOPHYS R L, 28(16), 2001, pp. 3095-3098
We investigated regional variations in the onset diameter of craters displa
ying a single layer ejecta morphology within +/- 30 degrees 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 ha
ve identified localized regions with unusually small onset diameters. The l
argest region is located in Solis and Thaumasia Planae. The 3-5 km onset di
ameter range in this area indicates a near-surface ice-rich reservoir (dept
h similar to 110 m). This unusual concentration of near-surface ice may hav
e resulted from magmatic-driven uplifts associated with the Tharsis rise, w
hich modified parts of a regional aquifer/drainage basin system and resulte
d in the transfer and concentration of subsurface volatiles in this region.