HR: 1340h
AN: P33A-1015 [Abstracts]
TI: Late Amazonian Glaciation at the Dichotomy Boundary on Mars: New Evidence from MRO for Glacial Thickness Maxima and Multiple Glacial Phases
AU: * Dickson, J L
EM: jdickson@brown.edu
AF: Brown University, Dept. Geo. Sci.
324 Brook St., Providence, RI 02906, United States
AU: Head, J W
EM: james_head@brown.edu
AF: Brown University, Dept. Geo. Sci.
324 Brook St., Providence, RI 02906, United States
AU: Marchant, D R
EM: marchant@bu.edu
AF: Boston University, Dept. Earth Sci., Boston, MA 02215, United States
AB:
Lineated valley fill (LVF) in fretted valleys at the dichotomy boundary has been interpreted as glacial in origin.
Unknown are 1) the original thickness of the glacier ice, 2) the amount of ice-surface lowering, through
sublimation, retreat and ice loss, to its presently observed level, and 3) whether there were multiple periods of
glaciation. We address these questions through analysis of an integrated LVF glacial landsystem along the
dichotomy boundary at the contact of Protonilus Mensae and Coloe Fossae (41°N, 54.5°E).
Analysis of MRO CTX and HiRISE data confirm the presence of a 5-km wide loop-like lobe emanating from LVF
that terminates in an elevated box canyon, and the remnant flow patterns do not correlate with present-day
topography, indicating that a substantially increased volume of ice was necessary to alter the flow regime and
deposit the observed features. Additionally, the upper limit of glacial deposits at this site is topographically
consistent with other regional glacial deposits in Coloe Fossae and Protonilus Mensae. The elevation difference
between the upper limit of glacial deposits and the current surface of the LVF at the study site is ~920 meters. We
interpret this difference to reflect the minimum amount of ice-surface lowering of the valley glacier system during
retreat. Consistent with a general lowering of the ice surface are multiple moraines and/or trimlines, and
changes in LVF flow patterns, including local flow reversals, as the ice retreated and decreased in thickness. The
clear superposition of several lobes out onto the current surface of the LVF indicates that a less extensive phase
of glaciation followed the lowering of the valley glacial landsystem. These data suggest that the major Late
Amazonian glaciation that produced LVF in this region involved significantly larger amounts of glacier ice than
previously thought, and that subsequent, less extensive local tributary glaciation followed.
DE: 5415 Erosion and weathering
DE: 5416 Glaciation
DE: 5422 Ices
DE: 5470 Surface materials and properties
DE: 6225 Mars
SC: Planetary Sciences [P]
MN: 2007 Fall Meeting