79 The Surface of Mars: Mineralogy, Geomorphology, and Habitability (Posters)
Sunday, 25 September 2016
9:00 AM - 5:30 PM
Exhibit Hall E/F
NUMERICAL SEDIMENTARY MODELING OF MARTIAN STEPPED FAN-DELTAS
Paper number: 79-4
Program: Technical Sessions
Time: 9:00 AM – 5:30 PM
Authors
-
Rebecca WilliamsWaunakee, WI
-
Brian M. HynekUniversity of Colorado, Boulder, CO
Abstract
Our main aim is to test the hypotheses put forth for the origin of these sedimentary bodies. Specifically, the (forward) simulations test several hydrologic scenarios, sediment discharges, grain size, basin bathymetry, timing of emplacement, water level variations, and morphodynamic evolution to characterize the hydrologic and sedimentary settings that match the observational evidence as reconstructed from available topography.
Results from simulations at constant water and sediment discharges while changing water level suggest that the formation of steps occur only when water level increases through time. We tested several water level scenarios from monotonic rise to complex water level variations including the occurrence of several (and of different duration) highstands followed both by continuing level rise and/or intervening temporary falls within the overall level rise. The morphodynamics of the resultant deposits show that rather regularly spaced steps are formed under monotonic level rise (in agreement with results from laboratory tank simulations), while longitudinal intermediate terraces are formed during the highstands. More interestingly, later steps do not bury previously formed steps even while maintaining constant river water and sediment discharges. Therefore, previously hypothesized retrogradational depositional conditions (i.e. water level rise with significant decrease of sediment flux) are not necessarily required to form stepped fans.
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-284699
© Copyright 2016 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.