Exhumed Fluvial Deposits: New Paleohydrological Tools Indicate Long-Duration Fluvial Activity on Early Mars

• Main Author: Hayden, Alistair Thompson
• Format: Others
• Language: en
• Published: 2021
• Online Access: https://thesis.library.caltech.edu/13869/2/HaydenDissertation_SUBMIT.pdf; Hayden, Alistair Thompson (2021) Exhumed Fluvial Deposits: New Paleohydrological Tools Indicate Long-Duration Fluvial Activity on Early Mars. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/68ft-xm49. https://resolver.caltech.edu/CaltechTHESIS:09072020-172907018 <https://resolver.caltech.edu/CaltechTHESIS:09072020-172907018>

<p>Fluvial sinuous ridges are common landforms on Mars that have been used for interpreting the history of ancient martian rivers. They are typically interpreted as eroded casts of an ancient river at a snapshot in time. However, some ridges might instead be channel belts that preserve river history, leading to significant differences in interpretation of paleohydrology, including flow direction, duration, and discharge. In this thesis, I used analog sites on Earth and techniques from fluvial sedimentology and fluvial geomorphology to determine that many ridges are exhumed channel belts, and to create and apply new tools for measuring bankfull discharge and duration of river flow from remote-sensing observations of these sedimentary deposits. I found evidence that rivers on ancient Mars were comparable in size to those on Earth today, and that they flowed for at least millions of years.</p> <p>I examined sinuous ridges in three terrestrial sites to better understand ridges on Mars: the Cretaceous Cedar Mountain Formation and Jurassic Morrison Formation of Eastern Utah, and the Miocene Caspe Formation of Northeast Spain. Ridges at all sites are capped with sandy units rich with dune and bar strata atop a mudstone pedestal and they cross each other at different stratigraphic levels, observations that together indicate that ridges are channel belts exhumed from floodplain sediments — the most common arrangement of fluvial stratigraphy. By compiling measurements of hundreds of terrestrial channel belts and their associated channels, I found that the best methods to reconstruct paleochannel bankfull geometry from such deposits are to use thickness of channel belts (1-4 times paleochannel depth) or radius of curvature of lateral accretion sets (half the channel width). Ridge width and planview wavelength, common proxies for paleochannel width, are significantly more uncertain due to channel amalgamation and ridge erosion by scarp retreat, which I quantified with geometry and a new erosion model. Intermittency factor converts bankfull discharge to average discharge, enabling measurement of duration of river flow. I calculated the intermittency factor for 206 fluvial deposits and USGS streamgages, and found that it ranges between 0.003-0.7 with a median of 0.10, with values depending on the ratio of catchment-averaged erosion rate to average precipitation but independent of timescale, river size, climate, or grainsize.</p> <p>Throughout the work, I applied the methods to sinuous ridges on Mars to demonstrate their applicability. I found that many ridges are likely channel belts, and that the ancient rivers they represent are likely smaller but longer than previously studies have indicated. Altogether, this contribution enables new quantitative analyses of ancient rivers on Earth and Mars, and provides evidence that ancient Martian climate was capable of supporting liquid water at many locations across the surface for at least millions of years.</p>