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JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 98, NO. E6, PAGES 11,061–11,078, 1993

Coastal Geomorphology of the Martian Northern Plains

Timothy J. Parker

Department of Geological Sciences, University of Southern California, University Park, Los Angeles

Donn S. Gorsline

Department of Geological Sciences, University of Southern California, University Park, Los Angeles

R. Stephen Saunders

Jet Propulsion Laboratory, California Institute of Technology, Pasadena

David C. Pieri

Jet Propulsion Laboratory, California Institute of Technology, Pasadena

Dale M. Schneeberger

The Mark Group, Santa Ana, California

Abstract

The northern lowland plains comprise approximately one third Mars' surface area. Most outflow channels and many valley networks debouch into the lowlands, yet there is little or no morphologic evidence to suggest that channel cutting continued far into the plains, despite a continued basinward regional topographic gradient. The immediate fate of the water discharged from these channels was dependent on the prevailing paleoclimate at the time of its emplacement. Though current models of the martian paleoclimate suggest that mean annual temperatures were likely below freezing throughout most of martian history, geomorphic evidence suggests that coastal erosion on a scale comparable to that of well-known terrestrial paleolakes occurred. These landforms can be traced to nearly complete closure of the northern plains and appear to require at least two, and perhaps several, highstands of a sea or ocean with temperatures above freezing at least for geologically brief periods of time. The latest highstand may have been as recent as Early Amazonian time. The elevations and areal extent of these landforms provide independent estimates of the martian water budget that can be compared to prevailing models of martian volatile evolution. Estimated volumes of water and sediment discharged by the major channel systems peripheral to the northern plains can be compared to the volume of the basin based on the available topography. Values for the circum-Chryse outflow channels alone are sufficient to have produced large bodies of standing water within the basin. These estimates may be comparable to the basin volume contained within the younger, least extensive highstand identified. The earlier, more extensive highstand delineates a basin with a much larger implied volume that may require the presence of a semi-permanent, possibly ice-covered ocean in the northern plains prior to major channeling events. The northern plains today probably consist of water-lain sediments interbedded to considerable depths with flood lavas from the major volcanic centers, with sediment comprising most of the present surface.

Received 3 February 1992; accepted 3 March 1993.

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Citation: Parker, T. J., D. S. Gorsline, R. S. Saunders, D. C. Pieri, and D. M. Schneeberger (1993), Coastal Geomorphology of the Martian Northern Plains, J. Geophys. Res., 98(E6), 11,061–11,078.

Copyright 1993 by the American Geophysical Union.