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- W1641602012 abstract "Introduction: The Cerberus Plains (CP) (Fig. 1) are located on the southeastern margin of the Elysium Rise and extend for over 3000-km from east to west and ~600-km from north-to-south. The plains are bounded to the northwest by the Athabasca Valles outflow channel and ridged Elysium lavas, to the north by cratered, knobby terrains, and to the south by the Medusae Fossae Formation and ridged plains. The Marte Valles outflow channel joins the eastern Cerberus Plains with the lower-elevation western Amazonis Planitia. A system of WNW-ESE trending fissures of the Cerberus Fossae cut across the Cerberus Plains, the northern knobby terrains, and portions of the ridged Elysium lavas. Since the Cerberus Plains exhibit smooth surfaces at Viking image resolutions and few impact craters, [1] and [2] interpreted this region as being the youngest on Mars and defined this region as the referent for Upper Amazonian units. The presence of teardrop islands in Marte Valles and the smooth character of the plains led them to interpret the surfaces in this region as fluvial deposits from floods emanating from Cerberus Fossae. On the basis of USGS Viking-based topographic maps which indicate that the plains lay in a closed basin, Scott and Chapman [3] interpreted surfaces in the region as pluvial sediments deposited on top of volcanic surfaces by a paleolake which subsequently debouched through Marte Valles and westward in the southwestern plains. However, Plescia [4, 5] noted the presence of sparsely cratered, lobate, convex-ridged surfaces with morphologies consistent with unmodified lava flows and interpreted the surfaces to be lava flows filling pre-existing fluvial channel systems. MOC images confirmed that these plains are covered by lava flows, and that they are very similar to flows in Iceland [6]. Sakimoto [7] identified several shields, edifices, and lava flows and argued for a period of plains-style volcanism in this region. We examine the spatial and stratigraphic relationships between Cerberus Plains volcanic units and surrounding units and derive constraints for volumes of volcanic materials extruded and the duration of volcanic activity within the Cerberus Plains." @default.
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- W1641602012 date "2003-07-01" @default.
- W1641602012 modified "2023-09-23" @default.
- W1641602012 title "Cerberus Plains Volcanism: Constraints on Temporal Emplacement of the Youngest Flood Lavas on Mars" @default.
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