
This VIS image shows a region of chaos near the terminal end of Morava Valles. Located in Margaritifer Terra, Morava Valles is one of several channels that empty northward towards Chryse Planitia. Morava Valles arises from a region of chaos. Chaos terrain is also found along the course of the channel and may occur where the channel flow fluid warmed the subsurface ice creating additional release points for melted subsurface ice. Chaos terrain is typified by regions of blocky, often steep sided, mesas interspersed with deep valleys. With time and erosion the valleys widen and the mesas become smaller. It has been proposed that a catastrophic outflow of subsurface water creates the chaos and provides the surface flow creating the channel. Orbit Number: 79002 Latitude: -11.1516 Longitude: 338.097 Instrument: VIS Captured: 2019-10-06 08:08 https://photojournal.jpl.nasa.gov/catalog/PIA23541
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NASA ID
PIA23541
Date Created
November 11, 2019
Center
JPL
Media Type
image
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Medium
960px