Fan-Shaped Deposits in Bigbee Crater
NASA/JPL-Caltech/UArizona
Fan-Shaped Deposits in Bigbee Crater
ESP_039893_1550  Science Theme: Fluvial Processes
Bigbee is a 21 kilometer-diameter impact crater located on the northern rim of Holden Crater in southern Margaritifer Terra, a region on Mars that is well known for its long record of water-rich activity.

The rim of Bigbee has been heavily modified from its original form, presumably by water and wind. Material eroded and removed from Bigbee’s rim was transported and deposited to the crater interior. Some of the darker-toned material near Bigbee’s northern rim has been incorporated into fan-shaped deposits with distinct margins at the outer part. The fan surfaces appear to lack obvious layering and channels.

The modification of Bigbee and other smaller craters on Holden’s rim may have been contemporaneous with a proposed period of relatively late, water-driven activity that formed fans in Holden and other craters in Margaritifer Terra (see Grant and Wilson, 2012).

Note: The cutout is 3.5-kilometer across and shows dark fan-like deposits on left side of image at the base of a light-toned scarp.

Written by: Sharon Wilson (narration: Tre Gibbs)  (11 February 2015)

This is a stereo pair with ESP_040394_1550.
 
Acquisition date
29 January 2015

Local Mars time
14:45

Latitude (centered)
-24.779°

Longitude (East)
325.370°

Spacecraft altitude
258.6 km (160.8 miles)

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POSTSCRIPT
NASA’s Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate, Washington. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.