Gullies in Utopia Planitia
NASA/JPL-Caltech/UArizona
Gullies in Utopia Planitia
PSP_006724_2165  Science Theme: Glacial/Periglacial Processes
Seen here are gullies in a northern hemisphere crater. The crater is well-preserved as indicated by its sharp rim and steep walls. Gullies are rarer in the northern hemisphere, possibly because there are fewer slopes for them to form on compared to the heavily cratered southern highlands.

This image captures a range of gully morphologies. The gullies on the north wall (south facing) are more abundant and evenly-spaced than those on the east and south walls, and they extend up to the crater rim on the northern side. These differences might occur because of differences in sunlight exposure and temperature variations.

The crater floor has a linear texture suggestive of flow. Ice-rich material might have moved off the crater walls, driven by gravity, and flowed towards the crater center.



Written by: Kelly Kolb  (16 April 2008)
 
Acquisition date
02 January 2008

Local Mars time
14:21

Latitude (centered)
36.385°

Longitude (East)
107.777°

Spacecraft altitude
297.4 km (184.8 miles)

Original image scale range
29.8 cm/pixel (with 1 x 1 binning) so objects ~90 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
3.5°

Phase angle
48.4°

Solar incidence angle
45°, with the Sun about 45° above the horizon

Solar longitude
11.6°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  329.8°
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RGB: red-green-blue
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Black & white is 5 km across; enhanced color about 1 km
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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.