Lots of Layers in Terby Crater
NASA/JPL/University of Arizona
Lots of Layers in Terby Crater
ESP_021942_1520  Science Theme: Future Exploration/Landing Sites
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Erosion has revealed many sedimentary rock layers in this image in Terby Crater.

Terby, a 170 kilometer (approximately 100 mile) crater along the northern edge of Hellas Planitia, is interesting to scientists because of its apparent modification by liquid water. Sedimentary rocks like those revealed in the plateaus of this image can be emplaced by both wind and water. Erosional features in Terby give us an enticing view into the layers and may contain clues as to whether water once flowed across the surface.

The enhanced-color subimage shows several gully-like features that cut across multiple sedimentary layers. (Up is to the left in this image.) Eroded material has been deposited in fans at the base of the plateau (lower right). The gully incisions reveal a fresher view (slightly bluish or purplish) of the layers making up the plateau than the uncut layers (brownish). There is a change in color (to a lighter, yellower tone) of the layers at the very top of the gully alcove (left) and the surface there becomes smoother and less steep. These differences in layer appearance likely indicate a difference in composition or resistance to erosion between the lighter and darker, and steeper and shallower, layers.

Terby Crater was at one point a potential landing site for the Mars Science Laboratory rover. It is no longer under consideration for that mission, but it is still on the candidate list for potential future missions.

Written by: Nicole Baugh  (27 April 2011)

This is a stereo pair with ESP_021797_1520.
 
Acquisition date
02 April 2011

Local Mars time
14:59

Latitude (centered)
-27.693°

Longitude (East)
74.736°

Spacecraft altitude
259.4 km (161.2 miles)

Original image scale range
26.3 cm/pixel (with 1 x 1 binning) so objects ~79 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
10.9°

Phase angle
29.1°

Solar incidence angle
40°, with the Sun about 50° above the horizon

Solar longitude
266.1°, Northern Autumn

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  358.7°
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non-map           (490MB)

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non-map           (358MB)

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RGB color
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ANAGLYPHS
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Full resolution JP2 download
Anaglyph details page

DIGITAL TERRAIN MODEL (DTM)
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ADDITIONAL INFORMATION
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Merged RGB label
EDR products
HiView

NB
IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images

USAGE POLICY
All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible:
NASA/JPL/University of Arizona

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.