Slope Streaks on the Rim of Henry Crater
Slope Streaks on the Rim of Henry Crater
PSP_006991_1905  Science Theme: Composition and Photometry
Named after a 19th century French astronomer, Henry Crater is a 165 kilometer (103 mile) diameter impact crater, located in Arabia Terra on a portion of the Martian highlands extending into the northern hemisphere. The rim of the crater is in the western side of the image and the slope streaks pictured here extend eastward down the slopes of the crater wall into the crater.

The subimage is a close-up view of dark and light-toned slope streaks. The slope streaks generally start at a point source and widen downslope as a single streak or branch into multiple streaks. Some of the slope streaks show evidence that downslope movement is being diverted around obstacles, such as large boulders, and a few appear to originate at boulders or clumps of rocky material. The darkest slope streaks are youngest and cross cut and lie on top of the older and lighter-toned streaks. The lighter-toned streaks are believed to be dark streaks that are lightening with time as new dust is deposited on their surface.

Slope streak formation is among the few known processes currently active on Mars making slope streaks some of the youngest features on the Martian surface. Many hypotheses have been proposed for the formation of slope streaks including dry avalanching, geochemical weathering, liquid stains or flows, and moisture wickering. Recent observations from HiRISE images have revealed that the dark interior of slope streaks is lower in elevation than the surroundings indicating that material must have been removed in the formation of the streak.

Written by: Maria Banks  (3 March 2008)
Acquisition date
23 January 2008

Local Mars time

Latitude (centered)

Longitude (East)

Spacecraft altitude
275.9 km (171.5 miles)

Original image scale range
27.9 cm/pixel (with 1 x 1 binning) so objects ~84 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection

Emission angle

Phase angle

Solar incidence angle
39°, with the Sun about 51° above the horizon

Solar longitude
21.5°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  6.6°
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

Black and white
map-projected   (1533MB)

IRB color
map-projected   (655MB)

Black and white
map-projected  (850MB)
non-map           (759MB)

IRB color
map projected  (242MB)
non-map           (609MB)

Merged IRB
map projected  (349MB)

Merged RGB
map-projected  (354MB)

RGB color
non map           (560MB)
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products

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

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

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.