Crater Floor Fan
NASA/JPL/University of Arizona
Crater Floor Fan
PSP_007696_1720  Science Theme: Landscape Evolution
twitter  •  tumblr

WALLPAPER
800
1024
1152
1280
1440
1600
1920
2048
2560



This image shows a fan of sediment on the floor of a large impact crater on Mars. The fan sits at the mouth of a small valley just to the south of the image.

The valley was likely carved by groundwater “sapping” (eroding the channel upstream by undermining the slope), and deposited this fan of material when it reached the broad crater floor. This might have formed a temporary lake within the crater, depending on the rates of transport and loss of water.

Several coarse stair-steps in the fan may correspond to layers, and form arcs around the mouth of the valley. There is little indication of smaller-scale layers such as those observed in some other fan deposits on Mars, likely indicating that this fan was deposited under different conditions or the layers are not well exposed.

The current surface has many light-toned patches, circular or irregular in shape. In some cases these appear to be shallow pits, but many appear level with their surroundings. The most likely explanation for these is that they are old impact craters, mostly eroded and filled with dust. Marks like this might also be boulders in a debris-flow deposit that later turned to rock and eroded—a similar effect is observed in some megabreccia elsewhere on Mars. However, the large size of some of the patches (as much as 25 meters) would require very large boulders, making this unlikely.

Written by: Colin Dundas  (9 April 2008)

This is a stereo pair with ESP_042666_1720.
 
Acquisition date
18 March 2008

Local Mars time
14:59

Latitude (centered)
-7.951°

Longitude (East)
213.415°

Spacecraft altitude
266.2 km (165.4 miles)

Original image scale range
26.6 cm/pixel (with 1 x 1 binning) so objects ~80 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
1.6°

Phase angle
50.2°

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

Solar longitude
46.5°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  36.1°
JPEG
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

JP2
Black and white
map-projected   (412MB)

IRB color
map-projected   (181MB)

JP2 EXTRAS
Black and white
map-projected  (179MB)
non-map           (234MB)

IRB color
map projected  (51MB)
non-map           (180MB)

Merged IRB
map projected  (110MB)

Merged RGB
map-projected  (107MB)

RGB color
non map           (178MB)
ANAGLYPHS
Map-projected, reduced-resolution
Full resolution JP2 download
Anaglyph details page

DIGITAL TERRAIN MODEL (DTM)
DTM details page

ADDITIONAL INFORMATION
B&W label
Color label
Merged IRB label
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.