Layering in Crommlin Crater
NASA/JPL/UArizona
Layering in Crommlin Crater
PSP_004421_1850  Science Theme: Sedimentary/Layering Processes

WALLPAPER
800
1024
1152



Crommlin Crater is a little over 100 kilometers (62 miles) across and contains a mound of layered rock deposits. Layering in geologic materials is interesting because it represents a record of deposition over time. By studying such layered sequences, scientists attempt to tell what the local climate and environment were like in the past.

This image runs along the eastern side of the layered mound within the crater. Upslope is to the west, to the left of the image, and downslope is to the east, to the right of the image. Along the slope of the mound, the layered exposures are visible. The subimage included here (approximately 1.7 kilometers or 1.1 miles across; 1750 x 1439, 2 MB) shows an area with a sequence of layers that is very regular, like looking at the pages of a book edge on, or at the layers in a slice of cake from the side. Presumably these layers were once more continuous, perhaps reaching all the way to the crater wall (off-image to the right), and were then cut into by erosion so that we now see the layer edges.

Further upslope, to the left, are knobs, mesas, terraces, and other indications that layers also exist here, but were eroded in a more irregular manner. Unfortunately, the finest layering and details are not visible because the Martian atmosphere above Crommlin Crater at this time was dusty, making a clear image difficult for the HiRISE camera to obtain. Within the regular sequence of layering, however, a pattern of several fine layers separated by single thicker, or darker, layers are apparent. This repeating pattern may indicate that the conditions in which the sediments were originally deposited repeated over time.

Crommlin Crater is especially interesting because it is located very close to Meridiani Planum, which is where the MER Opportunity Rover has been exploring layered rocks up close. Comparison of nearby layers studied from the rover on the ground and from the spacecraft above will provide greater insight into the age and origin of these deposits.

Written by: Patrick Russell  (1 August 2007)
 
Acquisition date
06 July 2007

Local Mars time
14:53

Latitude (centered)
4.984°

Longitude (East)
350.496°

Spacecraft altitude
274.4 km (170.5 miles)

Original image scale range
28.9 cm/pixel (with 1 x 1 binning) so objects ~87 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
18.5°

Phase angle
36.8°

Solar incidence angle
52°, with the Sun about 38° above the horizon

Solar longitude
271.6°, Northern Winter

For non-map projected images
North azimuth:  96°
Sub-solar azimuth:  326.0°
JPEG
Black and white
map projected  non-map

JP2
Black and white
map-projected   (3192MB)


JP2 EXTRAS
Black and white
map-projected  (1098MB)
non-map           (1254MB)


ADDITIONAL INFORMATION
B&W label
EDR products
HiView

NB
Black & white is 5 km across
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.