Very Fresh Impact Crater Superposing a Wrinkle Ridge in Hesperia Planum
NASA/JPL/University of Arizona
Very Fresh Impact Crater Superposing a Wrinkle Ridge in Hesperia Planum
ESP_025237_1600  Science Theme: Impact Processes
twitter  •  tumblr

HICLIP
720p (MP4)
Audio (MP3)

WALLPAPER
800
1024
1152
1280
1440
1600
1920
2048
2560

HIFLYER
PDF (11 x 17)

HISLIDES
PowerPoint
Keynote
PDF

The ridge captured in this HiRISE image is called a wrinkle ridge. This wrinkle ridge is located in Hesperia Planum, a region of over two million square kilometers (over 770,000 square miles) in the southern highlands of Mars. It is located northwest of the Hellas basin and adjacent to Tyrrhena Patera and contains abundant orthogonal and intersecting wrinkle ridges.

Wrinkle ridges are long, winding topographic highs and are often characterized by a broad arch with superposed narrow asymmetric ridges. These features have also been identified on the Moon, Mercury, and Venus. Their origin is attributed to horizontal compression or shortening of the crust due to faulting and folding. They commonly have asymmetrical cross sectional profiles and an offset in elevation on either side of the ridge.

Superposing or located on top of the wrinkle ridge, is a very fresh impact crater. We can tell that this crater is fresh because of its relatively sharp or crisp rim and unmodified shape. If you look closely, you can see faint rays of relatively fine material, boulders, and smaller secondary craters radiating from the crater and superposing the wrinkle ridge and older surrounding craters.

Written by: Maria Banks  (20 December 2011)
 
Acquisition date
14 December 2011

Local Mars time
14:50

Latitude (centered)
-19.735°

Longitude (East)
114.877°

Spacecraft altitude
256.2 km (159.3 miles)

Original image scale range
25.7 cm/pixel (with 1 x 1 binning) so objects ~77 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
4.0°

Phase angle
58.7°

Solar incidence angle
56°, with the Sun about 34° above the horizon

Solar longitude
43.4°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  43.8°
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   (709MB)

IRB color
map-projected   (428MB)

JP2 EXTRAS
Black and white
map-projected  (335MB)
non-map           (420MB)

IRB color
map projected  (135MB)
non-map           (381MB)

Merged IRB
map projected  (171MB)

Merged RGB
map-projected  (174MB)

RGB color
non map           (366MB)
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.