A Layered Mound in Juventae Chasma
NASA/JPL-Caltech/UArizona
A Layered Mound in Juventae Chasma
ESP_016712_1760  Science Theme: Sedimentary/Layering Processes
Many of the chasmata (the plural of “chasma”) in Valles Marineris contain light-toned mounds that are distinct from the darker rocks that define the walls. The light-toned mounds, like this one in Juventae Chasma, generally contain sulfates, which are salts of sulfuric acid that form when water is evaporating.

The darker material that we see is collecting near the base of the light-toned mound, and likely represents wind-blown debris.

Written by: Cathy Weitz (narration: Tre Gibbs)  (19 February 2018)
 
Acquisition date
18 February 2010

Local Mars time
15:01

Latitude (centered)
-3.438°

Longitude (East)
298.119°

Spacecraft altitude
268.0 km (166.6 miles)

Original image scale range
26.8 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
0.0°

Phase angle
50.3°

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

Solar longitude
53.4°, Northern Spring

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  35.8°
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   (767MB)

IRB color
map-projected   (338MB)

JP2 EXTRAS
Black and white
map-projected  (387MB)
non-map           (400MB)

IRB color
map projected  (117MB)
non-map           (332MB)

Merged IRB
map projected  (167MB)

Merged RGB
map-projected  (171MB)

RGB color
non map           (315MB)
BONUS
4K (TIFF)
8K (TIFF)

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-Caltech/UArizona

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.