HiRISE: High Resolution Imaging Science Experiment                  The University of Arizona
Home  New Images  Catalog  Anaglyphs  Stereo Pairs  Science in Motion  FAQ  HiBLOG  Themes  Software  Contact  Search


Saltating Gypsum into Dark Polar Dunes (PSP_009656_2780)

Saltating Gypsum into Dark Polar Dunes
Saltating Gypsum into Dark Polar Dunes (PSP_009656_2780)
Credit: NASA/JPL/University of Arizona

Gypsum is a common water-based mineral found in evaporative beds (ancient lakes or seas) on Earth. Gypsum rarely occurs in sand dunes on Earth as it is water-soluble (dissolves in water). However, gypsum can be trapped in basins that have no water outlets or receive very light precipitation and form beautiful dunes. The White Sands National Monument in the Tularosa Basin, New Mexico, is the largest gypsum dune field in the world. OMEGA, an instrument onboard the European Space Agency’s (ESA) Mars Express has detected gypsum deposits in the Martian north polar erg.

Where did the gypsum come from? Scientists propose that gypsum deposits formed as a result of melting or retreating ice sheets in a polar evaporate basal unit. In this image, gypsum may originate from the bright bedrock and may mix with saltating dark sand. However, the true source of the gypsum is still debated among planetary scientists.

The mafic (basaltic) dark dunes are predominately transverse with transitioning linear and barchanoid dunes with the wind coming from changing west-northwest and west-southwest directions. These dunes have several active processes occurring within them; grain avalanching is present at the crest of dunes and fading dark slope streaks are visible on the slipface.


Written by: Circe Verba

OBSERVATION TOOLBOX
Acquisition date:17 August 2008 Local Mars time: 4:19 AM
Latitude (centered):81.8 ° Longitude (East):158.7 °
Range to target site:322.4 km (201.5 miles)Original image scale range:from 32.3 cm/pixel (with 1 x 1 binning) to 64.5 cm/pixel (with 2 x 2 binning)
Map projected scale:25 cm/pixelMap projection:POLAR STEREOGRAPHIC
Emission angle:9.7 ° Phase angle:63.6 °
Solar incidence angle:71 °, with the Sun about 19 ° above the horizon Solar longitude:114.2 °, Northern Summer
For non-map projected products:
North azimuth:258 ° Sub-solar azimuth:317.0 °
F O R   M A P   P R O J E C T E D   P R O D U C T S
North azimuth:111.3°Sub solar azimuth173.2°

 

....................

SCIENCE THEME
Composition and Photometry

IMAGE PRODUCT INFORMATION
Grayscale label description
Color product label
EDR products


SUBIMAGES IN THIS OBSERVATION
[stunning subimage]
(2MB)



RESOURCES
About color products (PDF)
IAS Viewer help
HiRISE Online Image Viewer

WALLPAPER
800x600
1024x768
1152x864
1280x960
1440x1080
1600x1200
1920x1440
2048x1536
2560x1600


REFERENCE SHEET
PDF Reference Sheet


Share on Facebook


TRANSLATE

U S A G E   P O L I C Y

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: Image: NASA/JPL/University of Arizona


P O S T S C R I P T

For information about NASA and agency programs on the Web, visit: http://www.nasa.gov. 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. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona. The image data were processed using the U.S. Geological Survey’s ISIS3 software.