Domes on the Northern Plains
NASA/JPL/University of Arizona

Domes on the Northern Plains
PSP_008561_2205  Science Theme: Volcanic Processes
EspañolPortuguês



WALLPAPER

800  1024  
1152  1280  
1440  1600  
1920  2048  
2560  
This image shows a scene from the northern plains of Mars, near the edge of the lowland known as Acidalia Planitia.

Several features common to the area are visible. Most striking are the circular, pancake-shaped domes with pits or craters at the summit. These were once thought to be volcanic features, but recent research suggests that these are instead mud volcanoes. On Earth, mud volcanoes form when wet sediment is overpressured and squeezed out onto the surface. In many cases, these domes have finely fractured surfaces, which could be due to either desiccation (loss of water) or temperature changes in the ice.

The domes at this side are similar in color to the surrounding material, appearing as blue in HiRISE false color. However, this may be due to a thin coating of dust, as an impact crater in the color swath appears to expose material of a different color.

The image includes some large troughs, up to hundreds of meters wide. These are also widespread in the area, forming crudely polygonal patterns on a multi-kilometer scale. These are distinct from the small polygons like those at the Phoenix landing site, which form by thermal cycling in ground ice; the origin of these giant polygons is still a subject of ongoing research.


Written by: Colin Dundas   (10 July 2008)



 Image Products: All image links are drag & drop for HiView, or click to download
JPEG
Grayscale: map projected  non-map
IRB color: map projected  non-map
Merged IRB: map projected
Merged RGB: map projected
RGB color: non-map projected

JP2 DOWNLOAD
Grayscale: map-projected (809.5 MB)
IRB color: map-projected (334.3 MB)

JP2 EXTRAS
Grayscale: map-projected  (377.9 MB),
non-map  (382.6 MB)
IRB color: map projected  (128.6 MB)
non-map  (280.9 MB)
Merged IRB: map projected  (216.8 MB)
Merged RGB: map-projected  (210.2 MB)
RGB color: non map-projected  (270.1 MB)

ADDITIONAL IMAGE INFORMATION
Grayscale label   Color label
Merged IRB label   Merged RGB label
EDR products

About color products (PDF)
HiView main page

 Observation Toolbox
Acquisition date:24 May 2008 Local Mars time: 3:07 PM
Latitude (centered):40.254° Longitude (East):346.684°
Range to target site:300.9 km (188.1 miles)Original image scale range:30.1 cm/pixel (with 1 x 1 binning) so objects ~90 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:Equirectangular
Emission angle:0.7° Phase angle:41.4°
Solar incidence angle:42°, with the Sun about 48° above the horizon Solar longitude:76.1°, Northern Spring
For non-map projected products:
North azimuth:97° Sub-solar azimuth:357.5°
For map-projected products
North azimuth:270°Sub solar azimuth:172.5°

Context map

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: Image: NASA/JPL/University of Arizona
Postscript
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.