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


MER Spirit Rover at Martian Mid-Winter (PSP_008963_1650)

MER Spirit Rover at Martian Mid-Winter
MER Spirit Rover at Martian Mid-Winter (PSP_008963_1650)
Credit: NASA/JPL/University of Arizona

This image shows the MER Spirit rover at its location on the north edge of Home Plate in the Columbia Hills, and was taken on the southern hemisphere winter solstice at about 2 p.m. local time on Spirit’s 1,591st sol on Mars.

Home Plate is the elevated round and light toned mesa on the right side of the image. Spirit is visible at the large dark “bump” on the north-northeast edge of Home Plate. The image was acquired at mid-winter because that is the time of the clearest and least dusty atmosphere.

The optical clarity of the sky is measured as a value called “tau” and can range from 0.15 in winter to 6.0 (or higher) like that seen last summer. Spirit measured a “tau” of 0.19 the day before this image was acquired; the clarity of the sky was about as good as it gets. Another factor in making this image special is the low-angle lighting of mid-winter, which results in slightly longer shadows. Long shadows aid in detecting small features like rocks, outcrops, and low ridges and scarps. The bowl-like upturned edges of Home Plate are emphasized by this low-angle lighting.

Just east of Home Plate is a ridge, informally named Mitcheltree Ridge. During its field season last Martian summer, Spirit discovered unusual high silica deposits between the ridge and Home Plate. These deposits are comparable in many ways to high-silica spring deposits of Earth. To the south of Home Plate—a roughly circular area nearly the same size—is another mesa informally named Crossfield. Just to the southwest of that are two unusual features, a butte and a crater (informally named Von Braun and Goddard, respectively).

Another purpose of this image is to aid in selecting a traverse in the coming field season. Spirit will leave Home Plate, drive west and south around the north edge, south along the bottom of the valley between Home Plate and the long ridge to the west informally named Tsiolkovski, and then southward towards the butte and crater farther south.

Written by: L. S. Crumpler

OBSERVATION TOOLBOX
Acquisition date:24 June 2008 Local Mars time: 3:23 PM
Latitude (centered):-14.7 ° Longitude (East):175.5 °
Range to target site:262.8 km (164.3 miles)Original image scale range:52.6 cm/pixel
(with 2 x 2 binning) so objects ~158 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:3.4 ° Phase angle:66.1 °
Solar incidence angle:64 °, with the Sun about 26 ° above the horizon Solar longitude:89.9 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:44.4 °
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:270°Sub solar azimuth217.9°

 

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

SCIENCE THEME
Future Exploration/Landing Sites

IMAGE PRODUCT INFORMATION
Grayscale label description
Color product label
EDR products


SUBIMAGES IN THIS OBSERVATION
Spirit
(11MB)



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.