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


Mars Exploration Rover Landing Site at Gusev Crater (PSP_001513_1655)

Mars Exploration Rover Landing Site at Gusev Crater
Mars Exploration Rover Landing Site at Gusev Crater (PSP_001513_1655)
Credit: NASA/JPL/University of Arizona

This HiRISE image shows the landing site of the Mars Exploration Rover Spirit. The impact crater in the upper left-hand portion of the image is "Bonneville Crater," which was investigated by Spirit shortly after landing. In the lower right-hand portion of the image is "Husband Hill," a large hill that Spirit climbed and where it spent much of its now nearly three-year mission. (View the full subimage; 1663 x 1621, 8 MB)

The bright irregularly-shaped feature in area "A" of the image is Spirit's parachute, now lying on the Martian surface. Near the parachute is the cone-shaped "backshell" that helped protect Spirit's lander during its seven-month journey to Mars. The backshell appears relatively undamaged by its impact with the martian surface. Wrinkles and folds in the parachute fabric are clearly visible.

Area "B" of the image shows Spirit's lander. The crater in the upper left-hand portion of the image, just to the northwest of the lander, is the one that the Mars Exploration Rover team named "Sleepy Hollow."

Area "C" shows the damaged remnant of the heat shield that protected the vehicle during the high-speed entry through the Martian atmosphere. The heat shield impacted the surface after being separated from the vehicle during the final stages of the descent.

Area "D" of the image shows the current location of Spirit. Toward the top of the image is "Home Plate," a plateau of layered rocks that Spirit explored during the early part of its third year on Mars. Spirit itself is clearly seen just to the southeast of Home Plate. Also visible are the tracks made by the rover before it arrived at its current location.

Written by: Steve Squyres

OBSERVATION TOOLBOX
Acquisition date:22 November 2006 Local Mars time: 3:29 PM
Latitude (centered):-14.6 ° Longitude (East):175.5 °
Range to target site:270.7 km (169.2 miles)Original image scale range:27.1 cm/pixel
(with 1 x 1 binning) so objects ~81 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:15.8 ° Phase angle:73.6 °
Solar incidence angle:60 °, with the Sun about 30 ° above the horizon Solar longitude:139.1 °, Northern Summer
For non-map projected products:
North azimuth:96 ° Sub-solar azimuth:34.7 °
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 azimuth208.2°
A N A G L Y P H   P R O D U C T S
Left observation:PSP_001777_1650Convergence angle19.8°

 

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

SCIENCE THEME
Future Exploration/Landing Sites

STEREO PAIR
PSP_001777_1650

IMAGE PRODUCT INFORMATION
Grayscale label description
Color product label
EDR products


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



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.