HiRISE | Nili Patera Caldera and Dunes (ESP_017617

NASA/JPL/University of Arizona

Nili Patera Caldera and Dunes
ESP_017617_1890 Science Theme: Volcanic Processes

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Grayscale: map-projected (1315.7 MB)
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Grayscale: map-projected (644.7 MB),
non-map (711.9 MB)

IRB color: map projected (267.0 MB)
non-map (577.4 MB)

RGB color: non map-projected (559.7 MB)

ADDITIONAL IMAGE INFORMATION
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Acquisition date:	30 April 2010	Local Mars time:	3:10 PM
Latitude (centered):	9.020 degrees	Longitude (East):	67.511 degrees
Range to target site:	276.9 km (173.1 miles)	Original image scale range:	27.7 cm/pixel (with 1 x 1 binning) so objects ~83 cm across are resolved
Map projected scale:	25 cm/pixel and North is up	Map projection:	EQUIRECTANGULAR
Emission angle:	10.7 degrees	Phase angle:	57.1 degrees
Solar incidence angle:	48 degrees, with the Sun about 42 degrees above the horizon	Solar longitude:	84.3 degrees, Northern Spring
For non-map projected products:
North azimuth:	97 degrees	Sub-solar azimuth:	31.8 degrees
For map-projected products
North azimuth:	270 degrees	Sub solar azimuth:	205.5 degrees

NEARBY OBSERVATIONS

Nili Patera
Mound on Nili Patera Floor
Mound on Nili Patera Floor
Sand Dunes in Nili Patera Caldera
Nili Patera Ripples
Topography of Moving Dunes in Nili Patera

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.