Winter Sunrise over Phoenix
NASA/JPL/University of Arizona
Winter Sunrise over Phoenix
PSP_006561_2485  Science Theme: Glacial/Periglacial Processes


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This high latitude image shows a portion of the landing ellipse for the Mars Scout spacecraft Phoenix as seen during late winter on Mars. Phoenix will land somewhere within the ellipse on Memorial Day, 2008, but probably not within this image.

While the Phoenix lander will land in mid-spring and operate through the Martian summer, the current winter landscape looks somewhat different. The Sun is beginning to rise from the winter night and is only 10 degrees above the horizon to illuminate the surface in this image. As a result, what few rocks are present cast noticeable shadows, and every bump and undulation of the surface, now matter how small, is accentuated.

In this winter image, a blanket of carbon dioxide frost (dry ice snow) about a foot deep covers the surface. Bright patches in the image are areas where the frost is relatively clean, while in darker areas over much of the image, the frost is either dirty with atmospheric dust or the frost is somewhat translucent allowing us to see a little of the soil surface.

Summertime images of this region show that small hexagonal and polygonal patterns a few meters (yards) in size ubiquitously cover the entire region. These patterns are the result of annual thermal contraction in ice-cemented soil forming a honeycomb network of small fractures below the surface that manifest themselves as small shallow troughs at the surface. Interestingly, these patterns are not visible in this image. The shallow troughs that mark the polygons are currently filled in with carbon dioxide frost making them virtually invisible. As spring approaches the carbon dioxide frost will slowly sublimate (changes directly from ice to gas) and the polygons will once again become visible.Written by: Mike   (27 February 2008)

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Acquisition date
20 December 2007

Local Mars time:

Latitude (centered)

Longitude (East)

Range to target site
313.1 km (195.7 miles)

Original image scale range
31.3 cm/pixel (with 1 x 1 binning) so objects ~94 cm across are resolved

Map projected scale
25 cm/pixel

Map projection

Emission angle:

Phase angle:

Solar incidence angle
69°, with the Sun about 21° above the horizon

Solar longitude
5.5°, Northern Spring

North azimuth:

Sub-solar azimuth:
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

Black and white
map-projected   (1868MB)

IRB color
map-projected   (661MB)

Black and white
map-projected  (1235MB)
non-map           (753MB)

IRB color
map projected  (478MB)
non-map           (625MB)

Merged IRB
map projected  (489MB)

Merged RGB
map-projected  (485MB)

RGB color
non map           (542MB)
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products

IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images

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:
NASA/JPL/University of Arizona

For information about NASA and agency programs on the Web, visit: 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.