Phoenix Lander in Winter
Phoenix Lander in Winter
ESP_014393_2485  Science Theme: Glacial/Periglacial Processes
As the Phoenix lander started to get a glimpse of the Sun towards the end of the northern hemisphere winter, HiRISE decided to try imaging the site despite the low light levels. The power of the HiRISE camera helped us see it even under these poor conditions.

By matching up the images with the known location of the lander, we can identify the hardware, even disguised by frost and poor lighting. To make things worse, some of these images are also low-quality due to atmospheric haze, which often obscures the surface at this location and season.

In this image, the albedo (brightness) doesn't necessarily indicate the amount of frost. Keep in mind that each of these images is stretched differently for optimal contrast, so "bright" and "dark" can't be compared directly between images without doing complex calibrations. In fact, if you stretched all of them exactly the same, the darker areas in the frost-covered ESP images are still brighter than typical soil, like that surrounding the lander in the frost-free PSP_008855_2485 image.

In addition, other factors affect the relative brightness, such as the size of individual grains of carbon dioxide ice, the amount of dust mixed in with the ice, the amount of sunlight hitting the surface, and different lighting angles and slopes. The winds are also changing direction and strength, moving loose frost and dust around over time. Studying these changes will help us understand the nature of the seasonal frost and winter weather patterns in this area of Mars.

The amount of carbon dioxide frost is increasing as late winter transitions to early spring, so the layer of frost is getting thicker in each image, slowly encasing the lander. The maximum thickness was expected to be on the order of tens of centimeters, which would have reached its peak in September 2009.

Unfortunately, the Mars Reconnaissance Orbiter was in the midst of an extended safe mode following a spacecraft anomaly, so HiRISE was unable to capture an image at that time.

The Planetary Society has put together an animation comparing the hardware at different times.

Information about the images:

PSP_008855_2485 - 16 June 2008 - Ls 86 (northern hemisphere summer) - incidence angle 51.2 degrees - during active mission (frost-free, for comparison)

ESP_014103_2485 - 30 July 2009 - Ls 313 (northern hemisphere winter) - incidence angle 89.2 degrees

Written by: Ingrid Daubar Spitale & Mike Mellon  (2 November 2009)

Acquisition date
22 August 2009

Local Mars time

Latitude (centered)

Longitude (East)

Spacecraft altitude
312.0 km (193.9 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
84°, with the Sun about 6° above the horizon

Solar longitude
325.4°, Northern Winter

For non-map projected images
North azimuth:  100°
Sub-solar azimuth:  304.4°
Black and white
map projected  non-map

IRB color
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Merged IRB
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Merged RGB
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RGB color
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IRB color
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Black and white
map-projected  (169MB)
non-map           (125MB)

IRB color
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non-map           (126MB)

Merged IRB
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Merged RGB
map-projected  (52MB)

RGB color
non map           (113MB)
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’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. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.