Clumps on Phoenix Lander's Leg Strut Have Grown

The Robotic Arm Camera on the Phoenix Mars Lander took this view under the spacecraft on Sept. 1, 2008, the 97th Martian day of the mission after landing. The lander leg strut at upper left features clumps larger than those seen three months ago. Also, exposed patches beneath the lander are darker than they used to be. (NASA/JPL-Calech/University of Arizona/Max Planck Institute)

Phoenix's Robotic Arm Camera took this image on June 2, 2008, on the eighth Martian day of the mission after landing. The light feature in the middle of the image below the leg is informally called "Holy Cow." The dust, shown in the dark foreground, has been blown off of "Holy Cow" by Phoenix's thruster engines. (NASA/JPL-Calech/University of Arizona/Max Planck Institute)
"Holy Cow" and other patches beneath the lander are darker.
Clumps adhering to a leg strut on NASA's Phoenix Mars Lander are larger than they were three months ago, according to a recent photograph from the lander on the northern polar region of Mars.
The Robotic Arm Camera took the image on Sept. 1, 2008, at about 4 a.m. local solar time during the 97th Martian day, or sol, since landing. The view underneath the lander shows growth of the clumps adhering to leg strut seen at the upper left in the picture, compared with a view of the same strut in a similar image taken about three months earlier.
The view in the Sol 97 image is southward. Illumination is from the early morning sun above the northeastern horizon. This illumination is quite different from the illumination in the Sol 8 image, which was taken in mid-afternoon.
The science team has discussed various possible explanations for these clumps. One suggestion is that they may have started from a splash of mud if Phoenix's descent engines melted icy soil during the landing. Another is that specks of salt may have landed on the strut and began attracting atmospheric moisture that freezes and accumulates. The clumps are concentrated on the north side of the strut, usually in the shade, so their accumulation could be a consequence of the fact that condensation favors colder surfaces.
The flat, smooth patches of ice exposed underneath the lander seem to be partly covered by darker material left behind as ice vaporizes away in the recent image, compared with the one taken thee months earlier. The flat patch in the center of the image has the informal name "Holy Cow," based on researchers' reaction when they initially saw the feature.
The Phoenix Mission is led by Peter Smith of The University of Arizona, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif.
et cetera
- Extra Info |
- Contact Info
Sara Hammond, University of Arizona
520-626-1974
Guy Webster, NASA Jet Propulsion Lab
818-354-5011
Dwayne Brown
NASA Headquarters, Washington
202-358-1726


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