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Shortly after NASA’s Phoenix lander settles onto Mars’ frigid, northern plains on May 25, it will undertake what is literally a microscopic examination of the red sand beneath its feet. By doing so, it may find evidence that liquid water – generally agreed to be a prerequisite of life – once pooled here.
Examination of the Martian soil is part of the task of a sophisticated on-board instrument package known as MECA, for Microscopy, Electrochemistry, and Conductivity Analyzer (MECA). Two microscopes are part of this package, and it is their close-up views that might supply conclusive evidence for a watery past. According to John Marshall, a planetary geologist with the Carl Sagan Center at the SETI Institute, “this very detailed examination of the sand grains could supply a vital clue as to whether Mars was ever conducive to life – or if microscopic life might still have a foothold there.”
Imaging is a big part of the Phoenix mission. On the main deck of the lander is a stereo camera that will provide landscape views. The camera on the robotic arm can see sand and pebbles. But the MECA has both a low-power optical microscope for scrutinizing a field-of-view only millimeters in size, and an atomic force microscope able to make a “topographic map” of soil particles with detail a thousand times finer than its optical counterpart. The atomic force microscope works by means of a tiny stylus that “feels” its way over the sample.
| Dr. John Marshall Carl Sagan Center Principal Investigator |
Dr. Richard Quinn Carl Sagan Center Principal Investigator |
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“If you see little clay particles,” Marshall notes, “you say ah, hah! There’s been aqueous weathering here – chemical alteration of the grains. It would be just like the clay you find in your back yard.” |
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| View the Phoenix Lander simulation | Links | |