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NASA's Phoenix Mars Lander Checking Soil Properties

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This image shows a view from NASA's Phoenix Mars Lander's Stereo Surface Imager's left eye after delivery of soil to the Thermal and Evolved-Gas Analyzer (TEGA), taken on the 12th Martian day after landing (Sol 12, June 6, 2008). Soil is visible on both sides of the open doors of TEGA's #4 oven. Sensors inside the device indicate no soil passed through the screen and into the oven. (NASA/JPL-Caltech/University of Arizona/Texas A&M University)

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The Robotic Arm of NASA's Phoenix Mars Lander released a sample of Martian soil onto a screened opening of the lander's Thermal and Evolved-Gas Analyzer (TEGA) during the 12th Martian day, or sol, since landing (June 6, 2008). TEGA did not confirm that any of the sample had passed through the screen. The Robotic Arm Camera took this image on Sol 12. Soil from the sample delivery is visible on the sloped surface of TEGA, which has a series of parallel doors. The two doors for the targeted cell of TEGA are the one positioned vertically, at far right, and the one partially open just to the left of that one. The soil between those two doors is resting on a screen designed to let fine particles through while keeping bigger ones from clogging the interior of the instrument. Each door is about 10 centimeters (4 inches) long. (NASA/JPL-Caltech/University of Arizona/Max Planck Institute)

Soil rests on screen over open delivery door.


By University Communications
June 7, 2008

The arm of NASA's Phoenix Mars Lander released a handful of clumpy Martian soil onto a screened opening of a laboratory instrument on the spacecraft Friday, but the instrument did not confirm that any of the sample passed through the screen.

Engineers and scientists on the Phoenix team assembled at the University of Arizona are determining the best approach to get some of that material into the instrument. Meanwhile, the team has developed commands for the spacecraft to use cameras and the Robotic Arm on Saturday to study how strongly the soil from the top layer of the surface clings together into clumps.

Images taken Friday show soil resting on the screen over an open sample-delivery door of Phoenix's Thermal and Evolved-Gas Analyzer, or TEGA, an instrument for identifying some key ingredients. The screen is designed to let through particles up to one-millimeter (0.04 inch) across while keeping out larger particles, in order to prevent clogging a funnel pathway to a tiny oven inside. An infrared beam crossing the pathway checks whether particles are entering the instrument and breaking the beam.

The researchers have not yet determined why none of the sample appears to have gotten past the screen, but they have begun proposing possibilities.

"I think it's the cloddiness of the soil and not having enough fine granular material," said Ray Arvidson of Washington University in St. Louis, the Phoenix team's science lead for Saturday and digging czar for the mission.

"In the future, we may prepare the soil by pushing down on the surface with the arm before scooping up the material to break it up, then sprinkle a smaller amount over the door," he said.

Another strategy under consideration is to use mechanical shakers inside the TEGA instrument differently than the five minutes of shaking that was part of the sample-receiving process on Friday. No activities for the instrument are planned for Saturday, while the team refines plans for diagnostic tests.

Phoenix's planned activities for Saturday include horizontally extending a trench where the lander dug two practice scoops earlier this week, and taking additional images of a small pile of soil that was scooped up and dropped onto the surface during the second of those practice digs.

"We are hoping to learn more about the soil's physical properties at this site," Arvidson said. "It may be more cohesive than what we have seen at earlier Mars landing sites."

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute.

 

 

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