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Intense heat killed the Universe's would-be galaxies, researchers say 7/2/2009

Largest ever survey of very distant galaxy clusters completed 7/1/2009

New instrument has potential to detect water deep underground on Mars 6/30/2009

Salty ocean in the depths of Enceladus 6/30/2009

Galaxies coming of age in cosmic blobs 6/29/2009

Jets on Saturn's moon Enceladus not geysers from underground ocean, says study 6/28/2009

Milky Way's super-efficient particle accelerators caught in the act 6/28/2009

Better looks at Mars minerals for instrument on NASA's Mars Odyssey orbiter 6/27/2009

NASA lunar mission successfully enters moon orbit 6/26/2009

Magnetic field on bright star Vega 6/25/2009

Team finds definitive evidence for ancient lake on Mars 6/24/2009

Newly revised handbook of space technology now available 6/23/2009

Astronomy team among first to use massive new telescope 6/22/2009

Magnetospheric Multiscale mission enters implementation phase 6/22/2009

Herschel's daring test: A glimpse of things to come 6/22/2009

Phoenix Scrapes 'Almost Perfect' Icy Soil for Analysis (7/2/2008)

Tags:
mars, planets, landers, phoenix, water

This image was acquired by NASA's Phoenix Mars Lander's Robotic Arm Camera on the 35th Martian day of the mission, or Sol 34 (June 29, 2008). This image shows the trench informally called 'Snow White 5.' The trench is 4-to-5 centimeters (about 1.5-to-1.9 inches) deep, 24 centimeters (about 9 inches) wide and 33 centimeters (13 inches) long. Snow White 5 is Phoenix's current active digging area after additional trenching, grooming, and scraping by Phoenix's Robotic Arm in the last few sols to trenches informally called Snow White 1, 2, 3, and 4. Near the top center of the image is the Robotic Arm's Thermal and Electrical Conductivity Probe. Snow White 5 is located in a patch of Martian soil near the center of a polygonal surface feature, nicknamed 'Cheshire Cat.' The digging site has been named 'Wonderland.' This image has been enhanced to brighten shaded areas. (NASA/JPL-Caltech/University of Arizona/Max Planck Institute )
This image was acquired by NASA's Phoenix Mars Lander's Robotic Arm Camera on the 35th Martian day of the mission, or Sol 34 (June 29, 2008). This image shows the trench informally called 'Snow White 5.' The trench is 4-to-5 centimeters (about 1.5-to-1.9 inches) deep, 24 centimeters (about 9 inches) wide and 33 centimeters (13 inches) long. Snow White 5 is Phoenix's current active digging area after additional trenching, grooming, and scraping by Phoenix's Robotic Arm in the last few sols to trenches informally called Snow White 1, 2, 3, and 4. Near the top center of the image is the Robotic Arm's Thermal and Electrical Conductivity Probe. Snow White 5 is located in a patch of Martian soil near the center of a polygonal surface feature, nicknamed 'Cheshire Cat.' The digging site has been named 'Wonderland.' This image has been enhanced to brighten shaded areas. (NASA/JPL-Caltech/University of Arizona/Max Planck Institute )
Samples hold clues to history of Martian water, climate and possible habitability.

NASA's Phoenix Mars Lander enlarged the "Snow White" trench and scraped up little piles of icy soil on Saturday, June 28, the 33rd Martian day, or sol, of the mission. Scientists say that the scrapings are ideal for the lander's analytical instruments.

The robotic arm on Phoenix used the blade on its scoop to make 50 scrapes in the icy layer buried under subsurface soil. The robotic arm then heaped the scrapings into a few 10- to 20-cubic centimeter piles, or piles each containing between two and four teaspoonfuls. Scraping created a grid about two millimeters deep.

The scientists saw the scrapings in Surface Stereo Imager images on Sunday, June 29, agreed they had "almost perfect samples of the interface of ice and soil," and commanded the robotic arm to pick up some scrapings for instrument analysis.

The scoop will sprinkle the fairly fine-grained material first onto the Thermal and Evolved-Gas Analyzer, or TEGA. The instrument has tiny ovens to bake and sniff the soil to assess its volatile ingredients, such as water. It can determine the melting point of ice.

Phoenix's overall goals are to: dig to water frozen under subsurface soil, touch, examine, vaporize and sniff the soil and ice to discover the history of water on Mars, determine if the Martian arctic soil could support life and study Martian weather from a polar perspective.

Note: This story has been adapted from a news release issued by the University of Arizona

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