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Scientists discover new planet orbiting dangerously close to giant star 11/20/2008

Comet particles provide glimpse of solar system's birth spasms 11/19/2008

Complex systems and Mars missions help understand how life began 11/16/2008

APEX reveals glowing stellar nurseries 11/15/2008

Hubble directly observes a planet orbiting another star 11/14/2008

To widen path to outer space, engineers build small satellite 11/14/2008

Rocket Launching To Investigate The Northern Lights 11/12/2008

A pool of distant galaxies -- the deepest ultraviolet image of the universe yet 11/8/2008

Giant simulation could solve mystery of 'dark matter' 11/6/2008

Chandrayaan-1 now in lunar transfer trajectory 11/6/2008

Moore Foundation awards RIT $2.8M to develop 'noiseless' detector 11/4/2008

Magnetic Portals Connect Sun and Earth 11/2/2008

Researchers find clues to planets' birth 11/1/2008

Hubble scores a perfect 10 10/31/2008

GOCE launch delayed until 2009 10/30/2008

Frozen Water Confirmed on Mars (6/24/2008)

Tags:
mars, planets, landers, phoenix, water

These color images were acquired by NASA's Phoenix Mars Lander's Surface Stereo Imager on the 21st and 25th days of the mission, or Sols 20 and 24 (June 15 and 19, 2008). These images show sublimation of ice in the trench informally called 'Dodo-Goldilocks' over the course of four days. In the lower left corner of the left image, a group of lumps is visible. In the right image, the lumps have disappeared, similar to the process of evaporation. (Credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University)
These color images were acquired by NASA's Phoenix Mars Lander's Surface Stereo Imager on the 21st and 25th days of the mission, or Sols 20 and 24 (June 15 and 19, 2008). These images show sublimation of ice in the trench informally called 'Dodo-Goldilocks' over the course of four days. In the lower left corner of the left image, a group of lumps is visible. In the right image, the lumps have disappeared, similar to the process of evaporation. (Credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University)
The Phoenix Mars Lander continues searching for related minerals and organic substances.

Scientists relishing confirmation of water ice near the surface beside NASA's Phoenix Mars Lander anticipate even bigger discoveries from the robotic mission in the weeks ahead.

"It is with great pride and a lot of joy that I announce today that we have found proof that this hard bright material is really water ice and not some other substance," said Phoenix Principal Investigator Peter Smith of The University of Arizona, during a Friday news briefing to announce the confirmation of water ice.

"The truth we're looking for is not just looking at ice. It is in finding out the minerals, chemicals and hopefully the organic materials associated with these discoveries," said Smith.

The mission has the right instruments for analyzing soil and ice to determine whether the local environment just below the surface of far-northern Mars has ever been favorable for microbial life. Key factors are whether the water ever becomes available as a liquid and whether organic compounds are present that could provide chemical building blocks and energy for life. Phoenix landed on May 25 for a Mars surface mission planned to last for three months.

"These latest developments are a major accomplishment and validation of the Mars program's 'follow-the-water' exploration framework," said Doug McCuistion at NASA Headquarters, Washington, director of the space agency's Mars Program. "This specific discovery is the result of an outstanding team working with a robust spacecraft that has allowed them to work ahead of their original science schedule."

The key new evidence is that chunks of bright material exposed by digging on June 15 and still present on June 16 had vaporized by June 19. "This tells us we've got water ice within reach of the arm, which means we can continue this investigation with the tools we brought with us," said Mark Lemmon of Texas A&M University, College Station, the lead scientist for Phoenix's Surface Stereo Imager camera. Lemmon said the disappearing chunks could not have been carbon-dioxide ice at the local temperatures because that material would not have been stable for even one day as a solid.

The disappearing chunks were in a trench to the northwest of the lander. A hard material, possibly more ice, but darker than the bright material in the first trench, has been detected in a second trench, to the northeast of the lander. Scientists plan next to have Phoenix collect and analyze surface soil from a third trench near the second one, and later to mechanically probe and sample the hard layer.

"We have in our ice-attack arsenal backhoeing, scraping and rasping, and we'll try all of these," said Ray Arvidson of Washington University in St. Louis, lead scientist for Phoenix's Robotic Arm.

Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory in Pasadena, Calif., reported that an issue reported earlier this week related to producing thousands of duplicate copies of some file-maintenance data files has been diagnosed, and a corrective software patch will be sent to Phoenix within a few days.

Science operations continue in the meantime, though all data collected must be relayed to Earth on the same Martian day it is collected, instead of being stored to non-volatile memory when Phoenix powers down to conserve energy during the Martian night.

Images sent back Friday morning from Mars showed that the doors to the No. 5 oven on the Thermal and Evolved-Gas Analyzer opened part way. The instrument team is working to understand the consequences of this action.

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

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Comments:

1. MICHAEL J. SCHMITZ

6/25/2008 11:02:20 AM MST

DID YOU EVER THINK OF THE NEW ALIEN PROBE JUST OUTSIDE THE OZONE OF EARTH, OR IS THAT TO CLOSE FOR YOU?


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