Phoenix prepares to move arm

Mission scientists are eager to move Phoenix's robotic arm, for that arm will deliver samples of icy terrain to their instruments made to study this unexplored Martian environment.
The team sent commands for moving the arm on Tuesday morning, May 27, to NASA's Mars Reconnaissance Orbiter for relay to Phoenix. However, the orbiter did not relay those commands to the lander, so arm movement and other activities are now planned for Wednesday. The orbiter's communication-relay system is in a standby mode. NASA's Mars Odyssey orbiter is available for relaying communications between Earth and Phoenix.

NASA's Mars Reconnaissance Orbiter did send back spectacular first images of the landed Phoenix from orbit, views from the Phoenix lander of where it will work for the next three months, and a preliminary weather report.

A newly processed image from the high-resolution camera known as HiRISE on NASA's Mars Reconnaissance Orbiter shows a full-resolution view of the Phoenix parachute and lander during its May 25 descent, with Heimdall crater in the background.

"Phoenix appears to be descending into the 10 kilometer, or 6-mile, crater, but is actually 20 kilometers, or about 12 miles, in front of the crater," said HiRISE principal investigator Alfred S. McEwen of the University of Arizona, Tucson.

HiRISE has taken a new color image of Phoenix on the ground about 22 hours after it landed. It shows the parachute attached to the back shell, the heat shield and the lander itself against red Mars. The parachute and lander are about 300 meters, roughly 1,000 feet, apart.

Commands to be sent to the lander Wednesday morning include taking more pictures of the surroundings and making the first movements of the mission's crucial robotic arm.

A covering that had shielded the arm from microbes during its last few months before launch had not fully retracted on landing day, May 25, but it moved farther from the arm during the following day.

"The biobarrier had relaxed more and allows more clearance, but it was not a major concern either way," said Fuk Li, manager of the Mars Exploration Program at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

During the next three months, the arm will dig into soil near the lander and deliver samples of soil and ice to laboratory instruments on the lander deck. Following today's commands, its movements will begin with unlatching the wrist, then moving the arm upwards in a stair-step manner.

Phoenix principal investigator Peter Smith of the University of Arizona was delighted with new images of the workspace. "The workspace is ideal for us because it looks very diggable. We're very happy to see just a few rocks scattered in the digging area."

The Phoenix weather station, provided by the Canadian Space Agency, was activated within the first hour after landing on Mars, and measurements are now being recorded continuously. The data from the first 18 hours after landing have been transmitted back to the science team, and they have provided a weather report. The temperature ranged between a minimum of minus 80 degrees Celsius (minus 112 degrees Fahrenheit) in the early morning and a maximum of minus 30 degrees Celsius (minus 22 degrees Fahrenheit) in the afternoon. The average pressure was 8.55 millibars, which is less than a hundredth of the sea level pressure on Earth. The wind speed was 20 kilometers per hour (13 miles per hour), out of the northeast. The skies were clear. More instruments will be activated over the coming days, and the weather report will expand to include measurements of humidity and visibility.

Smith presented a new Surface Stereo Imager view of the American flag and a mini-DVD on the Phoenix's deck, about three feet above the Martian surface. The mini-DVD from the Planetary Society contains a message to future Martian explorers, science fiction stories and art inspired by the Red Planet, and the names of more than a quarter million Earthlings.

Credit: NASA/JPL/University of Arizona.
High resolution image.

Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) camera acquired this image of Phoenix hanging from its parachute as it descended to the Martian surface. Shown here is a 10 kilometer (6 mile) diameter crater informally called "Heimdall," and an improved full-resolution image of the parachute and lander. Although it appears that Phoenix is descending into the crater, it is actually about 20 kilometers (about 12 miles) in front of the crater.




Credit: NASA/JPL/University of Arizona.
High resolution image.

The HiRISE camera has acquired this image of the Phoenix landing site 22 hours after landing.

The image shows 3 unusual features, which were not present in the earlier HiRISE image PSP_007853_2485. We expect to find 3 main pieces of hardware: the parachute attached to the backshell, the heat shield, and the lander itself.

The parachute (lower left) is easy to identify because it is especially bright and the backshell is still attached to the parachute cords. The double dark marking at right seems most consistent with disturbance of the ground from impact and bouncing of the heat shield, which fell from a height of about 10 kilometers. The last object (upper left) is the Phoenix Lander whose two solar panels on either side of the lander are clearly visible.

This image was acquired on the ascending node of the orbit making it about 3:00PM local time on the surface. The rest of the HiRISE observation shows a cloud free day for Phoenix Lander operations.




Credit: NASA/JPL/University of Arizona.
High resolution image.

This closeup shows the Phoenix lander with its solar panels deployed on the Mars surface.



Credit: NASA/JPL/University of Arizona.
High resolution image.

This image, released on Memorial Day, May 26, 2008, shows the American flag and a mini-DVD on the Phoenix's deck, which is about 3 ft. above the Martian surface. The mini-DVD from the Planetary Society contains a message to future Martian explorers, science fiction stories and art inspired by the Red Planet, and the names of more than a quarter million earthlings.

Source: Jet Propulsion Laboratory
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