Wednesday, May 26, 2010
NASA has given up hope that the Phoenix Mars Lander will transmit any new signals after being buried under Martian ice. Daniel Stolte of University Communications tells us:
NASA's Phoenix Mars Lander has ended operations after repeated attempts to contact the spacecraft were unsuccessful. A new image transmitted by NASA's Mars Reconnaissance Orbiter, or MRO, shows signs of severe ice damage to the lander's solar panels.
An image of Phoenix taken this month by the High Resolution Imaging Science Experiment, or HiRISE, camera on MRO suggests the lander no longer casts shadows the way it did during its working lifetime.
"The latest HiRISE image appears to show that a solar panel of the Phoenix lander has collapsed," said University of Arizona planetary scientist Alfred McEwen, who is the principal investigator of the HiRISE camera project.
According to McEwen, it gets so cold during the Martian winter that carbon dioxide, which accounts for 95 percent of the planet's atmosphere, forms a frost blanket up to one or more feet thick
that covers the entire northern landscape each winter, including any spacecraft that might be on the surface.
Said McEwen: "The Mars Lander's solar panels were not designed to withstand significant loads of such carbon dioxide frost."
Last week, NASA's Mars Odyssey orbiter flew over the Phoenix landing site 61 times during a final attempt to communicate with the lander. No transmission from the lander was detected. Phoenix also did not communicate during 150 flights in three earlier listening campaigns this year.
Earth-based research continues on discoveries Phoenix made during summer conditions at the far-northern Mars site where it landed May 25, 2008. The solar-powered lander completed its three-month mission and kept working until sunlight waned two months later.
Phoenix was not designed to survive the dark, cold, icy winter. However, the slim possibility Phoenix survived could not be eliminated without listening for the lander after abundant sunshine returned.
"Before and after images are dramatically different," said Michael Mellon of the University of Colorado in Boulder, a science team member for both Phoenix and HiRISE.
"The lander looks smaller, and only a portion of the difference can be explained by accumulation of dust on the lander, which makes its surfaces less distinguishable from surrounding ground."
Apparent changes in the shadows cast by the lander are consistent with predictions of how Phoenix could be damaged by harsh winter conditions. It was anticipated that the weight of a carbon-dioxide ice buildup could bend or break the lander's solar panels.
"The Phoenix spacecraft succeeded in its investigations and exceeded its planned lifetime," said Fuk Li, manager of the Mars Exploration Program at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Although its work is finished, analysis of information from Phoenix's science activities will continue for many years to come."
During its mission, Phoenix confirmed and examined patches of the widespread deposits of underground water ice detected by Odyssey and identified a mineral called calcium carbonate that suggested occasional presence of thawed water.
The lander also found soil chemistry with significant implications for life and observed falling snow. The mission's biggest surprise was the discovery of perchlorate, an oxidizing chemical on Earth that is food for some microbes and potentially toxic for others.
"We found that the soil above the ice can act like a sponge, with perchlorate scavenging water from the atmosphere and holding on to it," said Peter Smith, Phoenix principal investigator at the UA. "You can have a thin film layer of water capable of being a habitable environment. A micro-world at the scale of grains of soil — that's where the action is."
The perchlorate results are shaping subsequent astrobiology research, as scientists investigate the implications of its antifreeze properties and potential use as an energy source by microbes. Discovery of the ice in the uppermost soil by Odyssey pointed the way for Phoenix. More recently, the MRO detected numerous ice deposits in middle latitudes at greater depth using radar and exposed on the surface by fresh impact craters.
"Ice-rich environments are an even bigger part of the planet than we thought," Smith said. "We are finding that a complex chemistry associated with the icy soil makes this vast region an excellent destination for future missions searching for Martian life."
NASA's MRO reached the planet in 2006 to begin a two-year primary science mission. Its data show Mars had diverse wet environments at many locations for differing durations during the planet's history, and climate-change cycles persist into the present era. The mission has returned more planetary data than all other Mars missons combined.
Odyssey has been orbiting Mars since 2001. The mission also has played important roles by supporting the twin Mars rovers Spirit and Opportunity. The Phoenix mission was led by Smith at the UA, with project management at JPL and development partnership at Lockheed Martin in Denver. The UA operates the HiRISE camera, which was built by Ball Aerospace and Technologies Corp., in Boulder. Mars missions are managed by JPL for NASA's Mars Exploration Program at NASA Headquarters in Washington.