Next Mars Soil Scoop Slated for Last of Lander's Wet Lab Cells

The chosen source for that sample is from the “Snow White” trench on the eastern end of the work area reachable with Phoenix's robotic arm. In July that trench yielded a sample in which another analytical instrument, the Thermal and Evolved Gas Analyzer, or TEGA, confirmed the presence of water ice. One of the three cells previously used on the wet chemistry laboratory also analyzed a sample from Snow White.

The wet chemistry laboratory mixes Martian soil with purified water brought from Earth as part of its process for identifying soluble nutrients and other chemicals in the soil. Scientists have used it to determine that the soil beside the lander is alkaline and to identify magnesium, sodium, potassium, chloride and perchlorate in the soil.

The Phoenix team plans to fill the last four of eight single-use ovens on the TEGA instrument without waiting for the analysis of each sample to be completed before delivering the next. The strategy is to get as many samples as possible delivered while there is still enough energy available for digging. The northern Martian summer is nearly half over. The amount of sunshine reaching Phoenix's solar panels, and consequently the amount of electricity produced by the panels, is declining.

“Now that the sun is not constantly above the horizon at our landing site we are generating less power every sol,” said Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, Calif. “When we landed in late May, and through much of our mission, we generated about 3,500 watt-hours every sol. We are currently at about 2,500 watt-hours, and sinking daily. With the remaining sols we need to scurry to squeeze the last bit of science out of the mission.”

One hundred watt-hours is equivalent to what is needed to illuminate a 100-watt bulb for one hour.

As TEGA bakes samples, it identifies the temperatures at which volatile ingredients in the soil are vaporized. It also has a mass spectrometer to identify the vapors. A valve that controls the flow of a carrier gas for transporting the vapors to the mass spectrometer is no longer reliable, but researchers anticipate that the remaining samples will yield enough vaporized water and carbon dioxide to carry any scarcer vapors to the spectrometer. The team is also examining possible operational workarounds for unanticipated opening of a valve controlling flow of calibration gas.

The Snow White trench is the chosen source for the next sample to go into a TEGA oven, as well as the next sample for the wet chemistry laboratory. For the TEGA sample, the team plans to use a rasp on the robotic arm to churn up ice-rich material from the hard floor of the trench. Ice-rich samples stuck inside the scoop during two attempts in July to deliver them to a TEGA oven. However, a test run on Aug. 30 verified that an ice-rich sample can be delivered using methods that minimize the time the sample is in the scoop and the exposure of the scoop to direct sunlight.

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

MEDIA CONTACTS:

Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov
Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov
Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu