NASA Mars Lander Sees Falling Snow, Soil Data Suggest Liquid Past

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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

NEWS RELEASE: 2008-183 Sept. 29, 2008

NASA Mars Lander Sees Falling Snow, Soil Data Suggest Liquid Past

PASADENA, Calif. -- NASA's Phoenix Mars Lander has detected snow falling from Martian
clouds. Spacecraft soil experiments also have provided evidence of past interaction between
minerals and liquid water, processes that occur on Earth.

A laser instrument designed to gather knowledge of how the atmosphere and surface interact on
Mars has detected snow from clouds about 4 kilometers (2.5 miles) above the spacecraft's landing
site. Data show the snow vaporizing before reaching the ground.

"Nothing like this view has ever been seen on Mars," said Jim Whiteway, of York University,
Toronto, lead scientist for the Canadian-supplied Meteorological Station on Phoenix. "We'll be
looking for signs that the snow may even reach the ground."

Phoenix experiments also yielded clues pointing to calcium carbonate, the main composition of
chalk, and particles that could be clay. Most carbonates and clays on Earth form only in the presence
of liquid water.

"We are still collecting data and have lots of analysis ahead, but we are making good progress on the
big questions we set out for ourselves," said Phoenix Principal Investigator Peter Smith of the
University of Arizona, Tucson.

Since landing on May 25, Phoenix already has confirmed that a hard subsurface layer at its far-
northern site contains water-ice. Determining whether that ice ever thaws would help answer
whether the environment there has been favorable for life, a key aim of the mission.

The evidence for calcium carbonate in soil samples from trenches dug by the Phoenix robotic arm
comes from two laboratory instruments called the Thermal and Evolved Gas Analyzer, or TEGA,
and the wet chemistry laboratory of the Microscopy, Electrochemistry and Conductivity Analyzer, or
MECA.

"We have found carbonate," said William Boynton of the University of Arizona, lead scientist for
the TEGA. "This points toward episodes of interaction with water in the past."

The TEGA evidence for calcium carbonate came from a high-temperature release of carbon dioxide
from soil samples. The temperature of the release matches a temperature known to decompose
calcium carbonate and release carbon dioxide gas, which was identified by the instrument's mass
spectrometer.

The MECA evidence came from a buffering effect characteristic of calcium carbonate assessed in
wet chemistry analysis of the soil. The measured concentration of calcium was exactly what would
be expected for a solution buffered by calcium carbonate.

Both TEGA, and the microscopy part of MECA, have turned up hints of a clay-like substance. "We
are seeing smooth-surfaced, platy particles with the atomic-force microscope, not inconsistent with
the appearance of clay particles," said Michael Hecht, MECA lead scientist at NASA's Jet
Propulsion Laboratory in Pasadena, Calif.

The Phoenix mission, originally planned for three months on Mars, now is in its fifth month.
However, it faces a decline in solar energy that is expected to curtail and then end the lander's
activities before the end of the year. Before power ceases, the Phoenix team will attempt to activate a
microphone on the lander to possibly capture sounds on Mars.

"For nearly three months after landing, the sun never went below the horizon at our landing site,"
said Barry Goldstein, JPL Phoenix project manager. "Now it is gone for more than four hours each
night, and the output from our solar panels is dropping each week. Before the end of October, there
won't be enough energy to keep using the robotic arm."

The Phoenix mission is led by Smith at the University of Arizona. Project management is the
responsibility of JPL with development partnership by Lockheed Martin in Denver. International
contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the
universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish
Meteorological Institute.

More information about Phoenix is at http://www.nasa.gov/phoenix .

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