Exploration: Secrets of the Soil
Is there life on today? This question has been fiercely debated by scientists for the past thirty years.
The evidence sent back from by two Viking Landers in 1976 and 1977 was inconclusive. In fact, NASA's first press release about the Viking tests announced that the results were positive. The "labeled Release" (LR) experiments had given positive results. But after lengthy discussions in which Carl Sagan participated, NASA reversed its position, mainly because another experiment detected no organics in the soil.
Yet to this day, Gilbert Levin, the principal designer of the LR
experiment, believes the tests pointed to life on (7). When the
same two experiments were run on soil from Antarctica, the same
conflicting results were obtained (LR - positive; organics - negative.)
Soil and ice from Antarctica certainly contains life. The test for
organics was negative because it is far less sensitive than the LR
experiment. The same problem could have caused the organics test on
to give a false negative.
Before oxygen could accumulate in Earth's atmosphere, all the
exposed iron had to rust. During that process, lasting hundreds of
millions of years, Earth was also a red planet. In the current issue of
the journal Nature, Corinna Wu asks: Could the oxygen that
rusted the iron on have been produced biologically? Could life on
have simply "run out of steam" after that stage of its development?
The answers to these profound questions will hopefully be made by
the Phoenix Probe's Thermal and Evolved Gas Analyzer (TEGA) built by
the University of Arizona and University of Texas, is a combination
high-temperature furnace and mass spectrometer instrument that
scientists will use to analyze Martian ice and soil samples. The
robotic arm will deliver samples to a hopper designed to feed a small
amount of soil and ice into eight tiny ovens about the size of an ink
cartridge in a ballpoint pen. Each of these ovens will be used only
once to analyze eight unique samples.
Once a sample is
successfully received and sealed in an oven, the temperature is slowly
increased at a constant rate, and the power required for heating is
carefully and continuously monitored. This process, called scanning
calorimetry, shows the transitions from solid to liquid to gas of the
different materials in the sample: important information needed by
scientists to understand the chemical character of the soil and ice.
As
the temperature of the furnace increases up to 1000°C (1800°F), the ice
and other volatile materials in the sample are vaporized into a stream
of gases. These are called evolved gases and are transported via an
inert carrier to a mass spectrometer, a device used to measure the mass
and concentrations of specific molecules and atoms in a sample. The
mass spectrometer is sensitive to detection levels down to 10 parts per
billion, a level that may detect minute quantities of organic molecules
potentially existing in the ice and soil.
With these precise
measurement capabilities, scientists will be able to determine ratios
of various isotopes of hydrogen, oxygen, carbon, and nitrogen,
providing clues to origin of the volatile molecules, and possibly,
biological processes that occurred in the past.
Posted Casey Kazan.
Related Galaxy posts:
Is there an Interplanetary Mars-Earth Microbe Shuttle?
"The Overview Effect": Is Space Travel Next Step in Human Evolution?
Lonely Hearts of the Cosmos Revisited -NASA's Phoenix Probe & the Search for
Life from the Center of the Earth - The Shadow World of Our Hidden
New Phoenix Mission Technology to Search for Life
2053 -A Space Odyssey? Renowned Cosmologist Says We Need Space Colonization NOW
Space Colonization -Our Future or Fantasy?
Cruising the Goldilocks Zone -The Search for "Super-Earths"
Non-Carbon Lifeforms -Why We May Overlook
James Cameron & Arthur C Clarke on Space Odyssey 2001 -A Video
Search for Extraterrestrial Genomes
Links:
http://www.nature.com/news/2007/070813/full/448742a.html







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