The paper's authors are David S. McKay and Everett K. Gibson, Jr., of NASA's Johnson Space Center in Houston, TX; Kathie L. Thomas-Keprta of Lockheed Martin in Houston, TX; Hojatollah Vali of McGill University in Montreal, Quebec; Christopher S. Romanek of the University of Georgia's Savannah River Ecology Laboratory in Aiken, SC; and Simon J. Clemett, Xavier D.F. Chillier, Claude R. Maechling, and Richard N. Zare of Stanford University in Stanford, CA.
Organic (complex, carbon-based) molecules are the requisite building blocks of life on Earth. The authors looked for signs of such molecules and other mineralogical and textural indications of past life within the pore space and fractures of meteorite Allan Hills 84001 (ALH84001), one of only 12 meteorites identified as having come from Mars. ALH84001 is the oldest of the Martian dozen, having crystallized from molten rock about 4.5 billion years ago, early in the planet's evolution, and it is the only Martian meteorite to contain significant carbonate minerals. (The carbonates formed some time after the rock, perhaps about 3.6 billion years ago.)
About 15 million years ago, a major asteroid impact on Mars threw ALH84001 into space, and about 13,000 years ago it fell onto an ice field in Antarctica. ALH84001, which shows little evidence of terrestrial weathering, was discovered by meteorite-hunting scientists in 1984 and only recently identified as Martian.
ALH84001 is riven with tiny fractures resulting primarily from impacts that occurred while the rock was on Mars. The secondary carbonates formed along with some of these fractures. The Science authors prepared thin sample sections that included these pre-existing fractures, and found on their surfaces a clear and distinct distribution of polycyclic aromatic hydrocarbons (PAHs), organic molecules containing multiple connected rings of carbon atoms - the first organic molecules ever seen in a Martian rock. A variety of contamination checks and control experiments indicated that the organic material was indigenous to the rock and was not the result of terrestrial contamination. For example, the authors noted that the concentration of PAHs increases inward, whereas terrestrial contamination likely would have resulted in more PAHs on the exterior of the rock.
The big question is: where did the PAHs come from?
It is thought that PAHs can form one of two ways: nonbiologi-cally, during early star formation; or biologically, through the activity of bacteria or other living organisms, or their degradation (fossilization). On Earth, PAHs are abundant as fossil molecules in ancient sedimentary rocks, coal and petroleum, the result of chemical changes that occurred to the remains of dead marine plankton and early plant life. They also occur during partial combustion, such as when a candle burns or food is grilled.
To address the origin of these PAHs, the authors examined the chemistry, mineralogy, and texture of carbonates associated with PAHs in the Martian meteorite. Under the transmission electron microscope, the carbonate globules were seen to contain fine-grained magnetite and iron-sulfide particles. From these and other analyses, the authors developed a list of observations about the carbonates and PAHs that, taken individually, could be explained by nonbiological means. However, "when considered collectively . . . we conclude that [these phenomena] are evidence for primitive life on early Mars." Some of their observations are as follows:
--American Association for the Advancement of Science News Release
On to the next article, Microrover Ready to Roll!
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