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ALH84001 Origin
Meteorite From the Ancient Crust of Mars by G. Jeffrey Taylor
Like most meteorites, it was partly covered with smooth, dark, glassy material, called the fusion crust, which formed when the rock blazed through the Earth's atmosphere. It was found in 1984 during the annual meteorite search in Antarctica. According to geologist Roberta Score, former laboratory manager in the meteorite curatorial facility and the explorer who actually found the meteorite, the rock looked greenish inside as it lay on the Antarctic ice. In the laboratory, however, it looks gray. (NASA photo.)
Orthopyroxene makes up about 95% of the rock, and the large size of the crystals suggests that the rock crystallized in a slowly-cooling magma body inside the Martian crust. The crystals contain numerous cracks and are separated by crushed
zones of much smaller crystals. These zones probably formed when high-pressure shock
waves, generated by an impact, crushed portions of the large crystals. Crushed zones and
other cracks in the rock contain the carbonate globules that have the features ascribed to
biological processes. (Photo courtesy of David Mittlefehldt, Lockheed
Engineering and Science Company.)
As discussed in The Evidence and the Debate, a big discussion centers on the origin of the globules, especially whether they formed from very hot fluids (more than 650 degrees Celsius) or cooler ones (between 0 and 80 degrees Celsius) . Life would not have survived high temperatures. (NASA photo.)
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