Mathematics – Logic
Scientific paper
Apr 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001psrd.repte..49t&link_type=abstract
Planetary Science Research Discoveries
Mathematics
Logic
Mars, Meteorites, Oxidized Crust, Water
Scientific paper
Mars is wet. Or at least it was wet. Vast canyons, numerous gullies, and even possible ocean deposits attest to the presence of abundant water on the planet, but magmas do not seem to have contained much of it. The logical way to transport water to the surface of a planet is in magma that erupts to form volcanoes and lava flows. Where did the water come from if not from magmas? Where did it go? Why are the magmas apparently so dry? Two studies of Martian meteorites may provide answers to these questions. Both use a combination of analyses of meteorites and laboratory experiments. One study, led by Harry Y. (Hap) McSween of the University of Tennessee (UT) and coworkers from UT, the Massachusetts Institute of Technology (MIT), Oakridge National Laboratory, and the University of South Florida, measured the abundances of water-soluble trace elements in crystals in a Martian meteorite. They found the centers of the minerals, which formed first and at high pressure, had much more of these elements than the rims. McSween and coworkers cite data showing that the elements are highly soluble in the presence of very hot water. Experiments at MIT show that magma must have contained about 1.8 wt% H2O to crystallize the minerals observed in the Martian meteorite studied. The scientists conclude that magmas have delivered lots of water to the Martian surface.
The other study, by Meenakshi (Mini) Wadhwa (Field Museum, Chicago) focused on the concentration of the element europium in six meteorites from Mars. By using experimental data obtained by Gordon McKay and Loan Le (Johnson Space Center), Wadhwa concludes that the magmas in which the meteorites formed experienced varying amounts of interaction with the crust of Mars, which must be oxidized. She suggests that the oxidation is due to chemical reactions of rock and water--probably the same water that carved the surface features on Mars.
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