[meteorite-list] August Geology Highlights
From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu Jul 29 17:41:17 2004 Message-ID: <200407292141.OAA03640_at_zagami.jpl.nasa.gov> http://www.eurekalert.org/pub_releases/2004-07/gsoa-ag072904.php Public release date: 29-Jul-2004 Contact: Ann Cairns acairns_at_geosociety.org 303-357-1056 Geological Society of America August GEOLOGY & GSA TODAY media highlights Boulder, Colo. - The August issue of GEOLOGY covers a wide variety of potentially newsworthy subjects. Topics include: water chemistry as a predictor of earthquakes; insights into Martian surface alteration; whether many small ruptures on the San Andreas fault might reduce occurrence of large earthquakes; impact of glacial-interglacial rhythms on rainforests; evidence of the Chesapeake Bay impact event found in Georgia; and how Richmond's Goochland terrane originated in Long Island, went out to sea, and ended up in Virginia. GSA TODAY's science article describes monitoring volcanic activity with satellite radar technology. Highlights are provided below. Representatives of the media may obtain complimentary copies of articles by contacting Ann Cairns at acairns_at_geosociety.org <mailto:acairns@geosociety.org">. Please discuss articles of interest with the authors before publishing stories on their work, and please make reference to GEOLOGY in articles published. Contact Ann Cairns for additional information or other assistance. Non-media requests for articles may be directed to GSA Sales and Service, gsaservice_at_geosociety.org <mailto:gsaservice@geosociety.org> GEOLOGY [snip] Global geologic context for rock types and surface alteration on Mars Michael B. Wyatt, Arizona State University, Geological Sciences, Mars Space Flight Facility, Tempe, AZ 85251, USA, et al. Pages 645-648. Interpretations of rock compositions from thermal emission spectra from Mars orbiting spacecraft indicate the widespread occurrence of basaltic and either andesitic or partly altered basalt surface compositions. It is important to distinguish andesitic and altered basalt compositions on Mars because each rock type has implications for planetary physical and chemical conditions and petrogenetic processes. Here we assess these conflicting interpretations of martian surface lithologies in light of new geologic context emerging from the Mars Global Surveyor and Mars Odyssey missions. Based on global geologic context, we propose a model to describe the distributions of martian surface compositions and argue that portions of Mars experienced surface alteration over a cold and episodically wet geologic history. We propose the formation of altered units through limited chemical weathering from basalt interactions with icy mantles deposited during periods of high obliquity. Alteration of sediments in the northern lowlands depocenter may have been enhanced by temporary standing bodies of water and ice. [snip] Age and temperature of shock metamorphism of Martian meteorite Los Angeles from (U-Th)/He thermochronometry Kyoungwon Min, Yale University, Geology & Geophysics, New Haven, CT 06511, USA, et al. Pages 677-680. All of the martian meteorites are believed to have experienced impact collision on Mars. Partly because the duration of impact-induced shock metamorphism is very short, constraining the timing and temperature of shock events has been problematic. We applied (U-Th)/He dating method to single grains of phosphates from the Los Angeles Martian meteorite. The most reliable (U-Th)/He age of 3.28 ? 0.15 Ma (2?) is suggested to represent the timing of shock metamorphism. This age is identical with the cosmic-ray exposure ages, suggesting that shock metamorphism was coeval with ejection of the Los Angeles precursor from Mars. The initial temperature of the shock metamorphism is deduced by modeling He diffusion in the phosphates. From these calculations, we conclude that the metamorphic temperature of the shock event was higher than 450 ?C. These results support the idea that shock pressures of some Martian meteorites were higher than 45 GPa, as inferred from the presence of a high-pressure form of SiO2. Single grain (U-Th)/He dating of phosphates may provide unique constraints on the timing and pressure-temperature dynamics of shock metamorphism in a wide variety of extraterrestrial materials. [snip] An upper Eocene impact horizon in east-central Georgia R. Scott Harris, Brown University, Geological Sciences, Providence, RI 02912, USA, et al. Pages 717-720. The authors report the discovery of shocked quartz grains in an upper Eocene sand layer exposed in the open-pit kaolin mines of east-central Georgia. Shocked quartz is formed during cataclysmic events when large asteroids or comets crash into the crust of the Earth. The shocked quartz grains in this layer probably represent the fallout of debris ejected from the impact that formed the Chesapeake Bay crater about 36 million years ago. The authors also suggest that the layer is the most likely source of the tektites that are scattered across central Georgia. Received on Thu 29 Jul 2004 05:41:13 PM PDT |
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