A gamma-ray spectroscopy survey of Omani meteorites
Patrick Weber, Beda Hofmann, Tamer Tolba, Jean-Luc Vuilleumier

TL;DR
This study used gamma-ray spectroscopy to analyze 33 meteorites from Oman, revealing information about their composition, weathering, terrestrial age, and recent falls, demonstrating the method's effectiveness in identifying recent meteorite arrivals.
Contribution
The paper presents the first gamma-ray spectroscopy survey of Omani meteorites, providing insights into their terrestrial ages, weathering states, and recent fall detection, which was not previously documented.
Findings
Potassium and thorium levels within typical ranges for meteorite types.
Detection of a recent fall (SaU 424) via 22Na activity.
Estimated fall rate of ~120 events per million km² per year.
Abstract
The gamma-ray activities of 33 meteorite samples (30 ordinary chondrites, 1 Mars meteorite, 1 iron, 1 howardite) collected during Omani-Swiss meteorite search campaigns 2001-2008 were nondestructively measured using an ultra-low background gamma-ray detector. The results provide several types of information: Potassium and thorium concentrations were found to range within typical values for the meteorite types. Similar mean 26Al activities in groups of ordinary chondrites with a) weathering degrees W0-1 and low 14C terrestrial age and b) weathering degree W3-4 and high 14C terrestrial age are mostly consistent with activities observed in recent falls. The older group shows no significant depletion in 26Al. Among the least weathered samples one meteorite (SaU 424) was found to contain detectable 22Na identifying it as recent fall close to the year 2000. Based on an estimate of the surface…
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