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Impact microcrater morphology on Australian microtektites

DRS at CSIR-National Institute of Oceanography

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Title Impact microcrater morphology on Australian microtektites
 
Creator ShyamPrasad, M.
Khedekar, V.D.
 
Subject extraterrestrial material
sediments
electron microscopy
cosmic dust
 
Description Scanning electron microscopy of 137 Australian microtekties and fragments from 4 sediments cores in the Central Indian Ocean reveals more than 2000 impact-generated features in the size range of 0.3 to 600 mu m. Three distinct impact types are recognized: destructive, erosive, and accretionery. A large variation in impact energy is seen in terms of catastrophic destruction demonstrated by fragmented microtektites through erosive impacts comprising glass-lined pit craters, stylus pit craters, pitless craters, and a small number of accretionery features as well. The size range of observed microtektites is from 180 to 2320 mu m, and not only are the smaller microtektites seen to have the largest number of impacts, but most of these impacts are also of the erosive category, indicating that target temperature is an important factor for retaining impact-generated features. Further, microcratering due to collisions in impact-generated plumes seems to exist on a larger and more violent scale than previously known. Although the microcraters are produced in a terrestrially generated impact plume, they resemble lunar microcraters in many ways: (1) the size range of impacts and crater morphology variation with increasing size; (2) dominant crater number densities in mu m and sub-mu m sizes. Therefore, taktite-producing impacts can lead to the generation of microcraters that mimic those found on lunar surface materials, and for the lunar rocks to qualify as reliable cosmic dust flux detectors, their tumbling histories and lunar surface orientations have to be known precisely
 
Date 2008-07-18T05:45:18Z
2008-07-18T05:45:18Z
2003
 
Type Journal Article
 
Identifier Meteoritics and Planetary Science, Vol.38; 1351-1371p.
http://drs.nio.org/drs/handle/2264/1254
 
Language en
 
Rights Copyright [2003]. It is tried to respect the rights of the copyright holders to the best of the knowledge. If it is brought to our notice that the rights are violated then the item would be withdrawn.
 
Publisher Meteoritical Society