Impact Studies
DOI: 10.1007/3-540-27548-7_2
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The Mechanics of Pseudotachylite Formation in Impact Events

Abstract: This paper presents a discussion of the basic constraints controlling the formation of pseudotachylites in the rapidly sheared rocks in the vicinity of a large meteorite impact. The prevailing opinion among many geologists is that pseudotachylites are formed by friction melting of rock. The principal mystery of pseudotachylite formation is not that friction can cause melting, but that it seems to form thick masses of it. Yet such thick masses ought to preclude melting by reducing the friction between sliding r… Show more

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Cited by 37 publications
(44 citation statements)
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“…Indeed, pseudotachylites have not been reported at Upheaval Dome. Pseudotachylite can be expected to form along a 1 mm think shear zone that is longer than 3 cm to 30 cm and has a shear strain of 3% to 10% [56]. The compactional deformation bands within the Wingate are typically several tens of centimeters in length and 1 mm to 3 mm in width.…”
Section: Discussionmentioning
confidence: 99%
“…Indeed, pseudotachylites have not been reported at Upheaval Dome. Pseudotachylite can be expected to form along a 1 mm think shear zone that is longer than 3 cm to 30 cm and has a shear strain of 3% to 10% [56]. The compactional deformation bands within the Wingate are typically several tens of centimeters in length and 1 mm to 3 mm in width.…”
Section: Discussionmentioning
confidence: 99%
“…Reimold and Gibson, 2005;Lieger et al, 2009). Moreover, although the total displacements and slip rates necessary to generate melt along a fault are easily achieved during crater formation, the volume of friction melt expected is very small (less than a few volume per cent) compared with the volume of collapsing material (Melosh, 2005). Hence, whether or not sufficient friction melt can be formed to lubricate crater collapse remains uncertain.…”
Section: Target Disintegration Into Blocksmentioning
confidence: 99%
“…Also, the mechanism(s) that produced the large thickness of clast-rich pseudotachylite zones remains to be identified. Single-slip events are unlikely to account for the observed thicknesses of pseudotachylite, as shear-induced melting on a shear fracture would reduce its friction and thus inhibit further melting by this process (Melosh 2005). As high slip rates over a longer time interval seem necessary to produce thick pseudotachylite zones, it is conceivable that the localized generation of clastrich pseudotachylite is genetically related to acoustic fluidization.…”
Section: Unsolved Structural Problemsmentioning
confidence: 99%