2006
DOI: 10.2138/am.2006.2061
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A shock-induced polymorph of anatase and rutile from the Chesapeake Bay impact structure, Virginia, U.S.A.

Abstract: A shock-induced polymorph (TiO 2 II) of anatase and rutile has been identifi ed in breccias from the late Eocene Chesapeake Bay impact structure. The breccia samples are from a recent, partially cored test hole in the central uplift at Cape Charles, Virginia. The drill cores from 744 to 823 m depth consist of suevitic crystalline-clast breccia and brecciated cataclastic gneiss in which the TiO 2 phases anatase and rutile are common accessory minerals. Electron-microprobe imaging and laser Raman spectroscopy of… Show more

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Cited by 35 publications
(21 citation statements)
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“…However, our experiments show that even at pressures of 10-23 GPa and temperatures of 1 500-1 800 ℃, SiO 2 solubility in rutile is still quite limited, with a maximum of 5.3 wt.% at 2 000 ℃ and 23 GPa, much lower than the high Si-rutile reported by Yang et al (2003). In nature, rutiles formed at ultrahigh pressures in metamorphic belts (Hwang et al, 2000) and shocked craters (Jackson et al, 2006;Goresy et al, 2001a, b) have structures similar to α-PbO 2 and ZrO 2 phases. They are all believed to form at high pressures but low temperatures (T<1 000 ℃ ).…”
Section: Discussionmentioning
confidence: 50%
“…However, our experiments show that even at pressures of 10-23 GPa and temperatures of 1 500-1 800 ℃, SiO 2 solubility in rutile is still quite limited, with a maximum of 5.3 wt.% at 2 000 ℃ and 23 GPa, much lower than the high Si-rutile reported by Yang et al (2003). In nature, rutiles formed at ultrahigh pressures in metamorphic belts (Hwang et al, 2000) and shocked craters (Jackson et al, 2006;Goresy et al, 2001a, b) have structures similar to α-PbO 2 and ZrO 2 phases. They are all believed to form at high pressures but low temperatures (T<1 000 ℃ ).…”
Section: Discussionmentioning
confidence: 50%
“…We can assume that in our TiO 2 :Er material, erbium induces a slight structural deformation which gives origin to new Raman bands in a similar way as in Refs. [21] and [23].…”
Section: Resultsmentioning
confidence: 99%
“…The formation of natural TiO 2 -II could be related to highpressure endogenic geological processes or bolide impact events. Occurrence of natural TiO 2 -II had been previously reported in ultrahigh-pressure metamorphic rocks [11,12], mantle-derived rocks [13], terrestrial impact structures [14][15][16], and tektite [17]. However, the mineralogical features and the formation conditions of natural TiO 2 -II still needs to be further investigated because of the very limited material that had been found.…”
mentioning
confidence: 99%