2011
DOI: 10.1556/ceugeol.54.2011.3.2
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Ringwoodite microstructures in L-chondrite NWA 5011: implications for transformation mechanism and source region in L parent body

Abstract: Ringwoodite, produced by shock metamorphism, is common in and adjacent to melt veins in highly shocked chondrites. Although ringwoodite can be crystallized from the silicate melt in the shock-veins or pockets, a major part of the easily observed ringwoodite in shock veins is formed by the transformation of olivine in host-rock fragments entrained in the melt or olivine along shock-vein margins. In this paper we examine the microstructures and textures of ringwoodites from NWA 5011 L-chondrite in order to bette… Show more

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Cited by 8 publications
(4 citation statements)
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References 18 publications
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“…The samples analysed in the present study have a deep royal blue colouration, typical of iron-bearing hydrous ringwoodites. The origin of blue colouration in ringwoodite and other high-pressure ferromagnesian silicates is currently uncertain, having been attributed to light scattering (e.g., Lingemann and Stöffler, 1998;Nagy et al 2011), or intervalence charge transfer (e.g., Taran et al 2009). Iron-bearing magnesian ringwoodite can vary in colour from colourless through pale green to deep blue/purple.…”
Section: Discussionmentioning
confidence: 99%
“…The samples analysed in the present study have a deep royal blue colouration, typical of iron-bearing hydrous ringwoodites. The origin of blue colouration in ringwoodite and other high-pressure ferromagnesian silicates is currently uncertain, having been attributed to light scattering (e.g., Lingemann and Stöffler, 1998;Nagy et al 2011), or intervalence charge transfer (e.g., Taran et al 2009). Iron-bearing magnesian ringwoodite can vary in colour from colourless through pale green to deep blue/purple.…”
Section: Discussionmentioning
confidence: 99%
“…In order to confirm their hypothesis, more investigation should be conducted on the meteoritic Rw, which represents the best natural specimen for studying high-P structural features, including the Mg-Si order-disorder state, due to its having much larger quench rates. Rw of various colors has been documented in many meteorites, including L ordinary chondrites [108][109][110][111][112], LL ordinary chondrites [14,26], and Martian meteorites like the shergottites [32,34,37]. If the relationship among the color, composition, inverse magnitude, P and T can be adequately quantified, a fine scale for accurately estimating the shock P-T conditions may be derived, which may serve well the theoretical evolution models of the early solar system.…”
Section: Discussionmentioning
confidence: 99%
“…ЛИТАСОВ, БАДюКОВ ные обломки первичных минералов, полностью преобразованных в высокобарические фазы (за исключением хромита). Текстура более крупных образцов метеорита NWA 5011 исследована в работе (Nagy et al, 2011), где отмечается, что максимальные размеры зерен оливина в зернистой матрице достигают 10 мм, а размер хондрул находится в пределах 0.5-4.0 см. Составы минералов хондрита NWA 5011 приведены в табл.…”
Section: Chrunclassified