2019
DOI: 10.1111/sed.12559
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Dolomite dissolution: An alternative diagenetic pathway for the formation of palygorskite clay

Abstract: Palygorskite is a fibrous, magnesium-bearing clay mineral commonly associated with Late Mesozoic and Early Cenozoic dolomites. The presence of palygorskite is thought to be indicative of warm, alkaline fluids rich in Si, Al and Mg. Palygorskite has been interpreted to form in peritidal diagenetic environments, either as a replacement of detrital smectite clay during a dissolutionprecipitation reaction or solid-state transformation, or as a direct precipitate from solution. Despite a lack of evidence, most diag… Show more

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Cited by 25 publications
(21 citation statements)
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“…Dolomite dissolution obviously followed dolomitization, and the presence of authigenic palygorskite ( Fig. 7A; see also Ryan et al, 2019) and calcite ( Fig. 8) in the dissolved cores of many dolomite crystals indicates that dolomite dissolution is concurrent with or pre-dates these phases.…”
Section: Paragenesis Interpretationmentioning
confidence: 93%
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“…Dolomite dissolution obviously followed dolomitization, and the presence of authigenic palygorskite ( Fig. 7A; see also Ryan et al, 2019) and calcite ( Fig. 8) in the dissolved cores of many dolomite crystals indicates that dolomite dissolution is concurrent with or pre-dates these phases.…”
Section: Paragenesis Interpretationmentioning
confidence: 93%
“…The fifth diagenetic event was the formation of palygorskite, which was previously interpreted by Ryan et al (2019) to be a replacement of smectite that in turn formed from Mg liberated by the dissolution of dolomite. This clay occurs both as an intercrystalline cement and as an intracrystalline cement inside of partially to completely dissolved dolomite cores.…”
Section: Paragenesis Interpretationmentioning
confidence: 98%
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“…Meteoric diagenesis is also important to the evolution of matrix-scale poresystems in rocks that have undergone dolomitization. Examples include 'dedolomitization' or the replacement of dolomite by calcite (Frank, 1981;Kupecz et al, 1993;Nader et al, 2008;Rameil, 2008;Vandeginste & John, 2012) commonly in the presence of calcium sulphate dissolution (Von Morlot, 1847;Bischoff et al, 1994;Arenas et al, 1999;Hauck et al, 2018) and the formation of hollow dolomite rhombs (Jones et al, 1989;Youssef, 1997;Ryan et al, 2019). Dolomite dissolution in the meteoric realm has also been implicated in the formation of dolomitic sediment variably referred to as 'pulverulent chalk' (Blank & Tynes, 1965), 'pulverulite' (Rose, 1972;Chafetz & Butler, 1980;Kahle, 2012), 'crushed dolomite' (Zogovi c, 1966), 'flour dolomite' (Ji et al, 2004), 'dolomite powder' (Machel et al, 2012), 'dolomite silt' (Hajna, 2003), 'dolomite sand' (James et al, 1993;Richter et al, 2018) and 'disintegrated dolomite' (Richter et al, 2018).…”
Section: Introductionmentioning
confidence: 99%