1990
DOI: 10.1016/0016-7037(90)90128-8
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Calculation of simultaneous isotopic and trace element variations during water-rock interaction with applications to carbonate diagenesis

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Cited by 999 publications
(527 citation statements)
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“…Burial diagenesis can result in signatures that are similar to carbonates influenced by meteoric diagenesis because temperature increases with burial and carbonates (such as metastable aragonite and high-magnesium calcite) are susceptible to recrystallization over time (Sandberg, 1975). However, fluid isotope compositions at depth (confounded by varying degrees of rock buffering; e.g., Banner and Hanson, 1990) may be quite different from those of surface environments, therefore carbonates forming in a burial environment may exhibit a wide range in ␦ 18 O carb extending to both negative and positive extremes. As a result, interpreting the ␦ 18 O carb of ancient rocks as resulting from primary marine precipitation, meteoric diagenesis or burial diagenesis has remained a longstanding problem in carbonate geochemistry.…”
Section: Introductionmentioning
confidence: 99%
“…Burial diagenesis can result in signatures that are similar to carbonates influenced by meteoric diagenesis because temperature increases with burial and carbonates (such as metastable aragonite and high-magnesium calcite) are susceptible to recrystallization over time (Sandberg, 1975). However, fluid isotope compositions at depth (confounded by varying degrees of rock buffering; e.g., Banner and Hanson, 1990) may be quite different from those of surface environments, therefore carbonates forming in a burial environment may exhibit a wide range in ␦ 18 O carb extending to both negative and positive extremes. As a result, interpreting the ␦ 18 O carb of ancient rocks as resulting from primary marine precipitation, meteoric diagenesis or burial diagenesis has remained a longstanding problem in carbonate geochemistry.…”
Section: Introductionmentioning
confidence: 99%
“…5), suggesting post-depositional alteration related to dolomitization processes, and thus resulting in a decrease of δ 13 C, as well as an increase in the Mn/Sr and Fe/Sr ratios like suggested by Brand and Veizer (1980). However, Banner and Hanson (1990) proposed that δ 18 O values decrease during post-depositional alteration too, but, in this case, the δ 18 O values show a behavior of rising (Fig. 5).…”
Section: And O Isotopic Variationsmentioning
confidence: 96%
“…Recognition of post-depositional alteration processes is extremely important to ensure the reliable application of C isotopic chemostratigraphy (Melezhik et al, 2001). According to Brand and Veizer (1980) and Banner and Hanson (1990), the interaction of carbonates with interstitial fluids during diagenesis, dolomitization or metamorphism leads to an increase in the Rb/Sr, Mn/Sr, Fe/Sr and 87 Sr/ 86 Sr ratios, Note: n.a.= not analyzed. and a decrease in the δ 13 C and δ 18 O values.…”
Section: And O Isotopic Variationsmentioning
confidence: 99%
“…Pre vi ous stud ies have dem on strated that shal low ma rine car bon ates d 13 C val ues are not readily af fected by diagenetic al ter ations (Ban ner and Hanson, 1990). Con versely, d 18 O values of ma rine car bon ate rocks are eas ily in flu enced by burial and me te oric diagenesis (Brand and Veizer, 1981;Brand, 2004).…”
Section: Geochemical Signatures Of Meteoric Diagenesismentioning
confidence: 99%
“…The in verted J-curve de lin eated by Musayr sam ples is in dica tive of diagenetic al ter ation gov erned by vari able de grees of fluid-rock in ter ac tion and me te oric or i gin of diagenetic flu ids (e.g., Meyers and Lohmann, 1985;Lohmann, 1988;Ban ner and Hanson, 1990). This in verted trend may be as so ci ated with dif fer ent iso to pic equil i bra tion be tween car bon ate com po nents and diagenetic flu ids at low fluid rock in ter ac tions (Bishop et al, 2014; Fig.…”
Section: Geochemical Signatures Of Meteoric Diagenesismentioning
confidence: 99%