Matches in SemOpenAlex for { <https://semopenalex.org/work/W3136304385> ?p ?o ?g. }
- W3136304385 endingPage "106125" @default.
- W3136304385 startingPage "106125" @default.
- W3136304385 abstract "Samples from three petrographically distinct, intrusive kimberlite bodies and associated kimberlite dykes from the eastern lobe of the Du Toitspan kimberlite pipe, Kimberley, South Africa, have been analysed for their bulk rock major and trace element compositions and their olivine and phlogopite compositions. The two dominant intrusive bodies (D13, D14) are distinguished by the one (D13) being phlogopite-rich and best classified as a macrocrystic hypabyssal phlogopite kimberlite, and the other (D14) being phlogopite-poor and best classified as a macrocrystic hypabyssal monticellite kimberlite. The minor D17 intrusive body is classified as a macrocrystic transitional hypabyssal serpentinized phlogopite kimberlite. The associated kimberlite dykes range texturally from aphanitic to macrocrystic and are classified as calcite kimberlites. The major kimberlite intrusions and their associated dykes show no evidence of crustal contamination and are characterised by broadly overlapping geochemistry except for distinctly higher K2O (> 2 wt%) and Al2O3 (>3 wt%) and flattening HREE patterns (Gd/YbN = 6.5–7.0) in the D13 – phlogopite kimberlite compared to the D14 – monticellite kimberlite and the calcite kimberlite dykes (Gd/YbN = 9.6–12.1). These distinguishing geochemical features of the D13 – phlogopite kimberlite are comparable to typical Group II kimberlites in southern Africa. However, their diagnostic incompatible trace element ratios (for example, Th/Nb, La/Nb, Ce/Pb, and Ba/Nb) are instead comparable to other kimberlite intrusions analysed in this study and to southern African Group I kimberlites in general. Semi-quantitative modelling suggests that these kimberlite intrusions could have derived by low (<1%) degrees of partial melting of a source region that is enriched in LREE (Lan = ~6.1; Ybn ~ 1.47) comparable to metasomatised peridotites from the underlying lithospheric mantle. The composition of the D13 phlogopite kimberlite is consistent with a partial melt of a modally metasomatised source containing a higher proportion of residual clinopyroxene relative to garnet (compared to that giving rise to the D14 monticellite kimberlite and calcite kimberlite dykes), as well as accessory amounts of phlogopite, i.e. a garnet phlogopite peridotite (GPP). The absence of K-anomalies on primitive mantle normalized diagrams for the D13 phlogopite kimberlite requires that phlogopite was not a residual phase during partial melting and was exhausted shortly before or at the moment of melt segregation. The higher Gd/Yb ratios and lower K2O in the D14 monticellite kimberlite and calcite kimberlite dykes can be explained by partial melting of a cryptically metasomatized, phlogopite – free, garnet peridotite (GP) source, containing a higher proportion of garnet relative to clinopyroxene. The low absolute K and strong negative K-anomaly on primitive mantle normalized diagrams for the D14 monticellite kimberlite were inherited from a source region that previously experienced cryptic metasomatism by a differentiated fluid already carrying a negative K-anomaly." @default.
- W3136304385 created "2021-03-29" @default.
- W3136304385 creator A5000514360 @default.
- W3136304385 creator A5074222144 @default.
- W3136304385 creator A5086906681 @default.
- W3136304385 date "2021-06-01" @default.
- W3136304385 modified "2023-09-27" @default.
- W3136304385 title "Phlogopite-rich and phlogopite-poor kimberlite intrusions within the Du Toitspan kimberlite pipe, South Africa: Petrogenetic relationships and localised source heterogeneity" @default.
- W3136304385 cites W1964041624 @default.
- W3136304385 cites W1968021533 @default.
- W3136304385 cites W1974656818 @default.
- W3136304385 cites W1976632769 @default.
- W3136304385 cites W1976788350 @default.
- W3136304385 cites W1978402924 @default.
- W3136304385 cites W1981711776 @default.
- W3136304385 cites W1988577050 @default.
- W3136304385 cites W1991965950 @default.
- W3136304385 cites W1993020314 @default.
- W3136304385 cites W1994520280 @default.
- W3136304385 cites W1999652704 @default.
- W3136304385 cites W2000169692 @default.
- W3136304385 cites W2020926877 @default.
- W3136304385 cites W2022197104 @default.
- W3136304385 cites W2027862110 @default.
- W3136304385 cites W2030433511 @default.
- W3136304385 cites W2030896910 @default.
- W3136304385 cites W2031894158 @default.
- W3136304385 cites W2034632918 @default.
- W3136304385 cites W2036540575 @default.
- W3136304385 cites W2042823735 @default.
- W3136304385 cites W2044078195 @default.
- W3136304385 cites W2044192993 @default.
- W3136304385 cites W2047680420 @default.
- W3136304385 cites W2054336385 @default.
- W3136304385 cites W2067504635 @default.
- W3136304385 cites W2069186333 @default.
- W3136304385 cites W2069879942 @default.
- W3136304385 cites W2075849098 @default.
- W3136304385 cites W2076511463 @default.
- W3136304385 cites W2082031187 @default.
- W3136304385 cites W2086210906 @default.
- W3136304385 cites W2096956171 @default.
- W3136304385 cites W2098071006 @default.
- W3136304385 cites W2103527049 @default.
- W3136304385 cites W2108348302 @default.
- W3136304385 cites W2110725824 @default.
- W3136304385 cites W2117071874 @default.
- W3136304385 cites W2124187529 @default.
- W3136304385 cites W2128847471 @default.
- W3136304385 cites W2133857316 @default.
- W3136304385 cites W2134786959 @default.
- W3136304385 cites W2136132741 @default.
- W3136304385 cites W2137289440 @default.
- W3136304385 cites W2138106109 @default.
- W3136304385 cites W2151586261 @default.
- W3136304385 cites W2152550713 @default.
- W3136304385 cites W2152895531 @default.
- W3136304385 cites W2153316475 @default.
- W3136304385 cites W2158909637 @default.
- W3136304385 cites W2159944708 @default.
- W3136304385 cites W2161423703 @default.
- W3136304385 cites W2165098324 @default.
- W3136304385 cites W2178718305 @default.
- W3136304385 cites W2281192504 @default.
- W3136304385 cites W2495585081 @default.
- W3136304385 cites W2530872012 @default.
- W3136304385 cites W2588114197 @default.
- W3136304385 cites W2732333591 @default.
- W3136304385 cites W2752217018 @default.
- W3136304385 cites W2790195753 @default.
- W3136304385 cites W2791335159 @default.
- W3136304385 cites W2791463551 @default.
- W3136304385 cites W2800797345 @default.
- W3136304385 cites W2887746132 @default.
- W3136304385 cites W2888716328 @default.
- W3136304385 cites W2907469324 @default.
- W3136304385 cites W2908255623 @default.
- W3136304385 cites W2982873563 @default.
- W3136304385 cites W3003730822 @default.
- W3136304385 cites W3012347654 @default.
- W3136304385 cites W3019256801 @default.
- W3136304385 cites W4254592414 @default.
- W3136304385 cites W905573843 @default.
- W3136304385 doi "https://doi.org/10.1016/j.lithos.2021.106125" @default.
- W3136304385 hasPublicationYear "2021" @default.
- W3136304385 type Work @default.
- W3136304385 sameAs 3136304385 @default.
- W3136304385 citedByCount "2" @default.
- W3136304385 countsByYear W31363043852021 @default.
- W3136304385 countsByYear W31363043852022 @default.
- W3136304385 crossrefType "journal-article" @default.
- W3136304385 hasAuthorship W3136304385A5000514360 @default.
- W3136304385 hasAuthorship W3136304385A5074222144 @default.
- W3136304385 hasAuthorship W3136304385A5086906681 @default.
- W3136304385 hasConcept C127313418 @default.
- W3136304385 hasConcept C17409809 @default.
- W3136304385 hasConcept C183282558 @default.
- W3136304385 hasConcept C2778882853 @default.