Petrogenesis of early cretaceous carbonatite and ultramafic lamprophyres in a diatreme in the Batain Nappes,Eastern Oman continental margin   总被引：1，自引：0，他引：1  

S. Nasir  S. Al-Khirbash  H. Rollinson  A. Al-Harthy  A. Al-Sayigh  A. Al-Lazki  T. Theye  H.-J. Massonne  E. Belousova 《Contributions to Mineralogy and Petrology》2011,161(1):47-74

Allochthonous carbonatite and ultramafic lamprophyre occur in a diatreme at the beach of the Asseelah village, northeastern Oman. The diatreme consists of heterogeneous deposits dominated by ‘diatreme facies’ pyroclastic rocks. These include aillikite and carbonatite, which intrude late Jurassic to early Cretaceous cherts and shales of the Wahra Formation within the Batain nappes. Both rock types are dominated by carbonate, altered olivine, Ti–Al–phlogopite and Cr–Al–spinel and contain varying amounts of apatite and rutile. The carbonatite occur as fine-grained heterolithic breccias with abundant rounded carbonatite xenoliths, glimmerite and crustal xenoliths. The aillikite consists of pelletal lapilli tuff with abundant fine-grained carbonatite autoliths and crustal xenoliths, which resemble those in the carbonatite breccia. The aillikite and carbonatite are characterized by low SiO₂ (11–24 wt%), MgO (9.5–12.4 wt%) and K₂O (<0.3 wt%), but high CaO (18–22 wt%), Al₂O₃ (4.75–7.04 wt%), Fe₂O_3tot (8.7–13.8 wt%) and loss-on-ignition (24–30 wt%). Higher CaO, Fe₂O_3total, Al₂O₃, MnO, TiO₂, P₂O₅ and lower SiO₂ and MgO content distinguish carbonatite from the aillikite. The associated carbonatite xenoliths and autoliths have intermediate composition between the aillikite and carbonatite. Mg number is variable and ranges between 58 and 66 in the carbonatite, 66 and 72 in the aillikite and between 48 to 64 in the carbonatite autoliths and xenoliths. The Asseelah aillikite, carbonatite, carbonatite xenoliths and autoliths overlap in most of their mineral parageneses, mineral composition and major and trace element chemistry and have variable but overlapping Sr, Nd and Pb isotopic composition, implying that these rocks are related to a common type of parental magma with variable isotopic characteristics. The Asseelah aillikite, carbonatite and carbonatites xenoliths are LREE-enriched and significantly depleted in HREE. They exhibit similar smooth, subparallel REE pattern and steep slopes with (La/Sm) _n of 6–10 and relative depletion in heavy rare earth elements (Lu = 3–10 chondrite). Initial ⁸⁷Sr/⁸⁶Sr ratios vary from 0.70409 to 0.70787, whereas initial ¹⁴³Nd/¹⁴⁴Nd ratios vary between 0.512603 and 0.512716 (εNd _i between 2.8 and 3.6). ²⁰⁶Pb/²⁰⁴Pb _i ratios vary between 18.4 and 18.76, ²⁰⁷Pb/²⁰⁴Pb _i ratios vary between 15.34 and 15.63, whereas ²⁰⁸Pb/²⁰⁴Pb _i varies between 38.42 and 39.05. Zircons grains extracted from the carbonatite have a mean age of 137 ± 1 Ma (95% confidence, MSWD = 0.49). This age correlates with large-scale tectonic events recorded in the early Indian Ocean at 140–160 Ma. Geochemical and isotopic signatures displayed by the Asseelah rocks can be accounted for by vein-plus-wall-rock model of Foley (1992) wherein veins are represented by phlogopite, carbonate and apatite and depleted peridotite constitutes the wall-rock. The carbonatite and aillikite magmatism is probably a distal effect of the breaking up of Gondwana, during and/or after the rift-to-drift transition that led to the opening of the Indian Ocean.  相似文献   

Geochemistry and petrology of Tertiary volcanic rocks and related ultramafic xenoliths from the central and eastern Oman Mountains     

Sobhi Nasir  Abdulrazak Al-Sayigh  Abdulrahman Alharthy  Ali Al-Lazki   《Lithos》2006,90(3-4):249-270

The Tertiary volcanic rocks of the central and the eastern parts of the Oman Mountains consist mainly of basanites with abundant upper mantle ultramafic xenoliths. The lavas are alkaline (42–43 wt.% SiO₂; 3.5–5.5 wt.% Na₂O + K₂O). They include primitive (11–14 wt.% MgO) features with strong OIB-like geochemical signatures. Trace element and Sr–Nd isotope data for the basanites suggest mixing of melts derived from variable degrees of melting of both garnet- and spinel lherzolite-facies mantle source. The associated xenolith suite consists mainly of spinel and Cr-bearing diopside wehrlite, lherzolite and dunite with predominantly granuloblastic textures. No significant difference in chemistry was found between the basanites and xenoliths from the central and eastern Oman Mountains, which indicate a similar mantle source. Calculated oxygen fugacity indicates equilibration of the xenoliths at − 0.43 to − 2.2 log units above the fayalite–magnetite–quartz (FMQ) buffer. Mantle xenolith equilibration temperatures range from 910–1045 + 50 °C at weakly constrained pressures between 13 and 21 kbar. Xenolith data and geophysical studies indicate that the Moho is located at a depth of  40 km. A geotherm substantially hotter (90 mW m^− 2) than the crust–mantle boundary (45 mW m^− 2) is indicated and probably relates to tectonothermal events associated with the local and regional Tertiary magmatism. The petrogenesis of the Omani Tertiary basanites is explained by partial melting of an asthenospheric mantle protolith during an extension phase predating opening of the Gulf of Aden and plume-related alkaline volcanic rocks.  相似文献