Crustal contamination and fluid/rock interaction in the carbonatites of Fuerteventura (Canary Islands, Spain): a C, O, H isotope study

Lithos ◽  
1998 ◽  
Vol 44 (3-4) ◽  
pp. 101-115 ◽  
Author(s):  
A. Demény ◽  
A. Ahijado ◽  
R. Casillas ◽  
T.W. Vennemann
1987 ◽  
Vol 96 (4) ◽  
pp. 455-464 ◽  
Author(s):  
A. P. Dickin ◽  
N. W. Jones ◽  
M. F. Thirlwall ◽  
R. N. Thompson

1987 ◽  
Vol 24 (1) ◽  
pp. 159-169 ◽  
Author(s):  
Joel D. Blum ◽  
Alex E. Blum ◽  
Terry E. Davis ◽  
John T. Dillon

Felsic plutonic rocks in the northwestern portion of the Ruby geanticline of north-central Alaska occur as two distinct rock suites: (1) silica-saturated monzonite and syenite and (2) silica-oversaturated granite. K–Ar mineral ages for each suite average 107 ± 6 Ma, and both suites plot along a single Rb–Sr whole-rock isochron that yields an age of 112 ± 4 Ma and an initial 87Sr/86Sr ratio of 0.70778 ± 0.00006. Whole-rock δ18O values range from + 6.75 to + 7.30‰. The two suites cannot be related by simple fractionation, yet they appear to have a chemically and isotopically similar parental magma. Based on chemical mixing calculations, observations of magma – wall-rock interaction and xenolith abundances, we suggest a model whereby a small amount of assimilation of siliceous wall rock by a portion of an originally silica-saturated magma caused an increase in silica saturation, which led to two distinct fractionation suites. The almost exactly silica-saturated composition and extremely high Sr concentrations indicate that the silica-saturated magma formed at high pressure. This evidence, combined with the initial 87Sr/86Sr ratio and δ18O values, leads us to suggest a lower crust or enriched mantle source for the magma. The silica-saturated suite may be representative of a parental magma that contributed to the melting of upper crustal siliceous wall rock throughout the Ruby geanticline. Whereas a small amount of crustal contamination led to the silica-oversaturated rocks that occur in the northwestern part of the Ruby geanticline, larger amounts of assimilation may have formed the largely anatectic granites of the same age that are found in the interior of the Ruby geanticline.


2008 ◽  
Vol 146 (2) ◽  
pp. 276-290 ◽  
Author(s):  
ADAR STEINITZ ◽  
YARON KATZIR ◽  
JOHN W. VALLEY ◽  
YARON BE'ERI-SHLEVIN ◽  
MICHAEL J. SPICUZZA

AbstractA multi-mineral oxygen isotope study sheds light on the origin, cooling and alteration of Late Neoproterozoic A-type granites in the Arabian–Nubian shield of southern Israel. The oxygen isotope ratio of zircon of the Timna monzodiorite, quartz syenite and alkaline granite are within the range of mantle zircon (δ18O(Zrn) = 5.3 ± 0.6‰, 2σ), supporting the co-genetic mantle-derived origin previously suggested based on geochemical data and similar ɛNd(T) values and U–Pb ages (610 Ma). Likewise, olivine norite xenoliths within the monzodiorite (δ18O(Ol) = 5.41 ± 0.07‰) may have formed as cumulate in a parent mantle-derived magma. Within the Timna igneous complex, the latest and most evolved intrusion, an alkaline granite, has the least contaminated isotope ratio (δ18O(Zrn) = 5.50 ± 0.02‰), whereas its inferred parental monzodiorite magma has slightly higher and more variable δ18O(Zrn) values (5.60 to 5.93‰). The small isotope variation may be accounted for either by small differences in the temperature of zircon crystallization or by minor contamination of the parent magma followed by shallow emplacement and intrusion by the Timna alkaline granite. The Timna alkaline granite evolved, however, from a non-contaminated batch of mantle-derived magma. The formation of Yehoshafat granite (605 Ma; δ18O(Zrn) = 6.63 ± 0.10‰), exposed ~30 km to the south of the mineralogically comparable Timna alkaline granite, involved significant contribution from supracrustal rocks. A-type granites in southern Israel thus formed by differentiation of mantle-derived magma and upper crustal melting coevally. Fast grain boundary diffusion modelling and measured quartz-zircon fractionations demonstrate that the Timna and Yehoshafat alkaline granites cooled very rapidly below 600 °C in accordance with being epizonal. One to three orders of magnitude slower cooling is calculated for 30 Ma older calc-alkaline granites of the host batholith, indicating a transition from thick orogenic to extended crust. Significant elevation of the δ18O of feldspars occurred through water–rock interaction at moderate temperatures (100–250 °C), most probably during a thermal event in Early Carboniferous times.


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