Abstract
The two main diamond associations are either of eclogitic or peridotitic mineralogy, exemplified by inclusions in diamond or rocks in which diamond has formed, notably xenoliths in kimberlites. Outside cratonic areas where kimberlites typically occur, diamonds have been recorded in alpine peridot-ites and gravels associated with them. Graphite pseudomorphs after di-amonds occur in the Beni Bousera peridotite massif (Kornprobst, 1969) within garnet pyroxenites or eclogites (Slodkevich, 1980b). They have cubic morphology and contain cpx inclusions of high pressure cubo-octahedral morphology similar to those in natural diamonds. They possess isotopically light δ13C values. The garnet pyroxenites have similar mineralogy to diamond bearing eclogite xenoliths and have a wide oxygen isotope variation (δ18O= 4.9 to 9.3%) – much greater than that of the associated peridotites.
They are believed to represent portions of hydrothermally altered sub-ducted oceanic lithosphere that resided at great depth (≫ diamond stability limit) before diapiric uprise and final cumulate segregation. The evolution of these rocks is compared with that of the sparsely diamondiferous alpine peridotites which probably have a simpler and shorter subduction history to relatively shallow depths.
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Nixon, P.H., Pearson, D.G., Davies, G.R. (1991). Diamonds: the Oceanic Lithosphere connection with Special Reference to Beni Bousera, North Morocco. In: Peters, T., Nicolas, A., Coleman, R.G. (eds) Ophiolite Genesis and Evolution of the Oceanic Lithosphere. Petrology and Structural Geology, vol 5. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3358-6_15
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DOI: https://doi.org/10.1007/978-94-011-3358-6_15
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