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Detailed Reference Information |
Peters, T. and Mercolli, I. (1998). Extremely thin oceanic crust in the Proto-Indian Ocean: Evidence from the Masirah Ophiolite, Sultanate of Oman. Journal of Geophysical Research 103: doi: 10.1029/97JB02674. issn: 0148-0227. |
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The Masirah Ophiolite is a good example of thin oceanic crust. Below pillow lavas and a sheeted dike complex with a relatively normal thickness of 1--1.5 km, the gabbroic lower crust barely exceeds 500 m in thickness. In spite of this reduced thickness, the oceanic crust preserves all members of a model ophiolite in a coherent lithostratigraphic sequence. The crust was formed during the uppermost Jurassic (circa 150 Ma) when the Indian-Madagascar plate separated from the African-Arabian plate and is therefore related to the opening of the coeval Somali basin. Geological relationships indicate that this portion of oceanic crust was formed at a ridge-transform intersect. The peculiarly reduced thickness of the gabbro layer is interpreted as the result of a weak magma supply at the edge of a ridge segment, rather than the consequence of a tectonic thinning. The cooling effect due to the vicinity of two large continental lithospheric blocks (Indian-Madagascar and African-Arabian plates) during this initial stage of the oceanization might have been an additional factor contributing to the reduction of the crustal thickness. ¿ 1998 American Geophysical Union |
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Abstract |
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Keywords
Marine Geology and Geophysics, Midocean ridge processes, Tectonophysics, Plate boundary—general, Marine Geology and Geophysics, Plate tectonics |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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