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Rapid continental breakup and microcontinent formation in the western Indian Ocean

Jenny CollierImperial College, U.KT. A. MinshullSouthampton University U.KJ. M. KendallLeeds University, U.KR. B. WhitmarshSouthampton University U.KGeorg RümpkerGFZ, Potsdam, GermanyP. JosephSeychelles National Oil Company, SeychellesPatrick J SamsonSeychelles National Oil Company, SeychellesC. I. LaneSouthampton University U.KV. SansomImperial College, U.KPieter VermeeschImperial College, U.KJ. O. S. HammondLeeds University, U.KJames WookeyLeeds University, U.KN. A. TeanbyLeeds University, U.KT. RybergGFZ, Potsdam, GermanyS. M. DeanSouthampton University U.K
2004en
ABI

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Two of the main factors that determine the nature of a rifted continental margin are rheology and magmatism during extension. Numerical models of lithospheric extension suggest that both factors vary with extension rate; yet until now extension rates of studied margins, as indicated by the rate of initial seafloor spreading, are mostly less than ‐30 mm/yr on each margin. This article presents the first geophysical results from the Seychelles‐Laxmi Ridge conjugate pair of rifted margins which separated at ‐65 mm/yr. The Seychelles, with its spectacular exposures of Precambrian granite, was the earliest scientifically recognized microcontinent and arguably remains the classic example of one [ Wegener, 1924; Matthews and Davies, 1966]. However, it is still unknown whether microcontinents result from plumes, changes in plate‐boundary forces, lithospheric heterogeneity, or a combination of these factors.

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