T139 Melt in the Crust and Upper Mantle: How Much, Where, for How Long, and What Significance for Geodynamics? (Posters)
Wednesday, 7 November 2001
1:30 PM - 5:30 PM
VISCOUS EMULSION DIFFERENTIATION OF SUPERHEATED IMPACT MELT SHEETS
Paper number: T139-19
Program: Technical Sessions
Time: 1:30 PM – 5:30 PM
Authors
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Bruce D. MarshJohns Hopkins Univ, Baltimore, MD
Abstract
Initially, the melt sheet was superheated and underwent vigorous thermal convection that homogenized both layers and cooled the magma down to its liquidus. Additional cooling was conductive, with the norite cooling from the base up and the granophyre cooling from the top down. The interface between the norite and granophyre, which is geochemically and mineralogically distinct, was the last to cool below the solidus. During the final stages of solidification, different types of foreign debris were "frozen" into the melt sheet. The debris includes blocks of granite that floated into the norite from the crater floor as well as remobilized fallback breccia that foundered and sank into the granophyre.
The emulsion model explains the geochemistry of the SIC, the presence of exotic rock types in the center of the complex, and also the textural variations through the norite. Impact melting is a process that was common during early Earth history and is capable of maximizing igneous diversity by concentrating preexisting heterogeneity.