Melt production in large-scale impact events: Implications and observations at terrestrial craters

Details Melt production in large-scale impact events: Implications and observations at terrestrial craters Melt production in large-scale impact events: Implications and observations at terrestrial craters

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992lmip.conf...32g&link_type=abstract

In Lunar and Planetary Inst., International Conference on Large Meteorite Impacts and Planetary Evolution p 32-33 (SEE N93-10112

Computer Science

Hypervelocity Impact, Impact Melts, Meteorite Collisions, Meteorite Craters, Chondrites, Depth, Diameters, Feldspars, Glass, Granite, Melting, Quartz, Shock Loads, Topography

Scientific paper

The volume of impact melt relative to the volume of the transient cavity increases with the size of the impact event. Here, we use the impact of chondrite into granite at 15, 25, and 50 km s(sup -1) to model impact-melt volumes at terrestrial craters in crystalline targets and explore the implications for terrestrial craters. Figures are presented that illustrate the relationships between melt volume and final crater diameter D(sub R) for observed terrestrial craters in crystalline targets; also included are model curves for the three different impact velocities. One implication of the increase in melt volumes with increasing crater size is that the depth of melting will also increase. This requires that shock effects occurring at the base of the cavity in simple craters and in the uplifted peaks of central structures at complex craters record progressively higher pressures with increasing crater size, up to a maximum of partial melting (approx. 45 GPa). Higher pressures cannot be recorded in the parautochthonous rocks of the cavity floor as they will be represented by impact melt, which will not remain in place. We have estimated maximum recorded pressures from a review of the literature, using such observations as planar features in quartz and feldspar, diaplectic glasses of feldspar and quartz, and partial fusion and vesiculation, as calibrated with estimates of the pressures required for their formation. Erosion complicates the picture by removing the surficial (most highly shocked) rocks in uplifted structures, thereby reducing the maximum shock pressures observed. In addition, the range of pressures that can be recorded is limited. Nevertheless, the data define a trend to higher recorded pressures with crater diameter, which is consistent with the implications of the model. A second implication is that, as the limit of melting intersects the base of the cavity, central topographic peaks will be modified in appearance and ultimately will not occur. That is, the peak will first develop a central depression, due to the flow of low-strength melted materials, when the melt volume begins to intersect the transient-cavity base.

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