Impact-induced chondrule flattening in the Allende CV3 carbonaceous chondrite: Shock experiments

Details Impact-induced chondrule flattening in the Allende CV3 carbonaceous chondrite: Shock experiments Impact-induced chondrule flattening in the Allende CV3 carbonaceous chondrite: Shock experiments

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995metic..30..344n&link_type=abstract

Meteoritics, vol. 30, p. 344 (1995).

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We have carried out shock-recovery experiments on the Allende CV3 carbonaceous chondrite using a single- stage propellant gun and succeeded in reproducing oriented, flattened chondrules like those observed in some natural CV3 chondrites. The Allende samples were shocked at equilibrium pressures of 11 and 21 GPa, which are close to the highest values in shock stages S2 and S3, respectively (Stöffler et al., 1991). Chondrules are flattened nearly perpendicular to the compaction axis with mean aspect ratios of 1.34 and 1.62 at pressures of 11 and 21 GPa, respectively; thus, the degree of chondrule flattening is proportional to the shock intensity. The chondrule flattening and foliation are mainly due to collapse of pores in the matrix under shock pressure. High matrix abundance of CV3 chondrites could result in much apparent chondrule flattening relative to ordinary chondrites. Optical and electron microscope observations show that textural and mineralogical characteristics of chondrules and matrix in the shock-loaded samples are very similar to those observed in naturally shocked CV3 chondrites. Our results provide strong support for the interpretation that the chondrule flattening and foliation in CV3 chondrites were caused by shock-induced pressure due to hypervelocity impacts on the meteorite parent bodies.

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