Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998m%26ps...33.1303h&link_type=abstract
Meteoritics & Planetary Science, vol. 33, no. 6, pp. 1303-1309.
Astronomy and Astrophysics
Astronomy
2
Scientific paper
Optical and SEM observations of hematite impact bombs from the Araguainha astrobleme (central Brazil) reveal an aerodynamically stable microstructure, which was interpreted to reflect the aerial crystallization of hypervelocity melt globules derived from Fe-rich sedimentary target rocks. The bombs are composed of an aggregate of preferentially oriented conic units with different degrees of packing, giving rise to porous and massive hematite varieties. These varieties generally occupy the front and rear of the bombs, respectively. Quartz fragments with planar deformation features are common in the porous domains, and are interpreted to represent ejected solid particles captured by the bombs during cooling. The absence of typical contorted shapes in these bombs is suggested to reflect the lack of spin during their ballistic trajectory. The bombs are enriched in Rh (4?), Ru, Ir and Pd (5?) and Pt (>30?) relative to the indigenous level of target sediments suggesting the presence of a projectile-derived component in their constitution. Single composition oxidic bombs (pure hematite and pure silica) predominate in this occurrence, indicating that a mechanism of segregation has operated in the ejected melt volumes.
Hippertt J.
Lana Cristiano
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