Pregraphitic and poorly graphitised carbons in porous chondritic micrometeorites

Details Pregraphitic and poorly graphitised carbons in porous chondritic micrometeorites Pregraphitic and poorly graphitised carbons in porous chondritic micrometeorites

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992gecoa..56.1665r&link_type=abstract

Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 56, April 1992, p. 1665-1671.

Computer Science

6

Carbonaceous Chondrites, Interplanetary Dust, Meteoritic Composition, Meteoritic Microstructures, Micrometeorites, Asteroid Belts, Comets, Dust Collectors, Earth Atmosphere, Porous Materials

Scientific paper

Two forms of crystalline carbon in porous chondritic micrometeorites W7029E5, U2011C2, and U2022C7/C8 are mixed layered pregraphitic carbons with C/(C+H+O+N) (at. pct) about 0.45. This bulk composition is inferred from the presence of three groupings of d(002) basal spacings at 0.45 nm, 0.37 nm, and 0.348 nm. Mixed layered carbons represent incomplete carbonization and graphitization of precursor material. In U2022C7/C8, carbonization mostly involved volatile loss. The formation of pregraphitic carbons indicates a sustained thermal regime in parent bodies of these micrometeorities (i.e., short-period comets, outer-belt asteroids, or protocomet nuclei). Temperatures of the sustained thermal regime remain unspecified, but carbon reactions were probably facilitated by catalytic support from layer silicates in these samples. Poorly graphitized carbon in U2022C7/C8 formed during a transient thermal event which is most likely flash-heating during micrometeoroid deceleration in the earth's atmosphere.

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