Processing of refractory meteorite inclusions (CAIs) in parent-body atmospheres

Computer Science

Scientific paper

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Aluminum Compounds, Atmospheric Composition, Calcium Compounds, Meteoritic Composition, Refractory Materials, Asteroids, Inclusions, Primitive Earth Atmosphere, Meteorites, Refractory Material, Inclusions, Cais, Parent Bodies, Dust, Atmosphere, Thermal Effects, Melting, Deceleration, Gases, Density, Formation, Origin, Mineralogy, Diagrams, Photomicrographs, Models, Calculations, Heating, Timescale

Scientific paper

Ca-Al-rich inclusions (CAIs) in refractory meteorites are shown to have been subject to partial melting during a suitably high gas density/small scale height regime arising during gasdynamic deceleration in a temporary atmosphere around an accreting parent body. The presence of dust in such an atmosphere would have increased the pressure gradient with height, lowering the boil-off rate, and permitting dust particles to become trapped in the partially melted material. CAIs may therefore be studied as probes of a primitive atmosphere.

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