A once-molten, coarse-grained, Ca-rich inclusion in Allende

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Calcium, Carbonaceous Meteorites, Chemical Composition, Inclusions, Meteoritic Composition, Crystallization, Mineralogy, Oxygen Isotopes, Meteorites, Allende Meteorite, Inclusions, Melilite, Textures, Chemistry, Condensation, Grains, Crystallization, Radiation, Cooling, Oxygen, Isotopes, Formation, Chronology, Analysis, Techniques, Photographs, Mineralogy, Data, Electron Microprobe, Phases

Scientific paper

A compact, spheroidal Type B inclusion in Allende contains melilite laths that project radially inward from the inclusion edge which show interference growth textures. The combined textural and chemical features of this object cannot be explained by independent vapor-solid condensation of grains in space, followed by random aggregation of these grains into an inclusion. Instead, it probably formed from a once-molten droplet that crystallized in response to radiative cooling from its outer surface. The crystallization sequence in this and another similar inclusion in which oxygen isotopes have been measured is melilite-spinel-anorthite-fassaite; this sequence shows that oxygen isotopic heterogeneities in coarse-grained inclusions were formed after complete solidification of these objects by partial exchange with a less O-16-rich gas, and not during or before a melting event.

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