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- W1593722503 abstract "Introduction: Chondrules and refractory inclusions [Ca, Al-rich inclusions (CAIs) and amoeboid olivine aggregates (AOAs)] are the major high temperature components of chondritic meteorites formed during transient heating events in the inner solar nebula. Mineralogical, chemical, and isotopic observations, and thermodynamic analysis suggest that refractory inclusions formed in an 16 O-rich (∆ 17 O ~ -20‰) gaseous reservoir at low total pressure (<10 -4 bar) and high ambient temperatures (near or above the condensation temperatures of forsterite; ~1300 K), and were subsequently isolated (physically or kinetically) from reactions with the high temperature nebular gas [1-6]. Gassolid reactions (evaporation-condensation) appear to have been the dominant processes during formation of refractory inclusions. Some CAIs (mostly in CV chondrites) experienced extensive melting accompanied by evaporation and mass-dependent isotopic fractionation of Mg and Si [7,8]. Both igneous and non-igneous CAIs are surrounded by 16 O-rich multilayered rims (called Wark-Lovering rims) with the outermost layers, composed of Al-diopside and forsterite, formed by gas-solid condensation [9]. Most CAIs show large 26 Mg excesses ( 26 Mg*) corresponding to an initial 26 Al/ 27 Al ratio" @default.
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- W1593722503 date "2004-11-01" @default.
- W1593722503 modified "2023-09-27" @default.
- W1593722503 title "THE GENETIC RELATIONSHIP BETWEEN REFRACTORY INCLUSIONS AND CHONDRULES. A. N." @default.
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