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Bulk compositions were determined by broad-beam electron microprobe analysis for thirteen of the least aqueously altered chondrules in Murray (CM2). These and literature data reveal compositional differences between CM-CO and ordinary chondrite (OC) chondrules:
  • 1.(a) CO chondrules are richer in refractory lithophiles and poorer in Cr, Mn and volatile lithophiles than OC chondrules; much lower refractory lithophile abundances in CM chondrules resulted from aqueous alteration,
  • 2.(b) in CM-CO chondrites, abundances of refractory lithophiles are higher in nonporphyritic than porphyritic chondrules, whereas in H-L-LL3 chondrites the converse is true,
  • 3.(c) Cr ranges are greater and Cr and Mn correlate more strongly in chondrules in CM-CO than in H-L-LL3 chondrites.
We find evidence for two important lithophile precursor components of CM-CO chondrite chondrules:
  • 1.(1) pyroxene- and refractory-rich, FeO-poor;
  • 2.(2) olivine-rich, refractory and FeO-poor.
The occurrence of a few FeO-rich chondrules attests to a third component similar to matrix: olivine- and FeO-rich, refractories not characterized. The first two components differ from those inferred for OC chondrules, consistent with formation at different locations. The pyroxene- and refractory-rich, FeO-poor lithophile precursor component probably formed by an incomplete evaporation of presolar silicates that brought these materials into the enstatite stability field.  相似文献   

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