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THE CLOVIS (no. 1), NEW MEXICO, METEORITE AND Ca, Al AND Ti‐RICH INCLUSIONS IN ORDINARY CHONDRITES
Author(s) -
Noonan Albert F.
Publication year - 1975
Publication title -
meteoritics
Language(s) - English
Resource type - Journals
eISSN - 1945-5100
pISSN - 0026-1114
DOI - 10.1111/j.1945-5100.1975.tb00007.x
Subject(s) - chondrite , chondrule , geology , breccia , meteorite , pyroxene , olivine , geochemistry , mineralogy , carbonaceous chondrite , astrobiology , physics
Microprobe analyses of the major silicates in Clovis (no. 1), New Mexico, establish it as an H3 chondrite. Inclusions identified in Clovis are: breccia fragments; angular and vesicular chondrule or rock fragments composed almost entirely of glass and olivine (Fa 12–22 ); chondrules, composed principally of pyroxene (Fs 2–33 ) and olivine (Fa 1–28 ); and Ca, Al and Ti‐rich inclusions. These refractory enriched inclusions, similar in composition to those found in some carbonaceous chondrites, are rare in ordinary chondrites but in this study were observed in Sharps, Virginia (H3), Gobabeb, South Africa (H4), Dimmitt, Texas (H4), Weston, Connecticut (H4–6) and Clovis. Sodium, known to rim similar inclusions in carbonaceous chondrites, also occurs in the interiors of inclusions observed in this study, sometimes in moderate amounts. The Na distribution is regarded as primary and is not attributable, at least in total, to secondary Na extraction from the host matrix.