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The evolution of enstatite and chondrules in unequilibrated enstatite chondrites: Evidence from iron‐rich pyroxene
Author(s) -
Weisberg Michael K.,
Prinz Martin,
Fogel Robert A.
Publication year - 1994
Publication title -
meteoritics
Language(s) - English
Resource type - Journals
eISSN - 1945-5100
pISSN - 0026-1114
DOI - 10.1111/j.1945-5100.1994.tb00599.x
Subject(s) - enstatite , chondrule , pyroxene , chondrite , geology , geochemistry , olivine , mineralogy , meteorite , astrobiology , physics
Abstract— FeO‐rich (Fs 6–34 ) pyroxene lacking cathodoluminescence (CL), hereafter black pyroxene, is a major constituent of some of the chondrules and fragments in unequilibrated (type 3) enstatite chondrites (UECs). It contains structurally oriented zones of Cr‐, Mn‐, V‐rich, FeO‐poor enstatite with red CL, associated with mm‐sized blebs of low‐Ni, Fe‐metal and, in some cases, silica. These occurrences represent clear evidence of pyroxene reduction. The black pyroxene is nearly always rimmed by minor element (Cr, Mn, V)‐poor enstatite having a blue CL. More commonly, red and blue enstatites, unassociated with black pyroxene, occur as larger grains in chondrules and fragments, and these constitute the major silicate phases in UECs. The REE abundance patterns of the black pyroxene are LREE‐depleted. The blue enstatite rims, however, have a near‐flat to LREE‐enriched pattern, ∼0.5–4x chondritic. The petrologic and trace element data indicate that the black pyroxene is from an earlier generation of chondrules that formed in a nebular region that was more oxidizing than that of the enstatite chondrites. Following solidification, these chondrules experienced a more reducing nebular environment and underwent reduction. Some, perhaps most, of the red enstatite that is common throughout the UECs may be the product of solid‐state reduction of black pyroxene. The blue enstatite rims grew onto the surfaces of the black pyroxene and red enstatite as a result of condensation from a nebular gas. The evolutionary history of some of the enstatite and chondrules in enstatite chondrites can be expressed in a four‐stage model that includes: Stage 1. Formation of chondrules in an oxidizing nebular environment Stage 2. Solid‐state reduction of the more oxidized chondrules and fragments to red enstatite in a more reducing nebular environment Stage 3. Formation of blue enstatite rims on the black pyroxene as well as on the red enstatite. Stage 4. Reprocessing, by various degrees of melting, of many of the earlier‐formed materials.