LOW-CA PYROXENES FROM LL-GROUP CHONDRITIC METEORITES - CRYSTAL STRUCTURAL STUDIES AND IMPLICATIONS FOR THEIR THERMAL HISTORIES

Citation
G. Artioli et G. Davoli, LOW-CA PYROXENES FROM LL-GROUP CHONDRITIC METEORITES - CRYSTAL STRUCTURAL STUDIES AND IMPLICATIONS FOR THEIR THERMAL HISTORIES, Earth and planetary science letters, 128(3-4), 1994, pp. 469-478
Citations number
47
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
0012821X
Volume
128
Issue
3-4
Year of publication
1994
Pages
469 - 478
Database
ISI
SICI code
0012-821X(1994)128:3-4<469:LPFLCM>2.0.ZU;2-A
Abstract
Crystal structural refinements of one orthorhombic (Pbca) and two mono clinic (P2(1)/c) single crystals, from chondrules of low-Ca pyroxenes from unequilibrated chondritic meteorites of the LL group, were carrie d out. The intracrystalline Fe-Mg distribution between the M1 and M2 c rystallographic sites of the Parnallee (LL-3) orthoenstatite is sugges tive of very rapid cooling, whereas both the structural state and intr acrystalline Fe-Mg distribution in the Soko Banja (LL-4) and Jolomba ( LL-6) clinoenstatites indicate rapid cooling from the high temperature polymorphs, with no significant re-equilibration at lower temperature s. These results imply that thermal metamorphism in the parent body, i f present, was insufficient to allow re-equilibration of the pyroxene minerals to low temperature, ordered crystal structures. The data also indicate that, assuming low or mild pressure and shock effects, there is no well defined correlation between equilibrium temperature of the mineral phases and the alleged petrologic type of the meteorites. Thi s evidence is consistent with a rubble pile model for the parent body accretional history, or with an onion shell model with very low therma l peak metamorphism, as is assumed for a very small object.