Incompletely compacted equilibrated ordinary chondrites

    Authors

    M. R. Sasso; R. J. Macke; J. S. Boesenberg; D. T. Britt; M. L. Rivers; D. S. Ebel;J. M. Friedrich

    Abbreviated Journal Title

    Meteorit. Planet. Sci.

    Keywords

    POROSITY; METEORITES; DENSITY; SHOCK; COLLECTION; ASTEROIDS; Geochemistry & Geophysics

    Abstract

    We document the size distributions and locations of voids present within five highly porous equilibrated ordinary cliondrites using high-resolution synchrotron X-ray microtomography (mu CT) and helium pycnometry. We found total porosities ranging from similar to 10 to 20% within these chondrites, and with mu CT we show that tip to 64% of the void space is located within intergranular voids within the rock. Given the low (S1-S2) shock stages of the samples and the large voids between mineral grains, we conclude that these samples experienced Unusually low amounts of compaction and shock loading throughout their entire post accretionary history. With Fe metal and FeS metal abundances and grain size distributions, we show that these chondrites formed naturally with greater than average porosities prior to parent body metamorphism. These materials were not "fluffed" on their parent body by impact-related regolith gardening or events caused by seismic vibrations. Samples of all three chemical types of ordinary chondrites (LL, L, H) are represented in this study and we conclude that incomplete compaction is common within the asteroid belt.

    Journal Title

    Meteoritics & Planetary Science

    Volume

    44

    Issue/Number

    11

    Publication Date

    1-1-2009

    Document Type

    Article

    Language

    English

    First Page

    1743

    Last Page

    1753

    WOS Identifier

    WOS:000273601100006

    ISSN

    1086-9379

    Share

    COinS