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    Chemistry of the Calcalong Creek lunar meteorite and its relationship to lunar terranes

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    Author
    Hill, D. H.
    Boynton, W. V.
    Issue Date
    2003-01-01
    Keywords
    lunar meteorites
    Calcalong Creek
    Lunar samples
    Lunar terranes
    trace elements
    
    Metadata
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    Citation
    Hill, D. H., & Boynton, W. V. (2003). Chemistry of the Calcalong Creek lunar meteorite and its relationship to lunar terranes. Meteoritics & Planetary Science, 38(4), 595-626.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655684
    DOI
    10.1111/j.1945-5100.2003.tb00029.x
    Additional Links
    https://meteoritical.org/
    Abstract
    The Calcalong Creek lunar meteorite is a polymict breccia that contains clasts of both highlands and mare affinity. Reported here is a compilation of major, minor, and trace element data for bulk, clast, and matrix samples determined by instrumental neutron activation analysis (INAA). Petrographic information and results of electron microprobe analyses are included. The relationship of Calcalong Creek to lunar terranes, especially the Procellarum KREEP Terrane and Feldspathic Highlands Terrane, is established by the abundance of thorium, incompatible elements and their KREEP-like CI chondrite normalized pattern, FeO, and TiO2. The highlands component is associated with Apollo 15 KREEP basalt but represents a variant of the KREEP-derived material widely found on the moon. Sources of Calcalong Creek's mare basalt components may be related to low-titanium (LT) and very low-titanium (VLT) basalts seen in other lunar meteorites but do not sample the same source. The content of some components of Calcalong Creek are found to display similarities to the composition of the South Pole-Aitken Terrane. What appear to be VLT relationships could represent new high aluminum, low titanium basalt types.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2003.tb00029.x
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    Meteoritics & Planetary Science, Volume 38, Number 4 (2003)

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