Non-Chondritic Inclusions in the LL Chondrite DOM85505

Details Non-Chondritic Inclusions in the LL Chondrite DOM85505 Non-Chondritic Inclusions in the LL Chondrite DOM85505

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27.1027p&link_type=abstract

Lunar and Planetary Science, volume 27, page 1027

Computer Science

Achondrites, Breccia, Chondrites, Cumulates, Metamorphism

Scientific paper

DOM85505 is a 31g LL Antarctic chondrite that was noted in the preliminary description to contain inclusions lacking chondritic texture. Angular inclusions in the host chondrite (LL5, S4) do not resemble any of the common achondrites in texture or mineral composition. The non-chondritic inclusions have similar bulk compositions and the same mineral compositions as the host chondrite and appear to be have formed as cumulates from an LL chondrite melt. Texturally similar non-chondritic inclusions in the L6 Yamato meteorites 75097 and 793241 derive from an H chondrite source but are also cumulates that have reacted with the host chondrite following incorporation.

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