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- W2023150404 abstract "Lunar sample 77135, an impact melt breccia full of vesicles, has been reinvestigated by electron microprobe and X-ray diffraction techniques and compared with a vesicular melt LL chondrite, Yamato 790964, in an attempt to understand their impact heating processes and subsequent cooling history. Notable similarities between the lunar and chondritic melt breccias include: abundant vesicles, similar pyroxene chemical zoning trends, the presence of variable amounts of clastic material, and similar chemical compositions except for K and Na contents of glass and mesostasis. Some constraints on the cooling history are estimated from Mg-Fe diffusion profiles in olivine and pyroxene. The burial depth of lunar sample 77135 during cooling was 0.2-100 m; the depth for the chondrite was probably smaller. Impact melts were probably produced and a layer of regolith retained on the parent body sufficiently thick to allow the olivines to homogenize during slow cooling." @default.
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- W2023150404 date "1984-12-10" @default.
- W2023150404 modified "2023-09-24" @default.
- W2023150404 title "Mineralogical comparison and cooling history of lunar and chondritic vesicular melt breccias" @default.
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- W2023150404 doi "https://doi.org/10.1029/jb089ib13p11581" @default.
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