Abstract
The olivine crystals from lunar regolith samples taken by the Soviet unmanned spacecrafts Luna-16 and Luna-24 were investigated. Eleven 0.5 –1.0 mm size olivine crystals were mounted in epoxy, polished and then etched in modified WO 4 solution. The Fe-group track densities up to 10 8 tracks.cm −2 (Fe-group) were measured under optical microscope. The tracks of length greater than 30 microns due to Z ≥ 36 cosmic ray nuclei are counted for VVH tracks density for all the crystals. The VVH / VH track densities ratio for these lunar olivine crystals varies from 1.25×10 −4 to 2×10 −3. It corresponds to the averaged depth of these crystals in lunar soil of 2–8 cm during galactic cosmic ray exposure. Lunar crystals are well suited for VVH track studies due to a very high track density. Two crystals were annealed at 430°C for 32 hrs. This procedure eliminates iron group tracks completely and leaves etchable tracks of nuclei with Z ⩾ 50 even in the olivine crystals with Fe-group tracks up to 1–2×10 8 tracks cm −2. We were able to measure two tracks with the length 195 and 210μm which were produced by ThU group of Galactic cosmic ray nuclei.
Published Version
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