Volatile chalcophile, siderophile and lithophile trace elements in lunar meteorite Yamato-82192

• Main Authors: Dennison,Jane E., Kaczaral,Patrick W., Lipschutz,Michael E.
• Format: Report
• Language: English
• Published: Department of Chemistry, Purdue University/Department of Chemistry, Purdue University/Department of Chemistry, Purdue University 1987
• Subjects: Yamato; Allan Hills; Memoirs of National Institute of Polar Research; Polar Research
• Online Access: https://nipr.repo.nii.ac.jp/?action=repository_uri&item_id=2122; http://id.nii.ac.jp/1291/00002122/; https://nipr.repo.nii.ac.jp/?action=repository_action_common_download&item_id=2122&item_no=1&attribute_id=18&file_no=1

Neutron activation analyses of Ag, Au, Bi, Cd, Co, Cs, Ga, In, Rb, Sb, Se, Te, Tl, U and Zn in whole-rock, melted and unmelted regolith samples of Yamato-82192 reveals a lunar highlands origin plus meteorite admixture, 2.4±0.8% Cl-equivalent for micrometeorites and ancient impact component. A small but real amount of mobile element loss occurred during the shock-melting episode that formed Y-82192. Differences in trace element and other trends indicate pronounced differences in the thermal histories of the parent regoliths of Allan Hills A81005 and Y-791197 and -82192 so that each must have been produced by a separate impact on the Moon.