K.H. Joy, R. Tart\u00e8se, S. Messenger, M.E. Zolensky, Y. Marrocchi, D.R. Frank, D.A. Kring<\/p>\n\n\n\n
Earth and Planetary Science Letters
Volume 540, 15 June 2020, 116265<\/p>\n\n\n\n
LINK<\/strong><\/a><\/p>\n\n\n\n “Highlights<\/p>\n\n\n\n \u2022 The lunar regolith has accumulated volatiles from impacting hydrated asteroids. “Projectiles striking the Moon have modified its crust and delivered volatile elements to its interior and surface. Direct evidence of impactor origins is recorded by the rare occurrence of sub-cm sized meteorite fragments identified in Apollo samples and lunar meteorites. The Bench Crater meteorite is a millimetre-sized carbonaceous chondrite collected in regolith on the rim of Bench impact crater at the Apollo 12 landing site. Transmission electron microscopy has previously shown that Bench Crater contains abundant hydrated silicates, establishing the survivability of hydrated material impacting the lunar surface. To provide further information on the volatile inventory of the Bench Crater meteorite, we report here the isotope compositions of hydrogen, nitrogen, carbon and oxygen. This is the first direct isotopic analysis of meteoritic material delivered to the lunar surface and provides context for volatile and organic element signatures in lunar regolith samples, and the survivability of volatile material delivered to planetary surfaces during impact bombardment. The Bench Crater meteorite is characterised by \u03b4D values ranging between \u221236 \u00b1 40 and 200 \u00b1 40\u2030, and bulk average \u03b413C of \u221213 \u00b1 30\u2030, and \u03b415N of \u221240 \u00b1 36\u2030 (all uncertainties at the 2\u03c3 confidence level). The oxygen isotope compositions measured in situ in matrix silicates and magnetite in Bench Crater are consistent with those measured in matrix and magnetite in CI and CM chondrite falls. Altogether, these new H, C, N and O isotope data, coupled to mineralogical and geochemical observations, suggest that Bench Crater may have been derived from an asteroidal parent body not represented in the terrestrial meteorite collection. This is a crucial outcome in the current context of sample-return missions to carbonaceous asteroids, and more broadly for investigating the flux of material delivered to the Earth-Moon system through time.”<\/p>\n\n\n\n More information:<\/p>\n\n\n\n BENCH CRATER METEORITE: HYDRATED ASTEROIDAL MATERIAL DELIVERED TO THE MOON<\/a>
\u2022 The Bench Crater meteorite preserves hydrated minerals that survived lunar impact.
\u2022 Bench Crater meteorite has unique mineralogical and stable isotope characteristics.
\u2022 Bench Crater may represent material not found in the current meteorite collection.
\u2022 Bench Crater is a critical ground truth for future lunar volatile resource missions.”<\/p>\n\n\n\n
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76th Annual Meteoritical Society Meeting (2013), Abstract 5315<\/p>\n\n\n\n