| | Journal (article/letter/editorial) | accepted in revised form .-Iugusr 2. 199 1 ) Abstract-The new lunar meteorite MAC88 105 has been studied by...mineral-chemical techniques and was compared with the Yamato lunar meteorites. Clast types and pyroxene...are not as common as in other lunar meteorites. The large and common granulitelike me&igneous clasts...crystals with fine-grained olivine and pyroxenes in the interstices. Pyroxenes with mg number = Mg X lOO/(...zoning trends more Mg-rich than the above mg range and than those of the VLT basalts common in lunar meteorites | | | Journal (article/letter/editorial) | mingled impact melt breccia from the highlands—A complete cross section of the lunar crust S. E. ROBERTS 1...Mg-suite, and gabbronorite lithologies as defined by the Apollo sample collection. Clasts representing magnesian...mineralogy although pyroxferroite grains are present. The juxtaposition of evolved, basaltic clasts without...these basaltic clasts may represent cryptomare. The lithologies found in NWA 10986 offer a unique and...section view of the Moon sourced outside of the Procellarum KREEP Terrane. rich terrain, the Procellarum | | | Report (volume) | MINERALOGY & GEOCHEMISTRY Volume 60 NEW VIEWS of the MOON EDITORS: Bradley L. Jolliff, Mark A. Wieczorek...This book is dedicated to the memory of the late Graham Ryder, who was one of the original four members of...of CAPTEM when the New Views of the Moon scientific initiative was first conceived. Graham, who was a...owing to his broad knowledge of the lunar samples and his residence at the Lunar and Planetary Institute...where CAPTEM met, was a logical choice to be one of the co-leaders of this lunarscience initiative. Not only | | Wittmann, Axel, Korotev, Randy L., Jolliff, Bradley L., Nishiizumi, Kunihiko, Jull, A. J. Timothy, Caffee, Marc W., Zanetti, Michael, Irving, Anthony J. (2019) Petrogenesis of lunar impact melt rock meteorite Oued Awlitis 001. Meteoritics & Planetary Science, 54 (10) 2167-2188 doi:10.1111/maps.13218 | Journal (article/letter/editorial) | of Earth and Planetary Sciences and the McDonnell Center for the Space Sciences, Washington University...in lunar craters larger than ~50 km in diameter. The composition of Oued Awlitis 001 points toward a crustal...incompatible-element-rich regions. Comparison of the bulk composition of Oued Awlitis 001 with Lunar Prospector...spectrometer data indicates a limited region of matches on the lunar farside. After its initial formation in an...than ~50 m. The cosmogenic nuclide inventory of Oued Awlitis 001 records ejection from the Moon 0.3 Ma ago | | | Report (issue) | GEOCHIMICA ETT COSMOCHIMICA ACTA + Journal ey The Geochemical ce and. The ercenitter] Society Albright College...miles). North is at the upper right edge of the disc. Seen above the planet are the satellites Dione (right)...spot at the south edge of a yellow band; in true color, the spot would appear brown and the band white...spot slightly above and to the left in this image moves eastward relative to the green spot at a rate that...it to pass the green feature in about 50 days. The convective clouds that appear between the two spots |
|
Luna 24 landing site, Mare Crisium, The Moon