| low-titanium basalt deduced from the iron isotopic signature in Luna 16, 20, and 24 soils Satoki Okabayashi,...low-titanium basalt deduced from the iron isotopic signature in Luna 16, 20, and 24 soils, Geochimica et Cosmochimica...undergone enhancements after acceptance, such as the addition of a cover page and metadata, and formatting...formatting for readability, but it is not yet the definitive version of record. This version will undergo...version to give early visibility of the article. Please note that, during the production process, errors may |
|
|
 |
Warren, Paul H. (2005) “New” lunar meteorites: Implications for composition of the global lunar surface, lunar crust, and the bulk Moon. Meteoritics & Planetary Science, 40 (3) 477-506 doi:10.1111/j.1945-5100.2005.tb00395.x |
Journal (article/letter/editorial) |
| Implications for composition of the global lunar surface, lunar crust, and the bulk Moon Paul H. WARREN Institute...significant implications for the interpretation of global Th data and for the Moon’s bulk composition. As...(Prettyman et al. 2002), the Lunar Prospector gamma-ray data imply that the average global surface Th...calibration yields implausibly high concentrations for the three most Th-poor documented sampling sites, it...in a misfit toward too-high Th when compared with the global regolith Th spectrum as constrained using |
|
|
 |
Barsukov, V. L., Nazarav, M. A., Tarasov, L. S. (1982) Moon rock mineralogy. International Geology Review, 24 (2) 238-248 doi:10.1080/00206818209452398 |
Journal (article/letter/editorial) |
| homepage: http://www.tandfonline.com/loi/tigr20 Moon rock mineralogy V. L. Barsukov , M. A. Nazarav &...& L. S. Tarasov (1982) Moon rock mineralogy, International Geology Review, 24:2, 238-248, DOI: 10.10...13:40 Moon rock mineralogy V.L. Borsukov, M.A. Nozorov, ond L.S. Torosov is restricted to the range...parts of the hloon (Vinogradov, 1975; Schmitt, 1975; Florenskiy et al., 1977). Nevertheless, the material...various laboratories throughout the world is reasonably representative, and the data can be combined with orbital |
|
|
 |
Jolliff, Bradley L., Wieczorek, Mark A., Shearer, Charles K., Neal, Clive R. - Eds. (2006) New Views of the Moon. Reviews in Mineralogy and Geochemistry Vol. 60. Mineralogical Society of America |
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 |
|
|
 |
(1981) Proceedings of the Twelfth Lunar and Planetary Science Conference - Section 2: Planets, Asteroids and Satellites. Geochimica et Cosmochimica Acta Supplement 16. The Geochemical Society and the Meteoritical Society |
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 |
|
|
