| Okabayashi, Satoki, Yokoyama, Tetsuya, Hirata, Takafumi, Terakado, Kazuo, Galimov, Erik M. (2020) Iron isotopic composition of very low-titanium basalt deduced from the iron isotopic signature in Luna 16, 20, and 24 soils. Geochimica et Cosmochimica Acta, 269. 1-14 doi:10.1016/j.gca.2019.10.020 | Journal (article/letter/editorial) | 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 | | | 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 | | Zeng, Xiaojia, Li, Shijie, Joy, Katherine H., Li, Xiongyao, Liu, Jianzhong, Li, Yang, Li, Rui, Wang, Shijie (2020) Occurrence and implications of secondary olivine veinlets in lunar highland breccia Northwest Africa 11273. Meteoritics & Planetary Science, 55 (1) 36-55 doi:10.1111/maps.13421 | Journal (article/letter/editorial) | breccias preserve the records of geologic processes on the Moon. In this study, we report the occurrence, petrography...petrography, mineralogy, and geologic significance of the observed secondary olivine veinlets in lunar feldspathic...dominated by interconnecting olivine mineral grains. The host clasts are mainly composed of mafic minerals...lithology. The studied olivine veinlets (~5 to 30 lm in width) are distributed within the mafic mineral...mineral host, but do not extend into the adjacent plagioclase. Chemically, these olivine veinlets are Fe-richer | | | 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 | | | 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 |
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