Preliminary examination of the Yamato-86032 lunar meteorite: II. Major and trace element chemistry
スポンサーリンク
概要
- 論文の詳細を見る
The chemical composition of the new lunar meteorite Yamato-86032 has been studied by several laboratories in a consortium study. A preliminary report on the first analytical results from seven laboratories is given in this paper. The meteorite, which is the largest lunar meteorite recovered so far, is more heavily shocked than the other five lunar meteorites, which makes it difficult to classify the rock exactly. Although it may be classified as an anorthositic breccia the trace element composition of Y-86032 is somewhat different from the composition of the other known lunar meteorites. The major element chemistry of Y-86032 is similar to the other lunar meteorites, except for the iron content, which is lower by a factor of about 1. 4. Since the magnesium abundance is nearly identical there is a disparity in the mg ratio. The REE abundances in Y-86032 are very low and comparable to Y-82192/3. There is no evidence of any KREEP component. The abundances of several lithophile and incompatible elements are lower in Y-86032 than in the other lunar meteorites. The siderophile element contents are low and vary between individual chips. Sc, Cr, Mn, and Co have significantly lower abundances than in Y-82192/3. The chemical investigations demonstrate that Y-86032 is a new and important sample from the lunar highlands.
- 国立極地研究所の論文
著者
-
Fukuoka Takaaki
Department of Environmental Systems, Rissho University
-
Lindstrom Marilyn
Code Sn21 Nasa Johnson Space Center
-
Koeberl Christian
Lunar and Planetary Institute
-
Warren Paul
Institute of Geophysics, University of California
-
Spettel Bernhard
Max-Plank-Institute fur Chemie
-
Warren Paul
Institute Of Geophysics And Planetary Physics University Of Califonia
-
Fukuoka Takaaki
Department Of Chemistry Faculty Of Science Gakushuin University
関連論文
- General characterization of Antarctic micrometeorites collected by the 39th Japanese Antarctic Research Expedition: Consortium studies of JARE AMMs (III)
- A consortium study of Antarctic micrometeorites recovered from the Dome Fuji Station
- VOLCANIC RECORDS AND DATING OF THE UPPER HALF OF THE H15 ICE CORE FROM MIZUHO PLATEAU, EAST ANTARCTICA
- Identification of tephra layers in the meteorite ice field based on trace element compositions and refractive indices of glass (abstract)
- Preliminary examination of the Yamato-86032 lunar meteorite: II. Major and trace element chemistry
- Boron systematics of Hisatsu and Kirishima basaltic rocks from southern Kyushu, Japan
- Lunar meteorite Yamato-86032: Mineralogical, petrological, and geochemical studies
- Chemistry of Yamato-791197 Antarctic meteorite: Evidence for its lunar highland origin
- Antarctic primitive achondrites Yamato-74025, -75300, and -75305:Their mineralogy, thermal history and the relevance to winonaite
- The Yamato-793605 martian meteorite consortium
- Chemical compositions of the ALH-77302 polymict eucrite
- Geochemical investigation of five lunar meteorites : Implications for the composition, origin and evolution of the lunar crust
- Geochemical investigation of two lunar mare meteorites: Yamato-793169: and Asuka-881757
- Geochemistry of lunar meteorite Yamato-82192: comparison with Yamato-791197, ALHA81005, and other lunar samples
- Yamato-793605, EET79001, and other presumed martian meteorites: Compositional clues to their origins
- Geochemistry of lunar meteorite Yamato-791197: Comparison with ALHA81005 and other lunar samples
- Boron and other trace element constraints on the slab-derived component in Quaternary volcanic rocks from the Southern Volcanic Zone of the Andes