Makoto Shima
Max Planck Society
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Featured researches published by Makoto Shima.
Earth and Planetary Science Letters | 1973
Makoto Shima; Masako Shima; H. Hintenberger
Abstract Within a region of 5 km × 10 km on a downhill slope of the Yamato Mounties, in 1969 the Japanese Expedition Team collected many stones. 9 of them were recognized as meteorites. On 4 of these findings we determined the chemical composition and the rare gas content. According to the mineralogical and the chemical composition, Yamato (a) is an enstatite chondrite, Yamato (b) a Ca-poor achondrite, Yamato (c) seems to be a carbonations chondrite Type III and Yamato (d) a olivine bronzite chondrite. Exposure ages are 1.7, 31, 25 and 4.3 my respectively.
Journal of the Oceanographical Society of Japan | 1970
Akihiko Okada; Makoto Shima
Chemical and X-ray analyses were performed on the fifteen manganese nodules collected from the Pacific Ocean floor. The results were discussed compared with the previous data on the manganese nodules. Minerals were found to be todorokite, δ-MnO2 and other silicates, montmorillonite, illite, phillipsite and α-SiO2. Average composition shows that copper is concentrated on the deep sea nodules more than the shallow ones, and that the todorokite rich nodules contain more copper and nickel than the δ-MnO2 rich ones. The analyses of fresh water iron-manganese precipitates by bacterial activity suggest that biological process is one of the important factors on the genesis of the sedimentary iron-manganese deposits, including the manganese nodule.
Journal of the Oceanographical Society of Japan | 1972
Akihiko Okada; Tadayuki Minakuchi; Makoto Shima
The thermal phase transformation of the iron-manganese phase of the Pacific Ocean manganese nodules were studied by the differential thermal and X-ray diffraction methods. X-ray powder patterns of the heated samples at the temperature of 600°C to 1000°C show the occurrence of hematite, bixbyite and cubic and tetragonal (Fe, Mn)3O4. Bixbyite produced by the heat treatment of the iron-manganese phase gives an abnormal X-ray pattern in comparison with the standard sample of bixbyite. Cubic (Fe, Mn)3O4 is produced not only by the reaction of bixbyite with hematite over 900°C, but also at the lower temperature, such as 600°C. While, tetragonal (Fe, Mn)3O4 is a reaction product of cubic (Fe, Mn)3O4 with bixbyite over 900°C in the case of manganese rich nodules. The species and quantities of the products after the heat treatment are assumed to be mostly influenced by the relative contents of iron and manganese in the manganese nodule.
Meteoritics | 1978
Kenzo Yagi; J.F. Lovering; Makoto Shima; Akihiko Okada
Memoirs of National Institute of Polar Research. Special issue | 1975
Makoto Shima; Masako Shima
The Journal of the Japanese Association of Mineralogists,Petrologists and Economic Geologists | 1968
Makoto Shima; Akihiko Okada
The Journal of the Japanese Association of Mineralogists,Petrologists and Economic Geologists | 1965
Makoto Shima
The Journal of the Japanese Association of Mineralogists,Petrologists and Economic Geologists | 1976
Kenzo Yagi; Yoshio Oba; Makoto Shima; Akihiko Okada
The Journal of the Japanese Association of Mineralogists,Petrologists and Economic Geologists | 1969
Akihiko Okada; Makoto Shima
The Journal of the Japanese Association of Mineralogists,Petrologists and Economic Geologists | 1969
Makoto Shima; Sadayo Yabuki