Fluorite deposits in Japan are distributed mostly in the Sn-W-Cu metallogenic provinces,which are related to the late Cretaceous ilmenite-series volcano-plutonic activities. They occur in hydrothermal veins related to felsic volcanics (4 ore deposits) and granite porphyry (the largest Hiraiwa deposits), in skarn bodies with biotite granite (5 deposits) and in hydrothermal veins within biotite granite (2 deposits). The production statistics indicate that 77 % of the ores were mined from porphyry- and volcanics-related vein type, and 23 % from granite-related skarn and vein types. The outstanding Hiraiwa deposits were formed by extensive fracturing due to regional shearing and magmaascent, and invasion of fractionated felsite magma, then by the associated hydrothermal activities.

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Muscovite in pegmatitic ore from the Tamayama native gold deposit, southern Kitakami Mountains, is dated at 111.7 ± 3.0 Ma, which is consistent with those of Cretaceous granitoids in the Kitakami Mountains. Pegmatitic ore and its host Hikami granitic rocks have been thermally metamorphosed by the Kesengawa granodiorite of Cretaceous age. A pressure corrected homogenization temperature (ca. 400 ^oC ) of quartz in the pegmatitic ore is beyond the closing temperature (ca. 350 ^oC ) of muscovite with respect to radiogenic argon. Therefore, the obtained K-Ar age of muscovite is considered to be rejuvenated due to contact metamorphism. An oxygen isotopic ratio of quartz in the pegmatitic ore (δ¹⁸OSMOW=10.0 ‰), resembles to that of quartz in an ilmenite-series pegmatite (ca. >10 ‰). The oxygen isotopic equibration temperature for a coexisting mineral pair of quartz-muscovite in the pegmatitic ore is calculated at 865 ^oC. The Hikami granitic rocks which host the pegmatitic ore, have also an ilmenite-series character. These data suggest that the pegmatitic ore from the Tamayama gold deposit is the final crystallization product of the Hikami granitic rocks which have been thermally metamorphosed intermittently after the formation of pegmatitic ore.

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The Geological Survey of Japan, AIST, has been publishing the 1:200,000 gravity map (Bouguer anomalies) series of Japan. A new gravity map of Miyazaki district has been published. We compiled gravity data from about 7,300 stations including 387 new gravity stations on land and also compiled sea surface gravimeter data (GH83-1 cruise of GSJ: about 5,900 points) within the map area. The Bouguer anomaly map with an assumed density of 2.3 g/cm³ (2300 kg/m³) shows clear correlation between the geological structure pattern and the gravity anomalies in general. Long wavelength pattern of the largest low anomalies is coincident with the Miyazaki-oki basin which located at the landward side of trench junction. And the geologically well-known bending pattern of the Shimanto belt caused by a counterclockwise rotation of southern Kyushu with respect to northern Kyushu is also seen in long wavelength anomaly pattern. Short wavelength low anomalies corresponding to Hitoyoshi, Kobayashi and Miyakonojo basins are apparent. And a low anomaly in Miyazaki plain and high anomalies surrounding the plain are clearly visible in a high-pass filtered map. Apparent short wavelength anomalies are seen in the Kyushu mountains but they are thought to be effects derived from an inappropriate assumption of the crustal model density (2.3 g/cm³: default value for the GSJ’s gravity map series) to this area. Optimum densities in northern part of the map should be larger than 2.3 g/cm³.

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In order to elucidate dissolution-adsorption-precipitation behavior of uranium nuclides (U238 and U-234) and chemically controlling factor under environmental conditions, a leaching experiment of uranium nuclides from JG-2 granite was preliminarily studied at 80℃ in chloride and sulfate systems. The results show that pH is an important factor that controls the U leach while the redox potential may also be important. It is estimated that sulfate type is superior to chloride type for U concentration in spring water. The reaction system and experimental conditions were discussed for better experiment. It was also shown that U-234/U-238 activity ratios were over 1, which is often observed in the environmental waters. Model calculation was conducted to discuss the parameters that effect on U-234/U-238 activity ratios.

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Fluxes of polycystine Radiolaria were examined to clarify temporal and regional variations in production and percentage assemblages in relation to hydrographic conditions. Three time-series sediment traps were deployed in the central North Pacific along 175˚E for about one year, beginning in June 1993. The trap sites were located in the subarctic, the transitional, and the subtropical water masses. Temporal fluxes of polycystines showed large variations during the experiment. In the subarctic water mass, high polycystine fluxes were observed during summer to fall, while in the transitional and subtropical regions any relationship was not seen between the polycystine fluxes and sea surface temperature. High polycystine fluxes observed from the subarctic and transition zones can probably be ascribed to high food availability. The polycystine annual mean flux through the experiment was highest at the subarctic site, while that of the transition site was lower than that of the subtropical site. This pattern does not parallel the latitudinal variation in the total mass, opal or organic matter fluxes recorded from the same experiments. The relative abundance of most of the families did not vary much during the experiment at each site; i.e., polycystine faunal composition remains fairly stable in each oceanic climatic zone. This is likely to be because most polycystine radiolarians are produced in the depths where there is little seasonal environmental change. Latitudinal changes of total polycystine assemblages of the three sites are clear. Plagiacanthidae dominate the assemblage from the subarctic site, and Actinommidae become abundant in the assemblage from the transitional zone. No single family dominates the total assemblage from the subtropical region. These faunal differences between the climatic zones probably relate to differences in temperature of the water at depths of 50-200 m where most polycystines live. Consequently, the percentage abundance of sinking polycystine radiolarians retain a great deal of environmental information on the water masses below the seasonal thermocline in each climatic zone, but possibly do not record much information about seasonal oceanographic changes in the surface layer above the seasonal thermocline.

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