The Journal of the Japanese Association of Mineralogists, Petrologists and Economic Geologists
Online ISSN : 1883-0765
Print ISSN : 0021-4825
ISSN-L : 0021-4825
Volume 60, Issue 1
Displaying 1-3 of 3 articles from this issue
  • HISASHI TAKESHITA, YOSHIO OJI
    1968 Volume 60 Issue 1 Pages 1-26
    Published: July 05, 1968
    Released on J-STAGE: August 07, 2008
    JOURNAL FREE ACCESS
    There are many hornblende gabbroic inclusions found in the later Miocene to the early Pleistocene lavas developed in the northern Fossa Magna district, central Japan. These lavas are all hypersthenic rock series rich in groundmass orthopyroxene. It is noticed that a few augite-olivine-basalt lavas are often intercalated in the enormous effusives (1000m in the maximum thickness) of the calc-alkaline andesites. For this study 18 new chemical analyses have been made by one of the writers (Õji). In addition to these, 3 analyses already published by Yagi and Yagi (1958) and one analysis reproted by S. Yamada (1934) are cited; of these six are ultramafic hornblende gabbros and three are pyroxene-(±hornblende)-diorites, both as inclusions, five are andesites and the rest are augite-olivine-basalts both occurring in intimate association. They include 12 analyses of the later Miocene or early Pliocene rocks from the Shigarami Formation and 10 analyses of the later Pliocene to Pleistocene rocks.
    In MgO-total iron-alkalis diagram the plots of the rocks including hornblende gabboric and dioritic inclusions and their host andesites are arranged along a calc-alkaline trend. The points of the gabbros are closer to MgO-total iron side, while the points of the andesites are plotted on the extension of the gabbro-diorite line twoard the alkali apex. From intimate association of the gabbro-andesite-basalt and their petrochemistry, the writers are led to the conclusion that a calc-alkaline andesite magma rich in mafic components (SiO2 range 52-56%) has been derived from basaltic magma by subtracting hornblende gabboric crystalline aggregates, without contamination by any granitic or sedimentary materials. It is estimated that a considerable amount of ultramafic hornblende gabboric mass should be remained by this means within the depths, for instance at the geosynclinial bottoms of the Fossa Magna, and that the volume of the gabbro should exceed that of the effusive andesite composing the volcanics. Any geological evidences for such an enormous mass of hornblende gabbro of Pliocene, or even of Miocene age, have not been found in the regions composed mainly of volcanic rocks. On the contrary hornblende gabbros are much more commonly found in granite regions of Japan and they are intimately associated with diorite intrusives which had been under condition of granitization, and hence they have somewhat different characters from the segregated gabbros here cited.
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  • YOTARO SEKI, KIMIO OKUMURA
    1968 Volume 60 Issue 1 Pages 27-33
    Published: July 05, 1968
    Released on J-STAGE: August 07, 2008
    JOURNAL FREE ACCESS
  • Yoshihiro Kitadai
    1968 Volume 60 Issue 1 Pages 34-45
    Published: July 05, 1968
    Released on J-STAGE: August 07, 2008
    JOURNAL FREE ACCESS
    By diffusion of solid states, pseudowollastonite, forsterite and cristobalite phases are identified.Then silica glass rod is used as silica component. The growth of cristobalite phase is observed, onthe contrary, silicate minerals do not develope according to the increase of diffusion time.
    The growth of cristobalite depends on heating time, temperature and the kind of oxide component. Thelarger interaction between metallic atom and oxygen, the smaller growth of cristobalite is observed. CaO component promote cristobalitization, compared with MgO. Interaction of Ca-O is smaller than that of Mg-O, therefore diffusion rate of CaO component is larger than that of MgO. Formation of cristobalite depends on the rate of diffusion.
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