1999
DOI: 10.2465/ganko.94.120
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Olivine-chromian spinel compositional relationships of the Cenozoic alkali basalts from Southwest Japan: implication for their mantle restites.

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Cited by 9 publications
(7 citation statements)
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“…Later magmatism (6–0 Ma) is characterized by eruptions of geochemically variable rocks. These rocks consist of subalkaline basalt and andesite including magnesian andesite (nonadakitic) and alkaline basalts with ultrasodic and ultrapotassic suites (Iwamori, ; Kimura et al, ; Koyaguchi, ; Nakamura et al, ; Shukuno & Arai, ; Tatsumi et al, ). In particular, the magmatism in the last 2 Myr is dominated by voluminous emplacement of high‐Sr andesites and dacites (adakitic; Kimura et al, ; Figure ).…”
Section: Tectonic and Geologic Backgroundmentioning
confidence: 99%
“…Later magmatism (6–0 Ma) is characterized by eruptions of geochemically variable rocks. These rocks consist of subalkaline basalt and andesite including magnesian andesite (nonadakitic) and alkaline basalts with ultrasodic and ultrapotassic suites (Iwamori, ; Kimura et al, ; Koyaguchi, ; Nakamura et al, ; Shukuno & Arai, ; Tatsumi et al, ). In particular, the magmatism in the last 2 Myr is dominated by voluminous emplacement of high‐Sr andesites and dacites (adakitic; Kimura et al, ; Figure ).…”
Section: Tectonic and Geologic Backgroundmentioning
confidence: 99%
“…The chromian spinel is relatively low in TiO 2 (<1 wt %), and plotted around the boundary between intraplate and arc magmas in the TiO 2 -Y Fe space [66]. The Bankawa alkali basalt shows a very primitive character in terms of the Fo (olivine)-Cr# (spinel) relationship [41,67,68] (Figure 8). Some of the olivine-spinel pairs in the host rock are plotted in or near the olivine-spinel mantle array, a residual spinel peridotite field (Figure 8) [41,67].…”
Section: Chemistry Of the Host Rockmentioning
confidence: 99%
“…The previous studies (Kimura, Gill, et al, 2014; Pineda‐Velasco et al, 2018; Sakuyama, Nakai, et al, 2014; Sakuyama et al, 2009) assumed that the magma source beneath SW Japan has trace‐element composition and mineralogy of the primitive (upper) mantle (PUM; McDonough & Rudnick, 1998; Sun & McDonough, 1989). This assumption is based on the predominance of fertile peridotites (clinopyroxene‐rich lherzolites) in xenoliths hosted in OIB (Arai & Muraoka, 1992) and chondritic‐REE patterns of clinopyroxene in these xenoliths (Abe et al, 1998), as well as low Cr/(Cr + Al) of spinel inclusions (<0.5 in molar) in forsteritic olivine phenocrysts (Fo > 85) in OIB (Shukuno & Arai, 1999); all of these features indicate that the mantle beneath the Chugoku district is fertile.…”
Section: Discussionmentioning
confidence: 99%
“…The calculation was iterated until the composition of magma reaches Fe-Mg equilibrium with the mantle olivine (K D ≡ (Fe 2+ /Mg) melt /(Fe 2+ /Mg) olivine where its compositional dependency is corrected following Tamura et al, 2000). The forsterite content (Fo ≡ 100 × Mg/(Mg + Fe 2+ )) of the mantle olivine is assumed to be 89 as was found in most magnesian phenocrysts in mafic rocks in this district (Aoki, 1977;Higashiyama et al, 2013;Iwamori, 1989;Koyaguchi, 1986;Nagasaki & Nagao, 1988;Takahashi et al, 2017;Zellmer et al, 2014; Table S36) or predicted from the compositional relationship of olivine phenocrysts and spinel inclusions (Shukuno & Arai, 1999; Table S36).…”
Section: Approach 1: Geothermobarometrymentioning
confidence: 99%