1966
DOI: 10.1007/bf00518082
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Ultramafic inclusions in basaltic rocks from Hawaii

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Cited by 254 publications
(53 citation statements)
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“…They have been observed as intergranular grains and as inclusions in silicate minerals in spinel lherzolite and spinel harzburgite xenoliths (Fig. 2;White 1966;Vakhrutshev and Prokoptsev 1972;MacRae 1979;Pasteris 1981;Amundsen 1987), garnet peridotite (e.g., Bishop et al 1975;Meyer and Tsai 1979) and pyroxenite xenoliths (e.g., O'Reilly and Griffin 1987;Wilshire et al 1988). Similar BMS grains are also found in abyssal peridotites ( Fig.…”
Section: Introductionmentioning
confidence: 83%
“…They have been observed as intergranular grains and as inclusions in silicate minerals in spinel lherzolite and spinel harzburgite xenoliths (Fig. 2;White 1966;Vakhrutshev and Prokoptsev 1972;MacRae 1979;Pasteris 1981;Amundsen 1987), garnet peridotite (e.g., Bishop et al 1975;Meyer and Tsai 1979) and pyroxenite xenoliths (e.g., O'Reilly and Griffin 1987;Wilshire et al 1988). Similar BMS grains are also found in abyssal peridotites ( Fig.…”
Section: Introductionmentioning
confidence: 83%
“…The lherzolite inclusions in the Aitutaki Island olivine nephelinite have mineral and whole-rock compositions similar to those of spinel lherzolite nodules occurring in undersaturated ba~alt on a worldwide basis (e.g., White 1966;Frey & Green 1974;Wilshire & Shervais 1975;Frey & Prinz 1978). It is generally agreed that these lherzolite inclusions have no direct genetic relationship with their host magmas, are accidental, and probably represent upper mantle material from which basaltic magma was derived (e.g., Frey & Green 1974;Hamlyn & Bonatti 1980).…”
Section: Discussionmentioning
confidence: 97%
“…Olivine in the lherzolites is Mg rich (F090-91) ( Table 2) and is compositionally similar to olivine in this rock type at worldwide occurrences (e.g., White 1966;Frey & Green 1974;Frey & Prinz 1978). In contrast, olivine in the clinopyroxenite G is substantially lower in MgO (richer in FeO), having Fo s2 , and is compositionally similar to the larger olivine grains in the host rock, which also average F0 82 (Table 2).…”
Section: Mineral Compositions Olivinementioning
confidence: 94%
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“…There is a significant body of published information on petrography, mineral chemistry, trace element and isotope geochemistry of the SLC pyroxenite xenoliths (e.g., White 1966;Green 1966;Jackson and Wright 1970;Frey, 1980;Sen, 1988;Keshav and Sen, 2001;Bizimis et al, 2005;Sen et al, 2005;Keshav et al, 2007). On the basis of the available literature I summarize the possible origin of these rocks: (1) Based on mineral thermobarometry and the Sr-Nd-Hf isotope composition of the xenoliths, G. Sen and his co-workers proposed that the pyroxenites are high pressure (> 20 Kb) cumulates from a melt similar to the HV lava series (e.g., Sen et al 1983 Lassiter et al (2000) to propose that they represent 80-100 Myr old cumulates formed at a mid oceanic ridge setting.…”
Section: Garnet Pyroxenite Xenolithsmentioning
confidence: 99%