Proceedings of the Ocean Drilling Program, 157 Scientific Results 1998
DOI: 10.2973/odp.proc.sr.157.139.1998
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Sulfur, chlorine, and fluorine in glass inclusions in olivine and clinopyroxene from basaltic hyaloclastites representing the Gran Canaria shield stage at Sites 953 and 956

Abstract: Sulfur, chlorine, and fluorine concentrations of primary silicate glass inclusions in olivine and clinopyroxene from basaltic hyaloclastites representing the Gran Canaria shield stage at Sites 953 and 956 were investigated using an electron microprobe. Inclusion compositions corrected for post-entrapment, host-mineral crystallization range from 46.3 to 54.4 wt% SiO 2 , and from 5.7 to 10.3 wt% MgO. Significant spread in S and Cl values (200-2390 ppm S, and 120-870 ppm Cl) and the lack of correlation between S … Show more

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Cited by 7 publications
(5 citation statements)
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“…The eucrites are the poorest in halogen contents. Dreibus et al (2000Dreibus et al ( , 2003, Meyer (2004); eucrites: Wänke et al (1972), Basaltic Volcanism Study Project (1981, Mittlefehldt et al (1998), Sawyer et al (2000; lunar glasses: Taylor et al (1991), Mars surface rocks (includes RAT samples and samples corrected for S contents): Gellert et al (2004), McSween et al (2004), Rieder et al (2004); ocean island basalts (OIB): Aoki et al (1981), Hansteen and Gurenko (1998) Fluorine/K ratios are independent of K content and most F/K ratios range from about 0.02 to 0.3 (Fig. 3A).…”
Section: F and CL Abundances In Planetary Basaltsmentioning
confidence: 98%
“…The eucrites are the poorest in halogen contents. Dreibus et al (2000Dreibus et al ( , 2003, Meyer (2004); eucrites: Wänke et al (1972), Basaltic Volcanism Study Project (1981, Mittlefehldt et al (1998), Sawyer et al (2000; lunar glasses: Taylor et al (1991), Mars surface rocks (includes RAT samples and samples corrected for S contents): Gellert et al (2004), McSween et al (2004), Rieder et al (2004); ocean island basalts (OIB): Aoki et al (1981), Hansteen and Gurenko (1998) Fluorine/K ratios are independent of K content and most F/K ratios range from about 0.02 to 0.3 (Fig. 3A).…”
Section: F and CL Abundances In Planetary Basaltsmentioning
confidence: 98%
“…The rocks are tholeiitic to alkali-basaltic, strongly altered breccias, lapillistones, and hyaloclastite tuffs with phenocrysts of generally fresh clinopyroxene, almost entirely altered olivine, and rare altered plagioclase. Melt inclusions within clinopyroxene phenocrysts were analyzed by , Hansteen and Gurenko (1998), and . The calculated compositions of parental magmas in equilibrium with olivine Fo 90-92 range from olivine basalt and picrite to alkali basalt.…”
Section: Geological Backgroundmentioning
confidence: 99%
“…The shaded fields show the range of whole rock data for comparison Edmonds et al 2001) and depend strongly on melt and fluid compositions (mainly H 2 O) as well as P-T conditions (Carrol and Webster 1994). Despite high chlorine solubility in mafic melts (e.g., Lassiter et al 2002), Cl degassing is recorded in numerous examples (e.g., Hansteen and Gurenko 1998).…”
Section: Variations In Volatiles During Melt Evolutionmentioning
confidence: 99%
“…Because the volatile elements in whole rocks are strongly affected by degassing before and during eruption (Hansteen and Gurenko 1998;Metrich et al 1999;Edmonds et al 2001;de Moor et al 2005;Wallace 2005), melt inclusions trapped in pristine igneous minerals are potentially the best data source to study initial volatile contents in primary and parental melts (Danyushevsky et al 2002). Melt inclusions also provide an opportunity to extend the data on melt compositions beyond the range covered by whole rocks towards more primitive compositions .…”
Section: Introductionmentioning
confidence: 99%