FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1569667377> ?p ?o ?g. }

• W1569667377 endingPage "256" @default.
• W1569667377 startingPage "255" @default.
• W1569667377 abstract "Abundant upper mantle (peridotite and pyroxenite) xenoliths occur in Miocene basaltic diatreme pipes and Quaternary lava flows on the Hyblean Plateau (Sicily, Southern Italy). Peridotites are spinel-facies protogranular-textured harzburgites and lherzolites (Fo90, En89, Cr-diopside, Cr-rich spinel), that equilibrated at temperatures between 950 and 1050°C. Even the freshest Hyblean peridotites exhibit some serpentine content. Major-element distribution and abundance reflect depletion (high MgO, low Al2O3) related to one or more melt extraction events, but evidence of modal and cryptic metasomatism does exist. For instance, phlogopite of metasomatic origin occurs rarely in these peridotites. Geochemical evidences of metasomatism includes Light Rare Earth Element (LREE) (e.g. LaN/YbN = 9-19). Sr-Nd and He isotopic signatures are also consistent with the refertilization of the lithospheric peridotite matrix (full descriptions in Sapienza and Scribano, 2000, Sapienza et al., 2005 and references therein).To better define the metasomatic reservoir, we performed in situ Os isotope analyses on sulphides from mantle peridotite collected from Valle Guffari Miocene diatreme. Eight peridotite xenoliths were cut in blocks, stuck on thin section glasses and polished on one side. Sulfides were imaged using a Cameca SX-100 electron microprobe. Then, Os isotope analyses were performed using a Merchantek LUV266 nm laser ablation microprobe (LAM) attached to a Nu Plasma multi-collector ICP (MC-ICP). The laser spot size was ~60 mm. Only 4 peridotite samples contain measurable sulfides, resulting in 11 analyses. Analytical details are in Pearson et al. (2002).Sulfides in the Hyblean peridotites are Ni-rich, often Ferich, and enclose a Cu-rich phase (Fig. 1). Their shape is variable, from spheroidal to irregularly shaped, usually displaying curvilinear margins (Fig. 1). The grainsize ranges from tens to ~250 mm. Sulfides are mainly related to the serpentine network. A few sulfides are olivine-enclosed but are too small to be analysed.187O/188Os ratios range from 0.110408 to 0.124398, which correspond to sub-chondritic values. 187Re/188Os ratios range from 0.0296463 to 1.41346, i.e. supra- to subchondritic values (Fig. 2). Five out of 6 sulfides from one sample (GE12) show similar 187Os/188Os but different 187Re/188Os, while the remaining sulfide and the other samples all align along an oblique array showing a negative correlation between 187Os/188Os and 187Re/188Os. Assuming the 187Re decay constant after Smoliar et al. (1996), 187Re/188Os- CHUR and 187Os/188OsCHUR after Walker and Morgan. (1989), we calculate Re-depletion ages (TRD) and model age (TMA). TRD represents the minimum melt-depletion age of the lithospheric mantle, since the calculation minimizes the effect of metasomatism-driven Re addition, while TMA assumes that the considered mantle portion remains in closedsystem conditions through time (Walker et al., 1989). Low- 187Os/188Os sulfides from peridotite GE12 show Paleoprotezoic to Archean TRD ages, while the other sulfides are Neoand Mesoproterozoic. TMA yields meaningless age (future or even older than the Earth’s formation), reflecting recent disturbance of the Re/Os ratio.GE12 sulfides show the same unradiogenic 187Os/188Os composition (except for one sulfide) but 187Re/188Os ranging from 0.8-1.4 (Fig. 2). This indicates that Os isotope composition does not depend on time-integrated in situ 187Re, but rather suggests the metasomatic effects with Re addition probably occurring shortly prior the eruption. The negative correlation between 187Os/188Os and 187Re/188Os in the other samples also supports the metasomatic origin of Re, and rather suggests mixing between two reservoirs with different Re-Os signatures (Wang et al., 2003; Fig. 2).Thus, the Hyblean peridotites we have studied experienced melt extraction event(s) – which would remove Re from the system - and underwent later metasomatic Re-enriching event(s). Although these preliminary Re-Os data - and the large associated uncertainties - on peridotite sulfides do not allow the calculation of a very detailed ages, TRD ages are realistic and require a Proterozoic-Archean minimum age for these portions of the Hyblean lithospheric mantle. Most sulfides in peridotite GE12 testify to recent Re addition, while the other peridotite sulfides and one GE12 sulfide seem to be the results of mixing between two metasomatic end-members. The low-187Os/188Os sulfides in sample GE12 may be representative of the low-187Os/188Os endmember. The occurrence of sulfides with different Os isotope signatures in sample GE12 confirms the importance of using in situ technique in such petrological study." @default.
• W1569667377 created "2016-06-24" @default.
• W1569667377 creator A5018490251 @default.
• W1569667377 creator A5020121719 @default.
• W1569667377 creator A5025343468 @default.
• W1569667377 creator A5073248661 @default.
• W1569667377 creator A5085523038 @default.
• W1569667377 date "2005-01-07" @default.
• W1569667377 modified "2023-10-05" @default.
• W1569667377 title "METASOMATISM IN THE HYBLEAN UPPER MANTLE: THE OS ISOTOPE CONTRIBUTION" @default.
• W1569667377 doi "https://doi.org/10.4454/ofioliti.v30i2.305" @default.
• W1569667377 hasPublicationYear "2005" @default.
• W1569667377 type Work @default.
• W1569667377 sameAs 1569667377 @default.
• W1569667377 citedByCount "0" @default.
• W1569667377 crossrefType "journal-article" @default.
• W1569667377 hasAuthorship W1569667377A5018490251 @default.
• W1569667377 hasAuthorship W1569667377A5020121719 @default.
• W1569667377 hasAuthorship W1569667377A5025343468 @default.
• W1569667377 hasAuthorship W1569667377A5073248661 @default.
• W1569667377 hasAuthorship W1569667377A5085523038 @default.
• W1569667377 hasConcept C127313418 @default.
• W1569667377 hasConcept C147717901 @default.
• W1569667377 hasConcept C151730666 @default.
• W1569667377 hasConcept C161509811 @default.
• W1569667377 hasConcept C167919410 @default.
• W1569667377 hasConcept C17409809 @default.
• W1569667377 hasConcept C183282558 @default.
• W1569667377 hasConcept C207319327 @default.
• W1569667377 hasConcept C2777018398 @default.
• W1569667377 hasConcept C2778882853 @default.
• W1569667377 hasConcept C42796848 @default.
• W1569667377 hasConcept C67236022 @default.
• W1569667377 hasConcept C77928131 @default.
• W1569667377 hasConcept C84372278 @default.
• W1569667377 hasConceptScore W1569667377C127313418 @default.
• W1569667377 hasConceptScore W1569667377C147717901 @default.
• W1569667377 hasConceptScore W1569667377C151730666 @default.
• W1569667377 hasConceptScore W1569667377C161509811 @default.
• W1569667377 hasConceptScore W1569667377C167919410 @default.
• W1569667377 hasConceptScore W1569667377C17409809 @default.
• W1569667377 hasConceptScore W1569667377C183282558 @default.
• W1569667377 hasConceptScore W1569667377C207319327 @default.
• W1569667377 hasConceptScore W1569667377C2777018398 @default.
• W1569667377 hasConceptScore W1569667377C2778882853 @default.
• W1569667377 hasConceptScore W1569667377C42796848 @default.
• W1569667377 hasConceptScore W1569667377C67236022 @default.
• W1569667377 hasConceptScore W1569667377C77928131 @default.
• W1569667377 hasConceptScore W1569667377C84372278 @default.
• W1569667377 hasIssue "2" @default.
• W1569667377 hasLocation W15696673771 @default.
• W1569667377 hasOpenAccess W1569667377 @default.
• W1569667377 hasPrimaryLocation W15696673771 @default.
• W1569667377 hasRelatedWork W1517721290 @default.
• W1569667377 hasRelatedWork W1964324070 @default.
• W1569667377 hasRelatedWork W1985787129 @default.
• W1569667377 hasRelatedWork W2000593660 @default.
• W1569667377 hasRelatedWork W2001180990 @default.
• W1569667377 hasRelatedWork W2007694935 @default.
• W1569667377 hasRelatedWork W2008106911 @default.
• W1569667377 hasRelatedWork W2013213907 @default.
• W1569667377 hasRelatedWork W2023887007 @default.
• W1569667377 hasRelatedWork W2030005096 @default.
• W1569667377 hasRelatedWork W2032838324 @default.
• W1569667377 hasRelatedWork W2047900361 @default.
• W1569667377 hasRelatedWork W2054901238 @default.
• W1569667377 hasRelatedWork W2058306817 @default.
• W1569667377 hasRelatedWork W2060472760 @default.
• W1569667377 hasRelatedWork W2373225677 @default.
• W1569667377 hasRelatedWork W2389223069 @default.
• W1569667377 hasRelatedWork W2966911950 @default.
• W1569667377 hasRelatedWork W2969824134 @default.
• W1569667377 hasRelatedWork W3143681281 @default.
• W1569667377 hasVolume "30" @default.
• W1569667377 isParatext "false" @default.
• W1569667377 isRetracted "false" @default.
• W1569667377 magId "1569667377" @default.
• W1569667377 workType "article" @default.