TY - JOUR
T1 - Helium isotopes in peridotite mineral phases from Hyblean Plateau xenoliths (south-eastern Sicily, Italy)
AU - Sapienza, Giovanna
AU - Hilton, David R.
AU - Scribano, Vittorio
PY - 2005/6/15
Y1 - 2005/6/15
N2 - Fourteen He isotope and abundance analyses have been performed on olivine, orthopyroxene, and clinopyroxene grains from selected spinel-facies peridotite xenoliths collected from the Hyblean Plateau, southeastern Sicily. These peridotites consist of protogranular-textured, spinel-facies lherzolites and lherzolitic harzburgites. Microthermometric data on olivine and pyroxenes reveal that the fluid inclusions (FIs) are nearly pure CO2, with densities ranging from 0.76 to 1.15 g/cm3. The densest inclusion trail occurs in an orthopyroxene grain and indicates a trapping-pressure of 0.98-1.14 GPa (estimated equilibration temperature of 1000 °C for pure CO2 system) corresponding to a depth of ∼ 36-41 km (for an average estimated density of the lithospheric column of 2.85 g/cm3). These are minimum estimates. The near-unimodal distribution of CO2 densities indicates that these xenoliths have been stored at the pressure interval of 0.75-0.95 GPa - Corresponding to a depth of ∼ 27-35 km (crust-mantle boundary or just below). En route to the surface, they have not had any significant interaction with shallower volatile reservoirs. He trapped in CO2-rich fluid inclusions ranges in abundance from 1.8 to 86.6×10-9 cm3 STP/g, with clinopyroxenes usually showing higher He contents than coexisting olivines and orthopyroxenes. The inter-mineral differences are due to physical properties of minerals. In contrast, He isotope ratios cover a narrow range (∼ 7.3 ± 0.3RA, where RA = air 3He/4He), indicating isotopic equilibration between the mineral phases. He composition indicates a MORB-type source for the metasomatic agent(s), influenced by relatively minor radiogenic production in the source. Therefore, in closed-system conditions, the calculated helium residence time is 790 Myr. Geophysical and geochemical studies suggest the existence of a common fluid reservoir in the mantle beneath the Central Mediterranean area. The most pristine He signature for the mantle endmember is found on Pantelleria Island (Sicily Channel): This He ratio is similar to that found in Hyblean peridotite minerals, testifying to a common source history. We conclude, therefore, that Hyblean xenoliths can be used as a powerful tool in defining the geochemical features of this portion of the upper mantle.
AB - Fourteen He isotope and abundance analyses have been performed on olivine, orthopyroxene, and clinopyroxene grains from selected spinel-facies peridotite xenoliths collected from the Hyblean Plateau, southeastern Sicily. These peridotites consist of protogranular-textured, spinel-facies lherzolites and lherzolitic harzburgites. Microthermometric data on olivine and pyroxenes reveal that the fluid inclusions (FIs) are nearly pure CO2, with densities ranging from 0.76 to 1.15 g/cm3. The densest inclusion trail occurs in an orthopyroxene grain and indicates a trapping-pressure of 0.98-1.14 GPa (estimated equilibration temperature of 1000 °C for pure CO2 system) corresponding to a depth of ∼ 36-41 km (for an average estimated density of the lithospheric column of 2.85 g/cm3). These are minimum estimates. The near-unimodal distribution of CO2 densities indicates that these xenoliths have been stored at the pressure interval of 0.75-0.95 GPa - Corresponding to a depth of ∼ 27-35 km (crust-mantle boundary or just below). En route to the surface, they have not had any significant interaction with shallower volatile reservoirs. He trapped in CO2-rich fluid inclusions ranges in abundance from 1.8 to 86.6×10-9 cm3 STP/g, with clinopyroxenes usually showing higher He contents than coexisting olivines and orthopyroxenes. The inter-mineral differences are due to physical properties of minerals. In contrast, He isotope ratios cover a narrow range (∼ 7.3 ± 0.3RA, where RA = air 3He/4He), indicating isotopic equilibration between the mineral phases. He composition indicates a MORB-type source for the metasomatic agent(s), influenced by relatively minor radiogenic production in the source. Therefore, in closed-system conditions, the calculated helium residence time is 790 Myr. Geophysical and geochemical studies suggest the existence of a common fluid reservoir in the mantle beneath the Central Mediterranean area. The most pristine He signature for the mantle endmember is found on Pantelleria Island (Sicily Channel): This He ratio is similar to that found in Hyblean peridotite minerals, testifying to a common source history. We conclude, therefore, that Hyblean xenoliths can be used as a powerful tool in defining the geochemical features of this portion of the upper mantle.
KW - CO fluid inclusions
KW - He isotopes
KW - Hyblean Plateau
KW - Mantle metasomatism
KW - Peridotite xenoliths
UR - http://www.scopus.com/inward/record.url?scp=19944392637&partnerID=8YFLogxK
U2 - 10.1016/j.chemgeo.2005.02.012
DO - 10.1016/j.chemgeo.2005.02.012
M3 - Article
AN - SCOPUS:19944392637
SN - 0009-2541
VL - 219
SP - 115
EP - 129
JO - Chemical Geology
JF - Chemical Geology
IS - 1-4
ER -