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Featured researches published by R. Kessel.


Nature | 2005

Trace element signature of subduction-zone fluids, melts and supercritical liquids at 120–180 km depth

R. Kessel; Max W. Schmidt; Peter Ulmer; Thomas Pettke

Fluids and melts liberated from subducting oceanic crust recycle lithophile elements back into the mantle wedge, facilitate melting and ultimately lead to prolific subduction-zone arc volcanism. The nature and composition of the mobile phases generated in the subducting slab at high pressures have, however, remained largely unknown. Here we report direct LA-ICPMS measurements of the composition of fluids and melts equilibrated with a basaltic eclogite at pressures equivalent to depths in the Earth of 120–180 km and temperatures of 700–1,200 °C. The resultant liquid/mineral partition coefficients constrain the recycling rates of key elements. The dichotomy of dehydration versus melting at 120 km depth is expressed through contrasting behaviour of many trace elements (U/Th, Sr, Ba, Be and the light rare-earth elements). At pressures equivalent to 180 km depth, however, a supercritical liquid with melt-like solubilities for the investigated trace elements is observed, even at low temperatures. This mobilizes most of the key trace elements (except the heavy rare-earth elements, Y and Sc) and thus limits fluid-phase transfer of geochemical signatures in subduction zones to pressures less than 6 GPa.


Earth and Planetary Science Letters | 1997

Chromatographic metasomatism of the Arabian—Nubian lithosphere

Mordechai Stein; Oded Navon; R. Kessel

Abstract Trace elements and isotopic ratios of calc-alkaline and tholeiitic dikes from the very last stage of the late Proterozoic, Pan-African orogeny in the northern Arabian–Nubian Shield (ANS), and alkali basalts from the overlying Phanerozoic section are used to constrain the composition and model the evolution of the lithospheric mantle in this region. The dikes and basalts are interpreted as lithospheric melts formed during the post-orogenic (and post-subduction) history of the shield. While the mafic member of all suites share a primitive La/Th ratio, the Nb/Th and Ce/Pb are distinct for each suite. The (Nb/Th) PM (primitive mantle normalized) is ∼0.2 in the calc-alkaline dikes and 1.4 in the tholeiitic dikes and the Phanerozoic alkali basalts. The (Ce/Pb) PM ratios are low in the dikes (0.4 in the calc-alkaline and 0.3 in the tholeiitic) and high in the Phanerozoic basalts (2.8). We suggest that the variations in the trace element ratios reflect sampling of different zones in the lithospheric mantle, which were formed by subduction related metasomatism of the mantle wedge. We constructed a chromatographic model to explain this zonation. In this model a plume-derived oceanic lithosphere is subducted and dehydrates at depth. Fluids released from the dehydrating slab metasomatize the overlying wedge and form amphibole-rich channels. Nb is preferentially taken by the amphibole and is enriched only in the lower zones of the column. The other elements (U, Th, REE and especially Pb and Rb) behave incompatibly. They are enriched in the fluid and transported efficiently to the melting zone in the centre of the wedge. Dehydration of the base of the wedge as it descends below the amphibole stability field depletes this region in Pb and Rb. After the end of subduction, the wedge is fossilized and forms the lithospheric mantle. The zone above the Nb concentration front is sampled by the calc-alkaline magmas. The tholeiitic magmas sample the zone below the Nb front. The Phanerozoic alkali basalts sample the dehydrated base where Nb is high and Pb and Rb low. Trace element patterns in amphibole xenoliths from Mount Carmel, Israel, are similar to the models prediction for amphibole in the residual base of the lithosphere. The model correctly reproduces the major features in the isotopic evolution of the Arabian–Nubian lithosphere, and has implications for the formation of HIMU-type magmas in mid-plate environments.


American Mineralogist | 2004

A novel approach to determine high-pressure high-temperature fluid and melt compositions using diamond-trap experiments

R. Kessel; Peter Ulmer; Thomas Pettke; Mark W. Schmidt; Alan Bruce Thompson

Abstract We have developed a novel analytical technique for diamond-trap experiments to directly analyze high-pressure, high-temperature fluid and melt compositions in equilibrium with mantle material. Experiments were conducted at a pressure of 6 GPa and temperatures between 900-1200 °C in a multi-anvil apparatus with a synthetic K-free eclogite doped with 860 ppm Cs, ~20 wt% H2O, and a layer of diamond aggregates serving as a fluid/melt trap. Experiments at identical conditions were analyzed with two different methods. In the new, “freezing,” approach, the capsule was frozen prior to opening and kept frozen during laser-ablation ICP-MS analysis, thus ablating the quenched fluid (precipitates together with water that unmixed upon quenching) in a solid state. Cesium, fractionating completely into the fluid or melt phase, was used as an internal standard for calculating the fluid compositions. Calculated uncertainties on H2O content in the fluid composition are 0.7-2.5%. In the conventional “evaporation” approach, water from the unmixed fluid was first evaporated from the capsule, then the remaining fluid precipitates were analyzed by LA-ICP-MS. The compositions of the residual eclogitic minerals were measured by electron microprobe, and the fluid composition was then determined by mass-balance. Uncertainties in mineral compositions lead to poor precision in fluid composition in this latter approach. Results of the two methods of fluid analysis were found to be in good agreement. Because the “freezing” approach analyzes the entire fluid directly and does not rely on mass balance for calculating fluid compositions, our new method provides a superior means for determining the composition of fluids. Secondly, it avoids loss of cations that remain soluble in water (e.g., Cs, K) after quenching the experiment.


American Mineralogist | 2001

Thermodynamic properties of the Pt-Fe system

R. Kessel; John R. Beckett; Edward M. Stolper

Abstract We determined activity-composition relationships for the Pt-Fe system by equilibrating Fe-oxides with Pt-Fe alloys at temperatures in the range of 1200-1400 °C and oxygen fugacities from 1.6 to 7.7 log units above the iron-wüstite (IW) buffer. The system is characterized by strong negative deviations from ideality throughout the investigated temperature range (e.g., γalloyFe<0.02 for XalloyFe <0.3). Our data are consistent with an asymmetric regular solution of the form: RT ln γalloyFe=[WG1+2(WG2-WG1)XalloyFe](XalloyPt)2 where WG1 = -138.0 ± 3.3 kJ/mol and WG2 = -90.8 ± 24.0 kJ/mol (1σ). Based on experiments at 1200-1400 °C, variations in the activity coefficients at a given composition are consistent with ln γ alloyFe(T1) / ln γalloyFe(T2) = T2 / T1. The Pt-Fe alloy composition in equilibrium with a FeO-bearing silicate liquid can be obtained from: where ΔG0r is the standard state free energy for the reaction 2Fealloy + O2gas +SiO2liq = Fe2SiOliq4 . We obtained values of αalloyFe from our model and used the program MELTS together with the thermodynamic properties of these elements to evaluate activities of SiO2 and Fe2SiO4 components in the liquid and ΔG0r . We provide sample calculations showing how to predict the optimum Fe concentrations for pre-saturation of Pt-bearing containers to reduce Fe loss from the charge during experiments on magmatic liquids at high temperatures and pressures from 1 atm to 40 kbar.


Geochimica et Cosmochimica Acta | 2003

Experimental determination of the activity of chromite in multicomponent spinels

R. Kessel; John R. Beckett; Edward M. Stolper

We determined activity–composition relationships in Pt-Cr and Pt-Fe-Cr alloys at 1300°C experimentally and used the results to constrain the thermodynamic properties of chromite–picrochromite spinels. The Pt-Cr binary is characterized by strong negative deviations from ideality throughout the investigated composition range and the activity–composition relationship can be fit by a four-suffix asymmetric regular solution with three binary interaction parameters. The ternary alloy was modeled as a four-suffix asymmetric regular solution; the three ternary interaction parameters in this model were constrained by combining interaction parameters for the three bounding binaries taken from this and previous work with results for a set of experiments in which the activity of Cr in Pt-Fe-Cr-alloys was fixed by coexisting Cr_(2)O_3 at known fO_2. The free energy of formation of FeCr_(2)O_4 at 1300°C was determined using the activities of Fe and Cr in Pt-alloys in equilibrium with oxide mixes of FeCr_(2)O_4 and Cr_(2)O_3. The free energy of formation of chromite from Fe+Cr_(2)O_3+O_2 is −202.7 ± 0.4 kJ/mol (1σ), indistinguishable from literature values. The corresponding free energy of formation of FeCr_(2)O_4 from the elements is −923.5 ± 2.1 kJ/mol (1σ), and the enthalpy of formation at 298 K is −1438 kJ/mol. The activity–composition relationship for the chromite component in (Fe,Mg)Cr_(2)O_4 solid solutions was determined from a set of experiments in which Pt-alloys were equilibrated with spinel + Cr_(2)O_3. (Fe,Mg)Cr_(2)O_4 spinels are nearly ideal at 1300°C; modeling our data with a one-site symmetric regular solution yields an interaction parameter of +2.14 ± 0.62 kJ/mol (1σ), similar to values based on data from the literature.


Earth and Planetary Science Letters | 2005

The water–basalt system at 4 to 6 GPa: Phase relations and second critical endpoint in a K-free eclogite at 700 to 1400 °C

R. Kessel; Peter Ulmer; Thomas Pettke; Mark W. Schmidt; Alan Bruce Thompson


Lithos | 2009

A new model for the evolution of diamond-forming fluids: Evidence from microinclusion-bearing diamonds from Kankan, Guinea

Y. Weiss; R. Kessel; William L. Griffin; I. Kiflawi; Ofra Klein-BenDavid; D.R. Bell; J.W. Harris; Oded Navon


Geochimica et Cosmochimica Acta | 2007

The thermal history of equilibrated ordinary chondrites and the relationship between textural maturity and temperature

R. Kessel; John R. Beckett; Edward M. Stolper


Precambrian Research | 1998

Petrogenesis of late Neoproterozoic dikes in the northern Arabian–Nubian Shield: Implications for the origin of A-type granites

R. Kessel; Mordechai Stein; Oded Navon


Earth and Planetary Science Letters | 2011

Geomagnetic field intensity: How high can it get? How fast can it change? Constraints from Iron Age copper slag

Ron Shaar; E. Ben-Yosef; Hagai Ron; Lisa Tauxe; Amotz Agnon; R. Kessel

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Amotz Agnon

Hebrew University of Jerusalem

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Hagai Ron

Hebrew University of Jerusalem

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Ron Shaar

Hebrew University of Jerusalem

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Lisa Tauxe

University of California

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Oded Navon

Hebrew University of Jerusalem

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E. Ben-Yosef

University of California

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Mordechai Stein

Hebrew University of Jerusalem

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