Current Issue

Volume 20

About the cover: Cathodoluminescence (CL)-RGB image of detrital quartz grains illustrating cements of different ages filling fractures and covering the outside of the grains. Different generations of cements have different CL-colours due to the physio-chemical conditions during formation. In Letter 2130, Hellevang et al. show that these CL-colour signatures together with textural characteristics and fluid inclusion temperatures can complement conventional methods used for unravelling past tectonism.
Photograph credit: Siri Simonsen. Download high-resolution cover.

In situ redox control and Raman spectroscopic characterisation of solutions below 300 °C

Abstract:
Redox reactions often occur and significantly affect many geological processes. To simulate redox reactions in low temperature (T < 400 °C) hydrothermal experiments, fused silica was used as a hydrogen membrane to impose an externally fixed H2 pressure (PH2) on a fused silica capillary capsule (FSCC; 150 μm inner diameter, 375 μm outer diameter and ∼6 mm long) to define the redox state of the sample in the FSCC. At 300 °C, it required less than 7 hours to reach osmotic equilibrium. In this study, a constant PH2 was imposed on an FSCC, which originally contained a 0.5 m (mole/kg H2O) SnCl4 + 0.5 m HCl aqueous solution, at 300 °C and vapour saturation pressure. In situ Raman spectra of the sample solution collected at 300 °C show that the reduction rate of SnIV to SnII species increased substantially with an increase of 1.1 bar of PH2. We characterised precipitation and dissolution of cassiterite under various P-T-pH-PH2 conditions and greatly increased our capabilities for performing rigorous hydrothermal experiments at temperatures below 400 °C, in which redox control is difficult to ensure without in situ approaches.

I.-M. Chou, R. Wang, J. Fang

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Geochem. Persp. Let. (2021) 20, 1–5 | doi: 10.7185/geochemlet.2135 | Published 2 December 2021

Early differentiation of magmatic iron meteorite parent bodies from Mn–Cr chronometry

Abstract:
Magmatic iron meteorite groups such as IIAB, IIIAB and IVA, represent the largest sampling of extraterrestrial core material from the earliest accreted distinct planetary bodies in the solar system. Chromium isotope compositions of chromite/daubréelite from seven samples, translated into 53Cr/52Cr model ages, provide robust time information on planetary core formation. These ages are within ∼1.5 Ma after formation of calcium-aluminium-rich inclusions (CAIs) and define the time of metal core formation in the respective parent bodies, assuming metal–silicate separation was an instantaneous event that induced strong chemical fractionation of Mn from the more siderophile Cr. The early core formation ages support accretion and differentiation of the magmatic iron meteorite parent bodies to have occurred prior to the chondrule formation interval. The calibration of Mn–Cr ages with established Hf–W ages of samples from the same magmatic iron meteorite groups constrains the initial ɛ53Cr of the solar system to −0.30 ± 0.05, and thus lower than previously estimated.

A. Anand, J. Pape, M. Wille, K. Mezger, B. Hofmann

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Geochem. Persp. Let. (2021) 20, 6–10 | doi: 10.7185/geochemlet.2136 | Published 13 December 2021

A novel carbon cycle turbulence index identifies environmental and ecological perturbations

Abstract:
Earth’s history has been characterised by complex interactions between life and the environment, which are often difficult to resolve. Here, we propose a new carbon cycle turbulence index (CTindex), based on the carbonate-carbon isotope (δ13Ccarb) record, to measure the extent of environmental perturbation over the last billion years. The CTindex trend is closely linked to Phanerozoic biotic extinction rates (ERs), as calculated from a palaeobiology database, supporting a strong environmental control on biotic ERs. We use the empirical CTindex—ER relationship to compare the extent of environmental perturbation due to greenhouse gas emissions with that during the Permian-Triassic (PTr) transition (∼252 Ma), representing the most severe mass extinction of the Phanerozoic. At the current peak of fossil fuel emissions, the CTindex indicates a moderate future environmental perturbation. However, if fossil fuel emissions increase into the next century, a pronounced CTindex peak greater than that which occurred during the PTr transition is indicated, which suggests the potential for a severe “sixth mass extinction” in the future.

Z.-H. Li, Z. Guo, Z.-Q. Chen, S.W. Poulton, Y. Bao, L. Zhao, F.-F. Zhang

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Geochem. Persp. Let. (2021) 20, 11–15 | doi: 10.7185/geochemlet.2137 | Published 30 December 2021

Comment on “190Pt-186Os geochronometer reveals open system behaviour of 190Pt-4He isotope system” by Luguet et al. (2019)

Abstract:

O.V. Yakubovich, A.G. Mochalov, V.M. Savatenkov, F.M. Stuart

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Geochem. Persp. Let. (2022) 20, 16–18 | doi: 10.7185/geochemlet.2201 | Published 13 January 2022

Reply to Comment on “190Pt-186Os geochronometer reveals open system behaviour of 190Pt-4He isotope system” by Yakubovich et al. (2022)

Abstract:

A. Luguet, G.M. Nowell, E. Pushkarev, C. Ballhaus

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Geochem. Persp. Let. (2022) 20, 19–21 | doi: 10.7185/geochemlet.2202 | Published 13 January 2022

Slab dehydration beneath forearcs: Insights from the southern Mariana and Matthew-Hunter rifts

Abstract:
The water flux delivered into the forearc mantle of currently active subduction zones remains poorly constrained. Estimates, which mostly derive from numerical modelling, have so far been untested, as shallow subduction processes are hindered by the serpentinised forearc mantle. Here, I examine the composition of near trench magmas from the southern Mariana and Matthew-Hunter rifts, which provides unique glimpses into slab dehydration underneath the forearcs of two modern subduction zones. The near trench magmas captured the water-rich slab fluids that usually serpentinise the cold forearc mantle. The near trench magmas possess higher markers in slab dehydration (Rb/Th = 3–141, Cs/Th = 0.04–17.79, H2O/Ce = 436–23,531) than do arc and back-arc magmas, implying that the subducted plates might dehydrate efficiently within 80 km from the trench.

J.M. Ribeiro

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Geochem. Persp. Let. (2021) 20, 22–26 | doi: 10.7185/geochemlet.2203 | Published 19 January 2022

Nitrogen isotope fractionation during magma ocean degassing: tracing the composition of early Earth’s atmosphere

Abstract:
The evolution of the nitrogen concentration and isotopic composition during the degassing of Earth’s magma ocean, and thus in the primitive atmosphere, is key to understanding how habitable conditions developed on Earth. To constrain nitrogen degassing from the magma ocean, we determined the variations of the N content at N2 gas saturation, N speciation, and N isotopic composition of a magma ocean analogue (basaltic komatiite) at oxygen fugacities (fO2) from IW−4.2 to IW (where IW is the logarithmic difference between experimental fO2 and that at Fe-FeO equilibrium). We performed a series of N degassing experiments in a piston cylinder at 1.5 GPa and 1550 °C in pure forsterite capsules. N concentrations in the mafic silicate melts decreased from 13,481 ± 735 ppm under the most reducing conditions to 798 ± 4 ppm at IW, controlled by N speciation (as determined by Raman spectroscopy), which changed from nitride (±N-H complexes) to molecular N2 with increasing fO2. Nitrogen occurs solely as N2 in the degassed gas, regardless of fO2. Nitrogen isotopic compositions (as determined by secondary ion mass spectroscopy) became significantly lighter in the degassed melt (quenched glass), down to −41 ± 13 ‰ relative to the initial composition (measured in an undegassed sample), following open system degassing trends (variable with fO2 conditions), indicative of Rayleigh fractionation. These findings imply that an atmosphere in equilibrium with a reduced magma ocean would be N-depleted, whereas with increasing magma ocean fO2 conditions, the primitive atmosphere would have become more enriched in N2 gas.

C. Dalou, C. Deligny, E. Füri

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Geochem. Persp. Let. (2021) 20, 27–31 | doi: 10.7185/geochemlet.2204 | Published 19 January 2022