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Licensed Unlicensed Requires Authentication Published by De Gruyter February 9, 2017

High-pressure high-temperature Raman spectroscopy of kerogen: Relevance to subducted organic carbon

Laurel B. Childress EMAIL logo and Steven D. Jacobsen
From the journal American Mineralogist


The amount of insoluble macromolecular organic matter in the Earth’s crust, commonly referred to as kerogen, far exceeds the mass of living organic matter. The fraction of kerogen in sediments subducted into the mantle remains poorly constrained and will vary depending on the physical-chemical properties of kerogen along different slab geotherms. We studied the pressure-temperature evolution of carbon vibrational frequencies in isolated kerogen, previously not subjected to metamorphism, using Raman spectroscopy in a sapphire optical cell up to 3.2 GPa and 450 °C, correspondingto colder subduction geotherms. For blue-green laser excitation, we find optical irradiance exceeding ~3 kW/cm2 induces changes in spectral features of the primary graphitic (G-band) and two main disordered modes (D1 and D2) that might otherwise be mistaken for thermal maturation. Whereas previous in situ studies have investigated the changes in these molecular vibrations of kerogen at high temperature or high pressure, we collected Raman spectra of isolated kerogen at simultaneous high P-T conditions. Although instantaneous and irreversible changes in band ratios of isolated kerogen were observed above ~350°C at room-pressure, long-duration (2–8 h) heating experiments at 450 °C and 2.7–3.0 GPa reveal no permanent change in band structure. The reduction in vibrational frequencies of the disordered carbon modes with temperature (dv/dT) at pressures >1 GPa is slightly less than found at room pressure, further indicating that pressure effectively increases the thermal stability of kerogen. Our results suggest that kerogen reaching depths of 60 km where the temperature is below ~450 °C may subduct into the mantle, providing a potential source for the organic-rich component of carbon recently detected in certain lower-mantle diamonds.


This research was supported in part by NSF grant EAR-1452344, the David and Lucile Packard Foundation, and the Carnegie DOE Alliance Center to S.D.J. L.B.C. was supported in part by a Schlanger Scientific Ocean Drilling Fellowship and by NSF award OCE-1144483 to Neal Blair at Northwestern University. We thank M. Siqueira at Almax-easyLab for discussions about fabrication of custom sapphire-anvils and W.A. Bassett for help with construction of the high-temperature sapphire cell.

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Received: 2016-2-10
Accepted: 2016-9-12
Published Online: 2017-2-9
Published in Print: 2017-2-1

© 2017 by Walter de Gruyter Berlin/Boston

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