TY - JOUR
T1 - Mineralogy and density of Archean volcanic crust in the mantle transition zone
AU - Ko, Byeongkwan
AU - Prakapenka, Vitali
AU - Kunz, Martin
AU - Prescher, Clemens
AU - Leinenweber, Kurt
AU - Shim, Sang Heon
N1 - Funding Information:
We are grateful for helpful discussions with E. J. Garnero, M. Li, A. K. McNamara, A. D. Anbar, S. J. Desch, C. Till, and R. L. Rudnick. K. Mossman and M. R. Gutierrez assisted with the FIB and STEM measurements at Arizona State University (ASU). Y.-J. Chang and P. Wallace assisted with the FIB and STEM measurements at University of Arizona. This study was supported by NSF (National Science Foundation, the United States) EAR-1725094, NSF EAR-1135452 (the Frontiers of Earth Systems Dynamics (FESD) program), and NASA (National Aeronautics and Space Administration, the United States) NExSS grant NNX15AD53G (PI S. J. Desch). The portions of this work was performed at GeoSoilEnviroCARS (The University of Chicago, Sector 13), Advanced Photon Source (APS), Argonne National Laboratory. GeoSoilEnviroCARS is supported by NSF - Earth Sciences (EAR-1634415) and Department of Energy (DOE) - GeoSciences (DE-FG02-94ER14466). Use of the COMPRES-GSECARS gas loading system was supported by COMPRES under NSF Cooperative Agreement EAR-1606856 and by GSECARS through NSF grant EAR-1634415 and DOE grant DE-FG02-94ER14466. This research used resources of the APS, a U.S. DOE Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. This research used resources of the Advanced Light Source, which is a DOE Office of Science User Facility under contract no. DE-AC02-05CH11231. Beamline 12.2.2 is supported by COMPRES, the Consortium for Materials Properties Research in Earth Sciences under NSF Cooperative Agreement EAR 10-43050. The experimental data are provided as a run table in supplementary material. There is no conflict of interest with this study.
Funding Information:
We are grateful for helpful discussions with E. J. Garnero, M. Li, A. K. McNamara, A. D. Anbar, S. J. Desch, C. Till, and R. L. Rudnick. K. Mossman and M. R. Gutierrez assisted with the FIB and STEM measurements at Arizona State University (ASU). Y.-J. Chang and P. Wallace assisted with the FIB and STEM measurements at University of Arizona. This study was supported by NSF ( National Science Foundation , the United States) EAR-1725094 , NSF EAR-1135452 (the Frontiers of Earth Systems Dynamics (FESD) program), and NASA ( National Aeronautics and Space Administration , the United States) NExSS grant NNX15AD53G (PI S. J. Desch). The portions of this work was performed at GeoSoilEnviroCARS (The University of Chicago, Sector 13), Advanced Photon Source (APS), Argonne National Laboratory. GeoSoilEnviroCARS is supported by NSF - Earth Sciences (EAR-1634415) and Department of Energy (DOE) - GeoSciences (DE-FG02-94ER14466). Use of the COMPRES-GSECARS gas loading system was supported by COMPRES under NSF Cooperative Agreement EAR-1606856 and by GSECARS through NSF grant EAR-1634415 and DOE grant DE-FG02-94ER14466. This research used resources of the APS, a U.S. DOE Office of Science User Facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357. This research used resources of the Advanced Light Source, which is a DOE Office of Science User Facility under contract no. DE-AC02-05CH11231. Beamline 12.2.2 is supported by COMPRES , the Consortium for Materials Properties Research in Earth Sciences under NSF Cooperative Agreement EAR 10-43050 . The experimental data are provided as a run table in supplementary material.
Publisher Copyright:
© 2020 Elsevier B.V.
PY - 2020/8
Y1 - 2020/8
N2 - The composition of Archean volcanic crust can be characterized by a higher Mg/Si ratio than modern mid-ocean ridge basalt (MORB), because of the higher degree melting from the warmer mantle in the Archean. Although modern MORB may become less dense than the surrounding mantle beneath the mantle transition zone (MTZ), the Mg-rich composition of Archean volcanic crust may result in the different density, and therefore different sinking behavior near the MTZ. In order to understand the compositional effect of Archean volcanic crust on the sinking behaviors and the scale of mantle mixing in the Archean, we investigated the mineralogy and density of Archean volcanic crust near the MTZ (470–910 km-depth). We conducted experiments at 19–34 GPa and 1400–2400 K using the laser-heated diamond anvil cell (LHDAC) combined with in-situ X-ray diffraction (XRD). The in-situ XRD and the chemical analysis revealed that Archean volcanic crust forms garnet and ringwoodite (84 and 16 vol%, respectively), which gradually transforms to Brg and CaPv (82 and 18 vol%, respectively) at 23–25 GPa and 1800 K. Our in-situ XRD experiments allowed us to measure the volumes of stable phases and to estimate their densities at high pressure and temperature. The results suggest that Archean volcanic crust maintains greater density than the pyrolitic mantle in the Archean regardless of temperature at 20–34 GPa (570–850 km-depth), promoting further sinking into the deeper mantle in the Archean. We also considered the density of the subducting slab in the Archean. The density model showed that the subducting slab is still denser or at least equally dense as the surrounding pyrolitic mantle in the Archean.
AB - The composition of Archean volcanic crust can be characterized by a higher Mg/Si ratio than modern mid-ocean ridge basalt (MORB), because of the higher degree melting from the warmer mantle in the Archean. Although modern MORB may become less dense than the surrounding mantle beneath the mantle transition zone (MTZ), the Mg-rich composition of Archean volcanic crust may result in the different density, and therefore different sinking behavior near the MTZ. In order to understand the compositional effect of Archean volcanic crust on the sinking behaviors and the scale of mantle mixing in the Archean, we investigated the mineralogy and density of Archean volcanic crust near the MTZ (470–910 km-depth). We conducted experiments at 19–34 GPa and 1400–2400 K using the laser-heated diamond anvil cell (LHDAC) combined with in-situ X-ray diffraction (XRD). The in-situ XRD and the chemical analysis revealed that Archean volcanic crust forms garnet and ringwoodite (84 and 16 vol%, respectively), which gradually transforms to Brg and CaPv (82 and 18 vol%, respectively) at 23–25 GPa and 1800 K. Our in-situ XRD experiments allowed us to measure the volumes of stable phases and to estimate their densities at high pressure and temperature. The results suggest that Archean volcanic crust maintains greater density than the pyrolitic mantle in the Archean regardless of temperature at 20–34 GPa (570–850 km-depth), promoting further sinking into the deeper mantle in the Archean. We also considered the density of the subducting slab in the Archean. The density model showed that the subducting slab is still denser or at least equally dense as the surrounding pyrolitic mantle in the Archean.
KW - Archean volcanic crust
KW - Density
KW - High P–T experiments
KW - In-situ X-ray diffraction
KW - Mantle transition zone
KW - Mineralogy
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U2 - 10.1016/j.pepi.2020.106490
DO - 10.1016/j.pepi.2020.106490
M3 - Article
AN - SCOPUS:85084948690
SN - 0031-9201
VL - 305
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
M1 - 106490
ER -