TY - JOUR
T1 - Regolith production rates calculated with uranium-series isotopes at Susquehanna/Shale Hills Critical Zone Observatory
AU - Ma, Lin
AU - Chabaux, Francois
AU - Pelt, Eric
AU - Blaes, Estelle
AU - Jin, Lixin
AU - Brantley, Susan
N1 - Funding Information:
This work benefitted from reviews by A. Dosseto, G. Hilley, and an anonymous reviewer, and editorial handling by P. Delaney. Discussions with P. Stille, P. Bierman, H. Lin, A. Dere, T. White, K. Singha, E. Kirby and R. Slingerland are also acknowledged. We thank Z. Ruge and B. Ketchum for help with regolith sampling. Logistical support and/or data were provided by the NSF-supported Susquehanna/Shale Hills Critical Zone Observatory. Financial support was provided by National Science Foundation Grant CHE-0431328 to SLB for Center for Environmental Kinetics Analysis and Grant EAR-0725019 to C. Duffy (Penn State) for Susquehanna Shale Hills Critical Zone Observatory. SLB and LM were partially funded by Department of Energy Grant DE-FG02-05ER15675 to SLB. Funding from the Region Alsace, France and the Laboratory network “REALISE” for LHyGeS (EOST), University of Strasbourg and CNRS to FC is also acknowledged.
PY - 2010/8
Y1 - 2010/8
N2 - In the Critical Zone where rocks and life interact, bedrock equilibrates to Earth surface conditions, transforming to regolith. The factors that control the rates and mechanisms of formation of regolith, defined here as material that can be augered, are still not fully understood. To quantify regolith formation rates on shale lithology, we measured uranium-series (U-series) isotopes (238U, 234U, and 230Th) in three weathering profiles along a planar hillslope at the Susquehanna/Shale Hills Observatory (SSHO) in central Pennsylvania. All regolith samples show significant U-series disequilibrium: (234U/238U) and (230Th/238U) activity ratios range from 0.934 to 1.072 and from 0.903 to 1.096, respectively. These values display depth trends that are consistent with fractionation of U-series isotopes during chemical weathering and element transport, i.e., the relative mobility decreases in the order 234U>238U>230Th. The activity ratios observed in the regolith samples are explained by i) loss of U-series isotopes during water-rock interactions and ii) re-deposition of U-series isotopes downslope. Loss of U and Th initiates in the meter-thick zone of "bedrock" that cannot be augered but that nonetheless consists of up to 40% clay/silt/sand inferred to have lost K, Mg, Al, and Fe. Apparent equivalent regolith production rates calculated with these isotopes for these profiles decrease exponentially from 45m/Myr to 17m/Myr, with increasing regolith thickness from the ridge top to the valley floor. With increasing distance from the ridge top toward the valley, apparent equivalent regolith residence times increase from 7kyr to 40kyr. Given that the SSHO experienced peri-glacial climate ~15kyr ago and has a catchment-wide averaged erosion rate of ~15m/Myr as inferred from cosmogenic 10Be, we conclude that the hillslope retains regolith formed before the peri-glacial period and is not at geomorphologic steady state. Both chemical weathering reactions of clay minerals and translocation of fine particles/colloids are shown to contribute to mass loss of U and Th from the regolith, consistent with major element data at SSHO. This research documents a case study where U-series isotopes are used to constrain the time scales of chemical weathering and regolith production rates. Regolith production rates at the SSHO should be useful as a reference value for future work at other weathering localities.
AB - In the Critical Zone where rocks and life interact, bedrock equilibrates to Earth surface conditions, transforming to regolith. The factors that control the rates and mechanisms of formation of regolith, defined here as material that can be augered, are still not fully understood. To quantify regolith formation rates on shale lithology, we measured uranium-series (U-series) isotopes (238U, 234U, and 230Th) in three weathering profiles along a planar hillslope at the Susquehanna/Shale Hills Observatory (SSHO) in central Pennsylvania. All regolith samples show significant U-series disequilibrium: (234U/238U) and (230Th/238U) activity ratios range from 0.934 to 1.072 and from 0.903 to 1.096, respectively. These values display depth trends that are consistent with fractionation of U-series isotopes during chemical weathering and element transport, i.e., the relative mobility decreases in the order 234U>238U>230Th. The activity ratios observed in the regolith samples are explained by i) loss of U-series isotopes during water-rock interactions and ii) re-deposition of U-series isotopes downslope. Loss of U and Th initiates in the meter-thick zone of "bedrock" that cannot be augered but that nonetheless consists of up to 40% clay/silt/sand inferred to have lost K, Mg, Al, and Fe. Apparent equivalent regolith production rates calculated with these isotopes for these profiles decrease exponentially from 45m/Myr to 17m/Myr, with increasing regolith thickness from the ridge top to the valley floor. With increasing distance from the ridge top toward the valley, apparent equivalent regolith residence times increase from 7kyr to 40kyr. Given that the SSHO experienced peri-glacial climate ~15kyr ago and has a catchment-wide averaged erosion rate of ~15m/Myr as inferred from cosmogenic 10Be, we conclude that the hillslope retains regolith formed before the peri-glacial period and is not at geomorphologic steady state. Both chemical weathering reactions of clay minerals and translocation of fine particles/colloids are shown to contribute to mass loss of U and Th from the regolith, consistent with major element data at SSHO. This research documents a case study where U-series isotopes are used to constrain the time scales of chemical weathering and regolith production rates. Regolith production rates at the SSHO should be useful as a reference value for future work at other weathering localities.
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U2 - 10.1016/j.epsl.2010.06.022
DO - 10.1016/j.epsl.2010.06.022
M3 - Article
AN - SCOPUS:77956009993
SN - 0012-821X
VL - 297
SP - 211
EP - 225
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
IS - 1-2
ER -