2018
DOI: 10.1002/2017gc007191
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Zircon (U‐Th)/He Thermochronometric Constraints on Himalayan Thrust Belt Exhumation, Bedrock Weathering, and Cenozoic Seawater Chemistry

Abstract: Shifts in global seawater 187Os/188Os and 87Sr/86Sr are often utilized as proxies to track global weathering processes responsible for CO2 fluctuations in Earth history, particularly climatic cooling during the Cenozoic. It has been proposed, however, that these isotopic records instead reflect the weathering of chemically distinctive Himalayan lithologies exposed at the surface. We present new zircon (U‐Th)/He thermochronometric and detrital zircon U‐Pb geochronologic evidence from the Himalaya of northwest I… Show more

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Cited by 31 publications
(50 citation statements)
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“…Studies of sandstone petrography and conglomerate clast composition, along with Nd isotope geochemistry of conglomerate clasts from the Kangra reentrant (Figure ), suggest that the inner‐Lesser Himalayan Sequence (iLHS) was already eroding at ~11 Ma (Brozovic & Burbank, ; Meigs et al, ; Najman et al, ). This inferred age for the onset of erosional unroofing of the iLHS agrees well with Nd isotopic results from the central Himalaya in Nepal (Huyghe et al, , ; Robinson et al, ) and with zircon (U‐Th)/He thermochronological data from outer‐Lesser Himalayan Sequence (oLHS) and iLHS rocks of the northwestern Indian Himalaya (Colleps et al, ). However, based on detrital zircon U‐Pb geochronological and Hf isotopic data from Late Paleocene to mid‐Miocene Sub‐Himalayan foreland basin deposits in the Subathu salient (Figure ), Ravikant et al () proposed sediment input from the iLHS as early as Late Paleocene/Early Eocene.…”
Section: Introductionsupporting
confidence: 87%
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“…Studies of sandstone petrography and conglomerate clast composition, along with Nd isotope geochemistry of conglomerate clasts from the Kangra reentrant (Figure ), suggest that the inner‐Lesser Himalayan Sequence (iLHS) was already eroding at ~11 Ma (Brozovic & Burbank, ; Meigs et al, ; Najman et al, ). This inferred age for the onset of erosional unroofing of the iLHS agrees well with Nd isotopic results from the central Himalaya in Nepal (Huyghe et al, , ; Robinson et al, ) and with zircon (U‐Th)/He thermochronological data from outer‐Lesser Himalayan Sequence (oLHS) and iLHS rocks of the northwestern Indian Himalaya (Colleps et al, ). However, based on detrital zircon U‐Pb geochronological and Hf isotopic data from Late Paleocene to mid‐Miocene Sub‐Himalayan foreland basin deposits in the Subathu salient (Figure ), Ravikant et al () proposed sediment input from the iLHS as early as Late Paleocene/Early Eocene.…”
Section: Introductionsupporting
confidence: 87%
“…However, based on detrital zircon U‐Pb geochronological and Hf isotopic data from Late Paleocene to mid‐Miocene Sub‐Himalayan foreland basin deposits in the Subathu salient (Figure ), Ravikant et al () proposed sediment input from the iLHS as early as Late Paleocene/Early Eocene. This age seems at odds with kinematic reconstructions of the Himalaya, which suggest that exhumation of the iLHS initiated with the growth of the LHD in the Late Miocene (e.g., DeCelles et al, , and references therein; Srivastava & Mitra, ; Webb, ; Webb et al, ), which is also suggested by Lesser Himalayan bedrock cooling age data (e.g., Colleps et al, ).…”
Section: Introductionmentioning
confidence: 94%
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“…Because our ages do not display such correlation (supporting information Figure S1), we expect that our samples were not affected by considerable radiation damage. Thus, the obtained average ZHe ages represent the time at which the samples cooled through an effective closure temperature range of ~180 to 200 °C (e.g., Colleps et al, ; Guenthner et al, ; Reiners et al, , ; Wolfe & Stockli, ). Furthermore, the lack of age‐eU correlations in all samples suggests that the samples moved rapidly through the partial retention zone (PRZ).…”
Section: Thermochronology Resultsmentioning
confidence: 99%
“…In this work, we use zircon (U‐Th)/He thermochronology (ZHe) to understand the thermal history of the Searchlight pluton and relate this history to possible mechanisms for its exhumation. We chose ZHe because of the moderate closure temperature of the system (180–200 °C to as low as ~130 °C; Reiners et al, , ; Wolfe & Stockli, ; Guenthner et al, ; Colleps et al, ). Specifically, we aimed to constrain the cooling history of this pluton—intruded at approximately 750 °C—as it was exhumed rapidly toward the surface.…”
Section: Methodsmentioning
confidence: 99%