2020
DOI: 10.1144/jgs2019-188
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Unroofing the Ladakh Batholith: constraints from autochthonous molasse of the Indus Basin, NW Himalaya

Abstract: The Indus Molasse records orogenic sedimentation associated with uplift and erosion of the southern margin of Asia in the course of ongoing India–Eurasia collision. Detailed field investigation clarifies the nature and extent of the depositional contact between this molasse and the underlying basement units. We report the first dataset on detrital zircon U–Pb ages, Hf isotopes and apatite U–Pb ages for the autochthonous molasse in the Indus Suture Zone. A latest Oligocene depositional age is proposed on the ba… Show more

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Cited by 21 publications
(16 citation statements)
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“…Despite the relatively limited scope of our data, this is the first regionally extensive multithermchronometric study from the IBSRs and reveals a postdepositional Miocene‐Pliocene cooling signal along the India‐Asia collision zone in NW India. Deposition continued regionally along the collision zone until Late Oligocene‐Early Miocene time (~26–23 Ma; Bhattacharya et al, 2020; Clift et al, 2002; Sinclair & Jaffey, 2001; Zhou et al, 2020), and there is no unequivocal evidence of cooling beginning in the IBSRs until ~22–20 Ma. Using the ZHe and AHe data sets, we calculate the amount of material removed since the onset of cooling at ~22–20 Ma.…”
Section: Discussionmentioning
confidence: 99%
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“…Despite the relatively limited scope of our data, this is the first regionally extensive multithermchronometric study from the IBSRs and reveals a postdepositional Miocene‐Pliocene cooling signal along the India‐Asia collision zone in NW India. Deposition continued regionally along the collision zone until Late Oligocene‐Early Miocene time (~26–23 Ma; Bhattacharya et al, 2020; Clift et al, 2002; Sinclair & Jaffey, 2001; Zhou et al, 2020), and there is no unequivocal evidence of cooling beginning in the IBSRs until ~22–20 Ma. Using the ZHe and AHe data sets, we calculate the amount of material removed since the onset of cooling at ~22–20 Ma.…”
Section: Discussionmentioning
confidence: 99%
“…The Tar Group consists of carbonate and siliciclastic rocks that are tectonically bounded to the south by the precollisional Dras-Lamayuru-Nidar Complexes and are juxtaposed in the north against the Indus Group. The Indus Group exhibits extreme along-strike variations in siliciclastic fluvial facies that unconformably overlie the Ladakh batholith (Bhattacharya et al, 2020;Brookfield & Andrews-Speed, 1984;Clift et al, 2002;Garzanti & Van Haver, 1988;Henderson et al, 2010Henderson et al, , 2011Searle et al, 1990;Sinclair & Jaffey, 2001;Singh et al, 2015;Steck, 2003;St-Onge et al, 2010;Tripathy-Lang et al, 2013;Wu et al, 2007;Zhou et al, 2020). The Indus Group is categorized into two subgroups: (i) the Early Eocene-Early Miocene Lower Indus Group and (ii) the Pliocene Upper Indus Group.…”
Section: Stratigraphymentioning
confidence: 99%
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