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Geologic map of the Marsyandi drainage, central Nepal digitized from the combined maps of Searle & Godin (2003) and Colchen et al. (1986). Solid lines represent the Main Central Thrust and South Tibetan Detachment (STD) as mapped by Searle & Godin (2003). The dashed line is the STD as mapped by Colchen et al. (1986). U^Pb zircon age distributions are shown for samples of river sediment taken from either tributaries draining single geologic units (A, C, D, F, H and I) or the main stem Marsyandi (B, E, G and K). 

Geologic map of the Marsyandi drainage, central Nepal digitized from the combined maps of Searle & Godin (2003) and Colchen et al. (1986). Solid lines represent the Main Central Thrust and South Tibetan Detachment (STD) as mapped by Searle & Godin (2003). The dashed line is the STD as mapped by Colchen et al. (1986). U^Pb zircon age distributions are shown for samples of river sediment taken from either tributaries draining single geologic units (A, C, D, F, H and I) or the main stem Marsyandi (B, E, G and K). 

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Fission-track and Ar-Ar dating of detrital minerals such as zircon and muscovite in foreland sediments provide estimates of exhumation rate during different periods of orogen growth. Interpretations of foreland cooling ages often assume that a population of foreland minerals provides a representative sample of the entire orogen. In reality, differe...

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... ¢rst part of our study focuses on the Marsyandi drai- nage, where six modern sand samples (A, C, D, F, H and I) were taken from small tributaries to de¢ne the contribu- tion from speci¢c formations (Fig. 4). Additionally, four sand samples were taken from the Marsyandi River where it crosses the STD (B), the Formation I^II contact (E), the MCT (G) and just above the con£uence with the Trisuli River (K). These samples were deliberately taken just downstream of where the Marsyandi crosses formational boundaries and were used to determine ...
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... tethyan strata (n = 962) (1986) and Fuchs (1980), with priority given in that order where features were inconsistent between maps (Fig. 4). Such a combination of maps was necessary because the oldest map was too large in scale and lacked su⁄cient de- tail in the Marsyandi region, while the younger two were not spatially extensive enough to cover the entire ¢eld area. As a result, the locations of features within the Marsyandi drainage are highly accurate, whereas some ...
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... distributions from the Marsyandi drainage show clear downstream trends re£ecting the input of zircons from successive formations (Fig. 4). Sample B characterizes the age distribution of the Marsyandi as it emerges from post- Ordovician Tethyan units. The trunk river then receives contributions from Formations II and III, which, based on their similarity, are treated as a single source in mixing calculations. Downstream of Formation II, sample E con- tains a large ...
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... II and III, which, based on their similarity, are treated as a single source in mixing calculations. Downstream of Formation II, sample E con- tains a large proportion of ages o700 Ma and a relative paucity of ages 41000 Ma, suggesting a larger contribu- tion from Formation II/III than would be expected based on its limited exposure area (Fig. 4 and Table 4). Further downstream, sample G shows a strong peak between 900 and 1000 Ma, and more ages 41000 Ma indicating a mod- erate, but not dominant, contribution from Formation I (sample F; Fig. 4). Samples H and I (Fig. 4) characterize Lesser Himalayan age distributions that are in excellent agreement with pre- viously reported ...
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... paucity of ages 41000 Ma, suggesting a larger contribu- tion from Formation II/III than would be expected based on its limited exposure area (Fig. 4 and Table 4). Further downstream, sample G shows a strong peak between 900 and 1000 Ma, and more ages 41000 Ma indicating a mod- erate, but not dominant, contribution from Formation I (sample F; Fig. 4). Samples H and I (Fig. 4) characterize Lesser Himalayan age distributions that are in excellent agreement with pre- viously reported ages shown in Fig. 3 (DeCelles et al., 2000; Martin et al., 2005).The contribution of Lesser Himalayan zircons is clear in sample K (Fig. 4) from the lowest Mar- syandi, which contains large peaks at ...
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... Ma, suggesting a larger contribu- tion from Formation II/III than would be expected based on its limited exposure area (Fig. 4 and Table 4). Further downstream, sample G shows a strong peak between 900 and 1000 Ma, and more ages 41000 Ma indicating a mod- erate, but not dominant, contribution from Formation I (sample F; Fig. 4). Samples H and I (Fig. 4) characterize Lesser Himalayan age distributions that are in excellent agreement with pre- viously reported ages shown in Fig. 3 (DeCelles et al., 2000; Martin et al., 2005).The contribution of Lesser Himalayan zircons is clear in sample K (Fig. 4) from the lowest Mar- syandi, which contains large peaks at $1800 and 2400 Ma. The ...
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... a mod- erate, but not dominant, contribution from Formation I (sample F; Fig. 4). Samples H and I (Fig. 4) characterize Lesser Himalayan age distributions that are in excellent agreement with pre- viously reported ages shown in Fig. 3 (DeCelles et al., 2000; Martin et al., 2005).The contribution of Lesser Himalayan zircons is clear in sample K (Fig. 4) from the lowest Mar- syandi, which contains large peaks at $1800 and 2400 Ma. The importance of the Tethyan Series and Formation II/ III contributions to sample K is apparent in the high age probability between $480 and 700 Ma. This interpreta- tion is con¢rmed by comparison with sample J, which contains noTethyan or Formation II/III ...
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... from generalizing from speci¢c sites to broader areas. For example, in the present study we treat the Tethyan Series as a single unit, even though it com- prises carbonates and siliclastics that have highly contrast- ing zircon concentrations. We de¢ne the zircon age distributions based on two samples from catchments with- in theTethyan rocks (Fig. 4).We did not speci¢cally sample Cambro -Ordovician Tethyan strata, and yet we now sus- pect that they contain an age signal that is more equivalent to that of Formation II than to that of the 'Tethyan' popula- tion that we ...

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