EGU25-11961, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-11961
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Friday, 02 May, 08:45–08:55 (CEST)
 
Room D2
Mid-crustal overpressure in the Tethyan Himalaya
Dominik R. Vlaha1, Andrew V. Zuza1, Victor E. Guevara2, Peter J. Haproff3, A. Alexander G. Webb4, Francisco Reyes2, Marie C. Genge5, Ariuntsetseg Ganbat6, Devynn Wilderman2, and Birendra P. Singh7
Dominik R. Vlaha et al.
  • 1Nevada Geosciences, University of Nevada, Reno, U.S.A, (dvlaha@unr.edu)
  • 2Amherst College, U.S.A
  • 3University of North Carolina Wilmington, U.S.A.
  • 4Freie Universität Berlin, Germany
  • 5The University of Hong Kong, Hong Kong S.A.R. China
  • 6University of Göttingen, Germany
  • 7Panjab University, India

Theory suggests the possibility for significant deviations between total pressure (or dynamic pressure) and lithostatic pressure during crustal metamorphism. If such deviations exist, the implications for orogenic reconstruction would be profound. Whether such non-lithostatic pressure conditions during crustal metamorphism are recorded and preserved in the rock record remains unresolved, as direct field evidence for this phenomenon is limited. Here, we investigate the Paleogene Tethyan Himalaya fold-thrust belt in Himachal Pradesh, northwestern India, which is the structurally highest part of the Himalayan orogen and deforms a ~10–15 km thick Neoproterozoic–Cretaceous passive margin stratigraphic section. Field-based kinematic studies demonstrate relatively moderate shortening strain across the Tethyan Himalaya. However, basal Tethyan strata consistently yield elevated pressure-temperature-time (P-T-t) estimates of 7–8 kbar and ~650°C, indicative of deep burial during Himalayan orogeny (ca. 20–45 Ma, 25–30 km depths). These P-T-t conditions can be reconciled by: (1) deep Cenozoic burial along cryptic structures and/or significant flattening of the Tethyan strata; (2) basal Tethyan strata recording metamorphism and deformation related to pre-Himalayan tectonism; or (3) non-lithostatic pressure conditions (i.e., tectonic overpressure).

 

To test these models, we systematically mapped the Tethyan fold-thrust belt along the Pin Valley transect in northwestern India, a classic site for stratigraphic, paleontological, paleoenvironmental, and structural reconstructions. The Pin Valley region provides an opportunity to study a structurally continuous metamorphic field gradient from the near-surface to structural depths between 10–15 km, which should reflect P conditions ≤4 kbar if lithostatic. We integrate a multi-method approach combining detailed geologic mapping with quantitative analytical techniques (e.g., thermometry, finite strain analyses, thermo/geochronology, and thermobarometry) to quantify the magnitude, kinematics, thermal architecture, and timing of regional deformation, metamorphism, and subsequent exhumation. Results show: (1) throw on shortening structures is moderate to low (≤4 km); (2) temperature-depth relationships record a continuous, but regionally elevated, upper-crustal geothermal gradient of ≥40 °C/km, which is inconsistent with deep burial models (≤25 °C/km); (3) minimal flattening of basal Tethyan strata; (4) upper Tethyan strata yield pre-Himalayan low-temperature thermochronology dates, further refuting deep Cenozoic burial; and (5) basal Tethyan P-T-t estimates confirm elevated mid-crustal conditions of ~7 kbar, 630°C at 10–15 km depths during the Cenozoic. Preliminary volume expansion calculations are minimal; therefore, mechanisms involving non-hydrostatic thermodynamics, deviatoric stresses, rock strength contrasts, and tectonic mode switching are being explored.

How to cite: Vlaha, D. R., Zuza, A. V., Guevara, V. E., Haproff, P. J., Webb, A. A. G., Reyes, F., Genge, M. C., Ganbat, A., Wilderman, D., and Singh, B. P.: Mid-crustal overpressure in the Tethyan Himalaya, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11961, https://doi.org/10.5194/egusphere-egu25-11961, 2025.