EGU21-15948
https://doi.org/10.5194/egusphere-egu21-15948
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

High-speed tensile fractures in granite and gneiss: an experimental study

Beno J Jacob1, Santanu Misra1, Venkitanarayanan Parameswaran2, and Nibir Mandal3
Beno J Jacob et al.
  • 1Indian Institute of Technology, Kanpur, indian Institute of Technology, Department of Earth Sciences, Kanpur, India
  • 2Indian Institute of Technology, Kanpur, indian Institute of Technology, Department of Mechanical Engineering, Kanpur, India
  • 3Jadavpur University, Department of Geological Sciences, Kolkata, India

Tensile fractures are ubiquitous in impact structures formed because of high strain rate deformations of the earth’s crust. At regions far from the point of meteorite impact, intense rupturing, fragmentation, and pulverisation are an implication of pressure waves limiting at the tensile strength of the host rock with little influence of shock deformation or shear failure. The branching and anastomosing of the fractures are controlled by the local stress state and anisotropy. Thus, a network of infilled fractures or impact breccia dikes is a common feature in the subsurface of impact sites.

We have investigated the failure processes under high strain rates responsible for the formation of Mode-I breccia dikes, at the laboratory scale. The control of planar fabric structures in the development of anastomosing tensile fracture networks was studied through high-strain-rate Brazilian disc tests on gneiss (foliated) and granite (isotropic) samples. A Split Hopkinson Pressure Bar, equipped with high-speed photography (~105 fps), was employed in the study. The gneissic foliation in the gneiss samples were oriented at θ = 0, 45 and 90° to the compression direction. The strength of granite lies between 24 and 26 MPa, and the gneisses failed in the range of 29-37MPa at about 70-90 μs. The fracture network formation was seen in the time series images. There is a stark disparity in the nature of failure of granite from gneiss and the geometry of clasts formed in each rock type. While granite samples fail with pulverised clasts localised along a single fracture spanning the diameter of the sample along the compression direction, the gneisses further developed a network of secondary fractures forming large elongate clasts. Preferential orientation of secondary crack growth in relation to the foliation is strongly influenced by θ in gneiss samples. The aspect ratio of the pulverised clasts (size < 10mm) formed in granite was about 1:2, whereas the gneisses produced larger clasts. The clasts in gneisses had an aspect ratio of 1:4 for θ = 45 and 90º, and 1:5 for θ = 0º.

The branching and anastomosing nature of fractures is similar in fracture networks observed from the field and in the experiments, thus providing an insight into the formation of high-speed impact breccia dikes in isotropic and foliated rocks. Our experiments demonstrate that monomict breccia dikes may by formed in situ inclusive of clasts, rather than by infilling in previously formed tensile fractures.

How to cite: Jacob, B. J., Misra, S., Parameswaran, V., and Mandal, N.: High-speed tensile fractures in granite and gneiss: an experimental study, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-15948, https://doi.org/10.5194/egusphere-egu21-15948, 2021.

Corresponding displays formerly uploaded have been withdrawn.