Abstract
During impact, the passage of the shock wave results in extensive in situ fracturing and autochthonous target rock brecciation. Target material is excavated and ejected in ballistic trajectories upward and outward from the impact site. As excavation of the brecciated volume advances, the excavated crater is formed. It delimits the provenance of material expelled from the crater and provides the void space for subsequent infilling of allogenic material and breccia (e.g., Melosh 1989; Turtle et al. 2005). Therefore, the disturbance beneath Mjølnir is expected to be associated with two types of breccia: allochtonous and autochthonous (Tsikalas et al. 1998b, 1999).
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Tsikalas, F., Faleide, J.I., Werner, S.C., Torsvik, T., Gudlaugsson, S.T., Eldholm, O. (2010). Impact Geophysics and Modelling. In: Tsikalas, F., Dypvik, H., Smelror, M. (eds) The Mjølnir Impact Event and its Consequences. Impact Studies. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-88260-2_4
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