Abstract.
The 40-km-diameter Mjølnir crater is proposed to have resulted from an oblique impact from the south/southwest direction and at a ~45° (possibly 30°–45°) angle from the horizontal. This is substantiated by several diagnostic structural and geophysical signatures related to obliquity and revealed through detailed re-assessment of Mjølnir’s well-established structure, morphology, and gravity and seismic velocity anomalies. The diagnostic signatures include: (1) a dominant N-S/NNE-SSW crater diameter elongation, (2) a consistent northward asymmetry both in the crater radius and the shallow part of the impact-induced seismic disturbance, (3) a peak ring breached towards the N/NE, (4) an annular gravity low with a horseshoeshape open towards the NE, (5) a transient cavity maximum-depth offset of 2 to 2.5 km towards south-southwest from the geometric crater center, combined with a similar structural uplift lateral offset towards the south, a similar central gravity high offset towards southwest, and an elongated traveltime central anomaly offset towards WSW. The oblique Mjølnir impact most probably generated a down-range sector/corridor of thicker ejecta deposits and faster travelling tsunami-waves, triggering short-term regional perturbations that are probably intensified within and adjacent to this sector.
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Tsikalas, F. (2005). Mjølnir Crater as a Result of Oblique Impact: Asymmetry Evidence Constrains Impact Direction and Angle. In: Koeberl, C., Henkel, H. (eds) Impact Tectonics. Impact Studies. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-27548-7_10
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