Abstract

The present study involves different aspect of brittle failure structures at Spi Res Anticline within the foreland fold belt of north Iraq. It aims to decipher whether the late Cretaceous orogenic episode has any fracturing consequence to the rock sequence of this period at investigated area. This was accomplished by comparison of various fracture modes between Upper Cretaceous and Tertiary rock sequence exposed at studied area. The study area is prevailed with widespread joints and tabular veins, little mesoscopic faults and scarce of pressure solution surfaces (stylolite). Joint analysis showed two extensional sets (ac and bc) and three shear systems (hko, hol and okl). However, hko acute about a and b system was prevailed and followed by ac and bc sets. The openings of most of joint sets were filled later by calcareous or siliceous precipitations without any kinematic indications, some refers to extension normal with vein walls and for a single growth episode. A little number of striated mesoscopic faults were registered throughout both Cretaceous and Tertiary rocks in study area. Most of them are reverse, others are normal and strike slip. Further, two sets of stylolite seams were found scarcely, peaks of the first oriented parallel with the bedding dip, whereas those of the other set trended parallel to bedding strike. The kinematic analysis of mesoscopic faults and shear joints in study area gave a number of compressive and strike slip stress tensors. The maximum horizontal stress (δmax ) of these tensors lie in N-S, NE-SW, E-W and NW-SE general trends. Accordingly, they were organized into two compressive tectonic regimes. One representing the component normal to the orogenic front, acted in N-S and NE-SW directions. Whereas the other representing the component parallel with the orogenic front, acted in E-W and NW-SE directions. Both components were resulted from oblique collision of Arabian and Eurasian plates. However, these two compressive tectonic regimes are supported by a couple sets of stylolites with their peaks either normal or parallel to the trend of Spi Res Anticline. No brittle failure structures belonging to orogenic episode of Late Cretaceous were recognized in the Upper Cretaceous succession of study area in the present investigation.

Highlights

  • The purpose of this study is to compare modes of brittle failure structures between Cretaceous and Tertiary successions exposing in Spi Res Anticline, and to elucidate their kinematic and dynamic implications

  • The pulsating manner of jointing caused interference among joint sets and systems formed in study area, and inconsistent relative age relationship arisen between such joint sets and systems

  • If Cretaceous rocks were containing fractures attributed to the end Cretaceous orogenic phase, such fractures would have been reactivated in the end of later Tertiary orogenic phase, and progressed into advanced types of brittle structures

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Summary

INTRODUCTION

The purpose of this study is to compare modes of brittle failure structures between Cretaceous and Tertiary successions exposing in Spi Res Anticline, and to elucidate their kinematic and dynamic implications. The least prevailed joints are hol acute about a and c, and okl acute about b and c (plate: photos 1, 2, 3; Fig. 4; Table 1) According to their geometrical relationship with the anticline trend and local bedding attitudes, they were divided kinematically into tension (ac and bc) sets and shear systems (hko, hol and okl) (Hancock, 1985). The prevailing joint sets and systems are the product of regional stress field regime resulted from Arabian –Eurasian plate collision. Such stress field was acting in pulses, each pulse consisting of direct compression succeeded by relaxation. The pulsating manner of jointing caused interference among joint sets and systems formed in study area, and inconsistent relative age relationship arisen between such joint sets and systems

29 L13 Pila Spi 13
70 SW 60 SW 70 NW 84 SE 40 SE 105 NW 82 NW 60 W 65 W
MODIFIED FRACTURES
JOINT DISTRIBTION
DIHEDRAL ANGLES OF SHEAR JOINT SYSTEMS
CONCLUSIONS
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