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Geology and structure

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Page 1: Geology and structure
Page 2: Geology and structure

GEOLOGY AND STRUCTURE OF PIR SOHAWA,

SANGADA, & SHADARA AREA, ISLAMABAD,

MARGALA HILLS AND MICROFACIES ANALYSIS OF CHORGALI FORMATION

Muhammad Wajid Manzoor

Roll No 09

Institute of Geology

University of the Punjab Lahore

Page 3: Geology and structure

PHYSIOGRAPHY OF THE PROJECT AREA

Introduction

Objectives of work

Climate

Vegetation

Mountains

Soils

Drainage Pattern

Valleys

Nullah Gravels

Terraces

Population

Page 4: Geology and structure

Map of study area (Goggle Earth).

Project area on toposheet 43G/1

Vegetation in study area

Valleys in Study area

Page 5: Geology and structure

TECTONIC FRAMEWORK OF PAKISTAN

Introduction

o Geographically Pakistan is located at the west of South Asian Subcontinent.

o Pakistan comprise of three tectonic plates and its major portion lies on the Indian

Plate.

Historical Background

• Pangea Breakage

• Location of Indian Plate in Gondwanaland

• Northward drift and Rotation of Indo-Pakistan Plate

Page 6: Geology and structure

• Schematic diagram of continents

spreading • Relative positions of the continents

from 225 m.y to the present

• Position of India’s plate in

Gondwanaland

• Different positions of the Indian Plate with

respect to time during Northward drift

from 71Ma to present position.

Page 7: Geology and structure

TECTONIC ELEMENTS OF PAKISTAN

Himalayas consist on series of Southward propagating thrust sheets that are

formed by the Collison of Indian and Eurasian Plates. Continuous collision creates

younger thrust towards south (Searle et al., 1997).

These thrusts are described as:

o Main Karakorum Thrust

o Main Mantle Thrust (MMT)

o Main Central Thrust (MCT)

o Main Boundary Thrust (MBT)

o Himalayan Frontal Thrust (HFT)

Page 8: Geology and structure
Page 9: Geology and structure

DIVISION OF HIMALAYAS

The closing and subduction of the Tethyan Ocean was followed by collision of

continents that produced different structures and mountain ranges like Himalayas

(Genser, 1964).

Himalayas form a 2,500 km long and 160-400 km wide range that surround the

Indian subcontinent.

The geology of Himalayas is quite complicated that start from sedimentary

sequence of Phanerozoic to Eocene.

Genseer (1964, 1981) and Wadia (1964) has divided Himalayas from north to

south into following divisions:

o Tethyan Himalayas

o Higher Himalayas

o Lesser Himalayas

o Sub-Himalayas

Page 10: Geology and structure

LITHOSTRATIGRAPHY OF STUDY AREA

The stratigraphic succession of study area consists of Mesozoic to Tertiary sedimentary rocks.

The lower Jurassic Datta Formation is not exposed here.

The Kawagarh Formation of Cretaceous age is also missing in study area.

In study area Hangu formation unconformably overlies the Lumshiwal Formation.

Formation Lithology Age Environment

Murree Formation Rddish to maronish sandstone having epidot mineral Early Miocene Fluvial

Kuldana Formation Variegated shale with marl and sandstone. Early to Middle Eocene Coastal plain tidal flat and brackish water.

Chorgali Formation Flaggy limestone with interbedded shale and marl. Early Eocene Lagoonal.

Margala Hill Limestone Limestone with intercalation of shale and marl. Early Eocene Shallow marine.

Patala Formation The greenish grey shale. The shale has splintery as well as blocky in nature. Late Paleocene Shallow marine, Lagoonal and outer shelf.

Lockhart Limestone Grey to medium grey, medium to thick bedded nodular limestone

containing Lockhartia.

Middle Paleocene Restricted, shallow marine embayment, shelf facies.

Hangu Formation Laterite band and White, light grey and reddish-brown medium to coarse

grained sandstone consisting chiefly of quartz.

Early Paleocene Very shallow marine and deltaic.

Unconformity

Lumshiwal Formation Greenish grey rusty brown glauconitic sandstone containing oyster shells. Lower Cretaceous Shore face and shallow marine deltaic.

Chichali Formation Black to light grey shale containing Belemnite. Late Jurassic to Early Cretaceous Restricted anoxic.

Unconformity

Samana Suk Formation Grey to medium grey limestone with dolomitic patches. Middle Jurassic Shallow marine.

Base not exposed

Page 11: Geology and structure

Smamana Suk Formation

Chichali Formation

Lumshiwal Formation

Hangu Formation

Lockhart Limestone

Patala Formation

Margala Hill Limestone

Chorgali Formation

Kuldana Formation

Murree Formation

Page 12: Geology and structure

STRUCTURE OF THE PROJECT AREA

The Sangada area is covered by rocks of Mesozoic-Cenozoic age.

That have undergone severe deformation during Himalayan orogeny demonstrated by

the development of mostly southeast verging faults and associated folds.

In addition to Margala Hill Limestone and Chorgali Formation, Lockhart Limestone

is commonly the most exposed oldest formation in most of the area.

Most of the faults are reverse, although some normal faults are also present.

The folds are predominantly Synclinal to Anticlinal.

The general trend of the outcrops is NE-SW, which is almost similar to trend of

overall Hazara Basin.

Page 13: Geology and structure

A brief description of the major structures follows:

o MBT:

MBT is passing in the south east of the mapped area near Shahdara village.

It is deeply dipping fault having NW-SE orientation.

This fault brings the older Samana Suk Formation in direct contact with Lockhart

Limestone.

o Ajwa Fault 1:

It is the SE dipping high angle fault, Which is present between Patala shale of Paleocene age and Chorgali Formation of Eocene age.

Extended downward between Lockhart Limestone and Chorgali Formation.

o Ajwa Fault 2 :

It is present between Patala shale and Chorgali Formation.

This fault dislocates the Patala shale, Margala Hill Limestone and ChorgaliFormation above the fault plane.

Page 14: Geology and structure

o Sangada Fault 1:

This fault is present between Chorgali Formation and Patala shale.

It runs SW-NE from Sangada area toward Kharian and up to the southwest of Nelaan

Bhota.

o Sangada Fault 2:

It truncates the Lockhart Limestone and splays of Mukhuial Faults with NW trending.

The dip angle of the fault is 450 NW.

o Makhuial Thrust 1:

The Makhuial Thrust 1 is trending SW-NE from Makhuial Peak running in the south

of Hariala toward Botha area.

The Paleocene Lockhart Limestone thrusted over Margala Hill Limestone of Eocene

age.

o Makhuial Thrust 2:

It is present between Patala shale of Paleocene age and Chorgali Formation of Eocene age with the same trend as that of Makhuial thrust 1.

Page 15: Geology and structure

o Hariala Fault:

This fault is present between Chorgali Formation and southeastern limb of syncline

within Lockhart Limestone, whereas Chorgali Formation above the fault plane moves

downward forming the normal fault.

o Khumal Gali Fault 1:

Margala Hill Limestone /Lockhart Limestone.

This is ENE trending fault dips northwestward with an angle of the dip is 600

o Khumal Gali Fault 2:

This fault is between Lockhart Limestone and Chorgali Formation.

Chorgali Formation is the upthrown block, above the fault plane.

o Khumal Gali Fault 3:

This fault is present between Kuldana Formation and Lockhart Limestone.

The fault is dipping to NW. The dip angle is 450.

Page 16: Geology and structure

o Khumal Gali Fault 4:

This fault is present between Lockhart Limestone and Chorgali Formation.

It is dipping at an angle of 430 to northwestward direction.

o Khumal Gali Fault 5:

It is present between Chorgali Formation and Patala Shale.

Its trend is ENE and it is dipping toward NW with an angle of 450.

o Ranias Synclines:

These are the two major synclines of Ranias area.

This important synclinal structure of the area extends NW-SE, northward from MBT toward Ajwa Restaurant.

The core of the syncline is comprising of lenses of Patala shale which is flanked by older formation, Lockhart Limestone.

o Ranias Anticlines:

Ranias anticline 1 and 2 are the subordinate anticlinal structure with two major synclines.

The Lockhart Limestone is present in the core of these anticline.

The trend of the anticlines is NW-SE.

Page 17: Geology and structure

o Sangada Syncline:

Sangada syncline is NW-SE trending major synclinal structure between Chorgali

Formation and Kuldana Formation.

The lens of Kuldana Formation is forming the core of the syncline.

o Hariala Synclines:

Hariala syncline is the NW-SE trending syncline, predominantly in Lockhart

Limestone.

The Patala shale is present in the core of the syncline in the form of lenses.

The SE limb of syncline 1 has faulted contact with Chorgali Formation.

o Hariala Anticlines:

The small anticlinal structures appear in a small depression (gali), with NW-SE

trend.

These anticlines are explained as the older formation Lockhart Limestone is

present in the core, above which younger Patala shale is present.

Page 18: Geology and structure

Map of the project area and cross

secession line A to A'

Cross sectional view of mapped area

from latitude longitude 33050'15'',

7307'00'' to latitude longitude

33047'13'', 7308'30''.

Page 19: Geology and structure

PALEOECOLOGY AND MICROFACIES ANALYSIS

o Paleoecology is the study of interactions between organisms and/or interactions

between organisms and their environments across geologic timescales.

o The dedicated study of past environments by studying the fossil records of

organisms that lived in that environment at the time (Wilson, 1975; Hottinger,

1998; Flugel, 2004).

o Therefore, paleoecologic analysis derives from two sources, fossils and associated

rooks.

Aim of Paleoecology:

o The aim of paleoecology is therefore to build the most detailed model possible of

the life environment of previously living organisms found today as fossils.

o Qualitative and quantitative foraminiferal analysis provides a high-resolution

database for the biostratigraphy and determines the main paleoenvironmental

parameters.

Page 20: Geology and structure

Observed Fauna:

o The protozoan most commonly observed as fossils are foraminifera.

o Foraminifera are found in all marine environments, from the intertidal to the

deepest ocean trenches, and from the tropics to the poles, but species of

foraminifera can be very particular about the environment where they

live(Flugel,2004).

The observed fauna includes the following :

o Nummulites

o Lockhartia

o Ostracodes

o Miliolid

Page 21: Geology and structure

Microfacies analysis

o Microfacies refers to the criteria appearing in thin section under microscope.

o Every facies of a deposition show well-defined petrographic, and paleontological properties which can be clearly differentiated from the properties of other facies in the same geological period.

Methodology:

Observed Facies:

o Bioclastic mudstone

o Bioclastic Wackstone

o Bioclatic Packstone

o Bioclastic Grainstone

Page 22: Geology and structure

Ramp facies:

Ramp facies reflect the protracted offshore energy gradients which are a

consequence of gradual water-depth change. Individual ramp depositional zones

differ strongly in their facies compositions (Burchette and wright 1992).

These facies are divided into the following:

o Inner ramp deposits

o Mid ramp deposits

o Outer ramp deposits

Page 23: Geology and structure

Conclusion

Based on field observations, Microfacies analysis of the Chorgali Formation in the

study area divided into four microfacies that are:

1. Bioclastic Mudstone

2. Bioclastic Wackestone

3. Bioclastic Packstone

4. Bioclastic Grainstone.

Microfacies analysis and sequence stratigraphic concept, the Chorgali Formation

was deposited in an area of low rate of subsidence, where the major controlling

factor is eustasy.

The Chorgali Formation is deposited in Inner to mid ramp.

Page 24: Geology and structure