STRATIGRAPHIC EVOLUTION ABDUL AND GEOCHEMISTRY OF THE MANNAN NEOGENE SURMA GROUP, Department of Geology, SURMA BASIN, , University of Oulu

OULU 2002 ABDUL MANNAN

STRATIGRAPHIC EVOLUTION AND GEOCHEMISTRY OF THE NEOGENE SURMA GROUP, SURMA BASIN, SYLHET, BANGLADESH

Academic Dissertation to be presented with the assent of the Faculty of Science, University of Oulu, for public discussion in Auditorium GO 101, Linnanmaa, on June 15th, 2002, at 12 noon.

OULUN YLIOPISTO, OULU 2002 Copyright © 2002 University of Oulu, 2002

Reviewed by Docent Kari Strand Doctor Kalle Kirsimäe

ISBN 951-42-6711-7 (URL: http://herkules.oulu.fi/isbn9514267117/)

ALSO AVAILABLE IN PRINTED FORMAT Acta Univ. Oul. A 383, 2002 ISBN 951-42-6710-9

ISSN 0355-3191 (URL: http://herkules.oulu.fi/issn03553191/)

OULU UNIVERSITY PRESS OULU 2002 Mannan, Abdul, Stratigraphic evolution and geochemistry of the Neogene Surma Group, Surma Basin, Sylhet, Bangladesh Department of Geology, University of Oulu, P.O.Box 3000, FIN-90014 University of Oulu, Finland Oulu, Finland 2002

Abstract The Surma basin is a part of the Bengal Basin situated in northeastern Bangladesh. The presence of eight gas fields and one oil field makes this an area that is interesting both economically and geologically. In spite of detailed geological and geophysical investigations, information available on palynostratigraphy and geochemistry for the area is scanty. The aim of the present work was to investigate the palynological assemblages, mineralogy and geochemistry of the Surma Group (SG) sequences in Surma Basin, Bangladesh. Core samples (n = 188) were gathered from the wells following: Patharia well-5, Rashidpur well-1, Atgram well- IX, Habiganj well-1, Kailastila well-1 and Fenchuganj well-2. They were provided by BAPEX (Bangladesh Petroleum Exploration Company). X-ray Fluorescence (XRF), Atomic Absorption Spectrometry (AAS), Loss of Ignition (LOI), X-ray diffraction (XRD), Transmission Electron Microscopy (TEM) and Scanning Electron Microscopy (SEM) were used for geochemical and mineralogical study of shale samples. In the palynological study, the distributions of pollens and spores were determined. For data analysis, SPSS computer programme was used. Palynological assemblages of the Surma Group of sedimentary sequence of Bangladesh include taxa range in age from the lower Miocene to the Upper Miocene which can be potentially used in dating and correlation. The Lower Miocene interval is correlated with the Simsang Palynological Zone IV of Meghalaya, India and the Bengal Palynological Zone (BPZ) V. The Upper Miocene is correlated with the Simsang Palynological Zone IV of Meghalaya, India and the BPZ Zone V of Bengal. They were deposited in two types of paleoenvironments ranging from the brackish type to shallow marine to brackish. The sequence contains reworked palynomorphs of BPZ IV and III namely Meyeripollies naharkotensis, Polypodiesporites Oligocenecus, Palmepollenities Eocencus and ornamented Tricolpate pollen of the - age which are mainly encountered in the lower Miocene sediments indicative of increased tectonic activity in the area. Geochemical ratios (SiO2/Al2O3, Cu/Zn, Maturity = K2O+ Al2O3/Na2O+MgO, Rb/K2O, K2O/Na2O, Cr/Rb, Zr/Rb, V/ Rb, Th/U etc.) were useful for determining grain size, maturity, tectonics and environment of deposition. High Ba enrichment was detected in the Patharia well-5 and showed high surface water productivity and diagenetic mobilisation. Tectonic descrimination was achieved using SiO2 and K2O/ Na2O ratio. XRD analysis revealed the minerals kaolinite, illite, chlorite, illite/smectite (I/S) and kaolinite/smectite (K/S) mixed layers. Kaolinite/Smectite here reported for the first time in Bangladesh. Clay mineral analyses provided evidence for diagenesis. Smectite diagenesis and dehydration have contributed to the generation of overpressure in the Bhuban Formation in the Patharia well-5. Geochemical ratios of the present study from the Surma Basin is undoubtedly a powerful technique and can be applied to any sedimentary basin analysis to infer the palaeoenvironment, palaeoclimate and palaeotectonics.

Keywords: palynostratigraphy, geochemistry, Surma Basin, Kaolinite-Smectite, Illite- Smectite, diagenesis, geochemical ratios, Bangladesh In the name of Allah, the Most Beneficent, the Most Merciful

Dedicated to: my parents and my wife

“And it is He Who spread out the earth, and set thereon mountains standing firm, and flowing rivers: and fruit of every kind He made in pairs, two and two he draweth the night as a veil over the day. Behold, verily in these things there are signs for those who consider” Holy Quran (13:3). “The world is sweet and verdant green, and Allah appoints you to be His regents in it, and will see how you acquit yourselves…” one of the sayings of Prophet Muhammad (peace be upon him).

Acknowledgements

Thanks to God and may His peace and blessings be upon all his prophets for granting me the chance and the ability to successfully complete this study. I wish to express my deepest gratitude to my supervisors Prof. Risto Aario and Prof. Vesa Peuraniemi for their valuable advice and guidance of this work. Special thanks and gratitude to Prof. Vesa Peuraniemi for his genuine support, valuable advice and sincere comments which helped me a lot to finish this study. The Institute of Geosciences and Astronomy, at the University of Oulu, Finland provided support, including field, laboratory and office work as well as analyses of samples. This study was partially financed by the University of Oulu through a post-graduate grant. I am very grateful to the authority of the University of Oulu. I am also grateful to the authority of the University of Rajshahi, Bangldesh for allowing me to undertake the present work. I also want to express my gratitude to the official referees of my dissertation work Dr. Kari Strand (University of Oulu) and Dr. Kalle Kirsimäe (University of Tartu, Estonia) whose comments and criticism were helpful in refining the draft version of the dissertation into its final form. I also want to express my thanks to Dr. Seppo Gehör (University of Oulu) for checking a major portion of the thesis and for his valuable comments and criticism during the preparation of the manuscript. I wish to thank Prof. Kauko Laajoki, who regularly gave his time to encourage me, especially during late night research sessions when he was the only companion during coffee breaks at the department. I also wish to thank Prof. Tuomo Alapieti, Director of the Institute of Geosciences and Astronomy, University of Oulu for providing scientific and other facilities of the department to my disposal. My sincere thanks are due to the opponent of this thesis, Prof. Raimo Uusinoka (University of Tampere), for giving his valuable time, despite of his tight schedules. I am grateful to the authority of the Bangladesh Petroleum Exploration Corporation (BAPEX) for providing the core samples for this study. I am grateful to Mr. Lutfor Rahman Chowdhury, General Manager, BAPEX for his valuable collaboration and practical assistance in palynological laboratory analysis. My sincere thanks to all my friends and collegues in BAPEX who co-operated nicely during the collection of core- samples and laboratory work. My sincere thanks to my friend Prof. Sifatul Qader Chowdhury, Department of Geology, University of Dhaka, Bangladesh for his nice suggestions towards the planning of this research work. I am also thankful to the numerous individuals who have directly or indirectly contributed to the completion of this work. Out of them at least two names should be mentioned here whom are my beloved students Prof. Badrul , department of geology and mining, University of Rajshahi, Bangladesh and Dr. M. Riajul Islam, University of Idaho, Moscow, Id. USA. I am deeply indebted to my friend Dr. Nuruddin Ashammakhi, Docent, Faculty of Medicine, University of Oulu, whose assistance and encouragement made this work possible towards the end. I cannot forget the sleepless nights he spent before the submission of the thesis and was helping me like a guide. I am also indebted to Prof. Mohammad Hassan, Head of the department of Geochemistry, Al-Azhar University, Egypt for giving suggestions and co-operation in the geochemical and mineralogical part of the thesis. Special thanks are due to the staff of the Institute of Electron Optics at the University of Oulu, and particularly to Mr. Olavi Taikina-Aho for their assistance with the microanalyses. I wish to express my gratitude to Mr. Brayan Dopp, Language Center, University of Oulu, for revising the English language of the manuscript. Also, I give my deep felt regards to Mrs. Kristiina Karjalainen, who has drawn many of the figures and has taken care of the electronic forms of them, Mrs. Ulla Paakkola, for preparing most of the thin sections and Mrs. Riitta Kontio, who co-operated in the geochemical laboratory works for this study. My heartful thanks to all of them. My sincere thanks to all of those who have co-operated both in Finland and in Bangladesh. Finally, I am particularly grateful to my wife, Syeda Wahida Akter, for helping and assisting me in all the stages of this work. Without her help this study would never have been possible. Her constant and continuous co-operation starting from laboratory analyses (cutting, crushing, seiving etc.) to the end of the work – a long way’s journey, proves her love and support during the whole course of this work. Special thanks to my daughter, Noor-E Sadia, for typing the major portion of this thesis and to all my other children for their patience and all kinds of support during all of my studies.

Oulu dated the 29th April, 2002 Abdul Mannan Contents

Abstract Acknowledgements Contents 1 Introduction ...... 11 2 Previous studies ...... 14 2.1 Palynology ...... 14 2.2 Geochemistry ...... 18 3 Aims of this study ...... 19 4 Study Area ...... 20 4.1 Stratigraphy ...... 20 4.2 Structure and tectonics ...... 27 4.3 Palaeogeography and Palaeotectonics ...... 29 4.4 Surma Basin (SB), Sylhet (North East Bangladesh) ...... 30 4.4.1 Wells studied ...... 30 4.4.2 Regional geologic setting ...... 31 5 Analytical methods ...... 35 5.1 Palynological slide preparation ...... 35 5.2 Geochemical analysis ...... 35 5.2.1 X-ray Fluorescence (XRF) ...... 36 5.2.2 Atomic Absorption Spectrometry (AAS) ...... 36 5.2.3 Loss of Ignition (LOI) ...... 36 5.2.4 Accuracy of analyses ...... 36 5.3 Mineralogical analysis ...... 38 5.3.1 X – Ray Diffraction (XRD) ...... 38 5.3.2 Transmission Electron Microscopy (TEM) ...... 38 5.3.3 Scanning Electron Microscopy (SEM) ...... 38 5.3.4 Petrographic microscopy (optical) ...... 38 5.4 Statistical analysis and ratios ...... 39 6 Stratigraphy ...... 40 6.1 Lithofacies ...... 40 6.2 Palynological study ...... 41 6.3 Pollen data and pollen assemblage zone ...... 41 6.4 Palynostratigraphic zonation ...... 41 6.4.1 Palynostratigraphic zonation of Fenchuganj well – 2 ...... 42 6.4.2 Atgram well – IX ...... 44 6.4.3 Habiganj well – 1 ...... 44 6.4.4 KailasTila well – 1 ...... 45 6.4.5 Patharia well – 5 ...... 45 6.4.6 Rashidpur well – 1 ...... 45 6.4.7 Comparison with surrounding areas (from India) ...... 46 6.4.8 Comparison with other Miocene Assemblages ...... 46 6.4.8.1 Assam and Meghalaya sequences ...... 46 6.4.8.2 Bengal Basin ...... 47 6.5 Palaeoenvironment and Palaeoclimate ...... 49 6.6 Age ...... 50 6.7 Maturity ...... 50 6.8 A list of palynomorph recovery from the Fenchuganj well-2 with their possible botanical affinity ...... 52 7 Geochemical results ...... 59 7.1 Major elements (XRF & AAS) ...... 59 7.1.1 Major elements ...... 59 7.2 Trace elements ...... 89 7.2.1 Barium enrichment ...... 100 7.2.2 Total Rare Earth Elements (∑REE) ...... 108 8 Mineralogical Results ...... 115 8.1 XRD ...... 115 8.1.1 Non Clay Minerals ...... 116 8.1.2 Clay minerals ...... 117 8.1.2.1 Diagenetic model of Surma Basin ...... 119 8.1.2.2 Implication of Smectite diagenesis and dehydration...... 120 8.1.2.3 Clay minerals of SG and its implication in petroleum geology. 121 8.1.2.4 Kaolinite - Smectite (K/S) mixed layer clay: a new mineral in Bangladesh ...... 122 8.2 TEM and SEM ...... 129 8.3 Petrography ...... 130 9 Discussion ...... 137 10 Conclusions ...... 146 11 References ...... 149 Appendices 1 Introduction

This thesis is fundamentally concerned with the stratigraphy (based on pollen analysis) and geochemistry of the Neogene Surma Group (SG) sediments from core samples of the Surma Basin (SB), Sylhet, Bangladesh. The SB is a sub-basin of the Bengal Basin situated in the northeastern part of Bangladesh. The basin is bounded on the north by the Shillong plateau, on the east and southeast by the Chittagong-Tripura fold belt of the Indo-Burman ranges and on the west by the Indian Shield platform, to the south and southwest it is open to the main part of the Bengal Basin. The thickness of the late Mesozoic and Cenozoic strata in the SB range is from about 13 to 17 km (Evans 1964, Hiller & Elahi 1984), and much of this strata is Neogene in age. The Bouger anomaly map shows gradually higher values (negative) towards the center of the basin (Alam et al. 1990). An Aeromagnetic interpretation map by Hunting (1980) indicates a gradual deepening of the towards the center of the basin and also reveal subsurface synclinal features and faults within the basin. Its topography is predominantly flat with some north-south trending ridges of twenty to several hundred meters elevation present on the north – eastern border. It is actively subsiding (Johnson & Alam 1991). The geology and the hydrocarbon potential of the SB has been investigated by many workers (Holtrop & Keizer 1970, Lietz & Kabir 1982, Hiller & Elahi 1984, Khan et al. 1988, Johnson & Alam 1991), detailed geochemical and palynological studies of SB sediments are lacking. A number of wells have been drilled in the SB with the discovery of eight gas fields and the recent discovery of commercial quantities of oil in the Sylhet – 7 well make this area more interesting economically and geologically. Core samples (n = 188) of the wells of Patharia well – 5, Rashidpur well – 1, Atgram well – IX, Habiganj well – 1, Kailastita well – 1 and Fenchuganj well – 2 were provided by the Bangladesh Petroleum Exploration Company (BAPEX) for the present study. A Palynological study was done from 74 samples. The samples studied are from 959 m down to 4735 m in depth. The study is aimed to determine the environmental conditions prevailing when the sediments were deposited. The study also included details of the geochemistry of the basin for understanding the tectono-environmental condition of the deposition of the sediments, as well as the diagenetic changes of the sediments during burial. 12

The SG is diachronous unit consisting of a succession of alternating shales, sandstones, siltstones and sandy shales with occasional thin conglomerates, indicative of repetitive deposition from pro – delta, delta front and paralic facies with intermittent, wholly marine facies (Holtrop & Keizer 1970). The group is divided into the Bhuban and the Bokabil Formations, based on differences in their gross lithologies (Mathur & Evans 1964). Tertiary palynostratigraphy is a notoriously difficult discipline and is confronted with various problems. For instance, the mean species duration is relatively high in angiosperms which form the dominant taxonomic group in most Tertiary vegetations. In addition, the occurrence of a plant species in a certain area is largely controlled by ecological, climatic and biogeographic factors. Hence, the first and last appearances of Tertiary palynomorphs in a given section are generally not considered to be very reliable stratigraphic indicators. Correspondingly, climate stratigraphy and biostratigraphy are now widely used in the Tertiary although there is no well – defined methodology available and there is always the problem of distinguishing autochthonous or parautochthonous from allochthonous palynomorphs (Ashraf et al. 1997). Palaeoclimate reconstructions in the Neogene are difficult because all methodological approaches used so far, i.e. the geological – palaentological approaches and the climate modeling approaches, suffer from considerable uncertainties (Utsechar et al. 1997). Detailed palynological studies of this area are lacking because of very poor preservation of the palynomorphs. Palynomorph recovery from the cores of the wells drilled in the area was low. Some parts, the wells were almost barren. The Palynomorph content in the prepared palynological slides for palynostratigraphic analysis was extremely poor. No palynomorphs (other than fungal spores) were detected in 38 slides out of 74 slides. Due to this, the idea of doing a quantitative analysis of the palynomorphs was abandoned except for the Fenchuganj well-2, the results of this well allowed for some quantitative considerations. The analysis have furnished definite evidence of palynological assemblages of the SG of the sedimentary sequence of Bangladesh, including taxa range in age from the lower Miocene to Upper Miocene, which can be potentially used in dating and correlation. The Lower Miocene interval is correlated with the Simsang Palynological Zone IV of Meghalaya, India (Baksi 1965) and the Bengal Palynological Zone (BPZ) V (Baksi 1971). The Upper Miocene is correlated with the Simsang palynolgical Zone IV of Meghalaya, India (Baksi 1965) and BPZ zone V of Bengal (Baksi 1971). No palynological research paper has been published from this region yet. Identification and comparison of the palynomorphs were made on the basis of the published literatures on Tertiary Palynology of the Assam and Bengal Basin of India (Neighbouring country). The works include Ghosh (1941), Sahni and coworkers (1947), Sen (1948), Lakhanpal (1955), Meyer (1958), Baksi (1962, 1965, 1971), Biswas (1962, 1965), Banerjee (1964), Sah and Datta (1966, 1968, 1974), Ghosh (1969), Venkatachala and Kar (1969), Datta and Sah (1970, 1974), Deb (1970), Banerjee and Misra (1972), Salujha and coworkers (1969, 1971, 1972, 1973 and 1974), Kar, Sing and Sah (1972), Banerjee and coworkers (1973), Sah and Sing (1974), Singh and Singh (1978), Singh and Tiwary (1979), Jain and Kar (1979), Dutta and Singh (1980), Mehrotra (1981, 1983), Reiman and Thanug (1981), Ramanujan (1982, 1987 & 1988), Handique and Dutta (1981), Varma and Patil (1985), Saxena and coworkers (1986a, 1986b), Singh and coworkers (1986a 1986b), Varma and 13 coworkers (1986), Singh (1977a,b), Singh and Rao (1990) and Kar (1990). Special attention was given to those works from adjacent areas of the present study area – the SB. The geochemistry of the SG sediments was carried out on the basis of 188 core samples of the wells following: Patharia well – 5, Rashipur well – 1, Atgram well – IX, Habigang well – 1, KailasTila well – 1 and Fenchuganj well – 2. Detailed inorganic geochemistry of the study area is presented for the first time. Many works have been done only for organic geochemistry (Shamsuddin 1989, Ahmed et al. 1991, Manzur et al. 1991, Rafiqul et al. 1993). Very few works were under taken for the inorganic geochemistry (Imam & Shaw 1985, Imam 1987, 1989, 1993, 1994 and Islam 1996) of the study area. The inorganic geochemistry of the SB was prepared on the basis of the chemical and minerological analysis. The chemical analysis includes X-Ray Fluorescence (XRF), Loss of Ignition (LOI) and Atomic Absorption Spectrometry (AAS). The mineralogical analyses were done by X-Ray Diffraction (XRD), Transmission Electron Microscopy (TEM), Scanning Electron Microscopy (SEM) and petrographic microscopy. The major elements like SiO2, Al2O3, MgO, CaO, Na2O, K2O, Fe2O3, TiO2, MnO and P2O5 were analyzed. Most of the important trace elements were also measured. Some statistical analyses were carried out such as Cu/Zn ratio in order to ascertain redox parameter, SiO2/Al2O3 for grain size, M = K2O + Al2O3/K2O + Na2O, Rb/K2O for maturity. Other ratios of Cr/Rb, Zr/Rb, V/Rb, Th/U and Cr/Th are sensitive indexes for provenence (Taylor & McLennan 1985, McLennan 1989, Condie and Wronkiewiez 1990, Götze 1998, Hassan et al. 1999) and were performed. Correlations between Cr, Rb, Zr and K2O%, TiO2% and Al2O3 (Grömet et al. 1984, Bellanca et al. 1999) were performed. A Tectonic classification graph, by using cross plots of SiO2 vs. K2O/ Na2O (Roser and Krosch 1986) was prepared to discriminate the tectonic setting of the area. A study of the clay mineralogy of shale was undertaken in order to find out the diagenetic changes that have taken place in the subsurface, to find out the environmental conditions and to discuss the implications of clay mineral diagenesis on major geologic processes such as overpressure generation and structural developments. The study also focuses on the evolution of climate variabilities during the Neogene by using the clay mineralogy analysis of Neogene shale samples of the Surma Basin. An attempt was made to ascertain the semi-quantitative estimate of the relative abundances of clay minerals of SB and also to ascertain the petroleum generation capability of sediments under study with the knowledge of clay mineral diagenesis. 2 Previous studies

2.1 Palynology

So far, no palynological research paper has been published from this region. Identification and comparison were made for this work on the basis of published literature on the Tertiary Palynology of the Assam and Bengal Basin of the neighbouring country, India. In India, the known records of Tertiary plants go back to the later part of the eighteenth century (Sonnerat 1782) which remained practically uninvestigated until the first quarter of the present century (Sahni 1921). Later, the first record of a fossil pollen from the Tertiary strata in India by palynological means was on the oil-bearing strata of Assam (Sahni et al. 1947). Since then a number of palynological studies on the Tertiary of India have been carried out (Sen 1948, Lakhanpal 1955, Meyer 1958, Baksi 1962, 1965, Biswas 1965, Banerjee 1964, 1967, Ghosh 1964, 1969, Sah & Datta 1966, 1968, Sah et al. 1966, 1968 and 1974, Datta & Sah 1967, Venkatachala & Kar 1969, Salujha et al. 1972a,b, Banerjee et al. 1973, Singh et al. 1978, 1986a,b, Singh 1977a,b, 1981, Singh & Tiwary 1979, Mehrotra 1981, 1983, Ramanujan 1982, 1987, 1988 and the references therein). In the Tertiary succession of India, the Jaintia Group (Paleocene-Eocene), Barail Group (Oligocene) and the Surma Group (Miocene-Pliocene) has been studied well. The Tertiary Palynology of Punjab Basin, Cambay Basin, Cauvery Basin, Bengal Basin and Assam Basin has given a good account of the palynology of the area and specially the Surma Group of Bengal Basin and Assam Basin were the guideline for the present study as a neighbouring area since no published paper was available till date. The main features (common assemblages and restricted occurrences) of the Tertiary palynology of India are presented in Table 1 and in Table 2. 15

Table 1. Tertiary Palynostratigraphy of India based on published work.

Age Name of the Common assemblages Restricted forms Reference basin Jaintia Punjab Todisporites, Dandotiaspora, Lycopodiacidites, Mathur 1964, Group Basin Osmundacidites, Couperipollis, Palypodiaceaesporites, Salujha et al. (Pal – Palmepollenites, Granodiporites, Triorites, 1969, Singh & Eocene) Cordosphaeridium, Nyssapollenites, Polycolpites, Khanna 1980 and Homotryblium, Gonyaulacysta, Microhystridium, Khanna & Sing Lygodiumsporites, Todisporites, Cannospharopsis, 1981, Sing et al. Cyathidites, Proxapertites, Hystrichospheridium, 1978. Couperipollis, Tricolpites and Oligosphaeridium, Palmidites Cleitosphaeridium, Cyclonephelium, Thalassiphora, Subathua, Araneosphara, Achilidinium, Verrutrucolpites and Podocarpidites Cambay Lygodiumsporites, Biretisporites, Polypodiaceaesporites, Varma & Basin Verrucatosporites, Arecipites, Maurisites, Dangwal 1964, Scizoaeoisporites, Spinizonocolpites, Venkatachala & Palmaepollenites, Proxaperites, Psilodiporites, Retitricolpits Choudhury 1977, Tricolpites, Nympheaceaepites, Margocolporites, Rhoipites, Rawat & Proteacidites, Cupuliferoipolenites, Venkatachala Palaeocaesalpiniaceaepites, Marginipollis, Cyathidites, 1977 and Mathur Cicatricosisporites etc. Intrapunctiporis, Couperipollis, et al. 1977. Assamialetes, Tricolporopollis, Todisporites, Palmidites ans Lakiapollis. Couvery Lygodiumsporites, Laevigatosporites, Venkatachala & Basin Scizaeosporites, Proxapertites, Spinainaperturites, Rawat 1973 and Couperipollis, Palmaepollenites, Psilodiporites, Marginipollis, Sastri et al. 1977. Lilicidites, Tricolpites and Margocolporites, Rhoipites, Myricipites. Caprifoliipites etc. Bengal Assamialetes, emendatus, Lycopodiales, Granutusporites, Baksi 1971. Basin (Zone Palmeopollenites and Ornamented tricolpate, – II and Couperpollis. tricolporate, Caesalpiniaceae, Zone – III) polycolpate, polycolporate (Hexacolpites) Couvery Lygodiumsporites, Laevigatosporites, Venkatachala & Basin Scizaeosporites, Proxapertites, Spinainaperturites, Rawat 1973 and Couperipollis, Palmaepollenites, Psilodiporites, Marginipollis, Sastri et al. 1977. Lilicidites, Tricolpites and Margocolporites, Rhoipites, Myricipites. Caprifoliipites etc. Couvery Lygodiumsporites, Laevigatosporites, Venkatachala & Basin Scizaeosporites, Proxapertites, Spinainaperturites, Rawat 1973 and Couperipollis, Palmaepollenites, Psilodiporites, Marginipollis, Sastri et al. 1977. Lilicidites, Tricolpites and Margocolporites, Rhoipites, Myricipites. Caprifoliipites etc. Couvery Lygodiumsporites, Laevigatosporites, Venkatachala & Basin Scizaeosporites, Proxapertites, Spinainaperturites, Rawat 1973 and Couperipollis, Palmaepollenites, Psilodiporites, Marginipollis, Sastri et al. 1977. Lilicidites, Tricolpites and Margocolporites, Rhoipites, Myricipites. Caprifoliipites etc. 16

Table 1 continued Age Name of the Common assemblages Restricted forms Reference basin Bengal Assamialetes, emendatus, Lycopodiales, Baksi 1971. Basin (Zone Palmeopollenites and Granutusporites, – II and Couperpollis. Ornamented tricolpate, Zone – III) tricolporate, Caesalpiniaceae, polycolpate, polycolporate (Hexacolpites) Jaintia Assam Basin Cyathidites, Lygodiumsporites eocenius, Verrutricolporites, Biswas 1962, Group Dandotiaspora Dilata, Polypodiisporites, Bacutricolporites sp. Sah & Datta Monolitesmawkmaensis, A, Onagraceae and 1966, 1968, Assamialetesemendatus, Couperipollis Polygalaceae 1974, Dutta & brevipinosus, Liliacisites Sah 1970, microreticulatus, Palmepollenites Salujha et al. sommunis, Tricolpites, Tricolporopollis 1971 Sein & Sah Schizoporis, Retialetes, Triorites, 1974, Sing Schizaeosporites, Palaeocaesaceaepites, 1977a,b, Sing & Nymphea, Caesalpinia etc Tewari 1979, Dutta & Jain 1980 and Mehrotra 1981. Barail Assam Basin Foldexina inaperturata, Meyeripollis, Schizaeoisporites and Biswas 1962, Group Cyathidites Couper, Lygodiumsporites Nympheaceaepites Baksi 1962, (Oligoce Potonie´, Todisporites Couper, Strialetes, 1965, Sah & ne) Magnastriatites Muller, Monolites Dutta 1966, Potonie´, Assamialetes, Jaintiapollenites, 1968, 1974, Caryophyllaceaepites, Triorites Mehrotra 1981, (Erdman) Couper, Pinuspollenites, 1983, Kar 1990 . podocarpidites, Striatites, Todisporites etc. Bengal Lygodium, Polypodium, Coniferae, Graminae Biswas 1963. Basin Cicatricosisporites, Bauhinia, and Cyperacea Barringtonia etc. Couvery Lacrimapollis pilosus, Verrucatosporites Magnastriatites Venkatachala & Basin bullatus, Malavacearumpollis cauveriensis Rawat 1973. paucibaculatus Surma Bengal Cicatricosisporites, Bauhinia, Palmaepollenites, Biswas 1963, Group Basin Rhizophoraceae, Hystrichospheridium, Nympheaeceapites and Deb 1970 and (Mio – Coniferaepites, , Graminae Barringtonia, histrichosphaerids Baksi 1962, Pliocene) Polygonaceapites zonoides Baksi, 1971. Tricolpate – tricolporate, triporate, monocolpate, dinoflagellate (BPZ – V, Baksi) Bisaccate conifer belonging to Cedrus, Baksi 1971. Pinus, Abies, Picea, Tsuga, Schizaeceae and Parkeriacea (BPZ – VI, Baksi) Couvery Verrucatosporites bullatus, Talisiipites retipilatus, Venkatachala & Basin Polypodiisporites ornatus, Costatipollenites pau- Rawat 1973. Lygodiumsporites sp., striatopollis and ciornatus, Tricolpites hystrichospherids. longicolpatus, Striatri- porites sp., Tiliaepolen- ites sp. etc. 17

Table 2. Published stratigraphic ranges of selected Palynomorphs in the Tertiary sequences in India (Neighbour country of Bangladesh).

No. Selected Palynomorphs Eocene Oligocene Miocene Pliocene LMU 1 Echitricolporites sp. 2 Graminidites sp. 3 Polypodiaceaesporites sp. 4 Proteacidites symphonemoides 5 Podocarpidites (Coniferipites) chattachari 6 Lirasporis intergranifer 7 Bombacacidites assamicus 8 Spinosopites acolporata 9 Cicatricosisporites (Ceratopteris) sp. and Parkeriaceaesporites sp. 10 Corrugatisporites terminalis 11 Palmaecolpollenites sp. cf. Monocolpopites broadcolpusi 12 Palmaepollenites eocenicus 13 Palmaepollenites subtilis 14 Eximispora tuberculata 15 Monosulcites brevispinosus 16 Monosulcites rarispinosis 17 Meyeripollis naharkotensis

In the Miocene, the climate changed to cool, sub-tropical to temperate and the flora was rich. The sediments were mostly fresh-water continental deposits, brackish lagoonal conditions existing only in parts of the Sub-Himalayan region, Cauvery and Bengal Basins and the southern part of Assam. Drier conditions existed in the Pliocene, as may be reasoned by the common occurence of Graminidites etc. Coastal or Lagoonal conditions existed in the Bengal and Kutch basins in the Pliocene. Most of the angiospermous genera known from the Paleogene and Early Neogene are derived from woody plants. In the Late Neogene, herbaceous angiospermous elements like grasses, chenopods, amaranths etc. are conspicuous. In summary, it can be stated that the Tertiary sediments in India can be distinguished from the by the predominance of angiospermous elements and the absence of such taxa as Trilobosporites, Appendicisporites etc. in the former. Statistical variations in the assemblage along with the disappearence of taxa like Nothofagidites seem to be more convenient for making the boundery between Eocene and Oligocene, at present. The boundary between the Oligocene and the Miocene is marked by the appearence of temperate to cold climate elements in the latter, along with the disappearence of, or the rare occurence of, Paleogene forms like Numphaeceapites, Triorites etc. In the Pliocene, herbaceous elements and grains of such advanced families as Gramiae, Compositae etc. are conspicuous in the assemblage. 18 2.2 Geochemistry

An extensive geological and geophysical (mostly seismic) survey has been carried out in order to describe the stratigraphy, regional setting, structural evolution, condition of deposition of sediments and the paleogeography of the basin. Despite the study of the geology and petroleum prospects (Bakhtine 1966, Holtrop & Keizer 1970, Alam 1972, Brunnschweiler 1966, Lietz & Kabir 1978, Khan et al. 1988, Imam 1987, 1989, 1993, 1994, Johnson & Alam 1991, Raghava & Mustaque 1994), relatively few attempts have been made to study the geochemistry of the area under study. Most of the geochemical works deal with the organic geochemistry of the sediments (Khan et al. 1988, Pairazian et al. 1985, Shamsuddin 1989, Manzur et al. 1991). Only the works of Imam (1987, 1989, 1993, 1994) are dealing with inorganic geochemistry. But his work was mostly with sandstones. Besides this, a few attempts were made on the mineralogy of the sediments from Bengal Basin as well as from the study area (Datta & Subramanian 1997, Datta et al. 1999, Islam & Lotse 1986, Biswas & Chowdhury 1995, Chowdhury et al. 1987). The work from this same Department of Geology, University of Oulu, Finland by Islam (1996) dealing with the weathering crust in Bangladesh, is a good addition to the account of inorganic geochemistry of the sediments of Bangladesh. Despite the works mentioned, no attempt was made on a detailed geochemical investigation of the area under study. 3 Aims of this study

1. To find out the ageframe of the Surma Group (SG). 2. To find out the environmental conditon prevailing when SG sediments were being deposited. 3. To find out paleoecological and paleogeographical conditons of the SG with the help of diagnostic and common palynomorphs. 4. To find out the geochemistry of the SG sediments and their diagenetic changes. 5. To correlate SG with Bengal palynological zonations, Assam palynological zonations, and the Garo hills of India. 6. To ascertain the botanical affinities of the most important spore – pollen encountered. 7. To provide some guidelines for the geochemical exploration in the area. 4 Study Area

Bangladesh extends from Latitude 20°43´ to 26°36´N and Longitude 88°3´ to 92°40´E. Bangladesh occupies the greater part of the Bengal Basin, covers part of the Himalayan piedmont plain and covers the eastern and southeastern hill ranges of the Sylhet, Chittagong and Chittagong Hill tracts (Paul & Lian 1975). The northeastern part of Sylhet (Jaintapur) is characterized by low rounded hillocks with cliffs and scarps. Fig. 1 shows the location and geology of the study area.

4.1 Stratigraphy

The stratigraphy of Bangladesh is somewhat problematic because the greater part of the country is covered by thick alluvium and almost all the strata are devoid of faunal fossils (Khan & Mominullah 1980). The works leading to the establishment of stratigraphy in Bangladesh are mainly based on lithologic interpretation. Figs 2 and 3 shows the details of the physiography and geology of Bangladesh. The lithostratigraphic units are defined and described in terms of their lithological composition and geographical location only (Fig. 4). 21

Fig. 1. Location map of the study area (Surma Basin, Sylhet, Bangladesh). (Map from Alam et al. 1990, permitted from Geol Surv Bangladesh.) 22

Fig. 2. Physiographic map of Bangladesh. (Map from Alam et al. 1990, permitted from Geol Surv Bangladesh.) 23

Fig. 3. Geologic map of Bangladesh. (Map from Alam et al. 1990, permitted from Geol Surv Bangladesh.)

Bangladesh occupies most of the Bengal Basin - a major geotectonic element of the Assam -Himalayan region and is considered apparently the largest depositional feature in the world today (Graham et al. 1975, Salt et al. 1986, Kuchl et al. 1989). The Bengal Basin is the site of the worlds largest delta (about 60,000 km2) formed by rivers (, Brahmaputra/Jamuna, Padma, Meghna) that drain a large proportion of the Himalayas (Johnson & Alam 1991). Bangladesh has a thick stratigraphic succession of mostly Tertiary sediments (Table 3). The thickness of practically all units increase in a southerly direction and the strata that are deltaic or shallow marine in the north become progressively more marine to the south (Alam 1989). 24

JAINTIA GROUP

Fig. 4. Cross-section of Bengal Basin from west to east ( Modified from Paul & Lian 1975). 25

Table 3. Stratigraphic Sequence in Bangladesh.

Geologic age Stable shelf Bengal foredeep Lithology Group Formation Group Formation Holocene Alluvium Alluvium Silt, sand, gravel and clay Pleistocene late Pliocene Dihing Modhupur Clay Pebbly sandstone, sticky clay Madhupur Maduhpur Mid-Pliocene E. Sandstone, coarse quartz pebbles, Pliocene Dupi Tila Dupi Tila petrified wood

Girujan clay Claystone with siltstone and Tipam sandstone Sandstone, coarse-grained cross- bedded pebbles of , Tipum quartzite, shale and lignite. Clay mostly at base. Miocene Surma Jamalgong Boka Bill Marine shale, pyritic gray marine fossils Surma Bhuban Sandy shale, sandstone, breccia interbeds Oligocene Barail Bogra Barail Jenam Siltstone, fine-grained sand- stone, carbonaceous shale Late Eocene Kopili Sandstone, locally glauconitic: shale, highly fossiliferous: thin Middle Eocene Sylhet calcareous beds limestone, num- Limestone ? ? mulitic, sandstone interbeds Early Eocene Jaintia Tura sandstone, coal and shale Sandstone ? ? Paleo-cene Late-Middle Upper Sibganj Sandstone, coarse yellow-brown, Cretaceous Gondo- Trapwash ? ? clay, white, volcanic ash wana Early Cretaceous Rajmahal Basalt, amygdaloidal, andesite, Jurassic Traps ? ? surpentinized, shale, agglomerate Late Permian Lower Sandstone, felspathic grey- Gondo-wana Paharpur ??wacke, coal, shale, sandstone, Early Permian coarse grained, shale, coal, thick Kuchma seams Pre-Cambrian Basement Gneiss and schist complex Sources: Based on Khan (1980) and Zaher & Rahman (1980). ? = not classified

Calcutta - Mymensing hinge zone of Eocene subdivides the Bengal Basin tectonically into two major subdivisions - shelf and geosynclinal area having different stratigraphic history. After the Pre-Cambrian era, the history of the basement complex was one of the peneplanation until Permo-Carboniferous time when Permian, Mesozoic and Gondowana sediments with coal accumulated in the western side of the basin. The break up of 26

Gondowanaland led to the eventual separation of peninsular India from the southern continents, permitting a Cretaceous marine transgression (Alam 1989). The Bengal Basin has been infilled with sediments from the north, east and west. During this process, the basin has generally deepened and the sea level has varied considerably from its present position. During the Cretaceous Period, the sea transgressed northwards towards the southern edge of the Shillong plateau and subsequently regressed far south into the Bengal Basin, causing at least four major transgressions and regressions. Argillaceous and arenaceous deposits accumulated on the stable shelf zone in freshwater to littoral facies. The sedimentation at the same time in the fore deep and mobile belt was marine, at least during the late Cretaceous (Alam 1989). From the Paleocene to the early Eocene, the shelf was subjected to repeated submergence and emergence marked by the Tura Sandstone (240 m). Extensive marine transgression took place in the Middle Eocene and the hinge-line was initiated due to a deeply seated basement fault between the stable shelf to the north – west and a geosynclinal trough to the south – east (Raju 1968). The Nummulitic Sylhet Limestone was deposited over most of the shelf area (about 245 m) in a shallow clear water and open marine shelf environment in a warm climate. During the Late Eocene Period, the Kopili Formation (238 m) consisting of carbonaceous pyritic shale and glauconitic sandstone (Ahmed & Zaher 1965) was deposited in a brackish to marine environment. The formation contains microforaminiferal assemblages of Globorotalia cocoensis biozone (Khan & Mominullah 1980). During the Paleocene to Eocene period, the Jaintia Group consists of three formations: Tura Sandstone, Sylhet Limestone and the Kopili Formation, which were deposited on the shelf (Total thickness is 725 m) in a shallow marine and marine environment. The upliftment of the Arakan – Yoma – Chin geanticline and basin – wide movement took place in Early Oligocene. The sea regressed from the Shillong Plateau area and fluviomarine Barail sediments were deposited along the southern rim of the Shillong Plateau; at the same time the area extending from the SB to the Chittagong Hill Tracts subsided and was filled with fine grained marine Barail shales and siltstones (Holtrop & Keizer 1969). The thickness of the Barail Group generally decreases towards the shelf. The deposition of the Barail Group in the fore deep basin and the mobile belt varies from 800 – 1000 m whereas on the shelf it is only 163 m and is represented by the Bogra Formation (Ahmed & Zaher 1965). The thickness of formations here is approximate and varies considerably from well to well. During the Miocene, a major uplift began in the Himalayas subjecting the Bengal Basin to related tectonic movements (Fairbridge 1983). The deep basin featured conspicuous subsidence and marine transgressions through much of the Miocene. The SG (5000 m) and the Tipam Group (2270 m) were then deposited in deltaic to shallow marine and continental environments, prograding to the southeast with depositional conditions changing to marine (Alam 1989). The SG has been divided into Bhubon and Boka Bil Formation in the geosynclinal facies of Bangladesh. The Bhubon Formation was deposited in an environment ranging from a shallow inner neritic to a lower deltaic plain, and that for the BokaBil Formation was in a range from marine at the bottom to transitional marine at the top. The top of the BokaBil Formation is also known as Upper marine shale (UMS) representing the last 27 widespread marine transgression over the Bengal Fore deep. During this period, a large delta complex started to build on the northeast side of the Bengal Basin. Smaller deltas were possibly building on the eastern side of the basin, presently occupied by Tertiary hills of Chittagong and Chittagong Hill Tracts (Alam 1989). During the Late Miocene Period, the Himalayan movements continued. The global eustatic regression in this period produced an important unconformity that is also seen in seismic reflections recorded for offshore in the (Curray & Moore 1979). The DupiTila and Dihing Formations were deposited by Pliocene marine transgressions and are represented by a thick sequence of about 2500m of fluvial and deltaic facies.The Quaternary was marked by the usual glacio-eustatic oscillations, superimposed on a general regression that has left widespread traces in the Bengal Basin (Morgan & McIntire 1959, Mallick 1971, and Bakr 1977). The Quaternary is represented in Bangladesh by the Tippera surface (Lalmai terrace and Chandina deltaic plain), Modhupur tract, Barind tract and Meghna flood plain (Bakr 1977), St. Martins limestone (the former is deltaic and the later represent a littoral facies) and Matamuhuri flood -plain of Maiskhal Island (Mannan 1993). Formation Modhupur clay is mottled and red, which is considered to be Pleistocene. It is followed by the Recent Alluvium consisting of loose gravel, sand, silt and clay with occasional pebbles and boulders. Peat deposits also occur locally (Khan & Mominullah 1980). The thickness of Alluvium ranges from zero to some tens of meter and increases toward the south.

4.2 Structure and tectonics

The structure and tectonics of Bangladesh and adjoining areas have been studied by a number of investigators including Bakhtine (1966), Sengupta (1966), Raju (1968), Holtrop & Keizer (1970), Alam (1972), Desikachar (1974), Graham et al. (1975), Guha (1978), Khan (1980), Matin et al. (1983), Banerjee (1984), Le Dain et al. (1984), Salt et al. (1986), Alam (1989), Rahman et al. (1990). The overall structure and tectonics of the Bengal Basin are briefly discussed below on the basis of the results of these investigations. Fig. 3 shows the generalized tectonic map of Bangladesh and adjoining areas. The Bengal Basin is bordered on the north by the Pre-Cambrian Shillong Plateau and to the west by the Indian Platform. To the east rises the Arakan-Yoma-Naga folded system, and to the south it plunges into the Bay of Bengal. The Bengal Basin is an exogeosyncline – that is, one in which thick detrital sediments within the craton were derived from uplift beyond the margin of the craton. The Bengal foredeep is a part of the exogeosyncline. The Bengal exogeosyncline is one of the worlds largest, and is part of the Bengal Geosyncline. The latter includes the Bengal Basin and the Bay of Bengal (Alam 1989). The major structures described below are: 1) shelf zone, 2) hinge zone, 3) Bengal foredeep, 4) mobile belt, and 5) Sub-Himalayan Fore deep. 1) Shelf zone is a major tectonic element of Bangladesh lying in the western and northwestern portion of it. The margin has a northeast-southwest trend along which the basement complex slopes steeply downward to form a hinge zone. The thickness of the 28 sediments over the shelf is about 3000m and they are marked by several unconformities (Alam 1989). The northern portion is known as the Rangpur platform and the southern is the Bogra shelf. The Indian shield and Shillong massif are connected by the Rangpur platform. The width of the platform is 100 km. Here, the slope is fairly smooth according to the seismic data. The sedimentary deposits of this area form monoclinal beds with dips of 1–2°. Towards the northern portion of the platform the plunge of the basement is about 3–4° and the depth of the basement is over 2000 m. Southern slope of the Rangpur platform is gently plunging towards the southeast and extends to the Calcutta-Mymensing hinge zone. The thickness of sedimentary rocks is increasing towards the southeast. The thickness of the sediments over the shelf is about 8000 m and they are marked by several unconformities. The basement complex near the western margin of the shelf is marked by a series of buried ridges and normal gravity faults. The east-west trending Dauki fault separates the stable shelf and the Shillong massif (Fig. 3). The shelf experienced the first marine transgression during the Late Cretaceous. The second major one was in the Miocene generated by the uplift of the Himalayan and Burman ranges. 2) Hinge zone is a narrow zone of 25 km in width. Here, the monoclinal dip is 5–6°. The bed dips over 20° in the hinge - line (Guha 1978). The hinge zone in the northeast seems to be connected with the Dauki fault by a series of east-west trending faults. It is also marked by deep basement faults probably started with the breakup of Gondowanaland. Parallel to the hinge zone is the Bengal foredeep, which consist of several smaller troughs and structural highs. 3) The Bengal foredeep, which is a large elongated trough, occupies the vast area between the hinge-line and Arakan-Yoma-Naga folded system. This is the deeper part of the Bengal Basin where the basement is deeply subsided here and the subsidence is directly related with the uplift of Himalayas-Burmese mountain chain. It is about 450 km wide in the south of Bangladesh and narrowing towards the northeast. The Basement is probably 12–15 km deep. The folded belts of the Indo - Burman ranges mark the eastern boundary of the Bengal foredeep. The total thickness of the sediments here is high which exceeds 12,000 m. According to gravity surveys and drilling data reported by Bakhtine (1966), Guha (1978), Khan (1980), Matin et al. (1983), the Bengal foredeep can be further subdivided into five sub -zones: 1) Faridpur trough, 2) Barisal gravity high, 3) Hatia trough, 4) Sylhet trough, and 5) South Shillong shelf zone. 4) Mobile belt: The eastern side of the Bengal Basin is bordered by a mobile belt known as Tripura - Chittagong fold belt, which extends north south as part of the Indo - Burmese mobile belt. In Bangladesh, this belt is represented mainly by the hills of the Chittagong Hill tracts, Chittagong and Sylhet, which appear to be analogous to the Sub - Himalayan or Siwalik ranges. They are characterized by the presence of long narrow folds composed of thick sandy shales of the Neogene age, which are 4000–8000 m thick (Alam 1989). The structure of this belt is of three categories: 1) On the west, they show box like forms, 2) the hills of the middle portion are of disturbed asymmetric structures, and 3) those on the eastside have more highly disturbed and complicated structures. 5) The Sub Himalayan fore deep is a continuous east - west Indo - Gangetic geosynclinal belt extending along the south foot of the Himalayas. Part of it cuts into 29

Bangladesh in the northwest corner (Fig. 3). The sediments of this unit include coarse to fine clastics that are derived directly from the Himalayan uplift and are essentially of fluvial mollasse in character. The north margin of this fore deep is strongly folded and faulted (Alam 1989).

4.3 Palaeogeography and Palaeotectonics

The paleogeography and paleotectonics of the Bengal Basin and surrounding areas have been studied by Dietz and Holden (1970), Curray and Moore (1971) Desikachar (1974), Graham et al. (1975), Banerjee (1981,1984), Curray et al. (1983), Gansser (1983), Le Dain et al. (1984), Salt et al. (1986), Alam (1989), Molnar (1984) and Klootwijk et al. (1992) gave a good account of the matter. Some of the important implications of these reconstructions are: 1. Basin development began in the Early Cretaceous epoch (ca. 127 Ma) when the rifted away from Antartica. After a plate reorganization ca.90 Ma, the Indian plate migrated rapidly northward and collided with Asia between ca. 55 and 40 Ma (Curray et al. 1983, Molnar 1984). 2. Sedimentation in the Bengal Basin has been controlled by the movement of the Indian plate, by the collision pattern of the Indian plate with the Burmese and Tibetan plates and by the uplift and erosion of the Himalayas and Indo-Burmese mountain ranges (Alam 1989). The sedimentation in the Basin has been almost continuous since the Cretaceous except for some localised discontinuities. The sedimentary sequences overlying the crystalline basement are invariably concealed under a thick cover of aluminium in Assam, West Bengal and Bangladesh (Banerjee 1984). 3. Folding in response to eastwards directed subduction beneath the western Indo- Burman Ranges has been responsible for the growth of the series of elongate N-S asymmetrical anticlinal structures of eastern Bangladesh. These structures form the attenuated frontal fold belt of the Chittagong Hill tracts and eastern margin of the SB (Salt et al. 1986). 4. The basin was formed as a result of unequal subsidence along certain specific trends in the northeastern portions of the Indian shield since the Cretaceous. The basin thus differentiated into several depressions and ridges, of which prominent were the Jessore depression and the Ridge. During the first phase of evolution the basin remained under the influence of the marine transgression till the end of Eocene when a major regressive phase took over most of its part (Banerjee 1984). The Eocene period was the period of maximum marine transgression. 5. In the Oligocene, large-scale uplift and erosion resulted in the marine retreat and progressive development of prograding deltaic conditions in the greater part of the basin. By the Miocene period, the impact of the collision of the Indian plate with the Tibetan and Burmese plates was severely felt in the basin, resulting in a large influx of clastic sediment both from the west and the east. The effect was a switch from flysch sedimentation to molasse sedimentation in most of the basin (Alam 1989). In the deeper part of the basin, the sedimentation was controlled by turbidities. The proto Bengal fan, similar to the present day Bengal deep sea fan (Curray and Moore 1974, 30

Graham et al. 1975) possibly played an important role in the sedimentation of the Bengal fore deep. Since Miocene times, the proto Bengal fan has been deformed by the compression of the Indian plate with the Burmese plate and was influenced by the tectonic activities of the Himalayas (Alam 1989). 6. During the Late Tertiary, the area experienced tectonic upheavals in the northeastern portion and the continuation of the fluvial delta complex co-existed in the lower plains since Plio-Pleistocene times. 7. Ninety East Ridge, lying on the Indian plate has been the site of a great "Megashear" or a gigantic "transform fault" along which the Indian plate glided a long distance towards the north without disrupting surrounding crustal plates (Dietz & Holden 1970). 8. Tectonic forces generated by the overridden Burmese plate from the east may have been responsible for east-west horizontal compression and differential vertical movement of the basinal materials to develop the folded belt of Chittagong and Chittagong Hill Tracts (Hossain 1985).

4.4 Surma Basin (SB), Sylhet (North East Bangladesh)

The Surma Basin is a sub-basin of the Bengal Basin situated in the northeastern part of Bangladesh. The basin is bounded on the north by the Shillong plateau, east and southeast by the Chittagong-Tripura fold belt of the Indo-Burman ranges, and west by The Indian Shield platform. To the south and southwest it is open to the main part of the Bengal Basin. The published Bouger anomaly map show gradual higher values (negative) towards the center of the basin. The Aeromagnetic interpretation map by Hunting (1980) indicates a gradual deepening of basement towards the center of the basin and also reveals subsurface synclinal features and faults within the basin. Its topography is predominantly flat with some north-south trending ridges of twenty to several hundred meters elevation present in the north-eastern border. It is actively subsiding (Johnson & Alam, 1991). The thickness of late Mesozoic and Cenozoic strata in the Sylhet Basin ranges from about 13 to 17 km has been estimated by some authors (Evans 1964, Hiller & Elahi 1984). Much of these strata are Neogene in age (Johnson and Alam 1991). The geology and hydrocarbon potential of the SB have been investigated by many workers (Holtrop & Keizer 1970, Lietz & Kabir 1982, Hiller & Elahi 1984, Khan et al. 1988, Chowdhury et al. 1987) but palynological studies are lacking. A number of wells have been drilled in the SB with the discovery of eight gas fields and the recent discovery of commercial quantities of oil in Sylhet–7 make this area more interesting to the geologists.

4.4.1 Wells studied

Wells studied for the present work include Atgram well – IX, Fenchuganj well – 2, Habiganj well – 1, Kailastila well – 1, Patharia well – 5 and Rashidpur well – 1 (Fig. 5). The necessary information of the wells is given in Table 4 as follows. 31

Table 4. Wells studied.

Well Name Location Drilled by Drilling time Total depth Atgram – IX 25°00´ 20´´N Parker drilling Co. 25.06.1981 – 4967,8m 92°24´ 30´´ E 10.06.1982 ( 16,288 ft ) Fenchuganj – 2 24°36´46´´ N PetroBangla* May 1980 3779m 91°57´23´´ E Habiganj – 1 24°13´55´´ N PSOC** 24.03.1963 – 3507,5m 91°22´47´´ E 22.05.1963 ( 11,500 ft ) Kailastila – 1 24°51´13´´ N PSOC** 31.08.1961 – 4140,9m 92°22´47´´ E 22.03.1968 ( 13,577 ft ) Patharia – 5 24°34´ N PetroBangla* 1989– 3436m 92°13´ E Rashidpur – 1 24°18´32´´ N PSOC** 22.02.1960 – 12,663ft 91°36´26´´ E 20.7.1960 * PetroBangla= National Petroleum exploration company of Bangladesh ** PSOC=Pakistan Shell Oil Company

4.4.2 Regional geologic setting

The Surma Basin is believed to come into existence in the Late to Post-geosynclinal phase. Partly a fault bounded trough, subsiding from the Oligocene or earlier Pliocene (Holtrop & Keizer 1970). The basin covers an area of roughly 10 000 km2 and is bounded in the north by the Pre-Cambrian Basement Complex (Wadia 1975) of the Shillong Massif and the Barail Ranges, by the Barail - Imphal Ridges in the east towards Assam and in the south by the Tripura High. In the west, The SB gradually ascends towards the Eocene Hinge Zone, while passing into The Bengal Foredeep (Khan et al. 1988). 32 e wells locations. with the sample Fig. 5. Showing the lithology of th of lithology Fig. 5. Showing the 33

The SB is a sub-basin of the Bengal Basin, the development of which began in the Early Cretaceous epoch (ca. 127 Ma) when the Indian plate rifted away from Antarctica (Johnson & Alam 1991). After a plate reorganization ca. 90 Ma, the Indian plate migrated rapidly northward and collided with Asia between ca. 55 and 40 Ma (Curray et al. 1983, Molnar 1984). The basin has been characterized by deltaic sedimentation since The Oligocene epoch. Today, the onshore part of the Bengal Basin is the site of the world's largest delta (about 60 000 km2) formed by rivers (Ganges, Brahmaputra/Jamuna, Padma, Meghna) that drain a large portion of the Himalayas (Johnson & Alam 1991). This subaerial delta feeds the world's largest submarine fan (Bengal Fan), which extends more than 3 000 km south into the Bay of Bengal (Curray & Moore 1974). The Bengal Basin gradually is being encroached on by the Indo-Burman ranges, an ~ 230-km-wide, active orogeine belt associated with eastward subduction of The Indian plate below Myanmar (Burma) (Brunnschweiler 1966, LeDain et al. 1984, Sengupta et al. 1990). In The Early Miocene, as the collision between the Indian and the Eurasian plates continued, there were further major phases of uplift in the Himalayas. Consequently, a large volume of clastic sediments was supplied to and began progressively to fill the Basin (Imam & Shaw 1985). SB is characterized by a large, closed, negative gravity anomaly (as low as 84 milligals), has minimal topography (elevations of about 5 to 20 m) and numerous lakes and swamps, and is actively subsiding (Johnson & Alam 1991). On the basis of seismic data, The SB cumulatively comprises an approximately 17 km thick (Hiller & Elahi 1984) sedimentary column from Post - Eocene Sylhet Limestone to Recent clastics. SB was structurally evolved by the contemporaneous interference of two major tectonic movements, i.e. the emerging of the Shillong Massif in the north and the west prograding mobile Indo-Burman Fold Belt (Hiller & Elahi 1984). The northern and eastern parts of the basin are far more complicated than the southern and western portions. The relief and complexicity increases towards the east (Haque 1982). The anticlines are commonly faulted and many produce gas (Johnson & Alam 1991). Structural relief between paired anticlinal crests and adjacent synclinal troughs may be as much as 7 000 m (Hiller & Elahi 1984), and the synclines have acted as major late Neogene and Quaternary depocenters. The folds decrease in amplitude westward, and are not present west of about 91° (Lietz & Kabir 1982), where the Sylhet trough merges with the main part of the Bengal Basin. The SG (Early Miocene - Quaternary) is a diachronous unit consisting of a succession of alternating shales, sandstone, siltstones and sandy shales with occasional thin conglomerates, indicative of repetitive deposition from pro-delta, deltafront, and paralic facies with intermittent, wholly marine facies (Holtrop & Keizer 1970). The group is divided into the Bhuban and the Bokabil Formations, based on differences in their gross lithologies (Mathur & Evans 1964) (Table 3). 34

Table 5. A chart showing the stratigraphy of the Surma Basin (SB) and surrounding areas including the Surma Group (SG) (*). Ages of nonmarine units are based on palynology. Data is from Baksi (1965), Chkaraborty (1972), Holtrop & Keizer (1970), Gupta (1976), Murthy et al. (1976), Banerji (1981,1984), and Murty (1983). Note that the time scale is not linear. Wavy lines show unconformities. The Time scale was adopted from Palmer (1983). 5 Analytical methods

5.1 Palynological slide preparation

Standard palynological techniques were utilized to isolate the palynomorphs. Palynomorphs mainly separated from shaly sequences. Samples were analyzed using conventional method for macrelation of spore/pollen from sediments. The subsequent acetolization has been carried out with the methods of Erdtman (1960). The samples were treated with 10 % HCl acid to dissolve carbonates and later with 10 % KOH to separate humas materials from taken sediment of 5–10 grams. After neutralization the residue was treated with concentrated HF acid to remove silicates. Palynomorphs were collected by filtration using 200 mm, 33 mm accordingly and in need, 10 mm polypropylene sieves were also used. After dehydrating, the residue was acetolized again. The residue was mainly preserved in glycerine jelly and glass slides were prepared on glycerine gelatine for microscope study.

5.2 Geochemical analysis

The core samples were a total of 188 in number and from 6 exploratory wells of Sylhet, Bangladesh: Habiganj well – 1, KailasTila well – 1, Rashidpur well – 1, Atgram well – IX well, Fenchuganj well – 2 and Patharia well – 5 (Sample analyzed for the study were 168 in number). The details of the samples are presented in the appendix-1 and 2. The present study includes major, trace and total REE (rare earth element) analysis of SG sediments (mainly shale) from the SB, Sylhet, Bangladesh. Sample preparation. The core samples were cut into pieces by using a rock cutter and then were crushed by a crushing machine to reduce the rock aggregate to monomineralic particles. These samples were divided into seven parts by a mechanical divider. One part was crushed by Vibrating Disk Mills (Herzog, type: Hsm 100 A) and six parts were sieved to get size fraction <0.06 mm and in some cases <0.125 mm. Both crushed and sieved fractions were analyzed. For clay mineralogical studies, clay size fractions were 36 separated by centrifugation. Thin sections were prepared both from original core and mixed powdered samples.

5.2.1 X-ray Fluorescence (XRF)

The crushed samples were used to determine the major element composition by XRF. Analyses were carried out with a Siemens SRS-X-Ray 303 AS XRF spectrometer with standard curves based on International Rock Standards at the Institute of Electron Optics, University of Oulu, Finland. Analysed major elements were SiO2, TiO2, Al2O3, Fe2O3, MnO, MgO, CaO, Na2O, K2O and P2O5 and trace elements were As, Ba, Bi, Ce, Cl, Cr, Cs, Er, Gd, La, Nb, Nd, Pb, Pr, Rb, Sc, Sr, Th, U, V, and Zr.

5.2.2 Atomic Absorption Spectrometry (AAS)

Two hundred mg of sample was taken into a Teflon crucible. Then one ml HClO4 and two ml HF were added and placed in the sand bath for heating. Afterwards, two ml conc. HCl was added to dissolve the sample and allowed to evaporate until there was no solution left. Finally, diluted fraction of the deposit was analysed for trace elements using a spectrum of AA300 with an acetylene-air flame. Organic maturity (OM) rich elements Co, Cr, Cu, Ni, Pb and Zn were selected for the analysis.

5.2.3 Loss of Ignition (LOI)

First the samples were dried at 110–120°C. Then dried samples were heated for two hours at 950°C and LOI was determined.

5.2.4 Accuracy of analyses

The accuracy determinations by both AAS and XRF was checked using certified reference materials. A correlation between the data of Cu, Zn, Ni and Pb (Patharia well-5 and Rashidpur well-1) measured by AAS and XRF was done and presented in figure 6. They are all in positive correlation. For the well, Rashidpur-1 three elements (Zn, Cr & Ni) are correlated strongly and Pb shows a positive which indicate that two results (AAS & XRF) are in good agreement. The error was found to be 3–4%. Nesbitt (1992) mentioned that for XRF analyses, the error in major oxides is about 1–2%. Wronkrewicz and Condie (1987) mentioned that the precision and accuracy are within 5% for most major elements and for minor and trace elements are 5–10% for the samples measured by XRF and INA 37

(Instrumental neutron activation) methods. However present study analyses bears 95 % confidence level.

70 140

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Ni ( XRF) B Pb ( XRF) ppm ppm

Fig. 6. A. Figure showing the correlation of the data (in ppm) of Cu, Zn, Ni and Pb for Patharia well – 5. All of them are in good positive correlation. B. Figure showing the correlation of the data of Cu, Zn, Ni and Pb for Rashidpur well-1. Three of them (Zn, Cu & Ni) are correlated strongly in positive and Pb shows also positive correlation means two results are in good agreement. 38 5.3 Mineralogical analysis

5.3.1 X – Ray Diffraction (XRD)

Crushed and clay fraction were examined by a SIEMENS D 5000 X-Ray diffractometer with Ni filtered CuKα radiation using 40 kV-40 mA. Samples were X-rayed using Ni- filter Cukα radiation with a scan range from 4 to 40º 2θ, a step size of 0.2º and a dwell time of 1s per step. The clay fraction (<2 µm) was separated out from the shale by disaggregating and despersing the sample in distilled water and immediately washed by centifugation. The fraction of <2 µm was isolated by centrifugation and suspension was dried on glass slides. The clay sample in oriented mounts were run under three separate conditions: i) air dry state. ii) after ethylene glycol treatment and iii) after heating to 550º C for 1 hour.

5.3.2 Transmission Electron Microscopy (TEM)

Clay-size fractions were prepared for a TEM study by dispersing the material in alcohol. The samples were placed on a formvar - coated TEM grid (150 mesh) and examined with JEOL, JEM-100 CX fitted with link AN10-25S and a Jeol JEM 1200 Leo 912 OMEGA equipped with the same microanalysis electron microscope. Various magnifications were used to obtain suitable micrographs of clay minerals. Electron microscopy is the only method capable of measuring the size of individual single particles. The method allows for direct measurement of the several dimensions of the particles and thus also the shape of the particles is to be taken into account (Bates 1971).

5.3.3 Scanning Electron Microscopy (SEM)

A few thin sections of clay-size fractions coated with an Au-Pd conductor (Polaron SEM coating unit E 150) were examined morphologically under JEOL JSM 6400 (with Link EXL, EDS) Scanning Electron Microscopy (SEM). The thin sections of representative samples were analysed for semiquantitative determination of primary and secondary minerals especially for Ba detection.

5.3.4 Petrographic microscopy (optical)

Thin sections were made both from the core samples for mineralogical analyses by petrographic microscope. 39 5.4 Statistical analysis and ratios

Data acquired from XRF and AAS was used for the analyses of major oxides, ΣREE and certain trace elements. Table 6 illustrates statistical analyses and ratios used in this study. Correlation of data between the present study and the published data was done whenever possible.

Table 6. Statistical analysis and ratios.

Subject Ratio / Crossplots Reference Grain size SiO2/ Al2O3 Björlykke 1974 Maturity (M) 1) K2O+Al2O3/ Björlykke 1974 Na2O + MgO 2) K2O/ Na2O; Björlykke 1974 Rb/ K2O Wedephol 1969 4) Cu/ Zn Hallsberg 1976 Major element % Major element Harker type ΣREE diagram ΣREE Bhatia 1985 Provenance 1) Cr/ Rb, Zr/ Rb, V/ Rb and Bellanca et al. 1999, Ba/Rb; 2) Cr/ Ni Garver & Scott 1995 Environment of deposition Cr/ V and Ni Dypvik 1979 Tectonic setting SiO2 vs. K2O/ Na2O Roser & Krosch 1986 Mineralogy 1) Crossplots of Cr, Rb, Zr, K2O% and Grömet et al. 1984 (Weathering & Diagenesis) TiO2 versus Al2O3 2) Crossplots of Cr+Ni, V, MnO% and Fe2O3 McLennan et al. 1983 versus MgO 3) Crossplots of U, Th, Ba, Al2O3 versus McLennan et al. 1983 K2O% 6 Stratigraphy

The stratigraphy of the Surma Basin (SB) and surrounding areas is summarized in Table- 2. The stratigraphy of the Neogene Surma Group sediments of SB is presented on the basis of core sample studies (n=188) and of palynological studies (74) of six exploratory wells: Atgram–IX, Fenchuganj–2, Habiganj–1, Kailastila–1, Patharia–5 and Rashidpur–1. The studied samples range in depth from 959m to 4735m. Detailed description of the various lithologies composing the Surma Group are provided in the measured cores of the wells (appendix-1) and also presented graphically (Fig. 5). The Surma Group (SG) is a thick sequence of clastic sediments consisting of an alternation of sandstone, shale and siltstone that infilled the vast basinal area of the Bengal Basin during Miocene-Pliocene time. In the subsurface, the unit is represented by thick sand-shale sequences in all the wells drilled in the area. The Surma Group unconformably overlies the Barail Group of the Oligocene age and is overlain by the sandstone dominating the Tipam Group of the Pliocene age (Holtrop and Keizer 1970). The SG is divided into a lower Bhuban formation and an upper Bokabil formation based on gross lithology.

6.1 Lithofacies

Two major lithofacies were identified in the SG unit: sandstone lithofacies A and combined facies B consisting of claystone, mudstone and shale. Facies B is the most abundant, whereas facies A is less common. These lithofacies generally are defined on the basis of grain size, clay content and depositional bedding characteristics. Facies A consist of massive, thinly inter-bedded and inter-laminated, fine to medium-grained sandstone. Facies B consists of laminated bluish, bluish gray and gray to black shale from gray to yellowish-gray siltstone to very fine grained sandstone. Lithofacies A may grade vertically into the combined lithofacies and be interbedded with the combined lithofacies. Facies B shows two types of lithofacies in the shaly layers. They are: 41

a) homogeneous shale and b) shale with sand or sand partings. The first type shares the most abundant lithofacies. Lithofacies B is composed of siltstone and sandstone lamine, layers are generally 1- 5mm thick. Thick intervals as much as 30-40cm are common in the lithofacies B.

6.2 Palynological study

Palynological studies based on 74 selected core samples from the wells of Atgram – IX, Fenchuganj – 2, Habiganj – 1, Kailastila – 1, Patharia – 5 and Rashidpur – 1. Details of the samples are given in appendix 1 and 2 (* marked). The samples were selected from all the cores of the wells representing the various lithostratigraphic positions. From individual cores, the samples were selected so that the top, bottom and the middle of the cores are represented. The study was aimed to establish the age of the SG, palynostratigraphy in order to better constrain reconstruction of palaeoenvironmental and palaeoclimatic variations in Bangladesh during the Neogene.

6.3 Pollen data and pollen assemblage zone

Pollen analysis has been performed on selected samples. In order to make sense of the considerable amount of data shown in a typical pollen diagram it is necessary to divide the diagram into pollen-stratigraphic units characterized by distinctive groups of pollen types. In this way, pollen zones were constructed from the samples of Fenchuganj-2 and are presented in Figs 7 and 8. Detailed palynological studies of this area is lacking because of poor preservation of the palynomorphs. Palynomorph recovery from the cores of the wells drilled in the area was few. In some parts the wells were almost void of specimen. Palynomorph content in the prepared palynological slides for palynostratigraphic analysis were extremely poor for the present study. No palynomorphs (other than fungal spores) were detected in 38 out of the 74 slides. Due to this, the idea of a quantitative analysis of palynomorphs was abandoned except for the Fenchuganj well – 2. The results of this well allowed us to make some quantitative analysis and a qualitative analysis was attempted for the remaining wells. No palynological research paper has been published from this region yet. Identification and comparison were made for the present study on the basis of published literature on the Tertiary Palynology of the Assam and the Bengal Basin of India (Table 1 and Table 2).

6.4 Palynostratigraphic zonation

Among the wells studied, palynomorph recovery was predominantly good only for the Fenchuganj well – 2. Both the qualitative and quantitative analysis of the palynoflora was 42 possible only for this well. A total of 35 samples were selected from 12 cores of this well for palynological study. The depth of the samples ranged from 957.6 m to 4095 m. The palynoassemblages from sediments recovered from SG (Miocene) are rich in pteridophytic spores and angiospermous pollen grains whereas the gymnospermous pollen grains and fungal remains are comparatively less represented. The assemblage consists of 63 genera and 95 species of palynomorphs. The SG sediments dominantly consist of shale with some sandstones. On the basis of the qualitative and quantitative analyses of the palynoflora, the SG sequence of this well has been divided into three biostratigraphic zonations. The following parameters have been taken into consideration to establish and recognize these zones: a) Maximum development of various palynotaxa, b) the first and last appearance of them, and c) decline, restricted occurrence and absence of certain palynotaxa. Then comparisons with other similar palynoassemblages of surrounding areas (India) were made along with interpretations regarding paleoclimate, environment of deposition and age.

6.4.1 Palynostratigraphic zonation of Fenchuganj well – 2

The three local palynostratigraphic zones in the SG sediments sequence of Fenchuganj well – 2 are as follows in ascending order of stratigraphy. iii) Disaccate Zone, ii) Tricolpate-trilete zone, and i) Palmepollenite zone. i) Palmepollenite zone. This zone constitutes the lower biostratigraphic unit of the SG. The zone is characterized by Palmepollenites which are abundant. Species restricted to this zone are lygodiumsporites, Trilete Cing 1a, Polypodiisporites Oligocenisus, Monolites mawkmaensis, Texodium, Tsuga, Inaparturate L1a, Inapeturate reticulate, Retipilonapites, Cl-grain 1a, Diporopollenites, Polycolpites sp, Monaporites anulatus, Polyporina, Chamopodiacea, Tricolporates (C3P3)-Pet 2a and Fusiformisporites. The following characteristic palynotaxa have been identified - Cyathidites minor, Lycopodium sporites, Cicatricosisporites macrocostatus, Schizacea, Trilete-L1a, Trilete- ret 1a, Trilete-granu 1a, Trilete-verru 1a, Trilete sig+rug 1a, Iaevigatosporites 1a, Verrucatosporites, Emparitus dissaccate, Inaperturate L1a, Couperipollis sp, Dicolpites Tricolpats C3-4a, C3-L2a, C3-ret 1a, C3-ret 2a, C3-verru 1a, Marginipolis sp, Meyeripollis naharilotensis, Carya, Betula, Triporopollenits sp, P3 L2a, P3 ret 2a, P3 grain 1a, Florschuetzia levipolli, Rhizophora, C3P3- L1a, C3P3 -L2a, C3P3-Pet 1a, Hystriokiospheridum and Fungus remains. Comments. The significant feature of this zone is that the Palmepollenite constitutes 31 % of the sequence. The dominance of this taxon, is, therefore, important and helps us in distinguishing from the overlying Tricolpate-trilete zone. Pteridophytic spores contains 48 % in this zone. Angiouspermous pollen grains represent 50% while gymnospermous pollen grains are insignificantly represented by 3.8 %. Among the pteridophytic spores, triletes are very abundant. Trilete spores are represented by Cicatricosisporites macrocostatus, Trilete levigates, Trilete reticulate, 43

Trilete granulate and Trilete verrulate. Monolete forms are mainly Laevigatosporites Type-1. Pollens of Graminidites have not been observed in this zone. Presence of Rhizophora pollen provides a basis to interpret the paleoenvironment of the drilled sequence. Last appearance: Monolites mawkamaensis, Monoporites anulatus, Tsuga, Texodium and Inaperturates L1a. ii) Tricolpate - trilete zone. Tricolpates (C3) and Triletes (T) are the most common forms of palynoforms. Some of the forms were restricted to this zone only. Species restricted to this zone are Tricopates rug1a type, Carpinus, Triporopollenits Scab 1a, Polygonacidites sp, Syncolporats sp, Trilete-rug 1a, Dandotriasporits sp. and Eximispera. Characteristics palynotaxa are Cyathidites minor, Triletes L1a type, Triletes ret 1a, Triletes grain 1a, Triletes-verru 1a, Disaccate striat, Palmepollenites, Couperipollis sp, Tricolpates (C3)-L1a type, C3-rat 2a, C3-scab 2a, C3-apl 1a, Marginipollis sp, Triporopollenites ret 1a, Rhizophora, Tricolporates (C3P3) Pet 1a type, C3P3 -Fov 1a, C3P3 - Scab 1a, Hystrichospheridum. Comments. This zone is characterized by very high frequency of Tricolpate-Triletes which is about 50% of the palynofossils. For this reason the zone is named after these taxon. Graminitides is conspicuous by its complete absence in this zone. Gymnospermous pollen grains are about 4%, the presence of Rhizopora pollen is important for paleoenvironmental interpretation. iii) Disaccate zone. This zone shows a clear dominance of Disaccate pollen. Ninety eight forms of disaccate were present in the zone. Species restricted to this zone are Sphagnum, Undulatisporites, Polypodiaceosprites, Trilete-fov 1a type, trilete-apl 1a type, Striatopollis bellus, Florschuetzia levipoli, Tricolporates granulates 1a, Tetracolporates L1a, Tetred and Alnipollenites. Characteristic palynotaxa identified in this zone are Cyathidites minor, Lycopodium sporites, Cicatricosisporites macrocostatus, Schizaccae, Trilete L1a, T–ret 1a, T–gran 1a, T -verru 1a, Laevigatosporites, Verrucatosporites, Emparitus, Monolet ret 1a, Palmepollenites, Couperipollis sp., Tricolpate L1, C3 - L2a, C3 - ret 1a, C3 - ret 2a, C3 - verru 1a, C3 - scab 2a, C3 - apl 1a, Marginipollis sp., Meyeripollis naharikotensis, Carya, Betula, Triporopollenites, P3 - L2a, P3 - ret 1a, P3 - ret 2a, P3 - grain 1a, Triolites L1a, Florschuezia meridonalis, Rhizophora, Nyssa pollenites sp., Triporopollenites - L1a, C3P3–L2a, C3P3–scab 1a, Hystrioispheridum. Comments. Disaccate is the dominant pollen of this zone. Pteridophytes are usually represented by the monolete forms such as Levigatosporites, and Verrucatosporites, as well as by a few trilete spores like Cyathidites minor. Monocolpate pollen occur in low frequencies and are represented by the genus palmepollenites. The microfloral association of the Palynological zone I can be compared with the palynological assemblage of the Simsang Palynological Zone IV of Meghalaya, India (Baksi 1965) and the Bengal Palynological Zone (BPZ) V (Baksi 1971) and indicate Lower to Middle Miocene age. The presence of Rhizophora pollen and the presence of dynoflagillates provide a basis to interpret the paleoenvironment of the drilled sequence as brackish to shallow marine deposits. Representative forms of Foraminifera also indicate that sediments may be deposited in shallow marine condition. 44

The microflora of the Palynological zone II can also be compared with those of the Simsang Palynological Zone IV of Meghalaya, India and BPZ V (Baksi 1971). Based on these comparisons the Palynological Zone II is presumed to be of Middle to Upper Miocene. It is interesting that the floral change from monolet pollen Palmepollines to Tricolpate – trilete could be recognized well by an increase in frequency by 50%. The presence of mangrove pollen Rhizophora indicates the brackish environmental deposition of this drilled sequence. The microfloral assemblage of the Palynological Zone III may be compared with Simsang Palynological Zone IV of Meghalaya, India (Baksi 1965) and BPZ Zone V of Bengal (Baksi 1971). According to these comparisons, the age of Palynological Zone-III is presumed to be Upper Miocene. A significant floral change has been observed in this zone by the abundance of dissacate pollen and a decline in the pteridophytic spores, particularly triletes. These pollens might have migrated from the extra-peninsular region in the north, which would have been sufficiently high during Lower Miocene.

6.4.2 Atgram well – IX

In this well, 15 samples were taken from a depth ranging from 3 638 m to 4 735 m, but the recovery of palynomorphs were from only four samples representing three different cores. The qualitative analysis of palynoassemblage reveals the presence of following taxa: Bisaccate, Laevigatosporites, Rhizophora, Disaccate, Gymnosperm, Cyathidites minor, Verrutriletes, Cicatricosisporites, Palmepollenites, Couperipolies, Polypo- diaexoisporites, Verrucatosporites, Simsangia, Meyerripollies Naharkotensis, Polypodeace, and Florschuetzia trilobata. Among Foraminifera, Hystrichosphaeridium and Veryhachium were present in the area. Some dinoflagillete cysts were also identified in the sequence. The age of the sequence has been identified as Miocene Foraminifera with Hystrichospheridium indicates a marine- brackish environment. Hystrichospherida is a widely distributed facies indicator. The presence of reworked microfauna elements and conifer pollens, together with the transgression indicators, indicate an increased tectonic activity in the Surma Basin during this period and they are related to the burial of the basin and the uplift of the Himalayas.

6.4.3 Habiganj well – 1

In this well, only three samples were productive out of 19 samples ranging from 1250 m to 3125 m. The three samples were representing three different cores. The qualitative analysis of palynoassemblage reveals the presence of the following taxa: Disaccate pollen, Pteridophyte Monoletes, Cicatrieosisporites, Laevigatosporites, Tetracolpates, Alnipollenites, Triporopollenites, Simsangia, Monocolpate, Triporate, Tricolpites, 45

Tricolporopollenites, Varrucosisporites sp., and Polypodiisporites. The samples were identified as Pliocene to Miocene in age.

6.4.4 KailasTila well – 1

In this well, ten samples ranging from 1 175 m to 3 969 m were taken for the study but only four samples were productive. The following palynotaxa were identified: Disaccate pollen, Pteridophyte Monoletes, Cicatricosisporites, Laevigatosporites, Tetracolpate, Alnipollenites, Triporopollenites, Simsangia, Monocolpate, Triporates, Bissaccates, Graminidites sp., Cyathidites, Polypodisporites, Trilete, Verrucosisporites, Polypodiacoispoiretes, and Lycodiumsporites. Some dinocysts (Indeterminate) were also observed. The samples were identified as Pliocene to Lower Miocene in age.

6.4.5 Patharia well – 5

The qualitative analysis of palynomorphs of the Patharia well-5 has been done on the basis of 12 core samples ranging from 956,1 m to 2 833 m taken from 5 cores. Summary of Palynostratigraphy of Patharia well-5 is given in Table 6. The samples were identified as Lower Miocene in age (Lower Bhuban). Characteristic palynomorphs are: Disaccate, Verrucatosporites, Simsangia, Cicatricosisporites, Polypodiaceoisporites, Palmaepollenites, Couperipollis, Gymnosperm, Triorite, Verrutriletes, Monocolpate, Meyernipollies Naharkotensis, and Florschuetzia. Forms of Foraminifera that were encountered in the core no. 3 and 4 are: Globogerine bulloids, Globoretalia, Globigerinoides, and Haplophragioides. The environment of deposition was brackish to shallow marine condition for this well. The samples studied were identified as Lower Miocene age (Lower Bhuban).

6.4.6 Rashidpur well – 1

Only few palynomorphs were recovered from the samples in this well. Five samples were productive out of 10 samples ranging from 1 081 m to 2 477 m. The palynomorphs encountered in this well were: Disaccate pollen, Pteridophyte monoletes, Cicatricosisporites, Laevigatosporites, Tetracolpate, Alnipollenites, Triporopollenites, Simsangia and Monocolpate. Some dinocyst (Indeterminate) were observed also. 46 6.4.7 Comparison with surrounding areas (from India)

The microfloral association of the Palynological zone I can be compared with the palynological assemblage of the Simsang Palynological Zone IV of Meghalaya, India (Baksi 1965) and the Bengal Palynological Zone (BPZ) V (Baksi 1971) and indicate a Lower to Middle Miocene age. The presence of Rhizophora pollen and the presence of dynoflagillates provides a basis for interpreting the palaeoenvironment of the drilled sequence as brackish to shallow marine deposits. Representative forms of Foraminifera also indicates that the sediments may be deposited in a shallow marine condition. The microflora of the Palynological zone II can also be compared with those of the Simsang Palynological Zone IV of Meghalaya, India and BPZ V (Baksi 1971). Based on these comparisons, the Palynological Zone II is presumed to be of Middle to Upper Miocene. It is interesting that the floral change from monocolpate pollen Palmepollines to Tricolpate - trilete could be recognized well by an increase in frequency by 50 %. The presence of mangrove pollen Rhizophora indicates the brackish environmental deposition of this drilled sequence. The microfloral assemblage of the Palynological Zone III may be compared with the Simsang Palynological Zone IV of Meghalaya, India (Baksi 1965) and BPZ Zone V of Bengal (Baksi 1971). According to these comparisons, the age of Palynological Zone-III is presumed to be Upper Miocene. A significant floral change has been observed in this zone by the abundance of dissacate pollen and a decline in the pteridophytic spores, particularly triletes. These pollens might have migrated from the extra-peninsular region in the north which would have been sufficiently high during the Lower Miocene.

6.4.8 Comparison with other Miocene Assemblages

6.4.8.1 Assam and Meghalaya sequences

Baksi (1965) reported Simsang Palynological Zone IV from the southern Shillong Plateau, Assam, now Meghalaya. That assemblage contained a few marine hystrichosphaerids and microforaminifers in the lowermost part. Marine micro-organism disappeared in the middle part of the zone. There are some common elements between the Miocene assemblages of Simsang Palynological Zone IV and the well studied. The abundance of bisaccate coniferous pollen belonging to Coniferipites Baksi and a restricted occurrence of Coniferipites chattacharai are the characteristic features of Simsang Zone IV assemblage. In the present study, bisaccates occur sporadically in the Miocene assemblages but Podocarpidites pollen resembling Conferipites chattacharai is restricted to the Miocene, as it is in Simsang Zone IV assemblage. Also, Baksi’s Schizaeaceaesporites and Parkeriaceaesporites appear to be equivalent to Magnastriatites howardi, but they are more abundant in the Simsang Zone IV (Sah and Dutta 1967), as they are in the Miocene of the studied well. 47

In addition, the long-range taxa Spinosopites acolporata, and Polypodiaceaesporites sp. of Baksi (= Verrucatosporites usmensis) and various palm pollen occur in both assemblages. Sah & Dutta (1967) described the stratigraphic succession of the Tertiary palynomorphs in Assam. They reported high abundances of Cicatricosisporites macrocostatus (Baksi et al. 1967) in the Miocene.

6.4.8.2 Bengal Basin

In describing the Bengal basin Zone V and VI, Baksi (1971) points out that they indicate a major shift of flora elements due to well recognized tectonic events related to the Himalayan orogeny, involving the uplift of the South Shillong Front and the associated development of progressively colder climates in the surrounding areas of the Bengal Basin (including the Surma Basin). Baksi also states that the Simsang Palynological Zone IV can be ”confidently” correlated with the Bengal Palynological Zone V by the index elements designated by him as ”Coniferipites – Cicatricosisporites Assemblage Zone”. This assemblage appears to be equivalent to Zone - III. Meyeripollis naharkotensis occurs sporadically in the Simsang palynological Zone IV (Miocene) of Meghalaya (Baksi 1965). In this respect the study area bears a significant resemblance to the Simsang Zone IV. Other resemblances are the presence of Schizaeaceaesporites sp. of Baksi, 1962 (= Magnastriatites howardi), small tricolporate pollen, Parkeriaceaesporites of Baksi, 1962 (= Verrucatosporites usmensis). Comment. Palynomorph recovery was very poor. Only Fenchuganj well-2 slides allow one to make quantitative analysis. 48

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Reconstruction of palaeoenvironment and palaeoclimatic variation in the Surma Basin of Bangladesh during the Neogene is based on complex stratigraphic sequences which include a variety of sediment facies and a variety of palynomorphs, indicating a range of depositional environments. The most frequent and qualitatively most important of these are illustrated in Figs 7 and 8. The most gross environments of deposition for the SG sediments are shallow marine to brackish interdeltaic environments. This interpretation is based on the predominance of lithofacies B and the distribution of pollen, spores, microplankton and dinoflagellets. The pollen flora with dominating angiosperm species suggest tropical to subtropical areas. The occurrence of aquatic ferns (Cicatricosisporites) indicate brackish conditions of sedimentation. The proximity of the sea is indicated by the presence of marine microplankton. Recording of microfauna such as Bolivia, Bulimina, Globigerina and Rotalia from Rashidpur well (Holtrop & Keizer 1969) is indicative of more open marine sedimentation. Foraminifera with Hystrichosphaeridium indicates a marine-brackish environment. Hystrichosphaerida is a widely-distributed facies indicator. The presence of reworked microflora elements and conifer pollens, together with the transgression indicators, indicates an increased tectonic activity in the SB during the Neogene and they are related to the Himalayas. The SB area were progressively coming under the tectonic control to the great Himalayan orogeny and the crustal shortening due to the collision of the Indian and Asian plates and have resulted in extensive uplifts and thrusting of the older rocks (Banerjee 1984). Throughout the Miocene, SB has witnessed a conspicuous subsidence and marine transgression. The transgression of the Miocene certainly affected the coastline. The above mentioned palaeo-environmental circumstances must at some stage have contributed to the retrogressive succession of the vegetation in the area. In this connection, it is pertinent to refer to some ecological aspects of palms, as they feature so prominently in the pollen sequence. At present, palms are considered to be very important in the evolution of tropical forest ecosystems and must have been even more so in the past (Moore 1973). The pteridophytic-rich assemblage may suggest the existence of an inland swamp flora during the time of deposition of these sediments. The presence of Foraminifera in association with a palynomorph assemblage containing mangrove forms and dinoflagellate cysts suggest a shallow marine environment. The sandstones with siltstone and shales were deposited in a shallow marine environment throughout the Miocene. The shallow marine and brackish environment reflects a marine transgression. The pollen spectra of SB contain a high percentage of regionally produced pollen of mixed sub - tropical vegetation. It reflects a mixture of palm and coniferous forest in which palmepollinite is dominant. Palynostratigraphic zones suggest a progressive improverishment of the mixed type of subtropical to tropical forest types existing there and the development of dominant palm vegetation. Grasses, according to the pollen data, were already established in this area during the early to Mid. Miocene and experiencing summer rainfall similar to the present day climate. 50

As far as known, the Rhizophora pollen type is unique and cannot be confused with pollen from other taxa (Germeraad et al. 1968, Muller 1964). The presence of Rhizophora in the Miocene sequence suggest the Neogene sediments of marine origin. The Surma Basin has undergone two successive phases of evolution. The marine transgressive phase, followed by a regressive phase resulting in a series of continental fluvio-deltaic to marginal marine sedimentation during the Neogene. The Great Himalayan Orogeny and associated tectonics dominated the SB during Miocene-Pliocene times. Major changes in sea level for Neogene are suggested based upon trangressive- regressive phenomena. A marked rise in sea level would have caused a marine transgression (Bandy 1968). The proximity of the sea is indicated by the presence of marine microplankton. The overall evidence thus suggests that vegetation was establishing on a marshy area close to the sea. It also suggests a subtropical humid climate (Srivastava 1970). Similar marine deposition and its environment were also identified for West Bengal, Meghalaya and Tripura geo-provinces of India (Banerjee 1984).

6.6 Age

Studies of pollen samples from the SG sediments of Surma Basin have indicated a Neogene age for the unit. On the basis of a regional study of dinoflagellates, SG can be assigned as early to late Miocene in age. This conclusion is based upon the following reasons: 1. The stratigraphic position of the SG unit 2. The absence of typical Oligocene assemblage and 3. A general resemblance of the microflora to the Miocene assemblages in Assam, Meghalaya and Bengal, India – the neighbouring country. In Assam sequence, which is very close to the Surma Basin, Magnastriatites howardi {= Cicatricosisporites macrocostatus (Baksi 1962), Sah & Dutta (1968) is restricted to the Miocene}. 4. An abundance of Conifer pollen and the presence of taxa Florschuetzia trilobata, F. levipol.

6.7 Maturity

Maturity. The maturity of palynomorphs is refered to color indices of thermal alteration index which attain during and after sedimentation. Fenchuganj well-2 samples were marked pale-yellow to brownish colour of polynomorphs indicating the mature stage from the depth below 3615 m (Core No. 10). From core 3 to 9, low maturity was assigned. According to the maturity study, the sediments within the depth range of 3615 – 4095m are to be considered as an organically matured stage. 51 ganj well – 2 of Surma Basin, Bangladesh. Surma of 2 well – ganj ing % variations of main taxa from Fenchu from taxa main variations of % ing Fig. 7. Pollem diagram show Fig. 7. Pollem diagram 52

Fig. 8. Pollen and spores from study areas (SB).

6.8 A list of palynomorph recovery from the Fenchuganj well-2 with their possible botanical affinity

Palynoflora taxa present in the well Fenchuganj –2. Botanical affinity 1. Cyathidites minor Cyatheaceae 2. Lycopodium sporites Lycopodiaceae 3. Sphagnum Sphagnaceae 4. Eximispra Unknown 5. Cicatricosisporites Schizaeacea 6. Undulatis porites Unknown 7. Dandotriasporites Unknown 53

8. Scizaoisporite Schizaeceae 9. Polypodiaceoisporite Polypodiaceae 10. Lygodiumsporites Schizaeceae 11. Trilete(T)-L1a Sphagnum 12. T – reticulate Sphagnum 13. T – granulate 1a Sphagnum 14. T – Verrulate 1a Unknown 15. T – rugosa 1a Unknown 16. T – Cing 1a Unknown 17. T – fovulate 1a Unknown 18. T – Sig + rug 1a Unknown 19. T – aperturate Unknown 20. Leavigatosporites 1a Polypodiaceae 21. Polypodiisporites sp. Polypodiaceae 22. Verrucatosporites Polypodiaceae 23. Emparitus Unknown 24. Polypodiisporites Oligocenicus Polypodiaceae 25. Monolites Mawkmaensis Polypodiaceae 26. Monolites reticulate 1a Polypodiaceae 27. Texodium Unknown 28. Disaccate Podocarpidites 29. Tsuga Pinaceae 30. Disaccate striat Podocarpidites 31. Inaperturate L1a Unknown 32. Inaperturate – reticulate Unknown 33. Retipilonapites Unknown 34. Palmaepollenites Arecaceae 35. Couperipollis sp. Palmae 36. Monocolpate (C1) – grain 1a Unknown 37. C1 – Echniiz 1a Unknown 38. C1 – L2a Unknown 39. Dicolpatis sp. Unknown 40. Liliacidites Liliaceae 41. Tricolpate (C3) – L1a Acer 42. C3 – L2a Acer 43. C3 – reticulate 1a Unknown 44. C3 – reticulate 2a Unknown 45. C3 – grain 1a Unknown 46. C3 – Verrulate Unknown 47. C3 – regose 1a Unknown 48. C3 – scab 2a Unknown 49. C3 – apl 1a Unknown 50. C3 – favulate 1a Unknown 51. Diporopollenites Unknown 52. Striatopollis Unknown 53. Marginipollis Unknown 54

54. Meyeripollis naharilotensis Unknown 55. Polycolpites sp. Lamiaceae 56. Tetracolpate (C4) – L1a Unknown 57. Monoporites anulatus Unknown 58. Carya Caryaceae 59. Carpinus Corylaceae 60. Betula Betulaceae 61. Triporopollenites Moraceae 62. Triporate (P3) – L1a Ovoidites 63. P3 – L2a Ovoidites 64. P3 – reticulate 1a Ovoidites 65. P3 – ret 2a Ovoidites 66. P3 – grain 1a Unknown 67. P3 – scab 1a Unknown 68. Periporate – reticulate 2a Unknown 69. Polyporina Malvaceae 70. Periporate – L1a Unknown 71. Chanopodiaeea Unknown 72. Polygonacidites sp. Dorseraceae 73. Florsechetzia meridonalis Unknown 74. Florsechetzia Levipol Unknown 75. Florsechetzia trilobata Unknown 76. Rhizophora Rhizophoraceae 77. Illex pollenites Aquifoliaceae 78. Rhoipites niditus Unknown 79. Nyssa pollenites Nyssa 80. Tricolporate (C3P3, sp.) – L1a Quercus 81. C3P3 – L2a Quercus 82. C3P3 – Pet 1a Unknown 83. C3P3 – Pet 2a Unknown 84. C3P3 – Fovulate 1a Unknown 85. C3P3 – Scab 1a Unknown 86. Tetracoliporites similes Unknown 87. Tetracolporates (C4P4) – L1a Unknown 88. Syncolporate sp. Unknown 89. Tetred Unknown 90. Alnipollenites Betulaceae 91. Hystrioispheridum Algae 92. Rusiformisporite Fungal spore 93. Fungus Fungi 94. Dinoflagellates 95. Foraminifera 55

Palmaepollenites Polypodissporities Polypodiaceoisporite

Verrucatosporites Verrucatosporites Dissacate alnipollenite

Dissacate pollen Monocolpate pollen Cicatricosisporite

Verrucatosporite Verrutrilete spore Palmepollenite

Plate 1. (All figures X500 magnification). 56

Verrutrilet Tricolporate reticulate Tricolpate verrucates

Tricolporate Tricolporate Tricolporate

Tricolporate levigate Mayeripollis naharkotensis Mayeripollis

Trilete spore Dicolpate pollen Palmaepollenites

Plate 2. (All figures X500 magnification). 57

Dynoflagelates Cicatricosisporites

Polypodiacedisporites Hystrichospheridium

Verrucatosporites Grami Pollenites

Plate 3. (All figures X500 magnification). 58

Meyeripollis Palmepollenite pollen Disaccate pollen naharkotensis

Cicatricosisporites Marco Hystrichospheridium Trilete Granulate cocostatus

Trilete spore Hystrichospheridium Florsechetzia trilobata

Alnipollenite Fungal pore Disaccate pollen Couperipollis spinson (Monocolpate)

Plate 4. (All figures X500 magnification). 7 Geochemical results

7.1 Major elements (XRF & AAS)

Major, trace and REE geochemistry of the core samples of SG sediments of the SB were studied in detail. The detail XRF and AAS analysis of the samples is presented in Appen- dix 2. The abundance of major elements analyzed in the samples are presented graphical- ly (Figs 9–14) for all the wells.

7.1.1 Major elements

The major element composition of the SG sediments of SB determined in this study is compared to the composites (Average shale, Pettijohn 1975, The North American Shale Composite, Grömet et al. 1984, AGV-1, Flanagan 1973, Bhuban shale of Jaintiapur, Syl- het, Bangladesh, Islam 1996, and well data from the present study) and presented in Table 8. In general, the bulk composition of the Neogene shale (NS) of the present study com- pares quite closely with these previously published estimates of average shale composi- tions. The ratio of SiO2/Al2O3 is centered within the range established for shales.

Table 8. Comparison of Chemical composition of shales. Wt% NASC* AGV-1 Bhuban Shale** Average Shale Present study (Grömet (Flanagan 1973) (R. Islam 1996) (Pettijohn 1975) Habiganj well-1 et al. 1984) (A. Mannan 2002) SiO2 64.82 60.41 68.65 58.10 61.63 TiO2 6.80 1.06 0.74 - 0.87 Al2O3 17.05 17.66 14.96 15.40 16.34 Fe2O5.706.264.554.026.95 MnO0.250.100.03-0.09 MgO2.831.571.032.443.01 CaO 3.51 5.02 0.05 3.11 1.93 Na2O1.314.360.771.301.57 K2O3.972.932.913.243.25 P2O5 0.15 0.50 0.09 - 0.16 * NASC = North American Shale Composite. ** Bhuban Shale = Sylhet, Bangladesh. These chemical results sug- gest that the present study data has the qualities of an average of averages. 60 4,0 5 3,5 4 3,0 ) ) 3 2,5 wt % wt wt % ( ( 2,0 O 2 2 K CaO CaO 1,5 ndix – 1 and 2. Dash 1 1,0 ,5

0 Depth

Depth (m) 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 m 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 8 1,4 7 1,2 le interval see Appe 6 1,0 5 (wt%) 3 O (wt %) O (wt ,8 2 O a 2 4 N Fe ,6 3 ,4 2 Depth Depth (m) 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 m 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 ,2 20 18 16 14 ,1 the well Atgram – IX. For details of samp details of IX. For well Atgram – the 12 (wt%) 3 O 2 10 MnO (wt %) (wt MnO Al 8 6 0,0

4 Depth

Depth m 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 m 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 k of sample intervals. k of 3,5 100 3, 90 2,5 80 2,0 70 1,5 (wt%) 2 MgO (wt %) (wt MgO 60 SiO 1,0 ,5 50 lines indicate the brea Fig 9. Major element variation curves for 0,0

40 Depth Depth m 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 m 3633 3634 3635 3636 3637 3638 3639 3640 4729 4733 4735 61 4,0 16 14 3,5 12 10 s indicate 3,0 8 O (wt%) 2,5 2 6 CaO (wt%) CaO K 4 2,0 2 1,5 0 Depth Depth 200 3141 3268 3730 3766 4094 3137- 3624- 3742- 3141 3268 3730 3766 4094 2190- 3259- 3265- 4086- (m) 2200 3137- 3624- 3742- 2190- 3259- 3265- 4086- (m) 2 9 1,7 tails of the sample. Dash line 1,6 8 1,5 7 1,4 (wt %) 3 O (wt %) O (wt 2 O 2 6 Na Fe 1,3 5 1,2 1,1 4 Depth Depth 200 3141 3268 3730 3766 4094 200 3137- 3624- 3742- 2190- 3259- 3265- 4086- (m) 2 3141 3268 3730 3766 4094 3137- 3624- 3742- 3259- 3265- 4086- 2190- (m) 2 ,8 20 – 2. SeeAppendix-1 and 2 for de ,7 18 ,6 16 ,5 ,4 14 (wt%) 3 O 2 ,3 MnO (wtMnO %) Al 12 ,2 10 ,1 0,0 8 Depth Depth 3141 3268 3730 3766 4094 3137- 3624- 3742- 2190- 3259- 3265- 4086- (m) 2200 3141 3268 3730 3766 4094 3137- 3624- 3742- 3259- 3265- 4086- 2190- (m) 2200 7 80 6 70 ) 5 wt % ( 4 (wt %) (wt O 2 60 g M SiO 3 50 2 1 40 Depth Depth 200 3141 3268 3730 3766 4094 3137- 3624- 3742- 3259- 3265- 4086- 2190- (m) 2 3141 3268 3730 3766 4094 3137- 3624- 3742- 2190- 3259- 3265- 4086- (m) 2200 Fig 10. Major element variation curves for the well Fenchuganj Fenchuganj well the for curves variation element Major 10. Fig the break of sample intervals. 62 ,0 4 16 14 1 3,5 ) 10 3,0 8 CaO /wt % /wt CaO O (wt%) 6 2 K 2,5 4 2 ,0 2

0 Depth Depth (m)

(m) 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 1,6 8,5 8,0 1,5 2 for details of the sample interval. Dash interval. 2 for sample details of the 7,5 7,0 1,4 6,5 (wt %) (wt O (wt %) O (wt 3 2 O 6,0 2 Na Fe 1,3 5,5 5,0 1,2

4,5 Depth Depth (m)

(m) 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 1,0 20 18 ,8 16 ,6 14 MnO (wt %) (wt MnO 4 , (wt%) 3 O 12 2 the well Habiganj – 1. See Appendix 1 and Al ,2 10 0,0 8 Depth Depth (m)

(m) 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 3,6 70 3,4 68 3,2 66 3,0 64 2,8 62 2,6 (wt %) (wt 2 60 2,4 SiO MgO (wt %) (wt MgO 58 2,2 2,0 56 1,8 54 Depth Depth (m) lines indicate the break of sample intervals. of sample break the indicate lines (m) variation curves for Fig 11. Major element 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 1255- 1256 1257- 1258 1259 1849- 1850 1851- 1852 3110- 3111 63 6 4,0 sh 5 3,5 4 3,0 3 O (wt %) O (wt 2 K CaO (wt %) CaO (wt 2 2,5 1 2,0 0 Depth Depth 1175 1176 1177 2272 2973 2974 3731 3968 3730 1175 1176 1177 2272 2973 2974 3731 3968 (m) 3730 (m) 1,6 9 1,4 8 1,2 7 1,0 (wt %) (wt 3 O 0 (wt %) 0 (wt 2 2 6 ,8 Fe Na ,6 5 ,4

4 Depth 1175 1176 1177 2272 2973 2974 3731 3968 Depth (m) 3730 1175 1176 1177 2272 2973 2974 3731 3968 (m) 3730 1. See Appendix 1 and 2 for details of the sample interval. Da ,16 20 ,14 18 ,12 16 (wt %) (wt 3 ,10 O 2 l A 14 MnO (wt %) (wt MnO ,08 12 ,06 10 ,04 Depth Depth 1175 1176 1177 2272 2973 2974 3731 3730 3968

(m) (m) 1175 1176 1177 2272 2973 2974 3730 3731 3968 70 1,6 68 1,4 66 1,2 64 (wt %) (wt 1,0 2 0 (wt %) 0 (wt 2 62 SiO Na ,8 60 ,6 58 ,4 56 Depth Depth 1175 1176 1177 2272 2973 2974 3731 3968 3730 1175 1176 1177 2272 2973 2974 3731 3968 (m) 3730 (m) Fig 12. Major element variation curves for the well Kailsatila – Kailsatila well the for curves variation element Major 12. Fig lines indicatesample intervals. the break of 64 4,0 20 3,5 lines 3,0 ) 2,5 10 wt % ( 2,0 O (wt %)O (wt 2 CaO CaO 1,5 K 1,0 ,5 0 Depth Depth Dash interval. sample (m)

(m) 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 9 2,0 8 1,8 7 2 for details of the 2 for details 1,6 6 (wt %) (wt 3 5 O (wt%) 2 O 1,4 2 a N Fe 4 1,2 3 2 Depth 1,0 Depth (m)

959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 (m) 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 ,7 22 20 ,6 18 ,5 16 ,4 14 (wt %) (wt 3 12 ,3 O 2 10 Al MnO (wt %) MnO ,2 8 the well Patharia – 5. See Appendix 1 and – 5. See Appendix 1 Patharia the well ,1 6 0,0 4 Depth Depth (m)

(m) 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 80 3,5 3,0 2,5 70 2,0 (wt %) (wt 2 MgO (wt (wt %) MgO 1,5 60 SiO 1,0 ,5 50 Depth Depth (m)

(m) 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 959- 964 1450- 1457 1837 2290- 2307 2828- 2834 3160- 3168 Fig 13. Major element variation curves for for curves variation element Major 13. Fig intervals. sample of break the indicate 65 6 3,8 h 3,6 5 3,4 4 3,2 3 O (wt %) O (wt 2 K CaO (wt %) (wt CaO 3,0 2 2,8 1 e sample interval. Das interval. e sample 2,6

0 Depth Depth (m)

(m) 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 1,8 8,5 1,7 8,0 1,6 7,5 and 2 for details of th 1,5 7,0 (wt %) 3 O (wt%) O 2 2 a 1,4 6,5 Fe N 1,3 6,0 1,2 Depth 5,5 Depth (m) (m) 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 ,18 19 ,16 18 17 ,14 16 ,12 (wt%) 3 O 2 15 l MnO (wt %) (wt MnO ,10 A 14 ,08 13 ,06 Depth 12 Depth (m) 1 for Appendix Rashidpur – 1. the rves See well (m) 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 12 68 10 66 k of sample intervals. 8 64 (wt %) (wt 2 6 62 MgO (wt %) (wt MgO SiO 4 60 2

58 Depth Depth (m) 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 Fig 14. Major element variation cu (m) brea lines indicate the 1081- 1087 1248- 1254 1827- 1832 2134- 2135 2472- 2473 66

Gulf coast shales have K2O contents that increase systematically with depth from ~2 to 4 wt% in the Paleocene-Eocene Wilcox Formation and from 2 to 5 wt% in the Oligocene - Miocene Frio-Anahnac succession (Bloch et al. 1998). For the present study all the welldata of K2O content varies between 2-3.5 wt%. Potter et al. (1980) has shown the geochemical properties of shales change with time. For example, several workers have reported significantly higher K2O in early Paleozoic shales ,than in younger shales. Comparison between the histogram of modern sediments of the Sylhet area (Islam 1996) and the SG sediments (Miocene) of Rashidpur well-1 shows a marked decrease of SiO2 content(Fig.15). The mean value of SiO2 varies from 79.0 to 62.65 (Fig.16a). The average value of Al2O3, K2O and TiO2 has enriched markedly from 9.7 (mean value) to 15.85, 1.75 to 3.12 and 0.63 to 0.86 respectively (also Fig.16b). SiO2. Most samples from the wells showed SiO2 contents between 60 and 70 wt%. The highest value was 89.40% in the Atgram well-IX well (Sample No. 83) which is a shale (this is an exceptional sample with very high content of SiO2). The highest value in general was 75.51% (Atgram well-IX) and 74.51% (Patharia well – 5), both the samples were sandy shale. Variation was least in Rashidpur well – 1 (Standard deviation = 1.54) suggestive of a uniform source composition during that interval. Sample interval (Depth) interval Sample Sample

Fig 15. Comparison between the silicon dioxide of modern sediments of Sylhet area and the SG sediments (Miocene) of Rashidpur well – 1 shows a marked decrease of SiO2 content. Dash line indicate the average line. For younger sediments it is 78 % and 63 % for the present study. Younger sediment data from Islam 1966. Samples are from Jaintiapur, Sylhet. (exposed rock) Figure 14 shows the actual depth of the samples of Rashidpur well – 1. 67

Al2O3 % SiO2 %

TiO2 % K2O %

Fig 16. A Histogram showing major oxides of Rashidpur well – 1. Percentages are in wt %. 68

Al2O3 % SiO2 %

TiO2 % K2O %

Fig 16. B. Histogram showing major oxides of modern sediments (Data from Islam 1996). Note the differences of oxides between the samples. Percentages are in wt %.

The SiO2/Al2O3 ratio (wt % SiO2/ wt % Al2O3) is also often used as a grain-size indi- cator (Dypvik 1979). A plot of this ratio prepared for all the wells has been presented. The grain size parameters studied show little fluctuations in fine grained sequence. The wells Atgram well-IX, Rashipur well-1, Habiganj well-1 and KailasTila well-1 have downward coarsening tendency and the Fenchuganj well-2 well show relatively coarse grained upward. The overall sequence of the SiO2/Al2O3 ratio shows the dominance of the fining with a coarsening tendency at the bottom for the wells mentioned. The SG sedi- ments (Neogene shale) reflects a shallowing of the depositional basin and the deposition of more altered material. Palynological and geochemical studies match well the shallo- wing conditions shown. The SiO2 content in all the wells studied seems to decrease with increasing Al2O3. As large amounts of quartz are found in the residual material, it is reasonable to assume that desilicification took place mainly by a destruction of aluminosilicates. A plot of Al2O3 against the SiO2%/Al2O3% ratio of samples from Patharia well-5 shows a strong negative correlation. The Fe2O3/ Al2O3, Na2O/Al2O3 and K2O/Al2O3 ratios in the samples vary 69 against the Al2O3 concentrations (Fig. 17). The results indicate the presence of clay mine- rals.

K2O/Al2O3 SiO2/Al2O3 Al Al 2 2 O O 3 3 (wt %) (wt %) (wt

Fe2O/Al2O3 Na2O3/Al2O3 Al Al 2 2 O O 3 3 (wt %) (wt (wt %) (wt

Fig 17. Crossplots of Al2O3 versus K2O/Al2O3, SiO2/Al2O3, Fe2O/Al2O3 and Na2O3/Al2O3 for Patharia well – 5 show negative correlation indicating the presence of clay minerals. Percentages are in wt %.

The percentage of selected major elements in Harker-type (%) variation diagrams for the rocks of the study area has been prepared (Fig. 18–22). In case of SiO2, Al2O3, Fe2O3, TiO2 and K2O, normal source variation and grain size variation give rise to similar trends. Except KailasTila well-1 and Rashidpur well-1, MgO also have similar trends. In the case of CaO, Na2O and MnO, the vectors were different. The results illustrate a similar ele- ments composition from all the samples, reflecting homogeneity of the sediment suite. Variation in the chemical composition reflects changes in the mineralogical composition of the sediments due to the effects of weathering, marine sedimentation and early diage- netic processes (Shaw & Weaver 1965, Drever 1971, Nesbitt & Young 1984,1989). The 70 abundance of Al, Si, K and Ti in shales may be perturbed from parent material by weathe- ring, transport and depositional processes (Nesbitt & Markovies 1996).

SiO (wt %) SiO2 (wt %) 2 Fig 18. Harker type major element (%) variation diagrams for Atgram well – IX. 71 2 TiO CaO

SiO2 SiO2 CaO O 3 2 O 2 Na Al

SiO2 SiO2 O 2 MnO K

SiO 2 SiO2 3 O 2 MgO Fa

SiO2 (wt %) SiO2 (wt %)

Fig 19. Harker type major element percentage variation diagram for Fenchuganj well – 2. 72

SiO2 (wt %) SiO2 (wt %)

Fig 20. Harker type major element percentage variation diagrams for Habiganj well – 1. 73 2 TiO MgO

SiO2 (wt %) SiO2 (wt %) O 3 2 O 2 Na Al

SiO2 (wt %) SiO2 (wt %) MgO CaO SiO (wt %) 2 SiO2 (wt %) 3 O O 2 2 K Fe

SiO2 (wt %) SiO2 (wt %) Fig 21. Harker type major element percentage variation diagrams for Kailastila well – 1. 74

SiO2 (wt %) SiO2 (wt %) Fig 22. Harker type major element percentage variation diagrams for Patharia well – 5. . 75

The different maturity parameters studied display complicated development with an increasing maturity having fluctuations in different depth interval. The maturity index (M) used in this study was defined by Björlykke as M = Al2O3 + K2O / MgO + Na2O (Björlykke 1974) and the parameter is stratigraphically controlled, showing the same trend in different districts. The index is also controlled by the clay mineral. The other two maturity parameters used for the present study were K2O/Na2O and Rb/K2O ratios (Björ- lykke 1971, Dypvik 1977, 1979). Dypvik has shown that high K2O/Na2O and Rb/K2O ratios are indicative of a Kaolinization process and typically mature sediment. All the maturity parameters used in this study show an apparently fluctuating maturity for all wells. In general, the lower portions showed increasing maturity. All the three maturity parameters showed a similar trend for the wells studied (Fig. 23–28). It is pos- sible to demarcate the wells stratigraphically by mature and immature zones. The matu- rity increases with depth, indicating renewed deposition, new weathering conditions and particularly source area variations. The study also showed that the maturity increases with the decrease of the silica content and grain size. The trend of K2O/Na2O ratios in Fig. 23–28 is interesting and is consistent with the grain size analysis. Na and K in the studied Neogene shales are mostly confined in the detrital illites. Deer et al. (1963) noted that fresh muscovite contains more K and Na than average illite. Micas are often degraded to illite during weathering by loss of K and Na, uptake of H2O and partial opening of the lattice. Coarser fractions of the sediment will tend to include fresher micas, alternatively, finer fractions carry more degraded illites and more smectites (Pearson 1979). An increase in sodium and potassium with coarseness of the sediment may then arise naturally. The ratio of K2O/Na2O shows a fluctuating scenario for all wells studied which are between 0.70 and 4.26. These differences obviously reflect in part the different original compositions of the source rocks. 76

M = K O + Al O /Na O + MgO SiO2/Al2O3 2 2 3 2 K2O/Na2O

Rb/K2O Cu/Zn

Fig 23. Showing the grain size (SiO2/Al2O3) and maturity (M) index curves for the well Atgram – IX. Note that the maturity curves are more or less similar and reverse to the curve of SiO2/ Al2O3 indicate that the maturity increases with the decrease of silica content and grain size. Figure 9 shows the actual depth of the samples. 77

M = K O + Al O /Na O + MgO SiO2/Al2O3 2 2 3 2 K2O/Na2O

Rb/K2O Cu/Zn

Fig 24. Showing the grain size (SiO2/Al2O3) and maturity (M) index curves for the well Fenchuganj – 2. Note that the maturity curves are more or less similar and reverse to the curve of SiO2/Al2O3 indicate that the maturity increases with the decrease of silica content and grain size. Figure 10 shows the actual depth of the samples. 78

M = K O + Al O /Na O + MgO SiO2/Al2O3 2 2 3 2 K2O/Na2O

Rb/K2O Cu/Zn

Fig 25. Showing the grain size (SiO2/Al2O3) and maturity (M) index curves for the well Habiganj – 1. Note that the maturity curves are more or less similar and reverse to the curve of SiO2/Al2O3 indicate that the maturity increases with the decrease of silica content and grain size. Figure 11 shows the actual depth of the samples. 79

M = K O + Al O /Na O + MgO SiO2/Al2O3 2 2 3 2 K2O/Na2O

Rb/K2O Cu/Zn

Fig 26. Showing the grain size (SiO2/Al2O3) and maturity (M) index curves for the well Kailastila – 1. Note that the maturity curves are more or less similar and reverse to the curve of SiO2/Al2O3 indicate that the maturity increases with the decrease of silica content and grain size. Figure 12 shows the actual depth of the samples. 80

M = K O + Al O /Na O + MgO SiO2/Al2O3 2 2 3 2 K2O/Na2O

Rb/K2O Cu/Zn

Fig 27. Showing the grain size (SiO2/Al2O3) and maturity (M) index curves for the well Patharia – 5. Note that the maturity curves are more or less similar and reverse to the curve of SiO2/Al2O3 indicate that the maturity increases with the decrease of silica content and grain size. Figure 13 shows the actual depth of the samples. 81

SiO /Al O / 2 2 3 K2O/Na2O Rb/K2O

Cu/Zn M = K2O + Al2O3/Na2O+MgO

Fig 28. Showing the grain size (SiO2/Al2O3) and maturity (M) index curves for the well Rashidpur – 1. Note that the maturity curves are more or less similar and reverse to the curve of SiO2/Al2O3 indicate that the maturity increases with the decrease of silica content and grain size. Figure 14 shows the actual depth of the samples.

The enrichment of MgO in all the wells is related to a decrease of CaO in the sequen- ces and the opposite is due to the weathering effect. A high MgO content is often correla- ted with low temperature oxidative diagenesis (Bhat & Ahmed 1990). In such a case, an increase of MgO in the rock is accompanied by a drop in CaO (Andrews 1980). Mg corre- lates well with Al only if samples with MgO greater than 3 % are omitted (Fig. 29 shows the correletion of Al2O3 and MgO for 3 wells) thus indicating that this element is origi- nally associated with aluminosilicate phases and assumes minor association with carbona- tes during diagenesis. (Bellanca et al. 1999). There are clear positive correlations between K content and the abundances of Al, Cs, Ba, Th and U (Fig. 30), suggesting that absolute abundances of these elements are prima- rily controlled by the amount of the dominant original clay mineral (illite). The higher K content is almost certainly due to the original presence of large quantities of illite (McLennan et al. 1983). Decreasing K2O/Na2O ratio in the well indicates the decreasing maturity of the sediments, reflecting reduced influx of highly Kaolinzed mate- rial. Factors such as increased erosion in relation to weathering, and/or transgression resulted in Kaolinite - depleted rocks (Dypvik 1979). This interpretation is reasonable 82 when combining the results of other geochemical ratios like Rb/K2O and Cs/K2O and also with the mineralogical data followed (Fig. 31). K2O show a strong positive correla- tion indicating their association with the aluminosilicate phases (Fig. 31). The absolute abundances of transition elements are correlated with the concentration of Mg (Fig. 32). The positive correlation is probably due to the incorporation of these ele- ments in chlorite, the other major clay mineral (McLennan et al. 1983). The sequences of the wells exhibit depletions of Na and Ca probably reflecting intense chemical weathering of their source rocks. Al2O3, CaO, Na2O and K2O are related with the chemical index of Alteration. They exhibit variations in the whole sequence as shown in Fig. 9–14, which reflect chiefly variable climatic zones or rates of tectonic uplift in source areas. It is notable that the peaks of MnO and CaO occur at the same positions. The Mn con- tent of the Neogene shale may be ascribed to concentrations of the element by secondary oxidation and would indicate that oxygen was present at the seafloor during their deposi- tion (Bellanca et al. 1999). A correct approach to interpret the chemical results in terms of paleoproductivity reconstruction and of aluminosilicate phase fluxes is to infer the principal elemental asso- ciations (Bellanca et al. 1999). Because Al concentration is reasonably thought to be a good measure of detrital flux, the excellent positive correlations of K2O, TiO2, Na2O and MgO with Al2O3 indicate that these elements are associated entirely with detrital phases as shown in figure 30. and also suggesting that they are associated with aluminous clay minerals such as illite or smectite, and indicate that weathering was an important factor in the source area, where K and Mg are fixed in clay minerals and Ca is preferentially leached (Nesbitt et al. 1980). Alternati- vely, the clays may have been more aluminous and later enriched in K to form illite (Fedo et al. 1995, 1996). 83 MgO (wt %) (wt MgO

Al2O3 (wt %) MgO (wt %)

Al2O3 (wt %) MgO (wt %) (wt MgO

Al2O3 (wt %)

Fig 29. Showing the crossplots of Al2O3 vs. MgO for (a) Rashidpur well – (b) Fenchuganj well – 2 and (c) Patharia well – 5. All are in positive correlation. Patharia – 5 well correlate strongly. 84

4,0 1,0

,8 3,0

,6

2,0

,4

1,0 ,2 wt % wt 2 O wt % 2 TiO

K 0,0 0,0 0 3 5 8 10 13 15 18 20 0 3 5 8 10 13 15 18 20

Al2O3 wt % Al2O3 wt %

180 300

160

140

120 200

100

80

60 100

40 m m pp

pp 20

0 Rb Rb

Cr 0 0 3 5 8 10 13 15 18 20 0 3 5 8 10 13 15 18 20

Al2O3 wt % Al2O3 wt %

1400

1200

1000

800

600

400

m 200 pp

Zr Zr 0 0 3 5 8 10 13 15 18 20

Al2O3 wt %

Fig 30. Shows the crossplot of K2O, TiO2, Cr, Rb and Zr versus Al2O3 of Patharia well – 5. Except Zr all are in positive correlation. 85

6 20

18

4 16

14 2 12

. % ) . % 10 0 ) ( Wt

3 8 O 2 (ppm

Al 6

U -2 0,0 ,5 1,0 1,5 2,0 2,5 3,0 3,5 4,0 0,0 ,5 1,0 1,5 2,0 2,5 3,0 3,5 4,0

K2O ( Wt. % ) K2O ( Wt. % )

40 30

30

20 20

10 10 ) ) 0 Cs ( ppm ( Cs Th ( ppm Th ( -10 0 1,0 1,5 2,0 2,5 3,0 3,5 4,0 1,0 1,5 2,0 2,5 3,0 3,5 4,0

K2O ( Wt. % ) K2O ( Wt. % )

4000

3500

3000

2500

2000

1500

) 1000 m pp

500 (

Ba 0 1,0 1,5 2,0 2,5 3,0 3,5 4,0

K2O ( Wt. % )

Fig 31. Crossplots of U, Th, Cs, Ba and Al2O3 versus K2O of Patharia well-5. All are in positive correlation. 86

300 9

8

7 200

6

5

100 ) 4 (Wt. % (Wt.

3 3 O 2 Cr + Ni ( ppm ) ppm ( + Ni Cr 0 Fe 2 1,0 1,5 2,0 2,5 3,0 3,5 1,0 1,5 2,0 2,5 3,0 3,5 MgO ( Wt. % ) MgO (Wt.%)

,7 180

,6 160

,5 140

,4 120

,3 100 ) ,2 80

,1 60

MnO ( Wt % Wt ( MnO 0,0

V (ppm ) (ppm V 40 1,0 1,5 2,0 2,5 3,0 3,5 1,0 1,5 2,0 2,5 3,0 3,5 MgO ( Wt. % ) MgO ( Wt. % )

Fig 32. Crossplots of (Cr+Ni), Fe2O3, MnO and versus MgO of Patharia well – 5. Except MnO all are in positive correlation.

Tectonic setting determination of SG sediments using SiO2 content and the K2O/Na2O ratio. Literature analyses of sandstones and shales from ancient sedimentary sequences of inferred tectonic settings have been used to establish a tectonic classification based on SiO2 content and K2O/Na2O ratio (Roser & Korsch 1986). Three first-order tectonic cate- gories, broadly similar to those of Crook (1974), have been made. Several depositional settings are possible under each category. The categories presented by Roser and Korsch (1986) and those which have been adopted for the present study are: 1) Passive Continental Margin (PM). Mineralogically mature (quartz-rich) sediments deposited in plate interiors at stable continental margins or intracratonic basins. Repre- sented by Ordovician and Silurian greywackes and shales from Australia that are recycled quartz - rich sediments derived from older adjacent continental terrains (Wyborn & Chap- pell 1983). 2) Active Continental Margin (ACM). Quartz-intermediate sediments derived from tectonically active continental margins on or adjacent to active plate boundaries. Repre- sented by rocks from: a) the Franciscan Complex, California (Bailey et al. 1964) and Kodiak Formation, Alaska (Connelly 1978) the Santa Ynez Mountains, California (Van de Kamp et al. 1976) which were deposited at a complicated continental margin where both subduction and strike - slip processes were active. Hence this category includes complex active margins including material derived from continental margin magmatic arcs (and deposited in a variety of basin settings including trench, forearc, intra-arc and back-arc) and material derived from uplifted areas associated with strike - slip faults and deposited in pull - apart basins. 87

3) Oceanic Island Arc (ARC). Quartz-poor volcanogenic sediments derived from ocea- nic island arcs. Represented by: a) the Baldwin Formation, Australia (Chappel 1968) which are forearc basin sediments derived from an andesitic island arc source, and b) The Uyak and Cape Current greywackes, Alaska (Connelly 1978), which were derived from an andesitic source and deposited in a trench adjacent to an active volcanic arc. Hence, sediments in this category were derived from an island arc source and were deposited in a variety of settings including forearc, intra-arc and back-arc basins and trenches. All the categories defined reflect the composition of rocks in the source areas. Reading (1982) defined five types of sedimentary basins related to plate tectonic setting. A binary plot of K2O/Na2O–SiO2 diagram prepared for all the six wells (Fig. 33). Data from the six wells of SB fall into distinct field of ACM which is consistent with the paleo- tectonic history of the Basin. Except 3 samples from Atgram well - IX which fall in PM and 2 samples from Patharia well-5 fall in Oceanic Island arc margin (ARC). The data suggest that the chemistry of Neogene Shale (NS) can indeed be used for tectonic discri- mination. Seismotectonic and tectonic reports of the region by Chandra (1978), Chaudhury and Srivastava (1976), Molnar (1984), Nandy and Dasgupta (1991) and Verma (1991) as well as the report from the study area by Khan (1985) are in good agreement with the present result. 88 O O 2 2 O/Na O/Na 2 2 K K

SiO2 SiO2 O 2 O 2 O/Na 2 O/Na 2 K K SiO2 SiO2 O O 2 2 O/Na O/Na 2 2 K K

SiO2 SiO2

wt % wt %

Fig 33. Tectonic discrimination diagram for shales of the wells 1) Fenchuganj well-2 (N=20), 2) Habiganj well-1 (N=19), 3) Kailastila well-1 (N=9), 4) Atgram well-IX (N=10), 5) Rashidpur well-1 (N=40) and 6) Patharia well-5 (N=73). PM = Passive margin; ACM = Active continental margin; ARC = Oceanic Island arc margin. Most of the samples are in Active Continental margin except 3 samples from Atgram well-IX which fall in Passive margin and 2 samples from Patharia well-5 fall in Oceanic Island Arc margin. (Roser & Korch 1986) 89 7.2 Trace elements

The trace element concentrations of the wells studied are given in appendix 2. Various geochemical ratios calculated for the trace-element geochemistry from the study area are displayed in Table 9. A number of bivariate plots of trace elements were prepared by using an SPSS compu- ter programme and are presented). Trace-element concentrations in sediments result from the competing influences of provenance, weathering, diagenesis, sediment sorting, and the aqueous geochemistry of the individual elements. REE, as well as, Th, Sc and to a les- ser extent Cr and Co are the most useful for provenance characterisation, because they are among the least soluble trace elements and are relatively immobile. These elements are believed to be transported exclusively in the terrigenous component of sediment and the- refore reflect the chemistry of their source (McLennan et al. 1980). The Cu/Zn ratio as a radox parameter, as put forward by Hallberg (1976), was com- puted for all the wells and is shown in figures 23–28. The Cu/Zn ratio of the wells shows fluctuations for the whole sequence indicating reducing and oxidizing conditions. The increasing value of the ratio indicates a reducing, depositional condition while decreasing Cu/Zn values suggest increased oxidizing conditions. However, the highest Cu/Zn ratio is seen in different depth levels in the wells studied, which will be discussed later in the dis- cussion chapter. The abundance of Th and U in the wells are quite variable. The average concentration of Th and U is 28 and 2 ppm respectively in the sediments and Th/U = 3.80 (min.) and 35 (max.) (Figs 34–39). The higher abundance of Th in the rocks reflects the presence of Th bearing minerals. The higher Th/U ratio probably indicates the derivation of these sedi- ments from the recycling of the crust. Recycles of sediments themselves lead to a further loss of U and increase in Th/U ratio. The higher value of the Th/U ratio in the core samp- les is because of oxidation. As originally pointed out by Taylor and McLennan (1985), the Th/U ratio does not change or record a change in source composition. The present observation suggests that the Th/U in NS does not record a change in source composition but is controlled by the weathering erosion - diagenesis cycle. Condie (1993) has shown a similar observation with a study of shales from upper continental crust, USA. According to McLennan et al. (1993) the Th/Sc ratio is a sensitive index of the bulk composition of the provenance. The abundances of Th in sedimentary rocks can be rela- ted to the abundances in the upper continental crust. Accordingly, the average La/Th and Th/Sc ratios are fairly constant in sedimentary rocks: ~ 2.8 and ~ 1.0 respectively (McLennan 1989). The average La/Th ratio of the samples investigated is 2.6, and corres- ponds closely with these data. The Rb and Th levels, in turn, suggest an enrichment of a felsic component (Lahtinen 1996). Rb and Ba are considered to some extent to be concentrated relative to K and fixed in clays during weathering (Nesbitt et al. 1980). Th is considered to reliably characterise the source composition (McLennan et al. 1990) Possibly, the main part of Th occurs in ferromagnesium minerals with subsequent attachment to clays during weathering. 90

Table 9. Major chemical and lithological characteristics of the wells of Surma Basin, Sylhet, Bangladesh.

Well N SiO2%SiO2/ K2O/ M* U/K2O Th/K2OBa/K2OCr/VNi/CuV/NiZr/Hf Al2O3 Na2O KailasTila-1 9 59.04 – 3.14 – 1.77 – 2.54 – 0.29 – 6.04 – 1.29 – 0.87 – 1.45 – 1.15 – 30.11 – 67.84 6.09 4.26 14.27 1.79 16.15 216.15 1.08 2.57 2.22 71.00 Atgram-IX 11 46.20 – 2.92 – 1.59 – 4.13 – 0.28 – .00– 150.99 – 0.16 – 1.15 – 1.67 – 16.13 – 89.40 18.98 3.06 10.33 4.60 7.48 431.03 1.18 2.43 2.95 48.20 Habiganj-1 19 55.41 – 3.27 – 1.64 – 3.91 – 0.27 – 7.64 – 144.44 – 0.89 – 1.38 – 1.66 – 36.67 – 67.43 6.14 2.59 4.60 2.37 12.32 203.11 1.14 2.70 2.20 229.00 Fenchuganj- 20 50.57 – 2.98 – 1.67 – 2.65 – 1.14 – 5.70 – 99.15 – 0.94 – 1.171 – 1.56 – 30.00 – 2 71.30 6.34 3.15 4.69 2.49 14.39 206.97 1.27 2.40 2.30 317.00 Rashidpur-1 40 58.76 – 3.31 – 1.81 – 1.65 – .00 – 7.19 – 140.94 – .82 – 1.57 – 1.36 – 24.00 – 66.30 5.03 2.60 4.89 1.43 10.36 302.36 14.00 12.00 3.08 285.00 Patharia-5 69 55.32 – 2.99 – 0.70 – 3.26 – .00 – .00 – 26.07 – 0.27 – 1.13 – 0.92 – 16.14 – 76.22 9.04 3.05 5.56 3.39 13.11. 286.00 2.59 3.82 4.18 1259.00

Well N Zr/Nb Th/U Th/Sc Th/Cr La/Th Cu/Zn Cr/Th Cr/Rb Zr/Rb V/Rb Ba/Rb Kailastila-1 9 12.39 – 4.75 – 1.21 – 0.17 – 1.17 – 0.11 – 3.60 – 0.55 – 1.08 – 0.52 – 2.02 – 29.58 35.00 2.21 0.28 2.13 0.52 5.96 1.00 2.69 1.08 4.25 Atgram-IX 11 13.38 – 3.80 – 1.27 – 0.21 – 0.74 – 0.27 – – 0.10 – 1.06 – 0.60 – 2.68 – 33.50 22.00 1.75 1.00 2.58 0.51 5.00 0.75 4.24 1.15 11.36 Habiganj-1 19 9.64 – 5.20 – 1.17 – 0.21 – 0.81 – 0.28 – 2.85 – 0.53 – 0.93 – 0.46 – 2.32 – 16.65 31.00 2.89 0.35 2.00 0.42 4.73 0.63 1.94 0.66 2.77 Fecnhuganj- 20 12.47 – 7.25 – 1.33 – 0.16 – 1.10 – 0.30 – 2.86 – 0.53 – 1.03 – 0.55 – 2.13 – 2 28.82 30.00 2.31 0.35 2.30 0.48 6.45 0.86 2.62 0.73 3.47 Rashidpur-1 40 7.82 – 6.25 – 1.76 – 0.18 – 1.18 – 0.07 – 3.61 – 0.53 – 0.93 – 0.60 – 2.32 – 15.44 30.00 2.64 0.28 2.16 0.45 5.44 0.91 2.15 0.77 5.54 Patharia-5 69 4.56 – 00 – 00 – 00 – 0.58 – 0.17 – 1.14 – 0.17 – 0.54 – 0.61 – 0.48 – 61.14 425.00 317.00 0.88 13.67 4.60 6.83 2.22 7.86 0.86 55.80 M* = maturity = Al2O3 + K2O/Na2O + MgO

Some four elements like V, Ba, Cr and Zr were normalized to Rb and the profiles were constructed and presented (Figs 34–39). The reason for normalization to Rb is that this element is inert with respect to biogenic processes (Emelyanov & Shimkus 1986). The stratigraphic distribution of V is clearly expressed in the V/Rb profiles for all the wells (Figs 34–39). Generally for the wells the curve shows higher values suggesting the shales were deposited under prevalently poorly oxygenated to euxinic conditions (Bel- lanca et al. 1999). Cr/Rb, Zr/Rb and Ba/Rb depth profiles display ratio values higher, on average for Neogene shales, which could be explained by enhanced terrigenous input during their deposition. Ba/Rb higher values at different depth could also reflect diagenetic mobiliza- tion of barite from sulphate-poor, strongly anoxic sediments to sulphate-bearing, dysoxic environments (Bellanca et al. 1999). Condie & Wronkiewiez (1990) used the Cr/Th ratio as a provenance indicator. The Cr/ Th ratio increases notably in the samples investigated. Many studies have noted anoma- lous concentrations of Cr and Ni in shale and have inferred the presence of ultramaffic rocks in the source region. Much of this work has focused on Archeon rocks (Danchin 1967, McLennan et al. 1983, Taylor et al. 1986, Wronkiewicz & Condie 1987). 91

Fig 34. Atgram Well – IX geochemical ratio graph. Figure 9 shows the actual depth of the samples. 92

Fig 35. Fenchuganj Well – 2 geochemical ratio graph. Figure 10 shows the actual depth of the samples. 93

Fig 36. Habiganj Well – 12 geochemical ratio graph. Figure 11 shows the actual depth of the samples. 94

Fig 37. Kailastila Well – 1 geochemical ratio graph. Figure 12 shows the actual depth of the samples. 95

Fig 38. Patharia Well – 5 geochemical ratio graph. Figure 13 shows the actual depth of the samples. 96

Fig 39. Rashipur Well – 1 geochemical ratio graph. Figure 14 shows the actual depth of the samples.

Most of these studies indicate that the high correlation coefficient between Cr and Ni is a result of their presence in clay minerals and, ultimately, their derivation from ultramaf- fic rocks. Garver & Royce (1993) suggest that where Cr and Ni concentrations are ano- malously high, a Cr/Ni ratio of about 1.2 to 1.6 should be expected if the elements were derived from a source with ultramafic rocks, higher ratios are probably indicative of deri- vation of these elements from mafic volcanic rocks. Therefore, anomalous concentrations of Cr and Ni can be used to determine if ultramafic rocks were in the source region, and then inferences as to the tectonic implications of this information can be explored (Garver & Scott 1995). Cr and Ni values are generally high for the samples investigated (Cr ~ 14- 20, Ni ~ 17-97 ppm). The average ratio of Cr/Ni is 2.2 with variation among the values between the wells. The higher concentration indicates that the source region was compo- sed of ultramafic rocks. Cr, V and Sc are all positively correlated with Al2O3 as shown in figure 30, suggesting that they may be bound in clays and concentrated during weathering (Fedo et al. 1996). Vanadium is thought to be enriched in organic rich, reducing environments while the Cr content often is relatively constant in the clastic fraction. Cr/V ratio (ppm Cr/ppmV) 97 may therefore be used as a redox index (Ernst 1970). Ni may be enriched in reducing environment. The Cr/V ratio was computed for all the wells studied (Table 9). Fig. 40 shows the sequence of Cr/V and Ni for the wells of Rashidpur – 1, Fenchuganj – 2 and Patharia – 5. Both the sequences are more or less similar indicating that they were deposited in the same reducing environment. High Cr/V ratios with Ni indicate that the depositional envi- ronment was well ventilated (Dypvik 1979), oxidizing condition. The Cr/V ratio also dec- reases through the sequence suggesting increasingly reducing syn-depositional condi- tions. Ni contents also indicate increasingly reducing conditions, which probably have a post-depositional origin (Dypvik 1979). A higher Cr/V ratio probably reflecting a source rock richer in Cr. The analysis also shows that Cr increases with the increase of vanadium. Fig.41. shows the cross-plots of Cr and V for 3 wells of SB. They are positively correlated. The analyses also indicate a higher K2O/Na2O ratio and lower Cr/V ratio. Differences in Cr/V ratios in the wells are the indicators of differences in the nature/degree of weathering. A high order positive correlation between V and Sc, low concentration of Sc and wide range of Cr/V ratio (0.8–14.00) indicate that mafic-ultramafic components were a sub- stantiate portion of the provenance, but their unstable minerals have been removed. The concentration of Cr and Ni vary between 19–202 ppm and 17–109 ppm respectively. The positive covariance between Zr–Cr, V–Ni and their concentration demonstrate that at the time of deposition the source area was subject to intense chemical and physical disintegration. According to Wronkiewicz and Condie (1989), chemical weathering of the mafic ultramafic source rocks would tend to selectively enrich weathering products in Cr and Ni. 98

Cr/V Ni ppm Sequence number (Depth) Sequence number Sequence number (Depth)

Cr/V Ni ppm SequenceSequence number number (Depth) (Depth) Sequence number (Depth) (Depth) SequenceSequence number number

Cr/V Ni ppm Sequence number (Depth) Sequence number Sequence number (Depth)

Fig 40. Sequence showing the geochemical ratio Cr/V and Ni for wells Rashipur – 1 (A-1 and A-2), Fenchuganj – 2 (B-1 and B-2) and Patharia – 5 (C-1 and C-2) indicating that they were deposited in the same environment. Fig. 14, 10 and 13 shows the actual depth of the samples of the wells mentioned. 99

Fig 41. Crossplot of Cr-V for (a) Patharia well – 5 (b) Rashidpur well – 1 and (c) Fenchuganj well – 2. All are in positive correlation.

Sr contents of NS vary from 170–178 ppm. The value reflects the "average" intensity of chemical weathering of the shale sources. Studies of modern weathering show that Ca, 100

Na and Sr are rapidly lost during chemical weathering and that the amount of these ele- ments lost in proportional to the degree of weathering (Wronkiewicz & Condie 1987, 1989, Condie 1991). The present study shows that NS typically have Ba/Sr and Rb/Sr ratios considerably higher which may also result from Sr loss during weathering. Intense tectonic activity and burial diagenesis reported in the literature from the study area sug- gest that the average intensity of chemical weathering may have been greater than after- wards. If Pre-Neogene weathering was more intense than in later times, a greater propor- tion of Ca and Sr should have ended up in seawater. Because of their short residence times in seawater, Ca and Sr should have been recycled in the Neogene Crust in shallow marine carbonates. Among Large-ion lithophile elements (LILE, Rb, Ba, Th, Sr, Cs, U and Pb), Ba and Rb are enriched throughout the sequence. U, Cs and Pb are strongly depleted whereas Sr exhibits gradual depletions for some wells and slightly enriched for other wells. Among High Field Strength Elements (HFSE, Zr, Nb, Hf, Ta, and V)) only Zr enriched throughout the sequences. Nb, Hf and Ta however, exhibit gradual depletion.

7.2.1 Barium enrichment

Ba values generally vary between 11 and 300 ppm (Bellanca et al. 1999). For the present study, significantly higher concentrations (up to 6 808 ppm) occur in the middle part of the section of Patharia well-5 which is interesting and deserves to be explored well. A detail study on Ba was undertaken by using XRD, STEM and SEM for some selected samples of Patharia well-5. The depth and the Ba concentrations of this well are given in Table 10. Barite deposits occur in a wide range of deep-sea locations (Torres et al. 1996). Their distribution, composition and correlation with sediment type have been discussed by a number of authors. A variety of mechanisms, including hydrothermal, biogenic and diagenetic processes, result in the accumulation of barium sulfate in the marine sedimen- tary environment. Barite can be formed by direct precipitation when a barium-enriched hydrothermal fluid reacts with sea water sulfate (Torres et al. 1996). These deposits are restricted to the vicinity of hydrothermal activity, as observed, for example, along the East Pacific Rise (Church 1979), the Gorda Ridge, north -eastern Pacific (Koski et al. 1988) and the Guaymas Basin, Gulf of California (Koski et al. 1988). High concentrations of micro-crystalline barite (up to 30 x 50 µm in size) in sedi- ments from the Eastern Equatorial Pacific, the Indian Ocean (Goldberg & Arrhenius 1958) and the Antarctic convergence Zone (Brahms et al. 1992) are thought to result from the precipitation of barium sulfate within microenvironments of decaying biological debris in the water column (Dehairs et al. 1980, 1990, Collier & Edmond 1984, Bishop 1988). Some earlier workers like Price and Calvert (1978) and Prevot & Lucas (1980) has given a good account of Ba enrichment. According to them Ba transported to the sea becomes largely separated already during the formation of hydrolyzate sediments. With reference to its adsorption properties, Ba behaves like potassium, which forms a univalent ion, while barium forms a bivalent ion. The ionic potential of K+ and Ba2+ is smaller and 101 the quantity adsorbed by clays great. Barium is adsorbed so strongly that it has largely been removed in the near-shore sediments. Therefore, barium is adsorbed in the hydroly- zates, and the argillaceous sediments are the richest in barium. In some cases marine deposits contain notable amounts of barium as barite concretions and nodules, which may carry as much as 82 % BaSO4 and are probably formed by chemical precipitations. Price and Calvert (1978) as well as Prevot and Lucas (1980) stated that Ba is someti- mes related to clay minerals or to iron oxides. Some recent workers stated that Ba enrichment in sedimentary deposits can be consi- dered as an indicator of a high flux of biogenic material to the sediments and therefore of high surface-water productivity (Schmitz 1987, Dymond et al. 1992, Van Os et al. 1994). Several diagenetic models have been proposed for the origin of barites. For example, Goldberg and coworkers (1969) suggested that barite nodules from the coast of California originated in a coastal lagoon or a shallow hydrothermal environment. In contrast, Dean & Schreiber (1978) concluded that for the barite at DSDP sites 369 and 370, deposits for- med diagenetically in sediments exposed at the sediment-water interface during long hia- tuses. SEM studies on some selected samples (with high Ba concentration) revealed that the Ba in Patharia well-5 is associated with SiO2 and clay minerals (Figs 42–43) Energy-dis- persive X-ray analysis, in conjunction with the SEM, was used to confirm barium and sulphur as the main constituents of these crystals (Figs 44–45). TEM study was underta- ken to detect barite crystals (Figs 56–58). TEM photographs showed the presence of barium crystals nicely. Under the SEM, a sample of barite occurrence revealed large crys- tals (10–38 µm). Large crystals are rounded to subrounded with broken surfaces, sho- wing a very fragile nature. Smaller barite crystals show euhedral shapes. A SEM study reveals also the presence of small barite crystals 2–8 µm in length in association with silica and clay minerals. Dehairs and coworkers (1980), Nuel and Shelton (1986), Breheret and Delemette (1989) and Mills (1971) found a similar type of Ba. In their study, they find that the Ba in suspended particles is dominantly in the form of barite and so conclude that it formed in the upper water column by the breakdown of organic matter, release of Ba, and formation of barite in a microenvironment. These beds from the present study area deposited in a shallow marine environment to be enriched by adsorbed Ba. During diagenesis oxidation conditions prevailed liberating sulfate ions. Meanwhile, due to compaction and lithification, Ba left clay minerals and combined with the liberated sulfate ions forming barite grains, existed in certain strati- graphic horizons of shales and shaly beds. In these beds, at depth of 1 451.5 m Ba is detected up to 6 808 ppm (Table 10). The development of barite fronts requires a labile Barium source which is not likely to be clastic detritus but rather a large "bio-barite" flux observed in areas of high biogenic opal productivity (Dehairs et al. 1980, 1990, Collier & Edmond 1984, Bishop 1988, Dymond et al. 1992). The deposition of "bio-barite" microc- rystals on the sea floor provides a source of labile barium, which can be subsequently remobilised diagenetically within the sediment column, in the zone of sulphate depletion (Torres et al. 1996). In the light of the discussions and observations on Barium it can be concluded that its occurence is controlled by barite and a diagenetic mechanism. The remobilisation of biogenic barium in sulphate depleted zones, and subsequent precipitation, results in the 102 accumulation of authigenic barite in several continental margin settings. Authigenic bari- tes are likely to occur in areas where intensive high productivity results in a large flux of biogenic barium to the ocean floor (Von Breymann et al. 1993). Ba enrichment also shows a high surface-water productivity. Ba/Rb values locally increasing (0.48–55.80 in Patharia well – 5) in NS could also reflect diagenetic mobilization of barite. In addition, Ba can be used to determine the provenance of various sediments. Cullers et al. (1988) suggested that Co and Ba might be also suitable for distinguishing silicic and basic sources of sands. The best provenance discrimination was obtained if the Ba/Sc and Ba/Co ratios were used. In the present study, the high Ba/Co and Ba/Sc ratios of the samples point to granitic rocks as possible source rocks of the SG sediments. Ba/Rb (0.48–55.80) values locally increasing from NS could also reflect diagenetic mobilization of barite from sulfate - poor, strongly anoxic sediments to sulfate bearing, dysoxic environments (Bellance et al. 1999). Finally, it was also considered whether or not the barium values are due to contamina- tion during drilling operations. The barium data are not due to contamination because of the followings. If contamination were occurring one would expect that the coarser (in comparison to clay fraction) sandy layers would be more contaminated. This is not in the case of the present data. The higher barium values observed are obtained for clay-rich shale samples. The sample no 180 of Patharia well-5 having high Ba values (2688 ppm), which is the only sample obtained from the shale with thin layer of sand. But with the similar lithology the nearest samples (179 & 181) show low barium concentrations. The sample nos. 149-160, having lithology of shale with sand, but the barium values are lower (appendix-2). Such characteristics, not possible if data contamination by drilling fluid was effective. Thus the barium data presented in this study can be useful in studies of provenance and pore-water chemistry. The high enrichment of Ba has also been encountered in other wells of Bangladesh as follows: 1. Well – Bakhrabad –1 (South of the study area) Ba – 2,638 ppm (Depth: 973.5 m) Ba – 7,881 ppm (Depth: 978 m) 2. Well Jaldi –1 (Coastal area) Ba – 1938 ppm (Depth:1645 m) 3. Well Cox’s Bazar –1 (Coastal area) Ba – 13,478 ppm (Depth: 2905m) 103

Fig 42. SEM photograph showing the colour bands of minerals present in the sample number 118 of Patharia well – 5. Band – 1 (red) for BaSO4, Band – 2 (green) for clay minerals and band – 3 (blue) for SiO2. Black band were not classified. Semi quantitative estimation of red colour µ band is given which proves that the mineral is Barite, BaSO4. Scale bar 500 m. 104

Fig 43. Backscattered electron image and colour band SEM photograph of sample number 118 of Patharia well – 5. Band – 1 (red) for BaSO4, Band – 2 (green) for clay minerals and Band – 3 (blue) for SiO2. Black band were not classified. Semi quantitative estimation of red colour µ band is given which proves that the mineral is Barite BaSO4. Scale bar 200 m. 105

Fig 44. Backscattered electron image of sample number 180 of Patharia well – 5 with the graph (down) showing the elemental composition of a Barite mineral. 106

Fig 45. Backscattered electron image of sample number 180 of Patharia well – 5 with the graph (down) showing the elemental composition of a Barite grain. 107

A

B Fig 46. A) SEM photograph showing a large Barite grain (White, X4500). B) SEM photograph showing higher concentration of Barium in the sample 118 of Patharia well – 5 (X1600). 108

Table 10. High Concentrations of Barium in Patharia well – 5.

Sample No Depth (mbsf) Concentration (ppm) 118 1 451.5 m 6 808 120 1 452.5 m 1 420 121 1 453.0 m 1 521 126 1 454.0 m 1 398 172 3 161.0 m 2 091 180 3 165.0 m 2 688

7.2.2 Total Rare Earth Elements (∑REE)

REE, lanthanum-lutetium are commonly-used indicators of igneous processes. The REE have a similar charge (3+), but a slight decrease in ionic radii from the light REE (LREE) to the heavy REE (HREE), known as the lanthanide contraction (Garver & Scott 1995). REE distributions in sedimentary rocks have played a central role (McLennan 1989). Sedimentary REE patterns may provide an index for the average provenance composi- tions. REE are particularly useful for studying provenance because of their low solubility during weathering and diagenetic processes (Bhatia & Taylor 1981). Table 11 shows the total of REE, HFSE and LILE elements for the Surma Basin. A plot of total REE content (∑REE) variation in relation to burial depth for all wells has been presented in Fig. 47. In general, the plot shows the variation in ∑REE content for the whole sequence of the wells. The average total content of REE is between 150 to 230 ppm. The ∑REE generally show systematic enrichment and subsequent depletion throug- hout the sequence. A comparison between the sequence of ∑REE and the maturity para- meters and also the grainsize parameter (SiO2/Al2O3) shows that ∑REE sequence has got a good relationship with these sequences as shown in figures 23–28 and figure 48. Thus, it can conclude that ∑REE pattern is compatible with the maturity and mineralogy of ter- rigenous detritus. 109

Fig 47. Showing the ΣREE content variation in relation to burial depth for all wells. (1) Habiganj well – 1, (2) Kailastila – 1, (3) Patharia – 5, (4) Fenchuganj well –2, (5) Rashidpur –1 and (6) Atgram – IX. Figures 9 – 14 shows the actual depth of the samples. See appendix. 1 and 2 for details of the samples.

A plot of ∑REE parameters against the parameters (K2O/Na2O ratio, SiO2/Al2O3 and Al2O3) shows an increase in ∑REE with an increase in the ratios mentioned. Thus the dominant source rocks from dacites to granite-gneisses and sedimentary rocks is ref- lected in the ∑REE characteristics of SG sediments (Fig. 48). Similar results were also observed by Bhatia (1985). Neogene shale (NS) have a significantly higher K2O and Al2O3 content due to the enrichment of clay minerals and thus have a higher K2O/Na2O ratio. ∑REE increases with an increase in K2O/Na2O and probably a decrease in SiO2/ Al2O3, as the dominant source rock changes from dacites to granite-gneisses and sedi- mentary rocks. REE abundance may also reflect its concentration in the clay-size fraction (clay minerals) with reference to mineralogy of terrigenous detritus (See also Bhatia 1985, Cullers et al. 1979). Clay minerals are a major carrier of the REE in sediments. Chaudhury and Cullers (1979) have suggested that the REE content in sediments may be diluted by quartz and thus it may be inversely related to the quartz content. In this study, the relationship in the hypothesis by Chaudhury and Cullers (1979) can be graphically demonstrated as shown in figuress 23–28 and 48. The significant variation in The ∑REE sequences pattern noted in the present work suggests that the variation in Tertiery (Miocene) sedimentary rock is possible and is cont- rolled by their source rocks and tectonic settings. 110 REE Σ

K2O/Na2O REE Σ

SiO2/Al2O3 REE Σ

Al2/O3 (wt %) Σ Fig 48. Plots of K2O/Na2O, SiO2/Al2O3 and Al2O3 versus REE for Patharia well-5 shales. Note the positive correletion indicating increasing maturity (arrow in Fig. a) due to changes in granite-gneiss and sedimentary source rocks and presence of clay minerals in ΣREE (Fig. c). Σ Σ REE increases with the decrease in SiO2/Al2O3 (arrow in b) indicate that REE content is inversely related to the quartz content. 111

Table 11. Total of ΣREE, HFSE and LILE. Samples 1–19 (Habiganj well – 1), samples 20– 29 (KailasTila well – 1), samples 30–69 (Rashidpur well – 1), samples 71–85 (Atgram well – IX), samples 86–114 (Fenchuganj well – 2), samples 115–152 and 154–188 (Patharia well – 5).

Sample ∑REE ∑ HFSE ∑LILE No (Total in ppm) (Total in ppm) (Total in ppm) 1 219,00 290,00 925,00 2 217,00 294,00 916,00 3 217,00 304,00 913,00 4 215,00 293,00 897,00 5 247,00 301,00 936,00 6 232,00 290,00 947,00 7 194,00 290,00 94,00 8 226,00 302,00 955,00 9 255,00 301,00 1189,00 10 256,00 294,00 1013,00 11 186,00 299,00 846,00 12 206,00 308,00 954,00 13 223,00 373,00 863,00 14 238,00 299,00 999,00 15 245,00 304,00 1009,00 16 262,00 285,00 1014,00 17 212,00 377,00 808,00 18 230,00 399,00 863,00 19 247,00 400,00 836,00 20 225,00 328,00 1052,00 22 203,00 338,00 800,00 23 215,00 294,00 900,00 24 276,00 339,00 1038,00 25 231,00 284,00 915,00 26 186,00 420,00 783,00 27 175,00 362,00 758,00 28 243,00 330,00 932,00 29 217,00 349,00 834,00 30 235,00 335,00 971,00 31 240,00 385,00 886,00 32 257,00 389,00 939,00 33 241,00 402,00 847,00 34 217,00 374,00 903,00 35 176,00 379,00 875,00 36 318,00 398,00 1017,00 37 217,00 353,00 866,00 38 233,00 346,00 840,00 39 239,00 386,00 875,00 40 252,00 215,00 873,00 112

Table 11 continued

Sample ∑REE ∑ HFSE ∑LILE No (Total in ppm) (Total in ppm) (Total in ppm) 41 235,00 343,00 906,00 42 192,00 394,00 851,00 43 220,00 340,00 1298,00 44 201,00 312,00 891,00 45 244,00 358,00 887,00 46 191,00 310,00 909,00 47 196,00 311,00 910,00 48 220,00 318,00 896,00 49 201,00 326,00 938,00 50 204,00 314,00 919,00 51 191,00 325,00 901,00 52 217,00 345,00 881,00 53 218,00 308,00 951,00 54 210,00 309,00 940,00 55 207,00 337,00 887,00 56 216,00 285,00 982,00 57 212,00 309,00 933,00 58 223,00 337,00 963,00 59 198,00 309,00 924,00 60 240,00 293,00 974,00 61 221,00 298,00 979,00 62 207,00 339,00 957,00 63 227,00 344,00 925,00 64 215,00 396,00 841,00 65 187,00 381,00 891,00 66 227,00 334,00 893,00 67 220,00 356,00 862,00 68 211,00 324,00 939,00 69 232,00 324,00 1015,00 71 186,00 295,00 891,00 72 215,00 296,00 898,00 73 194,00 303,00 866,00 74 237,00 301,00 991,00 75 232,00 283,00 932,00 76 212,00 292,00 894,00 77 214,00 307,00 921,00 78 149,00 376,00 592,00 79 204,00 377,00 983,00 80 257,00 434,00 869,00 85 54,00 152,00 452,00 86 184,00 332,00 710,00 88 194,00 373,00 765,00 113

Table 11 continued

Sample ∑REE ∑ HFSE ∑LILE No (Total in ppm) (Total in ppm) (Total in ppm)

90 250,00 317,00 87,00 91 210,00 315,00 1096,00 92 211,00 340,00 1035,00 95 267,00 354,00 1109,00 96 266,00 359,00 1021,00 97 215,00 380,00 925,00 99 238,00 332,00 968,00 100 244,00 343,00 1053,00 103 219,00 306,00 843,00 104 238,00 321,00 991,00 105 243,00 333,00 1046,00 108 240,00 360,00 986,00 109 203,00 289,00 855,00 110 186,00 305,00 786,00 111 207,00 320,00 795,00 112 224,00 325,00 975,00 113 221,00 331,00 828,00 114 213,00 280,00 886,00 115 246,00 307,00 921,00 116 250,00 310,00 914,00 117 221,00 316,00 1235,00 118 73,00 306,00 7205,00 119 208,00 344,00 1007,00 120 223,00 334,00 1828,00 121 292,00 360,00 1935,00 122 202,00 274,00 1046,00 124 215,00 370,00 908,00 125 241,00 337,00 1228,00 126 198,00 306,00 1834,00 127 161,00 279,00 789,00 128 216,00 333,00 903,00 129 235,00 290,00 1108,00 130 135,00 284,00 1164,00 131 137,00 265,00 1236,00 132 172,00 311,00 798,00 133 232,00 318,00 867,00 134 190,00 303,00 786,00 135 236,00 322,00 872,00 136 251,00 329,00 894,00 137 223,00 322,00 878,00 138 219,00 316,00 887,00 139 218,00 317,00 881,00 114

Table 11 continued Sample ∑REE ∑ HFSE ∑LILE No (Total in ppm) (Total in ppm) (Total in ppm) 140 232,00 318,00 983,00 141 230,00 312,00 910,00 142 241,00 287,00 903,00 143 216,00 287,00 896,00 144 237,00 285,00 903,00 145 227,00 211,00 929,00 146 249,00 311,00 922,00 147 255,00 184,00 1107,00 148 246,00 315,00 1020,00 149 225,00 257,00 933,00 150 229,00 322,00 981,00 151 246,00 215,00 971,00 152 218,00 210,00 1129,00 154 196,00 153,00 754,00 155 140,00 269,00 956,00 156 234,00 325,00 1070,00 157 160,00 318,00 889,00 158 165,00 269,00 720,00 159 161,00 275,00 196,00 160 183,00 251,00 516,00 161 254,00 609,00 999,00 162 230,00 355,00 847,00 163 220,00 291,00 938,00 164 225,00 303,00 991,00 165 237,00 348,00 925,00 166 231,00 305,00 1044,00 167 244,00 321,00 1019,00 168 204,00 307,00 881,00 169 221,00 315,00 934,00 170 227,00 323,00 870,00 171 272,00 325,00 1084,00 172 196,00 361,00 2546,00 173 183,00 339,00 1018,00 174 221,00 424,00 442,00 175 168,00 301,00 897,00 177 194,00 336,00 1076,00 178 2331,00 347,00 3343,00 180 173,00 212,00 3165,00 181 214,00 264,00 1001,00 183 220,00 314,00 1422,00 184 227,00 323,00 1151,00 185 194,00 338,00 1409,00 186 209,00 350,00 145,00 187 266,00 1328,00 1134,00 188 209,00 1350,00 1147,00 8 Mineralogical Results

8.1 XRD

X-ray Diffraction Analyses are based on a selected 15 representative core samples from three different wells: Atgram well-IX, Fenchuganj well-2, and Patharia well-5. The analyses aimed at documenting the gross mineralogy, clay mineralogy and depth dependent clay diagenesis of shales of SG sediments of Surma Basin. It was also aimed at discussing the implication of clay mineral diagenesis on major geologic processes like overpressure generation and structural developments, with a guideline for defining the optimum exploration strategy using clay technology as a powerful tool. The study also concentrates on the evolution of climate variabilities during the Neogene by using the clay mineralogy analysis of Neogene shale (NS) samples of SB. A clay fraction (< 2 µm) was separated out from the shale by disaggregating and despersing the sample in distilled water and immediately washed by centifugation. The fraction of <2 µm was isolated by centrifugation and suspension were dried on glass slides. The clay samples in oriented mounts were run under three separate conditions: i) air dry state. ii) after ethylene glycol treatment and iii) after heating to 550º C for 1 hour. The digital data were interpreted using Diffrac plus software of the Bruker Analytical X-ray system, which comprises a search-match routine based on a Powder Diffraction File. Minerals identified in the studied NS samples include quartz, kaolinite, illite, chlorite, illite/smectite, kaolinite/smectite mixed layers. However, minor amount of feldspar is still present in many of the samples, and trace amounts of calcite and dolomite are also present in many samples. X-ray diffractograms of separated clay fraction (< 2 µm) of some selected shale samples are shown in Fig. 50–54. A semi quantitative XRD analysis was done using a Diffrac plus computer program and the percentages of each of the minerals of NS were calculated and are given in Table 13. The program allows one to calculate the major diffraction peak heights. First, it measures the left and right angles (2-theta) of the peaks. The measuring of net height, raw 116 area and finally net area is followed. The net area of peaks are converted to the percentages. As an example in the sample number 124 are four peaks of kaolinite- smectite, illite-smectite, Quartz and Feldspar. The peak areas calculated for these peaks were 199, 148, 30 and 15 respectively. The total net area was 392, and thus individual mineral percentages were calculated as 51%, 37%, 8% and 4% respectively which is shown in the following table.

Table 12. Semi – quantitative XRD analysis of sample no. 124.

Sample No. Left Angle Right Angle Raw Area Net Area Net height Cps % 2-theta 2-theta CpsX2-th CpsX2-th 124 5,22 6,18 554 847 199 51% K/S 10,8 10,58 109 569 15 4% F 11,4 12,68 540 1038 148 37% I/S 20,6 21 124 471 30 8% Q

8.1.1 Non Clay Minerals

Quartz: Quartz forms one of the most abundant minerals in most of the samples. Quartz is identified by its distinctive reflections at 4.26 Å and 3.35 Å. The 3.35 Å peak of quartz was more intense than the other peaks. There was a coinciding in some samples, with a strong reflection of illite at 3.33 Å which makes this 3.35 Åpeak difficult to use, due to as quartz is abundance. The variation in the samples of Patharia well-5 was high. Fenchuganj well-2 and Atgram well-IX well samples do not show major variation. Feldspar: Feldspar is the next important non-clay mineral present in most of the samples but in minor amount. It is identified by distinct reflection in the spacing range of 3.8 Å to 3.2 Å No meaningful variation in the abundance of feldspar is evident from the XRD reflections of NS. Calcite: Calcite is identified by only a weak reflection at 3.01 Å showing its presence in trace amounts. Dolomite: Dolomite is identified by only a weak reflection at 2.8 Å, indicating a trace amount of the mineral. 117

Table 13. Relative clay & non-clay mineral abundance in clay fraction samples of Surma Basin, Bangladesh.

Sample No. Illite-Smectite Kaolinite Depth (m) Illite (%) Kaolinite-Smec- Chlorite (%) (%) (%) tite (%) * 77 3639 9 33 31 * 84 4733 64 13 * 84 (H) 4733 10 55 26 ** 91 3137 –3143 21 39 26 ** 91 (H) 3137 –3143 29 19 38 1 **100 3730 –3379 31 38 7 ***117 1450.5 21 38 5 118 (H) 1451.00 4 40 42 121 1452.00 14 57 22 121 (H) 1452.00 1 29 27 124 1454.5 37 51 124 (H) 1454.5 8 37 29 124 (G) 4 23 59 132 1829.5 28 70 1 132 (H) 1829.5 4 41 27 147 2290.5 29 71 147 (H) 2290.5 6 40 18 155 2294.5 14 18 68 168 2832.7 8 26 66 168 (G) 2832.7 13 33 54 172 3161.25 26 74 172 (H) 3161.25 10 48 42 180 3164.7 34 66 180 (H) 13 56 31 180 (G) 9 39 52 183 3166.2 6 37 32 8 183 (H) 6 46 19 *Atgram well – IX. ** Fenchuganj – 2 well. *** Patharia – 5 well (117–183). (H) = Heated, (G) = Glycolated

8.1.2 Clay minerals

Illite: Illite is the major clay mineral present in all the samples and is identified by a series of basal reflections at 10.1 Å, 4.98–5.01 Å 3.33 Å, and 2.89–2.92 Å On glycolation, illite is essentially nonexpanding. On heating to 550o C the (001) peak of illite may show a slight collapse. Values of less than 10 Å may be due to a K+ deficiency or the substitution of Fe2+ or Mg2+ for [Al3+]IV (Güven et al. 1980). Kaolinite: Kaolinite is another major component in all the samples. It is represented by a basal (001) reflection at 7.06-7.14 Å and (002) reflection at 3.53 Å, the collapse of Kaolinite structure to an amorphous material takes place on heating to 550° C and this 118 confirms the identification of the mineral. Kaolinite reflections do not show any systemic variation for the samples studied. Chlorite: Chlorite is represented by its basal reflections at 14.25 Å, 7 Å, 4.7 Å and 3.5 Å respectively. The basal reflection at 14.25 Å could not be used directly for the identification of chlorite because of an interfluence with an Illite-Smectite mixed layer, and 7.14 Å also could not be used for chlorite identification because of the interference and coincidence of kaolinite reflections. Illite-Smectite (I/S) mixed layer clay. None of the samples show discrete or pure smectite, but many have an illite/smectite layer phase. The amount of interlayering of illite with smectite in the mixed layer I/S has been found to vary depending upon the position of the sample in the stratigraphic sequence. The expandibility or the percentage of smectite could not be calculated due to the absence of 17 Å reflections. The apparent absence of 17 Å peak intensity in the diffraction profile of the clay fraction of the Neogene shale is possibly due to the transformation of illite/Smectite to illite during burial diagenesis. Imam (1993) studying the Neogene sediments of the Bengal Basin, Bangladesh, noted the disappearence of 17 Å peak intensity in the stratigraphically deepest samples. He pointed out that the absence of a 17 Å peak is diagenetic and caused by the illite/smectite becoming orderly interlayered with more than 60% illite layer. According to Srodon (1980). “If a reflection occurrs between 5.3° and 8.7° 2θ in the diffraction pattern of an ethylene glycol-solvated illite/smectite, the interstratification is ordered to some degree”. It can be noted that a reflection occurs between 5.3° and 8.7° 2θ in the studied samples of Neogene shale, and therefore the samples are ordered to some extent, according to Srodon. The transformation of smectite to illite through an intermediate mixed-layer illite/ smectite (I/S) clay is a widely recognized clay diagenesis reaction in shales with progressive burial (Weaver 1956, Dunoyer de Segonzac 1970, Perry & Hower 1970, Weaver & Beck 1971a,b, Hower et al. 1976, Boles & Franks 1979), and more recent works (Srodon 1999, Srodon et al. 1992, Sato et al. 1996) have given a good account of this. Mixed layer illite/smectite (I/S) is dominant in the clay-size fraction of many shales from Tertiary basins. The reaction of smectite to illite in these clays has received considerable attention because of its potential for: 1) flushing hydrocarbons from the shales (Burst 1969, Bruce 1984), 2) catalyzing hydrocarbon generation (John & Shimoyama 1972), 3) producing high pore - fluid pressures (Powers 1967) and 4) providing cementation agents to sandstones (Towe 1962, Boles & Franks 1979, Lahann 1980). Present study on Neogene shale of SB, Sylhet Bangladesh shows similar results from I/S interlayers of the Gulf coast. Illite/smectite provides a useful tool for explaining diagenesis and for reconstructing maximum burial conditions. Hower (1981) stated that the usual spacing for samples from shales and sandstones under air-dried conditions is close to 15 Å. In the present study randomly interstratified Illite/Smectite were identified by the reflection at the 14 Åpeak with air-dried, untreated samples as well as in heated (550°C) and glycolated samples. Fig. 50 shows the randomly interstratified I/S layer in air-dried samples. The same reflections at the 14 Åpeak were also identified in the samples heated to 550°C (Fig. 51) and glycolated samples (Fig. 53). 119

After Weaver's study of mixed-layer clays in sedimentary rocks (Weaver 1956), it became evident that the illitization of smectite progressing with depth in sedimentary basins is a universal phenomenon (Srodon 1999). The process was related to petroleum occurrences (Burst 1969) that generated the interest of the oil industry. The most distinctive feature of clay diagenesis in the NS is shown by the systematic change in illite/smectite mixed layer clay minerals with increasing stratigraphic and burial depths. Randomly interstratified illite/smectite mixed layer clay shows a progressive loss of smectite content via transition to the illite layer with increasing depth: This is referred to as "illitization" (Imam 1994). The problem of the smectite illitization mechanism has been vigorously debated from several standpoints over the past 30 years. Because of the abundance of this mineral, the illitization mechanism is helpful for understanding the evolution of pore water chemistry and sandstone cementation during diagenesis (Boles & Franks 1979). The diagenetic illitization of illite/smectite in shales has also been observed in other wells studied in the Bengal Basin (Imam 1983, 1987, 1993, Imam & Shaw 1985) and in many other basins of the world i.e. the Gulf Coast basin, USA (Perry & Hower 1970, Hower et al. 1976 and Berger et al. 1999), North Sea basin, U.K. (Pearson & Small 1988), Colorado basin, USA etc.

8.1.2.1 Diagenetic model of Surma Basin

Mixed layers are created by the process of weathering. The formation of mixed layers I/S and K/S and their evolution towards illite or chloride by the fixation of potassium, sodium or magnesium have taken place in the Neogene shale of SG sediments from the Surma Basin. Burial diagenesis occurs then on a population of mixed layer minerals where all proportions of illite/smectite and kaolinite/smectite are possible. The present study reveals that the transformation of smectite to illite took place through an intermediate mixed layer illite/smectite. It also shows the transformation of smectite to illite through mixed layer kaolinite/smectite. This is one path way with the adsorption of potassium and sodium to produce these illites. Another path way is the magnesium path way which produces chlorites due to adsorption of Mg2+. The diagenetic transition of smectite to illite is accompanied by the expulsion of interlayer water from smectite to the pore water system, which is referred to smectite dehydration (Powers 1967, Burst 1969, Perry and Hower 1970, Imam 1994). Mixed layers are intermediate stages which occur during aggradation by deep diagenesis. This aggradation is the result of an incorporation of certain cations taken up from interstitial solutions and of a rearrangement within the lattice. Clay minerals subject to deep burial diagenesis include I/S mixed layers due to the equilibrium between the minerals and interstitial solution under the physical and chemical conditions of deep diagenesis. The aggradation of degraded 2:1 clay minerals consists essentially of a loss of water, an adsorption of Na+, K+ and Mg2+ and a rearrangement of ions within the lattice. The ions migrate from the interstitial solution towards the interlayers, from the interlayers 120 towards the octahedral layers (Mg, Fe, Al) and finally to the tetrahedral layers according to the scheme presented by Millot and coworkers (1966). The transformation of clay minerals are thus an aggradation leading to illite and chlorite lattices. Kaolinite is unstable in this confined environment and the ions if releases provide ions for the aggradation of illite and chlorite. These transformations during deep diagenesis are irreversible at the depths at which they normally occur. The diagenetic evolution of the Surma basin has been presented as a proposed model in Fig. 49.

Fig 49. Diagenetic model of Surma Basin.

8.1.2.2 Implication of Smectite diagenesis and dehydration.

In Patharia well-5 subsurface overpressure has been encountered in the SG (Bhuban Formation) sediments with the top of overpressure at a depth of about 480 m. Considering the huge thickness of shale in early Neogene SG sequence, the smectite to illite diagenetic transition should have made a significant amount of water available in the subsurface for migration according to the clay dehydration model of Imam (1994). 121

According to Imam, the diagenetic transition of smectite to illite is accompanied by the expulsion of interlayer water from smectite to the pore water system, which is referred to as smectite dehydration. Powers (1967), Burst (1969) and Perry and Hower (1972) propose that clay dehydration models be related to the various stages of smectite to illite transition, in which the smectite diagenetic derives water available for migration in the subsurface. Such water may act as an agent in helping petroleum migration, overpressure generation and structural shaping (Potter et al. 1980). It is suggested by Imam (1994) that smectite diagenesis and dehydration have contributed to the generation of overpressure in the Bhuban Formation in Patharia well-5. Powers (1967) first advocated the idea that the smectite to illite transition may be related to abnormal fluid pressure generation at depth. Other models have been suggested for overpressure generation, i.e. compaction disequillebrium (Chapman 1980) and aquathermal pressuring (Barker 1972), but the smectite to illite diagenesis and consequent dehydration has been considered as one of the most important (Plumely 1980, Bruce 1984).

8.1.2.3 Clay minerals of SG and its implication in petroleum geology.

To conclude the subject of SG clay minerals, it is quite expected to mention some words on its implication in petroleum geology. In this connection a review of studies on the subject has been made and presented to understand them in a better way. The clay minerals have significant controls on the porosity and permeability properties of sandstones, and this may have implications on reservoir performances during drilling, production and well stimulation operations (Imam 1989). The pore systems of sedimentary rocks may be lined or filled with a variety of different clay minerals. These clays can greatly reduce permeability, increase acid or fresh water sensitivity, totally alter the electric log response and increase irreducible water saturations. The composition of the clays is of great importance because their different compositions will cause them to react differently to various drilling and completion fluids. As a result, fluids should be designed for the specific variety of clay present in the pores (Almon & Davies 1981). Clay minerals can cause formation damage and production problems during drilling, production and well stimulation operations. Smectite is water sensitive and would swell with fresh water, resulting in a loss of permeability. Kaolinite may be dislodged, migrate and block a pore throat during production. Chlorite is acid sensitive and would react during acid treatment to produce precipitates that could damage reservoir performances. Kaolinite can also choke pores and chlorite and smectite coat grain surfaces, reducing pore throat diameter. Some illite morphology bridges the gaps between grains and severely damages permeability and so on (Imam 1989). The clay mineralogy presented in the present study for the Neogene shales of the Surma Basin may provide a guideline for defining optimum exploration strategies and efficient well management. The engineering problem in Kaolinite-rich sands can be easily resolved through the use of any of the clay stabilization systems (such as polyhydroxy-aluminium compounds or cationic polymer systems), as long as the treatment is carried out early in the history of 122 a well (Haskin 1976). The production problems caused by the smectite type of clay minerals can be overcome by the use of oil base, potassium or ammonium chloride drilling, completion and stimulation fluids. If swelling has already occurred within the reservoir, the damage may be corrected by acidizing with a peak mixture of HCl and HF, providing injectivity is not totally lost (Almon and Davies, 1981). The main engineering problem posed by illite is that it creates large volumes of microporosity. Illite sometimes grows in pores as masses of long, hair like crystals, which can considerably reduce the permeability of sediment (Guven et al. 1980). In the presence of fresh water, these illites fibres tend to clump together, further reducing permeability. If these illites are not dissolved prior to production, they may break during production and will migrate to the pore-throats and act as a check valve (Almon & Davis 1981). Illite can be dissolved by using an acid mixture consisting of HCl and HF. Chlorite which is causing reservoir damage by its acid sensitive nature can be dealt with by using appropriate chemicals (an oxygen scavenger and an iron chelating agent) and care is taken to recover all the acid introduced into the well (Smith et al. 1969).

8.1.2.4 Kaolinite - Smectite (K/S) mixed layer clay: a new mineral in Bangladesh

The occurrence of interstratified Kaolinite/Smectites (K/S) in nature was first reported by Sudo & Hayaski (1956) and were subsequently confirmed by Altschuler et al. (1963). These minerals were rediscovered in the Tertiary clays of Yucatan by Schultz et al. (1971) and in hydrothermal deposits of lower Silesia by Wiewiora (1971,1973). Since then many occurrences of K/S have been described. Studies of the nature of layer sequences of such mixed-layer minerals, however, are few: Sakharov and Drits (1973), Cradwick and Wilson (1978), Kohyama and Shimoda (1974) and Tsuzuki and Sato (1974). Natural occurrences of K/S are limited. Kaolinite-Smectite in sedimentary rocks, is most often a detrital component, as shown by Theiry (1981) in his study of Eocene clays from the Paris Basin. Most probably, the abundance of K/S is highly underestimated because it is difficult to detect, in particular as a minor component (De'Vaux et al. 1990, Hughes et al. 1993, Cuadros et al. 1994). For the present study kaolinite-smectite mixed layer clays were found in wells Patharia-5, Fenchuganj-2 and Atgram-IX at different depths. In the Patharia well, K/S mixed layered were present at depths 1 454 m, 2 290,5 m and 3 161 m respectively. In Atgram-IX well it was at 4 733,8 m and in Fenchuganj-2 well at 3 730 m depth. The K/S was identified by its clear 7.2 Å peak and 3.5 Åpeak respectively. It shows a weak reflection at 2.5 Å peak. The K/S reflections do not show quantitatively significant differences between samples. The K/S reflections are all in similar positions and relatively sharp and intense (Fig. 50 – 54). Kaolinite-smectite mixed layer clay has been carefully examined by X-ray diffraction and rather unusual properties were discovered which cannot be attributed to a normal Kaolinite. 123 S+Chl, le nos. 183, 100 and 84. I/ and 100 le nos. 183, th Illite; Q, Quartz and F, Feldspar. Feldspar. F, and Quartz Q, Illite; th on (2 microns) of the samp on (2 microns) tite; Q+I, Quartz wi iented, non-heatedclay fracti Illite-Smectite with chlorite; I, Illite; K/S, Kaolinite-Smec K/S, I, Illite; with chlorite; Illite-Smectite Fig 50. X-ray diffraction pattern for the or Fig 50. X-ray diffraction 124 91 heated 91 nos. 180, 172, 132, 124, 121 and 121 and 172, 132, 124, 180, nos. , Q, Quartz and F, Feldspar. on (2 microns) of the sample microns) on (2 lite; Q+I, Quartz with Illite lite; Q+I, Quartz with ffraction pattern of clay fracti pattern of ffraction te; I/S, Illite-Smectite; I, Il te; I/S, Illite-Smectite; to 550º C. K/S, Kaolinite-Smecti Fig. 51. Characteristics Fig. 51. Characteristics X-ray di 125

Fig. 52. Characteristics X-ray diffraction patterns of K/S mixed layer clay fraction. A) diffraction of 10Å of the sample no. 91 of Fenchuganj well-2, H, heated; G, glycolated and U, Untreated. B) diffraction of heated, glycolated and untreated clay fraction of sample no 91 of Fenchuganj well-2, with 3.5Å. C) diffraction of heated, glycolated and untreated clay fraction of sample no 183 of Patharia well-5 with 10Å. 126 e; I, Illite; K/S, Kaolinite-Smectite; Q+I, Quartz with Quartz Q+I, Kaolinite-Smectite; K/S, Illite; I, e; (2 microns) of the sample nos. 180G, 168G, 124G and 118G of 124G and 118G 180G, 168G, sample nos. the microns) of (2 ol (G). I/S, Illite-Smectit tterns of the clay fraction and F, Feldspar. Fig. 53. X-ray diffraction pa 53. X-ray Fig. Patharia well-5 treated with ethylene glyc ethylene well-5 treated with Patharia Quartz Q, Illite, 127 ite; I, Illite; K/S, nos. 91 of Fenchuganj well-2, Fenchuganj of nos. 91 91H). I/S, Illite-Smect (2 microns) of the sample of (2 microns) ethylene glycol (91G) and heated to 550º C ( 550º C heated to and ethylene glycol (91G) Fig. 54. X-ray diffraction patterns of the clay of the clay fraction patterns Fig. 54. X-ray diffraction Untreated (91U), with treated Kaolinite-Smectite; Q+I, QuartzIllite with F,and Feldspar. 128

The X-ray diffraction pattern of kaolinite-smectite mixed layer (disoriented) does not resemble that of a pure Kaolinite. It differs in the number of reflections, their relative intensities and the exact angular position of the basal reflection. If an XRD pattern is similar to that of Kaolinite and if the reflection at about 7 Å shows larger d-values than that of halloysite (7 Å) and expands by treatment with ethylene glycol, the specimen can be identified as an interstratified Kaolinite. Fig 53 which shows an enlargement of 7 Å reflection after treatment with ethylene glycol, proves the idenfication of Kaolinite-Smectite mixed layer. Discrete Kaolinite in the sample will affect the position of neighbouring kaolinite/smectite peak (Tomita & Takahashi 1986). For more confirmation the samples were heated to 550° C and may be interpreted with the aid of the concept of Ross (1968). According to this idea we may explain the structure by assuming that the 2:1 type layers do not dehydroxylate; in this way the diffraction composed of 2:1 layers can be separated by X-ray amorphous metakaolinite material. On heating, the breakdown of kaolinite layers causes the reflection to gradually decrease and nearly to disappear, if further heated. The chemical formula of the K/S mixed layer was calculated and given by Wiewiora (1971) as follows: 1) Kaolinite layers have an ideal composition, Al2Si2O5(OH)4. 2) Smectite layers have the general formulae, Mx + y [(Al2 – y Mg y)(Si4 – x Al x) O5(OH)2] where M means Mg, Ca, Na, K. An additional assumption is necessary, that x = y. Srodon (1980) suggested that K/S forms by the dissolution of smectite layers and the crystallisation of kaolinite layers. Thus, the two pathways of kaolinization of smectite differ by the site of kaolinite nucleation: within versus outside smectite crystals. In most of the published cases, it can be shown that kaolinite/smectite forms at the expense of smectite (Altschuler et al. 1963, Drits & Sakharov 1976). Shinoyama et al. (1969) described randomly interstratified kaolinite-smectite from acid clay in Japan. In this case, 2:1 (two tetrahedral per one octahedral) expanding layers of smectite were distinguished. Wiewiora (1973), Sakharov & Drits (1973) propose crystallisation of K/S from solution. Most authors writing on the subject say that K/S always evolves from smectite. K/S originating from Kaolinite has not been reported. Wiewiora (1971) made an attempt to evaluate the proportions of kaolinite and smectite layers in the clay size fraction and found about 80–90 per cent of Kaolinite. Wiewiora (1971) observed the K/S peaks have combined diffraction effects indicating that kaolinite - nonexpanding and smectite - expanding layers are interlayered. After heating for 3 hours at 550° C kaolinite layers fully dehydroxylate. For the present case, the samples were heated to 550° C for 1 hour and the reflections of K/S were decreased to a noticeable mark. Fig. 50 shows the non-heated and fig. 51 shows the heated reflections of K/S mixed layer. After treatment with ethylene glycol, the samples were expanded much proving them as kaolinite-smectite mixed layer. Fig. 53 shows nicely the expansion of the reflections. A comparison between fig. 51 (heated) and Fig. 53 (glycolated) can provide a very useful basis for the understanding and identification of the K/S mixed layer. The matching number on Powder Diffraction File for K/S mixed layer was 29 – 1490. 129

Semi-quantitative analysis shows that K/S mixed layer was present by 74% when it attains maximum abundance in the well Patharia-5 at the depth of 3161.25m. Kaolinite/smectite mixed layer mineral also played an effective role in the diagenetic history of Surma Basin. The present study reveals that the transformation of smectite to illite took place through intermediate mixed layers of illite/smectite and kaolinite/smectite by the adsorption of potassium and sodium. Fig. 49 shows the diagenetic model of Surma Basin where K/S mixed layers were transformed to produce illite under a K-rich environment. The dominance of a kaolinite/smectite mixed layer in the clay mineral assemblage reflects the onshore position and shallow nature of the environment with warm climates and seasonal rainfall. The abundance of K/S mixed layers also indicates that all source areas for the sediments of Surma Basin had highly kaolinitic soil profiles, reflecting their intense weathering. Thus, the presence of a K/S mixed layer bears the evidence of climate, environment and diagenesis as well as a clue to provenance.

8.2 TEM and SEM

Non clay accessery minerals detected by TEM in SB include barite, rutile, Fe-oxides and K-feldspar (Fig. 56–58). TEM micro analyses reveal that the order of abundance of the octahedral cations is Al > Mg > Fe. Typical smectite and illite characterisation were done using TEM images. Quantitative analyses was undertaken for understanding different element concentrations of illite and smectite (Fig. 55). A Scanning electron microscope (SEM) has been used in the present study. The very high resolution obtained in the SEM readily describes the minerals. The analyses also reveals their morphology, textural relationship and growth habits. SEM analyses were carried out with magnifications between 100X and 3500X with Au–Pb coated samples. The minerals within the Surma Group sediments include quartz, calcite, chlorite, kaolinite, illite, smectite and barite. Quartz forms one of the most important diagenetic minerals in Surma Basin shales. The quartz occurs as quartz overgrowth. The quartz overgrowth include the small isolated and incomplete growth of quartz crystal faces on detrital grain (Fig. 60). Pittman (1972) and Imam (1986) have described such growths. Calcite forms an abundant cement in the SG shales. SEM studies reveal from the mutual textural relationship of calcite and quartz overgrowth, that the pore filling calcite post dates quartz overgrowth as the calcite is seen to envelope the crystal faces of quartz overgrowth (Fig. 59). Chlorite is also a common clay mineral in Neogene shale of SB. Chlorite occurs as pore filling materials and as a replacement of detrital grain. Some Common morphologies of chlorites are clusters of bladed or platy crystals. Illite is one of the most common clay minerals in the Neogene shale of SB. Under SEM, illite appears as sheets or large flacky crystals or as fibres. Kaolinite is also a common clay mineral of SB. It is like platelets crystal under SEM, usually altered from illite. The weathering of K-feldspar leads to the formation of kaolinite. Barite was also detected in Neogene shales. Some samples from Patharia well-5 having a very high concentration of Ba were studied under SEM. Quantitative analyses showed the Barite (BaSO4) was dominant (Fig. 59). The study also revealed that Ba was associated with SiO2 and clay minerals (Fig. 59). 130

Pittman (1979) suggested the source of silica for quartz overgrowth to be the result of: (1) pressure solution, (2) diagenesis of clay minerals, (3) decomposition of feldspar, (4) replacement of silicates by carbonates, (5) precipitation from percolating ground water, (6) dissolution of siliceous organism such as sponges, diatoms, radiolaria etc. and (7) hydration of volcanic glass. The transformation of smectite to illite during the clay mineral diagenesis of shales releases Si+4 ions as a by-product which could migrate to adjacent sandstone beds during shale dewater and could cause quartz cementation (Towe 1962, Boles & Frank 1979; Lahann 1980 & Boles 1981). The amount of Si+4 ions released into the pore water system would depend on the availability of shale containing smectite or illite/smectite mixed layer clay mineral and the degree of diagenesis. The increasing abundance of quartz overgrowth in deeply buried rock is correlated with an increasing degree of burial diagenesis of shales (Imam 1986). It is thus suggested that the illite/smectite clay diagenesis is one of the important sources of quartz cement in the Neogene shales. Replacement of quartz and feldspar by calcite and the dissolution of feldspar are both considered to be the potential source of quartz cement, as both would release silica into the pore water (Pittman 1979). In the present study, the replacement of silicate grains by calcite cement and the dissolution of feldspar were observed. Smectite to illite diagenesis in the illite/smectite clay in Neogene shales is an important source of quartz cement of SB. The replacement of silicate by calcite and dissolution of feldspar may also have been a minor source locally (Imam 1986).

8.3 Petrography

Thin sections of the Neogene shales of SB contain mainly quartz with minor amounts of muscovite, biotite, calcite and clay minerals like chlorite and illite. The quartz grains are monocrystalline, a few grains show a polycrystalline structure. The grain size was medium to fine quartz with normal extinction and most grains were fractured, subangular to subrounded. They were moderately sorted, at places, quartz were found to be ill sorted. The quartz also shows overgrowth. K-feldspar grains are abundant, their grainsize being comparable more with the finer fraction of the quartz. The K-feldspar grains are comparatively finer and plagioclose is rare (Fig. 60). The quartz is constituted of subangular to subrounded framework grains having medium sphericity with a dominant carbonate cement. Quartz grains are fractured provides the evidence of intense chemical weathering. Feldspar with a few mica minerals (biotite, muscovite) were present. Matrix of from less than 5% to over 15% were present and composed of very fine and fine quartz grains admixed with argillaceous material and chlorite flakes. The size of quartz grains shows a distinct bimodality in which the finer fraction is dominant. Plagioclase occurs as subhedral to euhedral grains. At places, muscovite is found interleaved with biotite. Mica occurs as massive grains and as flakes. They are seen changing to K-feldspar and show alteration to chlorite. The rocks are in general, very poor in heavy minerals. The sandstones are mineralogically immature. The finer grain shows more angularity than the coarser grains. Patharia well-5 samples show overgrowth of quartz grains and alternative lamine of quartzwacke and siltstone bands. 131

Diagenetic replacement of the feldspar grains by carbonate cement is observed. These are indicative of the poor textural as well as mineralogical maturity of the SG sediments. Lithic fragments are composed essentially of shale and chert and calcareous particles. Isolated patches of calcareous material were present as cementing material. Calcitic cementing material were also present as remnant particles and as antiperthitic cement between calcite and quartz grains. Some samples showed ferruginous cement. Rashidpur well samples are mostly sandy siltstone, micaceous shale and silty shale as constituents. Some of the wells contain an appreciable amount of clayey detrital matrix and chlorite flakes are important to mention.

500 nm

cps Si 500 nm O cps

Al

Si O Al

Mg K Fe

K Energy (keV) Mg Fe Fe

Energy (keV)

Fig. 55. A) Energy disperse X – ray spectra of typical illite from clay separates of sample no 84 of Atgram well – IX. Qualitative analysis shows different concentrations of Al, Si, K, Na, Mg and Fe. B) Energy disperse X – ray spectra of typical smectite from clay separates of sample no 124 of Patharia well – 5. Qualitative analysis shows different concentrations of Al, Si, K, Na, Mg and Fe. Large crystal is about 1700 nm in width. 132

Fig. 56. TEM – photographs of clay fraction showing clay minerals, silica and iron oxide. Sample from Patharia well – 5. 133

Fig. 57. (Top) TEM photographs of clay fraction showing illite (X14000) from the Patharia well – 5. (Bottom). TEM photographs of clay fraction showing kaolinite (X14000) from the Patharia well – 5. 134

Fig. 58. TEM photographs of clay fraction showing Barite grains (black). 135

Fig. 59. (A) SEM micrograph of quartz overgrowth with interlocking texture (calcite cement), Q, Quartz; Ch, Chlorite; (X3500). (B) SEM micrograph of quartz (Q) with interlocking clay minerals (I, Illite and K, Kaolinite). (C) SEM micrograph with a generalized view showing silica and clay minerals associated with some heavies (Barium and Titanium), I, Illite; Q, Quartz; Ba, Barite (X100). (D) SEM micrograph showing clay minerals (illite, kaolinite and chlorite). (E) SEM micrograph showing higher concentration of Barite (white grain) associated with quartz and clay minerals (X500). (F) SEM micrograph showing quartz, clay minerals and dominantly Barite (white grain), (X2000). Samples are from Patharia well – 5. 136

Fig. 60. A–D. Showing quartz, orthoclase feldspar and plagioclase feldspar as main constituent. Orthoclase are finer. Feldspar shows the alteration. Quartz and feldpar are of different grain sizes. Mica and calcite are common as accessory minerals. Grain boundaries and fractures on quartz and feldspar bears the evidence of intense weathering. Q, Quartz, F, Feldspar, C, Calcite, M, Mica, B, Biotite. 9 Discussion

Palynological evidence suggests that marked vegetation changes occurred that were related to paleoenvironmental changes in the Surma Basin during the Neogene. The qualitative assessment of the palynoassemblages recovered from the wells reveals a close similarity amongst themselves in their fair occurrences of pteridophytic spores, viz., Cyathidites, Cicatricosisporites, schizoeisporites. Among these, the Cyathideous forms are more frequent. Triporoletes characterize the brayophytic component while gymnospermous pollen are poorly represented specially in older rocks. A reworking of Oligocene-Eocene pollen taxa namely Meyeripollies naharkotensis, Polypodiesporites Oligocenecus and Palmopollenites Eocenecus has also been recorded. The palynological assemblages of the Surma Group of SB sedimentary sequences is dominated by trilete bearing pteridophytic spores and angiouspermous pollen. The gymnospermous component are very poor and monolete spores are rare. The qualitative and quantitative analyses of the palynofloral assemblages and its comparison with other known equivalent assemblages from India have been discussed. Pteridophytic spores are richly represented in the SG sediment of the Surma Basin. Their comparison with the extant flora indicates the presence of the Lycopodiaceae, polypodiaceae and Cyatheaceae. Plants of these families are mainly found in tropical and subtropical areas. Angiouspermous pollen also form a significant group and are represented by Palmaepollenites dominantly. The distribution of this pollen type is restricted to tropical and subtropical regions. Gymnospermous pollen grains are comparatively less represented in the assemblage than pteridophytic spores. The thallophytic remains are represented in the assemblage by dinoflagellate cysts, fungi and fungal spores. The quantitative analysis shows the palynoassemblages are populated by 63 genera and 95 species of angiospermous and gymnospermous pollen grains, pteridophytic spores, dinoflagellates cysts and fungal remains. On the basis of quantitative analysis three local palynostratigraphic zones were distinguished from the SG sediment sequence of Fenchuganj well-2. They were i) Palmepollenite zone (Z-1), ii) Tricolpate - trilete zone (Z-2) and iii) Dissacate zone (Z-3) in descending order of stratigraphy. The zone-1 constitutes the lower bio-stratigraphic unit of the SG with the dominant representation of palmepollenite (31%) taxa. Gymnospermous pollen grains are insignificantly representd 138 by 3.8%. Pteridophytic spores constitute a major portion of the assemblage. Among the pteridophytic spores, trilete spores form the dominant element while monolete spores remain insignificant. Cicatricosisporites macrocostatus is the most dominant throughout the zone. The presence of Rhizophora pollen provides a basis for interpreting the palaeoenvironment of the drilled sequence. The zone-3 shows a clear dominance of dissaccate pollen. Pteridophytes are being represented by the monolete forms levigatosporites and verrucatosporites. Cyathidites minor was the important constituent of triletes spores. A comparison of the present assemblages with those of known Miocene assemblages of Assam and Meghalaya (Baksi 1965, Singh et al. 1986, Banerjee 1964) and Bengal Basin (Baksi 1971, Deb 1970) of India have been attempted. Comparative study reveals that the SG sediments of Surma Basin, Bangladesh is closely comparable with that of the Assam and Maghalaya sequences (Garo Hills). The microfloral association of the Palynological zone I can be compared with the palynological assemblage of Simsang Palynological zone IV of Meghalaya, India (Baksi 1965) and Bengal Palynological zone (BPZ)-V (Baksi 1971) and indicate a Lower to Middle Miocene age. The presence of Foraminifera indicate that the sediments of this zone were deposited in shallow marine conditions. The presence of Rhizophora pollen and dynoflagellates indicate brackish to shallow marine deposits. The microflora of Palynological zone II can also be compared with those of the Simsang Palynological Zone IV of Meghalaya, India and BPZ V (Baksi 1971). Based on these comparisons, Palynological Zone II is presumed to be of Middle to Upper Miocene. It is interesting that the floral change from monocolpate pollen Palmepollenites to Tricolpate - trilete could be recognized well by an increase in frequency by 50%. The presence of mangrove pollen Rhizophora indicates the shallow marine to brackish environmental deposition of this drilled sequence. The microfloral assemblage of Palynological Zone III may be compared with Simsang Palynological Zone IV of Meghalaya, India (Baksi 1965) and BPZ Zone-V is presumed to be Upper Miocene. The qualitative assessment of the palyno assemblages recovered from the six wells of Surma Basin, Bangladesh reveals a close similarity amongst themselves. The common occurrence of pteridophytic spores, viz; Cyathidites, Cicatricosisporites, Schizoeoisporites is remarkable. Among these, the Cyathiceous forms are more frequent. Triporolets characterize the bryophytic component. The stratigraphy of Neogene SG sediments of the Surma Basin are presented on the basis of palynofacies and lithofacies of the unit. The SG unit contains sandstone lithofacies A and combined facies B consisting of claystone, mudstone and shale. Facies B is abundant and facies A is less common. In lithofacies, B shale is predominant in comparison to others consisting of siltstone and sandstone. The reconstruction of the paleoenvironment and paleoclimate in the Surma Basin during the Neogene is based on a complex stratigraphic sequence including a variety of lithofacies as well as palynofacies indicating shallow marine to brackish interdeltaic environments. This interpretation is based on the predominance of lithofacies B and the distribution of pollen, spores, microplankton and dinoflagellates. The sandstones with siltstone and shales were deposited in a shallow marine environment throughout the Miocene. 139

The angiosperm dominating pollen flora suggest a tropical to subtropical area. The occurrence of Cicatricosisporites, an aquatic fern, indicate a marine brackish environment. Palynomorph assemblage containing mangrove forms and dinoflagellates and dinoflagellates cysts suggest a shallow marine environment. The shallow marine and brackish environment reflects a marine transgression. The transgression of the Miocene certainly affected the coastline. Major changes in sea level for the Neogene are suggested based upon transgressive-regressive phenomena. A marked rise in the sea level would have caused a marine transgression (Bandy 1968). The transgression of the sea over a wide area might have increased humidity and moderated the temperature. There is a definite increase in the gymnosperm microflora indicative of marshland and warm climate (Srivasta & Banerjee 1969). A high frequency of Dissaccates indicates tectonic activity and an environmental change in the source area. The presence of reworked microflora elements and conifer pollen together with trangression inidicators, indicate an increased tectonic activity in the Surma basin during the Neogene and they are related to the Himalayas. The Surma Basin area has been progressively coming under the tectonic control of the Great Himalayan Orogeny and the crustal shortening due to the collision of the Indian and Asian plates and has resulted in extensive uplifts and thrusting of the older rocks (Benerjee 1984). The above mentioned paleoenvironmental circumstances must at some stages have contributed to the retrogressive succession of the vegetation in this area. In this connection, it is pertinent to refer to some ecological aspects of palm, as they feature so prominently in the pollen sequence. At present, palm are considered to be very important in the evolution of tropical forests ecosystems and must have been even more so in the past (Moore 1973). The pollen spectra of the Surma Basin contains a high percentage of regionally produced pollen of mixed sub-tropical vegetation. It reflects a mixture of palm and coniferous forest in which palmepollenite is dominant. Palynostratigraphic zones suggest a mixed type of subtropical to tropical forests types existing there and the development of dominant palm vegetation. Grass, according to the pollen data, were already established in the area during the early to Middle Miocene, and experiencing summer rainfall similar to the present day climate. The pollen evidence for a mixed tropical - subtropical forests could be consistent with the Miocene riverine environment in the area as suggested by the lithological data. The age of the Surma Group sediments of Surma Basin was assigned to the Neogene. On the basis of pollen investigations, the Surma Group was assigned to the early to late Miocene in age. The geochemistry of the shales in the SG sediments of the SB has been studied in details. The SG sediments are typical continentally-derived. A comparison of the NS of the present study with previously published shale compositions suggests that the present study has the qualities of an average of averages. Major element variation curves shows nicely their distribution and interrelation between the oxides present in the sequence. Common pictures are as follows: i) The increase of Al2O3 was related to the decrease of SiO2 ii) Increase of CaO and MnO was related to the decrease of Na2O, MgO and K2O iii) The fluctuation of Al2O3, Fe2O3 and MgO were more or less similar. 140

The decrease of SiO2 content in the wells with the increase of Al2O3 may be related to a desilicification phenomenon which took place mainly by the destruction of aluminosilicates. This is also associated with the formation of clay minerals and grain size variation of the sequence. The increase of CaO and MnO with the decrease of Na2O, MgO and K2O shows the variation in the chemical composition, reflecting changes in the mineralogical composition of the sediments due to the effects of weathering, marine sedimentation and early diagenetic processes (Shaw & Weaver 1965, Drever 1971, Nesbitt & Young 1984, 1989). Calcium shows a decreasing trend, except for a few intervals in the sequence of Miocene time. This decrease in the Calcium content can be attributed to the terrigenous influx and the low abundance of fossil shell and shell fragments, which contribute a major amount of the Calcium in them. The average magnesium content is low during lower to Middle Miocene. It shows a little higher content in the Upper Miocene sequences, which is due to Mg ions absorbed on clays. Manganese content increases at different intervals in the wells. Clay mineral content is found to cause a Mn enrichment (Becini and Turi 1974). The high K2O and low CaO contents of many samples are interesting. Many sedimentary processes can severely affect the abundance of these elements, including weathering (Nesbitt 1980), diagenesis and burial metamorphism (Hower et al. 1976). The high K content is almost certainly due to the original presence of large quantities of illite (McLennan et al. 1983). There are clear, positive correlations between K content and the abundances of Al, Cs, Ba, Th and U (Fig. 31), suggesting that the absolute abundances of these elements are primarily controlled by the amount of the dominant original clay mineral (illite) (McLennan et al. 1983). Decreasing the K2O/Na2O ratio in the wells (Fig. 23–28) indicates the decreasing maturity of the sediments, reflecting a reduced influx of highly Kaolinized material. Factors such as increased erosion in relation to weathering, and/or transgression resulted in Kaolinite-depleted rocks (Dypvik 1979). The trend of K2O/Na2O is interesting and is consistent with the grain size analysis. Na and K in the studied SG Neogene shale are mostly confined in the detrital illites. The variation of the curve K2O/Na2O obviously reflects in part the different original compositions of the source rocks. CaO, Na2O, MgO as well as iron were leached from the profile. K2O was commonly enriched strongly in profiles and suggested the geochemical evidence pointed to alkaline and reducing ground waters (McLennan et al. 1983). The sequences of the wells exhibit a depletion of Na and Ca (Fig. 9-14), probably reflecting intense chemical weathering of their source rocks. The variation of Al2O3, CaO, Na2O and K2O in the whole sequence, reflect chiefly variable climatic zones or rates of tectonic uplift in source areas. The enrichment of MgO in all the wells is related to the decrease of CaO, which in turn is due to the weathering effect. High MgO content is often correlated with low temperature oxidative diagenesis. In such a case, an increase of MgO in the rocks is accompanied by a drop in CaO (Andrews 1980). The positive correlation of Al2O3 and MgO (Fig. 29) indicate that Mg is originally associated with aluminosilicate phases and assumes a minor association with carbonates during diagenesis (Bellanca et al. 1999). The excellent positive correlations of K2O, TiO2 and MgO with Al2O3 (Fig. 29 & 30) indicate that these elements are associated entirely with detrital phases and also 141 suggesting that they are associated with aluminous clay minerals such as illite or smectite. It also indicate that weathering was an important factor in the source area, where K and Mg are fixed in clay minerals and Ca is preferentially leached (Nesbitt et al. 1980). The correlation between FeO and MgO (Fig. 32) appears positive suggesting the mineral chlorite controls the distribution of Al2O3, MgO and Fe2O3, indicating their association with the clay minerals. The variation of the oxides in the sequences reflect chiefly variable climatic zones or rates of tectonic uplift in source areas. The concentration of Fe is due to the formation of Fe-hydroxide and due to the presence of biotite. The higher concentration of Fe2O3 in the wells is indicative of oxidation, hydration and leaching processes involved during weathering (Mikkel & Henderson 1983). The different maturity parameters studied display complicated development with an increasing maturity of different depth intervals. The maturity index ratios are indicative of a kaolinization process and typically mature sediment. The maturity increases with the decrease of the silica content and grain size. Cu/Zn ratio of NS indicates fluctuating oxidizing-reducing conditions in the environment of deposition. The maturity index curves of the wells of SB provide a meaningful chemostratigraphic subdivision of bore holes with mature and immature zones. The study demarcated mature and immature zones of the wells of SB on the basis of various maturity indexes. They are given in the following table.

Table 14. Mature and immature zones of the wells by the maturity parameters.

Well Matured zone Immature zone Atgram well - IX 3647–3990m 3639–3640m Fenchuganj – 2 well (1) 3259.96–3269.55m 3137–3143m (2) 3624–3779m Habiganj well – 1 (1) 1849.22–1849.83m 1849.83–1850.74m (2) 1851.66–1852.65m Kailastila – 1 well 1175.30–1176.22m 2974.52–3731.24m Patharia well – 5 (1) 2831.00–2834.84m 2300–2307.25m (2) 3165.25–3166.75m Rashidpur –1 well (1) 1087.40–1248.93m 1248,93-1249.68m (2) 1250.6–1832.45m The higher abundance of Th in the rocks reflects the presence of Th bearing minerals. The higher Th/U ratio probably indicates the derivation of these sediments from the recycling of the crust. Recycles of sediments themselves lead to a further loss of U and an increase in the Th/U ratio. The higher value of the Th/U ratio in the core samples is because of oxidation. The increase of Th is also related to clay minerals. Th tends to increase with a fall in potassium and because a concentration of potassium is directly related to illite composition in sediments. Thorium concentration in sediments varies with illite content. Near shore sediments have degraded illites where concentrations of thorium (or uranium) could be higher and the reverse may be true with distance from the shore. Th/U is controlled by the weathering-erosion-diagenesis cycle. Condie (1993) has shown similar observation with the study of shales from the upper continental crust, USA. However, the whole sequence of Th/U ratio represents different stages in oxidation, leaching and deposition under marine conditions. 142

Four elements like V, Ba, Cr and Zr were normalized to Rb and the profiles of the wells were fluctuating at different depths. The reason for normalization to Rb is that this element is inert with respect to biogenic procceses (Emelyanov & Shimkus, 1986). Geochemical ratios of Cr/Rb, Zr/Rb and Ba/Rb display higher values on the average for Neogene shale of SB, which could be explained by an enhanced terrigenous input during their deposition. Higher values of Ba/Rb at different depths could also reflect a diagenetic mobilization of barite (Bellanca et al. 1999). Cr and Ni values are generally high for the Neogene shale samples of SB (Cr ~14–20, Ni ~ 17–97ppm). The average ratio of Cr/Ni is 2.2 with variation among the values between the wells. The higher concentration indicates that the source region was composed of ultramaffic rocks. Cr and V are positively correlated with Al2O3 (Fig. 30), suggesting that they may be bound in clays and concentrated during weathering (Fedo et al. 1996). Ni may be enriched in a reducing environment. Vanadium also is thought to be enriched in an organically rich, reducing environment. The sequences completed for Cr/V and Ni (Fig 40) are more or less similar, indicating that they were deposited in the same reducing environment. A higher Cr/V ratio probably reflecting a source rock richer in Cr. The weathering processes would also have different formations of clay minerals. Differences in Cr/V ratios in the wells are indicators of differences in nature or degree of weathering. Tectonic discrimination of SG sediments using SiO2 content and K2O/Na2O ratio indicates that the SB sediments were deposited in an active continental margin (ACM). Seismotectonic and tectonic reports of the region as well as the report from the study area are in good agreement with the present result. Mineralogical and geochemical data from the Surma Basin suggest that the detrital input was especially intence during the Neogene probably because of tectonic forces linked to the active upliftment of the Himalayas. The effect of variable degrees of weathering in source areas can be important in influencing alkali and alkaline earth element contents of terrigenous sedimentary rocks (Nesbitt et al. 1980, Reimer 1985). The degree of chemical weathering is a function chiefly of climate and erosion rate, the latter of which varies with the rate of tectonic uplift (Wronkewicz and Condie 1987). Neogene shale of the Surma Basin reflects a variety of climatic conditions and perhaps also different tectonic regimes. The Surma Group unit exhibits the greatest depletion in Ca and Mn and appears to reflect the most intensely weathered source rock. The Neogene shale of the SG also exhibits less depletion of the alkaline element and reflects an active uplift of the Himalayas (Wronkewicz and Condie 1987). The dominance of shale with sandstone in SG reflects a low-energy depositional environment. The distribution of HFSE (Zr, Nb, Hf, Th, and V), REE, Sc and Co of the Neogene shale of SB generally have relatively short residence times in seawater and are the least mobile during weathering, transport and diagenesis and thus provides a clue to the provenance of terrigenous sediments. The data presented in table-11 and in appendix- 2, in figures 34–39 and 47 indicate that REE, HFSE tend to increase and fluctuate in abundance with the stratigraphic height. This stratigraphic geochemical trend suggests that both granite and basalt sources increase with time during the deposition of SG sediments. 143

In terms of the distribution of Th-Hf-Co-Sc, the Neogene shales clearly show a large contribution of mafic and ultramafic components. The high to very high ratios of Cr/V and Ni/Co also reflect a significantly greater contribution of mafic-ultramafic components in the sources (Taylor & McLennan 1985). The relative contributions of granite and basaltic sources are reflected in the distribution of Zr and Cr in Neogene shale of SB, since these two elements are enriched in the whole sequence (Appendix-2). The enrichment of these elements again indicates increased input into the Surma Basin of both granite and basalt. The low Cr/Zr ratio (<2 in average) in the Neogene shales also indicates the importance of granite relative to basalt (Wronkewicz and Condie 1987). Taylor and McLennan (1985) have shown that Th/Sc and La/Sc ratios reflect the proportion of the mafic and ultramafic component compared to the felsic component. The abrupt increase of these ratios in Neogene shale of SB (Table 11, Appendix-2) attests to the importance of in the source areas. The best provenance discrimination was obtained if the Ba/Sc and Ba/Co ratios were used (Cullers et al. 1988). In the present study, the high Ba/Co and Ba/Sc ratios of the samples point to granitic rocks as possible source rocks. The high proportion of granitic source material entering the Surma Basin, as implied by the geochemistry of the Neogene shales may be derived from the Himalaya located towards the northern boundary of the Surma Basin, a model more consistent with previous source area studies of the Surma Basin (Ray 1982, Molnar 1984, Johnson and Alam 1991). The diagenetic history of the NS sequences has been studied in details. Illite, kaolinite, chlorite, I/S and K/S mixed layer are the main clay minerals in the SB. The transformation of smectite to illite through an intermediate mixed-layer I/S clay is a widely recognized clay diagenesis reaction in shales with progressive basal depth. Mixed layer kaolinite-smectite has been reported for the first time and is thus a new mineral in Bangladesh. Progressive illitization of illite/smectite mixed layer clay in SG shales is a depth - temperature related diagenetic change which means that I/S mixed layer clay gets progressively wider in illite at the expense of the smectite layer with increasing burial depth. The present study also reveals that smectite diagenesis and dehydration have contributed to the generation of overpressure in the Bhuban Formation in Patharia well-5. The dominance of detrital kaolinite is a clay mineral assemblage which also indicates illite and I/S, K/S, reflecting the onshore position and shallow nature of the environment. Since kaolinite is commonly deposited close to the source as a result of differential flocculation in fresh or brackish water and sedimentation. Kaolinite contents of NS mainly rely on climate and suggests that warmer conditions must have been associated with increased humidity on shore. The Surma Basin clay mineral assemblage also reflects physical and chemical weathering in the source area. Kaolinite reflects the composition of the soil under humid tropical conditions where chemical weathering predominates. Intensive weathering, involving warm temperatures and high rates of water percolation is most conducive for increased kaolinite formation in source areas (Gibson et al. 2000). Robert and Chamley (1987) proposed that higher rates of percolation could result from increased topographic relief and/or by increased amounts of rainfall. 144

An increase in topographic relief could result either from a significant relative lowering of sea level or by the relative tectonic uplift of the source area. The kaolinite increase could reflect a general Miocene temperature increase and/or the beginnings of increased precipitation and percolation. The high levels of kaolinite also indicate that all source areas for sediments of Surma Basin had highly kaolinite soil profiles reflecting the same intense weathering. The occurrence of kaolinite, which is not easily transported over large distances, rather suggest a deposition close to the shore where exposed land masses constitute a potential source of the mineral which is also in agreement with the palynological report of this study. The large abundance of illite and specially chlorite suggests an active erosion of exposed rocks. The clay mineral assemblage of the SB is strongly dominated by Illite/ Smectite and Kaolinite/Smectite content. This suggest warm climates with seasonal rainfall through much of the Miocene. The increased amount of illite also suggests a strong renewal of active erosional processes on land. The cause of such renewal could be tectonic (Chamley et al. 1997). The tectonic instability expressed by the clay mineral from open marine to a more restricted continental environment which has been inferred from the palynological analysis. Vegetational changes in the Surma Basin area also suggests an increase both in temperature and precipitation (Gibson et al. 2000). Bouquillon et al. (1990) noted that the clay mineral assemblage of illite and chlorite represent the characteristic signature of sediments derived from the Himalayas. Chlorite is a common product of the erosion of low grade metamorphic rocks and illite is obtained from the weathering of siliceous, igneous and high grade metamorphic rocks. Thus the clay mineral assemblages of the Surma Basin represents the sediments derived from the Himalayas. SEM revealed the quartz outgrowth in the Neogene SG sediments of the SB. The geochemical results are suggestive of a felsic continental source material mainly for these sediments. It is useful, however, to evaluate the data in relation to the tectonism of the area. Trace element geochemistry of the area has proved that it is a useful tool as a palaeoenvironment marker. The results presented show that the approach used can provide a meaningful chemostratigraphic subdivision of a bore hole and can also highlight geochemically anomalous zones. Statistically derived chemostratigraphic zonal sequences are in good agreement with the litho stratigraphy of the area. Regarding paleoenvironments, trace-element geochemistry indicates that the surface waters must have had intense primary productivity (Ba enrichment) and that the bottom conditions must have been anoxic and sulphidic. This is in good agreement with the observation of the faunal content of the sediment, reported by pollen analysis. The presence of micro plankton foraminifera, thought to live at greater depth stresses, that environmental conditions, must have allowed the presence of planktic fauna only in surface waters. The present study confirms that depositional conditions must have been reducing. The oxygen-minimum zone must have impinged on the seafloor for a sufficiently long time to allow sulphate reduction to occur at the base of the water column. Geochemical signatures recorded by the present data indicate a brackish-marine nature for the paleoenvironment. The occurrence of kaolinite, which is not easily transported over large 145 distances, suggest rather a deposition close to shore which is also in good agreement with the palynological report of this study. The tectonic instability expressed by the clay mineral from an open marine to a more restricted continental environment has also been inferred from the palynological analysis. Palynostratigraphic zones suggest a mixed type of subtropical and tropical forest types. The presence of foraminifera in association with a palynomorph assemblage containing mangrove forms and dinoflagellate cysts suggest a marine environment. The sandstone with siltstone and shale were deposited in a shallow marine environment throughout the Miocene. The shallow marine and brackish environment reflects a marine transgression. During the Miocene SB has witnessed a conspicuous subsidence and marine transgression. Major changes in sea level for the later Neogene are suggested based upon transgressive-regressive phenomena. A marked rise in the sea level would have caused a marine transgression (Bandy 1968). Undoubtedly, sea level and climate changes affected the deposition of the SG sediments of the Surma Basin. 10 Conclusions

An analysis of stratigraphic, sedimentologic, palynologic, geochemic and mineralogic data have been undertaken during the present investigation with the aim of providing a comprehensive and detailed analysis of Neogene Surma Group sediments from Surma Basin, Sylhet, Bangladesh. Particularly, the study was aimed at obtaining the age frame of the Surma Group and to review the stratigraphical data based on pollen analysis in order to better direct a reconstruction of palaeoenvironmental and palaeoclimatic variations in Bangladesh during the Neogene. In the present study, palynological and petrographic techniques were combined with major and trace-element analysis in order to gain more information on the provenance, sedimentary history and geochemistry of the Neogene Surma Group sediments of the Surma Basin. Palynological data indicate that the age of the Surma Group is Miocene. The sedimentary, palynological and geochemical study suggest that the deposition took place under shallow marine to brackish environmental condition. The paleoecological and paleogeographical conditions of the Surma Group include marine transgression with subsidence during the Miocene. During the late Miocene, a significant shift in the flora occurred by the growth of conifer forest. A strong marine influence in the depositional environment indicated by the presence of micro- foraminifera. The presence of hystrichospherids suggest a more open marine environment. Combined lithofacies B, accounts for more than two-thirds of the total formation contains plant and marine animal fossils. Palynological assemblages of the Surma Group of sedimentary sequence of Bangladesh include taxa range in age from the Lower Miocene to the Upper Miocene which can be potentially used in dating and correlation. Three palynological zones have been recognized from the well Fenchuganj -2. They are demarcated as zone -1 (Palmepollenite zone), zone -2 (Tricolpate – trilete zone) and zone - 3 (Dissacate zone). Surma Group sediments are correlated with Simsang Palynological Zone IV of Meghalaya, India and Bengal Palynological Zone (BPZ) V of India. Geochemical and mineralogical study of the Surma Group reveals the origin, condition of deposition, sedimentation, tectonics and diagenetic history of the formation. 147

Geochemical ratios were useful for determining grain size, maturity, tectonics and the environment of deposition. Trace element analysis indicates that Surma Group sediment contains elements which are environmentally sensitive. Trace-element geochemistry indicates that the surface waters must have had intence primary productivity (Ba enrichment) and that the bottom condition must have been anoxic and sulphidic. The higher values of Th/U ratio in the core samples is because of oxidation. Geochemical ratios of Cr/Rb, Zr/Rb and Ba/Rb show higher values due to enhanced terrigenous input during their deposition. Higher values for Ba/Rb reflect a diagenetic mobilization of barite. The enrichment of Ni and V was due to reducing environment. Mineralogical and geochemical data from the Surma Basin suggest that the detrital input was specially intense during the Neogene probably because of tectonic uplift linked to the upheaval of the Himalayas. The result of the integrated petrographic techniques with major and trace-element analyses suggest that the source area of the detritus consisted of the granites - major constituents of Himalayan rocks. Clay mineral analysis indicates that major components of the rock studied are quartz and clay minerals together with small amounts of feldspar. The principal detrital clay minerals are illite, kaolinite, I/S, K/S mixed layers and chlorite. Clay mineral distribution provides the evidence on diagenesis and clue to the provenance. A clay mineral suite with abundant illite, I/S, K/S, chlorite, quartz and feldspar reflects physical weathering in the source area. Kaolinite reflects the composition of the soil under humid tropical conditions where chemical weathering predominates. The absence of smectite is remarkable, which is due to its diagenetic convertion to illite/smectite and kaolinite/smectite mixed layers. The existence in noticeable amounts of mixed layers I/S and K/S is attributed to the degree of burial diagenesis. TEM and SEM study shows different element concentration of illite and smectite and quartz overgrowth. Quantitative analysis also showed the barite was dominant from the Ba grains. SEM study also provides that Ba was associated with SiO2 and clay minerals A summary conclusion is given in the follwing table. 148

Table 15. Summary conclusion.

Target/Method Results Comments 1) Age Miocene On the basis of pollen analysis. 2) Depositional Shallow marine to brackish By sedimentary, palynological and environment geochemical studies. 3) Paleoecology and Marine transgression with subsidence in By palynological and geochemical paleogeography Miocene. studies. Changes in sea level. 4) Palynological zones Three zones demarcated. On the basis of pollen analysis from Z-1 (Palmepollenite), the samples of Fenchuganj well – 2. Z-2 (Tricolpate - trilete) Z-3 (Dissaccate) 5) SiO2/Al2O3 Dominance of the fining with a Grain size indicator. coarsening tendency at the bottom. 6) Maturity index Increasing maturity with fluctuations at Different matured and immatured M=Al2O3+K2O/ different depth intervals. zones of the 6 wells were demarcated. MgO+Na2O, Maturity increases with the decrease of silica content and grain size. K2O/Na2O and Rb/K2O 7) Tectonic discrimination Data of six wells fall into the ACM The ratios were useful for tectonic by using SiO2 and K2O/ (Active Continental Margin) category. discrimination Na2O 8) Th/U The higher values were fluctuating in all The higher value of Th/U ratio is the six well sequences. because of oxidation. The sequence represent different stages in oxidation, leaching and deposition under marine conditions. 9) Ba Barium enrichment High surface water productivity and diagenesis mobilizations. 10) XRD Major components are quartz and clay Burial diagenesis. mineral together with feldspar. Clay minerals are illite, kaolinite, I/S, K/S mixed layer and chlorite. 11) SEM Quartz overgrowth Diagenesis Dominance of barite and its associations Anoxic and sulphidic bottom with silica and clay minerals. conditions. 12) Provenance Continental origin, Granitic rocks of On the basis of mineralogical and Himalaya. geochemical studies. The methodology adopted in the present study by using geochemical ratios can be applicable to any sedimentary basin of the world to infer palaeoclimate, palaeotectonics and palaeoenvironment. 11 References

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Habiganj well – 1

Sample No Core Depth (m) Lithology *1 1 1255.47 (Top) Light colour, bluish grey, shale, hard and compact, fine grained 2 1 1256.38 (Bottom) '' (thinly laminated) 3 1 1256.38 (Top) '' (fragile) *4 1 1257.3 (Bottom) '' 5 1 1257.3 (Top) '' 6 1 1257.21 (Bottom) '' 7 1 1258.21 (Top) '' *8 1 1259.12 (Bottom) '' 9 2 1849.22 (Top) '' *10 2 1849.83 (Bottom) Bluish grey shale, hard and compact, thiny laminated 11 2 1849.83 (Top) Bluish grey, sandy shale, micro-cross lami- nation present, light coloured *12 2 1850.74 (Top) Bluish grey shale with silt partings 13 2 1851.66 (Bottom) Dark colour, bluish grey shale (sandy). Hard and compact *14 2 1851.66 (Top) Hard and compact, bluish grey shale (dark in colour) 15 2 1852.65 (Bottom) '' *16 3 3110.64 (Top) Dark grey sandy shale 17 3 3110.64 (Bottom) '' 18 3 3111.55 (Top) '' * marked samples were used for pollen analysis.

KailasTila well – 1

Sample No Core Depth (m) Lithology *20 2 1175.30 (Bottom) Light coloured, grey shale, fragile *21 2 1176.22 (Top) Light grey shale with massif sand 22 2 1177.80 (Bottom) Light grey sandy shale *23 5 2272.89 (Bottom) Dark colour, bluish shale hard and compact *24 6 2973.82 (Top) '' (with sand partings, light colour) *25 6 2974.52 (Bottom) '' *26 7 3730.14 (Top) Hard and compact sandy shale, light grey coloured *27 7 3731.24 (Bottom) '' *28 8 3967.89 (Top) Bluish grey, hard and compact, sandy shale *29 9 3968.54 (Bottom) Dark coloured, hard and compact, sandy shale *30 2 1081.73 (Top) Bluish grey shale 31 2 1082.64 (Bottom) '' *32 2 1082.64 (Top) '' * marked samples were used for pollen analysis. Rashidpur well – 1 (depth and lithology of studied samples)

Sample No Core Depth (m) Lithology *33 2 1083.64 (Bottom) '' with sand partings 34 2 1083.64 (Top) '' 35 2 1084.62 (Bottom) '' *36 2 1084.62 (Top) Light grey sandy shale 37 2 1085.64 (Bottom) '' 38 2 1085.64 (Top) '' *39 2 1086.30 (Bottom) '' 40 2 1086.30 (Top) '' 41 2 1087.40 (Bottom) '' *42 2 1087.40 (Top) '' 43 2 1087.63 (Bottom) '' *44 3 1248.16 (Top) '' 45 3 1248.93 (Bottom) Bluish grey shale 46 3 1248.93 (Top) '' *47 3 1249.68 (Bottom) Light grey shale 48 3 1250.6 (Bottom) Light colour shale *49 3 1250.6 (Top) 51 3 1251.6 (Bottom) '' 52 3 1251.6 (Top) '' *53 3 1252.42 (Bottom) '' (moderately hard) 54 3 1252.42 (Top) '' 55 3 1253.22 (Bottom) '' 56 3 1253.22 (Top) '' 57 3 1254.25 (Bottom) '' 58 4 1827.89 (Top) Light coloured sandy shale *59 4 1828.69 (Bottom) '' 60 4 1828.60 (Top) Light coloured bluish grey sandy shale 61 4 1829.22 (Bottom) '' 62 4 1830.42 (Top) Light coloured bluish grey sandy shale *63 4 1832.45 (Bottom) Light coloured bluish grey shale 64 5 2134.5 (Top) Light coloured sandy shale *65 5 2135.54 (Bottom) '' *66 6 2472.23 (Top) Dark coloured sandy shale (hard and com- pact) 67 6 2473.42 (Bottom) '' 68 6 2473.76 (Bottom) '' *69 7 2677.97 (Bottom) Bluish grey sandy shale *70 3 4268.72 (Well-2) '' * marked samples were used for pollen analysis. Atgram well – IX (depth and lithology of studied samples)

Sample No Core Depth (m) Lithology *71 1 3633.52 (Top) Hard and compact, dark col- oured shale 72 1 3633.95 (Bottom) '' 73 1 3635.35 (Top) '' 74 1 3636.22 (Bottom) '' 75 1 3637.42 (Top) '' 76 1 3638.00 (Bottom) '' 77 1 3639.20 (Top) '' *78 1 3640.10 (Bottom) '' 79 2 3637.42 (Top) Hard and compact, dark col- oured sandy shale *80 2 3638.02 (Bottom) Light coloured sandy shale, hard and compact *81 3 3990.74 (Top) Medium grained sandstone *82 4 4729.15 (Top) Dark coloured, hard and compact shale 83 4 4733.85 (Bottom) '' 84 4 4733.85 (Top) '' *85 4 4735.41 (Bottom) '' * marked samples were used for pollen analysis. Fenchuganj well – 2 (depth and lithology of studied samples)

Sample No Core Depth interval (m) Lithology *86 4 2190-2200 (Top) Bluish grey shale with sand partings 87 4 2130-2200 (Bottom) '' 88 4 2190-2200 (Top) Bluish grey shale *89 4 2190-2200 (Bottom) Bluish grey sandy shale *90 7 3137-3143 (Top) Bluish grey shale 91 7 3137-3143 (Bottom) '' 92 7 3137-3143 (Top) '' *93 7 3137-3143 (Bottom) '' *94 8 3259.96–3269,55 (Top) '' 95 8 '' (Bottom) '' 96 8 '' (Top) '' *97 8 '' (Bottom) '' *98 10 3624-3615 (Top) Bluish grey sandy shale *99 10 3624-3615 (Bottom) Bluish grey, hard and compact shale 100 11 3730-3379 (Top) '' 101 11 '' (Bottom) '' (with sand partings) *102 11 3730-3779 (Top) Bluish grey shale, hard and compact 103 11 ''(Bottom) '' (with sand partings) *104 11 3770-3779 (Bottom) '' 105 11 '' (Top) '' 106 11 3770-3779 (Bottom) Bluish grey shale, hard and compact *107 12 4086-4095 (Top) '' 108 12 '' (Bottom) '' (with sand partings) *109 12 4089-4095.5 (Top) Bluish grey shale, hard and compact 110 12 '' (Bottom) '' 111 12 4086-4095.5 (Top) '' *112 12 '' (Bottom) '' 113 12 4086-4095.5 (Top) '' *114 12 '' (Bottom) '' * marked samples were used for pollen analysis.

Patharia well – 5 (depth and lithology of studied samples)

Sample No Core Depth (m) Lithology *115 1 959 – 964 Hard and compact, dark grey shale 116 1 '' Hard and compact, bluish grey shale *117 2 1450.5 – 1457.3 Bluish grey compact shale 118 2 '' Light grey shale 119 2 '' Bluish grey shale, hard andcompact 120 2 '' '' *121 2 '' Bluish grey shale with sand partings 122 2 '' Bluish grey shale 123 2 '' Light grey shale with intercalation of sandstone 124 2 '' '' *125 2 '' Bluish grey shale * marked samples were used for pollen analysis. Sample No Core Depth interval (m) Lithology 126 2 '' Bluish grey shale with sand partings, hard lami- nated 127 2 '' Light grey sandy shale, hard and compact *128 2 '' Light grey shale 129 2 '' Light grey sandy shale, hard and compact 130 2 '' '' 131 3 1829–1837 Bluish grey shale, hard and compact 132 3 '' '' *133 3 '' Black shale, hard and compact 134 3 '' '' 135 3 '' '' 136 3 '' '' 137 3 '' '' 138 3 '' '' 139 3 '' '' *140 3 '' '' 141 3 '' '' 142 3 1829–1837 Black shale, hard and compact 143 3 '' '' 144 3 '' '' 145 3 '' '' *146 3 '' '' 147 4 2290.5–2307.25 Bluish grey shale, hard and compact *148 4 '' '' 149 4 '' Bluish grey shale, thin partings of sandstone, hard and laminated 150 4 '' '' 151 4 '' '' 152 4 '' '' *153 4 '' '' 154 4 '' '' *155 4 '' Bluish grey shale, thin partings of sandstone, hard and laminated 156 4 '' '' 157 4 '' Bluish grey massive shale with and, *158 4 '' '' 159 4 '' Light grey shale with sand, hard and compact *160 4 '' Black shale with thin partings of sand *161 5 2828.75–2834.84 Blackish grey shale, very hard and compact *162 5 '' '' 163 5 '' Bluish grey shale with silt partings, hard and compact 164 5 '' '' 165 5 '' '' *166 5 '' '' 167 5 '' Black shale, hard and compact 168 5 '' '' 169 5 '' '' *170 5 '' '' Sample No Core Depth interval (m) Lithology 171 6 3160.7–3168.25 Dark black shale, very hard and compact 172 6 '' '' 173 6 '' '' 174 6 '' '' 175 6 '' '' 176 6 '' '' *177 6 '' '' 178 6 '' '' *179 6 '' Bluish grey shale, thin layer of sand, hard and compact 180 6 '' '' 181 6 '' '' 182 6 '' Bluish grey shale, thin layer of sand, hard and compact *183 6 '' Black shale, hard and compact 184 6 '' '' 185 6 '' '' 186 6 '' '' 187 6 '' '' *188 6 '' '' * marked samples were used for pollen analysis. Appendix 2 Major and minor trace elements of the core samples

12345678 wt% SiO2 61.63 61.86 61.76 61.52 61.22 60.94 61.20 0.90 TiO2 0.87 0.86 0.86 0.85 0.85 0.86 0.86 0.85 A12O3 16.34 16.25 16.05 15.80 16.30 16.74 16.81 16.23 Fe2O3 6.95 7.11 7.14 7.24 7.17 7.19 7.11 7.50 MnO 0.09 0.10 0.10 0.11 0.10 0.10 0.09 0.11 MgO 3.01 3.41 3.02 3.01 3.04 3.05 3.04 3.06 CaO 1.93 2.02 2.10 2.07 1.98 1.93 1.83 2.03 Na2O 1.57 1.58 1.56 1.54 1.54 1.56 1.58 1.54 K2O 3.25 3.24 3.22 3.16 3.26 3.35 3.35 3.25 P2O5 0.16 0.16 0.16 0.16 0.16 0.15 0.15 0.17 S 0.15 0.19 0.16 0.17 0.18 0.16 0.22 0.28 F 0.07 0.07 0.06 0.07 0.07 0.07 0.07 0.07 LOI* 2.73 5.59 5.67 5.62 5.64 5.69 5.49 5.59 Total 98.96 102.27 102.09 101.54 101.76 102.04 101.87 101.82 ppm Ba 480 468 476 472 485 488 487 497 Ce 82 87 85 87 95 94 84 84 Cl 197 228 210 210 216 247 241 240 Co*2425252223302223 Cr * 119 120 122 120 121 125 120 123 Cu*2727262627293028 Dy134245121 Er12629131077 Gd648263-212 Hf43404363 La 37 41 38 38 36 39 42 45 Nb 21 19 19 19 21 21 22 21 Nd 41 40 39 38 45 14 42 41 Ni*6462606061656661 Pb*2528232321262726 Pr 40 36 41 39 48 36 37 35 Rb 199 197 198 190 204 210 210 203 Sc 14 15 14 12 16 15 14 15 Sr 170 173 174 170 176 176 176 178 Th 31 28 28 28 29 28 29 30 U24012132 V 127 129 128 123 129 129 130 129 Zn*9695939494989796 Zr 224 227 233 228 233 221 220 232 * Marked elements have been measured by AAS rest of the elements by XRF #Sample1–8:Habiganjwell-1 9 10111213141516 wt% SiO2 59.73 58.56 55.41 61.51 65.26 58.96 59.55 58.73 TiO2 0.91 0.88 0.55 0.88 0.85 0.90 0.94 0.90 A12O3 17.61 17.93 9.02 16.73 15.40 17.61 17.99 18.15 Fe2O3 7.47 7.58 4.78 7.31 6.56 7.87 7.62 7.82 MnO 0.11 0.11 0.82 0.12 0.07 0.13 0.13 0.13 MgO 3.23 3.31 2.01 3.15 2.84 3.33 3.24 3.38 CaO 1.90 2.29 14.79 1.86 1.01 2.06 1.57 1.81 Na2O 1.46 1.42 1.29 1.53 1.47 1.43 1.45 1.44 K2O 3.54 3.68 2.11 3.35 3.13 3.55 3.57 3.66 P2O5 0.15 0.15 0.16 0.16 0.13 0.16 0.14 0.15 S 0.07 0.03 0.01 0.03 0.30 0.02 0.02 0.01 F 0.07 0.07 0.08 0.07 0.07 0.07 0.07 0.07 LOI* 5.94 6.42 12.78 15.70 4.12 6.22 5.85 6.14 Total 102.47 101.69 103.96 112.64 101.40 102.56 102.38 102.58 ppm Ba 719 541 388 519 472 530 543 537 Ce102966090939410291 Cl 406 404 149 397 96 348 368 415 Co*2827282727362824 Cr * 128 127 74 117 118 125 127 128 Cu*4140163925404742 Dy1062-0-1525 Er81210668144 Gd610439467 Hf142626-0553 La44426 1021464543 Nb 22 22 1 4 15 21 21 21 Nd 45 42 44 42 27 41 45 39 Ni*6972222235656468 Pb*3230454215302332 Pr 44 45 69 72 47 34 30 39 Rb 216 229 140 198 186 218 217 225 Sc16159 1513141717 Sr 171 170 271 162 143 169 165 167 Th 32 31 26 29 25 33 29 30 U31-523233 V 140 142 65 131 115 139 143 142 Zn* 199 192 57 96 89 102 106 101 Zr 229 212 245 236 304 226 230 213 * Marked elements have been measured by AAS rest of the elements by XRF. # Sample 9–16: Habiganj well-1 17 18 19 20 22 23 24 25 wt% SiO2 67.43 64.62 66.49 60.00 67.84 60.60 58.18 63.89 TiO2 0.78 0.83 0.81 0.92 0.76 0.92 0.95 0.85 A12O3 14.14 14.88 14.67 19.09 16.21 17.51 17.34 15.71 Fe2O3 5.96 6.39 6.22 7.89 5.79 7.92 8.32 7.09 MnO 0.08 0.12 0.07 0.14 0.06 0.08 0.12 0.09 MgO 2.58 2.74 2.64 1.91 1.99 3.28 3.36 3.31 CaO 1.27 2.07 1.00 0.93 0.78 2.44 1.89 1.44 Na2O 1.45 1.44 1.44 0.61 0.89 1.33 1.23 1.35 K2O 2.88 3.05 2.98 2.60 2.23 3.81 3.48 3.16 P2O5 0.13 0.13 0.13 0.05 0.04 0.16 0.17 0.15 S 0.28 0.27 0.30 0.02 0.08 0.11 0.04 0.25 F 0.06 0.07 0.06 0.05 0.05 0.07 0.08 0.07 LOI* 3.97 4.83 3.89 6.82 4.98 6.00 5.67 5.06 Total 101.18 101.64 100.88 101.27 101.89 103.51 100.66 102.42 ppm Ba 440 466 462 562 440 495 554 513 Ce 88 99 97 92 90 89 115 97 Cl 51 73 64 89 108 43 117 75 Co*3024262552202040 Cr * 104 113 109 151 106 123 147 117 Cu*2223232846443835 Dy147644153 Er137181412214 Gd72501785 Hf67659747 La 44 47 50 49 39 45 52 49 Nb 19 21 20 18 14 18 20 16 Nd 43 45 41 39 36 34 41 36 Ni*56606272101648074 Pb*2423224324222424 Pr 28 30 40 21 19 24 43 27 Rb 164 183 172 222 148 179 231 186 Sc 12 12 10 19 14 17 19 15 Sr 146 161 141 161 143 176 182 154 Th 22 25 26 42 28 23 35 23 U31134212 V 98 111 103 140 116 142 156 125 Zn* 82 78 80 261 88 92 96 99 Zr 310 322 333 256 271 223 249 215 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 17-19: Habiganj well-1, sample 20–25: Kailas Tila-1 well 26 27 28 29 30 31 32 33 wt% SiO2 64.40 67.25 59.04 63.14 62.83 62.81 62.42 63.53 TiO2 0.61 0.64 1.00 0.93 0.87 0.87 0.87 0.86 A12O3 10.94 11.04 18.47 16.49 15.57 14.85 15.66 14.62 Fe2O3 4.47 4.81 8.08 7.36 6.77 6.97 6.67 7.06 MnO 0.08 0.07 0.09 0.09 0.11 0.11 0.11 0.12 MgO3.923.893.162.893.173.343.133.11 CaO5.484.200.670.822.572.572.462.84 Na2O1.381.461.411.521.291.241.271.34 K2O2.512.583.573.153.022.942.982.75 P2O5 0.14 0.13 0.14 0.16 0.16 0.15 0.14 0.18 S 0.010.020.030.050.100.350.130.09 F 0.060.070.070.060.060.050.060.06 LOI* 7.12 6.04 5.15 4.44 5.76 5.22 6.02 6.05 Total 101.22 102.37 100.14 101.32 102.48 101.66 102.14 102.81 ppm Ba 423 439 464 501 552 474 513 450 Ce 82 78 103 99 101 96 108 99 Cl1528373401291127172 Co*2752352229272728 Cr * 72 75 137 118 136 129 137 138 Cu*1724443637383838 Dy31-051764 Er 12 -2 16 10 7 9 4 5 Gd110311055 Hf57865849 La 35 35 48 47 43 36 42 48 Nb 12 12 19 18 22 21 22 21 Nd 33 33 41 38 42 46 48 42 Ni*3541896584748284 Pb*1516272528232422 Pr 20 20 32 17 40 46 44 38 Rb 132 129 230 118 169 161 171 151 Sc 10 11 19 14 13 14 14 15.9 Sr 188 140 172 159 175 167 182 183 Th 18 19 23 24 25 29 30 28 U24132201 V 69 74 156 127 122 116 122 114 Zn 54 103 103 92 88 87 91 87 Zr 355 307 251 276 286 311 319 324 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 26 – 29 Kailas Tila-1 well, Sample 30 – 33 Rashidpur well-1 34 35 36 37 38 39 40 41 wt% SiO2 61.38 61.65 58.76 64.11 62.63 63.53 63.88 62.62 TiO2 0.86 0.87 0.76 0.88 0.87 0.87 0.89 0.87 A12O3 15.57 15.26 14.92 15.18 15.22 15.47 15.01 16.28 Fe2O3 6.65 7.09 6.97 6.91 6.94 6.39 6.77 7.03 MnO0.120.100.150.100.110.090.100.10 MgO3.233.093.083.113.453.083.133.30 CaO3.472.425.152.082.401.962.391.83 Na2O1.311.271.291.471.311.361.371.31 K2O2.912.862.803.302.862.942.803.04 P2O5 0.15 0.15 0.14 0.14 0.14 0.14 0.15 0.14 S 0.080.480.320.210.100.090.110.08 F 0.060.050.120.060.060.050.060.048 LOI* 6.73 5.54 6.53 5.09 5.98 5.46 5.66 5.73 Total 102.74 102.04 102.23 102.53 102.33 102.19 102.55 102.59 ppm Ba 481 479 504 490 462 482 484 506 Ce914711995939710094 Cl 79 90 77 88 80 77 77 74 Co*3323352829263131 Cr * 138 128 119 120 140 133 131 136 Cu*403834404393940 Dy221962048 Er019457137 Gd0612-686612 Hf63881665 La 41 43 58 42 41 46 44 40 Nb 22 21 20 20 -17 21 21 22 Nd 43 43 53 40 21 41 45 40 Ni*8873697344757681 Pb*2324212248242426 Pr 40 34 48 36 40 12 42 40 Rb 165 158 159 162 154 162 155 168 Sc 11 13 16 12 14 15 14 14 Sr 190 174 288 155 173 167 172 167 Th 29 29 29 26 -2 27 25 25 U034412624 V 121 119 118 111 119 120 116 130 Zn*9085819061928892 Zr 299 310 275 284 285 315 144 271 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 34–41: Rashidpur well-1 42 43 44 45 46 47 48 49 wt% SiO2 63.22 62.45 63.97 62.81 63.66 63.95 63.30 62.54 TiO2 0.83 0.83 0.84 0.81 0.85 0.82 0.84 0.86 A12O3 14.30 15.47 15.82 14.71 15.75 15.70 15.66 16.08 Fe2O3 6.74 6.88 6.54 8.15 6.75 6.47 6.91 7.12 MnO0.110.100.100.130.100.090.100.11 MgO3.473.282.802.849.812.752.452.89 CaO3.192.461.912.121.881.861.971.93 Na2O 1.36 1.36 1.241 1.57 1.63 1.54 1.58 1.58 K2O2.912.973.162.983.123.173.123.18 P2O5 0.15 0.16 0.17 0.21 0.17 0.16 0.18 0.18 S 0.125 0.09 0.122 0.11 0.13 0.12 0.14 0.13 F 0.063 0.07 0.07 0.06 0.06 0.06 0.07 0.06 LOI* 6.26 5.97 4.99 5.76 5.08 4.96 5.21 5.43 Total 102.92 102.33 102.32 102.17 101.94 102.13 102.29 101.85 ppm Ba 468 898 469 466 472 476 466 484 Ce 93 85 81 96 86 87 91 91 Cl 82 91 84 90 105 83 83 98 Co*5734264125163643 Cr * 124 126 103 106 103 102 110 111 Cu*353628252972730 Dy23357936 Er823686120 Gd2 146-13 12101 Hf45644362 La 40 41 43 48 40 40 43 42 Nb 39 21 21 20 21 21 21 22 Nd 20 41 37 44 40 40 40 43 Ni*7877514852365555 Pb*2323262227272627 Pr 30 34 28 46 26 31 40 39 Rb 158 162 180 177 182 185 187 190 Sc 13 14 12 14 12 11 12 13 Sr 169 176 175 181 182 178 176 184 Th 30 25 25 26 26 24 27 27 U11432211 V 110 120 112 112 119 111 117 128 Z* 83 87 91 84 91 92 94 93 Zr 305 273 244 288 244 245 248 258 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 42–49: Rashidpur well-1 50 51 52 53 54 55 56 57 wt% SiO2 63.39 62.97 63.48 62.078 63.21 63.58 61.34 62.45 TiO2 0.84 0.83 0.84 0.85 0.83 0.85 0.87 0.85 A12O3 15.91 15.35 15.52 16.33 16.67 15.33 17.72 16.19 Fe2O3 6.45 7.17 6.63 6.95 6.28 6.79 7.13 7.06 MnO 0.09 0.11 0.10 0.10 0.09 0.10 0.11 0.11 MgO2.802.852.872.912.762.813.022.88 CaO1.912.092.181.901.712.141.601.85 Na2O1.601.561.561.561.691.561.601.57 K2O3.193.073.133.293.323.033.593.26 P2O5 0.16 0.18 0.17 0.17 0.15 0.18 0.16 0.17 S 0.120.120.130.120.070.160.080.09 F 0.070.060.080.070.060.060.070.07 LOI* 5.13 5.55 5.35 5.43 5.08 5.24 5.51 5.37 Total 101.85 102.40 102.50 101.95 102.14 102.01 103 102.14 ppm Ba 479 475 463 496 498 471 515 484 Ce87881039397938290 Cl 51 46 65 70 74 67 77 84 Co*3124242164362424 Cr * 107 110 110 109 101 109 108 109 Cu*2425252832283530 Dy40302433 Er10-139810137 Gd25048296 Hf36744421 La 43 40 45 42 33 36 52 44 Nb -17 -18 -19 -18 21 21 22 21 Nd 21 20 21 21 40 37 38 42 Ni*3843444352545554 Pb*5254555421182420 Pr 22 20 23 21 41 41 35 41 Rb 191 182 184 202 192 179 213 194 Sc 13 14 14 13 13 11 15 12 Sr 180 178 171 181 183 179 179 183 Th 30 28 28 29 28 26 28 29 U34221214 V 121 117 117 126 122 119 131 123 Zn*9188919496899994 Zr 248 258 273 242 243 268 208 245 * Marked elements have been measured by AAS, rest of the elements by XRF # Sample 50–57: Rashidpur well-1 58 59 60 61 62 63 64 65 wt% SiO2 60.82 62.56 60.02 59.85 61.57 62.33 65.44 66.30 TiO2 0.89 0.88 0.91 0.91 0.92 0.88 0.82 0.79 A12O3 17.03 16.71 18.12 18.01 16.84 16.73 13.84 13.19 Fe2O3 7.77 6.90 7.82 7.85 7.61 7.31 6.05 5.66 MnO0.120.100.120.120.120.110.070.07 MgO3.132.993.263.263.023.012.832.74 CaO1.481.451.281.291.501.372.712.76 Na2O1.461.521.451.451.491.501.541.54 K2O3.313.233.503.483.263.252.922.78 P2O5 0.17 0.15 0.17 0.15 0.16 0.15 0.12 0.12 S 0.040.060.020.050.030.020.150.05 F 0.590.060.070.060.060.060.060.07 LOI* 5.62 5.23 5.77 5.82 5.34 5.29 5.33 5.20 Total 102.14 102.04 102.7 102.19 102.21 102.18 102.06 101.44 ppm Ba 511 495 518 517 513 495 456 551 Ce 99 90 99 94 93 96 92 95 Cl 78 65 71 53 83 64 78 73 Co*35262227383111341 Cr * 133 128 137 136 133 131 109 104 Cu*3636404036342625 Dy61194046-4 Er46121215131 Gd21683587-0 Hf44422366 La 46 45 41 41 44 54 37 38 Nb 21 16 22 22 22 21 21 19 Nd 41 44 45 45 43 33 40 42 Ni*7068717464665352 Pb*1819212221211617 Pr 45 24 39 45 42 39 39 38 Rb 204 190 214 216 199 194 171 148 Sc 14 15 17 16 16 14 12 10 Sr 181 174 178 178 174 173 154 138 Th 31 30 30 28 28 25 28 20 U31201131 V 133 127 143 142 127 132 105 94 Zn*999510310294938078 Zr 264 247 222 226 269 275 329 324 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 58 – 65: Rashidpur well-1 66 67 68 69 71 72 74 75 wt% SiO2 62.05 65.41 61.69 59.43 65.61 65.05 66.69 62.04 TiO2 0.91 0.86 0.93 0.93 0.79 0.79 0.78 0.84 A12O3 16.95 15.51 17.54 17.34 16.12 16.23 15.61 17.38 Fe2O3 7.11 6.56 7.39 7.34 6.71 6.95 6.44 7.68 MnO0.090.090.090.170.100.100.090.12 MgO2.852.622.962.902.722.772.662.93 CaO1.161.221.172.741.021.011.010.93 Na2O1.411.441.411.391.291.271.291.25 K2O3.293.073.423.623.473.533.393.70 P2O5 0.13 0.14 0.13 0.14 0.15 0.15 0.14 0.16 S 0.020.020.020.020.020.050.020.03 F 0.060.060.060.070.070.070.070.07 LOI* 5.22 4.68 5.38 6.36 4.58 4.61 4.40 5.10 Total 101.46 101.878 102.21 102.69 102.84 102.78 102.76 102.44 ppm Ba 481 462 482 527 534 533 519 582 Ce 103 101 95 103 95 89 76 99 Cl 49 55 55 52 29 46 32 33 Co*2552272734284655 Cr * 130 120 137 130 19 97 89 111 Cu*3327343736363349 Dy48219675 Er11191277916 Gd5-3-156955 Hf44145567 La 48 42 45 43 14 43 49 47 Nb 22 21 21 23 15 16 15 16 Nd 46 39 44 43 38 36 36 43 Ni*7064746151553860 Pb*2724252925262630 Pr 44 40 40 45 17 25 12 22 Rb 187 176 208 227 189 192 183 217 Sc 14 14 15 16 14 17 15 19 Sr 154 157 172 182 108 108 105 122 Th 26 27 29 31 19 22 19 26 U11215544 V 133 119 140 137 116 122 112 135 Z* 94 86 97 98 86 91 86 97 Zr 268 292 254 248 232 229 235 230 *Marked elements have been measured by AAS rest of the elements by XRF. # Sample 66 – 69: Rashipur well - 1, Sample 71 – 75: Atgram well-IX 76 77 78 79 83 84 85 86 wt% SiO2 64.20 46.20 64.32 75.51 72.02 70.22 89.40 71.30 TiO2 0.82 0.80 0.80 0.55 0.78 0.89 0.28 0.77 A12O3 16.37 16.47 16.68 7.76 12.87 13.77 4.71 13.28 MnO6.966.866.804.725.946.132.560.07 MgO0.110.100.090.170.090.060.022.42 CaO2.782.712.731.211.471.570.500.64 Na2O1.041.081.044.060.330.260.381.58 K2O1.271.261.241.090.930.960.492.66 P2O5 3.53 3.48 3.54 1.73 2.56 2.94 0.87 0.13 S 0.140.150.140.090.170.130.070.03 F 0.050.030.020.330.350.250.880.05 LOI* 4.63 4.61 4.60 4.25 4.81 5.06 2.26 3.44 Total 102.17 102.00 102.28 101.65 102.57 102.83 102.49 101.96 ppm Ba 555 538 547 330 685 516 375 416 Ce 92 86 86 63 90 113 25 79 Cl 47 34 35 35 73 52 24 71 Co*27363946514931884 Cr * 101 95 95 59 63 81 14 95 Cu*363636213025723 Dy1152239-37 Er9 1370 -013-07 Gd122 11171478 1 Hf675981089 La 47 45 41 27 41 49 16 41 Nb 16 15 16 10 16 19 5 14 Nd 38 38 35 28 39 44 16 35 Ni*5352493036341750 Pb*282626111814313 Pr 23 23 32 12 17 22 -8 14 Rb 201 186 196 79 127 156 33 137 Sc 14 15 15 8 11 13 3 13 Sr 114 108 111 147 128 147 37 114 Th 22 19 24 14 18 22 -0 18 U14533245 V 124 117 118 50 88 113 38 89 Zn* 100 96 89 45 96 74 26 71 Zr 214 229 241 335 307 352 129 280 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 76 – 85: Atgram well - IX, Sample 86: Fenchuganj well-2 88 90 91 92 95 96 97 99 wt% SiO2 57.80 59.82 59.82 62.44 51.73 50.57 61.86 63.01 TiO2 0.58 0.89 0.89 0.83 0.90 0.94 0.71 0.93 A12O3 9.11 16.38 17.15 15.17 16.68 16.96 12.66 15.96 MnO0.670.080.080.070.070.080.060.08 MgO 1.73 3.5 3.86 3.65 5.63 5.84 4.51 2.89 CaO 13.56 1.87 1.91 2.13 4.59 4.93 4.20 0.50 Na2O1.181.251.241.351.181.161.351.63 K2O2.013.523.593.323.663.652.853.32 P2O5 0.13 0.12 0.13 0.13 0.12 0.05 0.12 0.13 S 0.230.080.060.040.040.050.120.03 F 0.080.080.090.090.090.060.070.07 LOI* 11.43 6.26 6.32 6.20 9.89 10.33 7.91 3.97 Total 103.30 101.58 102.65 102.01 102.56 102.86 102.26 100.12 ppm Ba 349 529 669 633 634 525 561 558 Ce 73 108 101 93 101 111 88 101 Cl 10 38 49 17 77 121 107 50 Co*2126265227244242 Cr * 83 126 128 109 138 172 99 126 Cu*1536382837412525 Dy1430103410 Er813029119-0 Gd201106678 Hf15455566 La 33 47 49 48 49 45 47 52 Nb 11 19 17 17 20 20 14 18 Nd 27 48 36 43 49 46 40 40 Ni*3667655271755454 Pb* 9 20 21 17 20 18 17 17 Pr 32 29 22 25 43 44 28 27 Rb 121 229 226 204 244 247 164 202 Sc 13 18 18 16 19 20 13 17 Sr 255 149 138 131 167 171 144 155 Th 29 33 32 27 41 41 30 27 U -4 3 4 3 -0 -0 1 1 V 69 126 131 112 140 144 91 124 Zn*4993998288908383 Zr 317 237 240 271 274 281 313 261 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 88–99: Fenchuganj well-2 100 103 104 105 108 109 110 111 wt% SiO2 57.81 67.44 59.73 58.57 60.49 65.50 70.29 67.92 TiO2 1.01 0.84 1.02 1.03 0.89 0.78 0.66 0.74 A12O3 17.90 14.44 17.92 18.07 16.74 14.70 12.69 12.69 MnO 0.08 .13 0.12 0.10 0.10 0.09 0.09 0.13 MgO3.212.593.243.213.192.892.252.63 CaO0.460.920.550.491.381.492.161.99 Na2O1.341.591.421.361.391.431.411.46 K2O3.382.663.313.373.443.022.612.65 P2O5 0.14 0.18 0.16 0.14 0.14 0.14 0.12 0.16 S 0.080.030.040.040.070.030.010.04 F 0.070.060.070.060.070.070.040.06 LOI* 5.08 3.98 5.05 5.13 5.48 4.94 4.50 4.92 Total 100.26 101.26 101.19 100.24 100.78 101.54 102.00 102.47 ppm Ba 539 477 522 545 535 490 427 446 Ce 100 90 107 95 101 90 80 85 Cl 12 33 18 26 50 51 30 24 Co*3328322628253127 Cr * 198 129 152 202 130 112 89 107 Cu*503349523832628 Dy113182433 Er4377114107 Gd-476103676 Hf48885586 La 48 44 49 50 51 45 35 46 Nb 20 14 19 20 18 15 12 14 Nd 46 40 42 43 42 39 40 39 Ni*9766889076604959 Pb*2315242623162321 Pr 38 32 26 30 30 15 11 21 Rb 246 153 223 236 213 170 139 141 Sc 19 15 19 19 17 15 11 15 Sr 194 164 170 181 161 136 172 155 Th 36 20 30 35 31 25 21 20 U-03333324 V 156 111 151 157 134 107 88 92 Zn* 108 90 106 108 119 87 86 86 Zr 263 240 243 253 284 225 249 257 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 100 – 111: Fenchuganj well-2 112 113 114 115 116 117 118 119 wt% SiO2 60.65 65.86 66.12 59.86 60.50 63.60 69.31 62.14 TiO2 0.88 0.78 0.78 0.92 0.91 0.85 0.74 0.89 A12O3 17.02 14.41 14.99 18.10 17.70 15.98 12.16 16.97 MnO0.082.902.770.120.120.060.090.06 MgO3.321.851.293.293.232.872.163.08 CaO1.431.451.411.031.241.062.531.07 Na2O1.352.962.961.451.471.551.691.60 K2O3.510.140.133.423.343.032.383.26 P2O5 0.13 0.03 0.04 0.15 0.14 0.11 0.12 0.11 S 0.040.050.040.040.040.040.160.03 F 0.075.024.670.060.070.060.040.07 LOI* 5.55 5.51 4.53 4.39 4.82 5.30 5.41 4.94 Total 101.42 102.05 102.21 100.68 101.70 101.75 101.99 101.43 ppm Ba 540 467 535 503 500 918 6808 614 Ce 93 99 91 95 95 94 18 86 Cl 34 89 42 111 81 85 166 111 Co* 125 104 115 25 55 43 36 32 Cr * 8 7 18 150 141 124 85 130 Cu*4231343716312330 Dy 6 6 -0 6 5 - 1 5 Er210-057169 Gd1 14189106 6 3 Hf75724526 La 49 41 42 45 44 40 33 40 Nb 17 15 14 22 21 20 18 22 Nd 41 33 36 41 43 37 10 37 Ni*7357656633563257 Pb*282226181219714 Pr 32 27 26 45 46 43 - 28 Rb 25 17 12 212 204 149 122 192 Sc 17 13 12 16 16 12 11 13 Sr 153 140 130 146 151 118 238 138 Th 30 23 20 28 29 17 17 27 U23324423 V 133 104 112 141 138 116 76 125 ZN* 109 86 98 92 56 91 78 80 Zr 251 266 228 236 240 258 249 277 * Marked elements have been measured by AAS rest of the elements by XRF # Samples 112 – 114: Fenchuganj well-2; Samples 115 – 119: Patharia well-5. 121 122 124 125 126 127 128 129 wt% SiO2 70.75 61.01 66.26 61.46 59.69 74.51 65.96 66.63 TiO2 0.57 0.85 0.83 0.83 0.94 0.54 0.054 0.76 A12O3 9.51 16.82 15.12 15.51 17.75 9.88 10.12 14.12 Fe2O3 5.04 7.01 6.41 8.41 7.90 4.44 5.83 6.01 MnO0.130.060.050.140.100.100.220.06 MgO1.992.992.712.993.051.592.112.39 CaO3.991.001.211.930.832.506.061.22 Na2O1.331.541.721.511.651.491.341.57 K2O1.913.152.882.993.362.022.102.73 P2O5 0.270.110.10.250.150.210.540.10 S 0.130.040.160.870.060.130.040.02 F 0.600.080.400.070.070.040.080.05 LOI* 5.41 4.94 1.02 4.63 4.53 3.74 3.85 4.11 Total 101.43 99.83 98.54 102.10 101.40 101.40 99.04 100.06 ppm Ba 1521 720 570 812 1398 486 455 753 Ce132898810684688595 Cl 197 121 111 90 303 92 103 125 Co*43276327256774109 Cr * 74 131 112 124 129 11 10 11 Cu*1628243328342024 Dy2112-0-112 Er2610-8-92 Gd39451555 Hf 60 37 46 35 40 4 4 5 Nb 16 20 20 20 22 14 15 20 Nd 66 38 40 51 36 32 38 41 Ni*3055405356553239 Pb*1125131120171112 Pr 27 46 25 44 29 21 31 49 Rb 96 155 155 178 202 18 30 25 Sc 10 16 12 14 16 8 10 13 Sr 276 110 128 180 168 160 288 142 Th 21 20 27 27 25 16 24 29 U244233- 1 V 67 123 107 125 137 61 76 104 Zn*4426385545795673 Zr 295 215 306 255 238 229 249 229 * Marked elements have been measured by AAS rest of the elements by XRF # Samples 121 – 129: Patharia well – 5. 130 131 132 133 134 135 136 137 wt% SiO2 73.69 71.55 65.60 62.61 67.02 62.28 62.26 63.44 TiO2 0.51 0.65 0.79 0.87 0.75 0.86 0.87 0.84 A12O3 9.44 12.42 15.08 16.83 14.24 16.60 16.85 16.07 Fe2O3 3.80 5.00 6.47 6.79 6.05 7.09 6.78 6.92 MnO0.110.070.070.070.060.080.070.08 MgO1.442.292.803.042.643.133.043.03 CaO3.811.301.331.331.331.411.361.52 Na2O1.551.771.771.681.761.661.681.67 K2O1.992.532.943.272.843.263.273.17 P2O5 0.89 0.11 0.13 0.13 0.12 0.12 0.13 0.14 S 0.010.000.000.000.010.020.000.07 F 0.050.060.060.000.060.070.070.07 LOI* 4.45 3.69 4.38 4.85 4.13 4.93 5.81 4.87 Total 101.11 101.66 101.25 101.92 101.20 101.71 101.75 102.03 ppm Ba 843 964 465 479 466 478 481 496 Ce 59 50 68 92 76 95 100 96 Cl 106 59 122 68 153 68 64 54 Co* 144 95 33 28 32 26 39 41 Cr *607810511925117114113 Cu*1221283931384036 Dy147300134 Er15267974 Gd03843353 Hf77552646 La 28 34 34 48 36 42 43 20 Nb 14 17 20 21 19 21 21 42 Nd 29 23 33 41 36 45 42 64 Ni* 9 12 13 18 16 20 19 19 Pr 17 18 20 38 32 42 41 32 Rb 96 123 158 188 149 191 193 24 Sc 7 8 11 12 11 13 14 14 Sr 192 113 126 144 124 148 150 145 Th 19 13 20 26 22 27 29 26 U-12333433 V 568310012093120121116 Zn*507280988610210094 Zr 238 217 246 248 245 250 258 253 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 130 – 137: Patharia well-5 138 139 140 141 142 143 144 145 wt% SiO2 62.76 62.37 60.75 62.53 61.05 61.77 61.42 60.75 TiO2 0.84 0.87 0.87 0.85 0.87 0.85 0.07 0.87 A12O3 16.23 16.74 16.87 16.54 17.06 16.52 17.87 17.11 Fe2O3 6.95 6.87 7.41 6.55 7.30 6.98 7.36 7.31 MnO0.080.080.090.090.080.100.090.10 MgO3.053.063.133.003.163.083.193.24 CaO1.381.441.471.511.421.651.411.52 Na2O 1.67 1.66 1.59 1.6 1.61 1.62 1.62 1.56 K2O3.193.313.343.263.353.283.383.45 P2O5 0.14 0.14 0.16 .0.14 0.14 0.15 0.15 0.15 S 0.020.010.040.010.020.030.020.04 F 0.060.070.060.060.070.060.070.06 LOI* 4.76 4.98 5.19 5.05 5.09 5.04 5.11 5.26 Total 102.33 103.79 101.18 101.43 102.22 101.29 101.99 101.62 ppm Ba 488 473 554 521 493 487 488 506 Ce 96 85 95 95 91 96 93 97 Cl 61 60 58 51 49 52 53 46 Co*3049312834352629 Cr * 114 118 126 114 124 118 121 126 Cu*4141423961464243 Dy298110-381 Er051010374 Gd15-01448- Hf34344214 La 43 41 42 41 48 38 44 46 Nb 21 21 22 22 - - - 22 Nd 41 40 39 46 41 43 40 44 Ni*6565686369676870 Pb*1818231822182118 Pr 36 33 47 46 37 35 37 35 Rb 186 195 204 184 197 190 199 207 Sc 14 14 12 13 16 16 13 14 Sr 151 151 155 147 150 151 150 152 Th 29 27 30 26 28 27 27 30 U42311333 V 116 120 127 120 124 121 124 128 Zn*10010099949798102101 Zr 261 248 252 245 239 242 238 138 * Marked elements have been measured by AAS rest of the elements by XRF # Samples 138 – 145: Patharia well–5 146 147 148 149 150 151 152 154 wt% SiO2 61.01 58.84 57.93 59.90 60.63 61.00 61.56 76.22 TiO2 0.86 0.98 0.99 0.96 0.99 0.94 0.77 0.60 A12O3 16.61 18.53 19.38 17.00 18.17 17.74 17.24 10.22 Fe2O3 7.11 8.21 8.47 7.95 7.90 8.05 7.47 3.93 MnO 0.10 0.11 0.11 0.11 0.10 0.09 0.09 0.05 MgO3.103.183.283.113.103.202.941.47 CaO1.570.510.470.530.550.520.540.70 Na2O1.601.511.461.561.571.581.611.73 K2O3.333.363.543.203.293.231.131.95 P2O5 0.15 0.13 0.13 0.14 0.14 0.14 0.13 0.12 S 0.040.030.020.030.040.060.080.04 F 0.070.060.050.060.070.050.060.04 LOI* 5.09 5.06 5.39 5.03 4.89 4.75 4.56 2.40 Total 100.85 100.76 101.45 100.58 101.63 101.63 100.64 100.05 ppm Ba 506 559 536 522 560 564 706 462 Ce102102999387948884 Cl 88 147 150 130 143 208 176 228 Co*3030253436393736 Cr * 128 164 171 157 139 159 154 119 Cu*4350495148502118 Dy665-26020 Er5750.2131284 Gd1.63.4254936 Hf25416735 La 46 42 42 40 42 46 41 33 Nb 22 22 22 22 22 22 22 18 Nd 42 47 44 42 42 43 41 39 Ni* 52 104 96 109 106 106 72 64 Pb*1720283126222718 Pr 47 48 49 47 35 421 35 30 Rb 200 213 231 185 204 199 199 125 Sc 14 17 18 16 18 17 14 11 Sr 154 171 176 156 170 167 173 -31 Th 29 29 31 23 -1 -0.2 3 138 U22312203 V 122 150 164 142 146 143 136 97 Zn* 102 113 129 133 120 118 127 103 Zr 244 115 242 201 251 113 113 82 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 146 – 154: Patharia well–5 155 156 157 158 159 160 161 162 wt% SiO2 60.38 71.77 69.07 74.55 55.32 63.01 67.14 64.86 TiO2 0.94 0.74 0.68 0.62 0.59 0.93 0.78 0.85 A12O3 17.52 12.38 13.10 11.24 6.12 15.48 13.24 15.50 Fe2O3 8.19 5.51 5.91 4.89 3.03 8.29 6.11 6.60 MnO0.060.060.050.040.640.060.180.07 MgO3.172.182.161.731.103.102.222.75 CaO0.470.760.610.6518.730.802.541.17 Na2O1.651.781.791.811.141.641.781.59 K2O3.222.302.392.071.182.902.442.10 P2O5 0.11 0.14 0.11 0.11 0.09 0.12 0.18 0.13 S 0.250.130.410.530.010.480.040.03 F 4.703.223.282.8714.884.415.210.06 Total 100.96 101.19 99.84 101.38 103.07 101.62 102.07 101.87 ppm Ba 693 641 601 412 836 275 624 476 Ce 54 94 67 61 69 63 103 97 Cl 150 313 235 229 261 119 273 106 Co* 68 31 120 40 121 122 48 34 Cr * 83 158 104 111 85 140 159 117 Cu*1134222720113442 Dy31641200 Er1123419711 Gd524551544 Hf537564103 La 32 44 36 33 33 22 48 40 Nb 15 22 17 17 15 15 21 21 Nd 30 43 35 32 30 30 49 39 Ni* 42 101 74 75 71 28 75 83 Pb*162315131541726 Pr 17 42 21 34 24 46 43 39 Rb 87 199 113 122 92 63 161 171 Sc6 179108 121313 Sr 135 162 133 145 128 338 146 135 Th 14 26 16 18 13 38 32 26 U30314-642 V 63 142 85 87 65 54 126 115 Zn* 64 116 85 84 95 36 102 102 Zr 227 258 265 229 229 495 538 296 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 155 – 162: Patharia well–5 163 164 165 166 167 169 169 170 wt% SiO2 61.46 59.39 64.10 60.86 59.19 62.63 62.17 64.57 TiO2 0.90 0.98 0.86 0.91 0.99 0.85 0.90 0.87 A12O3 17.52 18.48 15.89 17.79 18.55 15.49 16.90 15.52 Fe2O3 7.54 8.29 7.03 7.76 8.34 7.05 7.40 7.09 MnO0.100.110.120.100.100.190.090.12 MgO2.943.212.682.103.212.652.892.84 CaO0.800.781.310.800.892.080.871.21 Na2O1.721.661.731.711.631.731.711.77 K2O3.333.563.013.393.572.953.182.92 P2O5 0.16 0.15 0.17 0.16 0.21 0.18 0.16 0.18 S 0.030.020.020.020.040.030.040.06 F 0.070.070.060.070.070.070.060.06 LOI* 4.68 5.12 4.67 4.78 4.99 5.03 4.53 4.43 Total 101.43 102.04 101.87 101.52 101.85 101.11 101.1 101.59 ppm Ba 523 535 521 605 563 493 521 494 Ce 85 94 94 98 100 80 94 92 Cl 102 184 141 128 139 94 106 143 Co*2039423636404042 Cr * 125 135 117 126 136 117 124 114 Cu*3844353953384328 Dy4523612-1 Er2612119065 Gd244741616 La 44 40 42 43 44 43 38 41 Nb 21 23 21 22 24 20 22 21 Nd 42 42 44 38 42 40 40 40 Ni*7478707391738185 Pb*2730262632202020 Pr 38 43 36 37 38 34 37 34 Rb 194 220 174 208 222 164 188 167 Sc 16 17 13 17 15 13 14 13 Sr 148 156 161 156 158 158 169 153 Th 26 29 27 29 29 23 25 24 U32235423 V 130 142 115 134 146 113 126 114 ZN*93979793121107112123 Zr 230 231 276 230 247 245 244 251 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 163 – 170: Patharia well – 5 171 172 173 174 175 177 178 180 wt% SiO2 59.45 61.51 65.62 66.75 72.38 65.46 72.62 59.28 TiO2 0.94 0.94 0.72 0.89 0.67 0.85 0.71 0.92 A12O3 18.21 17.42 13.06 14.92 12.13 15.81 11.51 18.35 Fe2O3 7.47 7.36 5.43 6.22 5.13 6.63 4.71 7.76 MnO0.070.080.270.070.060.070.050.08 MgO3.163.102.182.592.082.791.943.35 CaO0.891.014.320.980.920.841.720.81 Na2O1.631.741.721.791.851.811.871.64 K2O3.583.442.452.802.153.082.063.14 P2O5 0.24 0.12 0.12 0.13 0.12 0.13 0.13 0.12 S 0.070.060.060.070.060.050.080.10 F 0.080.060.060.060.060.050.080.07 LOI* 4.63 5.83 1.79 3.80 2.83 3.77 3.36 1.79 Total 00.65 103.08 98.00 101.52 100.69 101.58 101.30 98.81 ppm Ba 647 2091 591 713 610 695 3026 2688 Ce 104 80 71 95 65 80 48 68 Cl 119 402 114 222 185 210 311 447 Co*3629597552965545 Cr * 142 136 97 127 91 127 89 139 Cu*4334233221311946 Dy2127071-1 Gd1748260113 Hf48767522 La 48 43 34 39 34 39 35 46 Nb 22 22 18 20 17 18 15 22 Nd 48 30 38 42 33 35 23 27 Ni*8676597255684688 Pb*1923172215231129 Pr 48 30 33 35 27 31 5 18 Rb 209 200 139 153 122 171 99 220 Sc 17 16 12 11 8 11 9 18 Sr 165 181 239 152 127 150 181 184 Th 27 26 23 24 14 21 16 24 U33132132 V 139 131 92 113 77 114 75 140 Zn* 118 94 90 81 70 88 67 104 Zr 254 290 278 347 248 279 296 245 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 171 – 180: Patharia well – 5

181 183 184 185 186 187 188 wt% SiO2 66.27 60.81 62.17 68.44 63.55 58.73 64.64 TiO2 0.84 0.91 0.88 0.77 0.88 0.95 0.82 A12O3 15.21 17.90 17.18 13.71 16.44 18.51 15.56 Fe2O3 6.67 7.50 7.22 5.77 7.08 8.46 6.72 MnO 0.06 0.07 0.07 0.06 0.06 0.07 0.07 MgO 2.78 3.19 3.06 2.37 2.98 3.34 2.82 CaO 0.86 0.75 0.79 0.91 0.86 0.64 0.99 Na2O 1.82 1.68 1.11 1.78 1.74 1.65 1.77 K2O 2.92 3.56 3.39 2.66 3.24 3.68 3.01 P2O5 0.28 0.12 0.12 0.12 0.13 0.12 0.14 S 0.03 0.07 0.06 0.06 0.06 0.10 0.06 F 0.05 0.07 0.08 0.04 0.07 0.06 0.07 LOI* - 4.70 4.48 3.43 4.12 4.60 4.03 Total 97.86 101.60 101.44 100.38 101.46 101.17 101.37 ppm Ba 647 987 731 1068 747 681 747 Ce 83 91 91 78 84 112 84 Cl 240 196 157 269 221 360 221 Co* - 37 40 54 33 31 26 Cr * 121 137 132 108 126 145 126 Cu* - 39 37 26 34 46 33 Dy77367-07 Er109812676 Gd5-1-544-04 Hf8445414 La 43 44 48 37 45 59 45 Nb 20 22 21 18 21 22 21 Nd 38 40 40 31 36 44 36 Ni* - 84 79 58 72 79 68 Pb* - 21 24 20 21 19 23 Pr 28 30 42 26 27 44 27 Rb 161 211 198 144 186 226 186 Sc 13 15 15 10 15 18 15 Sr 1143 160 154 146 151 160 151 Th222272821242724 U3223535 V 114 135 133 100 125 158 125 Zn* - 91 89 73 90 102 93 Zr 199 249 257 284 284 1259 1284 * Marked elements have been measured by AAS rest of the elements by XRF # Sample 181 – 188: Patharia well – 5