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2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page A Table of Contents ABSTRACT ................................................................................................................................................... i DEDICATION .............................................................................................................................................. ii ACKNOWLEDGEMENT ........................................................................................................................... iii QUOTES ........................................................................................................................................................ iv CHAPTER ONE ................................................................................................................................. 1 INTRODUCTION .............................................................................................................................. 1 1.2 Problem Statement .................................................................................................................... 6 1.3 Aim ........................................................................................................................................... 6 1.4 Objectives ................................................................................................................................. 6 1.5 Importance of Research ............................................................................................................ 6 1.6 Scope of Work .......................................................................................................................... 7 CHAPTER TWO ................................................................................................................................ 8 COPPER OCCURRENCES AND DEPOSIT TYPES IN ZAMBIA ................................................. 8 2.1 Introduction .............................................................................................................................. 8 2.2 Copper Occurrences in Zambia ................................................................................................. 8 2.3 Copper Deposit Type ................................................................................................................ 9 2.3.1 The Central African Copperbelt ............................................................................................ 9 2.3.2 Distribution of Mineralisation in the Zambian Copperbelt (Kafue Anticline) .................... 12 2.3.3 Styles of Minerilisation in the Deposit of the Zambian Copperbelt.................................... 13 2.4 Styles of Minerilisation in Deposits of the Domes Region ..................................................... 15 2.5 Iron Oxide-Copper-Gold (IOCG) Deposits in the Greater Lufilian Arc ................................ 15 CHAPTER THREE .......................................................................................................................... 17 METHODOLOGY AND CHARACTERISTIC OF DEPOSITS .................................................... 17 3.1 Introduction ............................................................................................................................. 17 3.2 Methodology Flow Chart ........................................................................................................ 17 3.3 Selection and Characteristization Copper Deposits in Zambia ............................................... 18 3.4 The Kitumba Deposit .............................................................................................................. 19 3.4.1 Geographic Location ........................................................................................................... 19 3.4.2 Tectonic Setting .................................................................................................................. 19 3.4.3 Geology of Kitumba Deposit .............................................................................................. 19 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page B 3.5 The Konkola Deep Deposit ................................................................................................. 21 3.5.1 Geographic Location ........................................................................................................... 21 3.5.2 Tectonic Setting .................................................................................................................. 22 3.5.3 Geology of Konkola Deep Deposit ..................................................................................... 22 3.6 The Chambishi Main Deposit ................................................................................................ 24 3.6.1 Geographic Location ........................................................................................................... 24 3.6.2 Tectonic Setting .................................................................................................................. 24 3.6.3 Geology of Chambishi Main Deposit ................................................................................. 24 3.7 The Chimiwungo Deposit ....................................................................................................... 26 3.7.1 Geographic location ............................................................................................................ 26 3.7.2 Tectonic Setting .................................................................................................................. 26 3.7.3 Geology of Chimiwungo Deposit ....................................................................................... 26 3.8 The Kansanshi Deposit ........................................................................................................... 28 3.8.1 Geographic Location ........................................................................................................... 28 3.7.2 Tectonic Setting: ................................................................................................................. 28 3.8.3 Geology of Kansanshi Deposit............................................................................................ 28 3.9 Geophysical Forward Modelling ............................................................................................ 30 CHAPTER .................................................................................................................................................. 31 FOUR MODELLING ................................................................................................................................. 31 4.1 Introduction ............................................................................................................................ 31 4.2 Gravity and Magnetic Models for Kitumba Deposit ............................................................... 34 4.3 Gravity and Magnetic Models for Konkola Deep Deposit ..................................................... 37 4.4 Gravity and Magnetic Models for Chambishi Main Deposit .................................................. 40 4.4 Gravity and Magnetic Models for Chimiwungo Deposit ........................................................ 43 4.6 Gravity and Magnetic Models for Kansanshi Deposit ............................................................ 46 CHAPTER FIVE ........................................................................................................................................ 50 DATA ANALYSIS AND DISCUSSION ...................................................................................................50 5.1 Introduction ............................................................................................................................ 50 5.2 The Kitumba Deposit ............................................................................................................. 50 5.3 The Konkola Deep Deposit ..................................................................................................... 51 5.3 The Chambishi Main Deposit ................................................................................................. 53 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page C 5.4 The Chimiwungo Deposit ....................................................................................................... 55 5.5 The Kansanshi Deposit ........................................................................................................... 57 `CHAPTER SIX.......................................................................................................................................... 59 CONCLUSIONS AND RECOMMENDATIONS ..................................................................................... 59 6.1 Conclusions ............................................................................................................................. 59 6.2 Recommendations ................................................................................................................... 60 REFERENCES ........................................................................................................................................... 61 Appendix I .................................................................................................................................................. 63 Appendix II ................................................................................................................................................. 64 List of Figures Figure 1: (a) Long run historical copper production in (b) Short run historical copper production ............. 1 Figure 2: Copper production Histogram for the World and Zambia between 2001 and 2014. Data Source: US Geological Survey, Mineral Commodity Summaries 2012; US Geological Survey Mineral Information — Zambia ................................................................................................................................. 2 Figure 3: The national contributions of mining to the Zambian economy (after Oxford Policy Management (OPM), 2012). ......................................................................................................................... 3 Figure 4: Copper Occurrence distribution in Zambia. ( after Geological Survey Department (GSD), 1998) ...................................................................................................................................................................... 8 Figure 5: Tectonic Setting of Zambian, the Lufilian Arc and its structural zones (after Binda and Poranda 1995). ............................................................................................................................................................ 9 Figure 6: Zambian Copperbelt deposits distribution along the Kafue Anticline (modified from Selley et al., 2005). .................................................................................................................................................... 12 Figure 7: Generalized stratigraphic section through the Copperbelt deposits (modified from Selley et al., 2005). .......................................................................................................................................................... 13 Figure 8: Methodology flow chart illustrating in summary the methodology ............................................ 17 Figure 9: (a) Location of the selected deposits. (b) Tectonic controls of the selected deposits. ................ 18 Figure 10: Geological Map of Kitumba Deposit (after Intrepid Mines Limited, 2014). ............................ 19 Figure 11: The geological section of Kitumba deposit and its geophysical properties (after Intrepid Mines Limited, 2014)............................................................................................................................................. 21 Figure 12: Geological map of Konkola Deep deposit and the surrounding area (after Porter GeoConultancy, 2014). ............................................................................................................................... 22 Figure 13: The geological section through A-B of Konkola Deep deposit (after Porter GeoConultancy, 2014). .......................................................................................................................................................... 23 Figure 14: The geological map of Chambishi deposits (modified after Croaker, 2011). ........................... 25 Figure 15: Representative cross section through the Chambishi Main deposit(modified after Croaker, 2011). .......................................................................................................................................................... 25 Figure 16: Block view and Cross section of the Chimiwungo deposit (after Golder, 2003). ..................... 27 file:///C:/Users/New/Desktop/project%20vale%20draft%209.docx%23_Toc425478694 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page D Figure 17: the geological map of Kansanshi Deposit and a representative cross section across it. ............ 29 Figure 18: Creating a project and setting the parameters. ........................................................................... 31 Figure 19: Creating Synthetic grid. ............................................................................................................. 32 Figure 20: Creating Synthetic lines. ............................................................................................................ 32 Figure 21: Specification of modelling type and computation of the region gravity and magnetics. .......... 33 Figure 22: Selecting the line to model. ....................................................................................................... 33 Figure 23: Generating gravity and magnetic geophysical responses. ......................................................... 34 Figure 24: Block model of Kitumba deposit. .............................................................................................. 34 Figure 25: Block Model of Konkola deep deposit. ..................................................................................... 37 Figure 26: Gravity and magnetic properties of Konkola deep deposit section. .......................................... 38 Figure 27: Block model for Chambishi deposit. ......................................................................................... 41 Figure 28: Block Model for Chimiwungo deposit. ..................................................................................... 43 Figure 29: Block Model of Kansanshi deposit. ........................................................................................... 47 Figure 30: Gravity (blue line) and magnetic (red line) profile for Kitumba Deposit at a depth of 60m. .... 50 Figure 31: Plot of Change in depth with respect to the Magnetic and Gravity response for Kitumba deposit. ........................................................................................................................................................ 51 Figure 32: Gravity (blue line) and magnetic (red line) profile for Konkola Deep Deposit at a depth of 60m. ............................................................................................................................................................52 Figure 33: Plot of Change in depth with respect to the Magnetic and Gravity response for Konkola Deep deposit. ........................................................................................................................................................ 53 Figure 34: Gravity (blue line) and magnetic (red line) profile for Chambishi at a depth of 0m. ................ 54 Figure 35: Plot of Change in depth with respect to the Magnetic and Gravity response for Chambishi deposit. ........................................................................................................................................................ 54 Figure 36: Gravity (blue line) and Magnetic (red line) profile for Chimiwungo deposit at a depth of 100m. .................................................................................................................................................................... 55 Figure 37: Plot of Change in depth with respect to the Magnetic and Gravity response for Chimiwungo deposit. ........................................................................................................................................................ 56 Figure 38: Gravity (blue line) and Magnetic (red line) profile for Kansanshi Deposit at a depth of 80m. . 57 Figure 39: Plot of Change in depth with respect to the Magnetic and Gravity response for Kansanshi Deposit. ....................................................................................................................................................... 58 List of Tables Table 1: Zambia‘s mining taxes as a share of GDP and total taxes collected for 2008 and 2012 (Zambia Revenue Authority (ZRA), 2013). ................................................................................................................ 4 Table 2: Some IOCG deposit type of the Greater Lufilian Arc in Zambia (after Lobo-Guerrero, 2012). .. 16 Table 3: Gravity and Magnetic properties of the Kitumba Deposit (after Intrepid Mines Limited, 2014). 21 Table 4: Gravity and Magnetic properties of the Konkola Deep deposit (Telford el at, 1994). ................. 23 Table 5: Gravity and magnetic properties of the Chambishi Main deposit (Telford el at, 1994). .............. 26 Table 6: Gravity and Magnetic properties of Chimiwungo deposit (Telford el at, 1994). ......................... 27 Table 7: Gravity and Magnetic properties of Kansanshi Deposit (Telford el at, 1994). ............................. 29 Table 8: Depth relationship with Maximum Gravity and Magnetic Susceptibility for Kitumba Deposit .. 51 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page E Table 9: Depth relationship with Maximum Gravity and Magnetic Susceptibility for Konkola Deep deposit ......................................................................................................................................................... 52 Table 10: Depth relationship with Maximum Gravity and Magnetic Susceptibility for Chambishi Main deposit ......................................................................................................................................................... 54 Table 11: Depth relationship of Maximum Gravity and Magnetic Susceptibility for Chimiwungo deposit .................................................................................................................................................................... 56 Table 12: Depth relationship of Maximum Gravity and Magnetic Susceptibility for Kansanshi Deposit . 57 Gravity and Magnetic Simulation Models for the Deposits Kitumba Deposit Scenario 1 at 60m depth .............................................................................................................................. 35 Scenario 2 at 168m depth ............................................................................................................................ 35 Scenario 3 at 700m depth ............................................................................................................................ 36 Scenario 4 at 2000m depth .......................................................................................................................... 36 Scenario 5 at 5000m depth .......................................................................................................................... 37 Konkola Deep Deposit Scenario 1 at 100m depth ............................................................................................................................ 38 Scenario 2 at 170m depth ............................................................................................................................ 39 Scenario 3 at 270m depth ............................................................................................................................ 39 Scenario 4 at 670m depth ............................................................................................................................ 40 Scenario 5 at 1670m depth .......................................................................................................................... 40 Chambish Deposit Scenario 1 at 0m depth ................................................................................................................................ 41 Scenario 2 at 50m depth .............................................................................................................................. 42 Scenario 3 at 200m depth ........................................................................................................................... 42 Scenario 4 at 500m depth ............................................................................................................................ 43 Chimiwungo Deposit Scenario 1 at 50m depth .............................................................................................................................. 44 Scenario 2 at 200m depth ............................................................................................................................ 44 Scenario 3 at 400m depth ............................................................................................................................ 45 Scenario 4 at 750m depth ............................................................................................................................ 45 Scenario 5 at 1400m depth .......................................................................................................................... 46 Scenario 6 at 5600m depth .......................................................................................................................... 46 Kansanshi Deposit Scenario 1at 80m depth ............................................................................................................................... 47 Scenario 2 at 480m depth ............................................................................................................................ 48 Scenario 3 at 880m depth ............................................................................................................................ 48 Scenario 4 at 1280m depth .......................................................................................................................... 49 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page i ABSTRACT Copper is nonrenewable resource which is and has been an essential material to man since pre- historic times. This commodity has seen a somewhat positive gradient in demand from the time of its pre-historical use to date. Zambia is a major contributed to the production of Copper and it‘s the 2 nd largest African producingcountry. Now due to the increased demand of Copper which is mostly as a result of increased urbanization and industrialization of both developed economies like the US, UK, Germany Russia and also immerging economies like China, India, Brazil and South Africa, Exploration of this commodity is inevitable. Mineral exploration is a huge capital, risky and non-cash flow venture which incurs huge costs mainly at drilling stage but with the advancement in geophysical softwares the risk is reduced. This is because geophysical data allows for 2D and 3D modelling, thereby giving the subsurface features and this aids in determining the right orientation for drilling that will intercept the body. Forward modelling the process of calculating a response (e.g. a gravity measurement) from a given earth model whilst inversion modelling is the process that seeks to produce a 3D distribution of physical rock properties (e.g. density) that should meet an observation measured in the field. Hence by using the data available on the known deposits in Zambia in terms of their geology, stratigraphy and physical properties (density and magnetic susceptibility), Forward modeling was done to produce synthetic gravity and magnetic models at different depth so as to aid in the exploration of greenfield Copper. Forward modeling was done on the following deposits Kitumba, Konkola Deep, Chambishi, Chimiwungo and Kanshashi deposit. Selection of deposits was based on mainly their type of Copper deposits. The presence of sedimentary rocks except quartzites in the deposit modeled resulted in very low magnetic anomaly, this is likely because these rocks have relatively low magnetic susceptibility, sedimentary rocks also exhibits low gravity anomalies, sometimes negative depending on the set background values for the density while The presence of basement rocks in a body result in high magnetic and gravity anomaly, this is likely because these rocks have relatively high magnetic susceptibility and densities. Generally Strata-bound sedimentary copper deposits have a limiting depth of approximately 450m and 300m for gravity and magnetic response respectively. Therefore for a similar deposit in Western Province, magnetic and gravity methods will not be effective because the cover is over 600m in same areas. IOCG and Strata-bound Disseminated Copper deposits produce good gravity and magnetic response and the limiting depth is approximately 1500m and 1700m respectively. Vein-hosted copper deposit produces a good magnetic response with effective depth of approximately to 800m. Hence magnetic methods can be applied for exploration in Western Province. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page ii DEDICATION This thesis is dedicated to my Parents, Mr and Mrs Banda: for their support and belief they have always given me. To my brothers and Sisters (Saulosi, Candy, Mpando, Mapalo, Muchemwa and Mwila): success is always a guarantee when you put your very best. Pamela for her love and consistent push in making sure I excel during my stay at University of Zambia. My Good friends: Albert and Kelvin, you have been great company and last but not the least: Chi-alpha Christian Fellowship for being family to me and a hub for spiritual growth. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page iii ACKNOWLEDGEMENT I would like to express my sincere gratitude to the following people and company: Vale Zambia Limited for coming up with this project and facilitating the required resources for me to carry out this project. Special thanks go to my supervisor: Dr. O.N. Sikazwe for making that sound interpretation and writing of the report writing is archived. You always gave me a challenge to think out of the box. Mr S Nkemba for the advice and help he rendered at during consultations, it surely paid off. The Hold of Department (HOD) Mr S Musiwa and all the lectures in the geology, thank you for sharing your experience, knowledge and wisdom with me. Mr P Zimba thank you for your warm heart and assistance in printing this report. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page iv QUOTES Psalm 46:10 ―Be Still, and Know that I am God.‖ 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 1 CHAPTER ONE INTRODUCTION 1.0 Background Copper is and has been an essential material to man since pre-historic times. In fact, one of the major "ages" or stages of human history is named for a copper alloy, bronze. Copper and its many alloys have played an important role in many civilizations, from the ancient Egyptians, Romans to modern day cultures around the world. The price of copper has increased substantially with the highest record being nearly US $10000 per tonne in the year 2009 to 2011 (figure 1). Regardless of the overall increase in copper demand and prices in the long run, copper demand and prices take a twist in short run and thereby making the mining industry very uncertain. Currently the prices of copper have fallen to as low as US$ 6040 per tonne making some mines operate below the break-even point and hence leading to closure or care and maintenance. The world currently consumes more than 26 million tonnes of copper on an annual basis and as of the year 2013 approximately 18 million tonnes of copper was produced from mining (Appendix I) while the remaining 8 million tonnes was supplied from recycling of scrap. This huge consumption is because of the increased urbanization and industrialization of both developed economies like the US, UK, Germany Russia and also immerging economies like China, India, Brazil and South Africa. China alone is currently consuming about 40% of the total world copper consumption. Figure 1: (a) Long run historical copper production in (b) Short run historical copper production Zambia is a beneficially to the rise in copper demand and prices because the mining industry is the major single contributor to its Gross Domestic Product (GDP). Commercial-scale mining has taken place in Zambia for around 100 years, and is confidently expected to continue for many years to come. Industry has gone from private ownership in the early years, through a period of nationalization, and most recently back into private hands. As a result of the recent privatization, in excess of US$8 billion has been invested by the new owners. Some of this has been necessary to refurbish and modernize the infrastructure and operations of the ‗legacy‘ mines on the (a) (b) 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 2 Copperbelt, but most has been invested in new or expanded operations. This has been most noticeable in the Northwest Province, dubbed ‗the New Copperbelt‘. Resulting from this investment, annual finished production has risen from a low of 257,000 metric tonnes per annum to over 700,000 metric tonnes in 2013 (Figure 2). The total is confidently predicted to rise to over 1 million metric tonnes in the next couple of years and towards 1.5 million metric tonnes within 5–10 years. Zambia is the second largest copper producer in Africa from Democratic Republic of Congo (DRC) with copper production of 730,000 and 1.1 million tonnes respectively. Figure 2: Copper production Histogram for the World and Zambia between 2001 and 2014. Data Source: US Geological Survey, Mineral CommoditySummaries 2012; US Geological Survey Mineral Information — Zambia Zambia broadly conforms to the inverted pyramid pattern of macroeconomic contributions with very high contributions in some macro areas (notably exports and investment) but progressively lower contributions in other areas such as government revenues, GDP and employment (Figure 3). Since the early 2000s, mining investment has boomed with over US$10 billion in Foreign Direct Investment (FDI) since privatization. FDI flows have been dominated by mining: in 2011, new FDI into mining accounted for 86.2 per cent of total FDI. Whilst Copper mining accounts for over 80 per cent of export earnings. This is a high share even in comparison to other mineral- driven countries. Many decades of official statements of intent and policies intended to diversify the economy have met with limited success. Government revenues collected from mining have increased sharply in recent years to over 30 per cent of total tax revenues, according to official X 1 0 3 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 3 Zambia Revenue Authority (ZRA) data. Government revenues from mining were low (around 16 % of total tax revenues) until around 2008 but subsequently increased sharply (Table 1). In 2011, Zambia‘s GDP stood at US$18.4 billion in terms of market exchange rates, and US$21.93 billion in terms of purchasing power parity. The mining sector contribution to GDP is projected to grow to 20% over the medium term, to reach $1.35 billion by the end of 2015. This increase will position Zambia among the world‘s top five copper producers. The employment contribution of mining is the smallest of the direct macro contributions but still large in absolute terms. The absolute numbers of jobs in mining have increased substantially in response to higher levels of investment and production. The preliminary results of the national Labour Force Survey for 2012 (Central Statistical Office, 2013a) show total formal employment in mining in 2012 of over 90,000. This represents about 1.7 % of the labour force, 8.3 % of total formal sector jobs and around 25 % of total private sector formal jobs in 2012. The indirect and induced jobs associated with mining are significant contributors to local welfare. Multiplier calculations indicate that ―indirect‖ job creation (via spending on local supplies) and ―induced‖ employment (through mining employees spending their relatively high average incomes) together increase the total employment attributable to mining by a factor of between two and four; that is, for each direct job with a mining company or an on-site contractor, two to four additional jobs are created elsewhere in the economy (International Council of Mining and Metals, 2014). Figure 3: The national contributions of mining to the Zambian economy (after Oxford Policy Management (OPM), 2012). 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 4 Table 1: Zambia‘s mining taxes as a share of GDP and total taxes collected for 2008 and 2012 (Zambia Revenue Authority (ZRA), 2013). Year GDP in ZMW million Total taxes collected in ZMW million Mining taxes collected in ZMW million Mining taxes (%GDP) Mining taxes (% total taxes) 2008 54,839 9,670 1541 2.8% 16% 2012 11,049 20,723 6,619 5.9% 3 2% Note that the reported currency is in rebased format. From the above statistics it‘s clear that the backbone of the Zambia‘s economy is the mining industry. Hence to continue enjoying the contribution of the mining industry to the economy of Zambia, it‘s inevitable that mineral exploration should be the first priority because most of the deposits that where discovered in the 1930‘s in the Copperbelt are nearly depleted or depleted. Exploration is a very expensive, risky and noncash flow venture for companies but the advances in technology have seen enormous attempts to minimize the risk of exploration process. Geophysical applications in exploration are currently dynamic and advancements in software‘s have reduced the risk of exploration, thereby increasing the level of confidence in the process of exploration. That is, the use of geophysical inversion and forward modelling in mineral exploration has led to reduced risk in exploration. The forward modelling method is based on geological and geophysical intuition. The method allows construction of an initial model for the source body and then computes the model's magnetic effect that is to be compared with the observed anomaly (Shin et al., 2006). Forward modelling is the process of calculating a response (e.g. a gravity field) from a given earth model (e.g. a density distribution) whilst inversion modelling is the process that seeks to produce a 3D distribution of physical rock properties (e.g. density) that should meet an observation measured in the field (e.g. a gravity response). Developments in instrumentation, data collection, computer performance, and visualization have been catalysts for significant advances in modelling and inversion of geophysical data. Forward modelling, which is fundamental to intuitive geological understanding and practical inversion methods, has progressed from representations using simple 3D models to whole earth models using voxels and discrete surfaces. Inversion has achieved widespread acceptance as a valid interpretation tool and major progress has been made by integrating geological models as constraints for both voxel and multi-body parametric methods. As a consequence, potential field, IP and electromagnetic inversion methods have become an essential part of most mineral exploration programs. Until the 1960s most deposits were discovered by prospecting, or looking for clues on the surface with the help of outcropping geology. But geophysical techniques are increasingly taking the role of the prospector as exploration moves deeper into the subsurface. For the fact that most 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 5 surficial deposits have been discovered and are being exploited, the risk of exploration is high. The use of conventional geological and geochemical techniques on deep seated deposit is increasingly becoming less effective. Conventional geological and geochemical exploration techniques in western province of Zambia have proved to be ineffective. This is because of a thick sediment pile (Kalahari sands) which is about 600m thick in some areas. The Kalahari sands are believed to overlie an older Katanga Supergroup that is not exposed in western province. The Katanga Supergroup hosts the Cu-Co minerilisation in the Lower Roan Subgroup. With the difficulty faced in exploration in western province, forward modelling provides a plat- form that may make exploration possible and also reduce the risk faced in exploration by simply working on existing deposit models and making simulation at different depth to notice the response. The principle of application of any geophysical method is based on the contrast that the target has with the host rock. Gravity and magnetic methods are potential field methods and used for a wide range of applications and scales in geosciences. Traditionally, they have been used for large scale investigation of geologic structures. Smaller-scale applications of the gravity and magnetic methods are for mining exploration, environmental and engineering studies, etc. (Hinze, 1990; Reynolds, 1987; Sharma, 1997; Telford et al., 1996). In order to arrive at geologically meaningful anomaly values, the gravity or magnetic survey data are firstly processed to make appropriate corrections. After these steps, the surveydata is ready for interpretation or displaying as maps. Interpretation of potential field data is performed on either profile or map data. These data are most often interpreted by the use of inversion or data processing techniques. Spatial and frequency domain filtering, image processing and managing grids are essential tools in gravity and magnetic data interpretation. A potential field or image processing filter highlights different aspects of potential field data (Bhattacharyya, 1972; Clement, 1973; Gunn, 1975; Ku etal., 1971; Jacobsen, 1987; Telford et al., 1996; Vaclacetal., 1992). Filters can emphasize boundaries between geological contacts, highlight deeper or shallower sources, highlight features from different angles or reduce undesirable effects within the dataset. Filtering procedure can be undertaken in the frequency domain by means of Fourier Transform (FT) or in the spatial domain by convolution. Frequency domain filtering involves converting the dataset into the frequency domain, performing an operation on the data by applying the appropriate filter and then transforming the data back to the spatial domain. The most commonly used frequency domain filters include Reduction To Pole (RTP), pseudo gravity transformation, analytical continuations and derivative filters. Convolution methods involve convolving a filter impulse response (filter coefficients) with the dataset (Byerly, 1965). Magnetic anomalies are dependent on latitude. None pole at the polar region and dipolar at themed latitude. Hence the use of RTP filters. In addition to filtering, the main intention of gravity and magnetic data interpretation is calculating the potential field from the constructed model (forward-modeling).Various methods have been developed for different aims: simple geometries, sequence of isolated 2-Dor3-D 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 6 bodies or layers (Blakely, 1996; Jessel, 2001; Parker, 1972; Rasmussen and Pedersen, 1979; Telfordetal., 1996). 1.2 Problem Statement Exploration of copper in green field areas is very risky without the application of geophysical techniques. 1.3 Aim The aim of this project is to use the available data on known copper deposits in terms of their geology, stratigraphy and geophysical properties (density and magnetic susceptibility) to develop geophysical models to aid in green-field exploration. 1.4 Objectives To select deposits for forward modelling. Compile magnetic and gravity properties of the selected deposits. To develop gravity and magnetics profiles based on the geological models of selected deposits by using ModelVision geophysical software. To simulate gravity and magnetic responses at different depth. In order to determine the limiting depth at which the anomaly will be visible. To discuss the results, draw conclusions and write a report to be submitted as partial fulfillment for the award of Bachelors in Mineral Science in Geology at the University of Zambia. 1.5 Importance of Research Exploration is a huge capital, risky and non-cash flow venture which incurs huge costs mainly at drilling stage. Therefore in the process of minimizing costs it is important that a subsurface representation model is developed before the commencement of drilling so that the orientation of the drill holes are designed to intersect through the anomalous body. With the advancement in geophysical software (e.g Encom ModelVision magnetic and gravity geophysical software) it is possible to develop representative subsurface model from an observed ground geophysical survey and thereby design the effective drilling pattern as in the case for inversion modeling. Forward modeling is the reverse of inversion modeling and requires computation of geophysical responses from an existing model. It allows for simulation of a known model at different depth thereby allowing to determine the limiting depth to which the signal of the model will completely fade out. A comparison between computed geophysical responses and observed 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 7 ground geophysical responses conducted in a new area helps determine the depth at which the model in the new area lies provided the observed ground responses are similar with the computed geophysical responses. If from comparison, it is determined that the model lies at depth of greater than 1500m a decision is influenced to cut any further exploration because the model will definitely be uneconomical to exploit. Hence this research, although academic, is important because it attempts to minimize cost in exploration by the use of forward modeling. 1.6 Scope of Work The scope of this project is restricted to forward modelling of a few representative copper deposits. The geophysical response modelled for the existing deposits in this research is restricted to passive methods which are gravity and magnetics. This is because mainly of the limitation that comes with the software. ModelVison geophysical software only models gravity and magnetic data. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 8 CHAPTER TWO COPPER OCCURRENCES AND DEPOSIT TYPES IN ZAMBIA 2.1 Introduction Exploration works require that a target is first established and in this case the target is copper minerilasition. After which a target model should be developed in order to ease the selection process of the area to be explored, this process involves literature review on the type of deposits that are associated with the region in question and the controls of the mineralization. Hence in this chapter the main focus is to review the copper occurrences in Zambia and their style of mineralization. 2.2 Copper Occurrences in Zambia The Geological Survey of Zambia, in conjunction with the British Geological Survey, carried out detailed soil and stream sediment geochemistry between 1998 and 2000 for almost the entire Zambia. Based on the extensive data set, a series of statistical tools were used to model trace and major element distributions in Zambia. Copper occurrences are mapped and show that they are concentrated in the Copperblet, Northwestern, and Central and Lusaka Provinces (Figure 4). A relationship can be inferred from the geological map of Zambia with regard to the geological controls that give rise to different types of copper deposits (Appendix II). Figure 4: Copper Occurrence distribution in Zambia. ( after Geological Survey Department (GSD), 1998) 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 9 2.3 Copper Deposit Type There are three major types of copper deposits in Zambia namely stratiform sediment hosted copper deposits, Iron Oxide Copper Gold (IOCG) deposits and vein-hosted copper deposits. Majority of the deposits in Zambia are stratiform copper sediment hosted type and they basically make up the Zambia Copperbelt, which together with the Congolese belt make up the Central African Copperbelt. 2.3.1 The Central African Copperbelt The CACB is part of the Lufilian Arc, also known as the Katangan belt, a 700 km long and 150 km wide thrust-fold belt, which is part of the Pan‐African mobile belt lying between the Congo and Kalahari Cratons (Cailteux et al., 2005). The Lufilian Arc consists of Katanga Supergroup meta-sedimentary rocks that host the Central African Copperbelt deposits and which unconformably overlie a pre-Katangan basement (Mendelsohn 1961). The copper-cobalt orebodies occur in the Roan Group of the Katangan Supergroup. The RoanGroup meta- sedimentary rocks display a regional lateral variation of facies between Zambia-type and Congo- type successions. The CACB has world class sediment‐hosted stratiform Cu‐Co deposits. The Lufilian Arc is divided in five structural zones (de Swardt and Drysdall, 1964), namely; Katanga High (IV), Synclinorial Belt (III), Domes Region (II), External Arcuate Fold and Thrust belt (I) and Foreland (V) (Figure 5). Figure 5: Tectonic Setting of Zambian, the Lufilian Arc and its structural zones (after Binda and Poranda 1995). 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 10 The Katanga High to the southwest, in which only the upper parts of the Katanga Supergroup and almost all of the outcropping granitic intrusions of the Lufilian Arc are exposed (Petters, 1986; Selley et al., 2005). The Synclinorial Belt, where sediments are subjected to large scale folding during at least two deformation events, and low grade metamorphism, which reflects a change from a marginal shelf in the north, to a deeper basin (Cosi et al., 1992; Porada and Berhorst, 2000). The Domes Region, which includes the Zambian Copperbelt in its outer margins, represents thicker skinned deformation with upright folds, exposed basement domes (interpreted to represent culminations above thrust ramps), and upper-greenschist to upper-amphibolite facies metamorphism. The External Fold and Thrust Belt to the northeast, mainly in the DRC (where it hosts the Congolese Copperbelt), characterised by thin-skinned thrust/nappe-dominated deformation, absence of exposed basement, low-grade metamorphism and repetition of the Katangan stratigraphy. Foreland to the far northeast, an extension of the Katanga Basin within the DRC, produced during the second period of extension, characterised by less deformed Mwashya Subgroup and Nguba Group sedimentary rocks, and deposition of undeformed, late Kundelungu Group molasse rocks during and following the main compressive stage of the Lufilian orogeny. During the Lufilian orogeny the basin was inverted and the sedimentary layers were folded, thrusted and metamorphosed up to greenschist and amphibolite facies, with an increasing metamorphic grade from north to south (Cailteux et al., 2005). The tectonic evolution of the Lufilian arc and the Pan‐African belt is linked to the behavior of the Rodinia supercontinent. Intra‐continental rifting formed the sedimentary basin during the Rodinia break‐up, and the assembly of Gondwana led to the inversion and collisional deformation of the basin between the archean Congo and Kalahari cratons (Hanson, 2003). Although terms applied to sedimentary rocks are used to describe the rocks of the Zambian Copperbelt, the formations are distinctly metamorphic; in particular, the host rocks to the mineralization include mica schists, which may contain carbonates, talc or tremolite (Moine et al. 1986). The metamorphic minerals observed include, biotite, sericite, scapolite, tourmaline, chlorite, tremolite-actinolite, epidote and apatite (Mendelsohn 1961). The Katangan supergroup is divided into three groups, namely: Roan Group, Nguba Group and uppermost Kundelungu Group. It is composed of varying sequences of carbonates, shales and 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 11 siliciclastic sediments (Cailteux et al., 2005) and the groups are separated from each other by diamictites, which are associated with global glacial events (Batumike,Kampunzu, & Cailteux, 2006). The Roan Group is the oldest, overlying the basement rocks. The Nguba Group overlies the Roan Group. The Kundelungu Group sediments were deposited before, during and after the Lufilian orogeny (Cailteux et al., 2005). Roan Group The Roan Group is the lower unit of the Katanga succession and is divided into the Lower Roan and the Upper Roan Groups. The Roan Group unconformably overlies the Basement and represents the first phase of the initial uplift and rifting which resulted in the deposition of texturally immature proximally derived coarse conglomerates at the base. This was followed by a marine transgression and sedimentation of sub-arkosic sandstones, and rare siltstones deposited in fluvial, alluvial fan, aeolian and fan-delta environments. Shallow marine sediments which are a mixed carbonate platform-hypersaline lagoon evaporate environment, traditionally demarcate the boundary between the Lower Roan and the Upper Roan Group by the predominance of carbonate strata (e.g. Gray, 1932; Mendelsohn, 1961). The Upper Roan Group is characterized by laterally extensive, meter-scale, upward fining cycles of sandstone, siltstone, shales, dolomite, algal dolomite and local nodular anhydrite. Nguba Group Deposition of the Nguba Group (formerly Lower Kundelungu) commenced with a Glaciogenic diamictite (the Grand Conglomérate) approximately 10 to 100 meters (Francois, 1973; Cailteux 1994). In the upward deepening sequence and overlying the Conglomérate are dolostones, shales, siltstones carbonates, and mudstones. The Nguba is exposed in the core of the Lufukwe Anticline and probably correlates with the 750 Ma sturtian glacial deposits (Kampunzu et al., 2005). Kundelungu Group Overlying Nguba is the Kundelungu Group (formely Upper Kundelungu) that commences with a wide spread tectonically induced conglomerate of up to 50 m thick (`Petit Conglomerate‗) containing abundant fragments of Kankotwe Limestone in the Copperbelt region. This was previously been interpreted as a glacio-marine or glacio-fluvial deposit, but is now regarded as a unit of tectonically triggered mud-flow deposit (Cahen, 1978). This conglomerate is followed by sandstones, siltstones, and shale with a few tens of metres thick of limestone near the base. The Kundelungu subgroup terminates with a distinctive purple arkose. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 12 2.3.2 Distribution of Mineralisation in the Zambian Copperbelt (Kafue Anticline) Copper and cobalt mineralisation occurances in Zambia are mainly distributed along the Domes region. The main Zambian Copperbelt deposits are defined by two NW-SE trending parallel lines of Cu mineralisation which are approximately some 20 km apart, separated by the Palaeoproterozoic basement gneisses, granitoids and schists, and Mesoproterozoic conglomerates, quartzites and granitoids that make up the Kafue Anticline (Figure 7), within the eastern Domes Region of the Lufilian Arc. The majority of the deposits are in the SW of the two lines of mineralisation. Each of these two belts is 5 to 20 km wide and up to 150 km long. Ore grade mineralisation, however, tends to occupy linear, often more structurally complex, semicontinuous bands, up to 2 to 3 km wide, and as much as 17 km long, on the SW limb, interrupted by narrow barren gaps and cross folded anticlinal basement ridges (e.g., the Nkana- Mindola, Nchanga and Konkola strings of deposits). Figure 6: Zambian Copperbelt deposits distribution along the Kafue Anticline (modified from Selley et al., 2005). 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 13 Traditionally the ore deposits of the Zambian Copperbelt have been interpreted to lie within the Neoproterozoic Lower Roan Subgroup, composed principally of coarse siliciclastics (conglomerate to arkose and siltstone, with lesser carbonates). Some 65% of the mineralisation lies within a finer 0 to 100 m thick unit of generally carbonaceous argillites, carbonatic argillites and interbedded arenites (Copperbelt Orebody Member)within the coarser clastic succession. A further 25% lies within coarser footwall clastics and the remaining 10% within the coarse hangingwall clastics. Lithologically, 60% of the ore is hosted by argillites, and 40% in arkose, quartzite‘s and conglomerates. A generalized section through mines of the eastern part of the domes region and how they are correlated is shown in Figure 8. Figure 7: Generalized stratigraphic section through the Copperbelt deposits (modified from Selley et al., 2005). 2.3.3 Styles of Minerilisation in the Deposit of the Zambian Copperbelt Minerilsation in the Zambian Copperbelt differs in style among other deposits. The chief of styles are: 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 14 (a) Disseminated, generally fine-grained (<0.1 to 3 mm) sulphides within interstitial sites between detrital or authigenic grains, randomly distributed or aggregated to form bedding- parallel streaks and lenses. There is a correlation between the sizes of detrital and sulphide grains in this style of dissemination (Selley et al., 2005 and references cited therein). Sulphide may also occur replacing detrital grains and authigenic cements, including anhydrite, carbonate, quartz and feldspar, as well as diagenetic pyrite, anhydrite, carbonate, quartz, feldspar or heavy minerals such as rutile (Binda, 1975; Fleischer et al., 1976); (b) Vein-Hosted, which may occur as prefolding, layer-parallel and discordant veins or veinlets of sulphide, which have sharp contacts with argillaceous strata, and diffuse margins in arenites (Annels, 1989). Veining also occurs as late-tectonic, generally coarse-grained sulphide grains (commonly >0.5 to 3 cm) in quartz-carbonate (dolomite, calcite) veinlets and subordinate veins, which may also contain K-feldspar, chlorite, sericite, biotite, and, very locally, albite, tremolite, and below the zone of supergene dissolution, anhydrite. Veinlets are typically ~0.5 to 2 cm wide, but may locally be up to several tens of cm thick and extend for distances of several tens of metres or more, with densities of 1 to 5 per metre, following and stepping up through the stratigraphy. Veins also occupy tension gashes on a small scale and other structures at a high angle to bedding. Veins and veinlets can be particularly abundant at the tops and/or bottoms of the stratabound orebodies, commonly coinciding with rheologic contrasts and occupying shear zones and décollements at these locations. Veinlets often penetrate upwards from arenite hosted disseminated mineralisation into otherwise unmineralised, impermeable carbonaceous shales. Mineralised veins are restricted to zones of disseminated mineralisation, and contain the identical sulphide assemblages found within the enclosing disseminated mineralisation throughout the zoned sulphide assemblages (Hitzman et al., 2012, and references cited therein; Sillitoe et al., 2010). In addition to these Cu±Co vein systems, the Zambian Copperbelt contains volumetrically minor Cu-U-Mo-(Au)-(Ni) sulphide assemblages in post-folding veins with associated albite haloes, e.g., Mindola, which is the only known economic accumulation (Darnley et al., 1961). (c) Oxide Ores, usually gradationally overlying the hypogene ore, through a progression from primary sulphide (chalcopyrite-bornite-carrollite), through mixed oxide-sulphide (chalcocite- copper carbonate/sulphate-cuprite-native copper) to leached capping (usually ~30 m thick). The transition usually takes place over an interval of 30 to 70 m of the surface, although in some areas of deep faulting, malachite and chalcocite have been found to persist to depths of as much as 1 km at Konkola and >600 m at Nchanga Lower. As chalcocite generally occurs closest to the surface in the primary sulphide zonation, it is often difficult to differentiate between primary and supergene populations of the mineral (Selley et al., 2005). (d) Cupriferous Mica Mineralisation, which occurs at a number of deposits as an upper and/or lower fringe to sulphide orebodies, but never laterally. At the Mimbula-Fitula deposits, cupriferous micas persist to a depth of up to 150 m, although the bulk is in the zone from near 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 15 surface to a depth of 60 m. The cupriferous micas are brown to dark brown in colour, and are visually indistinguishable from unmineralised mica. Stockpiles of as much as 150 Mt @ 1.2% Cu have been accumulated at Chingola, and resources of in situ mineralisation and stockpiles at Nchanga are >275 Mt @ 1 to 1.4% Cu. The mineralisation is refractory. Copper is held in the mica lattices in the exchange position, tied largely to hydroxyl groups in interstratified phlogopite-cupriferous chlorite micas. Some copper is also absorbed on the surfaces of layered mineral structures. Under tropical or sub-tropical conditions of weathering, it has been shown that copper may be dissolved out of primary minerals, and where the adjacent rock is micaceous, Cu is 'soaked up' by the micas as it passes through the rock. Weathering of primary phlogopite causes exchanges of K ions by hydrated Cu and Mg ions, followed by chloritisation. The Cu content of this mineralisation ranges from 1 to 8% Cu (Diederix, 1977). 2.4 Styles of Minerilisation in Deposits of the Domes Region Minerilisation is not entirely restricted to in the Zambian Copperbelt. In recent years the western area of the domes region (figure 4) has been extensively explored and this has led to establishment of big mines such as Lumwana, Kansanshi and Sentinel. Lumwana in 2013 was the biggest copper producing mine in Africa with resources of 800 to 1000 Mt @ 0.5 to 0.7% Cu. These deposits have differences in the apparent mode of occurrence compared to the main copperbelt deposits fringing the Kafue Anticline. Kansanshi Cu-Ag deposit is a vein-hosted type occurring in the Nguba Group (Broughton et al, 2002) while the Sentinel Copper deposit is hosted in carbonaceous phyllite which is believed to be in the Mwashya (Hitzman et al., 2012). In Lumwana the Cu-Co deposit is hosted in the pre-Katangan basement schist (Bernau, 2007, unpublished.). 2.5 Iron Oxide-Copper-Gold (IOCG) Deposits in the Greater Lufilian Arc The IOCG deposits occur in and surrounding the granitoid massifs of the Lufilian Arc. IOCG deposits typically contain an iron-oxide nucleus (magnetite and/or hematite). Magnetite may be altered to martite and/or hematite, and the later replacement of part or all of the iron oxides by sulphides is common. Light REE and gold are sometimes present in economic quantities; uranium content may be significant; many other metals such as silver, cobalt, manganese, nickel and Precious Group Element (PGE) may occur in economic concentrations. The Greater Lufilian Arc of Zambia is a prospective zone for the discovery of additional economic IOCG mineralisation. Some of the known IOCG deposits and prospects in the region are marked by an abundance of: uranium, light Rare Earth Elements (LREE) minerals, phosphates, cobalt, barium-bearing minerals, silver, PGE, titanium-bearing minerals and vanadium, as well as copper and/or gold. Some deposits do not contain any anomalous copper. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 16 Table 2 describes some features of deposits being exploited and prospects that are akin to IOCG deposits. Table 2: Some IOCG deposit type of the Greater Lufilian Arc in Zambia (after Lobo-Guerrero, 2012). Deposits Tons x10 6 Cu Wt% Au g/t Minealisation Stlyes Associated Metals Associated Rocks Dunrobin Au deposit 0.002n.a 9.3* Structurally controlled; FeOx nucleates sulphidation+Au. Diss+ replacements in country rock. Qtz and py veins. Replecement FeOx bodies. Racoon- style FeOx-Py banding Ag, Bi, Mi, Pb, Sb, As Hosted by foled katangan carb + gtds Nampundwe Pyrite Deposit 23(Cu) 10(Fe) 0.79 X n.a. Selective replacement in folded sedimentary rocks. Specularite- matrix in polymictic multiphase ht bxs associated to gtds 16% pyrite 57% Fe LREE, Co, Au? Small bodies of gab + felsic intrusives, mag-bear diorite: lamprophyre dykes; qtz pods Kalengwe deposit 0.6 ini 1.9 fin 16 init 9.44 fin X n.a. Tabular replacement in sediments, ht bxs, supergene enrichment to chalcocite body; polymictic ht bxs: Cu sulph dissemination 50g Ag/t, LREE Gabic rocks, hosted by Katangan siliciclastics syenites + granites Kitumba deposit 11.9 2.44 0.04 Hypogene mineralization occurs as diss py and cp, associated with stwk veining and brecciation Co, Au, Ag and U Notes: *Dunrobin mine produced over 40,000 oz of gold by 1935. It produced 13,817 oz of gold from 1936 to 1961. altn = alteration; bear = bearing; bn = brown; bx = breccia; bxs = breccias; carb = carbonate; cp = chalcopyrite; diss = disseminated, dissemination; dol = dolomite, dolostone; FeOx = iron-oxide; fin = final; frac = fracture; gab = gabbro; gtd = granitoid; ht = hydrothermal; init = initial; LREE = light rare earth elements; mag = magnetite; n.a. = not available; po = pyrrhotite; py = pyrite; qtz = quartz; rk = rock; stwk = stockwork ;sulph = sulphide; undim. = undimensioned; X n.a. = metal is present but data is not available. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 17 CHAPTER THREE METHODOLOGY AND CHARACTERISTIC OF DEPOSITS 3.1 Introduction This chapter focuses on the selection of deposits that are representative and also describes the geology and geophysical characteristics of the selected deposits. 3.2 Methodology Flow Chart Figure 9 summarizes and illustrates the process applied to the research undertaken, from literature review through to report writing. Literature Review Deposit Selection Criteria Forward modelling of Selected Deposits Data Interpretation and Analysis Report Writing Geophysical Data compilation of Selected Deposits (gravity and magnetic Data) Figure 8: Methodology flow chart illustrating in summary the methodology 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 18 3.3 Selection and Characteristization Copper Deposits in Zambia To avoid biasness in the selection of deposits and to make sure that representative exploration models are developed, deposits were selected based on the geographical location, the tectonic setting, style of copper mineralization and the mode of exploitation. The following copper deposits were selected (Figure 10 a and b): The Kitumba IOCG deposit located in Mumbwa District, central Zambia within extreme southern portion of the Neoproterozoic Lufilian Arc and to be exploited by underground means; The Konkola Deep Strata-bound sedimentary copper deposit located in Chingola District, Copperbelt Zambia within the Zambian Copperbelt and being exploited by Underground means; The Chambishi Strata-bound sedimentary copper deposit located in Kitwe District, Copperbelt Zambia within the Zambian Copperbelt and being exploited by open pit; Lumwana‘s Chimiwungo Strata-bound metamorphic copper deposit located in Solwezi District, Northwestern Zambia within the domes region and being exploited by open pit means; and The Kansanshi Vein deposit type located in Solwezi District, northwestern Zambia within the Domes Region and being exploited by open pit means. Figure 9: (a) Location of the selected deposits. (b) Tectonic controls of the selected deposits. (a) (b) 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 19 3.4 The Kitumba Deposit 3.4.1 Geographic Location Kitumba Deposit is located in Mumbwa District in Central Province Zambia and it‘s about 160 km west of Lusaka City(#Location: 12° 6' 0" S, 26° 26' 0" E). 3.4.2 Tectonic Setting The Kitumba deposit is located within a giant iron oxide alteration system which is developed along a 26 km long north-northwest to south-southeast trending structural corridor referred to as the Kitumba Fault Zone (KFZ) within the extreme southern portion of the Neoproterozoic Lufilian Arc (Robertson, 2013). 3.4.3 Geology of Kitumba Deposit The geology of the Mumbwa area is described by Cikin and Drysdall (1971). The region is dominated by metasedimentary rocks of the upper units of the Neoproterozoic Katanga Sequence. These rocks are intruded by the large syn- to post-tectonic 566-533 Ma Hook Granitoid Suite and by younger post-tectonic syenites, diorites, porphyry granites, granites, diorites and gabbros. The east-northeast trending Mwembeshi Shear Zone (MSZ) runs along the southern margin of the Hook Granitoid Suite. The geology of the Kitumba deposit area is shown in Figure 11. . Figure 10: Geological Map of Kitumba Deposit (after Intrepid Mines Limited, 2014). 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 20 The northern part of the license is underlain by metasedimentary rocks of the middle to lower Kundelungu Group of the upper Katanga Sequence. These comprise carbonates and calc-arenites interlayered with shales and siltstones. The western and southwestern part of the license area is dominated by intrusive granitoids of the Hook Granitoid Suite. The deposit is hosted within a hematite-dominated breccia system which is developed along the Kitumba Fault Zone (KFZ) and which outcrops as a prominent north-south trending ridge forming part of the Kitumba Hills. Three principal rock type associations are recognised at Kitumba. Kundulungu Group calcareous siltstones and argillites are intruded by quartz-feldspar porphyry granite. These rocks are in turn extensively intruded by a feldspar porphyry diorite/syenite complex. The system is zoned from north to south, with deeper level magnetite dominated alteration south of Kitumba to the Sugar Loaf deposit (3.8 km southwest of Kitumba) and higher level hematite dominated alteration over Kitumba itself. These correspond to magnetic highs and lows, respectively. Copper mineralisation at Kitumba comprises a simple hypogene sulphide assemblage that is extensively overprinted by a complex largely redistributed supergene oxide assemblage. Kitumba represents a deeply weathered IOCG system with weathering and oxidation extending up to 500 m depth. Deep weathering is particularly pronounced in the vicinity of the KFZ and zones of high fracture intensity, where leaching of sulphides has generated acid, resulting in a porous and vuggy core, whilst iron is largely preserved. Hypogene mineralisation at Kitumba mainly occurs as disseminated pyrite and subordinate chalcopyrite, associated with stockwork veining and brecciation. Semi-massive concentrations of pyrite ± chalcopyrite are observed in places and are mostly concentrated beneath the richest supergene mineralisation adjacent to the KFZ. Primary sulphides are largely preserved within iron carbonate altered zones, sometimes relatively shallow, where carbonate has acted as a buffer preserving hypogene assemblages. A significant proportion of the mineralisation occurs in the form of secondary copper minerals withinthe supergene zone. Supergene enriched material is concentrated from 200 m below surface where it occurs as chalcocite +/- malachite, pseudomalachite, cuprite, native copper, and copper wad. The distribution of secondary copper minerals is related to remobilisation of copper; with secondary copper minerals commonly occurring along fractures and as linings in cavities. A section through the deposits is shown in Figure 11 and the geophysical properties of the lithologies tabulated in Table 3. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 21 Figure 11: The geological section of Kitumba deposit and its geophysical properties (after Intrepid Mines Limited, 2014). Table 3: Gravity and Magnetic properties of the Kitumba Deposit (after Intrepid Mines Limited, 2014). Lithology Estimated thickness (m) Density (gu) Mag Sus (x 10 -3 ) SI Laterite 45 1.92 0.5 Iron Oxide 70 5.18 60000 Quartz-feldspar granite 170 2.64 2.5 Feldspar Porphyry syenite >500 2.74 60 Breccia 80 3.96 0.0004 3.5 The Konkola Deep Deposit 3.5.1 Geographic Location The Konkola Deep deposit is located in Chililabombwe in the Copperbelt Province of Zambia about 30km from the town of Chingola. Konkola Deep deposit has coordinates (#Location: - 12° 22' 45"S, 27° 49' 45"E). 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 22 3.5.2 Tectonic Setting The Konkola section of the Zambian Copper Belt comprises a near continuous, NW-aligned, close to 20 km long by 2 to 4 km wide ribbon of ore within the Neoproterozoic Lower Roan Subgroup. It extends from the northern margin of the regional 'Kafue Anticline' basement block, and is down-folded, to emerge again on the rim of the Konkola basement dome to the northwest. 3.5.3 Geology of Konkola Deep Deposit This deposit is typically known as the Bancroft. The geology of this area is characterized by the higher grounds of Konkola being underlain by beds of the Basement Complex and lower roan group, and the low-lying country is underlain by a succession of shales and dolomites of the Upper Roan, Mwashia and Kundelungu Groups (Figure 13). A section through the deposits is shown in Figure 14 with the geophysical properties of the lithologies tabulated in Table 4. Figure 12: Geological map of Konkola Deep deposit and the surrounding area (after Porter GeoConultancy, 2014). A B 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 23 Figure 13: The geological section through A-B of Konkola Deep deposit (after Porter GeoConultancy, 2014). . Table 4: Gravity and Magnetic properties of the Konkola Deep deposit (Telford el at, 1994). Geology Thickness (m) Density (gu) Magnetic Susceptibility (x 10 -3 )SI Mwashya Subgroup 300-600 2.80 1.03 Upper Roan Supgroup dolostone 100-450 2.42 0.23 Shale and Grit 40-160 2.42 0.37 Hangingwall Aquifer dolostone 15-75 2.42 0.23 Hangingwall Quarztite 10-150 2.6 4 Ore Shale 0-60 2.87 0.95 Footwall Conglomerate 0-35 2.5 0.35 Footwall Sandstone 0-20 2.35 0.4 Porous Conglomerate 15-50 2.5 0.35 Argillaceous Sandstone 5-20 2.35 0.4 Footwall Quartzite 0-300 2.6 4 B A 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 24 3.6 The Chambishi Main Deposit 3.6.1 Geographic Location Chambishi area has three deposits namely: Chambishi Southeast, Chambishi West and Chambishi Main deposits. These deposits are ~360 km north of Lusaka and 28 km NW of Kitwe. Chambishi Southeast deposit is centred on a point ~10 km NW from the Mindola mine, while the Main and West deposits, which are separated by a narrow barren gap, are a further ~7 km to the NW, coordinates (#Location: 12° 39' 36"S, 28° 3' 21"E). 3.6.2 Tectonic Setting The Chambishi deposits are hosted by the Neoproterozoic Lower Roan Group Ore Formation of the Katanga Supergroup, within the Chambishi-Nkana basin, located on the mid-southwestern flank of the 'Kafue Anticline'. 3.6.3 Geology of Chambishi Main Deposit The geology of this area is characterized by an exposed sequence of the Katanga Super group and the Basement Rocks in the flanks(Figure 15). The Lower Roan Group hosts the Ore Formation around Chambishi. The Ore Formation has an averages 30 m thickness near-surface, thinning to 20 m down-dip, and to 6 m over granite basement highs. It consists of fine-grained biotite-quartz argillite with a basal zone that is strongly contorted, schistose, carbonate-rich, cut by quartz-dolomite-anhydrite veins and containing coarse aggregates of bornite and chalcopyrite. Associated quartz veins carry the same sulphide minerals. Above the basal zone, ore occurs as finely disseminated bornite and chalcopyrite, grading down-dip and up-section into pyrite. The Lower Roan Group is strongly deformed in the vicinity of Chambishi with the Chambishi Monocline as the main structure. Most intense folding occurs in the Ore and Hangingwall Formations. The orebodies pinch-out down dip corresponds to a change in the gradient of the footwall thickness. Chalcopyrite is the dominant Cu sulphide with minor bornite. Pyrite and pyrrhotite are typical co-existing gangue phases. Co mineralisation is unevenly distributed within the Cu orebody and present as Co-pyrite and carrollite. A section through the deposits is shown in Figure 16 with the geophysical properties of the lithologies tabulated in Table 5. 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 25 Figure 14: The geological map of Chambishi deposits (modified after Croaker, 2011). Figure 15: Representative cross section through the Chambishi Main deposit(modified after Croaker, 2011). A B B A 2014- 2015 [GENERATING GEOPHYSICAL MODELS TO AID IN COPPER GREENFIELD EXPLORATION] Special Project by Patson Banda Page 26 Table 5: Gravity and magnetic properties of the Chambishi Main deposit (Telford el at, 1994). Geology Thickness (m) Density (gu) Magnetic Susceptibility (x 10 -3 )SI Gabbro 170 3.03 70 Dolostone 200 2.42 2.0 Sandy Talc Schist 75-90 2.5 1 Schist and Quartzite 25 2.62 2.7 Upper Quartzite 12-25 2.6 4 Interbedded Schist and Quartzite 5-25 2.62 2.7 Hangingwall Quartzite 3-12 2.6 4 Copperbelt Ore Member 5-30 2.87 1.5 Mindolo Clastic Formation 0-150 2.48 2.2 Basement Granitoid >300 2.8 2.6 3.7 The Chimiwungo Deposit 3.7.1 Geographic location The Lumwana tenement is located 220 km northwest of the Zambian Copperbelt, and 65km from the provincial capital of Solwezi in the North Western Province of Zambia, (#Location coordinates: 12° 10' 44'' S , 25° 51' 5'' E). Lumwana tenement comprises of three ore bodies of which only two have been proven, these are Chimiwungo and Malundwe deposits. The Lubwe deposit is not economical for mining. 3.7.2 Tectonic Setting The Chimiwungo copper deposit is hosted within the Middle Thrust Sheet domain of the Mwombezhi Dome, one of several basement inliers of early to Mid-Proterozoic age. The basement domes are interpreted as antiformal stacks above mid to lower crustal ramps and consist of granite gneiss, migmatites and schist that vary in metamorphic grade from amphibolite facies in the domes region to green schist facies in the Kafue Anticline (Daly et al., 1984). 3.7.3 Geology of Chimiwungo Deposit The Chimiwungo deposit consists of lenticular horizons of sulphide mineralized kyanite schist that correlate poorly across the deposit. The copper mineralisation is hosted almost entirely within high
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