PHASE EQUILIBRIA AND SOLUBILITY MEASUREMENTS OF GASES IN WATER IN THE HYDRATE FORMATION REGION by Jason Gaudette Department of Chemical Engineering McGill University Montreal, Quebec, Canada July, 2007 A thesis submitted to McGill University in partial fulfillment of the requirements of the degree of Masters of Engineering © Jason Gaudette, 2007 Abstract Gas hydrates are a topic of intense investigation primarily due to the vast amount of methane trapped in the form of gas hydrate on Earth and to the possibility of reducing greenhouse gas emissions via the sequestration of carbon dioxide in the form of gas hydrate. In the present study, phase equilibrium relationships of pressure, temperature, and composition in the liquid, vapour, and hydrate phases for the pure propane-water and CO2-CH4 mixed hydrate-water systems have been investigated. In the first part of the study, the concentration of propane dissolved in water in the presence of propane gas hydrates has been measured at temperatures from 274 K to 277 K and pressures ranging from 150 kPa to 350 kPa. Solubility measurements in the absence of hydrate were found to be in agreement with literature values, which predict an increase in solubility as temperature is decreased. In the hydrate formation region, the solubility of propane decreased with decreasing temperature. Therefore, hydrate formation reverses the gas-liquid solubility trend. Results also show that pressure does not have a strong influence on solubility in the presence of gas hydrate. In the second part of the study, phase equilibrium relationships for a 50/50 CH4/CO2 mixed hydrate-water system have been investigated at temperatures between 274 K and 282 K and at pressures of 2000 kPa and 2500 kPa. In the absence of hydrate, solubility of each gas in the aqueous phase decreased with increasing temperature. In the hydrate formation region, solubility of both CH4 and CO2 in water was found to decrease with decreasing temperature. Therefore, ii as previously concluded with single gas systems, hydrate formation reversed the gas-liquid solubility trend for each gaseous component in the mixed hydrate system. Results also showed that pressure did not have a strong influence on the solubility of each component in the presence of mixed gas hydrate. Furthermore, by mole balance, water-free mixed hydrate composition and formation selectivity of CO2 hydrate over CH4 hydrate has been calculated to show that carbon dioxide hydrates do indeed form selectively over methane hydrates in the presence of the 50/50 gas mixture. iii Resumé L’étude des hydrates gazeux est un sujet de recherche très actif dû à la vaste quantité de méthane présente sur Terre sous cette forme ainsi que la possibilité de pouvoir réduire les émissions de gaz à effet de serre grâce à la séquestration du dioxyde de carbone sous forme d’hydrate gazeux. Cette étude présente les différentes relations d’équilibre de phases entre la pression, la température et la composition des phases liquide, vapeur et d’hydrate pour deux systèmes; un système propane-eau et un système CO2-CH4-eau. La première partie de cette étude consistait à déterminer la concentration de propane dissous dans l’eau en présence d’hydrates de propane à des températures et des pressions variant respectivement entre 274 et 277 K et 150 à 350 kPa. Les solubilités mesurées en absence d’hydrates étaient en accordance avec les données de littérature disponibles, prédisant une augmentation de la solubilité avec une diminution de température. La solubilité du propane dans la région de formation d’hydrate a une relation inverse par rapport à la solubilité dans la région gaz-liquide. Conséquemment, la solubilité du propane en présence d’hydrates diminue avec une diminution de la température. Les résultats obtenus montrent également que la pression a une faible influence sur la solubilité en présence d’hydrates gazeux. La deuxième partie de cette étude consistait à étudier les relations d’équilibre de phases pour un système d’hydrates mixte de CH4/CO2 –eau à des températures variant entre 274 et 282 K et des pressions variant entre 2000 et 2500 kPa. En l’absence d’hydrates, la solubilité de chaque gaz dans la phase iv liquide décroissait avec une augmentation de la température. Dans la région de formation d’hydrates gazeux, la solubilité du CH4 et du CO2 dans l’eau diminuait avec une diminution de la température. Similairement à des systèmes avec un seul gaz, la formation d’hydrate gazeux inverse la relation de solubilité gazliquide pour chaque gaz présent pour un système d’hydrate mixte. Les résultats obtenus démontrent également que la pression n’avait pas une influence significative sur la solubilité de chaque gaz en présence d’hydrates gazeux mixte. De plus, la composition sèche en hydrate gazeux et la sélectivité des hydrates de CO2 sur les hydrates de CH4 ont été calculées à l’aide d’un bilan de moles pour démontrer que les hydrates de dioxyde de carbone sont formés préférablement aux hydrates de méthane en présence d’un mélange 50/50 CH4/CO2. v Acknowledgements I would first like to thank Professor Phillip Servio for his supervision throughout my research project. His vast knowledge and innovative mind helped me to overcome numerous difficulties throughout the course of my research. Furthermore, his support and trust in allowing me to work freely and independently is greatly appreciated. I must also thank Professor Arturo Macchi for his guidance and advice in helping me to decide on a field of research that best suited my interests. Next, I would like to thank the members of Servio’s hydrate research team (John, Lindsay, Naomi, Juan, Yeshai, Shadi, Hal, and Sébastien) that I have worked with at McGill over the past two years. In particular, I would like to thank John for his early guidance in the laboratory, André for his help in the construction of the phase equilibrium apparatus and in the acquisition of supplies, Sébastien for his programming skills, and Shadi for his assistance with several phase equilibrium experiments. On a more personal note, I would also like to thank Yeshai, André, and my officemate, Shadi, for their close friendship and personal support. Furthermore, I would like to thank the staff and the excellent graduate student community at McGill University for their philosophical discussions and for enhancing my understanding of chemical engineering. Finally, I would like to thank my family and friends for their continued love and support and in helping to make these past two years a truly remarkable experience. vi Table of Contents 1 Introduction............................................................................................ 1 1.1 Gas Hydrates ........................................................................................... 1 1.2 Hydrate Structure .................................................................................... 5 1.3 Propane Hydrates .................................................................................... 7 1.4 Hydrates of Gas Mixtures ....................................................................... 8 1.5 Thermodynamics - Hydrate Formation and Equilibrium........................ 9 1.5.1 Hydrates of Methane and Carbon Dioxide ..................................... 9 1.5.2 Hydrates of Propane ..................................................................... 11 1.6 Gas Solubility in Water in the Hydrate Formation Region................... 12 1.6.1 Carbon Dioxide Solubility in the Hydrate formation region ........ 14 1.6.2 Methane Solubility in the Hydrate formation region .................... 15 1.6.3 Propane Solubility in the Hydrate formation region .................... 16 1.7 Hydrate Equilibrium for Systems Involving Gas Mixtures .................. 17 1.8 Thermodynamic Modeling.................................................................... 18 1.8.1 Chemical Potential........................................................................ 18 1.8.2 Fugacity of Liquids and Solids ..................................................... 20 1.8.3 Phase Equilibrium (Liquid water-Vapour-Solid hydrate) ............ 21 1.9 Research Objectives.............................................................................. 23 2 Materials and Methods........................................................................ 24 2.1 Reactor Design...................................................................................... 24 2.2 Equilibrium Apparatus.......................................................................... 25 2.3 Data Acquisition ................................................................................... 27 2.4 Additional Equipment ........................................................................... 28 2.5 Materials ............................................................................................... 29 2.6 Experimental Conditions ...................................................................... 30 2.7 Experimental Procedure........................................................................ 31 2.7.1 Three-Phase H-Lw-V Equilibrium................................................. 32 2.7.2 Solubility Experiments .................................................................. 32 2.7.3 Mole Balance ................................................................................ 34 3 Results and Discussion ........................................................................ 36 3.1 Propane Experiments ............................................................................ 36 3.2 50/50 Methane/Carbon Dioxide Experiments....................................... 38 3.2.1 Three-Phase H-Lw-V Equilibrium................................................. 38 3.2.2 Solubility Experiments .................................................................. 40 vii 3.2.3 4 Mole Balance ................................................................................ 43 Conclusions and Recommendations................................................... 44 4.1 4.2 Conclusions........................................................................................... 44 Recommendations................................................................................. 45 References.................................................................................................... 47 Appendix A: Detailed Reactor Schematics .................................................I viii List of Figures Figure 1.1. Basic hydrate cavity (512) and illustration of........................................ 6 Figure 1.2. The two types of cavities unique to Structure H .................................. 6 Figure 1.3. Partial phase diagram for methane (Deaton and Frost 1946). ............ 10 Figure 1.4. Partial phase diagram for carbon dioxide. Upper Line indicates the vapour pressure line for carbon dioxide and lower line indicates three-phase H-Lw-V equilibrium values (Deaton and Frost 1946)................................... 11 Figure 1.5. Overview of the phase equilibria for the water-propane system where Lw represents liquid water, LC3H8 liquid propane, V vapour, H hydrate and I ice. Q1 and Q2 represent the two quadruple points of the system. ................ 12 Figure 1.6. Typical plot of moles consumed vs. time in a hydrate formation experiment..................................................................................................... 13 Figure 1.7. Plot of equilibrium mole fraction as a function of pressure and ........ 15 Figure 1.8. Plot of equilibrium mole fraction as a function of pressure and ........ 16 Figure 2.1. Photograph of hydrate crystallizer...................................................... 25 Figure 2.2. Schematic diagram of the experimental solubility apparatus............. 27 Figure 2.3. Chandler digital gasometer................................................................. 29 Figure 2.4. Partial phase diagram for the propane-water system and experimental conditions for the measurement of dissolved propane in water. The line represents three-phase H-Lw-V equilibrium points (Deaton and Frost 1946). Below the line, gaseous propane and liquid water coexist at equilibrium, and above the line liquid water and propane hydrate may exist at equilibrium. . 31 Figure 3.1. Plot of equilibrium mole fraction of propane, x1, as a function of temperature at 250 kPa, 300 kPa, and 350 kPa respectively (three phase HLw-V equilibrium temperatures are 275.2 K, 276.0 K and 276.7 K respectively).................................................................................................. 37 Figure 3.2. Partial phase diagrams of the CH4-water (Deaton and Frost 1946), CO2-water (Deaton and Frost 1946), and 50/50 CH4/CO2-water systems. The solid points correspond to three-phase H-V-Lw points for the respective system. .......................................................................................................... 39 ix Figure 3.3. Comparison of the experimentally determined three-phase equilibrium for the 50/50 CH4/CO2-liquid water system to the prediction of the van der Waals and Platteuw model (van der Waals and Platteeuw 1959; Sloan 1998). ....................................................................................................................... 40 Figure 3.4. Plot of the equilibrium mole fraction of methane in water for the 50/50 CH4/CO2-liquid water system as a function of temperature at the indicated pressures........................................................................................................ 42 Figure 3.5. Plot of the equilibrium mole fraction of carbon dioxide in water for the 50/50 CH4/CO2-liquid water system as a function of temperature at the indicated pressures. ....................................................................................... 42 Figure 3.6. Comparison of experimental and literature (Sloan 1998) water-free mole fractions of methane in the hydrate phase under three-phase H-Lw-V equilibrium.................................................................................................... 43 x List of Tables Table 3.1. Mole fraction of propane in water, x1, at given temperatures and pressures........................................................................................................ 36 Table 3.2. Comparison of the experimentally determined solubility in the twophase vapour-liquid water region to those calculated using the correlations of Carroll and Mather and Chapoy (Carroll and Mather 1997; Chapoy, Mokraoui et al. 2004).................................................................................... 37 Table 3.3. Mole fraction of CH4 and CO2 in water at given temperatures and pressures a...................................................................................................... 41 xi 1 1.1 Introduction Gas Hydrates Gas Hydrates, or clathrate hydrates, are non-stoichiometric crystalline compounds in which suitable guest molecules are enclosed in a network of hydrogen-bonded water molecules. The water network is stabilized by weak van der Waals forces between the host and the internal guest molecules. Currently, more than 130 different compounds have been found as guests in water clathrates (Sloan 1998). Clathrate hydrates occur naturally within and below the permafrost zone and in sub-sea sediment where the existing pressures and temperatures allow for thermodynamic stability of the hydrate (Sloan 1998). Gas hydrates were discovered in 1810 by Sir Humphry Davy when he observed that a solid compound formed while mixing chlorine with water at 9°C (Davy 1811). This observation was later confirmed by Faraday who concluded that the ratio of water molecules to chlorine molecules was about 10:1 in the solid compound (Faraday 1823). Much of the early work pertaining to gas hydrates involved identifying guest molecules capable of forming hydrates and the pressure-temperature conditions at which hydrate formation occurs. Methane is one such suitable guest molecule, and during the 1930’s, it was recognized that the plugging of natural gas pipelines was often due to the formation of gas hydrates (and not ice) in the natural gas pipeline, causing a major problem for the rapidly growing gas and oil industry (Hammerschmidt 1934). At this time, intense industrial and academic research on gas hydrates commenced with 1 particular focus on phase equilibrium and inhibiting the formation of methane hydrates in natural gas pipelines (Englezos 1993). The next major advance in the field of gas hydrates occurred in the 1950’s when Pauling and Marsh determined the crystal structure of methane hydrates using X-ray diffraction. This initiated the development of a statistical thermodynamic model to predict hydrate formation and equilibrium. First presented by van der Waals and Platteeuw in 1959 (van der Waals and Platteeuw 1959), this model is still used today, though it has been revised numerous times over the past 50 years. Another milestone in the field of gas hydrates was the discovery of hydrates of natural gas in large quantities in the earth’s crust under the ocean and in permafrost regions of the world by Makogon and his coworkers, initiating large-scale hydrate research efforts throughout the world. While the exact amount of methane trapped in hydrates on Earth is uncertain, even conservative estimates are substantial. These estimates indicate that approximately 1016 kg of carbon are trapped in oceanic sediments in the form of hydrates, which far exceeds any existing hydrocarbon reserve on the planet (Buffett 2000). The vast supply of methane in hydrates has stimulated research into the extraction of this energy source and has also raised questions about the role of hydrates in past and present global climate change. There are concerns that if large stores of methane were to become unstable and be released into the atmosphere, it would have a devastating impact on the world’s climate as methane is known to be a strong greenhouse gas with a global warming potential of 21 times that of carbon dioxide (Englezos 2 1993). Furthermore, it has been hypothesized that large submarine landslides could occur as a result of the destabilization of large sub-sea methane hydrate reserves with catastrophic results (Suess, Torres et al. 1999). In addition to the ongoing research efforts to extract methane from hydrate reserves and monitor the release of greenhouse gases from these reserves, many studies have been carried out to explore other applications of gas hydrates. One major benefit of hydrates is their ability to efficiently transport and store of natural gas. Studies have shown that one cubic metre of methane hydrates contains approximately 160 sm3 of natural gas at reasonable temperatures (-10oC to 1oC) and pressures (1 to 10 atm) and it has been demonstrated in literature that it is economically beneficial to transport and store methane in hydrate form rather than to cryogenically cool or compress it (Khokhar, Gudmundsson et al. 1998), which requires both very low temperatures and extreme pressures. Carbon dioxide is another suitable guest molecule that can physically combine with water under the proper thermodynamic conditions to form clathrate hydrates (Englezos 1993). CO2 hydrates are of particular importance to researchers for two reasons. First, the presence of CO2 and water in natural gas streams and oil reservoirs complicates the extraction of natural gas, and second, CO2 is known to be a harmful greenhouse gas that contributes to the depletion of ozone, thus accelerating global warming. Scientists are currently exploring the option of trapping and sequestering carbon dioxide from industrial flue gases in hydrate form in deep ocean sediments to slow the depletion of the Earth’s ozone 3 layer (Ohmura and Mori 1999; Servio and Englezos 2001; Chatti, Delahaye et al. 2005). Gas hydrates have also proven themselves to be a promising separation technology. In the 1960’s, a process was developed to desalinate sea water via the formation of gas hydrates (Knox, Hess et al. 1961). By forming hydrates from seawater and decomposing them in a separate tank, the salt was removed from the water. Also, it is known that hydrates can be used to remove gases from hydrocarbon mixtures. For example, nitrogen and hydrogen sulfide can be separated from methane using hydrate technology. As mentioned earlier, one of the early reasons for studying gas hydrates was the problems they posed to the gas and oil industry. Hydrate plugs are still a persistent problem in industry today and the focus of many research efforts. Natural gas hydrate propagation in pipelines tends to gradually form a plug that separates the pipe into two pressure sections: a high pressure section between the well and the plug and a second section at low pressure between the plug and the recovery division. A blast can occur in the upstream section due to increased pressures, or alternatively, the plug can also behave as a projectile that destroys the pipe or pumping equipment as the pressure difference between the upstream and downstream sections increases (Sloan 1998). Various kinetic, thermodynamic, mechanical, and thermal inhibition processes have been proposed for the prevention of hydrate formation in pipelines, but pipeline blockage by gas hydrates remains a concern in the oil and gas industry. 4 1.2 Hydrate Structure In the 1950’s, x-ray diffraction studies identified the crystal structure of gas hydrates and allowed for the identification of various hydrate structures (Englezos 1993). At this time, two primary naturally occurring hydrate structures were recognized: structure I and structure II. When water networks are formed via hydrogen bonding, the basic cavity created is a polyhedron with 12 pentagonal faces. Structure I gas hydrates are formed when these cavities arrange themselves such that a manner that they are connected at their vertices. Because the basic cavity structure does not allow for precise packing in this manner, the resulting structure is a polyhedron with 12 pentagonal and two hexagonal faces (51262) consisting of 46 water molecules. A typical structure I hydrate guest molecule has a diameter in the range of 410-580pm. Thus, only smaller molecules such as methane, carbon dioxide, and ethane can form structure I hydrates (Englezos 1993). Structure II hydrates are formed when the cavities arrange themselves such that they link together via face sharing. The resulting structure is a polyhedron with 12 pentagonal faces and 4 hexagonal faces (51264) consisting of 136 water molecules. Molecules that form structure II hydrates typically have diameters less than 410pm or greater than 550pm (Englezos 1993). Examples of suitable gust molecules for structure II hydrates are propane and O2. 5 Figure 1.1. Basic hydrate cavity (512) and illustration of Structure I (51262) and Structure II (51264) hydrates Cavaties (Tohidi 2001). In the late 1980’s, a third naturally occurring hydrate structure was proposed by Ripmeester et al, termed structure H (sH) (Ripmeester, Tse et al. 1987). A structure H hydrate has three different types of cavities. Small molecules, such as methane or xenon, occupy the two smaller cavities and act as ‘helper’ gases while larger molecules, such as various neohexanes, occupy the larger cavity. Structure H hydrates require less energy to nucleate and grow than other hydrates, and are therefore the focus of much of today’s research efforts (Servio 2003). Figure 1.2. The two types of cavities unique to Structure H methane hydrates (Tohidi 2001). 6 All three naturally occurring hydrate structures form unit cells consisting of a set number of each of their cages. These unit cells combine to create a crystal. Not every cage in the unit cell has to be occupied by a guest molecule in the formation of a stable crystal. In fact, structures I and II can form stable crystals with gases that are not small enough to occupy the small cage. This means that stable structure I and II hydrates can still form without any of their small cages being occupied, which is not the case with structure H. Structure H requires at least two types of guest molecules to be stable. One guest must be large enough to stabilize the largest cage and this guest is typically a volatile liquid such as neohexane. The remaining guest molecules must be small enough to occupy the remaining two types of cages. Methane and hydrogen sulphide are example of two such guest molecules (Englezos 1993). 1.3 Propane Hydrates It is important to study gas hydrates not only because of the large potential they possess as a future energy source, but also because of the problems they pose to the petroleum industry during the production, transportation and processing of natural gas and oil. While most hydrate research focuses on methane, the primary component of natural gas, propane is another component of natural gas that is known to physically combine with water under correct temperature and pressure conditions to form structure II hydrates. Although propane hydrates form at relatively modest conditions of temperature and pressure when compared to other hydrate formers, their formation has been often overlooked by scientists because of the narrow temperature range between which the formation of propane hydrates 7 can occur. For storage and transportation of liquefied petroleum gases (LPG’s), composed mainly of propane and butane, it is important to know and be able to predict the conditions of hydrate formation in the presence of humidity or ice (Giavarini, Maccioni et al. 2003). 1.4 Hydrates of Gas Mixtures Recently, mixed hydrate systems are becoming a topic of increasing interest to researchers for their ability to separate hydrocarbon mixtures and due to the possibility of methane exploitation via supply of alternate hydrate formers to a hydrate reserve. It is well known that a hydrocarbon mixture (gas or liquid) can be separated by applying thermodynamic conditions that result in the desired fractionization through the formation of hydrates (Ng 2000). For example, acid gases such as hydrogen sulfide and carbon dioxide can be separated from methane using hydrate technology. Also, as an example of the exploitation potential of mixed hydrate systems, it is suggested that in-situ methane in a hydrate reserve can be selectively replaced with carbon dioxide under the correct thermodynamic conditions (Ohgaki, Takano et al. 1996). Furthermore, the formation of CO2 hydrates acts as a heat source as the enthalpy of CO2 hydration exceeds the energy required to decompose a methane hydrate. Therefore, methane hydrate dissociation could be further assisted by the heat supplied from the formation CO2 hydrates (Handa 1986). The net result of the process is the extraction of methane in combination with the semi-permanent storage of carbon dioxide in hydrate form. 8 1.5 Thermodynamics - Hydrate Formation and Equilibrium Thermodynamics is essential to better understand hydrate formation and growth conditions. Most studies in this field focus on finding the minimum conditions (temperature and pressure) necessary for an infinitesimal amount of hydrate in the system to be stable. These conditions are commonly referred to as the incipient hydrate formation conditions (Englezos 1993). In the hydrate formation region, the following phases may be present: solid hydrate, aqueous liquid, non-aqueous liquid, gas and ice. Incipient hydrate formation conditions are typically determined using the isothermal pressure-search method (Deaton and Frost 1946). This experimental procedure requires a hydrate forming system to be kept at a constant temperature while the pressure of the system is slowly increased and monitored for hydrate formation. The experimental pressure at which hydrates begin to form is the equilibrium pressure of the system at the temperature of the system. This procedure can be repeated over a range of temperatures to produce a partial phase diagram in the hydrate formation region. The advantage of this method over a method varying the temperature is that the thermal and mechanical equilibrium can be reached faster following a change in pressure than with a change in the temperature of the system. 1.5.1 Hydrates of Methane and Carbon Dioxide The conditions of formation of methane and carbon dioxide hydrates in water have been known to researchers for many years. Figures 1.3 and 1.4 illustrate partial phase diagrams for methane and carbon dioxide respectively. 9 Both carbon dioxide and methane combine with water to form structure-I hydrates under correct thermodynamic conditions. In the figures below, H-Lw-V lines indicate a series three-phase, solid hydrate-liquid water-vapour, equilibrium points. Below this line, liquid water and gas are in equilibrium (Lw-V), and above this line, hydrate and liquid water may be in equilibrium (H-Lw). 10000 9000 8000 H-Lw-V Pressure (kPa) 7000 H-Lw 6000 5000 Lw-V 4000 3000 2000 1000 0 272 274 276 278 280 282 284 286 288 Temperature (Deg.K) H-Lw-V for CH4 Figure 1.3. Partial phase diagram for methane (Deaton and Frost 1946). 10 6000 5000 LCO2-V Pressure (kPa) 4000 H-Lw-V 3000 H-Lw 2000 Lw-V 1000 0 272 274 276 278 280 282 284 Temperature (Deg.K) H-Lw-V for CO2 L-V for CO2 Figure 1.4. Partial phase diagram for carbon dioxide. Upper Line indicates the vapour pressure line for carbon dioxide and lower line indicates three-phase H-Lw-V equilibrium values (Deaton and Frost 1946). 1.5.2 Hydrates of Propane Propane forms structure II hydrate when combined with water under correct thermodynamic conditions. A partial phase diagram for propane is illustrated in Figure 1.5. In the propane-water system, the location of the two quadruple points occurs at relatively low pressures (PQ1 = 150 kPa and PQ2 = 600 kPa) with the upper quadruple point existing at a relatively low temperature (TQ2 = 279K) in comparison with other hydrate formers (den Heuvel, Peters et al. 2002). The nearly vertical H-Lw-LC3H8 equilibrium line restricts hydrate formation to temperatures just above TQ2. Therefore, while propane hydrate occurs at 11 modest pressures and temperatures, the thin borders of the formation region restrict hydrate formation potential (Giavarini, Maccioni et al. 2003). Figure 1.5. Overview of the phase equilibria for the water-propane system where Lw represents liquid water, LC3H8 liquid propane, V vapour, H hydrate and I ice. Q1 and Q2 represent the two quadruple points of the system. 1.6 Gas Solubility in Water in the Hydrate Formation Region Solubility measurements in the hydrate formation region are of particular importance to researchers because they help us to better understand hydrate formation kinetics, which is essential to the successful design of hydrate relevant processes. A typical hydrate formation curve is presented below in Figure 1.6. The onset of hydrate formation occurs at some time, tb, known as the turbidity time. For the purposes of kinetic modeling, the solubility or amount of gas dissolved in the aqueous phase at the turbidity point, neq, is desired. The 12 difference between the total number of moles consumed at the turbidity time, ntb, and neq is estimated to be the amount of gas consumed in the formation of the hydrate nuclei (Parrish and Prausnitz 1972). Figure 1.6. Typical plot of moles consumed vs. time in a hydrate formation experiment. Several studies have been performed to determine pure component solubility in the hydrate formation region, with particular focus on single component systems involving methane and carbon dioxide. Due to simplicity and lack of available models, a modified Henry’s Law was initially employed to determine gas solubility under H-Lw-V and H-Lw equilibrium (Sloan 1998; Servio and Englezos 2002). However, this approach displayed several fundamental inadequacies in the H-Lw region, and recently, more rigorous solubility experiments and more advanced models have been developed to improve the accuracy of pure component solubility predictions in the hydrate formation region (Hashemi, Macchi et al. 2006). 13 1.6.1 Carbon Dioxide Solubility in the Hydrate formation region In the CO2-water system, under V-Lw equilibrium, the solubility of carbon dioxide in water is known to decrease as system temperature is increased or pressure is decreased. However, in the hydrate formation region, solubility does not follow these same trends. Until recently, the limited experimental data on the solubility of carbon dioxide in the hydrate formation region exhibited contradicting results. Ohmura and Mori reviewed the literature pertaining to CO2 solubility and concluded that the solubility of carbon dioxide in the hydrate formation region should decrease with decreasing temperature (Ohmura and Mori 1999). Servio and Englezos later confirmed this conclusion experimentally and further added that gas solubility is not a strong function of pressure in the hydrate formation region (Servio and Englezos 2001). Figure 1.7 shows experimental results and model predictions for the solubility of carbon dioxide in and around the hydrate formation region (Hashemi, Macchi et al. 2006). Inflection points in the model represent the predicted three-phase H-Lw-V equilibrium points at the indicated pressure. To the right of the inflection point, the system is under twophase V-Lw equilibrium, and to the left, two-phase H-Lw equilibrium. 14 Figure 1.7. Plot of equilibrium mole fraction as a function of pressure and temperature for the CO2–water system in the hydrate formation region (Hashemi, Macchi et al. 2006). 1.6.2 Methane Solubility in the Hydrate formation region In 2002, Servio and Englezos showed that solubility measurements in the methane-water system displayed similar trends as observed with the carbon dioxide-water system in the hydrate formation region (Servio and Englezos 2002). Figure 1.8 shows experimental results and model predictions for the solubility of methane over a temperature range of 274-285K and at pressures ranging from 35 to 65 bar (Hashemi, Macchi et al. 2006). As with carbon dioxide, methane solubility was found to decrease with decreasing temperature and was not a strong function of pressure in the hydrate formation region. 15 Figure 1.8. Plot of equilibrium mole fraction as a function of pressure and temperature for CH4-water system in the hydrate formation region (Hashemi, Macchi et al. 2006). 1.6.3 Propane Solubility in the Hydrate formation region No previous literature exists on the subject of propane solubility in the hydrate formation region. In the vapour-liquid water equilibrium region, Henry’s Law and the correlations of Carroll and Mather and Chapoy for Henry’s constants are typically used to determine equilibrium propane solubility in water (Carroll and Mather 1997; Chapoy, Mokraoui et al. 2004). Henry’s law is shown in equation 1.1 below followed by the correlation of Carroll and Mather and the correlation of Chapoy for Henry’s constant for the propane-water system in equations 1.2 and 1.3. 16 xiw = Pi H iw (1.1) ln( H iw,1 / kPa) = 552.65815 + 0.077514T − 21334.4 / T − 8584949 ln(T ) (1.2) ln( H iw, 2 / kPa) = 552.64799 + 0.078453T − 21334.4 / T − 85.89736 ln(T ) (1.3) In the above correlations, xiw is the mole fraction of propane in water, Pi is the pressure of propane above the liquid in the system, T is liquid temperature, and Hiw,1 and Hiw,2 refer to Henry’s constants obtained using the correlations of Carroll and Mather and Chapoy respectively. These correlations are particularly important in assessing the accuracy and reliability of the experimental procedures proposed in this study. 1.7 Hydrate Equilibrium for Systems Involving Gas Mixtures A better understanding of the kinetics and phase equilibria for mixed hydrate systems is essential to further the study of the exploitation and separation potential of hydrate formation in the presence of gas mixtures. As stated previously, aqueous phase solubility experiments for pure methane and carbon dioxide in water in and around the hydrate formation region have been completed (Ohmura and Mori 1999; Servio and Englezos 2001; Servio and Englezos 2002) and several solubility models have been published to predict pure component solubility in water in the hydrate formation region (Hashemi, Macchi et al. 2006). Also, Ohgaki et al. have studied the phase equilibria of gaseous mixtures of methane and carbon dioxide in the presence of mixed gas hydrate as a function of 17 gas phase composition at a constant temperature of 280.3 K, and determined that the average distribution coefficient of methane between the gas phase and the hydrate phase is 2.5 at this temperature (Ohgaki, Takano et al. 1996). Furthermore, Sloan et al. has developed a model to predict the phase equilibria and mixed hydrate phase composition in the presence of gas mixtures (Sloan 1998). However, very little literature exists on the effect of temperature and pressure on methane and carbon dioxide solubility in water in the presence of mixed gas hydrate. 1.8 1.8.1 Thermodynamic Modeling Chemical Potential The following discussion of chemical potential is in accordance with the multiphase equilibrium text written by JM Prausnitz et al (Prausnitz 1986). In classical thermodynamics, open systems are those that can exchange matter and energy with their surroundings. Therefore, the fundamental equations (for U, H, A, G) of thermodynamics for closed systems, which can be found in any thermodynamics text book, need to be modified to account for the ability of the system to exchange matter. Taking internal energy, U, as an example, we can expand the expression for a closed system to account for the dependency on the amount of each component that is present. Therefore, we write U = U(S, V, n1, n2, …, nc-1, nc) (1.4) 18 where c is the number of components present. Taking the total derivative of the above expression, we obtain c ⎛ dU ⎛ dU ⎞ ⎛ dU ⎞ dU = ⎜ ⎟ dS + ⎜ ⎟ dV + ∑ ⎜⎜ ⎝ dS ⎠V ,ni ⎝ dV ⎠ S ,ni i =1 ⎝ dni ⎞ ⎟⎟ dni ⎠ S ,V ,n j (1.5) The new term, ⎛ dU ⎞ ⎜⎜ ⎟⎟ = μi ⎝ dni ⎠ S ,V ,n j (1.6) is the chemical potential of component i. By repeating the above procedure for enthalpy (H), Helmholtz energy (A), and Gibb’s energy (G), we obtain the following definition for the chemical potential of component i in a mixture, ⎛ dU ⎞ ⎛ dH ⎞ ⎛ dA ⎞ ⎛ dG ⎞ ⎟⎟ ⎟⎟ ⎟⎟ ⎟⎟ = ⎜⎜ = ⎜⎜ = ⎜⎜ μ i = ⎜⎜ ⎝ dni ⎠ S ,V ,n ⎝ dni ⎠ S , P ,n ⎝ dni ⎠ T ,V ,n ⎝ dni ⎠ T , P ,n j j j (1.7) j The chemical potential is an important variable in multiphase equilibrium predictions. 19 1.8.2 Fugacity of Liquids and Solids Fugacity is a variable that accounts for the difference between the chemical potential of interest, µ(P,T), and the chemical potential of the pure component at a reference pressure and temperature. Expressing the chemical potential of a component in a mixture in terms of its fugacity, we can write μ i = RT ln f i + Θ j (1.8) where Θj is a function of temperature. The fugacity of a component in a mixture in either the gas or liquid phase can be written as: RT ln ∞⎡ ⎛ dP ⎞ fi RT ⎤ ⎥ dV − RT ln Z ⎟⎟ = ∫ ⎢⎜⎜ − yi P dn V ⎢ ⎥ i ⎠ T ,V ,n j V ⎝ ⎣ ⎦ (1.9) where Z is the compressibility factor. In order to obtain the fugacity using the above expression, we need an appropriate equation of state written in a pressureexplicit form. Because of its simplicity and its relative success in predicting liquid-vapour equilibrium for methane-water systems, the Trebble-Bishnoi equation of state (Trebble and Bishnoi 1987) is used extensively in equilibrium solubility predictions for gas hydrates. The fugacity of a pure solid is related to the fugacity of a pure liquid by the following 20 c fi = fi sat ⎛ P ν c dP ⎞ ⎟ exp⎜ ∫ i ⎜ sat RT ⎟ ⎝ Pi ⎠ (1.10) where the subscript c denotes the condensed phase. We now have all the tools necessary to solve a three phase equilibrium problem. In the next section, a typical model for three phase, liquid-vapour-hydrate equilibrium is presented. 1.8.3 Phase Equilibrium (Liquid water-Vapour-Solid hydrate) The classic model for determining hydrate equilibrium pressures and temperatures was developed by van der Waals and Platteeuw (van der Waals and Platteeuw 1959) and later adapted by Parrish and Prausnitz (Parrish and Prausnitz 1972) to account for multiple hydrate formers. According to van der Waals and Patteeuw (vdWP), the basic conditions for three-phase equilibrium are that the chemical potential of water in the hydrate phase is equal to that of water in all other equilibrium phases. Δ μwH (T , P, Θ) = μWβ − μWH = μWβ − μWπ = Δ μwπ (T , P) (1.11) where μ wβ (T , P) is the chemical potential of the empty hydrate, which is purely hypothetical since a hydrate requires a guest molecule to form a stable phase, and μ wπ (T , P) is the chemical potential of water in all other equilibrium phases. In their approach, van der Waals and Platteeuw used statistical based on the following four key assumptions: 1. Guest molecules do not distort the hydrate cavity. 21 2. At most, one guest can occupy a hydrate cavity, and a guest cannot diffuse between hydrate cavities. 3. The interaction between guests in neighboring cavities is negligible. 4. Interactions beyond the surrounding water cavity are negligible. Parrish and Prausnitz proposed the following vdWP type model for the calculation of the chemical potential of water in the hydrate phase when one or more hydrate formers are present: μwH − μ wMT = Δμ wL = RT ∑ν m ln(1 + ∑ C mj f j ) − RT ln( x w ) m (1.12) j where νm is the number of cavities of type m per water molecule in the lattice (Sloan 1998), Cmj is the Langmuir constant and fj is the fugacity of component j. Values for the Langmuir constants can be obtained using the correlation of Parrish and Prausnitz. The RT ln( x w ) term is omitted if ice is the co-existing phase. Liquid and vapour phase fugacities can be calculated using an equation of state such as the Trebble-Bishnoi equation of state (Trebble and Bishnoi 1988). Combined with the following expression, taken from the work of Parrish and Prausnitz, it is then possible to determine the chemical potential of water in the equilibrium liquid and vapour phases: 22 P Δμ wπ (T , P) Δμ wπ (T0 , P0 ) T ΔH wπ ΔVwπ = −∫ dT + 2 ∫ RT dP − ln(γ w x w ) RT RT0 To RT Po (1.13) where Δμ wπ (T0 , P0 ) is the reference chemical potential taken at the reference temperature and pressure (T0,P0), usually taken to be the freezing point of water, and ΔH wπ and ΔVwπ are difference in the empty hydrate lattice and the additional water phase for enthalpy and volume (Parrish and Prausnitz 1972). This vdWP type model is used extensively in gas hydrate research for predicting phase equilibrium and modeling kinetic behavior of hydrate forming systems. With an understanding of this model, we now have all the tools necessary to study the phase equilibrium and solubility of pure and mixed gases in water in the hydrate formation region. 1.9 Research Objectives The main objective of this work was to study the phase equilibrium relations for gases in water in the presence of gas hydrate. First, the propane-water system was studied to generate accurate equilibrium solubility measurements of propane in liquid water in the presence of propane hydrate. Next, a 50/50 mixture of methane and carbon dioxide was used to study the phase equilibria of the CH4/CO2-water system in the presence of mixed gas hydrate. Three phase vapourliquid water-mixed hydrate equilibrium points were determined and measurements of each gas dissolved in the aqueous phase were examined to study the behavior of gas mixtures in the hydrate formation region. To complete the primary objectives of this study, many minor accomplishments were necessary: 23 1. Design and construct a crystallizer capable of withstanding pressures above 10,000 kPa. 2. Design and construct an apparatus to measure the phase equilibrium of pure and mixed gases in water in the hydrate formation region. 3. Develop a method to determine dissolved gas concentrations for pure and mixed gases in water in the hydrate formation region. 4. Perform experiments at the selected operating conditions using both propane and a 50/50 CH4/CO2 gas mixture as the hydrate formers. 2 2.1 Materials and Methods Reactor Design At the heart of the hydrate equilibrium apparatus is a high-pressure crystallizer constructed of 316-stainless steel and capable of handling pressures of up to 20,000 kPa. The crystallizer body has a 3 inch internal diameter, 1.75 inch wall thickness, and an internal volume of 550mL. The crystallizer lid is 1.88 inches thick and is secured to the reactor using six ½ inch rods extending from the reactor body and accompanying ½ inch bolts, and a pressure-tight seal is created using a 3-inch OD Buna o-ring. The front and back of the crystallizer contain circular polycarbonate viewing windows that are sealed with 2-1/8 inch OD, ¼ inch thick Buna o-rings (Hercules Bulldog Sealing Products, Dorval, QC). The crystallizer is equipped with a top mount Dyna/Mag magnetic mixer with rpm control capable of agitation at speeds up to 2500 rpm (Pressure Product Industries, 24 Warminster, PA). The mixer is attached to the reactor via a 1.5 inch parallel thread connection and is welded into place to minimize the potential for leaks. The crystallizer contains a total of five 1/8 inch female NPT ports, each equipped with Swagelok 1/8 inch male NPT to 1/8 inch male tube unions. Two of these ports are occupied by Omega high accuracy RTD probes for temperature measurement in the top and bottom of the crystallizer, and the remaining three ports are connected to 1/8 inch stainless steel Swagelok seamless tubing for the purposes of gas and liquid sampling, purging, and introducing liquid and gas into the reactor. Detailed schematics of the crystallizer are shown in Appendix A and a photograph of the crystallizer is shown below in Figure 2.1. Figure 2.1. Photograph of hydrate crystallizer 2.2 Equilibrium Apparatus The primary components of the hydrate equilibrium apparatus are illustrated in Figure 2.2. A variable volume gas feeding reservoir and a Baumann 51000 series low flow control valve (Laurentide Control, Montreal, QC) are 25 connected to the crystallizer and are used to hold the crystallizer pressure constant during experiments. Hydrate formation consumes gas, and therefore, the feeding reservoir must be pressurized higher than the crystallizer pressure throughout experiments so that gas will flow into the crystallizer and replace the gas consumed in hydrate formation. The absolute pressure in the crystallizer and the variable volume is measured using model 3051S Rosemount pressure transducers (Laurentide Control, Montreal, QC), programmed for pressure measurements over a range of 0-13,789 kPa with a reference accuracy of less that 0.065 % of the span. In addition to the crystallizer and reservoir, two additional gas reservoirs exist in the setup: the bias reservoir, and the bias reactor. The bias reservoir is identical to the reservoir but is not connected to the reactor. The reservoir and bias reservoir are pressurized together before experiments begin. Once the temperature and pressure in the reservoir and bias reservoir have equilibrated, the bias reservoir is isolated using a Swagelok 1/8 inch needle valve. The pressure difference between the bias reservoir (or initial reservoir pressure) and the reservoir is monitored using a model 3051S pressure transducer programmed for pressure measurements from 0 to 2000 kPa with reference accuracy of less than 0.065 % of the span. In order to improve the sensitivity of the Baumann control valve, a model 3051S Rosemount pressure transducer, spanned from 0 to 2000 kPa, measures the pressure difference between the bias reactor and the reactor. The bias reactor is a gas reservoir pressurized slightly higher than the crystallizer pressure and isolated using a Swagelok needle valve prior to experimentation. By using a bias reactor and transducer with a span of approximately 1/7 of that of the 26 crystallizer’s pressure transducer, the pressure controller is approximately 7 times more sensitive to pressure changes within the crystallizer. The crystallizer and reservoirs are all immersed in an insulated bath consisting of a 20 % glycol-water mixture. The bath is kept at constant temperature using a chiller that circulates glycol continuously through a 3/8 inch copper coil installed in the bath. The temperature inside the top and bottom of the crystallizer and in the variable volume reservoir is monitored using Omega RTD probes accurate to ±0.3 ºC. Figure 2.2. Schematic diagram of the experimental solubility apparatus. 1: Crystallizer; 2: Mixer; 3: Bias reactor; 4: Bias reservoir; 5: Variable volume feeding reservoir; 6: Propane tank; 7: Positive displacement pump; 8: Vacuum pump; 9: Sample cylinder. 2.3 Data Acquisition In the phase equilibrium apparatus, all pressure transducers and RTD measurements are recorded using a National Instrument data acquisition system 27 containing SCC modules (current and RTDs) for signal conditioning and a PCI data acquisition card with 18 bit resolution. The data is recorded in Labview 7.1 at a rate of 50 000 samples/sec and averaged to get one data point per second. The data is then exported and saved in a Microsoft Excel file. 2.4 Additional Equipment A motorized high pressure positive displacement (HPD) pump (Schlumberger Canada Ltd, Edmonton, AB) is required to displace the gas volume in the reactor at constant pressure in order to achieve two-phase mixed hydrate-liquid water equilibrium. Using a piston-cylinder arrangement, the HPD pump is capable of operating at pressures of up to 140 MPa and has a displacement volume of 5 to 500 mL with a volume resolution as low as 0.005 mL. A high-pressure filter assembly (Millipore, Bedford, MA) is used when necessary to ensure that liquid sample being analyzed does not contain any hydrates. The assembly is capable of withstanding a 20 MPa difference across the filter and removes all particles greater than 10 nm in diameter. A digital gasometer (Chandler Engineering, Tulsa, OK), shown in Figure 2.3 below, is used to measure the volume and temperature of gas expanded from the liquid sample bomb. The gasometer consists of two pyrex chambers of 1000 mL and 2000 mL respectively that can be used separately or in series to give a maximum volume of 3000 mL. A floating piston in each chamber is connected to a rack and pinion that allows for the pistons to be positioned through the use of 28 control knobs. When a sample is expanded into the gasometer, the movement and position of the pistons are monitored using dual digital volume meters calibrated in cubic centimeters. The temperature inside each chamber is monitored using omega thermocouples accurate to ±0.1 ºC. Volume measurements by the gasometer are accurate to 0.2 % of the volume reading. Figure 2.3. Chandler digital gasometer When necessary, a Varian CP-3800 gas chromatograph (Varian Inc., Mississauga, ON) is used to analyze vapour samples from both the reactor and the gasometer. The Varian CP-3800 is equipped with a thermal conductivity detector (TCD) and sample separation is accomplished using a packed column consisting of 80-100 mesh HayeSep® R packing, ideal for the separating mixtures of light hydrocarbons, air, and trace amounts of water. The gas chromatograph is connected to a PC and is operated via Varian’s Galaxie chromatography software. 2.5 Materials For propane experiments, high purity propane gas (MEGS, Montreal, QC) was used as the supply gas in the equilibrium apparatus. For gas mixture experiments, a mixture of 50 % ultra-high purity methane and 50 % ultra-high 29 purity carbon dioxide by mole (MEGS Specialty Gases, Montreal, QC) was used as the supply gas. For all experiments, distilled and deionized water was used as the aqueous phase in the crystallizer. 2.6 Experimental Conditions In both the propane and gas mixture studies, experiments were performed in and around the hydrate formation region to observe the effect of hydrate formation on the equilibrium behavior of the system. Therefore, in order to determine appropriate experimental conditions, accurate phase diagrams must be generated to determine incipient hydrate formation of the system being examined. For the propane-water system, the experimental data of Deaton and Frost was used to determine three phase hydrate-liquid water-vapour equilibrium points. Experimental conditions relative to these points are illustrated in Figure 2.4 below. As explained earlier, the narrow borders of the propane hydrate formation region restrict hydrate formation potential and limit experimental conditions to within a temperature range of only 4 K. 30 400 P /kPa 350 300 250 200 150 273.0 274.0 275.0 276.0 277.0 278.0 T /K Three Phase H-Lw-V Experimental Conditions Figure 2.4. Partial phase diagram for the propane-water system and experimental conditions for the measurement of dissolved propane in water. The line represents three-phase H-Lw-V equilibrium points (Deaton and Frost 1946). Below the line, gaseous propane and liquid water coexist at equilibrium, and above the line liquid water and propane hydrate may exist at equilibrium. For the 50/50 methane/carbon dioxide gas mixture experiments, accurate three-phase mixed hydrate-liquid water-vapour points were required over a temperature range of 274 K to 282 K before appropriate experimental conditions could be chosen. An experimentally determined partial phase diagram for the 50/50 CH4/CO2-water system is presented later along with the experimental pressure conditions for solubility measurements over the above range of temperatures. 2.7 Experimental Procedure For both the propane and gas mixture experiments, the procedure to determine dissolved gas concentrations in water was adapted from the work of Servio and Englezos (Servio and Englezos 2001; Servio and Englezos 2002). For 31 gas mixture experiments, additional incipient phase equilibria experiments and mole balance calculations were required to complete the study of the equilibrium behavior of the 50/50 methane/carbon dioxide-water system. 2.7.1 Three-Phase H-Lw-V Equilibrium For experiments performed using propane as the hydrate former, three phase hydrate-liquid water-vapour points were obtained from the work of Deaton and Frost (Deaton and Frost 1946). Three phase hydrate-liquid water-vapour points for the 50/50 CH4/CO2 gas mixture were determined using the isothermal pressure-search method over a range of temperatures from 274 to 282 K (Deaton and Frost 1946). 2.7.2 Solubility Experiments The hydrate crystallizer was filled with 250 mL of distilled and deionized water. Once the water had reached the desired temperature, supply gas (either pure propane or the methane/carbon dioxide gas mixture) was added to the equilibrium apparatus until the desired pressure was obtained. Next, the variable volume supply reservoir was pressurized to a level above that of the crystallizer to allow gas addition to the reactor in order to maintain constant pressure throughout the experiment. The procedure for the measurement of the concentration of dissolved gas in the bulk aqueous phase was dependent on which region of the phase diagram the experiment was conducted. If the experiment was to be carried out below the three-phase line in the two-phase V-Lw equilibrium region, a liquid sample was collected in an evacuated sample bomb that was removed from the 32 apparatus once it had reached equilibrium. If the experiment was to be carried above the three-phase line in the H-Lw equilibrium region, the gas volume in the reactor must be displaced with water in the reactor while maintaining constant pressure in the presence of hydrates. After equilibrium had been obtained between the liquid water and hydrate phases, a hydrate-free liquid sample was then collected in the evacuated sample bomb for analysis. An analytic flash technique was used to determine the concentrations of supply gas dissolved in the liquid sample (Servio and Englezos 2001; Servio and Englezos 2002). Using the gasometer, the contents of the sample bomb were brought to room temperature and atmospheric pressure. The gasometer accomplishes this by allowing the gas to evolve from the sample bomb into the floating piston where the gas volume and temperature are measured and recorded. The gas was then injected into the gas chromatograph for analysis. The number of moles of gas in the vapour phase within the gasometer was then calculated by niG = y i ,G ( P − PHV 2O ) V Z i RT (3.1) where P, V, R, T, yi,G and Zi are the atmospheric pressure, volume of the vapour in the gasometer, universal gas constant, gasometer temperature, mole fraction of component i in the gasometer, and the compressibility factor for methane or carbon dioxide respectively. Values for Zi were obtained from the TrebbleBishnoi equation of state (Trebble and Bishnoi 1987; Trebble and Bishnoi 1988). PHV 2O is the vapour pressure of water at the vapour temperature. Since the liquid sample volume and the solubility of supply gas in water at room temperature and atmospheric pressure are known (Carroll and Mather 1997; Yaws 2003), we can 33 proceed to calculating the mole fraction of each component, xi,eq, dissolved in the aqueous phase at the experimental conditions using the following mole balance equation xiR, g n H 2O xi ,eq = 1 − xiR, g xiR, g n H 2O 1 − xiR, g + niG (3.2) + ∑ n + n H 2O G i i where xiR, g is the mole fraction of residual gas dissolved in water at the gasometer temperature and atmospheric pressure (Wilhelm, Battino et al. 1977) and n H 2O is the number of moles of water in the sample bomb. Since the volume of the sample bomb was known, n H 2O could be calculated using steam tables (Perry and Green 1997) at the experimental temperature and pressure. 2.7.3 Mole Balance In experiments involving gas mixtures, a simple mass balance was completed to determine the water-free molar composition of the hydrate phase, z CH 4 and z CO2 , respectively (Ohgaki, Takano et al. 1996) under three-phase H-LwV equilibrium. Since both methane and carbon dioxide are known to form structure-I hydrate, it was assumed that hydrates formed from a mixture of methane and carbon dioxide will also be of structure-I. Therefore, a hydration number of q = 6.2 was assumed for the mass balance (Uchida, Hirano et al. 1999). In its most complete form, the mole balance performed on the gas mixture-water system is as follows: nCO 2,t = nCO 2,G + nCO 2, L + z CO 2 * n H (3.3) 34 nCH 4,t = nCH 4,G + nCH 4, L + (1 − z CO 2 ) * n H (3.4) n w ,t = n w , L + q * n H (3.5) y CO 2,G = xCO 2, L = nCO 2,G nCH 4,G + nCH 4,G (dry basis) nCO 2, L nCH 4, L + nCH 4, L + nw, L (3.6) (3.7) where the subscripts t, G, L, H, and w refer to total, gas, liquid, hydrate and water respectively. The above mole balance can be simplified by making two key assumptions. First, it can be assumed that the number of moles of methane and carbon dioxide dissolved in the liquid phase is negligible in comparison to the number of moles of methane and carbon dioxide present in the vapour phase above the liquid and in comparison to the number of moles of liquid water in the aqueous phase. Second, it can be assumed that the number of moles of water in the vapour phase is negligible in comparison to the number of moles of gaseous methane and carbon dioxide and in comparison to the number of moles of liquid water in the aqueous phase. The resulting approximation essentially relates any shift in gas phase composition of the closed hydrate forming system directly to the formation of carbon dioxide and methane hydrates. 35 3 3.1 Results and Discussion Propane Experiments Experiments were conducted over a range of 274 K to 277 K and 150 to 350 kPa in both the vapour-liquid water and hydrate-liquid water equilibrium regions. A series of replicate experiments at each temperature and pressure condition were performed with a maximum absolute average deviation from the mean of 4.6 %. The mean results at each temperature and pressure condition are presented in Table 1 and measurements at 250 kPa, 300 kPa, and 350 kPa respectively are plotted in Figure 3.1 below. Table 3.1. Mole fraction of propane in water, x1, at given temperatures and pressures T/K P/kPa 104 x1 Regiona 274.21 150 1.118 V-Lw 274.18 188 1.440 V-Lw 274.25 200 1.417 V-Lw 275.17 201 1.243 V-Lw 275.15 250 1.502 V-Lw 276.21 250 1.445 V-Lw 274.23 253 1.439 H-Lw 276.20 301 1.702 V-Lw 274.16 301 1.440 H-Lw 275.20 302 1.572 H-Lw 275.20 352 1.572 H-Lw 276.16 355 1.642 H-Lw 274.33 358 1.546 H-Lw a H, Lw, and V refer to solid hydrate, liquid water and vapour respectively 36 2.0 1.8 10 4 x1 250 kPa (H-Lw) 1.6 250 kPa (V-Lw) 300 kPa (H-Lw) 1.4 300 kPa (V-Lw) 350 kPa (H-Lw) 1.2 1.0 274.0 274.5 275.0 275.5 276.0 276.5 T /K Figure 3.1. Plot of equilibrium mole fraction of propane, x1, as a function of temperature at 250 kPa, 300 kPa, and 350 kPa respectively (three phase H-Lw-V equilibrium temperatures are 275.2 K, 276.0 K and 276.7 K respectively). In Table 2, the measurements taken in the vapour-liquid water region are presented and compared to the correlation of Carroll and Mather and the correlation of Chapoy (Carroll and Mather 1997; Chapoy, Mokraoui et al. 2004). As expected, the solubility in the absence of hydrate increases with decreasing temperature and the results obtained are close to literature values. Table 3.2. Comparison of the experimentally determined solubility in the two-phase vapourliquid water region to those calculated using the correlations of Carroll and Mather and Chapoy (Carroll and Mather 1997; Chapoy, Mokraoui et al. 2004). 104 x1(calc)a 104 x1(calc)b 100(x1a - x1)/x1a T/K P/kPa 104 x1 274.18 188 1.440 1.334 1.363 -8.0 274.21 150 1.118 1.063 1.086 -5.2 274.25 200 1.417 1.417 1.447 0.0 275.15 250 1.502 1.690 1.725 11.1 275.17 201 1.243 1.357 1.386 8.4 276.21 250 1.445 1.611 1.644 10.3 a Using Carroll and Mather’s correlation for Henry's constants. b Using Chapoy's correlation for Henry's constants. 100(x1b - x1)/x1b -5.7 -2.9 2.1 12.9 10.2 12.0 37 The results for the solubility of propane in the presence of propane hydrate show that at a given pressure, the solubility of propane in water decreases as the temperature decreases in the hydrate formation region. Therefore, the formation of gas hydrate reverses the gas-liquid solubility trend. This is in agreement with the conclusions of Ohmura and Mori (Ohmura and Mori 1999) and Servio and Englezos (Servio and Englezos 2001; Servio and Englezos 2002). The reason for the reversal in the gas-liquid solubility trend is a subject of much debate. Most recently, it has been suggested that a blockage at the gas-liquid interface by the hydrate and sharp changes in surface tension forces at the gas-liquid and hydrate liquid interfaces upon hydrate formation are responsible for the observed reversal in the gas-liquid solubility trend (Makogon 1997). Furthermore, it can also be seen that solubility is not a strong function of pressure in the hydrate-liquid water equilibrium region. This result is expected as both the hydrate and liquid water phases are condensed phases and are considered to be nearly incompressible. 3.2 3.2.1 50/50 Methane/Carbon Dioxide Experiments Three-Phase H-Lw-V Equilibrium Three-phase equilibrium experiments were carried out to determine threephase points for the 50/50 CH4/CO2 gas mixture- water system over a temperature range of 274 to 282 K. These points are plotted in Figure 3.2 along with the threephase equilibrium points for CH4-water and CO2-water systems respectively. 38 6000 5000 Pressure (kPa) 4000 50-50 Methane-Carbon Dioxide Experiments Carbon Dioxide 3000 Methane 2000 1000 0 272 274 276 278 280 282 284 Temperature (K) Figure 3.2. Partial phase diagrams of the CH4-water (Deaton and Frost 1946), CO2-water (Deaton and Frost 1946), and 50/50 CH4/CO2-water systems. The solid points correspond to three-phase H-V-Lw points for the respective system. The plot in Figure 3.3 compares the experimentally determined threephase equilibrium points to the predicted three-phase equilibrium line obtained using the van der Waals and Platteeuw type model combined with the SoaveRedlich-Kwong equation of state to describe the hydrocarbon fluid phases(Sloan 1998). The conventional van der Waals and Platteeuw model is shown to overestimate three-phase equilibrium pressures for mixed-hydrate formation in the presence of a 50/50 mixture of methane and carbon dioxide. One explanation for this is the ability of carbon dioxide, the larger of the two hydrate formers, to distort and the small cavity in the structure-I hydrate crystal. The result is an increased amount of carbon dioxide in the hydrate phase, leading to a lower pressure of incipient hydrate formation. Recently, several thermodynamic models 39 have incorporated corrections to improve the accuracy of the conventional van der waals and Platteeuw model for gas mixtures (Seo and Lee 2001; Ballard and Sloan 2002) with much success. 6000 5000 Pressure (kPa) 4000 50-50 Methane-Carbon Dioxide Experiments 3000 Model Predictions (Sloan, 1998) 2000 1000 0 272 274 276 278 280 282 284 Temperature (K) Figure 3.3. Comparison of the experimentally determined three-phase equilibrium for the 50/50 CH4/CO2-liquid water system to the prediction of the van der Waals and Platteuw model (van der Waals and Platteeuw 1959; Sloan 1998). 3.2.2 Solubility Experiments Solubility experiments were conducted at the three-phase equilibrium for the gas mixture and in the hydrate formation region. Experimental conditions ranged from 274 to 282 K at pressures of 20 and 25 bar respectively. The results of these experiments are summarized in Table 3.3 and in Figures 3.4 and 3.5 below. 40 Table 3.3. Mole fraction of CH4 and CO2 in water at given temperatures and pressures a T (K) P (bar) xeq,CH4 xeq, CO2 Region 274.5 20 0.0002742 0.001836 H-Lw 275.3 20 0.0002993 0.002064 H-Lw 276.3 20 0.0002997 0.002156 H-Lw-V 278.2 20 0.0002292 0.002177 V-Lw 279.8 20 0.0001689 0.002148 V-Lw 274.2 25 0.0003091 0.001840 H-Lw 277.1 25 0.0003546 0.001973 H-Lw 279.0 25 0.0003677 0.002207 H-Lw-V 280.4 25 0.0002325 0.002214 V-Lw a H, Lw, V are solid hydrate, liquid water and vapour, respectively As shown in Table 3.3, several solubility measurements were taken outside of the hydrate formation region to illustrate the expected trend of decreased solubility with increasing temperature for both methane and carbon dioxide in the absence of hydrate. In the hydrate formation region, results indicate that the solubility of each gas decreases with decreasing temperature. Therefore, the gas-liquid solubility trend is reversed in the hydrate formation region for each gas in the system. This conclusion is in agreement with experiments for pure methane and carbon dioxide (Servio and Englezos 2001; Servio and Englezos 2002) and with the conclusions of Ohmura and Mori (Ohmura and Mori 1999). Also, as with observations for pure component systems, solubility of methane and carbon dioxide does not appear to be a strong function of pressure in the presence of mixed gas hydrate. 41 0.00040 Methane Solubility (mol frac) 0.00035 0.00030 0.00025 20 bar 0.00020 25 bar 0.00015 0.00010 0.00005 0.00000 273 274 275 276 277 278 279 280 281 Tempeature (K) Figure 3.4. Plot of the equilibrium mole fraction of methane in water for the 50/50 CH4/CO2liquid water system as a function of temperature at the indicated pressures. 0.0025 0.0024 CO 2 Solubility (mol frac) 0.0023 0.0022 0.0021 20 bar 0.0020 25 bar 0.0019 0.0018 0.0017 0.0016 0.0015 273 274 275 276 277 278 279 280 281 Tempeature (K) Figure 3.5. Plot of the equilibrium mole fraction of carbon dioxide in water for the 50/50 CH4/CO2-liquid water system as a function of temperature at the indicated pressures. 42 3.2.3 Mole Balance With the liquid and vapour phases fully characterized for the three-phase H-Lw-V solubility experiments at 20 and 25 bar, a mole balance was completed to determine the water-free composition of the hydrate phase, z CH 4 and z CO2 , respectively. The results of the mole balance are shown in Figure 3.6 and were found to be close to theoretical predictions (Sloan 1998). 0.50 0.45 z CH4 (water-free mol fraction) 0.40 0.35 0.30 Experiments 0.25 Prediction of Sloan (1998) 0.20 0.15 0.10 0.05 0.00 276.2K, 20bar 279.0K, 25 bar Figure 3.6. Comparison of experimental and literature (Sloan 1998) water-free mole fractions of methane in the hydrate phase under three-phase H-Lw-V equilibrium. By defining the distribution coefficient of methane in the vapour and hydrate phases as S= yCH 4 * zCO2 yCO2 * zCH 4 (3.8) where y CH 4 , y CO2 , z CH 4 , z CO2 are the moles fractions of methane and carbon dioxide in the vapour and hydrate phases in the crystallizer, it was found that S = 43 2.0 and 1.7 for the 20 bar and 25 bar experiments respectively. Thus, in the presence of the 50/50 gas mixture at the experimental conditions shown in Figure 3.6, methane is approximately two times more likely to distribute itself into the gas phase than the hydrate phase, indicating that methane can indeed be selectively replaced by carbon dioxide in the hydrate phase. This is in agreement with the conclusions of Ohgaki et al (Ohgaki, Takano et al. 1996), who have also concluded that an increase in the fraction methane in the gas phase will result in a proportional increase in the distribution coefficient defined previously. 4 4.1 Conclusions and Recommendations Conclusions The solubility of propane in water in the hydrate formation region was measured using an analytical flash technique for temperatures ranging from 274 K to 277 K and pressures of 150 kPa to 350 kPa. Solubility results show that the amount of propane dissolved in water decreases with decreasing temperatures in the hydrate formation region. Furthermore, solubility was not found to be a strong function of pressure in the hydrate formation region. Also, phase equilibrium relationships of pressure, temperature, and composition of the liquid, vapour, and hydrate phases for the CO2/CH4 mixed hydrate system were investigated at temperatures between 274 K and 282 K and at pressures of 2000 kPa and 2500 kPa. In the absence of hydrate, solubility of each gas in the aqueous phase was shown to decrease with increasing temperature, as expected. In the hydrate formation region, results were found to be in 44 agreement with existing literature on single component systems as the solubility of both CH4 and CO2 in water were found to decrease with decreasing temperature in the presence of mixed hydrates. Therefore, hydrate formation reverses the gas-liquid solubility trend for each gaseous component in the mixed hydrate system. Results also show that pressure does not have a strong influence on the solubility of each component in the presence of mixed gas hydrate. It is hypothesized that a blockage at the gas-liquid interface by the hydrate and sharp changes in surface tension forces at the gas-liquid and hydrate-liquid water interfaces upon hydrate formation are responsible for the observed reversal in the gas-liquid solubility trend in the H-Lw equilibrium region. Also, it is expected that solubility of gas in the liquid phase does not vary with pressure in the H-Lw equilibrium region as both the hydrate and liquid water phases are considered to be nearly incompressible. Finally, using a mole balance, it was determined that the distribution coefficient of methane between the gas and hydrate phase is approximately 2 for the 50/50 gas mixture-liquid water-mixed hydrate system. Therefore, carbon dioxide hydrates do indeed form selectively over methane hydrates in the presence of the 50/50 gas mixture. 4.2 Recommendations Experimentation on the CH4/CO2-water system should be continued. By varying the composition of the supply gas to the system, the equilibrium behavior of the gas mixture could be studied over a range of compositions to determine phase equilibrium and solubility trends as a function of composition. Also, 45 analytical techniques such as Raman spectroscopy should be employed to directly determine the composition of the hydrate phase as a comparison to the mole balance approach used in this study. 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