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Article

Phase Equilibria of the CH4-CO2 Binary and the CH4-CO2-H2O Ternary Mixtures in the Presence of a CO2-Rich Liquid Phase

by
Ludovic Nicolas Legoix
1,2,*,
Livio Ruffine
2,*,
Jean-Pierre Donval
2 and
Matthias Haeckel
1
1
GEOMAR, Helmholtz Centre for Ocean Research Kiel, Wischhofstr. 1-3, D-24148 Kiel, Germany
2
Institut Français de Recherche pour l’Exploitation de la Mer (IFREMER), Centre de Bretagne, Département Ressources physiques et Ecosystèmes de fond de Mer, Unité des Géosciences Marines, BP70, 29280 Plouzané, France
*
Authors to whom correspondence should be addressed.
Energies 2017, 10(12), 2034; https://doi.org/10.3390/en10122034
Submission received: 20 September 2017 / Revised: 27 November 2017 / Accepted: 28 November 2017 / Published: 2 December 2017
(This article belongs to the Section I: Energy Fundamentals and Conversion)
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Abstract

:
The knowledge of the phase behavior of carbon dioxide (CO2)-rich mixtures is a key factor to understand the chemistry and migration of natural volcanic CO2 seeps in the marine environment, as well as to develop engineering processes for CO2 sequestration coupled to methane (CH4) production from gas hydrate deposits. In both cases, it is important to gain insights into the interactions of the CO2-rich phase—liquid or gas—with the aqueous medium (H2O) in the pore space below the seafloor or in the ocean. Thus, the CH4-CO2 binary and CH4-CO2-H2O ternary mixtures were investigated at relevant pressure and temperature conditions. The solubility of CH4 in liquid CO2 (vapor-liquid equilibrium) was determined in laboratory experiments and then modelled with the Soave–Redlich–Kwong equation of state (EoS) consisting of an optimized binary interaction parameter kij(CH4-CO2) = 1.32 × 10−3 × T − 0.251 describing the non-ideality of the mixture. The hydrate-liquid-liquid equilibrium (HLLE) was measured in addition to the composition of the CO2-rich fluid phase in the presence of H2O. In contrast to the behavior in the presence of vapor, gas hydrates become more stable when increasing the CH4 content, and the relative proportion of CH4 to CO2 decreases in the CO2-rich phase after gas hydrate formation.

1. Introduction

CO2 is ubiquitous in geological systems, and is encountered in geofluids in multiple phases (e.g., Lewicki et al. [1], Boiron et al. [2]). Generally, it is either generated by the degradation of organic matter, decomposition of carbonate rock, or post-genetic mantle processes. However, the occurrence of a CO2-rich gaseous, liquid, and gas hydrate phase is typically limited to volcanic systems [3,4,5,6], where it is often accompanied by admixtures of hydrocarbon gases such as CH4. Reconstructing the migration pattern of such fluids from their source within the sedimentary column to their discharge and fate into the H2O column requires a correct understanding of the involved thermodynamic phase equilibria. In addition, as society is increasingly concerned about mitigating CO2 emissions into the atmosphere, understanding the phase behavior of CO2-rich mixtures becomes more important for the design and conception of reliable carbon storage processes. Amongst the processes under investigation, the storage of CO2 in solid gas hydrates by replacing the CH4 from natural accumulations seems to be very promising, since it helps to meet the global energy demand, while reducing net global carbon emissions. CH4 production from gas hydrates coupled to CO2 sequestration has been investigated intensively; e.g., with some laboratory-scale experiments [7,8,9,10,11], and in a field-scale production test [12]. The method involves multiple phase equilibria, where a liquid aqueous and a CO2-rich phase coexist with vapor and solid gas hydrates, depending on the prevailing temperature and pressure conditions.
The present article starts by reviewing the experimental data available for both CH4-CO2 (Table 1) and CH4-CO2-H2O (Table 2) systems at equilibrium conditions involving a CO2-rich liquid phase. Then, the apparatus and approaches used to generate the new data are briefly described. In the third part of the paper, new experimental data will be presented and discussed.
An important requirement for the development of CH4 hydrate production coupled with CO2-sequestration is the knowledge of the contents of H2O and CH4 lost in the liquid CO2. Currently, a lack of CH4 solubility data for the liquid CO2 phase [34] hinders thermodynamic models to accurately evaluate the amount of CH4 that is lost in the liquid CO2 phase for such a production scheme. Few works have measured the phase properties of such mixtures at high pressures and temperatures ranging between 273.15 and 301 K (Table 1). Clearly, more measurements are needed in order to develop accurate thermodynamic models to quantitatively assess the CH4-to-CO2 hydrate conversion process.
Phase equilibria of the CH4-CO2 binary mixture have previously been investigated to determine its phase envelopes and phase compositions as a function of temperature and pressure [34,35]. This binary mixture exhibits a diagram of Type I in the classification of van Konynenburg [32,36]. Thus, in the pressure-composition space, the vapor-liquid equilibrium (VLE) envelopes are characterized by critical points located along a continuous line linking the critical points of CH4 (190.55 K; 4.60 MPa) and CO2 (304.21 K; 7.38 MPa) [37]. However, few data points are available for the CH4-CO2 VLE in the temperature range of 273.15 and 301 K (Table 1). This range is located between the freezing point of H2O and the critical temperature of CO2, and also includes the typical marine conditions favorable for the formation of gas hydrates.
Arai et al. [14] performed the VLE in a glass capillary cell. The pressure was then increased while keeping the temperature constant, and the resulting volume change of the mixture was measured with a cathetometer. The bubble point was determined by analyzing the pressure change with respect to the molar volume due to the vanishing of the vapor phase. Kaminishi et al. [13,38] investigated the VLE inside a high-pressure-stirred cell, and they were able to sample both phases. Xu et al. [15,39] used a similar method as the present work, with a gas chromatograph to analyze liquid and gas sampled from a high-pressure cell. Bian et al. [16] used a static method to analyze both phases and the critical pressure.
The CH4-CO2-H2O ternary system has been studied under multiple phase equilibrium. Al Ghafri et al. [32] did a very interesting study of this mixture at VLE, vapor-liquid-liquid equilibrium (VLLE), liquid-liquid equilibrium (LLE), and hydrate-vapor-liquid-liquid equilibrium (HVLLE). Indeed, in the p–T diagram, the VLLE region delimited by the Quadruple curve, the upper-critical end point (UCEP) curve, and the CO2 vaporization curve has been studied by Al Ghafri et al. [32], with composition measurements for all phases.
The CH4-CO2-H2O ternary system is able to form a CO2-rich liquid phase under relatively higher pressure, and this drastically changes the hydrate stability field in comparison with pure CO2. However, experimental data at hydrate-liquid-liquid equilibrium (HLLE) conditions are scarce (see comprehensive summary in Table 2). Considering experimental data from all authors, the temperatures investigated are between 282.92 and 294 K, with pressures ranging from 4.5 to 494 MPa, and the initial load of CO2 varying from 0.78 to 1 mole fraction. The data below 30 MPa are shown for the HVLLE and the HLLE in Figure 1, together with calculated dissociation curves of gas hydrate for pure CH4 and pure CO2 gas hydrate formers, and vapor pressure of pure CO2 [40].
The occurrence of the CO2-rich liquid phase is possible for such ternary systems with gas hydrates only for CH4 mole fractions of 0-0.225 for the initial CH4-CO2 gas feed [19]. Thus, it is possible to have an upper-quadruple point (Q2) where gas hydrate (H), liquid H2O (LH2O), CO2-rich liquid (LCO2), and vapor (V) phases coexist (HVLLE) [19]. However, for a given temperature, the CH4-CO2-H2O system is able to form a CO2-rich liquid phase under higher pressures than for pure CO2. The quadruple points Q2 for such mixtures are located at higher pressures, shifting the hydrate stability zone towards the high-pressure region accordingly. The Q2 for a CH4 molar fraction of 0.225 has been estimated by Bi et al. [19] to be at 287.9 K and 8.4 MPa. Thus, the Q2 zone is accurately described by several authors [17,18,19,32] (Table 2) (Figure 1, “+” orange symbols).
For temperatures below Q2, or a richer CH4 mole fraction, the area is well described and several stability points of mixed gas hydrates with vapor and aqueous phase, the hydrate-vapor-liquid equilibrium (HVLE), monitoring have been published as reviewed by Kastanidis et al. [41]. The same is true for the gas hydrate stability in the presence of a pure CO2-rich liquid phase (HLLE) (Table 2), whereas data for CH4 admixtures in the CO2-rich liquid phase exists only for 5.9 mol % CH4 (Table 2) [33]. These authors measured gas hydrate dissociation points using an isochoric step-heating method, keeping the H2O mole fraction between 0.53 and 0.57. The present article will also focus on the HLLE region with mixed CH4-CO2-hydrates.

2. Experiments

2.1. Experimental Apparatus

The phase equilibrium experiments were performed with the apparatus described by Ruffine et al. [42], which was modified to accommodate a high-pressure stirrer (minimaster, Premex Reactor AG, Lengnau, Switzerland) (Figure 2). It consists of a cylindrical 316Ti variable-volume high-pressure cell with a 17-4PH stainless steel moving piston (Hand-Operated Pressure Generator with optical cell, SITEC-Sieber Engineering AG, Maur, Switzerland). The cell can be operated at pressures up to 60 MPa, and temperatures ranging between 253 and 473 K. The volume of the cell varies from 20.8 (±0.6) to 65.4 (±0.3) mL. Both ends of the cell are closed by a sapphire window. At the top of the cell, a ROLSITM sampler (Rapid On-Line Sampler-Injector, Armines-CTP/MINES ParisTech, Fontainebleau, France) [43] was connected to a TCD-FID (Thermal Conductivity Detector-Flame Ionization Detector)-coupled GC-MS (Gas Chromatography-Mass Spectrometry) (7890A-5975C, Agilent, Santa Clara, CA, USA), allowing the withdrawal of an aliquot of a selected phase for compositional analysis. The GC-MS data were processed with the MSDChem software and the Chemstation integrator (Agilent, Santa Clara, CA, USA). To avoid condensation or partial vaporization of the sample, both the ROLSITM and the transfer line were heated up to 423 K with a thermal resistance controlled by a West 6100+ interface (ISE Inc., Cleveland, OH, USA). A high-pressure stirrer was connected at the bottom port of the cell to improve the mixing and shorten the time needed to achieve thermodynamic equilibrium. The stirrer speed, set by a 24 V/DC motor, could be varied between 200 and 1500 rpm. A high-pressure metering pump (Optos, Eldex Laboratories Inc., Napa, CA, USA) was used to inject liquids into the cell at pressures of up to 52.5 MPa with an adjustable flow rate of 0.1–10.0 mL min−1. The thermal regulation was achieved using a compact cooling circulator (ministat 230, Huber Kältemaschinenbau AG, Offenburg, Germany) filled with a mixture of H2O/EtOH (50/50 vol %).

2.2. Materials

All gases—pure components or gas mixtures—were supplied by L’Air Liquide. CH4 and CO2 had a claimed purity of 99.99 mol-%, while the standard mixture of CH4-CO2 had a certified composition of 10.04 (±0.20) mol-% of CH4. For all experiments requiring H2O, MilliQ-H2O with a resistivity of 18.2 MΩ cm was degassed prior to the injection.

2.3. Experimental Procedure

For VLE, CO2 was injected first at the desired temperature, followed by the injection of CH4 into the cell until reaching the desired final pressure. Equilibrium was reached quickly by using the stirrer. The composition of the liquid phase was analyzed with the GC.
For gas hydrate experiments, the temperature of the cell was set to 288.15 K and its volume to the maximum. A custom-made CH4-CO2 gas mixture, obtained from pure CH4 and CO2, was used for Mixtures 1, 2, 3, 6, 7, and the standard mixture from L’Air Liquide for Mixtures 4 and 5. The composition of the custom-made mixture was determined by GC. The cell volume was then reduced to form a liquid phase by pressure increase. H2O was injected afterwards, and the temperature was reduced to 276.85 K to allow the formation of gas hydrates. An isochoric stepwise heating procedure [44] with temperature increments of 0.5 K every 5 h was applied to determine the hydrate dissociation conditions. The composition of the CO2-rich liquid phase was measured by discrete sampling during gas hydrate formation and dissociation.

3. Results and Discussion

3.1. CH4-CO2 Binary System

Data at 288.15 and 283.15 K were used to validate the experimental procedure for the VLE study by comparison with those from Arai et al. [14] and Kaminishi et al. [13] (Table 3). Our data agree well with those of both research groups. For the isotherm at 283.15 K, our composition data at 8.08 MPa has a relative deviation from the one of Kaminishi et al. [13] by 2.1 %. Finally, the vapor pressures of pure CO2 for all isotherms were compared to the correlation from NIST [45,46] (Table 3).
Five isotherms were built from experiments performed at a temperature range of 274.15 to 290.15 K (Table 4, Figure 3) to complete the current database (Table 1). When comparing these data points to modelled isotherms [40] based on the established algorithm of Duan [35] which uses the Soave–Redlich–Kwong (SRK) equation of state (EoS), a good fit is obtained. This binary system has also been studied by Vitu et al. [34], using a group contribution approach and the Predictive PR78 EoS model including a temperature-dependent binary interaction parameter of 0.093–0.112.
In this work, a thermodynamic model was developed based on the SRK-EoS and applied to the system CH4-CO2. A temperature-dependent binary interaction parameter kij(CH4-CO2) = 1.32 × 10−3 × T − 0.251 was optimized over the temperature interval corresponding to the experimental bubble points between 274.15 and 290.15 K. A good agreement was also obtained for measurements outside of this temperature range (i.e., for the dew points and at 273.15, 293.4, and 301 K; Figure 3), demonstrating the predictive capability of the EoS. However, the present model does not reproduce the behavior of the system near the critical point with satisfactory accuracy. Thus, provided that the conditions of interest are not close to the critical point, a simple model based on a cubic EoS allows for a good description of the CH4-CO2 mixture at VLE at the temperature and pressure ranges encountered in most of the marine environment of interest for our study (i.e., CO2-rich seeps and gas hydrate deposits on continental margins). This is convenient to implement, for example, into gas hydrate reservoir models where a more sophisticated EoS would increase computational time too much.

3.2. CH4-CO2-H2O Ternary System

Seven gas hydrate dissociation points delimiting the HLLE were measured for CH4 mole fractions of 0.1–0.105 and 0.153–0.154 of the initial gas mixture (Table 5). The experimental data were compared with calculations of the CSMGem program [47]. The program systematically underestimated the gas hydrate dissociation pressure, with absolute deviations up to 7 MPa compared to our experimental data (Table 5). The p–T curve of gas hydrate dissociation of pure CO2 is strongly dependent on the temperature, showing a very steep slope. Likewise, the CH4-CO2 mixed gas hydrate dissociation appears to be strongly dependent on the temperature when no vapor phase is present (Figure 1).
The CH4-to-CO2 concentration ratio (i.e., without considering H2O composition, x*CH4) in the CO2-rich liquid phase decreased when gas hydrate was formed. In order to understand if this change is caused by hydrate formation or simply a p–T -effect, the CSMGem program [47] is here employed on the data (Table 5). Considering a case study with Mixture 2 at 288.15 K and 10 MPa, CSMGem predicts an aqueous and a CO2-rich liquid phase, as is visually observed in our experiments (Table 5). CSMGem computes that CH4 amounts to only 2% of the dissolved gases in the aqueous phase; i.e., x*CH4/(x*CH4 + x*CO2). Indeed, the CO2 is more soluble than CH4 in liquid H2O, and hence CH4 is enriched in the CO2-rich liquid phase when H2O is pumped into the CH4-CO2 mixture (Table 5, x*CH4 without gas hydrate). When the temperature is decreased from 288.15 to 276.85 K, mixed gas hydrates containing a CH4/CO2 ratio of 21/79 should form (CSMGem), thereby reducing the CH4-to-CO2 ratio in the CO2-rich liquid phase, as it was observed in the experiments.
The formation of gas hydrate was visually observed, relatively rapidly after the start of the stirring. Gas hydrates accumulated rapidly in the cell, and the stirrer was then switched off to prevent any damage (Figure 4). It was visually observed that the gas hydrate formed first at the H2O phase interface and then grew in the H2O phase before spreading across the entire surface of the sapphire window, blocking the view (Figure 4).
The time of incipient gas hydrate formation and the stirring conditions are summarized in Table 6 with no evident correlation between time of gas hydrate formation start and initial setup (composition, pressure, stirring speed).

4. Conclusions

Mixtures of CH4-CO2 and CH4-CO2-H2O involving a CO2-rich liquid phase are investigated under p–T conditions typical for marine environments, such as CO2-rich seeps of volcanic origin and gas hydrate deposits suitable for gas production via CO2 injection.
VLE data were measured and modelled with a simple Soave–Redlich–Kwong EoS for the CH4-CO2 system, at conditions between the freezing point of H2O and the critical point of CO2. This model enables, for example, the accurate prediction of how much CH4 is retained in the CO2-rich liquid phase. Subsequently, a set of data on gas hydrate dissociation was measured to evaluate the phase behavior of CH4-CO2 hydrate containing a CO2-rich liquid phase without any vapor phase. The measurements collected in this newly explored phase region (CH4-CO2-H2O HLLE) indicate that the added CH4 increases the stability of the resulting gas hydrates, which is the opposite trend compared to the region where a vapor phase is stable. Moreover, the formation of gas hydrates in this system consequently reduces the CH4 in the coexisting CO2-rich liquid phase.
For a CH4 production scenario under the investigated p–T conditions, this study indicates that mixed CH4-CO2 hydrates are more stable than pure CO2 hydrates, thus allowing the storage of CO2 in mixed gas hydrates under an extended temperature range for a given pressure. In addition, a more accurate model for calculating the CH4 content in the dense CO2 liquid phase is under development, which will improve the mass balancing of reservoir simulations of CH4 hydrate production via CO2 injection and also improve our understanding of the phase behavior of natural liquid CO2 seeps, where CH4 is a common admixture.
The CH4-CO2-H2O system still needs to be further investigated in the phase region presented here, particularly in the HLLE domain at the lower and upper end of CH4 concentrations allowing for a CO2-rich liquid phase. Indeed, already small additions of CH4 drastically affect the gas hydrate stability pressure, whereas high concentrations would provide more insights into the border of the HLLE region.

Acknowledgments

This work was supported by the SUGAR project, funded by the German Ministry of Research (Grant No. 03G0856A), and the ‘Hydrate as Geohazards’ project from the Unité des Géosciences Marines (IFREMER).

Author Contributions

Ludovic Nicolas Legoix and Livio Ruffine conceived and designed the experiments; Ludovic Nicolas Legoix, Livio Ruffine and Jean-Pierre Donval performed the experiments; Ludovic Nicolas Legoix analyzed the data; Ludovic Nicolas Legoix, Matthias Haeckel and Livio Ruffine wrote the paper.

Conflicts of Interest

The authors declare no conflict of interest.

Abbreviations

SymbolUnit
CO2-rich liquid phase composition of molecule iximole fraction
CO2-rich liquid phase composition of molecule i without H2Ox*imole fraction
Vapour phase composition of molecule iyimole fraction
Global composition of molecule i in the systemzimole fraction
Global composition of molecule i in the system without H2Oz*imole fraction

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Figure 1. Available experimental data describing gas hydrate equilibria for the (CH4)-CO2-H2O system in the presence of H-LH2O-LCO2-(V) phases below 30 MPa. HLLE: hydrate-liquid-liquid equilibrium; HVLE: hydrate-vapor-liquid equilibrium; HVLLE: hydrate-vapor-liquid-liquid equilibrium; VLE: vapor-liquid equilibrium.
Figure 1. Available experimental data describing gas hydrate equilibria for the (CH4)-CO2-H2O system in the presence of H-LH2O-LCO2-(V) phases below 30 MPa. HLLE: hydrate-liquid-liquid equilibrium; HVLE: hydrate-vapor-liquid equilibrium; HVLLE: hydrate-vapor-liquid-liquid equilibrium; VLE: vapor-liquid equilibrium.
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Energies 10 02034 g002 550
Figure 2. Sketch of the experimental set-up including the high-pressure cell, modified from Ruffine et al. [42].
Figure 2. Sketch of the experimental set-up including the high-pressure cell, modified from Ruffine et al. [42].
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Energies 10 02034 g003 550
Figure 3. Liquid and vapor phase compositions of the CH4-CO2 mixture between 273.15 and 301 K along eight isotherms: T = 273.15 K (cyan); T = 274.15 K (blue); T = 277.15 K (green); T = 283.15 K (grey); T = 288.15 K (288.5 K for Xu et al. [15] data) (orange); T = 290.15 K (purple); T = 293.4 K (black); T = 301 K (red). Experimental bubble points xCH4 from this work (filled dot), experimental bubble points xCH4 from other authors (empty dot), experimental dew points yCH4 from other authors (cross), critical point (star) [13,14,15,16]. Modelling of the bubble lines (solid-lines) and the dew lines (dotted-lines) is based on the SRK-EoS.
Figure 3. Liquid and vapor phase compositions of the CH4-CO2 mixture between 273.15 and 301 K along eight isotherms: T = 273.15 K (cyan); T = 274.15 K (blue); T = 277.15 K (green); T = 283.15 K (grey); T = 288.15 K (288.5 K for Xu et al. [15] data) (orange); T = 290.15 K (purple); T = 293.4 K (black); T = 301 K (red). Experimental bubble points xCH4 from this work (filled dot), experimental bubble points xCH4 from other authors (empty dot), experimental dew points yCH4 from other authors (cross), critical point (star) [13,14,15,16]. Modelling of the bubble lines (solid-lines) and the dew lines (dotted-lines) is based on the SRK-EoS.
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Figure 4. Photos showing different steps during gas hydrate formation and dissociation with Mixture 2. From left to right: (A) after H2O injection (LH2O-LCO2); (B) just after incipient formation start (H-LH2O-LCO2); (C) ca. 40 min after formation start (H-LH2O-LCO2); (D) ca. 170 min after formation start (H-LH2O-LCO2).
Figure 4. Photos showing different steps during gas hydrate formation and dissociation with Mixture 2. From left to right: (A) after H2O injection (LH2O-LCO2); (B) just after incipient formation start (H-LH2O-LCO2); (C) ca. 40 min after formation start (H-LH2O-LCO2); (D) ca. 170 min after formation start (H-LH2O-LCO2).
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Table
Table 1. Experimental data for the CH4-CO2 binary system at vapour-liquid equilibrium (VLE), between 273.15 and 301 K.
Table 1. Experimental data for the CH4-CO2 binary system at vapour-liquid equilibrium (VLE), between 273.15 and 301 K.
Isotherm Studied (K)Pressure Range (MPa)Number of Data Points (xCH4, yCH4)Reference
273.155.20–8.08(3, 4)[13]
283.156.12–8.08(3, 3)
273.154.15–8.41(3, 9)[14]
288.155.38–8.04(5, 7)
288.505.12–8.15(10, 10)[15]
293.405.73–7.98(13, 13)
301.006.86–7.70(6, 6) + Critical point[16]
274.153.64–8.33(9, 0)This work
277.153.94–8.20(11, 0)
283.154.60–8.08(4, 0)
288.155.17–7.63(4, 0)
290.155.44–7.82(6, 0)
Table
Table 2. Available experimental data for the CO2-H2O binary and CH4-CO2-H2O ternary mixtures involving a CO2-rich liquid phase.
Table 2. Available experimental data for the CO2-H2O binary and CH4-CO2-H2O ternary mixtures involving a CO2-rich liquid phase.
SystemPhasesT (K)CH4 CompositionDataReference
p (MPa)
CO2-H2OH-LH2O-LCO2-V
Point in p-T space		283.19 (±0.46)-9[17,18,19,20,21,22,23,24,25]
4.49 (±0.20)
H-LH2O-LCO2
Line in p-T space		282.92–294.00-61[23,24,25,26,27,28,29,30,31]
4.5–494
CH4-CO2-H2OH-LH2O-LCO2-V
Line in p-T space		283.86–285.560.0517–0.17503[17]
4.930–6.720(yCH4, vapor phase)
283.86–285.760.0596–0.20264[18]
4.930–7.251(yCH4, vapor phase)
283.51–287.040.05–0.2218[19]
4.74–8.37(z*CH4, gas load)
283.90–286.19-5[32]
4.925–7.62
284.150.0591[33]
5.81(z*CH4, gas load)
H-LH2O-LCO2
Surface in p-T space		285.75–286.950.0592[33]
12.25–19.97(z*CH4, gas load)
285.11–288.390.100–0.1547This work
7.17–27.71(z*CH4, gas load)
Table
Table 3. Relative deviation (RD) of solubility data (mole fractions) and vapor pressures (of pure CO2 with xCH4 = 0) between this work and literature values.
Table 3. Relative deviation (RD) of solubility data (mole fractions) and vapor pressures (of pure CO2 with xCH4 = 0) between this work and literature values.
RD %T (K)p (MPa)xCH4Reference
−5.4 (xCH4)288.157.630.1097This work
7.650.1160[14]
−2.1 (xCH4)283.158.080.1732This work
8.080.177[13]
1.7 (p)274.153.640This work
3.580[45,46]
1.8 (p)277.153.940This work
3.870[45,46]
2.2 (p)283.154.600This work
4.500[45,46]
1.6 (p)288.155.170This work
5.090[45,46]
1.9 (p)290.155.440This work
5.340[45,46]
Table
Table 4. Experimental measurements of bubble points (molar fraction of CH4 in the liquid phase) on the CH4-CO2 binary system.
Table 4. Experimental measurements of bubble points (molar fraction of CH4 in the liquid phase) on the CH4-CO2 binary system.
T (K)p (MPa)xCH4T (K)p (MPa)xCH4
274.153.640277.158.020.2005
274.154.110.0166277.158.130.2107
274.154.990.0518277.158.200.2185
274.155.900.0929283.154.600
274.156.600.1284283.155.370.0293
274.157.060.1545283.157.240.1145
274.157.560.186283.158.080.1732
274.158.040.2206288.155.170
274.158.330.2577288.156.620.0566
277.153.940288.156.800.0654
277.154.690.0266288.157.630.1097
277.155.260.0495290.155.440
277.155.970.0817290.156.090.0243
277.156.510.1083290.156.690.0496
277.157.040.1358290.157.270.0772
277.157.510.1643290.157.590.0951
277.157.710.1786290.157.820.1107
Table
Table 5. Experimental data of H-LH2O-LCO2 equilibria (HLLE) for the CH4-CO2-H2O ternary system. Values inside brackets are CSMGem [47] model values applied on the system.
Table 5. Experimental data of H-LH2O-LCO2 equilibria (HLLE) for the CH4-CO2-H2O ternary system. Values inside brackets are CSMGem [47] model values applied on the system.
TitleMix. 1Mix. 2Mix. 3Mix. 4Mix. 5Mix. 6Mix. 7
Composition
Mole fraction		z*CH40.1050.1050.1050.1000.1000.1530.154
zCH40.0310.0430.0380.0290.0520.1030.090
zCO20.2660.3690.3280.2630.4670.5720.492
zH2O0.7030.5880.6340.7080.4810.3250.418
x*CH40.1020.1100.1110.1060.1060.1540.155
without gas hydrate(0.088)(0.108)(0.108)(0.105)(0.102)(0.154)(0.157)
x*CH40.0950.1020.1060.0920.0890.1520.149
with gas hydrate(0.060)(0.072)(0.063)(0.097)(0.073)(0.138)(0.133)
Gas hydrate dissociationT (K)285.11285.90286.93287.77288.39287.24287.61
p (MPa)7.1710.0714.4520.9427.7113.9915.25
(6.33)(7.52)(11.73)(16.54)(20.87)(10.72)(12.08)
Table
Table 6. Incipient gas hydrate time of formation on the CH4-CO2-H2O ternary system.
Table 6. Incipient gas hydrate time of formation on the CH4-CO2-H2O ternary system.
TitleMix. 1Mix. 2Mix. 3Mix. 4Mix. 5Mix. 6Mix. 7
Stirrer rotation speed (rpm)100010001000100100700700
Time of incipient formation (min)18143318101056

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Legoix, L.N.; Ruffine, L.; Donval, J.-P.; Haeckel, M. Phase Equilibria of the CH4-CO2 Binary and the CH4-CO2-H2O Ternary Mixtures in the Presence of a CO2-Rich Liquid Phase. Energies 2017, 10, 2034. https://doi.org/10.3390/en10122034

AMA Style

Legoix LN, Ruffine L, Donval J-P, Haeckel M. Phase Equilibria of the CH4-CO2 Binary and the CH4-CO2-H2O Ternary Mixtures in the Presence of a CO2-Rich Liquid Phase. Energies. 2017; 10(12):2034. https://doi.org/10.3390/en10122034

Chicago/Turabian Style

Legoix, Ludovic Nicolas, Livio Ruffine, Jean-Pierre Donval, and Matthias Haeckel. 2017. "Phase Equilibria of the CH4-CO2 Binary and the CH4-CO2-H2O Ternary Mixtures in the Presence of a CO2-Rich Liquid Phase" Energies 10, no. 12: 2034. https://doi.org/10.3390/en10122034

APA Style

Legoix, L. N., Ruffine, L., Donval, J. -P., & Haeckel, M. (2017). Phase Equilibria of the CH4-CO2 Binary and the CH4-CO2-H2O Ternary Mixtures in the Presence of a CO2-Rich Liquid Phase. Energies, 10(12), 2034. https://doi.org/10.3390/en10122034

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