Seoni
Kim
ac,
Michael P.
Nitzsche
ab,
Simon B.
Rufer
b,
Jack R.
Lake
b,
Kripa K.
Varanasi
*b and
T. Alan
Hatton
*a
aDepartment of Chemical Engineering, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. E-mail: tahatton@mit.edu
bDepartment of Mechanical Engineering, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. E-mail: varanasi@mit.edu
cDepartment of Environmental Science and Engineering, Ewha Womans University, Seoul, 03760, Republic of Korea
First published on 13th February 2023
In recent years, the ocean has come to be recognized as a global-scale reservoir for atmospheric CO2. The removal of CO2 from oceanwater is thus considered a compelling approach to reduce ambient CO2 concentrations, and potentially achieve net-negative emissions. As an effective means of oceanic CO2 capture, we report an asymmetric electrochemical system employing bismuth and silver electrodes that can capture and release chloride ions by faradaic reactions upon application of appropriate cell voltages. The difference in reaction stoichiometry between the two electrodes enables an electrochemical system architecture for a chloride-mediated electrochemical pH swing, which can be leveraged for effective removal of CO2 from oceanwater without costly bipolar membranes. With two silver–bismuth systems operating in tandem in a cyclic process, one acidifying the ocean water, and the other regenerating the electrodes through alkalization of the treated stream, CO2 can be continuously removed from simulated oceanwater with a relatively low energy consumption of 122 kJ mol−1, and high electron efficiency.
Broader contextIndustrial emissions of carbon dioxide are wreaking havoc on the environment as the continuing accumulation of CO2 in the atmosphere leads to rising temperatures and disruption of the global climate patterns. To mitigate this problem, in addition to reducing CO2 emissions from point sources, much attention has been given to negative emissions technologies to remove carbon dioxide directly from the ambient environment, where the very dilute levels of CO2 make removal challenging. The total amount of CO2 emissions partitioning into the oceans rivals that retained by the atmosphere, and thus effective means for its removal could augment the other negative emissions technologies to reduce the environmental burden imposed by this greenhouse gas. Approaches to removing CO2 from oceanwater rely on adjusting the water pH from about 8.1 to less than 7 to ensure that the speciation of dissolved inorganic carbon (DIC) from carbonates and bicarbonates is changed to molecular CO2 which can then be stripped off under vacuum. It is desirable that approaches be identified that do not require addition of chemicals, nor lead to parasitic reactions with the formation of undesirable compounds. For this reason, electrochemical systems have been considered as good options for pH swing in oceanwater since, because the reactions are driven by supplying electrons in a controllable manner, we can avoid chemical use and parasitic reactions. Current studies on CO2 removal from oceanwater have used bipolar membrane electrodialysis (BPMED), although the high cost of bipolar membranes might impede the commercialization of the process, and some of these architectures even present risks of toxic redox-couples leaking into the oceanwater. We propose a new approach based solely on electrochemical modulation of the pH to initially release the CO2 and then to alkalize the treated water before it is returned to the ocean. This approach (i) does not require expensive membranes or addition of chemicals, (ii) is easy to deploy, (iii) does not lead to formation of byproducts or secondary streams, and (iv) requires a lower energy input (122 kJ mol−1) than do other approaches, to the best of our knowledge. In addition, a preliminary technoeconomic analysis which suggests that this ocean capture system can be economically feasible. |
The focus on atmospheric accumulation has not yet been matched by a similar drive to reduce CO2 in oceans and other surface waters, which, since the dawn of the industrial era, have acted as large-scale carbon sinks, absorbing 30–40% of anthropogenic CO2 emissions.21,22 The resulting increased acidification of ocean waters has already led to destruction of coral reefs,23,24 and reduced carbonate ion concentrations harm shellfish and other marine life.25,26 Since the total amount of CO2 emissions partitioning into the oceans rivals that retained by the atmosphere, effective means for its removal could augment the other negative emissions technologies to reduce the environmental burden imposed by this greenhouse gas. The concentrations in oceanwater (on a volumetric basis) are much higher at 100 mg L−1 than that in the ambient air (0.77 mg L−1),27,28 and thus smaller volumes will need to be treated than in DAC, which could provide a processing advantage. Moreover, while direct air capture requires both capture of the CO2 by chemical complexation with a sorbent, and subsequent breaking of these bonds when the CO2 is recovered as a pure gas, only the latter step is needed for CO2 removal from surface waters, which avoids one of the steps usually required for CO2 mitigation from gaseous sources.29–31
Approaches to solving this challenging problem need to be identified that do not require addition of chemicals, nor lead to parasitic reactions with the formation of undesirable compounds. CO2 from the air dissolves in seawater as carbonic acid, which speciates as bicarbonate and carbonate ions by releasing protons according to the reactions32
CO2 + H2O ⇄ H2CO3 ⇄ HCO3− + H+ | (1) |
HCO3− ⇄ CO32− + H+ | (2) |
Since this equilibrium is based on the proton concentration, the dissolved inorganic carbon (DIC) can be converted back to molecular CO2 by simply lowering the pH of the ocean water; the CO2 can be removed as a pure gas by stripping under vacuum. The pH of the treated water can then be raised before it is returned to the ocean, which has the benefit of countering the acidification of the oceans, and fostering the further absorption of CO2 from the atmosphere. The discharge of the CO2-depleted water into the ocean after treatment imposes significant limitations in choosing a method of altering pH.29 For example, modulation of the pH through addition of acid or base raises concerns about residual chemicals affecting the marine ecosystem, as well as the added cost of chemical supplies. For this reason, electrochemical systems have been considered as good options for the pH swing of oceanwater due to their reversibility.29,33,34 Since the reactions are driven by supplying electrons in a controllable manner, we can avoid chemical use and parasitic reactions.31,35,36
To date, two approaches have been proposed for electrochemically driven CO2 removal from seawater: electro-deionization30,34 and electrodialysis.29,33,37–39 In the electro-deionization process, water splitting reactions generating hydrogen and oxygen gases occur at each electrode to modulate the pH, driving CO2 removal from the oceanwater.30,34 However, the high resistivity of the system and high overpotentials for the reactions lead to a high overall process energy consumption. In contrast, bipolar membrane electrodialysis (BPMED) provides a more energy-efficient means to dissociate water molecules.33,38 The water dissociation catalysts embedded in a bipolar membrane enable decomposition of water molecules into protons and hydroxide ions without generating gases,40 dramatically reducing the energy consumption to 242 kJ per mol of CO2 removed.37 The energy efficiency can be further improved by introducing a redox-couple in the electrolyte. By adopting the ferricyanide/ferrocyanide redox pair, Digdaya et al.29 demonstrated energy consumptions as low as 155 kJ mol−1. However, the high cost of bipolar membranes might impede the commercialization of the process, and these architectures present risks of toxic redox-couples leaking into the oceanwater.41
We describe here a new approach based solely on electrochemical modulation of the pH to initially release the CO2 and then to alkalize the treated water before it is returned to the ocean. This approach does not require expensive membranes or addition of chemicals, is easy to deploy, and does not lead to formation of byproducts or secondary streams. The CO2 removal modules can be installed on stationary platforms co-located with wind farms or solar islands in the seas, or on cargo ships plying the oceans; they can also be integrated with on-shore desalination processes to take advantage of the installed water-handling facilities. The captured CO2 can be injected directly from platforms into sub-surface geologic structures for long term sequestration, or used as a feedstock for fuels or for commodity and specialty chemicals production.
A bismuth (Bi) electrode was used in which Bi reacts under an oxidizing potential to form bismuth oxychloride while releasing protons into the oceanwater feed according to the half reaction:47
Bi + Cl− + H2O ⇄ BiOCl + 2H+ + 3e− E° = 0.16 V (vs. SHE) | (3) |
Silver chloride (AgCl) was selected as a counter electrode, because of its low overpotential, rapid kinetics, and high capacity for chloride ions. In ocean water, under reducing conditions, AgCl releases chloride ions without impacting the proton concentration, by the following half reaction:48
AgCl + e− ⇄ Ag + Cl− E° = 0.23 V (vs. SHE) | (4) |
Based on the stoichiometry of the Bi reaction, two protons are released when three electrons are applied, decreasing the pH of the oceanwater to induce the speciation of the DIC toward molecular CO2; simultaneously, three chloride ions are released by the AgCl electrode, but one is lost to the formation of BiOCl. The overall reaction can be expressed as
Bi + 3AgCl + H2O ⇄ BiOCl + 3Ag + 2Cl− + 2H+ ΔE° = 0.07 V | (5) |
From the positive cell potential for the overall reaction, the forward reaction should be spontaneous. Then, on reversal of these reactions, the CO2-depleted oceanwater can be re-alkalized, giving sufficient alkalinity to ocean water to reabsorb CO2, while regenerating the electrodes for the next cycle. This approach, which relies on a swing in chloride ion concentration between two different Cl− capture electrodes, bismuth and silver, to modulate the solution pH, is shown in this paper to have high faradaic efficiency under cyclic flow conditions, with a CO2 capture energy of 122 kJ mol−1.
(6) |
(7) |
(8) |
[CO2(aq)] = KHPCO2 | (9) |
(10) |
(11) |
The initial concentration of aqueous CO2 is constant no matter the pH, and is determined by its partial pressure in the ambient air, PCO2. The concentrations of HCO3− and CO32−, on the other hand, are strongly affected by the proton concentration, and thus the total dissolved inorganic carbon (DIC) concentration is a function both PCO2 and [H+]:
[DIC] = [CO2(aq)] + [HCO3−] + [CO3−] | (12) |
The activity coefficients for the charged species were calculated from the Debye–Hückel extension law:
(13) |
(14) |
As shown in Fig. 2(a), the total DIC of the seawater in equilibrium with the ambient environment is at a concentration of 1.76 mM at pH 8.06, and the relative distributions of HCO3− and CO32− in this solution are 56% and 43%, respectively, under the ionic strength conditions used here. These values are significantly different from those calculated for ideal solution conditions with all activity coefficients set to unity (Fig. S1, ESI†), where the DIC concentration is larger at 2.5 mM, emphasizing the importance of incorporating the strong effect of ionic strength in thermodynamic analyses of CO2 speciation in seawater. It is clear that the total DIC solubility decreases sharply with decreasing pH, so that most of the DIC exists as molecular CO2 when the pH approaches neutral or slightly acidic conditions.
The equilibrium speciation calculated under different charging conditions can be used to estimate the energy requirement for electrochemical modulation of the proton concentration for CO2 desorption. Under constant current operation, the corresponding release rates of Cl− and H+ from the electrodes can be assumed to be constant. Given that net two moles of Cl− are released when three moles of electron flow in the electric circuit, the concentration of Cl− as a function of the applied charge Q can be written as
(15) |
The aqueous feed solution is assumed to be in equilibrium with the ambient environment (containing 420 ppm of CO2), and thus the concentration of molecular CO2 is determined by Henry's Law, while [HCO3−] and [CO32−] are functions of the oceanwater pH, or [H+], as in eqn (10) and (11). Charge neutrality in the solution will then be satisfied through the balance equation
[H+] + [Na+] = [Cl−] + [HCO3−] + 2[CO32−] + [OH−] | (16) |
Since [OH−] is a function of [H+], as determined by the water dissociation constant (Kw = 10−14),32 and the concentrations of the remaining ionic species are also functions of [H+], the overall concentration of dissolved inorganic species in the feed introduced to the electrochemical modules can be determined. This total DIC remains constant at [DIC]0 during charging, which impacts only the relative concentrations of the individual inorganic carbon species, which can be determined from
(17) |
(18) |
(19) |
The changing distributions in the various components as charge transfer occurs are shown in Fig. 2(b). Of particular interest here is the concentration of molecular aqueous CO2 as a function of applied charge, as it is this quantity that will determine the conditions needed for effective stripping from the solution post-charging. Note that at low pH with a total [DIC]0 of about 1.8 mM, the fugacity, or effectively the partial pressure, is approximately 0.07 bar, and thus either a vacuum or a sweep gas must be used to strip the CO2 from the unsaturated solution. The pH is shown as a function of applied charge in Fig. 2(c). Initially, HCO3− and CO32− exist in a 1:0.7 ratio, but the proportion of carbonate quickly decreases− with a lowering of the pH, to generate primarily HCO3−, which then decomposes to form molecular CO2 (or carbonic acid). Because proton release from the electrode is buffered by these combination reactions with HCO3− or CO32−, the relatively slow decrease in pH from 8.0 to about 6.0 is expected Fig. 2(c); when most of the HCO3− has been consumed, the pH drops rapidly, approaching 5.0.
The reverse process is operative during the regeneration step, in which the concentration of Cl− increases linearly with applied charge, and [Na+] again remains constant (Fig. S2b, ESI†). The total DIC concentration is also constant, determined by the residual CO2 remaining in solution following the stripping step; we set it here as 5% of the initial DIC in oceanwater on the assumption that 95% of the DIC is removed by stripping (i.e., [DIC]0 = 0.1 mM for an initial oceanwater DIC of 2 mM). The calculated concentrations of individual inorganic carbon species during the regeneration step, determined from eqn (17)–(19) with [DIC]0 = 0.1 mM, are shown in Fig. 2(d), while the pH is shown in Fig. 2(e). It was assumed that the same total amount of charge was applied to the cell as in the first step to ensure complete regeneration of the electrodes. As the buffer capacity is low for the CO2-depleted oceanwater, the pH increases rapidly to 10 and ultimately reaches 11 by the end of the cycle. The proportion of CO32− in the DIC increases rapidly at the beginning of this process, reaching 99% when 64 C/L of charge is applied.
The electrochemical thermodynamic cycle can be constructed with the half-cell equilibrium potentials calculated according to the Nernst equation:
(20) |
(21) |
(22) |
(23) |
Since the equilibrium electrochemical potentials of the system are determined by the concentrations of H+ and Cl−, and these concentrations are dependent on the charge transferred, the equilibrium cell voltages for the pH decrease and electrode regeneration steps will also depend on the applied charge, as plotted in Fig. 2(f). In the absence of an overpotential, the voltage gap between the two steps was found to be significantly below 1 V, with an estimated thermodynamic minimum energy for the process given by
(24) |
The cell voltage (i.e., difference in potentials between the two electrodes) plateaued at 0.1 V in the first step and between 0.6 and 0.7 V in the subsequent step (Fig. 4(c)), resulting in an average voltage gap of 0.55 V between the two steps. Given that the cell voltage of the BPMED in previous reports is usually above 1 V, this suggests that our proposed electrochemical system can be competitive energetically with the state-of-the-art process. The potential at each electrode was also monitored with a reference electrode during the operation (Fig. 4(d)). The electrochemical potential for the silver electrode was 0.1 V and 0.2 V (vs. Ag/AgCl) in the first and second steps, respectively, showing 0.1 V of potential difference between the two steps. On the other hand, the potential gap for the bismuth electrode was relatively large, 0.45 V calculated from the values of 0 V and −0.45 V (vs. Ag/AgCl) in the first and second steps, respectively. This indicates that the resistance due to the Bi/BiOCl reaction, which is significantly larger than that of the Ag/AgCl reaction, is the primary determinant of the energy consumption in this system. Given that the standard potential of Bi is −0.05 V (vs. Ag/AgCl), the reaction kinetics for the Bi to BiOCl oxidation is quite fast. On the other hand, the kinetics for the reduction reaction (BiOCl to Bi) is sluggish as water dissociation should be involved in the reaction mechanism to generate H+.
Fig. 5(b) shows the measured voltage when the system operated under constant current conditions. A negative current (−1 mA cm−2) was applied for 30 minutes to Cell 1 to decrease pH in the ocean water, while a positive current (+1 mA cm−2) was applied for same amount of time to Cell 2 to increase the pH of CO2-depleted oceanwater. During the operation, the voltage of the charging cell was maintained at 0.7 V, while that of discharging cell was about 0.1 V. The voltage gap between two cells was 0.6 V on average, which is similar to the result shown for the static cell. Fig. 5(c) shows the pH profile during the operation. The pH of the effluent from the cells operating in the acidification mode decreased to 6, indicating that the ocean water was acidified, while in the regeneration cells the pH approached 12, as anticipated. The pH profiles were similar no matter which of the two cells was being used for acidification, and there was no observable decline in performance over ten cycles. When the acidified oceanwater passed through the membrane contactor, the CO2 was stripped out by the nitrogen sweep stream; there was a rapid increase in the measured CO2 concentration to 8000–10000 ppm in the sweep stream when the current was applied to the electrochemical cells, as shown in Fig. S6 (ESI†), from which the average amount of CO2 removed per cycle of 0.0543 mmol, shown in Fig. 5(d), could be calculated, indicating that 87% of the DIC was removed from the oceanwater These calculations allowed for the fact that a small amount of CO2 (about 500 ppm) was released even during the rest period when no current was applied, which was subtracted from the concentration of CO2 released during the operation when estimate the amount of released CO2 in each step that could be attributed to pH modulation. Meanwhile, the pH measured in the re-alkalizing cell effluent reached about 10–11, which is consistent with the thermodynamic calculation (Fig. 2(e)). This value is much higher than the pH of the initial oceanwater, which was about 8, owing to the reduction in buffering capacity after most of the DIC was removed from solution. After discharge of the effluent into the ocean, the solution will be restored to pH ∼8, the typical pH of oceanwater, by absorbing CO2 from the atmosphere.
Fig. 5(e) shows the relative faradaic efficiency (η) and the energy consumption during operation. Based on the stoichiometry of the electrochemical reactions, the theoretical maximum FE is 67%, as two protons are released for every 3 electrons applied to the system. Therefore, the relative η was defined as the η divided by the theoretical maximum η. During the 10-cycle operation, the average relative FE was 90.4%, and 122 kJ mol−1 of energy was expended, on average. Compared to previous studies that had electrochemical energy consumption of more than 155 kJ mol−1, our proposed system is energetically competitive at the applied current densities, with the caveat that these current densities are lower than those used in earlier studies; further development of this process may require increased current densities to reduce total electrode area needed.
The contents of bismuth and silver in the effluent were measured by ICP-MS. No bismuth was detected in the effluent solution, but the content of silver was 0.255 mg L−1. Means for the amelioration of this slow loss of silver will need to be addressed through identification either of other electrode compositions, or of methods to prevent the dissolution of the silver electrode.
Additional tests were carried out using synthetic seawater with the same composition as seawater. As shown in Fig. S7 (ESI†), the amount of released CO2 decreased over the 4-cycle operation, dropping to 31% in the second cycle and further decreasing to 13% after four cycles relative to the first cycle. The reason for the rapid decrease is attributed to possible Mg(OH)2 formation on the electrode surface owing to the high local surface pH relative to that in the bulk flow. This pH difference is due to the establishment of a concentration boundary layer to balance the concentration-driven proton fluxes with the applied reducing current. With a lowered current density (+0.125 mA cm−2) in the regeneration step, the pH difference between the bulk and surface was reduced, and hence also the precipitation of fouling compounds such as Mg(OH)2, culminating in a 96% performance retention in the second cycle and 67% in the fourth. Strategies to enhance the overall stability of these electrochemical systems under more realistic conditions are clearly needed, and will be a focus of our future studies.
Fig. 6(a) shows the COMSOL abstraction of the experimental flow cell, reduced to an equivalent 2D axisymmetric domain to minimize computational intensity while retaining essential transport characteristics. Fig. 6(b) illustrates the corresponding pH distributions during acidification and alkalization operations, with the r-coordinate compressed by a factor of 10 for clearer visualization. Due to the sluggish kinetics of conversion from HCO3− to CO2 relative to H+ diffusion timescales, a sharp reaction front can be observed during forward operation, dividing the channel into a highly acidic (pH ∼ 3.5) top region near the Bi electrode and a region of unaffected seawater near the Ag counter electrode. Prior to alkalization, 95% of DIC buffering capacity has been removed from the cell, resulting in a much smoother pH profile, with inhomogeneities primarily owing to recirculation effects near the inlet.
Fig. 6(c) illustrates the dependence of cell potential on pH experienced at the bismuth electrode, highlighting notable values in the system. Losses in performance due to variations in open circuit potential throughout the channel can be formulated as a concentration overpotential:
ηk = |ΔΦeq([H]surf) − ΔΦeq([H]bulk)| | (25) |
Fig. 6(d) indicates the total measured overpotential experienced by the bismuth electrode in the real system relative to the inlet conditions, compared to average calculated concentration overpotentials relative to the inlet and channel cross section. Acidification calculations suggest that a significant portion of the Bi overpotential during this step might be due to an excess concentration of protons at the bismuth surface, whereas spatial variations in concentration likely only account for only a small portion of the re-alkalization overpotential. Mixing is therefore an important consideration in a real system, as improving the spatial uniformity of conversion of DIC to CO2 at a pH closer to 6 could improve energetics in the acidification step.
vQ = IaεSz | (26) |
(27) |
We can use a similar analysis to look at the regeneration modules, and explore scenarios for the reduction of the final pH in these modules. In many cases, it would be desirable to ensure that the pH did not reach levels of 9.5 or greater at which precipitates of, say, Mg(OH)2, form, which may foul the electrodes and reduce the overall efficiency of the process. A strategy to overcome this limitation would be to mix the decarbonated solution with fresh oceanwater as shown in Fig. 7(e) so that the residence time restrictions can be disentangled from the current density needs, and, moreover, the buffering capacity of the bicarbonate solution may limit the overall increase in pH. In Fig. 7(f) we illustrate the results from such a mixing of the acidified, decarbonated stream with fresh oceanwater in different proportions, which has the effect of increasing slightly the pH of the feed to the regeneration unit, but also decreases the required residence time in the unit for constant total charge transferred (i.e., constant Ia). With increasing addition of ocean water, the pH of the regeneration stream decreases, which is the desired effect. Since this increase in volumetric flow to the unit would be at the expense of added pumping costs, however. This simple model provides added insight into different operational strategies, but will need to be augmented with more detailed analyses that account for transport and other kinetic limitations within the cells, a topic for future studies.
For the electrochemical system, cost estimates for the cell stack capital expenditures (CAPEX), cell stack electricity costs, and pumping capital and operating costs are shown in Fig. 8(a). The CAPEX of the Bi/AgCl electrode cell stack at scale is estimated using alkaline water electrolyzer costs adjusted for our process specifics. Cell electricity costs are calculated using the experimental 122 kJ mol−1-CO2 as the base required energy and adding ohmic losses through the electrolyte which become relevant at high current densities and large cell gaps. Pumping investment and operating costs are calculated given the flow rate and pressure drop through the cells. Detailed calculations and assumptions can be found in ESI.†
The model cell stack operational current density and electrode gap are varied in the TEA as shown in Fig. 8(b), highlighting some key physical system design tradeoffs. At low current densities, large electrode areas are required and cause cell CAPEX costs to dominate. Beyond 76 mA cm−2, additional benefits from increasing current density are outweighed by increased ohmic losses through the oceanwater and increased pumping costs due to higher required flow velocities. Pumping costs dominate for slim electrode gaps, while ohmic losses drive costs at large electrode gaps, resulting in an optimum at 1.1 mm. The minimized system cost at these optimized parameters is $56 per tCO2 with cost components shown in Fig. 8(c).
The balancing act between the current density, gap width, and pumping costs is generalizable to all electrochemical DOC systems with flow between parallel electrodes, including electrodialysis systems. A notable effect of this interplay is the constraint of the current density to a value much lower than the >1 A cm−2 typically sought for large-scale industrial electrochemical plants.50–53 The inflexibly low conductivity of oceanwater and extremely high required oceanwater throughput are fundamental characteristics which elevate the relevance of electrolyte ohmic losses and limitations on the cell gap for current DOC systems compared to other large-scale electrochemical technologies. To the best of our knowledge, this effect has not been explored in previous technoeconomic or system analyses, which assume operation at higher current densities in excess of 100's of mA cm−2.
However, these physical tradeoffs reveal avenues for continued system cost reduction. Moving away from parallel-electrode architectures towards alternatives such as inter-digitated electrodes could decouple the opposing nature of electricity costs and pumping costs. With such a design, larger cell gaps which minimize pumping costs could be attained while keeping ohmic losses low and allowing higher current density operation. Though our base energy consumption of 122 kJ mol−1-CO2 is a record-low, it may still be substantially decreased towards the thermodynamic limit of 32 kJ mol−1-CO2. Finally, high cell stack CAPEX costs at low current densities motivate the development of electrodes which operate efficiently at higher current densities by mitigating the overpotentials shown in our transport modeling.
The $56 per tCO2 initial cost estimate of our asymmetric electrochemical pH-swing system is comparable to that of electrodialysis system costs under the same assumptions.29 The promising energetics of our process yield lower cell electricity costs, though our initial investment CAPEX estimates are slightly higher (see ESI† Note S3). However, our analysis does not account for replacements and O&M costs which we expect to be significantly lower for our system involving only two electrodes, no redox couples, and no membranes which typically require frequent replacement. The reduced part count and simplicity of our system is promising for its scalability.
Our electrochemical system cost estimates fall within commonly accepted targets of $100 per tCO2,54 but other system costs are critical to evaluate as well. Previous analyses indicate that intake filtration, pumping and gas separation costs may incur total process costs as high as $2000 per tCO2.29,37 At present, these costs dominate those associated with the electrochemical system and motivate further work in reducing degassing costs and pumping costs in addition to electrochemical improvements.
For convenience, in the small demonstration unit a nitrogen sweep gas was used to emulate the drawing of a vacuum for disengagement of the CO2 (at a fugacity of ∼0.07 bar) from the acidified water, since the partial pressure of CO2 in the sweep stream will be on a par with the actual pressure of pure CO2 obtained under vacuum degasification at, say 0.01 bar. As with other published processes for CO2 removal from ocean waters, this low-pressure CO2 would need to be compressed either for use as a feedstock for production of chemicals, materials and fuels, or for sequestration in sub-surface geologic formations.
The techno-economic analysis shows that this ocean capture system can be economically feasible with costs ranging from $50–$100 per ton CO2 depending on the current applied and the gap between electrodes, and could be lowered to $56 per ton CO2 under optimized conditions. However, these calculations only considered the economic feasibility of the electrochemical system itself, and it is necessary to perform an integrated analysis, including other equipment such as intake systems, gas separations, and compression.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: https://doi.org/10.1039/d2ee03804h |
This journal is © The Royal Society of Chemistry 2023 |