Characterization Results

The compositions of the NS and IS samples were determined by XRF analysis and are given in Table 1. The SiO₂ in the NS sample was a little lower and MgO was somewhat higher when compared with the chemical formula of sepiolite. In addition, the sample was determined to contain 2.38 wt.% CaO. These results were due to the sample containing magnesite (MgCO₃) and dolomite (MgCa(CO₃)₂) as impurities. Approximately 90% of NS by weight was sepiolite. The SiO₂ content of IS was quite low indicating that it was a low-grade sepiolite ore.

Table 1.

Chemical compositions of NS and IS

The XRD pattern of NS (Fig. 1) conformed to the standard pattern of sepiolite (JCPDS card No.13-0595). No impurities were identified except for small amounts of magnesite and dolomite indicating that the NS sample was a high-purity sepiolite. The sharp peaks in the XRD pattern of NS revealed the well crystallized character of the sample. The main reflection was observed in the 5–9°2θ region. This corresponds to an interlayer distance of about 12.43 Å. The XRD of the IS sample indicated the existence of plentiful dolomite (Fig. 1). The intensity of the 110 reflection, observed at 7.08°2θ, was that from which the interlayer distance was calculated to be 12.49 Å. The variations in d ₁₁₀ spacing of sepiolite have been studied by several researchers (Suarez and García-Romero Reference Suarez and Garcia-Romero2012; Yeniyol Reference Yeniyol2014; Suarez et al. Reference Suarez, Garcia-Rivas, Garcia-Romero and Jara2016). Sepiolite samples from the eastern part of Eskişehir were reported to appear together with other magnesic phyllosilicates and carbonates (dolomite and magnesite). Two distinct forms of sepiolite were distinguished in these samples: a well crystallized sepiolite with a 110 reflection at 12.07–12.3 Å, and a poorly crystallized sepiolite in which the 110 reflection occurs at 12.7–13.0 Å. In the XRD pattern of randomly oriented samples in which smectite predominates, the (001) basal reflection is weak and asymmetric and is centered at 12.5 Å (Yeniyol Reference Yeniyol2014).

Fig. 1.

XRD patterns of NS and IS (S: sepiolite, M: magnesite, D: dolomite)

The data in Table 2 indicate the surface areas, pore volumes, and average pore diameters for the NS and IS samples. The BET specific surface area of NS (182.19 m² g^–1) was three times larger than that of IS (63.78 m² g^–1). In addition, larger micro and total pore volumes of NS showed that the material had a more porous structure.

Table 2.

Textural properties deduced from N₂ adsorption at 77 K for NS and IS

S: surface area; V: pore volume; D _p: pore diameter

The morphologies of the NS and IS samples were also studied by SEM. As seen in Fig. 2, the morphologies of the two sepiolite samples are significantly different. The NS sample showed a more porous and fibrous morphology. Scattered acicular minerals and mineral aggregates were found on the surface of the sample. In contrast, in the photomicrograph of IS, a rough surface with irregular particles of micron and submicron size was observed and most of these particles were subhedral. Small amounts of fibrous particles were also observed on the surface of IS. The fibrous structure of NS continued to exist after the adsorption of Ni but its morphology had changed a little. The SEM images of the Ni-adsorbed IS sample (IS-Ni) indicate smaller particle size than the raw sample (IS). The surface was covered with micrometric particles.

Fig. 2.

SEM images of NS, IS, NS-Ni, and IS-Ni samples. Scale bars are 2.00 μm

Analysis by energy dispersive X-ray spectroscopy (EDS) showed that the NS consisted of Mg, Si, O, and C while the IS consisted of Mg, Si, O, C, Ca, and Al (Fig. 3). The EDS spectra of the NS-Ni and IS-Ni samples illustrated the existence of Ni in the samples, thus proving the adsorption. 3.72% and 2.90% of Ni were detected on NS-Ni and IS-Ni, respectively.

Fig. 3.

EDS elemental analyses of NS, IS, NS-Ni, and IS-Ni samples

The various functional groups in the sepiolite samples (NS and IS) and also in the Ni-loaded samples (NS-Ni and IS-Ni) were measured with FTIR (Fig. 4, Table 3). The IR bands at 3690 cm^–1 for NS and 3687 cm^–1 for IS were assigned to the surface Mg–OH stretching vibration (Eren and Gumus Reference Eren and Gumus2011; Frost et al. Reference Frost, Locos, Ruan and Kloprogge2001). The bands at 3572 cm^–1 for NS and 3564 cm^–1 for IS were related to the stretching modes of water molecules coordinated with Mg ions. The 3421 cm^–1 and 3397 cm^–1 bands for NS and IS, respectively, were attributed to zeolitic water and the band at 3261 cm^–1 for NS was assigned to the coordinated water (Frost et al. Reference Frost, Locos, Ruan and Kloprogge2001; Lazarevic et al. Reference Lazarevic, Jankovic-Castvan, Djokic, Radovanovic, Janackovic and Petrovic2010; Franco et al. Reference Franco, Pozo, Cecilia, Benítez-Guerrero, Pozo and Martín Rubí2014). The bands at 2932 and 2904 cm^–1 were attributed to the C–H stretching vibrations (Alkan et al. Reference Alkan, Tekin and Namli2005). The presence of dolomite and magnesite impurities was confirmed by the bands at 2532, 1452, 884, and 728 cm^–1 for NS and by the bands at 2531, 1822, 1448, 885, and 730 cm^–1 for IS (Lescano et al. Reference Lescano, Castillo, Marfil, Barbosa and Maiza2014; Kıpçak and Isıyel Reference Kιpçak and Isιyel2015; Sabah and Ouki Reference Sabah and Ouki2017; Wu et al. Reference Wu, Zhang, Liu, Zhang and Chung2017). These bands proving the presence of carbonate are in agreement with the results of chemical analysis and XRD patterns given in Fig. 1. The band at 1659 cm^–1 for NS was due to the –OH bending vibrations of zeolitic water (Qiu et al. Reference Qiu, Yu, Song, Wang, Zhong and Tian2013; Sabah and Ouki Reference Sabah and Ouki2017). The bands in the 1250–400 cm^–1 range were characteristic of the silicate structure of sepiolite. The bands observed at 1210, 1077, and 1016 cm^–1 for NS and at 1212 and 1012 cm^–1 for IS were produced by the Si–O vibrations (Eren et al. Reference Eren, Gumus and Ozbay2010; Ahribesh et al. Reference Ahribesh, Lazarevic, Jankovic-Castvan, Jokic, Spasojevic, Radetic, Janackovic and Petrovic2017). The band observed at 784 cm^–1 for NS was the O–H bending vibration of Mg–Fe–OH (Duman et al. Reference Duman, Tunç and Polat2015). The bands at 749 and 747 cm^–1 for NS and IS, respectively, were assigned to the Si–O bonds (Xu et al. Reference Xu, Jiang, Yu, Xu, Liang, Zhou and Hu2017). The band at 471 cm^–1 observed in the spectrum of NS could be attributed to an O–Si–O bending (Lescano et al. Reference Lescano, Castillo, Marfil, Barbosa and Maiza2014; Eren et al. Reference Eren, Gumus and Ozbay2010). The bands at 440 and 427 cm^–1 originated from octahedral–tetrahedral bonds (Si–O–Mg bonds). The bands at 690 and 645 cm^–1 for NS and at 690 and 655 cm^–1 for IS corresponded to the Mg–OH bond vibrations (Lazarevic et al. Reference Lazarevic, Jankovic-Castvan, Djokic, Radovanovic, Janackovic and Petrovic2010; Ahribesh et al. Reference Ahribesh, Lazarevic, Jankovic-Castvan, Jokic, Spasojevic, Radetic, Janackovic and Petrovic2017).

Fig. 4.

FTIR spectra of NS, IS, NS-Ni, and IS-Ni samples

Table 3.

Functional groups in NS, NS-Ni, IS, and IS-Ni samples

Some slight shifts were observed in the IR absorption bands of the samples after Ni²⁺ adsorption (Fig. 4). For the NS sample, the shift in the –OH stretching band after Ni²⁺ adsorption from 3421 to 3424 cm^–1 was attributed to the attachment of Ni²⁺ to the –OH groups. The shift of the band at 1659 to 1661 cm^–1 and the weakening intensity of this band after adsorption indicated the decrease in the zeolitic water content with the replacement of the introduced Ni²⁺ ions. The shift of the 1210 cm^–1 band to 1212 cm^–1 confirmed the involvement of the Si–O bond linkage in the Ni²⁺ adsorption process. For the IS sample, the band of the triple bridge group Mg₃OH shifted from 3687 to 3684 cm^–1. The shift from 3397 to 3419 cm^–1 in the absorption band of –OH stretching vibrations indicated clearly the involvement of the –OH group as active sites for binding of Ni²⁺ cations. The shift in the stretching vibration band of Si–O from 1212 to 1214 cm^–1; and the bending vibration band of Mg–OH from 690 to 685 cm^–1 were also observed. These shifts in the absorption bands suggested that –OH and Si–O groups functioned as adsorption sites for Ni²⁺ ions from solution.

Effect of Adsorbent Dosage

Adsorbent dosage plays a major role in the adsorption process because it determines the capacity of an adsorbent for a given initial concentration of adsorbate. In order to investigate the effect of adsorbent dosage on the efficient removal of Ni²⁺, batch experiments were carried out with 50 mg L^–1 Ni²⁺ solution by varying the adsorbent dose from 0.1 to 1.0 g/50 mL. While the adsorbent dosage increased from 0.1 to 0.6 g/50 mL, the removal percentages of Ni²⁺ ions for NS and IS samples increased from 36.68 to 97.61% and from 36.70 to 99.07%, respectively (Fig. 5). Further increases in the adsorbent dosage up to 1.0 g/50 mL failed to cause any significant change in the removal yields. This behavior may be explained by the increased surface area and effective adsorption sites on the adsorbent surface with increasing adsorbent dosage (Uddin Reference Uddin2017). The optimum adsorbent dosage was chosen, therefore, as being 0.6 g/50 mL for both adsorbents.

Fig. 5.

Effect of adsorbent dosage on the removal of Ni²⁺ ions by NS and IS (pH: 6.0, t: 24 h, C ₀: 50 mg L^–1, T: 25°C). The error bars represent the standard deviation

Effect of Initial pH

The pH of the solution is one of the parameters that has a significant effect on the adsorption of metal ions because the surface charge density of the adsorbent and the metal speciation depend on the pH. The change of pH affected significantly the morphology of Ni species in the solution, which further affected the adsorption process of this metal. The main species of Ni was Ni²⁺ when the pH of the solution was <7.0. When the pH was >7.0, Ni(OH)₂ occurred and its proportion apparently increased with increasing pH (Sheikhhosseini et al. Reference Sheikhhosseini, Shirvani, Shariatmadari, Zvomuya and Najafic2014; An et al. Reference An, Jiang, Nan, Yu and Jiang2019). The effect of pH was studied at various pH values ranging from 2 to 8 (Fig. 6). Ni²⁺ adsorption capacities of both adsorbents increased with increasing pH until 4, and then stayed almost constant. This situation is related to the active sites on the adsorbents. At lower pH values, the concentration of H⁺ ions is high, causing competition between the proton and metal ions for vacant adsorbent sites. The removal efficiency, therefore, is less at lower pH values. Furthermore, when the active sites are protonated, the surface is positively charged and the adsorption of metal ions on the surface is reduced. The final pH values of the solutions after the pH experiments were checked and found to be <7 (for initial pH ≤7) or just above 7 (for initial pH = 8). This meant that the main species of Ni in the solutions were Ni²⁺ ions. Mg–OH and Si–OH groups on the sepiolite (S) surface were reported to play important roles in metal ion adsorption. S–O–Ni⁺ and (S–O)₂–Ni complexes might be formed in the interactions between Ni²⁺ ions and the S–OH surface functional groups (Lazarevic et al. Reference Lazarevic, Jankovic-Castvan, Jovanovic, Milonjic, Janackovic and Petrovic2007). In addition, the clay surface may also be negatively charged providing adsorption sites for metal cations. Accordingly, the Si–O^– groups formed by the break-up of Si–O–Si bonds might be complexed as (Si–O)₂–Ni (Yavuz et al. Reference Yavuz, Altunkaynak and Güzel2003). The original pH value of the Ni²⁺ solution was 6; therefore, this value was chosen as the optimum pH value and applied throughout all of the adsorption experiments. In addition, Ni precipitation was reported to be negligible at pH 6 (Carvalho et al. Reference Carvalho, Vignado and Fontana2008).

Fig. 6.

Effect of initial pH on the adsorption of Ni²⁺ ions by NS and IS (adsorbent dosage: 0.6 g/50 mL, t: 24 h, C ₀: 50 mg L^–1, T: 25°C). The error bars represent the standard deviation

Effect of Contact Time

The time required to achieve equilibrium for the metal ions and adsorbent is very important in the adsorption experiment because it depends on the nature of the system used. The effect of contact time on the adsorption of Ni²⁺ ions was investigated between 15 and 2880 min time intervals at 25, 35, and 45°C (Fig. 7). During short contact times, adsorption was very fast (within 15 min, >50% was adsorbed) due to the presence of numerous active sites on the adsorbent surface. The adsorption rate then decreased because of the decrease in the number of adsorption sites and in the Ni²⁺ concentration gradient. The equilibrium was almost reached in 960 min for NS and 720 min for IS. However, experiments were carried out with 24 h of contact time to achieve equilibrium at the solid/liquid interface and to ensure the best adsorption conditions at higher concentrations (Guerra et al. Reference Guerra, Batista, Correa da Costa, Viana and Airoldi2010).

Fig. 7.

Effect of contact time on the adsorption of Ni²⁺ ions by NS and IS at three temperatures (adsorbent dosage: 0.6 g/50 mL, pH: 6, C ₀: 50 mg L^–1). The error bars represent the standard deviation

Effect of Initial Concentration

The effect of initial concentration on the amount of Ni²⁺ ions adsorbed was studied with varying initial concentrations (50–500 mg L^–1) at three different temperatures of 25, 35, and 45°C. According to the results (Fig. 8), the adsorption capacities of both sepiolites increased with increasing initial Ni²⁺ concentration. This result showed that the initial concentration of Ni²⁺ provided a driving force to overcome the mass transfer resistances between the adsorption medium and adsorbent. With more Ni²⁺ in solution, more active sites of the sepiolites were involved in the adsorption process. Larger ion concentrations enhanced the mass transfer driving force, and increased the equilibrium uptake capacity of metal ions. The adsorption capacity increased also with increasing temperature, indicating that the reaction follows the endothermic pathway. The increase in the adsorption capacity with temperature may be due to various factors such as increase in the inter-reaction between adsorbent and adsorbate, formation of new adsorption sites, and an increasing rate of intraparticle diffusion at higher temperatures.

Fig. 8.

Effect of initial concentration on the adsorption of Ni²⁺ ions by NS and IS at three temperatures (adsorbent dosage: 0.6 g/50 mL, pH: 6, t: 24 h). The error bars represent the standard deviation

Adsorption Kinetics

In order to investigate the controlling mechanism of the adsorption processes, pseudo-first order, pseudo-second order, and intraparticle diffusion kinetics models were applied to the experimental data. The pseudo-first order model was first developed by Lagergren (Reference Lagergren1898). The differential form of the model is described by Eq. 5 (Lagergren Reference Lagergren1898):

(5) $\frac{d{q}_t}{\mathrm{dt}}=k_1\left(q_e-q_t\right)$

where q _e and q _t (mg g^–1) are the amounts of metal ions adsorbed per gram of adsorbent at equilibrium and at any time t (min), respectively, and k₁ (min^–1) is the rate constant of pseudo-first order adsorption. By integrating the equation with the suitable boundary condition (i.e. q ₀ = 0), the expression becomes:

(6) $q_t=q_e\left(1-e^{-k_{1}t}\right)$

The differential form of the pseudo-second order kinetics rate equation is expressed as (Ho and McKay Reference Ho and McKay1998):

(7) $\frac{d{q}_t}{\mathrm{dt}}=k_2{\left(q_e-q_t\right)}^2$

where k₂ (g mg^–1 min^–1) is the rate constant of pseudo-second order adsorption. The integrated form is:

(8) $q_t=\frac{k_2{q}_e^{2}t}{1+k_2{q}_{e}t}$

The nonlinear plots for the pseudo-first order and pseudo-second order kinetics models for the adsorption of Ni²⁺ by NS and IS at 25°C (Fig. 9) were processed using nonlinear optimization techniques to yield the parameters k₁, k₂, and q _e (Table 4). The intraparticle diffusion model is described by the following equation (Weber and Morris Reference Weber and Morris1963):

(9) $q_t=k_p{t}^{1/2}+C$

where k_p (mg g^–1 min^–1/2) is the intraparticle diffusion rate constant and C is the experiment constant. By plotting q _t vs t ^1/2 (Fig. 10), the rate constant is obtained from the slope and C from the intercept. The plot of q _t vs t ^1/2 should be linear if intraparticle diffusion is involved in the adsorption process, and becomes the rate-controlling step if this line passes through the origin. When the plot does not pass through the origin, this is an indication of some degree of boundary layer control and shows that intraparticle diffusion is not the only process affecting the rate.

Fig. 9.

Pseudo-first order and pseudo-second order kinetics plots for the adsorption of Ni ²⁺ ions by NS and IS at 25°C

Table 4.

Kinetics parameters for the adsorption of Ni²⁺ ions by NS and IS at three temperatures

Fig. 10.

Intraparticle diffusion plots for the adsorption of Ni ²⁺ ions by NS and IS at three temperatures

The determination coefficients (R²) for the pseudo-second order kinetics model are larger than those for pseudo-first order and intraparticle diffusion models, indicating that the pseudo-second order model is more suitable for describing the adsorption behavior of Ni²⁺ onto the NS and IS (Table 4). Besides, the q _e values calculated by the pseudo-second order model were closer to the experimental q _exp than pseudo-first order, suggesting that the curve modeled by the pseudo-second order equation is more consistent with the experimental data. The increase in rate constants (k₂) with increasing temperature indicated the endothermic nature of adsorption.

Adsorption Isotherms

Adsorption isotherms are used to study the equilibrium distribution of metal ions between solid adsorbent and liquid phase. The two best known isotherm models are the Langmuir and the Freundlich. The non-linear form of the Langmuir equation, which is valid for monolayer adsorption onto a homogeneous surface with a finite number of identical sites, is (Langmuir Reference Langmuir1918):

(10) $q_e=\frac{q_m{K}_L{C}_e}{1+K_L{C}_e}$

where C _e (mg L^–1) is the equilibrium metal ion concentration, q _e (mg g^–1) is the amount of metal ion adsorbed per unit weight of adsorbent at equilibrium, K_L (L mg^–1) is the Langmuir constant related to the enthalpy of adsorption, and q _m (mg g^–1) is the maximum adsorption capacity.

The Freundlich adsorption isotherm has been interpreted as adsorption to heterogeneous surfaces sites. The non-linear Freundlich equation is (Freundlich Reference Freundlich1926):

(11) $q_e=K_F{C}_e^{\frac{1}{n}}$

where K_F (mg^1–1/n L^1/n g^–1) is roughly an indicator of the adsorption capacity and n of the adsorption intensity. Values of n > 1 indicate favorable adsorption conditions. The Freundlich isotherm (Fig. 11, Table 5) was best fitted for both adsorbents with larger determination coefficients (R² ≥ 0.974 for NS and R² ≥ 0.965 for IS) and lower chi-square values (χ² ≤ 0.601 for NS and χ² ≤ 0.117 for IS). The R² values calculated for the Langmuir isotherm model (Table 5) were in the range of 0.774–0.859 for NS and 0.747–0.806 for IS, indicating that the data fit the Freundlich adsorption equilibrium model better than the Langmuir. The results indicated further that the Ni²⁺ adsorption occurs on a heterogeneous surface by multilayer coverage. The calculated values of the Freundlich adsorption isotherm constant n were >1, which also led to the conclusion that the adsorption processes were favorable.

Fig. 11.

Langmuir and Freundlich isotherm plots for the adsorption of Ni²⁺ ions by NS and IS at three temperatures

Table 5.

Langmuir and Freundlich constants for the adsorption of Ni²⁺ ions by NS and IS at three temperatures

The Ni²⁺ adsorption capacities of the two sepiolite samples (Table 6) revealed that differences are due to the properties of each adsorbent, such as structure, functional groups, and surface area. The experimental data for the present study are comparable to other reported values (Yavuz et al. Reference Yavuz, Altunkaynak and Güzel2003; Alemayehu and Lennartz Reference Alemayehu and Lennartz2010; Sheikhhosseini et al. Reference Sheikhhosseini, Shirvani, Shariatmadari, Zvomuya and Najafic2014). Although both of the adsorbents studied have large adsorption capacities, the NS sample was greater because of its greater BET surface area, porosity, and sepiolite content.

Table 6.

Comparison of the adsorption abilities of various adsorbents for Ni

Thermodynamic Parameters

The determination of thermodynamic parameters is of great importance in evaluating the spontaneity and the heat change of the adsorption processes. Changes in Gibbs free energy (ΔG°), enthalpy (ΔH°), and entropy (ΔS°) were determined to estimate the effect of temperature on Ni²⁺ adsorption onto NS and IS. The relationship between the adsorption equilibrium constant and temperature is given by the van’t Hoff equation:

(12) $ln{K}_d=\frac{-\Delta G°}{RT}=\frac{∆S°}{R}-\frac{∆H°}{RT}$

and, if total activity coefficients for the solute and solvent cancel or equal unity,

(13) $K_d=\frac{q_e}{C_e}$

where K_d (L g^–1) is the thermodynamic equilibrium constant, q _e (mg g^–1) is the amount of Ni²⁺ adsorbed at equilibrium, and C _e (mg L^–1) is the equilibrium concentration of Ni²⁺ in solution. R and T are the universal gas constant (8.314 J mol^–1 K^–1) and the absolute solution temperature (K), respectively. The values of ΔS° and ΔH° were calculated from the intercept and the slope of the linear plot of lnK_d vs 1/T (Fig. 12), respectively. From the values of ΔH° and ΔS°, ΔG° can be calculated using the relation below:

(14) $∆G°=\Delta H°-T\Delta S°$

Fig. 12.

Plots of ln K_d vs 1/T for estimation of thermodynamic state functions

The negative values of ΔG° (between –5.70 and –11.92 kJ mol^–1 for NS; –5.24 and –11.93 kJ mol^–1 for IS) at all the temperatures indicated that Ni²⁺ adsorption was spontaneous and thermodynamically feasible (Table 7). The greater negative values for ΔG° with increasing temperature indicated that the extent of the adsorption reaction increased with higher temperatures. Values for ΔG° for physical adsorption are usually between 0 and –20 kJ mol^–1, whereas for chemical adsorption they are often in the range of –80 to –400 kJ mol^–1 (Özcan et al. Reference Özcan, Ömeroğlu, Erdoğan and Özcan2007), indicating that physical adsorption was the probable mechanism for Ni²⁺ removal by NS and IS . The positive ΔH° values (86.77 kJ mol^–1 for NS) and (94.51 kJ mol^–1 for IS) showed that the adsorption of Ni²⁺ onto these minerals was endothermic, so an increase in entropy had to be the driving force in order to obtain the spontaneous condition ΔG° < 0. The entropy changes were 334.41 J mol^–1 K^–1 for IS and 309.81 J mol^–1 K^–1 for NS, which values exceeded those for ΔH° and thus satisfied the spontaneous condition. The positive values for ΔS° indicated a decrease in the order of the system, probably because Ni²⁺ ions were less hydrated on the clay surfaces than in the aqueous solution (Sheikhhosseini et al. Reference Sheikhhosseini, Shirvani, Shariatmadari, Zvomuya and Najafic2014).

Table 7.

Thermodynamic state functions for the adsorption of Ni²⁺ ions by NS and IS

Reusability Studies

Regeneration and reuse of adsorbent is an important matter in adsorption studies as it increases the economic value of the adsorption process. Estimating the regeneration ability of an adsorbent after it has been used for adsorption is, therefore, necessary. For this purpose, a 0.1 M HCl solution was used to elute Ni²⁺ adsorbed on the sepiolite samples. The dissolution rate of sepiolite has been reported to increase with increasing acid concentration (Özdemir and Kıpçak Reference Özdemir and Kιpçak2004). The dissolution rate of magnesite containing dolomite has also been reported to increase significantly above 0.1 M hydrochloric acid concentration (Özdemir et al. Reference Özdemir, Çakιr and Kιpçak2009). A more concentrated acid solution was not used, therefore, as a regenerant in the present study. The adsorption capacities of the two adsorbents tended to decrease with increasing number of cycles (Fig. 13a). After the third cycle, however, the NS and IS samples still had relatively large adsorption capacities of 8.63 mg g^–1 and 8.43 mg g^–1, respectively. The acid solution may have counteracted some of the loss in adsorption capacity in subsequent cycles by increasing the surface area, porosity, and active centers of the NS and IS, as noted by Lazarevic et al. (Reference Lazarevic, Jankovic-Castvan, Jovanovic, Milonjic, Janackovic and Petrovic2007). These results suggested that the samples exhibited reusability and could be a potential recyclable adsorbent for the removal of Ni²⁺ ions from aqueous solution.

Fig. 13.

a Reusability of NS and IS for Ni²⁺ adsorption, b extent of dissolution of Mg and Ca during regeneration

To test the stability of the adsorbents further, the Mg and Ca concentrations in the solutions after each regeneration cycle were measured, and the extent of dissolution of these elements with each cycle was calculated (Fig. 13b). The extent of dissolution of Ca (~55–100% for NS and ~33–73% for IS) was greater than of Mg (~13–24% for NS and ~18–55% for IS), showing that the dolomite is readily soluble. The amount of Mg dissolved from NS was less from cycle to cycle (flatter slope) than for IS, indicating that NS was more stable in the acidic regeneration medium.

Cost Estimation

Successful industrial implementation of an adsorptive removal technique for a contaminant depends heavily on the cost of the adsorbent as well as its physicochemical properties. The availability of adsorbent, processing requirements, treatment conditions, and reusability are the main parameters affecting the adsorbent cost. The estimated total costs together with the break-up costs to prepare 1 kg of adsorbent are summarized in Table 8. In addition, the comparisons of the costs of adsorbents used in this study with others reported previously are given in Table 9. The removal costs per kg of adsorbate were calculated using the estimated adsorbent costs and the removal capacities of adsorbents. The costs calculated for NS and IS were comparable with the other reported adsorbents (Baseri and Tizro Reference Baseri and Tizro2017; Ong et al. Reference Ong, Pingul-Ong, Kan and de Luna2018). The present study has, therefore, confirmed that NS and IS, as cost-effective and eco-friendly adsorbents, could be used for the treatment of wastewater containing Ni²⁺.

Table 8.

Cost estimation for the adsorbents used in this study

Table 9.

Comparison of estimated cost of adsorbents reported for Ni removal