The Role of Strontium in CeNiO3 Nano-Crystalline Perovskites for Greenhouse Gas Mitigation to Produce Syngas

The transition metal-based catalysts for the elimination of greenhouse gases via methane reforming using carbon dioxide are directly or indirectly associated with their distinguishing characteristics such as well-dispersed metal nanoparticles, a higher number of reducible species, suitable metal–support interaction, and high specific surface area. This work presents the insight into catalytic performance as well as catalyst stability of CexSr1−xNiO3 (x = 0.6–1) nanocrystalline perovskites for the production of hydrogen via methane reforming using carbon dioxide. Strontium incorporation enhances specific surface area, the number of reducible species, and nickel dispersion. The catalytic performance results show that CeNiO3 demonstrated higher initial CH4 (54.3%) and CO2 (64.8%) conversions, which dropped down to 13.1 and 19.2% (CH4 conversions) and 26.3 and 32.5% (CO2 conversions) for Ce0.8Sr0.2NiO3 and Ce0.6Sr0.4NiO3, respectively. This drop in catalytic conversions post strontium addition is concomitant with strontium carbonate covering nickel active sites. Moreover, from the durability results, it is obvious that CeNiO3 exhibited deactivation, whereas no deactivation was observed for Ce0.8Sr0.2NiO3 and Ce0.6Sr0.4NiO3. Carbon deposition during the reaction is mainly responsible for catalyst deactivation, and this is further established by characterizing spent catalysts.


Introduction
Among the various well-established CO 2 conversion processes, such as electrochemical catalysis, photocatalysis, and thermal catalysis, methane reforming using carbon dioxide, commonly known as dry reforming of methane (DRM), has recently attracted scientists primarily because DRM converts major greenhouse gases, i.e., carbon dioxide and methane, to synthesize hydrogen and carbon monoxide, also called synthesis gas, which is further utilized to produce liquid hydrocarbons [1][2][3][4][5][6][7][8]. Hence, the DRM process not only plays a role in greenhouse gas mitigation and thus serves as a cause of climate change, but also generates synthesis gas, a mixture of equimolar hydrogen and carbon monoxide suitable for the production of hydrocarbon via the well-known Fischer-Tropsch synthesis process [9][10][11][12][13]. It is well established that the proper choice and suitable design of a catalyst plays significant role in catalytic activity and stability during DRM [14][15][16]. Both noble metal-based and transition metal-based catalysts have been reported for DRM, but noble metal-based catalysts are expensive and less abundant despite their excellent catalytic activities [8]. Therefore, transition metal-based catalysts serve as an efficient alternative for DRM. Among transition metal-based catalysts, nickel (Ni)-and cobalt (Co)-based catalysts This research article demonstrates the impact of strontium incorporation into ceriumand nickel-based nanocrystalline perovskites (CeNiO 3 ) in dry and/or CO 2 reforming of methane. The catalytic activity performances are specifically elucidated in relation to their characterizations before and after reaction. Overall, the study is focused on exploring the insights of cerium replacement with strontium and the influence of this replacement on catalytic conversions and durability under reforming conditions.

Thermal Decomposition of Precursors
Thermal decomposition curves, including thermogravimetric (TG) and their differentials (DTG) of the precursors as a measure of their calcination temperatures, are shown in Figure 1. It can be seen from Figure 1 that each precursor, a gel-like mixture of metal nitrates and glycine, decomposed differently and both CeNiO 3 and Ce 0.8 Sr 0.2 NiO 3 demonstrated twostep decomposition, whereas three-step decomposition was observed for Ce 0.6 Sr 0.4 NiO 3 . Overall, the decomposition temperatures of CeNiO 3 were relatively higher than strontiumincorporated Ce 0.8 Sr 0.2 NiO 3 and Ce 0.6 Sr 0.4 NiO 3 . The onset temperature for initial weight loss (first-step decomposition) of~8%, in the case of CeNiO 3 , was found to be~75 • C; weight loss then reached its maximum at~150 • C, and finally finished at~300 • C. This first-step decomposition was assigned to the removal of the adsorbed water and/or release of adsorbed gases. The second-step decomposition exhibited a weight loss of~21% observed in the temperature range of 300-550 • C (with peak maximum at 420 • C), which could be ascribed to the decomposition and/or combustion of organic matter. Despite showing an almost similar decomposition trend, the DTG peak temperatures for first-and second-step decomposition for Ce 0.8 Sr 0.2 NiO 3 dropped slightly down to 145 and 410 • C, respectively. In contrast, Ce 0.6 Sr 0.4 NiO 3 demonstrated three-step decomposition, and the onset temperature for initial weight loss was observed to be 130 • C, which was attributed to the release of physically adsorbed water and/or gases. Second-and third-step decompositions, occurring at 450 and 870 • C, elucidated the combustion of organic matter present in the precursor.
2.1.2. X-ray Diffraction (XRD) Figure 2 presents the XRD patterns of the as-prepared nanocrystalline perovskites with and without the incorporation. MDI Jade ® software was used to analyze XRD data. The data analysis shows that a significant number of peaks corresponding to CeNiO 3 were recorded [42][43][44][45], whereas diffraction peaks detected at 2θ values of 37.3 • , 43.3 • , and 62.9 • were related to cubic NiO. Moreover, remaining peaks were assigned to oxides and carbonates of strontium, as labeled in Figure 2 [46].  Figure 3 shows the N 2 adsorption-desorption isotherms and pore-size distributions of air-calcined precursors (700 • C, 5 h), and their BET surface areas and pore parameters are summarized in Table 1. Figure 3 shows that all of the samples displayed a type II isotherm with a H3 hysteresis loop in the relative pressure (P/P 0 ) range of 0.8-1.0, indicating that these samples possessed macro-pores. The specific surface areas observed (17.3-25.6 m 2 /g) are in accordance with the literature, except that these values were slightly higher than the reported specific surface area, i.e., below 10 m 2 /g for similar types of materials [47]. The surface area of Ce 0.8 Sr 0.2 NiO 3 catalyst was higher (25.6 m 2 /g) than that of the other fabricated catalysts. However, no clear trend as a function of Sr substitution extent was observed. Although Sr doping did not much affect the surface area, it greatly influenced the pore size and pore volume; the highest values were found for x = 0.2 and the lowest for x = 0.0. The increase in pore volume post Sr addition indicates that Sr could play a role in influencing the catalytic activity, which is discussed in Sections 2.2 and 3. Furthermore, the elemental analysis of as-synthesized catalysts revealed that CeNiO 3 catalyst exhibited an Ni/Ce ratio of 1, and hence, both Ni and Ce had similar compositions as measured from ICP-OES (Table 1). The chemical compositions of Sr-incorporated catalysts show that Ce was replaced with Sr.

Morphological Study (TEM) of Fresh and Reduced Perovskites
Transmission electron microscopy (TEM) was utilized to analyze the morphology of the fresh, reduced, and used nanocrystalline perovskite catalysts, and microscopic images of all the catalysts before and after reaction are shown in Figure 4. ImageJ ® software was used for image processing and data analysis. The particles were observed to be spherical in shape, and the average particle sizes were between 5-34, 12-27, and 14-25 nm for CeNiO 3 , Ce 0.8 Sr 0.2 NiO 3 , and Ce 0.6 Sr 0.4 NiO 3 fresh catalysts, respectively. It is interesting to note that insignificant sintering was observed for reduced catalysts, and particle sizes were 8-45, 15-42, and 18-40 nm for CeNiO 3 -, Ce 0.8 Sr 0.2 NiO 3 -, and Ce 0.6 Sr 0.4 NiO 3 -reduced catalysts, respectively.

Temperature-Programmed Reduction (TPR)
TPR is mainly utilized to examine the reducibility, the metal-support interaction, and to find the activation and/or reduction temperature that results in metallic particles required for the catalytic reforming reaction. Figure 5 presents the reduction profiles, indicating the variations in metal-support interaction and/or the reducibility of CeNiO 3 post Sr addition. The reduction profiles can be divided into two regions (region I < 525 and region II > 525 • C). The small reduction peak in region I below 220 • C in each catalyst is related to the reduction of weakly interacting nickel oxide species, whereas the reduction peaks appearing between 220 and 525 • C correspond to two-step reduction of Ni 3+ to Ni 2+ and Ni 2+ to Ni 0 [44,48]. The reduction profiles in region II are ascribed to either the reduction of ceria and/or the reduction of perovskite to metallic nickel at higher temperature [49]. CeNiO 3 -and Sr-incorporated catalysts reduce according to the reactions below: There were no significant change in the reduction peak temperatures (~290 • C) of CeNiO 3 or Ce 0.8 Sr 0.2 NiO 3 ; however, the peak intensity of Ce 0.8 Sr 0.2 NiO 3 reduced to one third of CeNiO 3 , indicating the suppression of a number of reducible species post Sr addition. This trend completely changed when Sr was further added (Ce 0.6 Sr 0.4 NiO 3 ), and more species reducible at higher temperatures were observed. It is reported that the addition of Sr to a supported Ni catalyst enhanced metal-support interaction and new peaks were found at higher temperature, which is in agreement with the TPR results of Ce 0.6 Sr 0.4 NiO 3 but is contradictory to the Ce 0.8 Sr 0.2 NiO 3 reduction profile, where a small shoulder was observed in region II. The enhanced reducibility and/or easier reduction of Ce 0.8 Sr 0.2 NiO 3 can be attributed to a possible lowering of the valence state of Ni cations incorporated into the oxide. The role of these findings in influencing the catalytic activity is discussed in Section 2.2.

Catalytic Performances
As-synthesized nanocrystalline Ce x Sr 1−x NiO 3 (x = 0.6-1) perovskites were studied for their performance in dry methane-reforming reaction at 700 • C. Prior to the dry-reforming reaction, all the catalysts were subjected to reduction/activation using hydrogen as a reducing gas to generate the required metallic nickel crystallites as active sites. Figure 6a,b shows methane (CH 4 ) and carbon dioxide (CO 2 ) conversions versus time-on-stream. It can be seen from Figure 5a that CeNiO 3 demonstrated a higher CH 4 conversion than Sr-incorporated catalysts. CeNiO 3 exhibited an initial CH 4 conversion of 54.3% and deactivated down to reach 50.1% after 7 h time-on-stream, leading to a deactivation factor of 7.7% ( Table 1). The deactivation factor based on first-order kinetics also showed the same deactivation trends, as shown in Table 1 [50,51]. The impact of incorporating Sr into CeNiO 3 over initial CH 4 conversion was obvious, and decreased from 54.3% (CeNiO 3 ) to 13.1% (Ce 0.8 Sr 0.2 NiO 3 ) and 19.4% (Ce 0.6 Sr 0.4 NiO 3 ) when x changed from 1 to 0.6. The loss in catalytic activity, in the case of Sr-incorporated catalysts, can be attributed to either nickel species agglomeration facilitated by Sr addition after the reduction or the covering of nickel active sites with Sr. Based on the TEM images of reduced catalysts, it is obvious that no significant sintering was observed after reduction; hence, the main reason behind the lower activity of Sr-incorporated catalysts might be nickel active sites covered with Sr. Interestingly, no deactivation was observed for strontiumincorporated perovskites (Ce 0.8 Sr 0.2 NiO 3 and Ce 0.6 Sr 0.4 NiO 3 ) and hence, deactivation factors were negative in these catalysts (Table 1). Moreover, conversions increased for the initial 90 min before becoming constant for strontium-incorporated perovskites, which is associated with the reduction of nickel species remaining oxidized even after activation under hydrogen atmosphere prior to reaction. The catalyst's deactivation and associated factors behind deactivation are discussed in Section 3. Like Figure 6a,b shows a similar trend for CO 2 conversions as a function of time. CO 2 conversions of 64.8, 26.3, and 32.5% were exhibited by CeNiO 3 , Ce 0.8 Sr 0.2 NiO 3 , and Ce 0.6 Sr 0.4 NiO 3 , respectively, which eventually reached final CO 2 conversions of 58, 36, and 33.6%, respectively. It is noteworthy from Figure 6 that CO 2 conversions were higher than CH 4 conversions. This finding leads to the fact that some side reactions were simultaneously taking place, such as the reverse water-gas-shift reaction (CO 2 + H 2 → CO + H 2 O) producing H 2 /CO molar ratios lower than unity, i.e., H 2 /CO = 1.0, since hydrogen was consuming CO 2 (Figure 6c), as well as the Boudouard reaction and CO disproportionation reaction (2CO → CO 2 + C). A dedicated section discusses the catalytic performance results in relation to their characterizations in Section 3.

Characterization of Spent Perovskites
The post dry reforming perovskites were further analyzed using different characterizations to explain the catalytic activity and/or stability results. Among the tested catalysts, only CeNiO 3 deactivated over time, whereas Sr-incorporated catalysts showed increasing CO 2 and CH 4 conversions. Moreover, CO 2 conversions higher than CH 4 conversions ( Figure 6) paved the way for side reactions, including reverse CO disproportionation and reverse water-gas-shift reaction. These post dry-reforming catalysts were characterized by temperature-programmed oxidation (TPO) and transition electron microscope (TEM) to explore the modifications experienced by perovskites during the dry-reforming reaction.

Temperature-Programmed Oxidation (TPO)
The possibility of carbon formation over the catalyst's surface post dry-reforming reaction was demonstrated by TPO analysis, as shown in Figure 7. It is obvious that one broad peak was displayed in the temperature range of 110 to 500 • C for each catalyst. The TPO peak maxima were 285, 300, and 335 • C for Ce 0.6 Sr 0.4 NiO 3 , Ce 0.8 Sr 0.2 NiO 3 , and CeNiO 3 , respectively. These peak maxima suggest the formation of less-reactive surface carbides and/or polymeric carbon species during dry methane-reforming reaction, as reported earlier in the literature [52,53]. The hydrogenation degree of surface carbon species is related to TPO peak temperature, and these surface carbon species transform into graphitic carbon as TPO peak temperature moves towards higher temperatures. Furthermore, the peak temperature implies that the interaction between polymeric carbon species and catalyst surface varies and becomes weaker after Sr incorporation, as exhibited by the decrease in TPO peak maxima from 335 to 285 • C for CeNiO 3 and Ce 0.6 Sr 0.4 NiO 3 . It is noteworthy that the carbon deposition over perovskite samples in this work was significantly lower than scandium-and magnesium-modified Ni-and Co-based bimetallic catalysts supported over an expensive SBA-15 support [3] and strontium-promoted Ni and Co-Al 2 O 3 catalysts [4]. It can be concluded that cerium oxide and strontium incorporation influence the formation of carbon, carbon suppression, and carbon interaction with the catalyst surface.

Transition Electron Microscopy (TEM) and Elemental Analysis
In order to gain insight into the morphological changes and/or formation of deactivating coke over the surface of spent catalysts, TEM microscopic images were recorded post dry-reforming reaction. From the TEM images of spent catalysts in Figure 4g-i, particle sizes were found to be 10-70, 18-50, and 20-67 nm for CeNiO 3 , Ce 0.8 Sr 0.2 NiO 3 , and Ce 0.6 Sr 0.4 NiO 3 , respectively. The deposition of carbon over the catalysts' surface and obvious catalyst particle agglomeration were also evident, which suggests the contribution of sintering towards the deactivation of CeNiO 3 . No deactivation, in the case of Sr-incorporated perovskites, was observed even after carbon deposition and particle agglomeration. These findings are further elaborated below in Section 3. Moreover, the elemental analysis of spent catalysts demonstrated that no variations in the chemical compositions of the catalyst were observed during the reaction.

Discussion
Prior to the dry methane-reforming reaction study, as-prepared nanocrystalline perovskites were characterized to envisage their activity performance during reforming reaction. Thermogravimetric analysis results, i.e., TG-DTG analysis data, illustrate the conversion of precursors into perovskites post calcination treatment at temperatures demonstrated by DTG (Figure 1 and Table S1). XRD diffraction profiles of as-synthesized catalysts (Figure 2) revealed the presence of nickel oxide, perovskite structure, and cerium dioxide along with carbonates and oxides of strontium. The formation of macroporous higher-specific-surface-area perovskite, e.g., 25.6 m 2 /g for Ce 0.8 Sr 0.2 NiO 3 , was obtained from nitrogen adsorption-desorption isotherms ( Figure 3 and Table 1). TEM demonstrated (Figure 4) spherical-shaped particles with various sizes with and without strontium incorporation. The reduction profiles using TPR ( Figure 5) exhibited easier reduction of oxides in CeNiO 3 and Ce 0.8 Sr 0.2 NiO 3 , whereas stronger metal-support interaction and difficult-to-reduce oxides were formed in Ce 0.6 Sr 0.4 NiO 3 . Pre-reforming reaction characterization results indicate a higher number of reducible species, larger specific surface area, and a wide range of spherically shaped nanoparticles post strontium incorporation. Hence, it was expected that Sr-incorporated perovskite, such as Ce 0.8 Sr 0.2 NiO 3 , would potentially outperform the rest of the catalysts, but Figure 6 shows lower activity of this catalyst. The mechanism associated with dry methane reforming requires reactant adsorption over the active sites of the catalyst as an initial step. The reactants then dissociate and finally react with each other to form products that eventually leave the catalyst surface following desorption [4]. Nickel, in its metallic form, serves as the active site for the adsorption of CH 4 [3]. Catalytic activity results reveal the loss in activity in terms of both CH 4 and CO 2 conversions post Sr incorporation into CeNiO 3 , which could be ascribed to the loss of active sites due to metal particle agglomeration, the presence of unreduced nickel oxides post activation, and/or active site coverage with carbonates or oxides of strontium [4,7]. TEM data show the extent of metal agglomeration or sintering prior to, during, and post reforming reaction, and it is evident that the degree of sintering remained the same and can be ruled out as a deactivation factor contributing to the lower activity of Sr-incorporated catalysts. Furthermore, the presence of strontium oxide and strontium carbonates, as evidenced by XRD, substantiate the hypothesis that coverage of nickel active sites by strontium species causes loss of catalytic activity in Sr-incorporated catalysts.
The activity results versus time-on-stream as a function of catalyst stability are shown in Figure 6. Despite higher activity, CeNiO 3 perovskite deactivated over time, which is attributed to carbon formation as well as active metal sintering. These observations are substantiated by TEM and TPO characterization results of used catalysts. It is interesting to note that strontium-incorporated perovskites did not show any deactivation despite carbon deposition and sintering. The degree of agglomeration or sintering remained the same for all perovskites during the dry methane-reforming reaction. This suggests that methane decomposition [3], a prevalent DRM side reaction at higher reaction temperature, is the main source of carbon deposition causing catalyst deactivation, in accordance with TPO peak maxima-i.e., a higher temperature (335 • C) is required to gasify carbon formed over the surface of CeNiO 3 than that of strontium-incorporated perovskites. Moreover, CO 2 conversions in strontium-incorporated perovskites increased over time, which was not the case with CeNiO 3 . These findings infer that carbon gasification is promoted in an oxidative environment in strontium-incorporated perovskites, leading to no deactivation in these catalysts. The reaction mechanism and associated impact of Sr incorporation is further shown in Figure 8. The investigation of reduced La 2-x Sr x NiO 4 perovskite oxides by Rynkowski et al. [7] inferred that Sr incorporation in smaller amounts exhibited lessactive but stable catalytic performance in comparison with strontium-free catalysts. The study of the role of LaNiO 3 perovskites after partially substituting Ni and La for dry methane-reforming reaction revealed that La replacement with Sr leads to a loss of catalytic activity [54]. Furthermore, the comparison of findings in this work with already published literature ( Table 2) revealed that the current conversions outperformed similar perovskites such as CeNiO 3 [55] or similar combinations with varying A and/or B substitutions in ABO 3 [56][57][58][59]. Since the main focus of this work was to demonstrate the deactivation factors as a function of catalytic stability of perovskites, it is obvious that the perovskites in this work showed lower deactivation factors than [55,59] despite using higher space velocity.

Materials and Methods
Nanocrystalline perovskites, i.e., Ce x Sr 1−x NiO 3 (x = 0.6-1), were prepared via the self-combustion method, and glycine and metallic nitrates were used as precursors. Initially, in 100 mL of deionized water, appropriate amount corresponding to x of hydrated cerium nitrate (Ce(NO 3 ) 3 ·nH 2 O, purchased from Sigma-Aldrich, St. Louis, MO, USA, with a purity of 99.9%), 1 mmole of nickel nitrate hexahydrate (Ni(NO 3 ) 2 ·6H 2 O purchased from Sigma-Aldrich with a purity of 99.9%), and appropriate amount corresponding to 1 − x of Sr(NO 3 ) 2 were dissolved. Then, glycine (purity of 99.5%) was added to metal nitrate solution as an ignition promoter by keeping the glyceine-to-metal-ions ratio close to unity. The mixtures were systematically stirred to obtain a homogenous gel-like solution by water elimination at 60-70 • C. Since the onset temperature for ignition reaction is~250 • C, the gel was subjected to this temperature to produce powdered precursors that were eventually calcined under oxidative atmosphere at 700 • C for 6 h, leading to the formation of the perovskite structure. The nomenclature Ce x Sr 1−x NiO 3 , where x varies between 0.6 and 1, was used in all cases just as standardization, as it is usual in the literature.
The thermogravimetric analysis (TGA), including differential curves (DTG) of the perovskite precursors, was recorded using a TGA/SDTA851e thermal analyzer (purchased from Mettler-Toledo, Switzerland). The samples were subjected to heating from room temperature to 1000 • C using a heating rate of 20 • C/min under inert atmosphere (by flowing nitrogen at 100 mL/min). The following characterizations were employed over calcined catalysts. X-ray diffraction profiles were recorded using a scan rate of 0.2 • /min between 10 and 80 • on an XRD-6000 diffractometer (purchased from Shimadzu, Columbia, MD, USA) equipped with monochromatic radiation of CuK (λ = 1.5406 Å). Braunner, Emmet, and Teller (BET) specific surface areas of the samples were measured on a NOVA2000 BET system (purchased from Quantachrome, Boynton Beach, FL, USA). Temperature-programmed oxidation (TPO) and reduction (TPR) profiles were conducted on an Autochem 2920 apparatus (purchased from Micromeritics, Norcross, GA, USA). A total of 30 mg of each sample was placed in a U-shape quartz tube. The sample was first pretreated under synthetic air flowing at 50 mL/min at 300 • C for 1 h followed by cooling it down to room temperature. In order to record TPR patterns, samples were subjected to reducing atmosphere by flowing 10% H 2 /Ar at 25 mL/min while the sample temperature was raised from room temperature to 900 • C at 10 • C/min. The TPO samples were pretreated in a way similar to TPR. TPO profiles were recorded for the spent catalysts post dry-reforming stability tests to identify carbon formed over the catalyst surface. The samples were subjected to oxidative environment by flowing 10% O 2 /He at 25 mL/min and raising the sample temperature from room temperature to 800 • C at 10 • C/min. The morphology of fresh and used perovskite catalysts was analyzed by transmission electron microscopy (TEM) using a JEM-210 microscope (purchased from JEOL, Tokyo, Japan) equipped with an accelerating voltage of 80 kV. The chemical compositions in the as-synthesized catalysts were measured by using inductively coupled plasma optical emission spectroscopy (ICP-OES ELAN 6100 purchased from Perkin Elmer, Waltham, MA, USA).
The dry methane-reforming reaction was conducted in a tubular fixed-bed reactor (i.d. 1 cm, catalytic bed length 3 mm) at 700 • C and 1 atm pressure. The feed gas, comprising methane and carbon dioxide (1:1) balanced with nitrogen, was flown at 70 mL/min with a space velocity of 84,000 mL g cat.
−1 h −1 . The catalysts were subjected to activation/reduction, prior to reaction, by flowing 10% H 2 in nitrogen mixture (40 mL/min) at 700 • C for 2 h. After activation, the hydrogen mixture was replaced with helium to remove any leftover hydrogen and subsequently the reaction was carried out at 700 • C for over 7 h time-on-stream. The analysis of the reforming products and unconverted reactants was carried out using on-line gas chromatograph GC 3800 (purchased from VARIAN, Palo Alto, CA, USA) equipped with two columns (packed with Porapak N and 13X molecular sieves) and two thermal conductivity detectors. The results were reproducible with an error of ±5%. The conversions and molar ratios were calculated using following equations [60,61]: nH 2 nCO = F H2,out F CO,out (5)

Conclusions
This study demonstrated the catalytic performance results of strontium-incorporated Ce x Sr 1−x NiO 3 (x = 0.6-1) nanocrystalline perovskites for dry methane reforming. The extent of finely dispersed nanocrystalline particles over the surface of the catalysts, their reducibility, and their textural properties, including specific surface area, were determined by characterizing the catalysts prior to the reforming reaction. It was revealed that these factors significantly influenced the catalytic activity as well as durability. Strontium-free CeNiO 3 perovskite demonstrated higher activity in terms of CH 4 and CO 2 conversions but showed deactivation over time-on-stream. Despite relatively lower conversions, strontium incorporated perovskites (Ce 0.8 Sr 0.2 NiO 3 and Ce 0.6 Sr 0.4 NiO 3 ) remained stable over the 7 h time-on-stream. The lower activity in strontium-incorporated perovskites was attributed to the coverage of active (nickel) sites with carbonates of strontium, which is also reported in the literature. The post-reforming characterizations of perovskites helped to investigate the deactivation cause. Despite finding active metal agglomeration or sintering over all catalysts post-reforming, the insignificant sintering was ruled out as major cause of deactivation substantiated with no activity loss for strontium-incorporated catalysts. This suggests that carbon formation during the reforming reaction was the main cause of deactivation. This was further confirmed by analyzing TEM and TPO results of spent perovskites. Stable and/or increasing CO 2 conversions higher than CH 4 conversions in strontium-incorporated perovskites facilitated carbon gasification, which prevented deactivation. These results presented the key role of the strontium incorporation in Ce x Sr 1−x NiO 3 (x = 0.6-1) perovskites to ensure stable catalytic performance for longer periods of time to avoid deactivation, a common challenge to cope with for nickel-based catalysts.