ISIJ International
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Fundamentals of High Temperature Processes
Evolution of Mercury from Iron Ores in Temperature-Programmed Heat Treatments
Javzandolgor BudYuuki MochizukiNaoto Tsubouchi
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Supplementary material

2022 Volume 62 Issue 1 Pages 20-28

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Abstract

The behavior of Hg released from iron ores during temperature-programmed heat treatments (TPHTs) in air has been mainly studied using an online monitoring method. The Hg release behavior in TPHT significantly depends on the type of ore being processed, which includes forms evolved as Hg0 and Hg2+, and forms that remain thermally stable up to 950°C. In addition, the TPHT experiments for model Hg compounds suggested the presence of several types of Hg forms (HgCl2, Hg2Cl2, HgS, HgO, HgSO4, and associated mineral-Hg) in the iron ores used. The amounts and proportions of suggested forms of Hg species substantially depend on the type and composition of the iron ore used. These observations may be important in designing an efficient method for the removal of Hg from iron ore and gaseous Hg.

1. Introduction

Mercury is one of the most hazardous elements, and it spreads into the environment from many sources. The total amount of mercury emitted in nature was 2500±500 t/year in 2018,1) and the mercury emitted in the environment does not disappear or fade away, instead, it changes its form, and exists in nature for decades. Mercury emissions are not only a local problem anymore; they spread across the world through the air, water, and even via the food chain, and adversely affect human health.2) Following the accelerated development of population and consumption, the manufacturing industry continues to grow annually; however, mercury emissions have become more dangerous in several sectors.3) Most of the Hg emissions originate from Asia; in particular, East and Southeast Asia produce 39% of the total global emissions, and industrial fields and fossil fuel usage are the primary sources of Hg emissions in this region. Ferrous and non-ferrous metal productions are primary anthropogenic sources worldwide.4) In the field of energy production, coal combustion has the highest percentage of mercury emission sources. Consequently, the control and reduction of emissions are one of the primary challenges facing the industry in this century. A number of scientists are working on the determination and measurement of mercury contents in coal and reported sufficient data to elucidate the emission process of Hg from coal combustion and pyrolysis.5,6,7,8,9,10,11) Unfortunately, the information and results available on the existence and evolution behavior of Hg from iron ore, which is a major raw material for the metallurgic industry and pig-iron and steel productions, are insufficient. However, the availability of data and information on the release forms and behavior of Hg will facilitate the improvement of the emission control and reduction technology. Recently, various Hg removal processes have been adopted, such as coal washing, air pollution control devices (APCDs), and wet flue gas desulfurization (FGD).12) However, improving the removal methods and elucidating the release behavior of Hg from iron ore, as well as mercury adsorption from steel production and iron ore applications, remains crucial. To define the existence of Hg species in iron ores and determine their release behavior from iron ore, this study was conducted to examine the interaction between Hg species and other substrates.

2. Experimental

2.1. Iron Ore Sample

One Australian limonite (AUL) and four types of hematite (INH, AUH, BRH, and ISH) mined from different countries (India, Australia, Brazil, and South Africa) were used in this study. These particle sizes were −250 μm. All samples were obtained from the Japan Iron and Steel Federation. Table 1 presents the compositions of all iron ores used. The total Fe and Hg contents of the samples ranged from 57–67 mass%-dry and 79 to 305 dry μg/g, respectively. The gangue components and combined-water (H2O) content s in the samples (all in mass%-dry) were as follows: Si, 0.55–2.3; Al, 0.5–1.2; Mn, 0.02–0.7; P, 0.04–0.08; Ti, 0.02–0.07; Ca, 0.01–0.16; Mg, 0.01–0.11; S, 0.01–0.02; and H2O, 0.37–9.16 mass%.

Table 1. Gangue components of iron ore samples used in this study.
SampleCountryCodeComposition, mass%-dryHg μg/g
Total-FeSiAlFe(II)MnPTiCaMgSH2O
LimoniteAustraliaAUL57.12.31.20.090.040.070.160.110.019.16101
HematiteIndiaINH61.82.01.11.00.700.060.050.010.030.014.182
HematiteAustraliaAUH62.81.60.960.150.130.080.040.020.030.024.4227
HematiteBraziliaBRH66.20.550.570.600.050.040.010.020.011.72305
HematiteSouth AfricaISH66.91.20.50.30.020.050.020.050.010.010.3779

2.2. Temperature-Programmed Heat Treatment (TPHT)

The TPHT experimental was carried out by flow-type quartz made fixed-bed reactors. The apparatus was shown in Fig. S1 in Supporting Information. First, 5.0-g iron ore sample was charged in a quartz cell and placed into the reactor, and then the reactor was heated up to 950°C by a 10°C/min rate in air flow. The temperature of the K-type thermocouple reactor was maintained. The details of this apparatus have been described in.12)

2.3. TPHT for Hg Pure Compounds and Mixtures of Hg Compounds and Fe2O3

The TPHT operations of several model Hg compounds were also conducted to investigate the nature of Hg release from iron ore. As experimental samples, we prepared physical mixtures of iron oxide (99.9%) with various commercially available Hg species (HgCl (99%), HgCl2 (99.5%), HgS (99%), HgO (98%), and HgSO4 (99%)) in proportions selected to ensure a mercury concentration of 100 mg/g for each mixture. Particle size of all reagents used were −250 μm. It should be noted that the mercury content should originally be 100 μg/g to match the mercury concentration in the ore; however, the amount was significantly small that it was difficult to measure it by weight during the preparation of Fe2O3/Hg compound mixtures. The general term “Hg compound/Fe2O3” is used to refer to these mixtures. Mixture samples were subjected to TPHT via the procedure described above for iron ore, and total Hg was solely analyzed. In this study, the reproducibility and analytical errors were within ±10% and ±5%, respectively, for measurements of gaseous Hg and Hg in the solid phase.

2.4. Hg Analysis

Hg was measured in the as-received iron ore and solid sample after the TPHT was conducted via mixed acid dissolution12) and reduction using cold vapor atomic absorption spectrometry (AAS) (Hiranuma Sangyo, HG-450). Gaseous total-Hg, which evolved in TPHT, was analyzed at 1-s intervals by non-dispersive double-beam direct UV AAS using a mercury analyzer (Nihon Instruments, EMP(WLE)-2/SGM-8) equipment and SnCl2 solution, while Hg0 was measured using a KCl solution instead of a SnCl2 solution. The apparatus was shown in Fig. S1 in Supporting Information. The amount of Hg2+ was calculated as the difference between the amount of total Hg released to the released amount of Hg0. The release amount of total Hg, Hg0, and Hg2+ was calculated based on the respective amounts of their content in iron ores. Hg in the ore represents the Hg concentration in the as-received iron ore.

3. Results and Discussion

3.1. Release Behavior of Total-Hg during TPHT of Iron Ore

Figure 1 illustrates the release behavior of total Hg from iron ore samples during TPHT up to 950°C in an air environment. Hg release started at approximately 100°C for all samples; however, release profiles were entirely different for each sample used. For BRH (Fig. 1(a)), the Hg release profile exhibited main and shoulder peaks at 600°C and 800°C, respectively. The Hg evolution was determined up to 950°C. Hg release from AUH (Fig. 1(b)) exhibited broad peaks at 150°C and 550°C, and a distinct major peak was observed at 750–800°C. Figure 1(c) illustrates the Hg release profile of the INH. Hg release was observed at 200°C, and broad main peaks were measured at approximately 600°C. In the case of ISH (Fig. 1(d)), three broad peaks were observed at approximately 200°C, 500°C, and 700°C, respectively. For AUL (Fig. 1(e)), Hg was released above 100°C, and the release profile exhibited shoulder and main peaks at approximately 300°C and 350°C, respectively. Almost no Hg release was observed above 500°C. From these results, it was determined that the total Hg release profile depends on the iron ore type. In other words, the evolution profiles indicate that Hg species in ores may exist in at least four forms (i.e., volatile forms below 400°C, at 400–600 or 700°C, at 600–950°C, and at thermally stable temperatures up to 950°C).

Fig. 1.

Release behavior of total Hg during TPHT. (a) BRH, (b) AUH, (c) INH, (d) ISH, and (e) AUL. (Online version in color.)

Figure 2 presents the mass balance of the TPHT examination. It was obtained by integrating the formation rate profiles for gaseous total Hg shown in Fig. 1. Gaseous-Hg and solid-Hg in residues ranged from 16% to 73% and 30% to 75%, respectively. The mass balances were within a logical range of 100±10%. The order of solid-Hg was INH ≒ BRH < AUH < ISH ≪ AUL. It is observed that Hg in AUL exists in a form that is difficult to release. In contrast, almost 60%–70% of total Hg was released from all ore samples with ease, except for AUL. This may indicate that Hg exists in ores and the release-form because gaseous-Hg are relatively different. In accordance with previous studies,5,6,7,8,9,10,11) most of the Hg content in coal evolves in the gaseous form at low temperatures during pyrolysis or combustion. In contrast, 30%–75% of the total Hg content of iron ore remain in the solid phase even after heating to 950°C. These results suggest that the Hg content assume significantly different forms in iron ore and coal, which indicates that several thermally stable forms of Hg exist.

Fig. 2.

Distribution of Hg contents for iron ore samples. (Online version in color.)

Figure 3 presents the results of the relationship between the Hg content in the ores presented in Table 1 and the amount of gaseous Hg in Fig. 2. Although there were a few variations for low Hg-content ores, there was a positive correlation between the Hg content in the ores and the amount of gaseous Hg.

Fig. 3.

Relationship between Hg content in as-received iron ore and released amount of total-Hg. (Online version in color.)

In other words, the ore with higher Hg content has more volatile Hg species, thus suggesting that the Hg content in the ore depends primarily on the thermally unstable mercury species. These results may also guide the development of methods to manage the Hg released during the thermal treatment of iron ore during the steelmaking process.

3.2. Evolution Behavior of Hg0 and Hg2+ during TPHT

The evolution profile of gaseous Hg0 during TPTH was investigated to elucidate the Hg forms in iron ore. The evolution profiles of Hg0 from the ore samples are presented in Fig. 4. For the BRH sample (Fig. 4(a)), the Hg0 evolution profile exhibited a large and high-intensity peak at 610°C. Figure 4(b) presents the Hg0 profiles of the AUH samples. Release started at 100°C, and provided three smaller peaks than BRH at 150°C, 600°C, and 750°C. Hg0 evolution from INH (Fig. 4(c)) was observed at 200°C, and the profile exhibited two small peaks at 550°C and 650°C , and the Hg0 release continued until 950°C. In the case of ISH (Fig. 4(d)), the Hg0 evolution profile exhibited two broad peaks at 200°C and 450°C, and a shoulder peak at 700°C. The evolution reached to 950°C. In the case of AUL (Fig. 4(e)), almost no Hg0 evolution was observed. From these results, the Hg0 evolution also depends on the iron ore type.

Fig. 4.

Release profiles of Hg0 during TPHT. (a) BRH, (b) AUH, (c) INH, (d) ISH, and (e) AUL. (Online version in color.)

Figure 5 summarizes the evolution profiles of the total Hg, Hg0, and Hg2+. Here, the Hg2+ profiles were determined by calculating the difference between the total Hg and Hg0 evolution profiles. For BRH (Fig. 5(a)), the shoulder peak that was released at 500–550°C in the total Hg profile disappeared in the Hg0 profile, and the intensity of the main peak at 600°C was similar to the total Hg peak. Nevertheless, the intensity of detachment that appeared at 600–950°C was decreased. Compared with the total Hg, the elimination amount of Hg0 decreased, which can be attributed to the increased Hg2+ elimination. In other words, in the high-temperature range, the total Hg content for the BRH release was in both Hg0 and Hg2+ forms. In Fig. 5(b), the release profile of total-Hg from AUH matched with Hg0 at 100–250°C and 550–700°C temperature ranges, while the Hg2+ profile matched total-Hg at 250–550°C. Compared with the other sample profiles, AUH had the highest Hg2+ peak (at approximately 750°C). In the case of INH (Fig. 5(c)), the total Hg profile was observed to be similar to that of Hg0 and Hg2+. Regarding the ISH (Fig. 5(d)), total-Hg and Hg0 nearly matched with each other, and Hg2+ release started above 850°C. This shows that there is almost no release of Hg2+ from ISH up to 850°C. For AUL (Fig. 5(e)), the main peak of the total-Hg appeared at a temperature range of 300–400°C, and at that temperature range, Hg2+ also exhibited the main peak. These two peaks had approximately the same formation rate and exhibited a total Hg profile primarily originating from Hg2+. From these results, we can observe that the evolution behavior of Hg2+ similarly depends on the iron ore type.

Fig. 5.

Release profiles of Hg0 and Hg2+ forms during TPHT of iron ore. (a) BRH, (b) AUH, (c) INH, (d) ISH and (e) AUL. (Online version in color.)

Figure 6 presents the distribution of Hg forms during TPHT for all five samples used in this study. The AUL sample has the highest percentage of solid-Hg and the lowest Hg2+, while AUH exhibits the highest Hg2+ content. The distribution percentages of Hg2+ increased in the following order: AUL < ISH < INH < BRH < AUH. When comparing INH, AUH, BRH, and ISH, the ores with higher Hg volatilization rates tend to emit mercury as Hg0.

Fig. 6.

Distribution of Hg forms during TPHT. (Online version in color.)

Figure 7(a) presents the relationship between the amount of volatilized total Hg and Hg concentration in iron ore. There was a relatively optimal correlation between the amount of volatilized total Hg and Hg concentration. This correlation was also observed in the case of volatility based on percentage; however, the correlation coefficients were smaller than those in the case of volatility based on weight. A positive correlation was also observed between the Hg0 and Hg2+ volatiles (Fig. 7(b)). In addition, released amounts of total Hg and Hg2+ or Hg0 exhibit a good positive correlation (Fig. 7(c)). These results indicate that the higher the amount of Hg in the ore, the more Hg content to be volatilized as Hg0.

Fig. 7.

Relationship among Hg content in iron ore, released amount of total-Hg, Hg2+, or Hg0. (Online version in color.)

Next, to examine the effect of ore content on Hg volatilization, we examined the relationship between Hg volatilization and each element content, as presented in Table 1, and the results obtained are shown in Fig. 8. Although variations exist (Fig. 8(a)), a linear negative correlation is observed among the total Hg, Hg0, Hg2+, and Si content in the ores. However, a curved negative correlation exists between the Ca content and total Hg, Hg0, and Hg2+; and the amount of gaseous Hg tends to decrease with increasing Ca content in the ores. Although the Si and Ca contents in the ore are overwhelmingly larger than those of Hg, the increase in the content of these species may influence Hg release. A detailed investigation on this issue is a topic for future research.

Fig. 8.

Relationship between gangue components and released amount of total-Hg, Hg2+ or Hg0. (a) Si content, (b) Ca content. (Online version in color.)

3.3. Hg Release during TPHT of Model Compounds

To investigate the volatilization form of Hg from iron ore, the total Hg evolution behavior of pure Hg compounds during TPHT is shown in Fig. 9, and the results are summarized in Table 2. The evolution of Hg from HgCl also starts above 100°C, and the evolution profile peaks at approximately 180°C and 200°C. The evolution behavior of Hg from these two pure Hg compounds exhibits asymmetric evolution profiles. However, HgS, HgO, and HgSO4 exhibit symmetrical profiles with peaks of Hg evolution rate at approximately 400°C, 600°C, and 700°C, respectively. The order of the evolution peak temperatures was HgCl2 < HgCl < HgS < HgO < HgSO4. This order was consistent with previous reports on the TPHT of pure Hg compound species.7,8,13) In contrast, the maximum TPHT peak temperatures of HgO, HgS, and HgSO4 in this study (Table 2) appear at higher temperatures than those of other research groups using air atmosphere;14,15,16,17) however, the above three species were in close agreement with previous reports that adopted nitrogen atmosphere.18) Although Hg-TPHT has been conducted by several researchers to investigate the morphology of Hg in samples such as coal, coal ash, and gypsum, the maximum TPHT peak temperature and evolution temperature of pure Hg compound species are different.7,8,9,14,15,18,19,20,21,22,23,24) Previous studies investigating Hg morphology in solids derived from coal utilization and gypsum via TPHT partitioned the peaks above 600°C into HgSO4 peaks.9,19) Considering the above points, the results of the TPHT in Table 2 are considered logical. It is well known that the decomposition of HgCl2, HgCl, HgS, HgO, and HgSO4 in air follows Eqs. (1), (2), (3), (4), (5), (6), (7), (8), (9).24,25)   

H g 2 C l 2 H g 0 ( g ) +HgC l 2 ( g ) (1)
  
HgC l 2 H g 0 ( g ) +C l 2 ( g ) (2)
  
HgOH g 0 ( g ) +0.5 O 2 ( g ) (3)
  
HgOH g 0 ( g ) +O( g ) (4)
  
H g 0 ( g ) +O( g ) H g 2 O( g ) (5)
  
HgSH g 0 ( g ) +0.5 S 2 ( s ) (6)
  
HgS+ O 2 ( g ) H g 0 ( g ) +S O 2 ( g ) (7)
  
HgS O 4 1/3HgS O 4 2HgO( s ) +2S O 2 ( g ) + O 2 ( g ) (8)
  
HgS O 4 2HgO( s ) 3H g 0 ( g ) +S O 2 ( g ) +2 O 2 ( g ) (9)
Fig. 9.

Release profiles of total-Hg from pure Hg-compounds and mixture of Hg compound and Fe2O3 (a) HgCl and HgCl/Fe2O3, (b) HgCl2 and HgCl2/Fe2O3, (c) HgS and HgS/Fe2O3, (d) HgO and HgO/Fe2O3, and (e) HgSO4 and HgSO4/Fe2O3. (Online version in color.)

Table 2. Summaries for Hg-TPHT results of pure Hg compounds and physical mixture of Fe2O3 and pure Hg compounds.
Hg speciesPure Hg compoundsFe2O3 mixture
Present workRef. [19]
Peak temp., °CRange, °CPeak temp., °CRange, °CPeak temp., °C bRange, °C
HgCl2150100–700138±490–350180 (m), 400 (s)100–550
Hg2Cl2180, 200100–600119±960–250180 (w), 350 (s)90–450
HgO (red)600500–700308±1, 471±5200–360, 370–530500 (s)400–600
HgS400250–500n.a.an.a.a450 (m)300–450
HgSO4720600–800583±8500–600550 (m)420–650

a Not analysis. b Peak intensity Designated by Hg-TPHT: w (weak), m (medium), s (strong).

However, the Hg elimination reaction from HgS and HgSO4 is unclear,25) and it has been reported that the HgSO4·2HgO produced in Eq. (8) was thermally stable up to 600°C.24) The complexity of the reaction may also be responsible for the different Hg-TPHT results in different research groups. Although there are some problems with the TPHT described above, the results of Hg evolution from iron ore can be compared with the results presented in Table 2, because the evolution behavior of Hg from ore and the TPHT of pure Hg compounds were carried out in the same apparatus and reaction conditions (temperature rise rate and atmosphere) in this study.

Figure 9 also presents the results of Hg evolution from a mixture of Fe2O3/Hg compounds. The evolution of Hg from HgCl/Fe2O3 is observed above 100°C, and the profile exhibits two peaks at 180°C and 350°C, respectively (Fig. 9(a)). Interestingly, this profile is relatively different from that of HgCl, and a new peak appears at 350°C. The evolution of Hg from HgCl2/Fe2O3 is observed above 100°C. It exhibits an asymmetric weak peak at approximately 180°C, and then decreased at 300°C. Although the evolution profile of Hg from HgCl2 is not observed above 300°C (Fig. 9(b)), a large peak appears at approximately 420°C for the HgCl2/Fe2O3 mixture. This tendency is similar to that of the HgCl/Fe2O3 mixture.

HgS/Fe2O3 exhibits a similar Hg evolution behavior to that of the pure compound. In contrast, the Hg evolution rates of HgO/Fe2O3 (Fig. 9(d)) and HgSO4/Fe2O3 (Fig. 9(e)) exhibit symmetrical evolution profiles with velocity peaks at approximately 500°C and 550°C, respectively. The evolution behavior of Hg from the physical mixture of Hg compounds and Fe2O3, excluding HgS, relatively differs from that of pure Hg. In other words, two peaks are observed for Hg chloride/Fe2O3, and the peak temperatures of HgO and HgSO4/Fe2O3 shift to lower temperatures compared to those of the pure compound. The 1st peak observed at approximately 200°C for HgCl or HgCl2/Fe2O3 was derived from HgCl and HgCl2, respectively. However, because the 2nd peak is not observed in the pure compound, it is considered to be triggered by the evolution of HgCl and HgCl2 species interacting with Fe2O3 during the heating process. According to previous reports, the adsorption of gaseous Hg0 on Fe2O3 does not occur.26) Therefore, the above interaction may be triggered by the solid-solid reaction between the HgCl species and Fe2O3. However, the peak temperatures of HgO/Fe2O3 and HgSO4/Fe2O3 shift to lower temperatures. A similar shift of the TPHT peak was reported in a previous study of the Hg-TPHT of a mixture of various Hg compounds and some substrates (SiO2, CaSO4·2H2O).24) It has been speculated that the decrease in the peak temperature of the Hg evolution profile was owing to the autocatalysis reaction by the substate.24,27) Therefore, the decrease in the Hg evolution peak temperature from the HgO and HgSO4/Fe2O3 mixed samples may be triggered by Fe2O3 acting as a catalyst. The details of this discussion will be the topic for future research.

According to previous studies that investigated the behavior of Hg release from coal, bauxite, and sequential leached coal, the Hg species released at high temperatures above 600°C are those associated with silicate,5,6,15) montmorillonite,10) refractory silicate, and mineral matrices.11) Consequently, the high-temperature Hg release observed at ≥ 600°C for all ores may be owing to the mineral matter present in ores.

3.4. Proportion of Hg Species Evolved during TPHT

Based on the results presented in Fig. 9, Fig. 10 shows the results of the curve fitting of the Hg evolution profile observed in Fig. 3. Here, HgClFe2O3 and HgClFe2O3 in Fig. 10 depict the Hg species that interacted with Fe2O3, as shown in Fig. 9. Table 3 presents the proportion of Hg forms calculated based on the curve-fitting results. As shown in Fig. 10, the Hg species volatilized above 600°C was not identified in this study; hence, the Hg species are unknown. In the AUL, Hg species that evolved until 600°C were mainly classified as HgCl, HgClFe2O3, HgS, and HgO. According to curve-fitting, HgS is the most abundant species, followed by unknown species, and HgClFe2O3 species accounts for a significant proportion. In the INL, the Hg forms volatilized below 600°C are assigned to HgClFe2O3, HgS, HgCl2Fe2O3, HgO, and HgSO4, and the presence of HgCl2 and HgCl species is not observed. The Hg species volatilized above 600°C were unknown species. In INL, although the presence of HgCl2 was not observed, HgCl2 Fe2O3 was detected. Using the model compounds described above, HgCl2Fe2O3 may be assigned as the source owing to the secondary reaction with HgCl2 and Fe2O3 from the experimental results (Fig. 9). In AUH, HgCl2, HgCl, HgO, and HgSO4 account for most of the volatile species below 600°C, and HgClFe2O3, HgS, and HgCl2Fe2O3 are observed in small amounts. Similar to the INL, unknown species account for most of the volatile species. The volatile Hg species in the ISH mainly comprise HgCl, HgCl2Fe2O3, HgO, and HgSO4, with small amounts of HgClFe2O3 and HgS. In addition, half of the volatiles are unknown. Although unknown species account for 80% of the volatiles from BRH, the others comprise HgO and HgSO4. From these results, it was determined that the forms of Hg evolution below 600°C were primarily assigned to HgCl2 and HgCl. HgClFe2O3, HgS, HgCl2Fe2O3, HgO, and HgSO4, and their proportions depended on the type of iron ore.

Fig. 10.

Proportion of the Hg-species that evolved during TPTH. (a) AUL, (b) INH, (c) AUH, (d) ISH, and (e) BRH. (Online version in color.)

Table 3. Summary of information in Fig. 9 and proportion of Hg forms.
SampleProportion of Hg evolution form, %-evolution basis
HgCl2HgClHgClFe2O3HgSHgCl2Fe2O3HgOHgSO4Unknown
AUL29163605329
INH0033531670
AUH351114580
BRH1010271178
ISH01722913750

The present study simulates the desorption behavior of mercury in the sintering process of iron ore. However, in the sintering process, carbonaceous substances for combustion and materials for adjusting basicity are added to iron ore. These substances are thought to affect the mercury desorption from iron ore during heating treatment. In the future, it will be important to study the mixture of iron ore with carbonaceous and basicity adjustment substances.

4. Conclusions

This study is focused on the determination of Hg release forms and profiles from iron ore during temperature-programmed heat treatment. The evolution behavior of Hg in iron ores depends on the type of iron ore. The Hg species that evolved during the heating treatment consisted of both Hg0 and Hg2+.

When the physical mixture of HgCl or HgCl2 and Fe2O3 was heated, the evolution profile showed that in addition to the evolution peak when the pure mercury chloride species was solely THTP, owing to a secondary reaction, a new evolution peak emerged on the high-temperature side. In the case of the physical mixture of HgO or HgSO4 and Fe2O3, the Hg evolution peak observed in the pure compounds shifted to the lower temperature side. The curve-fitting of Hg evolution behavior for iron ore indicated that the Hg species that evolved below 600°C were chlorides, sulfide, sulfate, and oxide species. However, the Hg species that evolved at temperatures above 600°C, which account for most of the desorbed Hg in several ores, were unknown.

Supporting Information

Figure S1 in Supporting Information is apparatus of Temperature-Programmed Heat Treatment.

This material is available on the Journal website at https://doi.org/10.2355/isijinternational.ISIJINT-2021-295.

Acknowledgments

This study was supported in part by a Grant-in-Aid for Challenging Research (Exploratory) from the Ministry of Education, Culture, Sports, Science and Technology, Japan, by the Iron and Steel Institute of Japan (ISIJ), and by the Steel Foundation for Environmental Protection Technology (SEPT).

References
 
© 2022 The Iron and Steel Institute of Japan.

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