Ross K.
Taggart
a,
Nelson A.
Rivera
a,
Clément
Levard
b,
Jean-Paul
Ambrosi
b,
Daniel
Borschneck
b,
James C.
Hower
c and
Heileen
Hsu-Kim
*a
aDepartment of Civil and Environmental Engineering, Duke University, Durham, NC 27708, USA. E-mail: hsukim@duke.edu; Tel: +1-919-660-5109
bAix Marseille Univ, CNRS, IRD, INRA, Coll France, CEREGE, Aix-en-Provence, France
cCenter for Applied Energy Research, University of Kentucky, Lexington, KY 40511, USA
First published on 28th September 2018
Coal combustion ash is a promising alternative source of rare earth elements (REE; herein defined as the 14 stable lanthanides, yttrium, and scandium). Efforts to extract REE from coal ash will depend heavily on the location and speciation of these elements in the ash. This study sought to identify the major chemical forms of yttrium (Y), as a representative REE in coal fly ash samples selected from major coal sources in the United States. Y speciation was evaluated using both bulk scale analyses (sequential extractions, Y K-edge X-ray absorption near-edge spectroscopy – XANES) and complementary analyses at the micron scale (micro-focus X-ray fluorescence and micro-XANES). Sequential selective extractions revealed that the REE were primarily in the residual (unextracted fraction) of coal fly ash samples. Extraction patterns for yttrium resembled those of the lanthanides, indicating that these elements were collectively dispersed throughout the aluminosilicate glass in fly ash. Bulk XANES analysis indicated that Y coordination states resembled a combination of Y-oxides, Y-carbonate, and Y-doped glass, regardless of ash origin. However, in the microprobe analysis, we observed “hotspots” of Y (∼10–50 μm) in some samples that included different Y forms (e.g., Y-phosphate) not observed in bulk measurements. Overall, this study demonstrated that yttrium (and potentially other REEs) are entrained in the glass phase of fly ash and that microscale investigations of individual high-REE regions in fly ash samples do not necessarily capture the dominant speciation.
Environmental significanceCoal combustion residues are large volume waste materials that have generated much attention for their disposal impacts to the environment. These impacts could be mitigated by instead extending the value chain of the waste and utilizing the ash as a source for rare earth elements (REEs). REEs such as yttrium are key constituents in many modern technologies, yet the global supply market for REEs is unstable. This work investigated differences between bulk- and micro-scale yttrium speciation in coal fly ash as a means to understand the chemical forms of REE in fly ash. This information is crucial to the development of efficient REE extraction processes for newly generated and legacy coal fly ash. |
Previous studies have shown several modes of occurrence for the REE that include forms evenly distributed throughout the glassy matrix of the fly ash as well as discreet mineral phases within the ash matrix.23,25–28 For example, one study utilized electron microprobe wavelength dispersive elemental mapping to show that cerium (measured as a proxy for all REE) was dispersed throughout the glassy matrix of the fly ash particles.26 More recent microscopy studies indicated that some REE trace phases from the coal such as monazite crystals may persist in the ash but are fragmented due to thermal shock.25 REE nanoparticles may also contribute to REE enrichment in coal ash in the absence of discrete REE mineral phases.12 Analysis by SHRIMP-RG ion microprobe (15 μm spot size) found that Fe- and Ca-enriched aluminosilicate glass phases of fly ash were enriched in REE relative to the bulk ash while the quartz was consistently depleted.29 The high-Al glass phase mirrored the bulk REE distribution. A recent X-ray absorption near-edge spectroscopy (XANES) study used Ce as a proxy for REE and identified Ce both dispersed in the glass phase and as micro-scale hotspots, consistent with previous studies.23 Collectively these findings indicate that REEs partition into the aluminosilicate glass, the most abundant component of fly ash.30 However, because microscopy-based studies entail spot measurements within a highly heterogeneous ash matrix, it is unclear if these analyses are representative of the total element speciation in the sample.
The objective of this research was to examine and compare the speciation of REE in coal combustion fly ashes, with a focus on yttrium, through a combination of bulk and micro-scale approaches. In this study, sequential extractions were used to determine the fraction of REE and other elements associated with the major operationally-defined phases of fly ash: water soluble, exchangeable/acid soluble, reducible, and oxidizable. Yttrium K-edge XANES was also used to complement the determination of REE-bearing fractions via sequential extraction by investigating the speciation of REE in fly ash. Yttrium was used as a proxy for REEs due to the frequent co-localization of REEs in minerals, coals, and coal ashes.29,31 Previous studies have similarly used Ce as a proxy for REEs.23,26 Yttrium was chosen because it is one of four REEs (Ce, La, Nd, and Y) with high enough concentrations in fly ash for X-ray absorption spectroscopy (XAS) and it is categorized as a “critical” REE due to high demand.6 Furthermore, the Y K-edge (17038 eV) lacks the spectral interferences which hinder Ce LIII-edge measurements. Another study using Y K-edge XANES found that the local coordination of Y in calcite resembles that of Ho, suggesting that Y is a valid proxy at least for heavy REEs (HREE; lanthanides Tb to Lu and Y due to its similar atomic radius).32 We expected bulk XAS to show that yttrium was associated with the glassy aluminosilicate phase in fly ash rather than as a distinct yttrium mineral. We hypothesized that there would be greater variation in yttrium speciation observed using micro-XANES because individual high yttrium mineral particles could exist in the fly ash sample without influencing the bulk spectra. By exploring both the distribution and speciation of yttrium and other REE in fly ash using the above techniques, we sought to identify characteristics that could eventually lead to improvements in REE recovery processes.
Sample ID | Sample no. | Plant ID (location) | CCP type | Elemental composition (%) | Y (mg kg−1) | Rare earth elements | |||||
---|---|---|---|---|---|---|---|---|---|---|---|
Si as SiO2 | Al as Al2O3 | Fe as Fe2O3 | Ca as CaO | Total (mg kg−1) | Critical (%) | HNO3-extractable (%) | |||||
App-FA1 | 93938 | I (Kentucky) | Fly ash, boiler 1 storage silo | 54.1 | 28.4 | 10.9 | 1.28 | 99.3 | 703 ± 0.3 | 35.3 ± 0.1 | 16.7 ± 0.6 |
App-FA2 | 93963 | H (Kentucky) | Fly ash, boiler 2 | 52.1 | 26.5 | 14.1 | 2.05 | 103.8 | 655 | 38.3 | 19.5 |
App-FA3 | 93932 | W (South Carolina) | Fly ash | 54.2 | 28.4 | 7.6 | 4.01 | 107.6 | 669 ± 5.1 | 36.7 ± 0.2 | 43.7 ± 2.2 |
App-PA | 93965 | C (Kentucky) | Pond ash | 57.4 | 28.7 | 5.72 | 1.32 | 75.5 | 531 | 36.2 | 23.2 |
IL-FA1 | 93895 | H (Kentucky) | Fly ash, boiler 3, ESP row 2 | 45.7 | 21.2 | 26.4 | 1.87 | 82.7 | 554 | 38.1 | 26.7 |
IL-FA3 | 93964 | H (Kentucky) | Fly ash, boiler 3 | 48.5 | 23.1 | 22.2 | 1.89 | 81.8 | 524 | 38.5 | 12.7 |
PRB-FA1 | 93966 | DE (Texas) | Fly ash | 38.3 | 22.5 | 5.21 | 22.9 | 50.7 | 406 ± 7.1 | 35.0 ± 0.1 | 52.4 ± 6.1 |
PRB-FA2 | 93973 | SC (Georgia) | Fly ash | 39.2 | 20.7 | 5.98 | 22.4 | 50.5 | 384 | 36.1 | 53.3 |
RSA-FA1 | 93969 | MA (South Africa) | Fly ash, classified | 53.7 | 31.5 | 3.68 | 4.98 | 69.0 | 622 | 30.4 | 20.4 |
All samples in Table 1 were examined for bulk Y speciation by XANES and for micron-scale elemental analysis via micro-focus X-ray fluorescence (μXRF). A subset of these were further analyzed for Y speciation at the micron scale by μXANES. For the sequential extractions, three samples (APP-FA1, IL-FA-1, and PRB-FA1) were selected based on their high total REE content and were also chosen to represent each of the three major U.S. coal basins. A summary of analyses performed for each sample is shown in Table S1.†
For one sample (APP-FA1), the sequential extraction procedure was repeated except that 1 M oxalic acid (still adjusted to pH 2 using HNO3) instead of acetic acid was used in the F2 step. Oxalic acid was chosen due to its high affinity for aluminum and ability to dissolve aluminosilicates, which comprise the bulk of fly ash particles. We hypothesized that oxalic acid would dissolve more of the glass phase, thereby making a higher percentage of the REE accessible. We also hypothesized that this would lead to a corresponding difference in the XRD patterns between the acetic acid and oxalic acid treatments.
For XRD analysis of solids collected between each extraction step, the samples were dried, ground by mortar and pestle, and dispersed with ethanol on zero-background silicon discs which were then mounted to sample holders. The original untreated fly ash samples were ground and then packed into back-loading XRD sample holders. XRD spectra of the original and extracted fly ash samples were collected on a Panalytical X'Pert Pro MPD instrument equipped with an X'Celerator detector and Co-Kα radiation source (λ = 1.79 Å). Samples were scanned over a 2θ range of 5° to 75° with a step size of 0.033°. The background signal from the amorphous phases of the fly ash was subtracted to normalize all diffractograms. Spectra were analyzed using X'Pert Highscore Plus v2.2b and the ICDDPDF-2 database (2003).
Three of the fly ash samples (App-FA1, IL-FA1, PRB-FA1) were further examined after extraction with oxalic acid or acetic acid to help understand results of the sequential extraction data. These samples are the same set selected for the sequential extraction experiments, but the extractions for XANES analysis were performed separately. The ash samples were extracted overnight with 1 mol L−1 oxalic acid or 1 mol L−1 acetic acid, rinsed with MilliQ water, allowed to dry, and loaded into sample holders as described previously.
Bulk yttrium speciation was analyzed by Y K-edge XANES collected in fluorescence mode on Beam Line 11-2 at the Stanford Synchrotron Radiation Lightsource (SSRL) utilizing a Si(220) phi = 0 crystal and a harmonic rejection mirror set to 20 keV. Yttrium energy calibration was performed with a Y metallic foil and the derivative of the first inflection point calibrated to 17038 eV. A germanium 100-element detector was used to collect fluorescence data along with an Al foil and a Sr filter to reduce the fluorescence signal of the other elements and scatter peak, respectively. Yttrium reference materials were analyzed in transmission mode (Fig. 4). All samples were held in a liquid nitrogen cryostat (77 K) during the collection of spectra.
For microprobe analysis, the samples were prepared in thin sections (30 μm thickness) by Spectrum Petrographics. Both μXRF and μXANES spectra were obtained at Beam Line 2-3 at the SSRL using a Si(111) phi = 0 crystal and a vortex silicon drift detector. The μXRF measurements were performed at an X-ray energy of 17100 eV with a nominal spot size of 5 μm by 5 μm. Yttrium hotspots were identified in fly ash thin sections via μXRF and the Y speciation of selected spots were analyzed by K-edge μXANES. Elemental fluorescence maps were analyzed using Sam's MicroAnalysis Toolkit (SMAK).40 The same yttrium reference compounds utilized for bulk Y-XANES were also analyzed by Y-μXANES (Fig. 4).
Each XANES and μXANES spectra was produced by averaging two separate scans (prior to normalization). Averaging, normalization, and linear combination fitting were performed using the software Athena.41 The linear combination fitting range was 17008 eV (30 eV below the Y K-edge) to 17158 eV (120 eV above the Y K-edge). Fits were selected to minimize both the R-factor (Table S2†) and the number of reference materials. Each sample spectrum was initially modeled to identify a combination of two reference spectra that could best fit the data. For each model fit, a third reference was added to the model only if both of the following conditions were met: (i) adding the third reference decreased the R-factor by 20% or more, (ii) the additional reference contributed ≥10% to the total fit weight.
Second, despite their differing geological origin, all three ash samples shared the same set of highly mobile elements. Arsenic, molybdenum, and selenium had the highest recoveries among all measured elements for the Illinois and Appalachian basin ashes (Fig. 1A and C). These elements are also known to be volatile during the combustion process.22,42–47 Selenium also had the highest recovery for the Powder River Basin ash (Fig. 1B). Although Mo recovery was lower than expected for the Powder River ash, it had the highest recovery of all elements in the initial water leach at over 20% for all ash samples. Arsenic was the only highly mobile element not recovered by the water leach but had the highest total recovery for both Appalachian ash treatments. Paradoxically, total recovery for arsenic was among the lowest in the Powder River Basin ash.
Third, using oxalic acid instead of acetic acid in the F2 extraction for APP-FA1 (Fig. 1D) changed the distribution of elemental recoveries between the leachable fractions but did not appreciably increase the total recovery of REEs (sum of F1–F4 fractions). We initially hypothesized that oxalic acid would produce higher REE recoveries because it forms strong complexes with Al3+ and can dissolve amorphous aluminosilicates such as the glass in fly ash. Previous research has determined that extractions should target the abundant glass phase where REE are hosted.7,9,28,29 While the use of oxalic acid instead of acetic acid in the acid soluble (F2) step significantly increased total REE recoveries in this fraction, less REE recovery was observed in the subsequent reducible (F3) fraction. This result suggests that oxalic acid liberated REE forms that were soluble in the F3 step. However, the majority of REE remained in the residual regardless of whether acetic acid or oxalic acid was used in the F2 extraction step.
Quartz, mullite, and iron oxides were the primary crystalline phases identified by XRD (Fig. 2 and 3), consistent with previous studies.21,23,28 Quartz was easily identified in all three ash samples. Mullite was also found in all three ashes, but at low concentration in the Powder River Basin ash sample. Iron minerals identified in IL-FA1 and App-FA1 included maghemite and hematite. PRB-FA1 (Fig. 3) had noticeably different mineralogy than the Appalachian and Illinois Basin ashes. The presence of minor periclase (MgO) and anhydrite (CaSO4) peaks is consistent with the higher Ca and Mg content of Powder River Basin ashes. Several prominent peaks (∼11° 2θ and ∼19° 2θ) could not be matched to plausible compounds.
The sequential extraction of the fly ash samples mostly did not change the XRD spectra for the solids. An exception was the Fe-oxide peak located at ∼42° 2θ in IL-FA1. The relative intensity of this peak decreased to a minimum after acetic acid extraction (F2) and then increased in relative intensity after the F3 and F4 extractions. The same Fe peak in App-FA1 also disappeared following the acetic and oxalic acid extractions (F2) but this peak never reappeared after F3 and F4 steps.
Linear combination fitting of the sample XANES spectra resulted in model fits with R-factors ranging from 0.000357 to 0.000797 for all nine ash samples (Table S2†). The weighted fits of reference spectra added to between 98.6% and 99.5% for the samples. Although the sample set included nine different ashes from four different coal basins, the spectral fits comprised similar reference materials (Fig. 5). All bulk ash fits were comprised primarily of Y2O3 (18% to 51%) and Y-doped glass (22% to 76%). Monazite was the next most represented reference, making up between 22% and 31% of the fits for five samples. The only other standards included in the bulk fits were YPO4 for App-FA2 (18%) and Y2(CO3)3 in IL-FA1 (30%) and App-PA (32%). For all Appalachian Basin and Illinois Basin samples, the Y2(CO3)3 reference spectra could be replaced by the monazite reference spectra without significantly altering the quality of the fit, indicating that the monazite and Y2(CO3)3 components may represent the same species. Y2(SO4)3, and the Y-doped hematite were not represented in any of the best fits for the untreated bulk fly ash samples.
After extracting the ash samples overnight with 1 M oxalic acid (Fig. 5 and Table S3†), most of the bulk XANES fits were dominated by Y-doped glass rather than Y2O3. App-FA1 and IL-FA1 were fit by the same standards as previously, which is consistent with the low REE recovery by oxalic acid during sequential extractions (Fig. 1D). However, the other Appalachian Basin fits were dominated by Y-doped glass (71–85%) with minor contributions from Y2O3. The standards comprising the Illinois Basin sample fits were unchanged after oxalic acid extraction, but the fit for IL-FA3 contained more Y-doped glass instead of Y2O3 and monazite. The Powder River Basin fits were profoundly changed by oxalic acid extraction: before they were mostly Y2O3 and Y-doped glass; afterwards, the Y2O3 was replaced by 47–65% Y2(SO4)3. The fit of the South African fly ash (RSA-FA1) remained mostly Y-doped glass but gained 20% Y2(SO4)3 contribution.
Separate samples of App-FA1, IL-FA1, and PRB-FA1 were subjected to acetic acid extraction and bulk XANES analysis (Fig. S5† and Table S3†). For all three samples, Y-doped glass (59% to 76%) dominated the fits after acetic acid extraction with 23–40% Y-doped hematite.
For Appalachian Basin ashes, we observed Y hotspots with spectral features that resembled YPO4. Points 1 and 2 of App-FA1 (shown in Fig. 6) were fit by 50–74% YPO4, while the bulk XANES fit contained no YPO4. The Y hotspot in Map 4 for App-FA3 closely matched the YPO4 spectrum, suggesting that this point was a discrete Y-phosphate particle (Fig. 7). In contrast, the Y-enriched areas of Map 6 from the same sample resembled the bulk XANES fits for Appalachian Basin ashes (Y2O3 and Y-doped glass) and the Y abundance was more distributed across Map 6 compared to the concentrated spot in Map 4.
Although the bulk XANES fits for IL-FA1 resembled those of the Appalachian Basin ashes, most of the Y hotspot fits were very different (Fig. 8). All μXANES fits included Y2O3 (36–63%) and a combination of Y2(CO3)3, and/or YPO4. All but one of the points analyzed included Y2(CO3)3 at 35–49%. Fits for two points contained YPO4 contributions (32% and 59%) like the Appalachian ashes. A second set of fits for IL-FA1 μXANES points (Fig. S6†) was less uniform, with 79–100% Y-doped glass in four points, 15–65% Y-doped hematite in three points, and 20–38% Y2O3 in two points. One fit contained 34% YPO4 spectra and another 63% monazite spectra.
For the Powder River Basin ashes, there was greater variation in fits between individual high-Y points (Fig. 9 and S6†). All but one of the high-Y PRB-FA1 points contained less Y2O3 and Y-doped glass than the bulk fit. The common features shared by the PRB-FA1 μXANES fits were major Y-doped hematite (44–66%) and YPO4 (20–57%) contributions in all but one point. The last point appeared to be comprised of glass (73%) and Y2O3 (27%). For PRB-FA2, both the bulk and micro-focus fits contained Y2O3 (43–54%). However, where the bulk fit contained 53% glass, three Y-hotspots contained 48–59% monazite and the last contained 52% Y2(CO3)3. As with the bulk ash fits, the monazite and Y2(CO3)3 components of the fits may represent the same species due to the similarity of the reference spectra.
Volatile elements (e.g. As, Se, Mo) tend to sorb to fly ash particles collected at the later (and cooler) stages of the flue gas control process.22,42–47 Therefore, these elements were much more extractable.30,53
The distribution of individual REE recoveries in each fraction differed noticeably between samples and was changed by using oxalic acid for F2. For PRB-FA1, the recovery of the lanthanides and Y occurred primarily in F4 (30.5 ± 3.4%), with the remainder split between F3 (16.9 ± 1.2%) and F2 (14.0 ± 2.1%). For IL-FA1, this distribution was the opposite, with recoveries decreasing slightly from F2 (4.8 ± 1.2%) to F3 (4.2 ± 0.7%) to F4 (2.4 ± 0.4%). App-FA1 had a similar extraction profile to IL-FA1, with low recoveries of REEs and high recoveries for volatile elements (As, Se, Mo), suggesting that the REEs were hosted in phases not easily leached by the sequential extraction solutions. Aggressive leaching or ash pretreatment such as alkaline digestion is required to extract further REE from Appalachian- and Illinois Basin-derived ashes.7,19,20
In the exchangeable/acid soluble extraction step (F2), App-FA1 was extracted with acetic acid and a replicate was extracted with oxalic acid of the same molarity. The primary effect of the oxalic acid extraction was to concentrate the recovery of REE and most other elements in the acid-soluble fraction (F2) at the expense of the reducible (F3) fraction. This was most evident in As, which was extracted mostly in F3 (73%) when using acetic acid and overwhelmingly in F2 (98%) when using oxalic acid. Recoveries from the reducible (F3) fraction were much lower following oxalic acid extraction. The only element with significant F3 or F4 recovery was Se with 28.3% recovery in F4; however, this was also true when using acetic acid. Overall recoveries for the volatile elements were significantly higher using oxalic acid: 102% vs. 83% As recovery, 91% vs. 71% Se recovery, and 76% vs. 52% Mo recovery. Overall REE recoveries were also slightly higher using oxalic acid. The metal chelating potential of oxalate (a dicarboxylate) compared to acetate (a monocarboxylate) may have enhanced the recovery of leachable elements.
Our extraction protocol included an initial distilled water leach (F1) that could be interpreted as simple environmental leaching conditions (especially relative to the subsequent extraction steps). This F1 extraction fraction is relevant because one of the largest potential ash sources for REE reclamation are legacy ash ponds which have been exposed to environmental weathering for years, sometimes decades. The only elements consistently mobilized by distilled water were Mo, Se, Ca, and Na. Aqueous REE recoveries were negligible. Molybdenum was the element with the highest aqueous recovery across all samples: 24.9% for IL-FA1, 23.8% for PRB-FA1, 21.9% for App-FA1 using acetic acid, and 20.5% for App-FA1 using oxalic acid. Aqueous Se recovery was similar for all samples, ranging from 6.2% to 8.5%. The higher aqueous leaching potential of these elements is well-known and expected given their adsorption to the surface of the ash particles.24,30,53–55
Calcium was the next most mobile element for the non-Powder River samples, with 22.1% recovery in IL-FA1, 12.5% for App-FA1 extracted with acetic acid, and 11.7% for App-FA1 extracted with oxalic acid. Although PRB-FA1 has significantly higher Ca content than Illinois or Appalachian basin ashes, the aqueous recovery for Ca was much lower at only 3.7%.
Overall uranium (U) recoveries were greater than REE recoveries except for PRB-FA1, suggesting that U is associated with particle surfaces.24,56 Thorium recoveries were always less than REE recoveries. The high mobility of U with respect to REE may present a problem for leaching and concentrating REE from fly ash, as REE separation processes often are not selective for REEs over U. It is important to understand the relative extractability of Th and U to avoid concentrating them to hazardous levels during REE recovery.
The crystalline mineral composition of the ash samples did not change much between extraction steps (Fig. S1–S4†). However, the relative intensities of the peaks did change with each extraction step. For instance, the prominent maghemite and hematite peaks of the Illinois Basin ash located at ∼39° 2θ and ∼42° 2θ decreased in amplitude following the F1 and F2 extraction steps and then increased after the F3 and F4 extraction steps (Fig. 2). A potential reason for this trend is that some Fe-oxide phases were extracted during the F1 and F2 steps, but then subsequent extracting reagents resulted in conversion of other Fe phases into these oxide forms that were detectable by XRD. The similarity of the spectra for the two App-FA1 extractions (Fig. S3 and S4†) was surprising given the effect oxalic acid had on leaching and our initial hypothesis that oxalic acid would be effective at attacking the amorphous aluminosilicates that comprise the background signal.
Differences in the major oxide composition of the ash samples manifested in the XRD results. The amplitudes of Fe-oxide peaks for the App-FA1 spectra were only half that of the same peaks in the IL-FA1 spectra. This difference can be attributed to the much higher Fe-oxide fraction of Illinois Basin ashes relative to Appalachian Basin ashes.7 The absence of prominent mullite and Fe-oxide peaks in the PRB-FA1 spectra is consistent with the composition of Powder River Basin ashes, which have lower Al- and Fe-oxide content than eastern U.S. coal ashes. Although the Al-oxide content of IL-FA1 (21.2%) and PRB-FA1 (22.5%) were similar, only IL-FA1 had identifiable mullite peaks. The low mullite concentration in PRB-FA1 suggests that the Al in Powder River Basin ashes is found primarily in amorphous glass phases rather than the mullite found in Appalachian and Illinois Basin ashes.
Recoveries for Sc by the sequential extractions were unexpectedly low relative to other REE recoveries. This difference was most pronounced for PRB-FA1, with only 11.6% total Sc recovered compared to 61.6 ± 5.5% of the other REE. The divergent extraction behaviors of Sc and the other REE indicate that they have differing modes of occurrence in PRB-FA1 and should not be categorized together in this case. Using oxalic acid, most Sc recovery occurred in F2 (i.e. by oxalic acid), while acetic acid recovered <0.7% of Sc. These results suggest that recoverable Sc resides in a phase leachable by oxalic acid but not acetic acid, such as Fe or Mn oxide. However, for App-FA1 and IL-FA1, both Sc and the other REEs remained mostly unrecovered, suggesting that they are associated with the glass phase.
Micro-focus XANES revealed that Y hotspots differed from the bulk mode of Y occurrence. These hotspots were 10–20 μm in diameter, within the typical size range of fly ash particles. However, the synchrotron micro-focus technique used in this study had a spot size of 2 μm × 2 μm, meaning that it was capable of distinguishing regions within individual ash particles.
Fits of Y hotspots also varied between samples, suggesting that the geological origin of the feed coal heavily influences microscale Y speciation in the ash. The striking similarity of microscale fits for IL-FA1 (Fig. 8) suggests that these points are the same Y species, while the greater variability between Y hotspots in PRB-FA1 may indicate multiple different microscale Y species. For PRB-FA1, the predominance of Y-doped hematite in the fits was unexpected given the lower Fe-oxide content of Powder River Basin ashes relative to eastern U.S. coal ashes. High YPO4 weights in App-FA1, App-FA3, and PRB-FA1 fits suggest that these points are composed at least partially of xenotime (yttrium orthophosphate). Several of the Y hotspots in the Illinois Basin ash also resembled YPO4, suggesting that yttrium phosphate minerals may be present in samples from all three coal basins. This is consistent with previous studies showing REE phosphate minerals in coals and coal ashes.18,23,28,57,58 The stark contrast between YPO4-like points (e.g. App-FA3 Map 4) and those resembling the bulk fits (App-FA3 Map 6) highlights the importance of scale when considering Y speciation.
While the μXANES spectra were often best fit with 2 or 3 reference materials, one could question the existence of 2-3 distinct Y phases in a small area (∼2 × 2 μm2) or in a single fly ash grain. Recent studies using higher resolution techniques (e.g. electron microscopy) have shown REE-bearing particles (0.01–1 μm diameter) within or on the surface of fly ash grains.25,59,60 Thus, multiple phases of Y in a single grain cannot be ruled out. Another explanation for our μXANES model fits is that the Y coordination state within each grain does not perfectly resemble the local coordination in our selection of reference materials.
Overall, the yttrium bulk XANES and μXANES analyses demonstrated that REE speciation in fly ash is heterogeneous and that with microscopy-based analyses, one can find areas of greater Y concentration (“hotspots”) with distinct phases of Y that differ from the bulk average. However, our analysis of these Y-hotspots comprised only 1.1% to 2.6% of the total Y μXRF signal and <0.2% of total area. Thus, previous work using microscopy-based methods might not be evaluating representative forms of REE. For extraction/recovery purposes, bulk Y speciation is more informative.
Bulk- and micro-scale XANES focusing on yttrium demonstrated that Y speciation of individual Y hotspots can drastically differ from the major form of Y observed at the bulk scale. The speciation of these hotspots also differed between samples but often shared features within the same sample. These findings indicate that micro-scale investigations of Y speciation in fly ash may not be representative of all Y forms in the sample. They also point to multiple modes of Y occurrence in fly ash, with minor high-Y points that do not necessarily reflect the dominant Y species. Therefore, for resource recovery applications, extraction methods should target the bulk forms of REE in fly ash, which appear to be associated with the aluminosilicate glass. Except for Powder River Basin ashes, aggressive leaching or alkaline digestion methods are required to recover REE from the glass phase.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c8em00264a |
This journal is © The Royal Society of Chemistry 2018 |