research papers\(\def\hfill{\hskip 5em}\def\hfil{\hskip 3em}\def\eqno#1{\hfil {#1}}\)

Journal logoSTRUCTURAL
CHEMISTRY
ISSN: 2053-2296

Ce, Gd and Yb accumulation in microalgae: an L-edge XAS study

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aCawthron Institute, 98 Halifax Street East, Nelson, 7010, New Zealand, bSchool of Food Technology and Natural Sciences, Massey University, Riddet Road, Palmerston North, 4410, New Zealand, and cAustralian Synchrotro, Australian Nuclear Science and Technology Organisation, 800 Blackburn Road, Melbourne, VIC, 3168, Australia
*Correspondence e-mail: [email protected]

Edited by X. Wang, Oak Ridge National Laboratory, USA (Received 22 April 2025; accepted 8 August 2025; online 18 August 2025)

The extraction and separation of rare earth elements (lanthanides) can be difficult due to their chemical similarities. Biological processes can have very selective activity towards different elements. We investigated the use of microalgae for this purpose by looking at the inter­action of Ce, Gd and Yb with the microalga Chlamydomonas reinhardtii, which has been induced to form polyphosphate granules. X-ray absorption spectroscopy with XANES and EXAFS at the Ce L3-edge, Gd L3-edge and Yb L3-edge was used to characterize the inter­action between the lanthanides and the phosphate-containing algae. All three of the lanthanides, added as the chloride salt to the algae, appeared to react to form phosphate com­pounds. These form both in the presence of phosphate granules or when there is only a low level of P present. CePO4 could be determined by XANES, but the structures of GdPO4 and YbPO4 were determined by EXAFS analysis without reference to the XAS spectra of the standard com­pounds. It is proposed that C. reinhardtii or other similar microalgae may be useful in the selective removal of rare earths from solution.

1. Introduction

Rare earth elements (lanthanides) are important for many technological applications. These include phosphors for lighting and displays, batteries, magnets and catalysts (Hu et al., 2024View full citation). Geopolitical considerations (Fan et al., 2023View full citation) and the limited range of high-grade ore deposits available (Zhao et al., 2023View full citation) provide incentives to find new sources of lanthanides that might include lower concentration deposits, by-product streams from other extraction processes and urban mining (Sedykh et al., 2022View full citation). New extraction methods may be needed for the lower concentration sources, including radioactive waste sources (Jun et al., 2023View full citation), and these methods could be greener, and more sustainable methods (Zapp et al., 2022View full citation) include biomining (Vo et al., 2023View full citation).

A possible method to extract lanthanides from solution could be adsorption or absorption by bacteria and algae (Birungi & Chirwa, 2014View full citation). For instance, the removal of La, Y, Sm, Nd and Eu from wastewater by bacteria was demonstrated by Sun et al. (2022View full citation) and Jacinto et al. (2018View full citation), and the removal of Y, Ce, Eu and Tb from solution by red algae has also been demonstrated (Iovinella et al., 2022View full citation). Cyano­bacteria can absorb Ce from wastewater (Sadovsky et al., 2016View full citation). It has also been shown that Cd can accumulate in the microalga Chlamydomonas reinhardtii (Penen et al., 2017View full citation). These pieces of evidence suggest that biological methods could be a means to separate mixtures of lanthanides if the absorption is significantly different for different lanthanides (Plouviez et al., 2024bView full citation).

To enhance the absorption of lanthanides into algae, the presence of phosphate, including polyphosphate granules that can be generated in some microalgae (Plouviez et al., 2024bView full citation; Cliff et al., 2023View full citation; Plouviez & Brown, 2024View full citation), has been considered (Plouviez et al., 2024bView full citation). This is based on the strong affinity that many rare earths have for phosphate, where the main mineral forms are monazite and xenotine, which are lanthanide phosphates. The affinity for phosphate increases along the lanthanide series from La to Lu (Wilharm et al., 2021View full citation).

A suitable technique for studying the chemistry of lanthanides in the solid state is X-ray absorption spectroscopy, either the near-edge region with XANES (X-ray Absorption Near Edge Spectroscopy) to give chemical information or an examination of the crystal structure in the local environment of the element of inter­est using EXAFS (Extended X-ray Absorption Fine Structure). Both require similar data collection. For the rare earth elements, the X-ray absorption edges easily accessible include the K-edges and the L-edges. Specifically, the L3-edge has been shown to be more sensitive to changes in chemical environment (Asakura et al., 2015View full citation, 2021View full citation).

It has been shown previously that Ce and Gd could absorb onto and within C. reinhardtii when the algae contains granules of polyphosphates (Plouviez et al., 2024bView full citation). Here we investigate the chemistry of Ce, Gd and Yb when this absorption has occurred, to understand the changes that have occurred in the rare earths with the P-containing algae. This range of Ce, Gd and Yb was chosen to represent a light, medium and heavy rare earth, with variation in the filling of electronic shells which should result in some slight differences in chemical bonding. Because standard phosphate com­pounds were not available for Gd and Yb, data measurements from an EXAFS analysis were required to assess whether these com­pounds had formed.

2. Materials and methods

2.1. Cultures

Chlamydomonas reinhardtii (CC-1690) culture main­ten­ance and cultivation were performed as described in Plouviez et al. (2021View full citation). Briefly, the microalga was sequentially cultivated on low-phospho­rus (1 mg P l−1) minimal media. The day of the experiment, 25 ml of culture was used to analyze the initial dry weight, optical density, total phospho­rus and dissolved phosphate, and also for microscopic observations (Plouviez et al., 2021View full citation).

Algal cultures were supplemented with a P dose equivalent to a final concentration of 10 mg P l−1, using a 1 M stock solution of potassium phosphate (46 g l−1 KH2PO4 and 115 g l−1 K2HPO4) and either CeCl3, GdCl3 or YbCl3 at a final concentration of 6, 10 or 11 mg l−1, respectively.

The cultures were harvested by centrifugation at 10000 g for 3.5 min (Sigma 6–16 centrifuge) in several batches. The pellets were rinsed with distilled water and centrifuged again before being mixed to make a com­posite sample and frozen at −80 °C. The algae pellets were finally freeze dried in a Buchi Lyovapor L-300 for 36 h at 0.2 mbar (1 bar = 105 Pa) with a tem­per­a­ture profile starting at −30 °C and finishing at 20 °C.

2.2. XAS/XANES

The information provided here follows recent guidelines for reporting XAS data (Paripsa et al., 2024View full citation). XAS scans at the Ce, Gd and Yb L3-edges were recorded at the MEX1 beamline at the Australian Synchrotron, ANSTO.

The MEX1 beamline uses X-rays from a bending magnet source and was configured for harmonic rejection for the energies of inter­est using a vertically collimating mirror translated to its rhodium stripe before a water-cooled Si(111) double crystal monochromator on an azimuth angle of 0°, and a vertical and horizontal focusing mirror also translated to its flat rhodium stripe after the monochromator. Energy resolution for MEX is (ΔE/E) of 1.4 × 10−4. Solid samples were pressed into 7 mm pellets for analysis. Standard com­pounds were mixed with cellulose powder and pressed into pellets for analysis and measured in transmission mode using 15 cm Ionitech gridded ion chambers filled with nitro­gen to an absolute pressure of 2 bar. Samples showing low concentrations (<2 wt%) of Ce, Gd and Yb were analysed in fluorescence mode using a four-element silicon drift detector. Samples were run using a beam size of 0.5 mm vertical × 3 mm horizontal, giving a photon flux of 3 × 1011 photons s−1. Ambient tem­per­a­ture (20 °C) and atmospheric pressure under helium were used as the sample environment. Beam energy was calibrated using Cr, Co and Cu metal foils for Ce, Gd and Yb, respectively, by aligning the peak of the first derivative of their respective K-edges to reference values.

Sample scans employed variable step sizes, with a large step for the pre-edge region, a very small step over the edge region, a larger step size for the post-edge (XANES) region, and a larger and variable step size increasing in proportion to k for the EXAFS region. The recorded energy range was expanded to include the edge energy of the reference metal foils with a small step size in the region of the reference metal edge. The energy range and step sizes used are listed in Table 1[link]. This scanning was run in continuous scanning mode (not discrete steps).

Table 1
Parameters used for data collection

Element Region Start energy (keV) End energy (keV) Step size (keV) Step size varies by k Time per step (s) Number of points
Ce 1 5.523 5.703 0.01   1 18
(Cr ref.) 2 5.703 5.773 0.00025   1 280
  3 5.773 5.985 0.035 yes 1 134
  4 5.985 6.012 0.0002   0.2 135
  5 6.012 6.160 0.0035   1 43
               
Gd 1 7.043 7.090 0.01   1 5
(Co ref.) 2 7.090 7.131 0.00025   0.1 164
  3 7.131 7.22 0.01   1 9
  4 7.22 7.293 0.00025   1 292
  5 7.293 7.800 0.0035 yes 1 242
               
Yb 1 8.744 8.924 0.01   1 18
(Cu ref.) 2 8.924 8.994 0.00025   1 280
  3 8.994 9.493 0.0035 yes 1 240

ATHENA (Ravel & Newville, 2005View full citation) software was used to process the XAS spectra. ATHENA was used for background removal, with E0 unconstrained, and for spectra normalization.

2.3. EXAFS

Data for EXAFS was recorded over a k of 10.6 Å−1 for Ce, 11.95 Å−1 for Gd and 11.8 Å−1 for Yb. Data processing and fitting used only a portion of this data range, as detailed in Table 2[link]. Bond lengths were calculated using ATOMS and FEFF6 (within ARTEMIS) (Ravel & Newville, 2005View full citation), with CIF data taken from the Crystallographic Open Database (COD) (Gražulis et al., 2009View full citation). ARTEMIS was used to fit spectroscopic data to crystal structure data. Where we had not been able to measure the spectra of the reference com­pounds of inter­est (GaPO4 and YbPO4), we calculated the EXAFS spectra from the CIF data taken from the COD (Table 2[link]), and these are also available on the Materials Project, where a com­pilation of many FEFF files are also available (Jain et al., 2013View full citation; Mathew et al., 2018View full citation).

Table 2
Fitting parameters used for EXAFS analysis in ATHENA (Ravel & Newville, 2005View full citation)

Compound   Fourier transform kmin Fourier transform kmax Fitting space Rmin used in fitting Rmax used in fitting Longest scattering path used Number of scattering paths used
CeO2   2 10 R 1 6 4.766 14
CeCl3·7H2O   2 10 R 1 6 4.939 158
CePO4   2 10 R 1 6 4.980 151
CePO4 in C. reinhardtii   2 10 R 1.7 5 4.980 151
Gd2O3   3 11 R 1 6 4.910 36
GdCl3·7H2O   3 11 R 1 5 2.911 2
GdPO4 in C. reinhardtii   3 11.5 R 1 6 3.227 8
Yb2O3   3 11.8 R 1.5 5 4.865 22
YbPO4 in C. reinhardtii   3 11.5 R 1.5 4.5 4.360 20

2.4. Inductively coupled plasma mass spectrometry (ICP–MS)

The samples were prepared by the following method. The sample (1.0 ml) was added to a 15 ml centrifuge tube and 1.5 ml 69% HNO3 (Tracepur, Merck) and 0.5 ml 37% HCl (Tracepur, Merck) were added. The vessels were sealed and placed in a 100 °C water bath for 30 min. The digest was diluted with 13 ml Type-1 water to a 15 ml final volume. The solutions were qu­anti­tatively analysed for desired elements on an Agilent 7700 ICP–MS in He mode to reduce polyatomic inter­ferences. Calibration standards were prepared in a matrix matched solution from 1000 ppm single element standards (CPI Inter­national, USA). A 20 ppb solution of Y was used to monitor drift and matrix effects. All results are in µg g−1 and have been back calculated to the original sample.

3. Results

3.1. P, Ce, Gd and Yb accumulation in C. reinhardtii samples

The transition from P deplete to P replete conditions in the absence of added rare earths triggered P accumulation in C. reinhardtii up to (2.50 ± 0.42)% P in the dry weight of algae. Similar concentrations were measured for the cultures supplemented with P and the rare earths with (2.40 ± 0.31)% P, (2.60 ± 0.01)% P and (2.32 ± 0.15)% P for the samples supplemented with Ce, Gd and Yb, respectively. ICP–MS analysis of dried C. reinhardtii samples showed that the microalgae supplemented by both P and either Ce or Gd accumulated Ce at 0.57 ± 0.54% Ce and Gd at 1.5 ± 0.9% Gd. This absorption amounts to 17% of the Ce and 27% of the Gd available from solution.

A large shift (3.4 eV) is observed in E0 (the absorption edge energy) in the XANES spectra with oxidation state, with CeIVO2 at 5729.0 eV and CeIIICl3 and CeIIIPO4 at 5725.3 and 5725.5 eV, respectively. With algae, the oxidation state of Ce, based on E0, is clearly III at 5724.6 eV with higher P level and 5724.9 eV with only low levels of P, which is not a significant shift. In the near-edge region [Fig. 1[link](b)], the difference between the algae with or without extra P and between CeCl3 and CePO4 are subtle and not helpful in identifying differences in structure. In the k plots [Fig. 1[link](c)], the structure of CeCl3 is clearly differentiated. It is then apparent that the C. reinhardtii samples do not contain CeCl3, but com­pounds much closer to CePO4. This is also supported by the R plot [Fig. 1[link](d)], where the different bond lengths of CeCl3 than CePO4 are apparent.

[Figure 1]
Figure 1
Ce L3-edge XAS for C. reinhardtii and standard com­pounds. (a) XANES, (b) near-edge region, (c) EXAFS function k2χ(k) and (d) Fourier transform moduli of the EXAFS spectra.

3.2. XAS Ce

The bond lengths determined from an EXAFS analysis shown in Fig. 1[link](d) clearly differentiate between the different reference com­pounds and identify that CePO4 is the dominant form of Ce in the algae. The most intense scattering peaks determined from FEFF6 calculations from published structures for these com­pounds are given in Table 3[link]. The shortening of the Ce—O bond at higher oxidation state is clearly visible in the data recorded here. The distinctive Ce—P bonds at 3.2–3.3 Å are a clear characteristic of CePO4 which is visible in the R plots.

Table 3
Structural parameters for selected bonds in Ce com­pounds and C. reinhardtii calculated by ATOMS (Ravel & Newville, 2005View full citation) from CIF files and by fitting of the structure to the EXAFS data recorded here

Compound (CIF used) Bond R (Å) from ATOMS of CIF Relative intensity from ATOMS R (Å) from EXAFS fit N σ22) ΔR r factor for fit of com­pound
CeO2 Ce—O 2.34 100 2.38 8 0.0078 −0.00057 0.15
(4343161) Ce—Ce 3.83 67 3.82 12      
  Ce—O 4.49 51 4.48 24      
                 
CeCl3·7H2O Ce—O 2.51 100 2.51 4 0.0042 0.0058 0.13
(2201515) Ce—O 2.54 73 2.54 3      
  Ce—Cl 2.91 42 2.92 2      
                 
CePO4 Ce—O 2.465 100 2.46 3 0.020 −0.0092 0.11
(9001646) Ce—O 2.53 60 2.52 2      
  Ce—O 2.58 60 2.57 2      
  Ce—O 2.64 28 2.64 1      
  Ce—O 2.78 25 2.77 1      
  Ce—P 3.20 18 3.19 1      
  Ce—P 3.28 17 3.27 1      
  Ce—P 3.75 35 3.74 3      
  Ce—Ce 4.08 30 4.07 2      
                 
CePO4 in C. reinhardtii Ce—O 2.465 100 2.47 3 0.0059 0.0063 0.14
(9001646) Ce—O 2.53 60 2.53 2      
  Ce—O 2.58 60 2.59 2      
  Ce—O 2.64 28 2.65 1      

From the bond lengths it is apparent that the C. reinhardtii samples do not contain CeCl3, but rather contain CePO4, corroborating the XANES E0 data discussed above. There appear to be no difference in the structure of the Ce com­pounds in C. reinhardtii with or without P. Clearly, CePO4 forms with the algae in both cases, and that there is enough P present for this under P-limited conditions for normal cell growth. No significant portion of Ce remains as CeCl3, the form in which it was added.

3.3. XAS Gd

For the Gd analysis, no Gd phosphate standard was available for com­parison. We therefore relied on EXAFS analysis of the bond lengths, and a com­parison with EXAFS calculated from available crystal structure data, for a full inter­pretation. EXAFS analyses of GdPO4 measured at the L3-edge have been reported previously (George et al., 2010View full citation; Morss et al., 1996View full citation; Yoon et al., 2002View full citation).

In the near-edge region, the difference between the algae with or without extra P and between GdCl3 and Gd acetyl­ace­ton­ate are subtle and not helpful in identifying differences in structure, although Gd2O3 is clearly different and not similar to the algae samples or the other standards. In the near-edge region, the Gd in C. reinhardtii looks the same with and without extra P (Fig. 2[link]).

[Figure 2]
Figure 2
Gd L3-edge XAS for C. reinhardtii and standard com­pounds. (a) XANES, (b) near-edge region, (c) EXAFS function k2χ(k) and (d) Fourier transform moduli of the EXAFS spectra. GdPO4 in parts (c) and (d) are derived spectra from literature crystal structures.

However, in the k plot, there are clear differences between Gd in C. reinhardtii and the standards GdCl3 and Gd acetyl­ace­to­nate in the range 8.5–10.5 Å−1. The differences are also pronounced in the R plot, where the peaks at 3.2 and 4.1 Å in the algae samples are not present in the standards (Fig. 2[link]).

The bond lengths determined from an EXAFS analysis clearly differentiate between the different reference com­pounds and identify that GdPO4 is the dominant form of Gd in the algae. The most intense scattering peaks determined from FEFF6 calculations from published structures for these com­pounds are given in Table 4[link]. The bond lengths of 3.2 and 4.1 Å corresponding to Gd—P and Gd—Gd provide strong evidence of the presence of GdPO4 in the algae samples, both with extra P and with low levels of P. To confirm this, a full fitting of the crystal structure of GdPO4 to the EXAFS data for the C. reinhardtii with P granules was performed (using ARTEMIS running FEFF6) (Fig. 2[link]). This provided an adequate fit to the structure.

Table 4
Structural parameters for selected bonds in Gd com­pounds and C. reinhardtii calculated by ATOMS (Ravel & Newville, 2005View full citation) from CIF files and by fitting of the structure to the EXAFS data recorded here

Compound (CIF used) Bond R (Å) from ATOMS of CIF Relative intensity from ATOMS R (Å) from EXAFS fit N σ22) ΔR r factor for fit of com­pound
Gd2O3 Gd—O 2.34 100 2.38 8 0.0078 −0.00057 0.15
(1010338) Gd—Gd 3.83 67 3.82 12      
  Gd—O 4.49 51 4.48 24      
                 
GdCl3·7H2O Gd—O 2.51 100 2.51 4 0.0042 0.0058 0.13
(2310334) Gd—O 2.54 73 2.54 3      
  Gd—Cl 2.91 42 2.92 2      
                 
GdPO4 in C. reinhardtii Gd—O 2.465 100 2.46 3 0.020 −0.0092 0.11
(1530459) Gd—O 2.53 60 2.52 2      
  Gd—O 2.58 60 2.57 2      
  Gd—O 2.64 28 2.64 1      
  Gd—O 2.78 25 2.77 1      
  Gd—P 3.20 18 3.19 1      
  Gd—P 3.28 17 3.27 1      
  Gd—P 3.75 35 3.74 3      
  Gd—Gd 4.08 30 4.07 2      

3.4. XAS Yb

For the Yb analysis, we also did not have a Yb phosphate standard for com­parison. We therefore again relied on EXAFS analysis of the bond lengths, and a com­parison with EXAFS calculated from available crystal structure data, for a full inter­pretation. An EXAFS analysis of YbPO4 measured at the L3-edge has been reported previously (Louvel et al., 2015View full citation), as well as a Raman spectroscopy analysis (Becker et al., 1992View full citation).

In the near-edge region, the difference between the algae with or without extra P and between YbCl3 and Yb in C. reinhardtii are subtle but, based on the experience with Ce and Gd, we do not expect this to be definitive in identifying differences in structure, although Yb2O3 is clearly different and not similar to the algae samples or YbCl3. In the near-edge region, the Yb in C. reinhardtii looks the same with and without extra P.

However, in the R plot, the differences are pronounced, where the peak at 3.0 Å in the algae samples is not present in the standards (Fig. 3[link]). Also apparent in the R plot is the longer radial distance for the Yb—Cl bond length, forming the dominant low radial distance peak, com­pared with the Yb—O bond length in YbPO4 or Yb2O3. From this, the YbCl3 structure is easily able to be ruled out as a possible structure in C. reinhardtii.

[Figure 3]
Figure 3
Yb L3-edge XAS for C. reinhardtii and standard com­pounds. (a) XANES, (b) near-edge region, (c) EXAFS function k2χ(k) and (d) Fourier transform moduli of the EXAFS spectra. k data is smoothed (11 point average). YbPO4 in parts (c) and (d) are derived spectra from literature crystal structures.

The bond lengths determined from an EXAFS analysis clearly differentiate between the different reference com­pounds and identify that YbPO4 is the dominant form of Yb in the algae. The most intense scattering peaks determined from FEFF6 calculations from published structures for these com­pounds are given in Table 5[link]. We were not able to get convergence of a fit of the data for Yb in C. reinhardtii to YbCl3.

Table 5
Structural parameters for selected bonds in Yb com­pounds and C. reinhardtii calculated by ATOMS (Ravel & Newville, 2005View full citation) from CIF files and by fitting of the structure to the EXAFS data recorded here

Compound (CIF used) Bond R (Å) from ATOMS of CIF Relative intensity from ATOMS R (Å) from EXAFS fit N σ22) ΔR r factor for fit of com­pound
Yb2O3 Yb—O 2.36 100 2.30 6 0.011 −0.057 0.46
(1548520) Yb—Yb 3.48 48 3.43 6      
  Yb—Yb 3.96 36 3.90 6      
  Yb—O 4.05 22 4.00 6      
  Yb—O 4.21 19 4.15 6      
                 
YbCl2 Yb—Cl 2.793 100          
(2310334) Yb—Cl 2.836 48          
  Yb—Cl 2.889 100          
  Yb—Cl 2.922 32          
  Yb—Yb 4.235 15          
  Yb—Cl 4.292 22          
  Yb—Yb 4.360 27          
  Yb—Yb 4.552 25          
                 
YbPO4 in C. reinhardtii Yb—O 2.27 100 2.16 4 0.0071 −0.11 0.28
(9001660) Yb—O 2.36 92 2.24 4      
  Yb—P 2.98 29 2.87 2      
  Yb—O—P 3.43 10 3.32 8      
  Yb—O—O 3.69 42 3.58 8      
  Yb—Yb 3.72 56 3.60 4      

The bond length of 3.0 Å corresponding to Yb—P provides evidence of the presence of YbPO4 in the algae samples, both with extra P and with low levels of P. To confirm this, a full fitting of the crystal structure of YbPO4 to the EXAFS data for the C. reinhardtii with P granules was performed (using ARTEMIS running FEFF6) (Table 5[link]). The fit to the structure of YbPO4 was poor, but is probably adequate for the noisy quality of the data. The data did not require smoothing prior to fitting, because of the nature of using a Fourier transform for this fitting, which separates the high-frequency noise; however, for the purposes of displaying the experimental data, an 11-point moving average was used.

4. Discussion and conclusions

Previously, we have shown that phosphate granules that form in C. reinhardtii are com­posed of polyphosphates, some in the form of inositol phosphate (otherwise known as phytate) (Plouviez et al., 2024aView full citation). We then showed with scanning transmission X-ray microscopy that the addition of Gd to these algae results in an association of Gd with P, including with the polyphosphate granules inside the algae (Plouviez et al., 2024bView full citation). With Ce there was an association of Ce with P but not within the algae. That previous work did not investigate the inter­actions of Yb.

P K-edge XANES on the Gd- and Ce-doped algae with extra phosphate showed some change in the chemistry of P, suggesting that there is a chemical inter­action between the rare earths and phosphate (Plouviez et al., 2024bView full citation). However, the P atom is inter­acting only at a distance, via the O atom bonded to phospho­rus, and therefore the chemical changes observed at the P atom are not large. A more sensitive measure of that inter­action is the work described here, where this same inter­action is observed from the rare earth atom. The change is one that is more direct, with the lanthanide inter­acting not with a chloride ion in the com­pound added, but with a phosphate ion, a larger difference in electronic inter­action. It is an inter­action specific to the lanthanide ion – so that if the phosphate is in a variety of states, with some bonded to lanthanide and some not, this will not confound the results, unlike with P K-edge XAS.

In this work, we have found that XANES was very useful in identifying the chemical structures present for Ce. There were significant differences in the near-edge spectra for the different Ce com­pounds and we had a spectrum of CePO4 for com­parison which provided a good match. For Gd and Yb we were not able to record spectra of the phosphate com­pounds from standards, so we had to rely on EXAFS analysis of the crystal structure. Fortunately, crystal structures of Gd and Yb phosphates are available in the literature, so it was possible to model the EXAFS spectrum from these structures to fit with the data recorded in this work and find a good match to GdPO4 and a reasonable match to YbPO4.

The L3-edge for Ce, Gd and Yb provided sufficient sensitivity to chemical changes to be useful for analytical purposes. Other studies have investigated this sensitivity in more detail for each of the elements at the X-ray edge (Asakura et al., 2015View full citation, 2021View full citation), with many studies on Ce and some specifically on Gd (George et al., 2010View full citation; Morss et al., 1996View full citation; Yoon et al., 2002View full citation) and Yb (Louvel et al., 2015View full citation).

This study suggests that microalgae with phosphate may be a useful method of capturing rare earths from solutions. These are living organisms so the tolerance of these organisms to the presence of lanthanides also needs to be considered if this is to be a viable extraction technique. This was not directly addressed in the work presented here. However, other studies have investigated aspects of tolerance to lanthanides. In Chlorella sp., Ce3+ slightly boosted biomass production in concentrations up to 7 µM, but in C. reinhardtii, Ce has been found to decrease photosynthetic yield at concentrations of 1–200 µM (Röhder et al., 2014View full citation). Although it has also been found that in C. reinhardtii, Ce3+ does not inhibit cell growth when the Ce is stabilized by phosphate (Röhder et al., 2014View full citation). The protective effect of polyphosphate accumulation has also been observed with uranium, where it increases tolerance for the cyano­bacterium Anabaena torulosa (Chandwadkar & Acharya, 2023View full citation).

The extraction and separation of rare earth elements (lanthanides) can be difficult due to their chemical similarities (Baldwin et al., 2018View full citation). Biological processes can have very selective activity towards different elements. However, all three of the lanthanides added to the algae as chloride reacted to form phosphate com­pounds. These formed both in the presence of polyphosphate granules or when there was only a low level of P present. Nevertheless, C. reinhardtii or other similar microalgae may be useful in the removal of rare earths from solution, with the selectivity to different lanthanides yet to be determined.

Acknowledgements

The authors thank Stuart Morrow, School of Chemical Sciences, The University of Auckland, for the ICP–MS analysis. Open access publishing facilitated by Massey University, as part of the Wiley–Massey University agreement via the Council of Australian University Librarians.

Conflict of interest

The authors declare that they have no known com­peting financial inter­ests or personal relationships that could have appeared to influence the work reported in this paper.

Data availability

Raw data and fitted data are available on request.

Funding information

Funding for this research was provided by: Australian Nuclear Science and Technology Organization (grant No. M20433); New Zealand Synchrotron Group; French Embassy of New Zealand, Pacific Fund (grant No. 2337); Ministry of Business, Innovation and Employment (grant No. MAUX2302).

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