Published January 21, 2021 | Version Supplemental Material
Journal Article Open

Distribution Coefficients of the REEs, Sr, Y, Ba, Th, and U between α-HIBA and AG50W-X8 Resin

  • 1. ROR icon California Institute of Technology
  • 2. ROR icon University of Chicago
  • 3. ROR icon Korea Institute of Geoscience and Mineral Resources

Abstract

Rare-earth elements (REEs) are known for their similar behaviors, which make their purification through chromatographic techniques particularly challenging. The use of α-hydroxyisobutyric acid (α-HIBA) in combination with a cation-exchange resin is perhaps the most widely used chromatographic technique to separate individual REEs from each other. However, only limited REE partition data between α-HIBA and cation resins exist, which makes it challenging to develop and optimize purification techniques using this platform. Here, we report distribution coefficients (K_d) of REEs, as well as Sr, Y, Ba, Th, and U, between α-HIBA at pH = 4.50 and AG50W-X8 cation-exchange resin, obtained by batch equilibration experiments. For all 19 elements, the distribution coefficients decrease with increasing acid concentration. For the REEs, a linear relationship is observed in log–log space between K_d values and α-HIBA molarity. While the K_d values have been calibrated at pH = 4.50, formulas are provided allowing recasting of the K_d values at any pH. To test the accuracy of the data, we compare elution curves simulated using the newly determined distribution coefficients to actual elution curves. The close agreement between simulated and experimental elution curves demonstrates that the distribution coefficients obtained in this study are effective to devise multielement extraction and purification scheme for high-precision elemental and isotopic analyses of REEs for various applications.

Additional Information

© 2020 American Chemical Society. Received: October 1, 2020; Revised: December 2, 2020; Accepted: December 2, 2020; Published: December 15, 2020. We thank the three anonymous reviewers and editor Joel D. Blum for constructive criticisms, which greatly helped us to improve the manuscript. This work was supported by grants NASA grants NNX17AE86G, NNX17AE87G, 80NSSC17K0744, and 80NSSC20K0821 and NSF grant EAR-2001098 to N.D.; grant GP2020-003 (provided by Korea Institute of Geoscience and Mineral Resources) to S.-G.L.; NASA grant 80NSSC20K1398 (PI: F.L.H.T., FI: H.L.), NSF grant EAR-1824002, and start-up funds (provided by Caltech) to F.L.H.T. Author Contributions. N.D., F.L.H.T., and S-G.L. conceived the study. S.-G.L. and F.L.H.T. performed the partitioning experiments. H.L. and F.L.H.T. processed and interpreted the data. E.H. conducted Elution 2. H.L. wrote the first draft under F.L.H.T.'s guidance. All authors contributed to writing and/or editing of the manuscript. The authors declare no competing financial interest.

Attached Files

Supplemental Material - sp0c00273_si_001.pdf

Supplemental Material - sp0c00273_si_002.zip

Files

sp0c00273_si_001.pdf

Files (25.6 MB)

Name Size Download all
md5:9921c2e609f35273d8aa26ecb8a711c5
289.2 kB Preview Download
md5:614e48d0d1a32274220e433022cfe058
25.3 MB Preview Download

Additional details

Identifiers

Eprint ID
107104
DOI
10.1021/acsearthspacechem.0c00273
Resolver ID
CaltechAUTHORS:20201215-141038772

Related works

Funding

NASA
NNX17AE86G
NASA
NNX17AE87G
NASA
80NSSC17K0744
NASA
80NSSC20K0821
NSF
EAR-2001098
Korea Institute of Geoscience and Mineral Resources
GP2020-003
NASA
80NSSC20K1398
NSF
EAR-1824002
Caltech

Dates

Created
2020-12-15
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)