Article (Scientific journals)
Abnormal concentrations of Cu-Co in: Haumaniastrum katangense, Haumaniastrum robertii and Aeolanthus biformifolius: Contamination or hyperaccumulation?
Van Der Ent, A.; Malaisse, François; Erskine, P. D. et al.
2019In Metallomics, 11 (3), p. 586-596
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Keywords :
Binary alloys; Cobalt compounds; Contamination; Copper alloys; Copper compounds; Energy dispersive spectroscopy; Scanning electron microscopy; Soil pollution; Tissue; X ray absorption spectroscopy; Abnormal concentrations; Central African Copperbelt; Herbarium specimens; Hyperaccumulation; Hyperaccumulator plant; Mineral particles; Synchrotron x ray absorption spectroscopy; Tissue concentrations; Cobalt alloys; Aeolanthus biformifolius; Article; Haumaniastrum katanganse; Haumaniastrum robertii
Abstract :
[en] The Central African Copperbelt of the DR Congo and Zambia hosts more than 30 known Cu-Co hyperaccumulator plant species. These plants can accumulate extraordinarily high concentrations of Cu and Co in their living tissues without showing any signs of toxicity. Haumaniastrum robertii is the most extreme Co hyperaccumulator (able to accumulate up to 1 wt% Co), whereas Aeolanthus biformifolius is the most extreme Cu hyperaccumulator (with up to 1 wt% Cu). The phenomenon of Cu-Co hyperaccumulator plants was studied intensively in the 1970s through to the 1990s, but doubts arose regarding earlier observations due to surficial contamination of plant material with mineral particles. This study set out to determine whether such extraneous contamination could be observed on herbarium specimens of Haumaniastrum robertii and Aeolanthus biformifolius using scanning electron microscopy with energy-dispersive spectroscopy (SEM-EDS). Further, synchrotron X-ray absorption spectroscopy (XAS) was used to identify the chemical forms of Cu and Co in newly collected Haumaniastrum katangense plant material from the DR Congo. The results show that surficial contamination is not the cause for abnormal Cu-Co concentrations in the plant material, but rather that Cu-Co enrichment is endogenous. The chemical form of Cu and Co (complexation with carboxylic acids) provides additional evidence that genuine hyperaccumulation, and not soil mineral contamination, is responsible for extreme tissue concentrations of Cu and Co in Haumaniastrum katangense. © 2019 The Royal Society of Chemistry.
Disciplines :
Phytobiology (plant sciences, forestry, mycology...)
Author, co-author :
Van Der Ent, A.;  Centre for Mined Land Rehabilitation, Sustainable Minerals Institute, University of QueenslandQLD, Australia, Université de Lorraine-INRA, Laboratoire Sols et Environnement UMR1120, France
Malaisse, François ;  Université de Liège - ULiège > Département GxABT > Biodiversité et Paysage
Erskine, P. D.;  Centre for Mined Land Rehabilitation, Sustainable Minerals Institute, University of QueenslandQLD, Australia
Mesjasz-Przybyłowicz, J.;  Department of Botany and Zoology, Stellenbosch University, Private Bag X1, Matieland, 7602, South Africa
Przybyłowicz, W. J.;  Department of Botany and Zoology, Stellenbosch University, Private Bag X1, Matieland, 7602, South Africa, AGH University of Science and Technology, Faculty of Physics and Applied Computer Science, Kraków, 30-059, Poland
Barnabas, A. D.;  Department of Botany and Zoology, Stellenbosch University, Private Bag X1, Matieland, 7602, South Africa
Sośnicka, M.;  GFZ, German Research Centre for Geosciences Telegrafenberg, Potsdam, D-14473, Germany, University of the Witwatersrand, 1 Jan Smuts Ave Braamfontein, Johannesburg, 2000, South Africa
Harris, H. H.;  Department of Chemistry, University of AdelaideSA, Australia
Language :
English
Title :
Abnormal concentrations of Cu-Co in: Haumaniastrum katangense, Haumaniastrum robertii and Aeolanthus biformifolius: Contamination or hyperaccumulation?
Publication date :
2019
Journal title :
Metallomics
ISSN :
1756-591X
eISSN :
1756-5901
Publisher :
Royal Society of Chemistry, United Kingdom
Volume :
11
Issue :
3
Pages :
586-596
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 22 December 2021

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