Trace element fractionation through halite crystallisation: Geochemical mechanisms and environmental implications.

Ab-initio calculation De-icing salt Dead Sea Environmental pollution REE Zr-Hf decoupling

Journal

The Science of the total environment
ISSN: 1879-1026
Titre abrégé: Sci Total Environ
Pays: Netherlands
ID NLM: 0330500

Informations de publication

Date de publication:
25 Jun 2020
Historique:
received: 16 12 2019
revised: 12 03 2020
accepted: 12 03 2020
pubmed: 29 3 2020
medline: 29 3 2020
entrez: 29 3 2020
Statut: ppublish

Résumé

Halite is an important mineral for industry, agriculture and food production. It crystallises during water evaporation, and the progressive increase of dissolved metal ions in the brine occurs simultaneously. Thus, halite exploitation may deliver metal ions into the environment and the mechanism of this trace element accumulation has to be studied. In this work, we investigate the distribution of lanthanides and Y (hereafter called rare earth elements, REE), Zr and Hf between crystallising halite and brines in the Dead Sea as geochemical tools for recognising the mechanism of metal ion removal from brines and accumulation in halite. Halite forms cubic crystals where octahedral planes sometimes occur under particular thermal gradient conditions. Our findings indicate that crystal morphology influences the mechanism of metal ion removal from brines because octahedral surfaces are polar unlike those that are cubic. Accordingly, octahedra preferentially fractionate aqueous charged species such as [Hf(OH)

Identifiants

pubmed: 32217400
pii: S0048-9697(20)31439-X
doi: 10.1016/j.scitotenv.2020.137926
pii:
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

137926

Informations de copyright

Copyright © 2020 Elsevier B.V. All rights reserved.

Déclaration de conflit d'intérêts

Declaration of competing 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.

Auteurs

P Censi (P)

DiSTeM, University of Palermo, Via Archirafi 22, 90123 Palermo, Italy. Electronic address: paolo.censi@unipa.it.

I Sirota (I)

Geological Survey of Israel, 32 Yesha'yahu Leibowitz, Jerusalem 9371234, Israel; The Fredy and Nadine Herrmann Institute of Earth Sciences, Edmond J. Safra Campus, The Hebrew University of Jerusalem, Givat Ram, Jerusalem 91904, Israel.

P Zuddas (P)

Sorbonne Université, CNRS, METIS, F75005 Paris, France.

N Lensky (N)

Geological Survey of Israel, 32 Yesha'yahu Leibowitz, Jerusalem 9371234, Israel.

M Merli (M)

DiSTeM, University of Palermo, Via Archirafi 22, 90123 Palermo, Italy.

F Saiano (F)

SAF, University of Palermo, Viale delle Scienze Ed. 4, 90128 Palermo, Italy.

D Piazzese (D)

DiSTeM, University of Palermo, Via Archirafi 22, 90123 Palermo, Italy.

F Sposito (F)

SIDERCEM S.R.L., Via Libero Grassi 7, 93100 Caltanissetta, Italy.

M Venturelli (M)

SIDERCEM S.R.L., Via Libero Grassi 7, 93100 Caltanissetta, Italy.

Classifications MeSH