Celestine Mineralisation in Jabal Hafit, Al-Ain (United Arab Emirates): Constraints from Geochemical and Sr-S Isotope Systematics

Sami, Mabrouk, Amin, Bahaa M., Sanislav, Ioan V., Al-Ahbabi, Ahad, Alali, Maryam, Malek, Meera, Aldhaheri, Mariam, Almenhali, Aya, Alhejji, Suhail S., Li, Chun-Feng, Abukhadra, Mostafa R., and Fathy, Douaa (2026) Celestine Mineralisation in Jabal Hafit, Al-Ain (United Arab Emirates): Constraints from Geochemical and Sr-S Isotope Systematics. Minerals, 16 (6). 575.

[img]
Preview
PDF (Published Version) - Published Version
Available under License Creative Commons Attribution.

Download (25MB) | Preview
View at Publisher Website: https://doi.org/10.3390/min16060575


Abstract

Celestine (SrSO4) is the principal ore of Sr and a sensitive tracer of diagenetic fluid–rock interaction in carbonate–evaporite successions. This study presents integrated petrographic mineral chemistry and Sr–S isotopic data for epigenetic celestine hosted by Asmari carbonates at Jabal Hafit, Al Ain (UAE), to constrain fluid source, and mechanisms of SrSO4 precipitation during basin diagenesis. Field and SEM observations show celestine as stratabound, vug- and fracture-filling euhedral to subhedral crystals within dolomitised limestone, suggesting precipitation after initial lithification during early-to-mid burial diagenesis. Electron microprobe analyses show nearly stoichiometric SrSO4 (55.15–57.30 wt.% SrO; 42.43–44.35 wt.% SO3) with very low Ba and Ca. The characteristically high Sr/Ba signature of the celestine reflects a complex diagenetic history driven by efficient Sr remobilisation during carbonate recrystallisation within an inherently Ba-poor marine sequence. Measured 87Sr/86Sr ratios are tightly clustered (0.707841–0.707854) with a high degree of isotopic homogeneity, which indicates a stable, well-buffered fluid reservoir, while the absolute values align with an Oligocene marine signature. Sulphur isotope values (δ34S = +27.3 to +29.1‰) are enriched relative to coeval marine sulphate, which could be attributed to closed-system Rayleigh fractionation driven by bacterial sulphate reduction. We propose that celestine precipitated from stable, marine-buffered burial brines, where supersaturation was achieved through coupled Sr enrichment from carbonate diagenesis and microbial modification of the sulphate reservoir.

Item ID: 92085
Item Type: Article (Research - C1)
ISSN: 2075-163X
Copyright Information: © 2026 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license.
Date Deposited: 11 Jun 2026 02:43
FoR Codes: 37 EARTH SCIENCES > 3703 Geochemistry > 370302 Inorganic geochemistry @ 40%
37 EARTH SCIENCES > 3703 Geochemistry > 370303 Isotope geochemistry @ 40%
37 EARTH SCIENCES > 3705 Geology > 370508 Resource geoscience @ 20%
SEO Codes: 28 EXPANDING KNOWLEDGE > 2801 Expanding knowledge > 280107 Expanding knowledge in the earth sciences @ 100%
More Statistics

Actions (Repository Staff Only)

Item Control Page Item Control Page