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Formation of black opal in the pegmatites from Volyn (Ukraine) – an example for interaction of silica with organic matter

Franz, Gerhard ; Khomenko, Vladimir; Chornousenko, Vsevolod; Zeh, Armin 1; Schiperski, Ferry; Gouzy, Simon; Gernert, Ulrich; Nissen, Jörg
1 Institut für Angewandte Geowissenschaften (AGW), Karlsruher Institut für Technologie (KIT)

Abstract:

Black opal, a variety of opal pigmented by organic matter, from Volyn, western Ukrainian Shield, was investigated by means of scanning electron microscopy (SEM), electron microprobe analyses (EMPAs), μ-X-ray fluorescence (μXRF) element mapping, X-ray diffraction (XRD), and Fourier transformed infrared (FTIR) spectroscopy, and was dated by U-Pb by laser ablation (LA-ICP-SF-MS). Opal occurs as several centimeter large blocks and as cement in a breccia within pegmatites, which intruded into granites of the ca. 1.7–1.8 Ga old Korosten pluton. Opal samples were collected underground in miarolitic cavities of the pegmatites, which also host kerite, fossilized organic material (called Volyn biota). Inclusions in opal are typical pegmatitic minerals such as alkali-feldspar, Li-mica, and quartz. Buddingtonite and ammonium-bearing muscovite, as well as shape relicts of the fossils in opal, indicate interactions of organic material with the pegmatite.

The XRD data indicate opal-CT with a complex pattern of the ∼ 4 Å peak. Its microstructure, as seen in SEM and back-scattered electron maps, consists of nanograins 15–35 nm in size, arranged in sphere-like structures, in some samples ∼ 5 µm-large and monodisperse, in others polydisperse with diameters of between 1 and 10 µm, and as lepispheres. ... mehr


Verlagsausgabe §
DOI: 10.5445/IR/1000193719
Veröffentlicht am 01.06.2026
Cover der Publikation
Zugehörige Institution(en) am KIT Institut für Angewandte Geowissenschaften (AGW)
Publikationstyp Zeitschriftenaufsatz
Publikationsjahr 2026
Sprache Englisch
Identifikator ISSN: 0935-1221, 1617-4011
KITopen-ID: 1000193719
Erschienen in European Journal of Mineralogy
Verlag Copernicus Publications
Band 38
Heft 3
Seiten 305–324
Vorab online veröffentlicht am 22.05.2026
Nachgewiesen in Scopus
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