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Grokhovskyite, CuCrS₂, was observed in small sulfide inclusions (up to 50–80 µm) in Ni-rich iron (kamacite) of the Uakit iron meteorite (IIAB) in the Republic of Buryatia, Russia. The grain sizes of this mineral are usually less than 5 μm, and the biggest detected crystals are 10 × 5 μm in size. It is commonly associated with daubréelite, troilite, schreibersite, and, sometimes, with carlsbergite and uakitite. Within inclusions, the mineral forms elongated splintered crystals, or, rarely, needle-shaped grains in daubréelite. The grokhovskyite-containing associations in the Uakit meteorite seem to form due to high-temperature (>1000 °C) separation of Fe-Cr sulfide liquid, which is locally enriched in Cu, from Fe-Ni metal melt. Physical and optical properties of grokhovskyite are quite similar to those of synthetic CuCrS₂: yellow–brown and non-transparent phase with metallic luster; Mohs hardness ≈ 4; gray to light gray color with yellow tint in reflected light; weak to medium bireflectance, anisotropy, and pleochroism; density (calc.) = 4.559 g/cm³. Grokhovskyite is structurally related to the Cr-containing disulfide minerals with general formula Me⁺CrS₂ (where Me⁺ = Na, Cu, Ag), including caswellsilverite, NaCrS₂; schöllhornite, Na_0.3CrS₂·H₂O; and cronusite, Ca_0.2CrS₂·2H₂O. Structural data were obtained for one grokhovskyite crystal using the EBSD technique. Fitting of the EBSD patterns for a synthetic α-CuCrS₂ model (trigonal R3m; a = 3.4794(8) Å; c = 18.702(4) Å; V = 196.08(10) ų; Z = 3) resulted in the parameter MAD = 0.57–1.16° (good fit). Analytical data for grokhovskyite (n = 36, in wt.%) are as follows: Cu—32.97; Cr—27.65; Fe—3.69; Ni—0.16; S—35.71; Na, Zn, V, Mn, and Co—below detection limit (<0.005 wt.%). The empirical formula is (Cu_0.930Cr_0.952Fe_0.118Ni_0.005)_2.005S_1.995; however, different concentrations of Fe are indicated in two individual grains of grokhovskyite (0.09–0.17 apfu). Such variations may be explained by Fe incorporation in the grokhovskyite structure according to the scheme ^IVCu⁺ + ^VICr³⁺ → ^IVFe²⁺ + ^VIFe²⁺. The three main bands (near 110, 250, and 310 cm⁻¹), which are common of synthetic CuCrS₂, were observed in the Raman spectra of grokhovskyite. Full article

For the first time, chromium disulphides, known from meteorites, such as caswellsilverite, NaCrS₂; grokhovskyite, CuCrS₂; and a potentially new mineral, AgCrS₂, as well as the products of their alteration, such as schöllhornite, Na_0.3CrS₂∙H₂O, and a potentially new mineral with the formula {Fe_0.3(Ba,Ca)_0.2} CrS₂·0.5H₂O, have been found in terrestrial rock. Layered chromium disulphides were found in unusual phosphide-bearing breccia of the pyrometamorphic Hatrurim Complex in the Negev Desert, Israel. The chromium disulphides belong to the central fragment of porous gehlenite paralava cementing altered host rock clasts. The empirical formula of caswellsilverite is (Na_0.77Sr_0.03Ca_0.01)_Σ0.81(Cr³⁺_0.79Cr⁴⁺_0.18V³⁺_0.01 Fe³⁺_0.01)_Σ0.99S₂·0.1H₂O, and the end-member content of NaCrS₂ is 76%. It forms single crystals in altered pyrrhotite aggregates. Grokhovskyite has the empirical formula {Cu⁺_0.84Fe³⁺_0.10Ca_0.06 Na_0.01 Sr_0.01Ba_0.01}_Σ1.03(Cr³⁺_0.94 Fe³⁺_0.05 V³⁺_0.05)_Σ1.00S₂·0.35H₂O, and the CuCrS₂ end-member content is 75–80%. A potentially new Ag-bearing chromium disulphide is characterised by the composition (Ag_0.89Cu_0.07)_Σ0.96(Cr_0.98 Fe_0.03V_0.01Ni_0.01)_Σ1.04S₂. Caswellsilverite, grokhovskyite and AgCrS₂ form in gehlenite paralava at high temperatures (near 1000 °C) and low pressure under reducing conditions. The structure of the layered chromium disulphides, MCrS₂, is characterised by the presence of hexagonal octahedral layers (CrS₂)¹⁻, between which M-sites of the monovalent cations Ag, Cu and Na set. A low-temperature alteration of the layered chromium disulphides, when schöllhornite and {Fe_0.3(Ba,Ca)_0.2}CrS₂·0.5H₂O form, is reflected in the composition and structural modification of the layer with monovalent cations, whereas the octahedral layer (CrS₂)¹⁻ remains unchanged. Full article