TL;DR: In this paper, the Mossbauer spectra of s7Fe for a series of compositions between FeO.7SS4 and FeNizS4 were analyzed, showing that the doublet with small isomer shift and quadrupole splitting increased with increasing iron (0.23-0.53 mmjsec).
Abstract: The crystal chemistry and mineralogical properties of the thiospinels of the series polydymite (Ni3S4}-violarite (FeNizS4}-greigite (Fe3S4) have been studied using synthetic and natural samples and emphasizing the intermediate compositions ("violarites," (Fe, NihS4)' In the series Ni3ScFeNizS4, increasing iron correlates with increasing thermal stability, a nearly linear decrease in a and increase in reflectance (R% at 589 nm), although spectral reflectance curves show more complex behavior. Mossbauer spectra of s7Fe for a series of compositions between FeO.2SNiz.7SS4 and FeNizS4 consist essentially of a doublet with a small isomer shift and quadrupole splitting, the former increasing with increasing iron (0.23-0.53 mmjsec). This is interpreted as low-spin Fez + in the octahedral sites, although further examination of the spectra suggests a possible contribution from iron (-18%) in tetrahedral coordination. These data are in agreement with bonding models previously proposed for the thiospinels. Although electron microprobe analyses of natural samples indicate that solid solution extends completely from Ni3S4 to Fe3S4' bonding models suggest that compositions more iron-rich than FeNizS4 may be metastable. The formation of such possibly metastable compositions, the observation in this work of violarites which are 1-2 wt.% sulfur-poor relative to stoichiometric M3S4, and the confusion over the low-temperaure phase relations involving violarite are all attributed. to its formation by alteration of pre-existing minerals (notably pentlandite). Reaction mechanism and kinetics are therefore crucial in the formation of this mineral in nature.
TL;DR: In this paper, a single crystal X-ray diffraction study of a partially violaritized pentlandite grain has shown that violarite has the same crystallographic orientation as the host pentlandites and the alteration can be effected by removal of excess metal atoms from pentlanditic and redistribution of the remainder.
Abstract: Violarites of the general composition (Fe, Ni) 3 S 4 from a variety of natural Fe-Ni sulfide assemblages have been studied by electron microprobe analysis. The violarite solid solution extends from the Ni-rich end member polydymite to at least 17 at. percent Ni, compositions more Fe-rich than FeNi 2 S 4 being characteristic of pyrrhotite-bearing assemblages and compositions more Ni-rich than FeNi 2 S 4 of Ni-rich assemblages that do not contain pyrrhotite. Most of the violarites have compositions in the range of 56 to 57 at. percent S and thus are slightly S-deficient relative to the ideal M 3 S 4 composition.The predominant mode of formation of violarite is by alteration of pentlandite. Violarite also forms from millerite, but alteration of pyrrhotite to violarite has not been confirmed in the present study. A single crystal X-ray diffraction study of a partially violaritized pentlandite grain has shown that violarite has the same crystallographic orientation as the host pentlandite and the alteration can be effected by removal of excess metal atoms from pentlandite and redistribution of the remainder. It is suggested that violarite forms readily from pentlandite because of the ease with which the pentlandite structure can be converted to that of violarite.The stability field of violarite in the Fe-Ni-S system must enlarge to more Fe-rich compositions, toward the Fe-S join, as the temperature decreases. Likely phase relations at temperatures sufficiently low to include smythite and the extension of the violarite field to 17 at. percent Ni have been schematically presented.
TL;DR: The Black Swan disseminated ores as mentioned in this paper are dominated by millerite-pyrite-polydymite assemblages in both serpentinites and talc carbonates, with no evident relationship to the progression of carbonation.
Abstract: The Black Swan disseminated orebody occurs predominantly within the partially carbonated serpentinite core of a zoned serpentinite–talc-carbonate ultramafic cumulate body of komatiitic parentage. The Black Swan disseminated sulfides depart significantly from the characteristic pattern observed in otherwise similar deposits in Western Australia and Canada, which display magnetite-bearing pentlandite-rich sulfide aggregates (“blebs”) in serpentinites, and S-rich millerite-bearing assemblages in talc carbonates. The Black Swan disseminated ores in contrast are dominated by millerite-pyrite–(polydymite) assemblages in both serpentinites and talc carbonates, with no evident relationship to the progression of carbonation. Sulfides show three types of intergrowth with gangue minerals, which can occur separately or all together: intergrowth with magnetite, at least some of which appear to be primary magmatic in origin; fine intergrowth with interlocking lath-textured antigorite; and intergrowth with carbonate minerals. Carbonate commonly replaces the core of sulfide blebs while retaining the primary magmatic outline. Carbonate replacement of sulfide roughly parallels the overall progression of carbonation of the whole rock, but no systematic relationship of the other intergrowth types to carbonate content is observed in the serpentinites. Serpentine mineralogy, determined by microbeam Raman spectroscopy, comprises lizardite, which occurs in pseudomorphic mesh textures after olivine, and antigorite, formed by variable degrees of overprinting of original lizardite mesh textures, ranging to a completely overprinting interlocking texture with no relic igneous texture. This progression is interpreted as the result of mild thermal metamorphism of original lizardite serpentinite. This progression is completely independent of carbonate content and is also apparently independent of extent of sulfide-antigorite intergrowth, which is interpreted as being early, and related to volume expansion during initial sea-floor serpentinization. Talc is almost completely absent from serpentinites, while carbonate content varies widely. Whole-rock Ni and S data are very strongly correlated in millerite-poor, pentlandite-rich samples and poorly correlated in samples where millerite is the dominant Ni-bearing sulfide. On this basis we conclude that the pentlandite assemblages are slightly modified survivors of the original magmatic event, while the millerite-pyrite assemblages formed during the earliest stages of serpentinization. Overprinting of the early serpentinization event by talc carbonate had essentially no effect on sulfide mineralogy, other than inducing intergrowth with carbonate. A number of distinctive features, such as magnetite-rich bleb cores, the association of sulfides with segregation vesicles and chromite “shells,” the subspherical morphology of the blebs, and preferential replacement of bleb cores, are considered to be inherited from the magmatic phase and are attributed to an original high but variable oxygen and halogen content of the sulfide melt component. Exsolution of this component during solidification of the blebs in some cases produced sulfide-centered bubbles now preserved as segregation vesicles, while in other cases oxygen was retained within the bleb forming magnetite-sulfide intergrowths. Chromite shells formed as a result of exsolved oxygen interacting with komatiite magma. Volatile-rich blebs solidified in some cases with hollow or porous cores, which were subsequently exploited by carbonate replacement.
TL;DR: The application of a range of experimental techniques shows that "amorphous nickel sulfide" (the material precipitated from aqueous solutions of Ni(II) salts and S(II-) under ambient conditions) is actually a hydrated nanoparticulate material with an approximate formula NiS.
Abstract: The application of a range of experimental techniques shows that “amorphous nickel sulfide” (the material precipitated from aqueous solutions of NiII salts and SII− under ambient conditions) is actually a hydrated nanoparticulate material with an approximate formula NiS·1.5H2O. The particles comprise a crystalline, anhydrous core (diameter ca. 1−3 nm) with the millerite (NiS) structure, surrounded by a hydrated shell phase. The materials prepared under acidic conditions (pH = 3 and 5) transform with age to form polydymite (Ni3S4) and heazlewoodite (Ni3S2), while materials prepared at pH = 7 and 9 do not undergo this transformation. At pH = 12, the preparation procedure yields NiAs-type NiS as a metastable phase.
TL;DR: In this article, a uniform hollow carbon-coated polydymite (Ni3S4) microspheres were synthesized in a solution via an in situ carboncoating and Ostwald ripening-based route.
Abstract: Uniform hollow carbon-coated polydymite (Ni3S4) microspheres were synthesized in a solution via an in situ carbon-coating and Ostwald ripening-based route The thin carbon coating layer and the hollow core enhanced the electrochemical performance of Ni3S4 as a Li-ion battery anode At a current density of 01C (about 100 mA g−1), they exhibited an extremely high reversible capacity of about 1003 mA h g−1 These polydymite-based composites also displayed a long stable cycling performance and a high capacity retention, with a reversible capacity of 480 mA h g−1 at 1C rate and a capacity retention of about 83% after 500 cycles