Ni3Fe Phase Research Articles

X-ray characterization of nanocrystalline Ni3Fe

X-ray microstructure characterization of nanocrystalline Ni3Fe was made employing Rietveld’s powder structure refinement method, the Warren–Averbach’s method and modified Williamson–Hall method. Ni3Fe particles were synthesized within a silica matrix by a sol–gel method. Particle size (10–15) nm and r.m.s. strain (∼10−3) values of Ni3Fe were found to be anisotropic in nature. Stacking faults, change in lattice parameter, dislocation density (edge type) values indicate the amount of disordering in the Ni3Fe phase. Lattice distortion in terms of several microstructural parameters also corroborates the results obtained from Mössbauer spectra analysis. Other associated co-developed phases like, crystalline SiO2, Fe2SiO4 (trace amount) have been identified and NiO has been characterized by X-ray powder diffraction. A significant correlation between these two different types of characterization has been shown to be present.

Low-temperature phase decomposition in metal from iron, stony-iron, and stony meteorites

The microstructure of the outer taenite rim and cloudy zone of meteoritic metal was investigated using high resolution scanning electron microscopy and analytical electron microscopy. The micro-structure is formed by a series of complex phase transformations at <-400°C. These transformations are interpreted using the Fe-Ni phase diagram. The outermost subzone (zone 1) of the outer taenite rim is composed of two single-phase layers, Ni 3Fe and FeNi (tetrataenite). The Ni 3Fe phase appears at the border between kamacite and the outer taenite rim. The inner two subzones (zones 2 and 3) in the outer taenite rim are two-phase with a matrix of tetrataenite and low Ni bcc precipitates. The three zone structure is a general feature in the outer taenite rim of metal particles in all major types of meteorites. The cloudy zone is composed of an island region and a bcc single phase honeycomb region containing ∼9.0 wt% Ni. The island region is a two-phase mixture of a L1 0 ordered fee tetrataenite matrix and low-Ni bee precipitates. The high-Ni taenite region, γ 2, resulting from the monotectoid reaction, γ 1 → α + γ 2 at 400°C remains as a supersaturated solid solution to lower temperatures and corresponds metallographically to the outer taenite rim. The width of the outer taenite rim varies inversely with the cooling rate of the meteorite. The γ′, Ni 3Fe, phase is formed when the high-Ni γ 2 phase containing ∼53 wt% Ni undergoes an eutectoid reaction, γ 2 → α + γ′ at about 345°C. The cloudy zone develops by spinodal decomposition below 350°C. Metastable γ 2 island region of high Ni content and metastable γ 1 honeycomb region of low Ni content are formed. The size of the constituents of the cloudy zone increases with increasing Ni content because the higher Ni regions enter the spinodal region at higher temperatures. The precipitates in the island region of the cloudy zone and in zones 2 and 3 of the outer taenite rim have essentially the same Ni content (14.2–14.7 wt%) and form at lower temperatures when the Ni content of γ 2 is located in the γ 1 + γ 2 miscibility gap but outside the spinodal. If cooling rates or metamorphic reheating is to be studied at or below 400°C, the low temperature phase transformations must be considered. Improvement in simulation models will be difficult to make, however, because the diffusion rates in ordered FeNi, tetrataenite, and ordered Ni 3Fe are not known.