Features attributed to ferric iron in remotely sensed spectral data of Mars and the magnetic nature of Martian soil at the Viking landing sites are consistent with the occurrence of hematite (αâFe2O3) as both superparamagnetic (nanocrystalline) hematite (spâHm) and largerâdiameter hematite (bulkâHm) particles. These hematite particles most likely occur in pigmentary form, that is, as particles dispersed throughout the volume of a relatively spectrally neutral (silicate?) material. Likely physical forms of this pigmented volume include rocks, dust and soil particles, and coatings (weathering rinds) thereon. Accommodation of Martian data by hematite is a result of differences in optical and magnetic properties of spâHm and bulkâHm particles. Optical, magnetic, and Mossbauer properties of spâHm particles dispersed within particles of highâarea silica gel are reported in this study and compared to the corresponding properties of bulkâHm powders. Samples were prepared by calcining (âŒ550°C) powders of highâarea silica gel that had been impregnated with ferric nitrate solutions. The samples are classified according to type of Mossbauer spectrum observed at 293 K. (1) Type S + D samples, which by Mossbauer granulometry contain hematite particles both larger and smaller than 10(2) nm, are characterized by a hematite sextet plus superparamagnetic doublet. (Uncertainties are given in parentheses and refer to the final digit(s).) (2) Type D samples, which contain hematite particles smaller than 10(2) nm, are characterized by only a superparamagnetic doublet and so contain only spâHm. The presence of larger particles in type S + D samples is consistent with X ray diffraction data; the diffraction patterns of type S + D samples are characterized by a few, broad hematite lines, and type D samples have no lines because the particles are too small to coherently scatter X rays. Measurements of internal field strengths (Hint) at 22 K for both type S + D and type D samples show that Hint is not constant but decreases with decreasing particle diameter from 54.0 T for bulkâHm to 46.6 T for 5.4ânm spâHm. This dependence implies that phase identifications based solely on comparisons to bulk values of Hint are equivocal when superparamagnetic particles are present. SpâHm (<10ânm diameter) is much more magnetic than bulkâHm; the saturation magnetization at 293 K for type D samples is 7(2) A m2/kg as compared to 0â0.5 A m2/kg for bulkâHm. Optical properties of type S + D samples are similar to those of bulkâHm; in particular, a wellâdefined band minimum is present near 860 nm. Optical properties of type D samples, with only spâHm at 293 K, are significantly different in that a stepâshaped feature instead of a wellâdefined band is centered near 860 nm. The transition from wellâdefined band to stepâshaped feature occurs at a hematite particle diameter of âŒ10 nm. The position of the UVâvisible absorption edge and the absorption strength at 860 nm depend on the number density of spâHm particles, the Fe2O3 concentration, and the physiochemical properties of the support material. For 7(2)ânm spâHm particles dispersed within silica gel particles (35â to 74âÎŒm powder with 6ânm pore diameter) the absorption edge shifts toward the visible, and the absorption strength at 860 nm increases with increasing number density of the spâHm particles. Visually, the color change is from nearly white to tan to dark red. Optical properties of samples containing 7(2)ânm spâHm particles are essentially independent of temperature between 173 and 293 K.
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