Andreyivanovite

andreyivanovite

florenskyite

serpentine

gehlenite

Images

Formula: FeCrP
Phosphide of iron and chromium, florenskyite group
Crystal system: Orthorhombic
Colour: Creamy white
Environments

Metamorphic environments
Meteorites

Localities

At the Hatrurim Basin, Tamar Regional Council, Beersheba Subdistrict, Southern District, Israel, iron phosphides with significant variations of Cr (up to 18 wt%) and V (up to 8.6 wt%) contents were detected in gehlenite-bearing breccia. Investigations of the Fe2P phosphides showed that when the V+Cr content is higher than 0.26 apfu (atoms per formula unit), a transition from the hexagonal barringerite to orthorhombic allabogdanite takes place; allabogdanite is a high-pressure (greater than 8 GPa) paramorph of barringerite. Pseudowollastonite associated with Cr-V-bearing allabogdanite is an indicator of phosphide crystallisation at high temperature (greater than 1200°C) and low pressure. Thus, at the low pressure close to ambient, when more than 13at% (atomic percentage) Fe in Fe2P is substituted by Cr and V, the orthorhombic paramorph is stable. The orthorhombic phosphide with the highest Cr and V contents belongs to the andreyivanovite species. This is the first finding on Earth of that very rare mineral first described from the Kaidun meteorite AM 108.8.1506-1515)

The Kaidun meteorite, Hadhramaut Governorate, Yemen, the type locality of andreyivanovite, fell in 1980. It is a unique breccia containing an unprecedented variety of fragments of different chondritic as well as achondritic lithologies. Andreyivanovite was found as individual grains and linear arrays of grains with a maximum dimension of 8 µm within two masses of Fe-rich serpentine. In one sample, it is associated with Fe-Ni-Cr sulphides and florenskyite. Andreyivanovite is creamy white in reflected light, with a metallic lustre. It could have formed as a result of cooling and crystallisation of a melted precursor consisting mainly of Fe-Ni metal enriched in P, Ti, and Cr. Serpentine associated with andreyivanovite would then have formed during aqueous alteration on the parent asteroid (AM 93.8.1295-1299).

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