SERPENTINITE-HOSTED NICKEL, IRON, AND COBALT SULFIDE, ARSENIDE, AND INTERMETALLIC MINERALS IN AN UNUSUAL TECTONIC SETTING, SOUTHWEST ARIZONA
The most common opaque mineral in CR serpentinite is abundant (~ 5 %) magnetite, intimately intergrown with mesh-textured serpentine derived from olivine. Magnetite encloses and is intergrown with far less abundant, but ubiquitous, small (~ 30–100 µm) grains of pentlandite to cobaltoan pentlandite and heazlewoodite (Ni₃S₂). A few rocks also contain sparse pyrrhotite. Five additional minerals are even less abundant, typically several tiny (~ 5–20 µm) grains per thin section: chalcopyrite, bismuthinite, awaruite (Ni₃Fe), and two of the six naturally occurring Ni arsenides: orcélite (Ni₄.₇₅As₂) and maucherite (Ni₁₁As₈). Despite the difficulty of analyzing small grains by EMPA, most of these minerals closely match ideal and published compositions.
Textural relations imply this generalized sequence: formation of pentlandite (s.l.) and heazlewoodite, then partial replacement of pentlandite by heazlewoodite, with magnetite formation throughout and continuing after. These mineral assemblages indicate a highly reduced pore fluid, typical of serpentinization. Traces of awaruite are probably remnants of an early, most reduced stage. The observed sequences of mineral inter- and overgrowths and replacements suggest progressively less reducing conditions as serpentinization proceeded; a trend reported from other serpentinites.
Heazlewoodite, awaruite, orcélite, and maucherite apparently are new minerals for Arizona. (On-line reports of awaruite in the Canyon Diablo meteorite are apocryphal.) As our study continues, we will not be surprised to find additional unusual minerals.