Although much of this iron has been significantly oxidized by terrestrial weathering, some metallic portions are preserved. The presence in Santa Catharina of the phosphide barringerite, a mineral usually unstable in association with metal, attests to a high cooling rate. However, a low cooling rate is considered necessary for the formation of some unique FeNi-metal phases. Those FeNi-metal mineral phases present in Santa Catharina include an ordered Fe-deficient tetrataenite (44.6 wt%) associated with a disordered paramagnetic, Fe-rich antitaenite (48.9 wt%), and a disordered Fe-deficient, face-centered cubic phase (6.5 wt%); these phases were identified by synchrotron X-ray diffraction techniques (Scorzelli et al., 2007). Based on noble gas data, Santa Catharina has a CRE-age of 140 m.y.
Santa Catharina shares many taxonomic characteristics with Twin City, which prompted Wasson and Kallemeyn (2002) to classify them as a unique duo within the IAB iron complex. Twin City contains slightly less Ni (30%) and troilite than Santa Catharina, and instead of an ataxitic structure, it exhibits a rudimentary orientation of kamacite spindles into a Thomson (Widmanstätten) structure. Although to a much lower degree than Santa Catharina, Twin City has suffered significant deterioration from thousands of years of terrestrial weathering. The specimen of Santa Catharina pictured above is a 6.84 g oxidized fragment, while a grouping of unoxidized fragments are pictured below. A close-up view of a large unoxidized specimen exhibited at the Muséum National d'Histoire de Paris can be seen at their website.