57Fe Mössbauer Analysis of Meteorites and Tektites

Abstract

This review presents studies on iron meteorites (Campo del Cielo fall and an unregistered iron meteorite), an unregistered stony meteorite from Northwest Africa, and 13 tektites from the American, European, and Australasian strewn fields. The main experimental technique used in the studies was Mössbauer spectroscopy, both in transmission and backscattering geometries. For the latter, a MIMOS II spectrometer was used. Additionally, optical and scanning electron microscopies and X-ray diffraction were used. In the studied iron meteorites, kamacite is found as the main mineral. Campo del Cielo meteorite exhibits Widmanstätten patterns and schreibersite inclusions. The unregistered iron meteorite has Neumann lines and schreibersite inclusions. We have assigned Campo del Cielo as an octahedrite and the unregistered iron meteorite as a hexahedrite. The unregistered stony meteorite is composed mainly of iron-free silicates; at 4.2 K, the spectrum indicates maghemite and 1% troilite. The Cambodian tektite appeared individualized from other australasites, unlike the moldavite, which tends to cluster with them. Our analyses do not allow dismissing doubts on the provenance of tibetanites. The Fe3+/Fe2+ ratio was found to be higher for Muong Nong-type tektites than for splash-form tektites, as expected from their morphology and solidification from melt at lower temperature.

Magnetite in Muong Nong‐Type Australasian Tektites From South China

“…AASF tektites generally have rather weak natural remanent magnetization (NRM) (10 −8 –10 −6 Am 2 /kg) (e.g., Gattacceca et al., 2022; Pan et al., 2023a). The paramagnetic signals caused by dispersed Fe 2+ ions dominate tektites' magnetic properties, which are interpreted to be caused by rapid cooling in a reducing environment (Costa et al., 2021; Pan et al., 2023a; Rochette et al., 2015). The three main morphological types of tektites in AASF, splash‐form, Muong Nong‐type, and ablated splash‐form (Barnes, 1963; Chapman, 1971; Nininger & Huss, 1967) exhibit diverse magnetic properties, which can be attributed to differences in their precursor materials and/or thermal histories (Donofrio, 1977; Pan et al., 2023a; Senftle & Thorpe, 1959; Werner & Borradaile, 1998).…”