Studies on Al Kidirate and Kapoeta meteorites
Hyperfine Interactions, 1994•Springer
Abstract Mössbauer spectroscopy (20–300 K), magnetic susceptibility measurements (77–
350 K), scanning electron microscopy and X-ray diffraction experiments have been
performed on two meteorite samples: one from an old fall (Kapoeta) and another from a very
recent fall (Al Kidirate). The two specimens differ in their mineralogy. Chondrules appear to
be absent in Kapoeta and it is probably a pyroxene-plagioclase achondrite with
ferrohypersthene as the most abundant mineral. On the other hand, the Al Kidirate meteorite …
350 K), scanning electron microscopy and X-ray diffraction experiments have been
performed on two meteorite samples: one from an old fall (Kapoeta) and another from a very
recent fall (Al Kidirate). The two specimens differ in their mineralogy. Chondrules appear to
be absent in Kapoeta and it is probably a pyroxene-plagioclase achondrite with
ferrohypersthene as the most abundant mineral. On the other hand, the Al Kidirate meteorite …
Abstract
Mössbauer spectroscopy (20–300 K), magnetic susceptibility measurements (77–350 K), scanning electron microscopy and X-ray diffraction experiments have been performed on two meteorite samples: one from an old fall (Kapoeta) and another from a very recent fall (Al Kidirate). The two specimens differ in their mineralogy. Chondrules appear to be absent in Kapoeta and it is probably a pyroxene-plagioclase achondrite with ferrohypersthene as the most abundant mineral. On the other hand, the Al Kidirate meteorite is an ordinary chondrite and the specimen consists of olivine, orthopyroxene, troilite and kamacite. The Mössbauer measurements confirm the above characterization, showing a paramagnetic doublet for the Kapoeta sample and at least two paramagnetic doublets and magnetic sextets for the Al Kidirate specimens. The former were assigned to Fe in pyroxene sites, while the latter was assigned to Fe in pyroxene, olivine, Fe-S and Fe-Ni alloys. The difference in the mineralogy of the two meteorites has also been reflected in the temperature-dependent magnetic susceptibility. The magnetization and the hyperfine interaction parameters will be discussed in relation to the mineralogy.
Springer
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