The study, published in European Journal of Mineralogy, affirms that the mineral is chladniite, a complex phosphate belonging to the fillowite group, which contains sodium, calcium, magnesium and iron, and has a trigonal structure. It has been found in a pegmatite, an igneous (magmatic) rock, formed from the slow cooling and solidification of magma.
Chladniite was first encountered in 1993, in the iron meteorite Carlton IIICD. So far, it had only been observed in this type of meteorites, characterized by having undergone fusion and differentiation processes such as igneous rocks. The name of the mineral is in honor of the German physicist and musician Ernst Florens Friedrich Chladni (1756-1827), pioneer in the study of meteorites, who defended its extraterrestrial origin.
The crystalline structure of the mineral has been determined by fixing a very thin section of the rock onto a glass substrate, and by passing synchrotron light through the set, with the technique called through-the-substrate X-ray-microdiffraction. This technique, driven by researchers from ICMAB, began in collaboration with the Spanish-Catalan line of the European Synchrotron Radiation Facility (ESRF) in Grenoble (France) and has subsequently been developed and refined together with researchers from the MSPD line of the ALBA Synchrotron.
Two of the innovative features of this characterization technique are both the use of a very fine glass substrate, which allows the easy location of the area to be irradiated, and the use of focalized synchrotron light, which allows enlightening a very small area of the rock and, therefore, the diffraction of individual crystals.
First terrestrial occurrence of the complex phosphate chladniite: crystal-structure refinement by synchrotron through-the-substrate microdiffraction
Vallcorba, Oriol; Casas, Lluís; Colombo, Fernando; Frontera, Carlos; Rius, Jordi
European Journal of Mineralogy Volume 29 Number 2 (2017), p. 287 - 293
MSPD beamline at ALBA Synchrotron
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