Abstract

Mössbauer spectra of nonweathered ordinary chondrites consist of four main mineral phases: olivines, pyroxenes, metallic phase and troilite. These minerals represent more than 95% of the whole mass of an ordinary chondrite. Distribution of these mineral phases in micro-scale is not homogeneous. Nevertheless, preparation of representative sample of ordinary chondrite for Mössbauer measurements is possible. To do that a part of 1 g nonweathered material, selected from inside of meteorite without any specific intention is needed. The Warsaw group has been working on investigation of meteorites for 25 years and has analysed about 150 Mössbauer spectra of various meteorites. Among them we found 15 spectra, which could be suspected of being non-representative. These spectra were obtained from Baszkówka, Amber, Bjurböle, Krasnoi-Ugol and Chelyabinsk meteorites. The analysis of how the samples of meteorites were selected for investigation, has shown that the non-representativeness of samples may be due to: intentional choice of sample, preparation of sample from a too small part of material or the use of non-credible source of meteoritic samples. For confirmation of these assumptions, we used a new method of classification of ordinary chondrites – the 4M method. It turned out that this method is a very useful tool for investigation of non-representative samples of equilibrated ordinary chondrites.

Highlights

  • Ordinary chondrites are a class of stony meteorites

  • For two samples of the Bjurböle meteorite the percentages of the spectral area of olivine, pyroxene, troilite, and mineral phase are shown

  • Based on the obtained results, we can assume that samples: Chelyabinsk No 1, Chelyabinsk No 2, Chelyabinsk No 3, Chelyabinsk No 4, Chelyabinsk No 5, Baszkówka B1, Baszkówka B2, Baszkówka B3, Baszkówka B4, Mbale W, Mbale K, KrasnoiUgol, Bjurböle (A) and Amber are not representatives for the whole meteorites

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Summary

Introduction

Ordinary chondrites are a class of stony meteorites. They are the most numerous group of meteorites falling on Earth. The Warsaw group has been using the Mӧssbauer spectroscopy to classify ordinary chondrites since 2014 [2,3,4,5,6,7,8]. A method called 4M was developed, based on a mathematical analysis of the percentages of Mössbauer spectral areas of four mineral phases present in ordinary chondrites [7]. This method uses the Mahalanobis distance and the levels of similarity to the individual types of ordinary chondrites. Present version of 4M method was elaborated for nonweathered ordinary chondrites ­(Fe3+ ≤ 7%)

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