The magnetic hysteresis characteristics of the meteorites Allende, Canyon Diablo, El Hammami, Ghubara, Gold Basin, Nantan and Sichote Alin

  • Minoru FUNAKI National Institute of Polar Research, Kaga 1-chome, Itabashi-ku, Tokyo 173-8515, Japan
  • Igor KAPIŠINSKÝ Astronomical Institute of the Slovak Academy of Sciences, Interplanetary Matter Division, Bratislava, Slovak Republic
  • Igor TÚNYI Geophysical Institute of the Slovak Academy of Sciences, Bratislava, Slovak Republic
  • Oto ORLICKÝ Geophysical Institute of the Slovak Academy of Sciences, Bratislava, Slovak Republic
Keywords: ordinary meteorites, ataxites – Ni-rich iron meteorites

Abstract

The magnetic hysteresis characteristics of the respective samples have allowed to class as the Carbonaceous Chondrite the Allende meteorite, as the ordinary chondrites the El Hammami, Ghubara and Gold Basin meteorites. But the meteorites Canyon Diablo, Nantan and Sichote Alin have been preferentially classed as the ataxites – Ni-rich iron meteorites, containing mainly taenite, instead of the originally classed as the iron meteorite-coarse octahedrite, IIICD type of iron meteorite and the iron-coarsest octahedrite IIB, respectively.

Author Biographies

Igor KAPIŠINSKÝ, Astronomical Institute of the Slovak Academy of Sciences, Interplanetary Matter Division, Bratislava, Slovak Republic

Dúbravská cesta 9
845 05 Bratislava

Igor TÚNYI, Geophysical Institute of the Slovak Academy of Sciences, Bratislava, Slovak Republic

Dúbravská cesta 9
842 28 Bratislava

Oto ORLICKÝ, Geophysical Institute of the Slovak Academy of Sciences, Bratislava, Slovak Republic

Dúbravská cesta 9
842 28 Bratislava

Published
2021-05-10
How to Cite
FUNAKI, M., KAPIŠINSKÝ, I., TÚNYI, I., & ORLICKÝ, O. (2021). The magnetic hysteresis characteristics of the meteorites Allende, Canyon Diablo, El Hammami, Ghubara, Gold Basin, Nantan and Sichote Alin. Contributions to Geophysics and Geodesy, 35(4), 401-408. Retrieved from https://journal.geo.sav.sk/cgg/article/view/389
Section
original research papers republished in OJS