Hostname: page-component-848d4c4894-nmvwc Total loading time: 0 Render date: 2024-07-04T00:02:42.199Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermomagnetic Study of Chondrules

Published online by Cambridge University Press:  14 August 2015

B. Lang ,
M. Pekala ,
E. Krôl ,
A. Nowakowski ,
P. Martin ,
Yu. Stakheev  and
G. Baryshikova
B. Lang
Affiliation:
Department of Chemistry, Warsaw University, Warsaw
M. Pekala
Affiliation:
Department of Chemistry, Warsaw University, Warsaw
E. Krôl
Affiliation:
Institute of Geophysics, Polish Academy of Sciences, Warsaw
A. Nowakowski
Affiliation:
Institute of Geochemistry, Mineralogy and Petrology, Warsaw University, Warsaw
P. Martin
Affiliation:
Department of Physics, Essex University, Colchester
Yu. Stakheev
Affiliation:
Vernadskiy Institute of Geochemistry, Moscow
G. Baryshikova
Affiliation:
Vernadskiy Institute of Geochemistry, Moscow

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Thermomagnetic and saturation magnetization curves were obtained for separate chondrules and fine matrix grains from one H- (Allegan) and four L-type (Bjurböle, Elenovka, Saratov, Nikolskoe) chondrites. Mineralogical and petrological data were recovered from chondrule thin sections. The differences observed in the obtained curves seem to suggest episodes in the story of chondrules predating their incorporation into matrices.

Type
IV: The Interplanetary Dust Complex 2. Physical Properties
Information
Symposium - International Astronomical Union , Volume 90: Solid Particles in the Solar System , 1980 , pp. 371 - 374
Copyright
Copyright © Reidel 1980