Iron meteorites are Fe-Ni alloys that are thought to represent samples of the cores of differentiated asteroids. A minority of the iron meteorites contain silicate inclusions, the so-called silicate-bearing or non-magmatic iron meteorites. The presence of chemically evolved silicate inclusions in a high-density Fe-Ni metal raises questions about their origin. The IIE group belongs to the non-magmatic iron meteorites and contains primitive as well as evolved silicate inclusions. The object of this thesis is to investigate the formation processes of the silicate-bearing iron meteorites by examination of the primitive IIE irons.
| Date of Award | 10 Dec 2015 |
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| Original language | English |
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| Awarding Institution | - Université libre de Bruxelles
- Vrije Universiteit Brussel
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| Supervisor | Steven Goderis (Co-promotor), Philippe Claeys (Promotor) & Vinciane Debaille (Promotor) |
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- Impact
- Asteroid
- Planetary evolution
The record of primitive IIE meteorites: Implications for the formation of silicate-bearing iron meteorites
Van Roosbroek, N. ((PhD) Student), Claeys, P. (Co-promotor), Debaille, V. (Promotor). 10 Dec 2015
Student thesis: Doctoral Thesis