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Naji, M. |
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Motta, Antonella |
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Aletan, Dirar |
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Mohamed, Tarek |
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Ertürk, Emre |
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Taccardi, Nicola |
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Kononenko, Denys |
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Petrov, R. H. | Madrid |
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Alshaaer, Mazen | Brussels |
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Bih, L. |
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Casati, R. |
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Muller, Hermance |
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Kočí, Jan | Prague |
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Šuljagić, Marija |
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Kalteremidou, Kalliopi-Artemi | Brussels |
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Azam, Siraj |
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Ospanova, Alyiya |
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Blanpain, Bart |
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Ali, M. A. |
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Popa, V. |
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Rančić, M. |
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Ollier, Nadège |
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Azevedo, Nuno Monteiro |
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Landes, Michael |
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Rignanese, Gian-Marco |
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Claeys, Philippe
Vrije Universiteit Brussel
in Cooperation with on an Cooperation-Score of 37%
Topics
Publications (6/6 displayed)
- 2022Artificial weathering of an ordinary chondritecitations
- 2019Two generations of exsolution lamellae in pyroxene from Asuka 09545: Clues to the thermal evolution of silicates in mesosideritecitations
- 2019The tale of pyroxene in mesosiderite ASUKA 09545, inferred from two generations of exsolution lamellae
- 2019Evaluating the impact of acetic acid chemical pre-treatment on ‘old’ and cremated bone with the ‘Perio-spot’ technique and ‘Perios-endos’ profilescitations
- 2016Orbital component extraction by time-variant sinusoidal modeling
- 2014TEM investigation of shock-induced polymorphic transformation of olivine
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document
The tale of pyroxene in mesosiderite ASUKA 09545, inferred from two generations of exsolution lamellae
Abstract
Mesosiderites consist of a breccia containing roughly equal amount of metal and silicate interpreted as a mixture of basaltic material from the crust and metal from the core of two differentiated parent bodies or even from mixing<br/>within the same parent body. The metal portion metal has recorded the slowest cooling rate from ca. 550°C ever measured in the Solar System. The formation processes of mesosiderites are still debated. In particular, the cooling history of the silicate fraction in mesosiderite is not completely unraveled, so far, although most of the estimates agree that silicate cooling rate was fast until ca. 800°C