The crust structure of the Morasko meteorite – a preliminary hypothesis
A small piece of the Morasko meteorite, weighing 970 g, yields traces of its journey through the Earth’s atmosphere and of its impact into a mineral substrate, such as reflected in the meteorite’s crust. This is seen in the crust structure in the form of sintered as well as fusion and semi-fusion la...
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Format: | Article |
Language: | English |
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Sciendo
2017-03-01
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Series: | Geologos |
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Online Access: | https://doi.org/10.1515/logos-2017-0005 |
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author | Stankowski Wojciech T.J. |
author_facet | Stankowski Wojciech T.J. |
author_sort | Stankowski Wojciech T.J. |
collection | DOAJ |
description | A small piece of the Morasko meteorite, weighing 970 g, yields traces of its journey through the Earth’s atmosphere and of its impact into a mineral substrate, such as reflected in the meteorite’s crust. This is seen in the crust structure in the form of sintered as well as fusion and semi-fusion layers for which ablative niches are optimum sites. Subsequent weathering processes have resulted in significant mineralogical changes in the crusts. The meteorite crusts originated during polygenetic processes. |
first_indexed | 2024-12-18T01:10:46Z |
format | Article |
id | doaj.art-d2469a2e6e61427ab96391c0b133e8bd |
institution | Directory Open Access Journal |
issn | 2080-6574 |
language | English |
last_indexed | 2024-12-18T01:10:46Z |
publishDate | 2017-03-01 |
publisher | Sciendo |
record_format | Article |
series | Geologos |
spelling | doaj.art-d2469a2e6e61427ab96391c0b133e8bd2022-12-21T21:26:06ZengSciendoGeologos2080-65742017-03-01231535610.1515/logos-2017-0005logos-2017-0005The crust structure of the Morasko meteorite – a preliminary hypothesisStankowski Wojciech T.J.0Institute of Geology, Adam Mickiewicz University, Krygowskiego 12, 61-680Poznań, PolandA small piece of the Morasko meteorite, weighing 970 g, yields traces of its journey through the Earth’s atmosphere and of its impact into a mineral substrate, such as reflected in the meteorite’s crust. This is seen in the crust structure in the form of sintered as well as fusion and semi-fusion layers for which ablative niches are optimum sites. Subsequent weathering processes have resulted in significant mineralogical changes in the crusts. The meteorite crusts originated during polygenetic processes.https://doi.org/10.1515/logos-2017-0005sintered crustfusion crustgenesissemeds |
spellingShingle | Stankowski Wojciech T.J. The crust structure of the Morasko meteorite – a preliminary hypothesis Geologos sintered crust fusion crust genesis sem eds |
title | The crust structure of the Morasko meteorite – a preliminary hypothesis |
title_full | The crust structure of the Morasko meteorite – a preliminary hypothesis |
title_fullStr | The crust structure of the Morasko meteorite – a preliminary hypothesis |
title_full_unstemmed | The crust structure of the Morasko meteorite – a preliminary hypothesis |
title_short | The crust structure of the Morasko meteorite – a preliminary hypothesis |
title_sort | crust structure of the morasko meteorite a preliminary hypothesis |
topic | sintered crust fusion crust genesis sem eds |
url | https://doi.org/10.1515/logos-2017-0005 |
work_keys_str_mv | AT stankowskiwojciechtj thecruststructureofthemoraskometeoriteapreliminaryhypothesis AT stankowskiwojciechtj cruststructureofthemoraskometeoriteapreliminaryhypothesis |