The crust structure of the Morasko meteorite – a preliminary hypothesis

dc.contributor.authorStankowski, Wojciech T.J.
dc.date.accessioned2017-06-19T12:53:35Z
dc.date.available2017-06-19T12:53:35Z
dc.date.issued2017-05
dc.description.abstractA 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.pl_PL
dc.identifier.citationGeologos, 2017, 23, 1, 53-56pl_PL
dc.identifier.doihttps://doi.org/10.1515/logos-2017-0005
dc.identifier.isbn978-83-232187-4-6
dc.identifier.issn1426-8981
dc.identifier.urihttp://hdl.handle.net/10593/17936
dc.language.isoengpl_PL
dc.publisherInstytut Geologii UAMpl_PL
dc.rightsinfo:eu-repo/semantics/openAccesspl_PL
dc.subjectsintered crustpl_PL
dc.subjectfusion crustpl_PL
dc.subjectgenesispl_PL
dc.subjectSEMpl_PL
dc.subjectEDSpl_PL
dc.titleThe crust structure of the Morasko meteorite – a preliminary hypothesispl_PL
dc.typeArtykułpl_PL

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Uniwersytet im. Adama Mickiewicza w Poznaniu
Biblioteka Uniwersytetu im. Adama Mickiewicza w Poznaniu
Ministerstwo Nauki i Szkolnictwa Wyższego