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⇱ Rietmeijer, Frans J. M. (1996) Cellular precipitates of iron oxide in olivine in a stratospheric interplanetary dust particle. Mineralogical Magazine, 60 (403) 877-885 doi:10.1180/minmag.1996.060.403.03

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Rietmeijer, Frans J. M. (1996) Cellular precipitates of iron oxide in olivine in a stratospheric interplanetary dust particle. Mineralogical Magazine, 60 (403) 877-885 doi:10.1180/minmag.1996.060.403.03

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Reference TypeJournal (article/letter/editorial)
TitleCellular precipitates of iron oxide in olivine in a stratospheric interplanetary dust particle
JournalMineralogical MagazineISSN0026-461X
AuthorsRietmeijer, Frans J. M.Author
Year1996 (December)Volume60
Issue403
PublisherMineralogical Society
Download URLhttps://rruff.info/doclib/MinMag/Volume_60/60-403-877.pdf+
DOIdoi:10.1180/minmag.1996.060.403.03Search in ResearchGate
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Mindat Ref. ID117Long-form Identifiermindat:1:5:117:3
GUID0
Full ReferenceRietmeijer, Frans J. M. (1996) Cellular precipitates of iron oxide in olivine in a stratospheric interplanetary dust particle. Mineralogical Magazine, 60 (403) 877-885 doi:10.1180/minmag.1996.060.403.03
Plain TextRietmeijer, Frans J. M. (1996) Cellular precipitates of iron oxide in olivine in a stratospheric interplanetary dust particle. Mineralogical Magazine, 60 (403) 877-885 doi:10.1180/minmag.1996.060.403.03
In(1996, December) Mineralogical Magazine Vol. 60 (403) Mineralogical Society
Abstract/NotesAbstractThe petrology of a massive olivine-sulphide interplanetary dust particle shows melting of Fe,Ni-sulphide plus complete loss of sulphur and subsequent quenching to a mixture of iron-oxides and Fe,Ni-metal. Oxidation of the fayalite component in olivine produced maghemite discs and cellular intergrowths with olivine and rare andradite-rich garnet. Cellular reactions require no long-range solid-state diffusion and are kinetically favourable during pyrometamorphic oxidation. Local melting of the cellular intergrowths resulted in three dimensional symplectic textures. Dynamic pyrometamorphism of this asteroidal particle occurred at ∼1100°C during atmospheric entry flash (5–15 s) heating.

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