Abstract
A grain of fayalitic olivine with oscillatory Fe-rich and Fe-poor zoning occurs in the Antarctic Lewis Cliff 90500 CM meteorite, suggesting reaction via diffusion. This grain is continuously enclosed by a fine-grained rim ranging from 20 to 100 μm in thickness. Phyllosilicates and other hydrous phases occur at three broken edges of the grain as well as within its surrounding rim, suggesting in situ alteration via aqueous processes. This olivine grain plus its rim provides evidence for both anhydrous reaction that predated the accretion of the meteorite parent body and hydrous alteration that presumably occurred on the parent body.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 2201-2211 |
| Number of pages | 11 |
| Journal | Geochimica et Cosmochimica Acta |
| Volume | 67 |
| Issue number | 12 |
| DOIs | |
| State | Published - Jun 15 2003 |
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ASJC Scopus subject areas
- Geochemistry and Petrology
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Oscillatory zoned fayalitic olivine from the Lewis Cliff 90500 CM2 meteorite. / Hua, Xin; Li, Jia; Buseck, P R.
In: Geochimica et Cosmochimica Acta, Vol. 67, No. 12, 15.06.2003, p. 2201-2211.Research output: Contribution to journal › Article
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TY - JOUR
T1 - Oscillatory zoned fayalitic olivine from the Lewis Cliff 90500 CM2 meteorite
AU - Hua, Xin
AU - Li, Jia
AU - Buseck, P R
PY - 2003/6/15
Y1 - 2003/6/15
N2 - A grain of fayalitic olivine with oscillatory Fe-rich and Fe-poor zoning occurs in the Antarctic Lewis Cliff 90500 CM meteorite, suggesting reaction via diffusion. This grain is continuously enclosed by a fine-grained rim ranging from 20 to 100 μm in thickness. Phyllosilicates and other hydrous phases occur at three broken edges of the grain as well as within its surrounding rim, suggesting in situ alteration via aqueous processes. This olivine grain plus its rim provides evidence for both anhydrous reaction that predated the accretion of the meteorite parent body and hydrous alteration that presumably occurred on the parent body.
AB - A grain of fayalitic olivine with oscillatory Fe-rich and Fe-poor zoning occurs in the Antarctic Lewis Cliff 90500 CM meteorite, suggesting reaction via diffusion. This grain is continuously enclosed by a fine-grained rim ranging from 20 to 100 μm in thickness. Phyllosilicates and other hydrous phases occur at three broken edges of the grain as well as within its surrounding rim, suggesting in situ alteration via aqueous processes. This olivine grain plus its rim provides evidence for both anhydrous reaction that predated the accretion of the meteorite parent body and hydrous alteration that presumably occurred on the parent body.
UR - http://www.scopus.com/inward/record.url?scp=0038346233&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=0038346233&partnerID=8YFLogxK
U2 - 10.1016/S0016-7037(02)01374-1
DO - 10.1016/S0016-7037(02)01374-1
M3 - Article
AN - SCOPUS:0038346233
VL - 67
SP - 2201
EP - 2211
JO - Geochmica et Cosmochimica Acta
JF - Geochmica et Cosmochimica Acta
SN - 0016-7037
IS - 12
ER -