AIP Conference Proceedings 2009
DOI: 10.1063/1.3222879
|View full text |Cite
|
Sign up to set email alerts
|

Cathodoluminescence Characterization of Maskelynite and Alkali Feldspar in Shergottite (Dhofar 019)

Abstract: Dhofar 019 is classified as an olivine-bearing basaltic shergottite and consists of subhedral grains of pyroxene, olivine, feldspar mostly converted to maskelynite and minor alkali feldspar. The CL spectrum of its maskelynite exhibits an emission band at around 380 nm Similar UV-blue emission has been observed in the plagioclase experimentally shocked at 30 and 40 GPa, but not in terrestrial plagioclase. This UV-blue emission is a notable characteristic of maskelynite. CL spectrum of alkali feldspar in Dhofar … Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

1
3
0

Year Published

2017
2017
2024
2024

Publication Types

Select...
2

Relationship

0
2

Authors

Journals

citations
Cited by 2 publications
(4 citation statements)
references
References 5 publications
1
3
0
Order By: Relevance
“…Similar emission bands have been reported in the CL spectra of experimentally shocked sanidine, microcline, and albite above 30 GPa (partly at 20 GPa) and those of maskelynite in Martian meteorites (Kayama et al 2012). Such a spectral pattern is characteristic of maskelynite and diaplectic feldspar glass, and undetectable in crystalline plagioclase (Kayama et al 2009a(Kayama et al , 2009b(Kayama et al , 2012. On the other hand, the CL spectroscopy of the dark portion exhibits only a blue emission band at~410 nm ( Fig.…”
Section: High-pressure Polymorphs Of Plagioclasesupporting
confidence: 78%
See 2 more Smart Citations
“…Similar emission bands have been reported in the CL spectra of experimentally shocked sanidine, microcline, and albite above 30 GPa (partly at 20 GPa) and those of maskelynite in Martian meteorites (Kayama et al 2012). Such a spectral pattern is characteristic of maskelynite and diaplectic feldspar glass, and undetectable in crystalline plagioclase (Kayama et al 2009a(Kayama et al , 2009b(Kayama et al , 2012. On the other hand, the CL spectroscopy of the dark portion exhibits only a blue emission band at~410 nm ( Fig.…”
Section: High-pressure Polymorphs Of Plagioclasesupporting
confidence: 78%
“…Crystalline plagioclase in rocks also shows the blue emission bands (Kayama et al. , , ). Therefore, the bright and dark portions observed in the panchromatic CL images correspond to maskelynite and residual plagioclase, respectively.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…On the other hand, there are claims that maskelynite can be formed via quenching from a shock melt as a fused plagioclase glass under high pressure (Chen and El Goresy, 2000). Cathodoluminescence (CL) techniques have been used as pivotal tools, for example, geochemistry, petrology, mineralogy, and crystallography (e.g., Kayama et al, 2009a). CL microscopy enables the observation of various features such as the two-dimensional distribution of silica polymorphs and chemical zoning in plagioclase.…”
mentioning
confidence: 99%