Pyroxferroite: Stability and X-ray Crystallography of Synthetic Ca0.15Fe0.85SiO3 Pyroxenoid
@article{Lindsley1970PyroxferroiteSA, title={Pyroxferroite: Stability and X-ray Crystallography of Synthetic Ca0.15Fe0.85SiO3 Pyroxenoid}, author={Donald H. Lindsley and Charles W. Burnham}, journal={Science}, year={1970}, volume={168}, pages={364 - 367} }
Synthetic Ca0.15Fe0.85SiO3 pyroxenoid has the same (pyroxmangite) structure and very nearly the same composition as pyroxferroite, a new mineral found in Apollo 11 lunar samples. The synthetic material is not stable below pressures of approximately 10 kilobars. It appears likely that the lunar pyroxferroite has persisted in a metastable state for some billions of years.
52 Citations
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References
SHOWING 1-10 OF 20 REFERENCES
Ferrosilite III: A Triclinic Pyroxenoid-Type Polymorph of Ferrous Metasilicate
- GeologyScience
- 1966
The relationships between the triclinic unit cell of ferrosilite III and those of pyroxmangite, rhodonite, and wollastonite lead to the hypothesis that this polymorph of ferrous metasilicate has a…
Mineralogy and Deformation in Some Lunar Samples
- GeologyScience
- 1970
Overall homogeneity, igneous textures, and absence of xenoliths in the crystalline rocks indicate derivation from a common titanium-rich magma by internal, anorogenic volcanism rather than by impact.
Mineralogy and Composition of Lunar Fines and Selected Rocks
- GeologyScience
- 1970
Detailed descriptions are given of small craters produced by hypervelocity particle impact on glass and iron-nickel fragments in the fines and of surface rocks is attributed to mechanical ahrasion and not to cratering.
Electron-Microprobe Analyses of Phases in Lunar Samples
- GeologyScience
- 1970
Gross similarities between euctites and Apollo 11 volcanic rocks indiacate similar evolutionary environments, but detailed mineralogical differences suggest either separate origins or if eucrites are lunar, chemical inhomogeneities on the lunar surface.
Mineralogy and Petrography of Lunar Samples
- GeologyScience
- 1970
The lunar samples consist largely of augite, calcic plagioclase, and ilmenite, which resemble the calcium-rich achondritic meteorites (eucrites and howardites) in composition and structure.
Diffraction and M�ssbauer Studies of Minerals from Lunar Soils and Rocks
- GeologyScience
- 1970
In addition to identification of minerals, including rare amphibole, mica, and aragonite, a detailed study of the important rock-forming minerals of the plagioclase, pyroxene, and olivine groups has begun.
Petrologic History of Moon Suggested by Petrography, Mineralogy, and Crystallography
- GeologyScience
- 1970
Crystal-liquid differentiation of out-gassed convecting moon with growing Fe-rich core, olivine-pyroxene mantle, plagioclase-rich dynamic crust underlain by nonspherical, inversely stratified ferrobasalt is suggested.
Mineralogy and Petrology of Some Lunar Samples
- GeologyScience
- 1970
Chemical analyses and norms of four samples are presented which confirm original estimates of low silica, unusual abundance of titania, and low oxidation state of the rocks. Accounts are given of…
Petrology of Unshocked Crystalline Rocks and Shock Effects in Lunar Rocks and Minerals
- GeologyScience
- 1970
On the basis of rock modes, textures, and mineralogy, unshocked crystalline rocks are classified into a dominant ilmenite-rich suite (subdivided into intersertal, ophitic, and hornfels types) and a…
Age of the Moon: An Isotopic Study of Uranium-Thorium-Lead Systematics of Lunar Samples
- GeologyScience
- 1970
The fine dust and the breccia have a concordant age of 4.66 billion years on the basis of 207Pb/206Pb, 206PB/238U, 207P b/235U, and208Pb-232Th ratios, and six crystalline and vesicular samples are distinctly younger than the dust and Breccia.