Bytownite

Bytownite — FTIR1,801 points · 4004000 cm⁻¹
500100015002000250030003500400000.02000.04000.06000.08000.100Wavenumber (cm⁻¹)Absorbance

Spectrum Details

Modality
FTIR
Category
mineral
Material Type
Tectosilicate
Sample ID
HS105.1B, HS105.2B, HS105.3B, HS105.4B, HS105.6
Collection Locality
Essex County, New York
Spectral Purity
1b2_3_4_ # Bytownite HS105.1B # 1= 0.2-3, 2= 1.5-6, 3= 6-25, 4= 20-150 microns SPECTRAL_PURITY: 1b2_3_4_ # Bytownite HS105.2B # 1= 0.2-3, 2= 1.5-6, 3= 6-25, 4= 20-150 microns SPECTRAL_PURITY: 1b2b3b4b # Bytownite HS105.3B # 1= 0.2-3, 2= 1.5-6, 3= 6-25, 4= 20-150 microns SPECTRAL_PURITY: 1b2_3_4_ # Bytownite HS105.4B # 1= 0.2-3, 2= 1.5-6, 3= 6-25, 4= 20-150 microns SPECTRAL_PURITY: 1b2_3_4_ # Bytownite HS105.6 # 1= 0.2-3, 2= 1.5-6, 3= 6-25, 4= 20-150 microns
Composition / XRD
None # XRF, EPMA, ICP(Trace), WChem COMPOSITION_TRACE:
Sample Description
Part of the albite-anorthite solid solution series. Grain size fractions are indicated by the extension after the sample number: .1B = IMAGE_OF_SAMPLE: NO PHOTO
XRD Analysis
40 kV - 30 mA, 6.5-9.5 keV File: labrd105.mdi References: Borg and Smith (1969); Kroll (1983); PDF2 #41-1486, 19-0926 Found: Plagioclase feldspar, probably intermediate composition Comments: Peaks are moderately sharp peaks but show poorly resolved alpha1-alpha2 components, perhaps due to some variation in composition or structural state. Line-based search-match returns 10 plagioclase feldspars in the first 10 hits; the most likely hit (and only feldspar) from profile-based search-match is #41-1481, disordered An83Ab17 (bytownite). The delta 2 theta(131)-(1-31)=1.82 degrees and corresponds to low plagioclase (or intermediate albite) structural state and composition less than 53% anorthite component (Kroll, 1983, fig. 12). Reflections diagnostic of low plagioclase composition (Kroll, 1983, p. 328-9) yield Si/Al=1.3:1 (bytownite composition). There were unindexed reflections: 8.55 Angstroms (weak) is observed in other patterns and may be instrumental in origin; 4.23 Angstroms (very weak) could be explained by a trace of K-feldspar; and 1.829 Angstroms (moderately weak) remains unexplained.
X Units
cm⁻¹
Y Units
Absorbance
Data Points
1,801

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Attribution

USGS Spectral Library Version 7, U.S. Geological Survey

License: Public Domain

DOI: 10.3133/ds1035

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