WANG Ling, ZHU Demao, SUN Jinyu, HU Aiping, ZHANG Feng. Identification Characteristics of Gem-Grade Natural Glass[J]. Journal of Gems & Gemmology, 2015, 17(3): 43-47.
Citation: WANG Ling, ZHU Demao, SUN Jinyu, HU Aiping, ZHANG Feng. Identification Characteristics of Gem-Grade Natural Glass[J]. Journal of Gems & Gemmology, 2015, 17(3): 43-47.

Identification Characteristics of Gem-Grade Natural Glass

More Information
  • Received Date: December 04, 2014
  • There are two kinds of gem-grade natural glass in daily inspection,obsidian and tektite,which have similar appearance.It is difficult to distinguish them.Obsidian and tektite are formed under different geological environments,and possess different physical and chemical characteristics.By using the conventional gemmological tests as well as scanning electron microscope(SEM),energy dispersive spectrometer(EDS),and Fourier transform infrared spectrometer(FTIR),this article contrasted the physical properties and chemical compositions of obsidian and tektite.
    Both tektite and obsidian are mainly composed of SiO2, and Al2O3. The content of SiO2.in tektite is about 71.3%~79. 3%, while SiO2, of obsidian is about 70%. Otherwise, FeOT in obsidian is less than that in tektite, and content of alkali (R2O) is more in obsidian. Tektite is formed under ultra-high temperature and pressure, and it shows highly non-crystallizing and disordering. Stretching vibration mode of [SiO4 ] appears at 1 200~900 cm-1 in tektite and obsidian. Comparing with tektite, obsidian is formed under lower temperature and pressure. The absorptions at 750~500 cm-1and 1 170 cm-1 indicate the existence of quartz and plagioclase. In conclusion, different forming condition of obsidian and tektite caused differences in chemical compositions and infrared absorption characteristics. Therefore.these two kinds of natural glass can be identified in daily gem inspection.

  • [1]
    . 徐征, 李志刚, 曹姝旻.天然玻璃与玻璃的鉴别[J]. 宝石和宝石学杂志, 2007, 9(1):22-22.
    [2]
    . Alvarez L W, Alvarez W, Asaro F, et al.Extraterrestrial cause for the Cretaceous-Tertiary extinction[J]. Science, 1980(208):1 095-1 108.
    [3]
    . French B M.Traces of catastrophe:A handbook of shockmetamorphic effects in terrestrial meteorite impact craters[D]. Houston:Lunar and Planetary Institute, 1998.
    [4]
    . Melosh H J.Impact cratering:A geologic process[M]. New York:Oxford University Press, 1989.
    [5]
    . Chao E C T.Comparison of the Cretaceous-Tertiary boundary impact events and the 0.77-Ma Australasian tektite event;relevance to mass extinction[M]. Denvor:U.S.Geological Survey Bulletin, 1993.
    [6]
    . Glass B P.Tektites[J]. Journal of Non-Crystalline Solids, 1984(67):333-344.
    [7]
    . Koeberl C.Geochemistry of tektites and impact glass[J]. Annual Review of Earth and Planetary Sciences, 1986(14):323-350.
    [8]
    . McCall G J H.Tektites in the geological record:showers of glass from the sky[M]. United Kingdom:the Geological Society Publishing House, 2001:256.
    [9]
    . Montanari A, Koeberl C.Impact stratigraphy:the Italian record[M]. New York:Springer-Verlag, 2000:364.
    [10]
    . 潘兆橹.结晶学及矿物学(下册)[M]. 北京:地质出版社, 1994:74.
    [11]
    . 吴瑾光.近代傅里叶变换红外光谱技术及应用[M]. 北京:科学技术文献出版社, 1994:133.
    [12]
    . Williams O, Jeanloz R.Spectroscopic evidence for pressure induced coordination changes in silicate glasses and melt[J]. Science, 1988(239):902-905.

Catalog

    Article Metrics

    Article views (162) PDF downloads (35) Cited by()
    Related

    /

    DownLoad:  Full-Size Img  PowerPoint
    Return
    Return