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Reanalysis of the cosmic dust L 2011 S2 and L 2009 I14 NASA samples

In: Contributions to Geophysics and Geodesy, vol. 36, no. 1
Igor Kapišinský - Jozef Ivan - Karol Iždinský - Zdeněk Pánek - Milina Zemánková
Detaily:
Rok, strany: 2006, 63 - 71
Kľúčové slová:
cosmic/interplanetary dust, chemistry, analytical electron microscope, porous chondritic micrometeorites
O článku:
In this study the cosmic dust samples L 2011 S2 and L 2009 I14 have been reanalysed. Particles were obtained from the NASA Johnson Space Center(JSC) Cosmic Dust Collection. The reanalysis of the particle L 2009 I14 near the equilibrium state shows the 6.7 mass % of SiO2, and 60; 16.7; 5.4 and 11.2 mass % of pyroxene, cordierite pentlandite and iron silicide Fe2Si, respectively. In the case far from equilibrium state there can not be excluded a presence of other phases as bronzite or hypersthene or klinoferrosilite as well as troilite and pyrrhotite and sluggish crystallised pyroxene. For particle L 2011 S2 it was not possible to make any reliable qualitative conclusions due to problems mentioned in the paper.
Ako citovať:
ISO 690:
Kapišinský, I., Ivan, J., Iždinský, K., Pánek, Z., Zemánková, M. 2006. Reanalysis of the cosmic dust L 2011 S2 and L 2009 I14 NASA samples. In Contributions to Geophysics and Geodesy, vol. 36, no.1, pp. 63-71. 1338-0540.

APA:
Kapišinský, I., Ivan, J., Iždinský, K., Pánek, Z., Zemánková, M. (2006). Reanalysis of the cosmic dust L 2011 S2 and L 2009 I14 NASA samples. Contributions to Geophysics and Geodesy, 36(1), 63-71. 1338-0540.