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  • 1
    ISSN: 1573-4889
    Keywords: titanium ; titanium alloys ; oxidation kinetics ; whiskers
    Source: Springer Online Journal Archives 1860-2000
    Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision Mechanics
    Notes: Abstract The oxidation kinetics of pure titanium and of Ti-6Al-4 V by water vapor were studied between 650 and 950°C and from 0.5 to 18 Torr. The results showed a marked similarity of the oxidation behavior for both the alloy and pure titanium. The rate curves had the same appearance. At low temperatures (below 750°C) they exhibited two stages. At high temperature the first of these stages was not observed. Scanning electron microscopy (SEM) and electron probe analyses of the scale showed that the structure of the scales was also similar over the temperature range 750–900°C: they consisted of two layers of rutile, and, in the case of the alloy, of a thin sublayer of alumina between the other two. Furthermore, SEM examination of the surface of oxidized specimens revealed the existence of whiskers.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2019-07-13
    Description: A field campaign was organized in September 2006 by Centro de Astobiologica (Spain) and Washington University (St Louis, USA) for the geological study of the Rio Tinto river bed sediments using a suite of in-situ instruments comprising an ASD reflectance spectrometer, an emission spectrometer, panoramic and close-up color imaging cameras, a life detection system and NASA's CheMin 4 XRD/XRF prototype. The primary objectives of the field campaign were to study the geology of the site and test the potential of the instrument suite in an astrobiological investigation context for future Mars surface robotic missions. The results of the overall campaign will be presented elsewhere. This paper focuses on the results of the XRD/XRF instrument deployment. The specific objectives of the CheMin 4 prototype in Rio Tinto were to 1) characterize the mineralogy of efflorescent salts in their native environments; 2) analyze the mineralogy of salts and oxides from the modern environment to terraces formed earlier as part of the Rio Tinto evaporative system; and 3) map the transition from hematite-dominated terraces to the mixed goethite/salt-bearing terraces where biosignatures are best preserved.
    Keywords: Geosciences (General)
    Type: Lunar and Planetary Science Conference; Mar 12, 2007 - Mar 16, 2007; Houston, TX; United States
    Format: application/pdf
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