Chemistry:Zerodur

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Short description: Extremely durable glass-ceramic
Opening of the ELT secondary mirror ZERODUR® blank mould containing the glass at first annealing at the Schott AG 4-meter blank annealing facility in Mainz, Germany.[1]

Zerodur (notation of the manufacturer: ZERODUR®), a registered trademark of Schott AG,[2] is a lithium-aluminosilicate glass-ceramic[3] produced by Schott AG since 1968.[4] It has been used for a number of very large telescope mirrors including GTC, Keck I, Keck II,[5] and SOFIA, as well as some smaller telescopes (such as the GREGOR Solar Telescope). With its very low coefficient of thermal expansion (CTE) it can be used to produce mirrors that retain acceptable figures in extremely cold environments such as deep space.[6] Although it has advantages for applications requiring a coefficient of thermal expansion less than that of borosilicate glass, it remains very expensive as compared to borosilicate. The tight tolerance on CTE, ±0.007×106 K−1, allows for its use in high-precision applications.

Applications

The Keck II Telescope showing the segmented primary mirror made of Zerodur
  1. Optics
  2. Microlithography
  3. Measurement technology[4]

Properties

Zerodur has both an amorphous (vitreous) component and a crystalline component. Its most important properties[7] are:

  • Particularly low thermal expansion: in the range 0 to 50 °C it has a mean of 0 ± 0.007×106 K−1, which is two orders of magnitude better than that of fused quartz.[8][9]
  • High 3D homogeneity[9] with few inclusions, bubbles and internal stria (as contrasted to Cer-Vit).
  • Hardness similar to that of borosilicate glass, so that it can be ground and polished more easily than fused quartz.
  • High affinity for coatings.
  • Low helium permeability.
  • Non-porous (as contrasted to sintered ceramics).
  • Good chemical stability similar to that of fused quartz.
  • Fracture toughness approximately 0.9 MPa·m1/2.[3][10]

Physical properties

See also

References

  1. "Secondary Mirror of ELT Successfully Cast - Largest convex mirror blank ever created". http://www.eso.org/public/news/eso1715/. 
  2. "Zerodur®". http://www.unitedlens.com/page175.html. 
  3. 3.0 3.1 Viens, Michael J (April 1990). "Fracture Toughness and Crack Growth of Zerodur". NASA Technical Memorandum 4185. NASA. https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/19900011871_1990011871.pdf. 
  4. 4.0 4.1 "Schott AG Zerodur description". http://www.schott.com/advanced_optics/english/syn/advanced_optics/products/optical-materials/zerodur-zero-expansion-glass-ceramic/zerodur/index.html?so=uk&lang=english. 
  5. Döhring, Thorsten; Peter Hartmann. "Properties of Zerodur Mirror Blanks for Extremely Large Telescopes". Proc. SPIE. SPIE. http://www.optics.arizona.edu/optomech/Fall10/grad%20student%20reports/Properties%20of%20Zerodur%20Mirrors%20for%20Large%20Telescopes.pdf.  (dead link 7 July 2020)
  6. Baer, JW; WP Lotz. "Figure testing of 300 mm Zerodur mirrors at cryogenic temperatures". http://www.4dtechnology.com/reflib/Figure%20testing%20of%20300%20mm%20Zerodur%20mirrors%20at%20cryogenic%20temper.pdf. 
  7. "ZERODUR® Extremely Low Expansion Glass Ceramic: SCHOTT Advanced Optics - SCHOTT AG". http://www.schott.com/advanced_optics/english/products/optical-materials/zerodur-zero-expansion-glass-ceramic/zerodur/index.html. 
  8. "SCHOTT CTE Grades". http://www.schott.com/advanced_optics/english/syn/advanced_optics/products/optical-materials/zerodur-zero-expansion-glass-ceramic/zerodur/index.html. 
  9. 9.0 9.1 [1][|permanent dead link|dead link}}]
  10. Hartmann, P. (18 December 2012). "ZERODUR - Deterministic Approach for Strength Design" (PDF). Optical Engineering (NASA) 51 (12): 124002. doi:10.1117/1.OE.51.12.124002. Bibcode2012OptEn..51l4002H. http://opticalengineering.spiedigitallibrary.org/article.aspx?articleid=1486944. Retrieved 11 September 2013. 
  11. Senf, H; E Strassburger; H Rothenhausler (1997). "A study of Damage during Impact in Zerodur". J Phys IV France 7 (Colloque C3, Suppltment au Journal de Physique I11 d'aotit 1997): C3-1015-C3-1020. doi:10.1051/jp4:19973171. http://hal.archives-ouvertes.fr/docs/00/25/54/63/PDF/ajp-jp4199707C3171.pdf. Retrieved 31 August 2011. 

External links