Generated by DeepSeek V3.2| Zerodur | |
|---|---|
| Name | Zerodur |
| Density | 2.53 g/cm³ |
| Youngs modulus | 90.3 GPa |
| Thermal expansion | ≈0 ± 0.10 × 10−6/K (0–50 °C) |
| Poisson ratio | 0.24 |
| Flexural strength | 50 MPa |
| Manufacturer | SCHOTT AG |
Zerodur. It is a lithium-aluminosilicate glass-ceramic produced by the German company SCHOTT AG, renowned for its extremely low coefficient of thermal expansion. This unique property makes it an ideal material for high-precision applications where dimensional stability over a wide temperature range is critical, such as in astronomical telescope mirrors and precision measurement systems. Its development represented a significant advancement in materials science for optics and metrology.
The material is composed of a fine-grained crystalline phase, primarily high-quartz solid solution, embedded within a residual glass phase. This specific microstructure, achieved through controlled crystallization, is responsible for its near-zero thermal expansion behavior. Key properties include exceptional homogeneity, high stiffness, and good chemical durability, comparable to that of borosilicate glass. Its optical transparency in the visible spectrum is limited, but it transmits well in the infrared, making it suitable for certain optical components. The material's stability is often compared to that of fused quartz, but with superior thermal performance for many engineering applications.
Production begins with the melting of raw materials, including silicon dioxide, aluminum oxide, lithium oxide, and nucleating agents like titanium dioxide and zirconium dioxide, in high-temperature furnaces. The molten glass is formed into blanks, which are then subjected to a precise two-stage heat treatment process. This ceramming process first induces nucleation, followed by a growth phase where the desired crystalline structure forms. Final steps include precision annealing, grinding, and polishing, often using techniques developed for large astronomical optics. The entire process is tightly controlled by SCHOTT AG to ensure the consistent, high-quality material required for demanding applications in science and industry.
Its primary application is as the substrate for large primary mirrors in major astronomical telescopes, including those at the European Southern Observatory's Very Large Telescope and the Gran Telescopio Canarias. It is also used in ring laser gyroscopes for inertial navigation systems, substrates for extreme ultraviolet lithography masks, and precision reference bodies in metrology, such as bases for coordinate-measuring machines. In satellite technology, components made from this material ensure the stability of instruments on missions like the Gaia (spacecraft) astrometry observatory. The material's stability is crucial for the performance of interferometers used in gravitational wave detectors like LIGO.
The material was developed in the late 1960s by researchers at SCHOTT AG in Mainz, Germany, in response to the growing need for dimensionally stable mirror substrates for large telescopes. Its invention was driven by the limitations of traditional materials like Pyrex and fused silica under variable thermal conditions. The successful commissioning of the Max Planck Institute for Astronomy's Calar Alto Observatory telescopes, which used early versions, demonstrated its viability. Continuous refinement of the ceramming process by SCHOTT AG has enabled the production of ever-larger monolithic blanks, supporting the ambitious goals of modern astrophysics and precision engineering.
Compared to fused silica, it offers a significantly lower and more consistent thermal expansion coefficient, though fused silica has superior transmission in the ultraviolet. Unlike metals such as aluminum or beryllium, it does not conduct heat well, but its dimensional stability is far superior for precision applications. When compared to other glass-ceramics like Cervit, it generally offers comparable near-zero expansion but with different manufacturing heritage and specific property profiles. For ultralightweight mirrors, silicon carbide composites offer high stiffness-to-weight ratios, but often with greater thermal expansion and different fabrication challenges. The choice between these materials depends on the specific requirements of the optical system, balancing factors like thermal performance, weight, and cost.
Category:Glass-ceramics Category:Optical materials Category:German inventions