DCSIMG

“Masterpiece” delivered

SCHOTT manufactured an extremely curved secondary mirror substrate made of ZERODUR® glass-ceramic in Mainz, Germany, for the ESO´s Extremely Large Telescope

It is only ten centimeters thin – and that with an extreme curvature, a diameter of 4.25 meters and a weight of three tons. The ZERODUR® glass-ceramic mirror substrate manufactured by SCHOTT for the secondary mirror (Mirror 2 = M2) of the Extremely Large Telescope (ELT) of the ESO (European Southern Observatory) is a technological masterpiece. After sixteen months of production time, it left the main plant in Mainz in a huge, extra-wide transport box mid of January 2019. Now it will receive its “final touch” or, more precisely, its fine polishing in France at REOSC, a SAFRAN Group company. The actual mirror layer made of silver with a wafer-thin layer of silicon oxide as a protective film will be applied at the coating facility of the Paranal Observatory in Chile before it is mounted in the telescope.

The requirements for the casting of the 4.25 m mirror substrate were extremely high due to very narrow specifications for the glass quality. Last year, a highly convex mirror substrate only ten centimeters thin was ground from the blank weighing more than ten tons on state-of-the-art CNC machines. Dr. Thomas Westerhoff, Head of the Strategic Business Field ZERODUR® at SCHOTT: “It was a great challenge for our melting team and the experts running the CNC machines. A workpiece with this geometry had never been manufactured before: The M2 will be the largest convex mirror ever made.” In the ELT, it will reflect the light from the 39-meter main mirror extremely precisely onto the downstream mirror. After the “First Light,” the commissioning of the ELT in 2025 on the mountain Cerro Armazones in Chile, its outstanding performance will provide the sharpest view into space compared to previous telescopes. The ELT is ideally equipped for the search for Earth 2.0.

SCHOTT is manufacturing the substrate material for four of the five mirror components of the ELT optics: for the ESO´s ELT 39-meter primary mirror with 798 hexagons (plus 131 replacement segments), the 4.25-m secondary mirror that is now being delivered, the 4-m tertiary mirror and the segmented fourth mirror (M4). The ZERODUR® glass-ceramic used has a very low thermal expansion. This predestines it for astronomical applications where maximum precision is essential. In observing stars, the excellent image quality of the mirrors is always maintained, even when the temperature changes. SCHOTT has been producing this stable material that is resistant to temperature changes and practically doesn’t expand for about 50 years. The process know-how has been continuously developed further. Only in this way was it possible for ZERODUR® to become the “standard material” for telescope mirrors on Earth and in space – and for masterpieces such as the extreme M2 for the ELT to succeed.

The mirror substrate for the M2 of the Extremely Large Telescope, will have an extreme curvature.
The mirror substrate for the M2 of the Extremely Large Telescope, will have an extreme curvature.
The secondary mirror support for the ELT is ten centimeters thin, 4.25 meters in diameter and weighing three tons.
The secondary mirror support for the ELT is ten centimeters thin, 4.25 meters in diameter and weighing three tons.

January 18th, 2019

Dr. Thomas Westerhoff
Advanced Optics
SCHOTT AG

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