SKYVA
Vacuum Coating System for Large Astronomical Mirrors

Are you looking for a coating solution for large telescope mirrors? SKYVA coating systems were developed specifically for this application: they deposit homogeneous, highly reflective metal layers on large, curved substrates up to 8.4 m in diameter and are available in several chamber sizes. This enables scaling from small, through medium, to large aperture areas.

For maximum reflectance we rely on requirement-optimized ("enhanced") silver and aluminum coating systems. Silver offers the highest reflectance in the visible and near-infrared range but requires a precisely matched protective layer to ensure long-term stability and corrosion resistance. Aluminum provides very good reflectance across a broader spectrum including UV and is more robust in many applications.

SKYVA supports both coating materials — from "protected" or "enhanced" silver coatings to optimized, protected aluminum coatings — as well as multilayer systems that tailor reflectivity curves to your spectrum and ensure excellent layer uniformity even on curved surfaces.

Additionally, we offer the system optionally with a peripheral washing unit for cleaning the mirror prior to re-coating.

SKYVA sys­tems sup­port pro­tec­ted and en­hanced alu­min­um and sil­ver coat­ings, as well as ap­pli­ca­tion-spe­cif­ic mul­ti­lay­er sys­tems with tai­lored re­flec­tiv­i­ty cur­ves. Cus­tom­ized cham­ber di­men­sions, mir­ror fix­tures, and han­dling sys­tems en­able the equip­ment to be adap­ted to dif­fer­ent mir­ror ge­o­met­ries and pro­ject re­quire­ments, aligning with lo­cal in­dus­trial stan­dards and re­gional tech­ni­cal part­ner­ships.

Au­to­mat­ed pro­cess se­quences, ad­vanced con­trol sys­tems, recipe man­age­ment, fault di­ag­no­sis, and in­tu­i­tive hu­man-ma­chine in­ter­fac­es en­able re­pro­du­ci­ble coat­ing re­sults. Op­tional re­mote mon­i­tor­ing and con­trol sup­port ef­fi­cient op­er­a­tion and main­ten­ance, par­tic­u­lar­ly at re­mote ob­ser­va­to­ry sites. Pe­riph­er­al equip­ment, in­clud­ing mir­ror-clean­ing and mea­sure­ment sys­tems, is also avail­able, with dedicated en­gi­neer­ing and train­ing pro­grams for lo­cal op­er­a­tors.

Would you like to learn more? Explore the content below or contact us.

Highest reflectivity

on the most demanding mirror geometries

Reliable operation & mechanical stability over decades

with maximum substrate safety

Fully automatic processes

including modern control/visualization for the operator

References

Reference Projects

VON ARDENNE can point to a proven track record of references. The coating system SKYVA 8400 at the Vera C. Rubin Observatory on Cerro Pachón in northern Chile is the largest and youngest system realized by VON ARDENNE to date. The coating system is fully integrated into the ground floor of the building complex. The Mirrors M1 to M3 are transported directly to the system via an elevator mechanism to be regularly recoated, ensuring highest reflectivity for optimal sky observations.

Other noteworthy SKYVA projects include the coating system at the Gran Telescopio Canarias. Here, an ASTA 2800 system from former Vakuumtechnik Dresden (VTD*) has been successfully in operation since 2006. Beyond that, an ASTA 2400 system is in operation at Shamakhy Astrophysical Observatory.

*VTD was fully integrated into the VON ARDENNE Group in 2023.
 

 SKYVA8400SKYVA2400SKYVA2000
VTD name ASTA 2800ASTA 2400
Mirror sizemax. 8.400 mmmax. 2.400 mm~ 2.000 mm
Vacuumturbopumps
cryopumps
cryopumpsdiffusion pumps
cryotrap
Pre-treat­ment(magnetron)plasma glow dischargeplasma glow discharge
Coating optionsmagnetron PVD
8 sources
evaporation
(thermal/electron beam)
evaporation
(thermal)
Working principlerotating sourcesrotating mirrorrotating mirror
Weight (approx.)128 tons9 tons6.5 tons
Project siteVera C. Rubin Observatory
Chile
Gran Telescopio Canarias (GTC)
Spain
Shamakhy Astrophysical Observatory
Azerbaijan
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Marko Schöbitz

Technical Sales ManagerVON ARDENNE GmbH

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