Overview: Silicon Cladding for Lightweight Mirrors

Lightweight substrates that reduce the areal density of large telescope mirrors are frequently difficult to polish directly to an optical figure. A polishable cladding layer addresses this by providing a workable surface over a low-density structural substrate. ZeCoat develops low-stress silicon cladding that yields such a surface without imparting the film-induced distortion that would otherwise compromise the mirror figure of thin, lightweight optics.


The Technology

The principal constraint on a thick cladding layer is intrinsic film stress, which produces substrate curvature that degrades figure — a limitation that is most severe for the thin, low-mass mirrors the technology targets. ZeCoat deposits silicon by pulsed ion-assisted evaporation, producing a dense, polishable layer at residual stress low enough to preserve the underlying figure. The deposited silicon can subsequently be polished and figured to an optical finish, allowing advanced low-density substrates to support a conventionally finished optical surface.


Abstract & Publications

SBIR Contracts

Benefits

  • Adds a dense, polishable surface to lightweight substrates.
  • Low residual film stress preserves mirror figure during cladding.
  • Enables the optical finish required for high-resolution UVOIR imaging.
  • Combines low areal density with conventional surface quality.

Applications

  • Lightweight space telescope mirrors.
  • Surface finishing of large UVOIR optics.
  • Advanced ceramic and composite mirror substrates.