Silvering is the chemical process of coating a non-conductive substrate such as glass with a reflective substance, to produce a mirror. While the metal is often silver, the term is used for the application of any reflective metal.

Most common household mirrors are "back-silvered" or "second-surface", meaning that the light reaches the reflective layer after passing through the glass. A protective layer of paint is usually applied to protect the back side of the reflective surface .[1] This arrangement protects the fragile reflective layer from corrosion, scratches, and other damage.[2] However, the glass layer may absorb some of the light and cause distortions and optical aberrations due to refraction at the front surface, and multiple additional reflections on it, giving rise to "ghost images" (although some optical mirrors such as Mangins, take advantage of it).

Therefore, precision optical mirrors normally are "front-silvered" or "first-surface", meaning that the reflective layer is on the surface towards the incoming light. The substrate normally provides only physical support, and need not be transparent. A hard, protective, transparent overcoat may be applied to prevent oxidation of the reflective layer and scratching of the metal. Front-coated mirrors achieve reflectivities of 90–95% when new.


Aluminising tank at Mont Mégantic Observatory used for re-coating telescope mirrors.[3]

Ptolemaic Egypt had manufactured small glass mirrors backed by lead, tin, or antimony.[4] In the early 10th century, the Persian scientist al-Razi described ways of silvering and gilding in a book on alchemy,[citation needed] but this was not done for the purpose of making mirrors.

Tin-coated mirrors were first made in Europe in the 15th century. The thin tinfoil used to silver mirrors was known as "tain".[5] When glass mirrors first gained widespread usage in Europe during the 16th century, most were silvered with an amalgam of tin and mercury,[6]

In 1835 German chemist Justus von Liebig developed a process for depositing silver on the rear surface of a piece of glass; this technique gained wide acceptance after Liebig improved it in 1856.[7][8] The process was further refined and made easier by French chemist Tony Petitjean (1857).[9] This reaction is a variation of the Tollens' reagent for aldehydes. A diamminesilver(I) solution is mixed with a sugar and sprayed onto the glass surface. The sugar is oxidized by silver(I), which is itself reduced to silver(0), i.e. elemental silver, and deposited onto the glass.

In 1856-57 Karl August von Steinheil and Léon Foucault introduced the process of depositing an ultra-thin layer of silver on the front surface of a piece of glass, making the first optical-quality first surface glass mirrors, replacing the use of speculum metal mirrors in reflecting telescopes.[10] These techniques soon became standard for technical equipment.

An aluminum vacuum-deposition process invented in 1930 by Caltech physicist and astronomer John Strong, led to most reflecting telescopes shifting to aluminum.[11] Nevertheless, some modern telescopes use silver, such as the Kepler space observatory.[12][13] The Kepler mirror's silver was deposited using ion assisted evaporation.[12][13]

Modern silvering processesEdit

To speed up the reaction process of the silver, the ornaments are shaken in hot water, Lauscha

General processesEdit

Silvering aims to produce a non-crystalline coating of amorphous metal (metallic glass), with no visible artifacts from grain boundaries. The most common methods in current use are electroplating, chemical "wet process" deposition, and vacuum deposition.

Electroplating of a substrate of glass or other non-conductive material requires the deposition of a thin layer of conductive but transparent material, such as carbon. This layer tends to reduce the adhesion between the metal and the substrate. [2]:p.3,107 Chemical deposition can result in better adhesion, directly or by pre-treatment of the surface.

Vacuum deposition can produce very uniform coating with very precisely controlled thickness.[2]



The reflective layer on a second surface mirror such as a household mirror is often actual silver. A modern "wet" process for silver coating treats the glass with tin(II) chloride to improve the bonding between silver and glass. An activator is applied after the silver has been deposited to harden the tin and silver coatings. A layer of copper may be added for long-term durability.[14]

Silver would be ideal for telescope mirrors and other demanding optical applications, since it has the best initial front-surface reflectivity in the visible spectrum. However, it quickly oxidizes and absorbs atmospheric sulfur to create a dark, low-reflectivity tarnish.


The "silvering" on precision optical instruments such as telescopes is usually aluminum. Although aluminum also oxidizes quickly, the thin aluminum oxide (sapphire) layer is transparent, and so the high-reflectivity underlying aluminum stays visible.

In modern aluminum silvering, a sheet of glass is placed in a vacuum chamber with electrically heated nichrome coils that can evaporate aluminum. In a vacuum, the hot aluminum atoms travel in straight lines. When they hit the surface of the mirror, they cool and stick.

Some mirror makers evaporate a layer of quartz or beryllia on the mirror; others expose it to pure oxygen or air in an oven so that it will form a tough, clear layer of aluminum oxide.


The first tin-coated glass mirrors were produced by applying a tin-mercury amalgam to the glass and heating the piece to evaporate the mercury.


The "silvering" on infrared instruments is usually gold. It has the best reflectivity in the infrared spectrum, and has high resistance to oxidation and corrosion. Conversely, a thin gold coating is used to create optical filters which block infrared (by mirroring it back towards the source) while passing visible light.

See alsoEdit


  1. ^ Watson, Don Arthur (January 1986). Construction Materials and Processes. Gregg Division, McGraw-Hill. ISBN 9780070684768.
  2. ^ a b c H. Pulker, H.K. Pulker (1999): Coatings on Glass. Elsevier 1999
  3. ^ "Daily events and images of the installation of the BBSO New Solar Telescope". Big Bear Solar Observatory. Retrieved 6 January 2020.
  4. ^ Fioratti, Helen. "The Origins of Mirrors and their uses in the Ancient World". L'Antiquaire & the Connoisseur. Archived from the original on 2011-02-03. Retrieved 2009-08-14.
  5. ^ "tain". Oxford English Dictionary (1st ed.). Oxford University Press. 1933.
  6. ^ de Chavez, Kathleen Payne (Spring 2010). "Historic Mercury Amalgam Mirrors: History, Safety and Preservation" (PDF). Retrieved 2014-03-11.
  7. ^ Justus Liebig (1835). "Ueber die Producte der Oxydation des Alkohols". Annalen der Chemie. 14 (2): 133–167. Bibcode:1835AnP...112..275L. doi:10.1002/jlac.18350140202.
  8. ^ Justus Liebig (1856). "Ueber Versilberung und Vergoldung von Glas". Annalen der Chemie und Pharmacie. 98 (1): 132–139. doi:10.1002/jlac.18560980112.
  9. ^ "English Patents of Inventions, No. 1681". Retrieved 15 August 2019.
  10. ^ - Era of Huge Reflectors
  11. ^ "Mirror, Mirror: Keeping the Hale Telescope optically sharp" Archived 2009-10-11 at the Wayback Machine by Jim Destefani, Products Finishing Magazine, 2008
  12. ^ a b Fulton L., Michael; Dummer, Richard S. (2011). "Advanced Large Area Deposition Technology for Astronomical and Space Applications". Vacuum & Coating Technology (December 2011): 43–47. Archived from the original on 12 May 2013. Retrieved 6 April 2013.
  13. ^ a b Ball Aerospace and Technologies Corp. (September 25, 2007). "Ball Aerospace Completes Primary Mirror and Detector Array Assembly Milestones for Kepler Mission". Retrieved 6 April 2013.
  14. ^ Episode 305 of How It's Made, filmed at in Anjou, Quebec, Canada

External linksEdit

  •, Diy mirror / mirroring / silvering