# Silvering

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{{short description|Application of reflective coatings to mirrors}}
{{About|the process of applying a metallic surface to glass|the application of silver to a metal surface using mercury|Mercury silvering|the use of electricity to apply metal coating to an object|Electroplating|the formation of metallic silver in photographic film|Photographic printing#Silver mirroring}}
[[File:Silver mirror reaction.jpg|thumb|upright|Silvering on the inside of a glass [test tube](/source/test_tube)]]
'''Silvering''' is the [chemical](/source/chemistry) process of coating a non-conductive substrate such as [glass](/source/glass) with a [reflective](/source/reflectivity) substance, to produce a [mirror](/source/mirror).  While the metal is often [silver](/source/silver), the term is used for the application of any reflective metal.

==Process==
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](/source/paint) is usually applied to protect the back side of the reflective surface.<ref name=Watson-1986-01/> This arrangement protects the fragile reflective layer from corrosion, scratches, and other damage.<ref name=Pulker-Pulker-1999/> However, the glass layer may absorb some of the light and cause distortions and [optical aberration](/source/optical_aberration)s due to [refraction](/source/refraction) at the front surface, and multiple additional reflections on it, giving rise to "ghost images" (although some optical mirrors such as [Mangin mirror](/source/Mangin_mirror)s take advantage of it).

Therefore, precision [optical](/source/optics) mirrors normally are "front-silvered" or "[first-surface](/source/first-surface_mirror)", 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](/source/oxidation) of the reflective layer and scratching of the metal. Front-coated mirrors achieve reflectivities of 90–95% when new.

== History ==
[[File:Aluminizing tank.jpg|thumb|upright|Aluminising tank at [Mont Mégantic Observatory](/source/Mont_M%C3%A9gantic_Observatory) used for re-coating telescope mirrors.<ref name=BBSO-NJIT-sec4/>]]

[Ptolemaic](/source/History_of_Ptolemaic_Egypt) [Egypt](/source/Egypt) had manufactured small glass mirrors backed by [lead](/source/lead), tin, or [antimony](/source/antimony).<ref name=Fioratti-2009/> In the early 10th century, the Persian scientist [al-Razi](/source/Muhammad_ibn_Zakariya_al-Razi) described ways of silvering and [gilding](/source/gilding) in a book on [alchemy](/source/alchemy),{{citation needed|date=October 2016}} but this was not done for the purpose of making mirrors.

Tin-coated mirrors were first made in [Europe](/source/Europe) in the 15th century. The thin tinfoil used to silver mirrors was known as "tain".<ref>{{cite OED1 |tain}}</ref> When glass mirrors first gained widespread usage in Europe during the [16th century](/source/16th_century), most were silvered with an [amalgam](/source/amalgam_(chemistry)) of [tin](/source/tin) and [mercury](/source/mercury_(element)).<ref name=deChavez-2010-spr/>

In 1835 [German](/source/Germany) [chemist](/source/chemist) [Justus von Liebig](/source/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.<ref name=Liebig-1835/><ref name=Liebig-1856/>
The process was further refined and made easier by the chemist Tony Petitjean (1856).<ref name=Petitjohn-1856/> This reaction is a variation of the [Tollens' reagent](/source/Tollens'_reagent) for aldehydes. A solution of [diamminesilver](/source/diamminesilver)(I) is mixed with a sugar and sprayed onto the glass surface. Silver(I) oxidizes the sugar, reducing itself to silver(0), i.e. elemental [silver](/source/silver), which deposits onto the glass.

In 1856-1857 [Karl August von Steinheil](/source/Karl_August_von_Steinheil) and [Léon Foucault](/source/L%C3%A9on_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](/source/first-surface_mirror) glass mirrors, replacing the use of [speculum metal](/source/speculum_metal) mirrors in [reflecting telescope](/source/reflecting_telescope)s.<ref name=STScI-huge-refl-p2/>{{dead link|date=February 2023}} These techniques soon became standard for technical equipment.

An aluminum vacuum-deposition process invented in 1930 by Caltech physicist and astronomer [John Strong](/source/John_D._Strong), led to most reflecting telescopes shifting to aluminum.<ref name=Destefani-2008/> Nevertheless, some modern telescopes use silver, such as the [Kepler Space Telescope](/source/Kepler_(spacecraft)). The ''Kepler'' mirror's silver was deposited using [ion-assisted evaporation](/source/electron-beam_physical_vapor_deposition).<ref name=BallAerosp-2007-09-25/><ref name=Fulton-Dummer-2011/>

== Modern silvering processes ==
{{See also|Electroplating|Electroless deposition|Vacuum deposition}}
[[File:Silvering of glass ornaments Lauscha.jpg|thumb|right|220px|To speed up the reaction process of the silver, the ornaments are shaken in hot water, [Lauscha](/source/Lauscha)]]

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

Electroplating of a substrate of glass or other non-[conductive](/source/Electrical_conductivity) 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.<ref name=Pulker-Pulker-1999/>{{rp|style=ama|pp= 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.<ref name=Pulker-Pulker-1999/>

===Metals===

====Silver====
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](/source/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.<ref name=HowItsMade-ep305/>

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](/source/Silver_oxide) and absorbs atmospheric [sulfur](/source/Silver_sulfide) to create a dark, low-reflectivity tarnish.

====Aluminum====
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](/source/vacuum) chamber with electrically heated [nichrome](/source/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](/source/quartz) or [beryllia](/source/Beryllium_oxide) on the mirror; others expose it to pure [oxygen](/source/oxygen) or air in an oven so that it will form a tough, clear layer of [aluminum oxide](/source/aluminum_oxide).

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

====Gold====
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 reflecting it) while passing visible light.

==See also==
* [Dielectric mirror](/source/Dielectric_mirror)
* [List of telescope parts and construction](/source/List_of_telescope_parts_and_construction)
* [Optical coating](/source/Optical_coating)
* [Mercury glass](/source/Mercury_glass)
* [Mercury silvering](/source/Mercury_silvering)
* [Metallizing](/source/Metallizing)

==References==
{{reflist|25em|refs=

<ref name=BallAerosp-2007-09-25>
{{cite web
 |title=Ball Aerospace completes primary mirror and detector array assembly milestones for Kepler Mission
 |date=25 September 2007
 |publisher=Ball Aerospace and Technologies Corp.
 |website=spaceref.com
 |url= http://www.spaceref.com/news/viewpr.html?pid=23610
 |access-date=6 April 2013
}}
</ref>

<ref name=BBSO-NJIT-sec4>
{{cite web
 |title=Daily events and images of the installation of the BBSO New Solar Telescope
 |publisher=[Big Bear Solar Observatory](/source/Big_Bear_Solar_Observatory)
 |type=blog
 |url=http://www.bbso.njit.edu/telblog/section4.html
|website=www.bbso.njit.edu
 |access-date=6 January 2020
}}
</ref>

<ref name=deChavez-2010-spr>
{{cite web
 |first=Kathleen Payne |last=de Chavez
 |date=Spring 2010
 |title=Historic mercury amalgam mirrors: History, safety, and preservation
 |website=Williamstown Art
 |url=http://www.williamstownart.org/techbulletins/images/WACC%20Historic%20Mercury%20Mirrors.pdf
 |access-date=2014-03-11
}}
</ref>

<ref name=Destefani-2008>
{{cite magazine
 |first=Jim |last=Destefani
 |date=March 2008
 |title=Mirror, mirror: Keeping the Hale Telescope optically sharp
 |magazine=[Products Finishing](/source/Products_Finishing) Magazine
 |id=PF mag article&nbsp;030805
 |url=http://www.pfonline.com/articles/030805.html
 |archive-url=https://web.archive.org/web/20091011082949/http://www.pfonline.com/articles/030805.html
 |archive-date=2009-10-11
}}
</ref>

<ref name=Fioratti-2009>
{{cite web
 |first=Helen |last=Fioratti
 |title=The Origins of Mirrors and their uses in the Ancient World
 |website=L'Antiquaire & the Connoisseur
 |url=http://www.lantiquaire.us/origins-of-mirrors.html
 |access-date=2009-08-14 |url-status=dead
 |archive-url=https://web.archive.org/web/20110203052336/http://www.lantiquaire.us/origins-of-mirrors.html
 |archive-date=2011-02-03
}}
</ref>

<ref name=Fulton-Dummer-2011>
{{cite journal
 |last1=Fulton  |first1=L. Michael
 |last2=Dummer  |first2=Richard S.
 |year=2011
 |title=Advanced Large Area Deposition Technology for Astronomical and Space Applications
 |journal=Vacuum & Coating Technology
 |volume=2011 |issue=December |pages=43–47
 |url=http://e-ditionsbyfry.com/Olive/ODE/VTC/Default.aspx?href=VTC/2011/12/01
 |access-date=6 April 2013  |url-status=dead
 |archive-url=https://web.archive.org/web/20130512233653/http://e-ditionsbyfry.com/Olive/ODE/VTC/Default.aspx?href=VTC%2F2011%2F12%2F01
 |archive-date=12 May 2013
}}
</ref>

<ref name=HowItsMade-ep305>
{{cite AV media
 |number=305
 |series=[How It's Made](/source/How_It's_Made)
 |title=Episode&nbsp;305
 |place=[Anjou, Quebec](/source/Anjou%2C_Quebec), Canada
 |quote=Episode&nbsp;305 filmed at [http://www.laverreriewalker.com/ Verrerie-Walker].
}}
</ref>

<ref name=Liebig-1835>
{{cite journal
 | first = Justus  | last = Liebig  | author-link = Justus Liebig
 | year = 1835
 | title = Ueber die Producte der Oxydation des Alkohols  |language=de
 | trans-title = Regarding the products of oxidation of alcohols
 | journal = [Annalen der Chemie](/source/Liebigs_Annalen)
 | volume = 14  | issue = 2  | pages = 133–167
 | doi = 10.1002/jlac.18350140202  | bibcode = 1835AnP...112..275L
 | url = https://zenodo.org/record/1426914
}}
</ref>

<ref name=Liebig-1856>
{{cite journal
 | first = Justus  | last = Liebig  | author-link = Justus Liebig
 | year = 1856
 | title = Ueber Versilberung und Vergoldung von Glas  |language=de
 | trans-title = Regarding the silvering and gilding of glass
 | journal = [Annalen der Chemie und Pharmacie](/source/Liebigs_Annalen)
 | volume = 98  | issue = 1  | pages = 132–139
 | doi = 10.1002/jlac.18560980112  | url = https://zenodo.org/record/1427076
}}
</ref>

<ref name=Petitjohn-1856>
{{cite patent
 | country  = GB
 | number   = 1681
 | status   = patent
 | title    = Silvering, Gilding, and Platinizing Glass
 | gdate    = 1856-01-12
 | fdate    = 1855-07-24
 | inventor-last = Petitjean
 | inventor-first = Tony
 | url      = https://books.google.com/books?id=nQcADAPqbO0C&q=anthony+petitjohn+silvering&pg=RA29-PA7
}}
</ref>

<ref name=Pulker-Pulker-1999>
{{cite book
 |first1=H.K.
|last1=Pulker
 |date=1999-03-29
 |title=Coatings on Glass
 |publisher=[Elsevier Science](/source/Elsevier_Science)
|url=https://books.google.com/books?id=ho2pYhOiEMcC
|isbn=9780080525556
}}
</ref>

<ref name=STScI-huge-refl-p2>
{{cite web
 |title=Era of huge reflectors, page&nbsp;2
 |series=Amazing-space
 |website=[Space Telescope Science Institute](/source/Space_Telescope_Science_Institute) (stsci.edu)
 |place=Baltimore, MD
 |url=http://amazing-space.stsci.edu/resources/explorations/groundup/lesson/eras/huge-reflectors/page2.php
}}
</ref>

<ref name=Watson-1986-01>
 {{cite book
 |last=Watson |first=Don Arthur
 |date=January 1986
 |title=Construction Materials and Processes
 |publisher=McGraw-Hill
 |department=Gregg Division
 |isbn=9780070684768
 |language=en
 |url=https://books.google.com/books?id=NKVRAAAAMAAJ
 |via=Google Books
}}
</ref>

}} <!-- end "refs=" -->

==External links==
*[https://web.archive.org/web/20110510201943/http://tions.net/CA256EA900408BD5/vwWWW/house~04~16 Tions.net], Diy mirror / mirroring / silvering

Category:Chemical processes
Category:Mirrors
Category:Silver

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Adapted from the Wikipedia article [Silvering](https://en.wikipedia.org/wiki/Silvering) by Wikipedia contributors ([contributor history](https://en.wikipedia.org/wiki/Silvering?action=history)). Available under [Creative Commons Attribution-ShareAlike 4.0 International](https://creativecommons.org/licenses/by-sa/4.0/). Changes may have been made.
