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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{One source|date=August 2019}}&lt;br /&gt;
[[Image:Foslarge sm.jpg|thumb|The Faint Object Spectrograph (FOS). This picture was taken after FOS was brought back to the Earth again. Credit: [[NASA]]/[[ESA]].]]&lt;br /&gt;
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The &amp;#039;&amp;#039;&amp;#039;Faint Object Spectrograph&amp;#039;&amp;#039;&amp;#039; (FOS) was a [[spectrograph]] installed on the [[Hubble Space Telescope]]. It was replaced by the [[Space Telescope Imaging Spectrograph]] in 1997, and is now on display in the [[National Air and Space Museum]] in Washington DC.&lt;br /&gt;
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==FOS facts==&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;Instrument type&amp;#039;&amp;#039;&amp;#039;: 	                                         Spectrograph&lt;br /&gt;
*&amp;#039;&amp;#039;&amp;#039;Wavelength range&amp;#039;&amp;#039;&amp;#039;: 	                                                115 to 850&amp;amp;nbsp;nm&lt;br /&gt;
&lt;br /&gt;
A technical description of the construction and operation of the FOS can be found in NASA technical report CP-2244.&amp;lt;ref name=&amp;quot;CP-2244&amp;quot;&amp;gt;{{cite tech report |title=The Space Telescope Observatory |number=CP-2244 |institution=NASA |url=http://hdl.handle.net/2060/19820025420 |date=1982}}, page 55. A 40 MB PDF file.&amp;lt;/ref&amp;gt;  The instrument used two [[digicon]] detectors, &amp;#039;blue&amp;#039; and &amp;#039;red&amp;#039;, and had a spectral resolution of about 1300 over the 115&amp;amp;nbsp;nm to 850&amp;amp;nbsp;nm range.  It had a number of apertures of varying size, but the aberration of the HST mirror meant that, until COSTAR was installed, the smallest apertures suffered very serious loss of light; even the largest 4.3-arcsecond aperture collected only 70% of the light from a point source.&lt;br /&gt;
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The digicons suffered from inadequate magnetic shielding, which meant that a static image was smeared over several pixels; the red digicon suffered most from this.  Also, either the blue detector or one of the mirrors in the system was contaminated in such a way as to remove sensitivity below 150&amp;amp;nbsp;nm; this was a serious problem since it makes the [[Lyman-alpha]] line at 121.6&amp;amp;nbsp;nm inaccessible.&lt;br /&gt;
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==References==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
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==External links==&lt;br /&gt;
*{{Commonscatinline}}&lt;br /&gt;
*[https://archive.today/20121214233815/http://www.stsci.edu/hst/fos The Faint Object Spectrograph (FOS)]&lt;br /&gt;
*[http://www.spacetelescope.org/news/html/heic0112.html ESA/Hubble Release about FOS]&lt;br /&gt;
*[http://www.spacetelescope.org/about/general/instruments/fos.html FOS at ESA/Hubble]&lt;br /&gt;
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{{Hubble Space Telescope}}&lt;br /&gt;
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[[Category:Hubble Space Telescope instruments]]&lt;br /&gt;
[[Category:Space science experiments]]&lt;br /&gt;
[[Category:Spectrographs]]&lt;br /&gt;
[[Category:Space hardware returned to Earth intact]]&lt;br /&gt;
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{{observatory-stub}}&lt;/div&gt;</summary>
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