Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage Conditions May Apply Usage Conditions Apply There are restrictions for re-using this media. For more information, visit the Smithsonian's Terms of Use page. IIIF provides researchers rich metadata and image viewing options for comparison of works across cultural heritage collections. More - https://iiif.si.edu View Manifest View in Mirador Viewer Usage conditions may apply

The Faint Object Spectrograph (FOS), one of the original axial instruments launched with the Hubble Space Telescope (HST) in April 1990, provided confirming evidence for a massive black hole in 1994 in the giant elliptical galaxy M87. It also engaged in many other observing programs, observing individual stars in other galaxies as well as the impact of Comet Shoemaker-Levy 9 on Jupiter. But most significantly it refined quantitative measurements of the characteristics of massive black holes from studies of accretion disks at the centers of galaxies. After almost seven years of service, FOS was removed from HST on February 13, 1997 by the Space Shuttle crew (STS 82, Discovery) during a servicing mission to provide room for a new instrument. The instrument was transferred to NASM by NASA's Goddard Space Flight Center in 1999.

 Display Status

This object is on display in Mary Baker Engen Restoration Hangar at the Steven F. Udvar-Hazy Center in Chantilly, VA.

Mary Baker Engen Restoration Hangar
Object Details
Date 1999 Country of Origin United States of America Type INSTRUMENTS-Scientific Manufacturer Martin Marietta
 Dimensions 3-D (Object Only): 100.3 × 90.2 × 222.9cm, 499.9kg (3 ft. 3 1/2 in. × 2 ft. 11 1/2 in. × 7 ft. 3 3/4 in., 1102lb.)
Support (Rolling Base Only): 130.2 × 22.9 × 130.2cm (4 ft. 3 1/4 in. × 9 in. × 4 ft. 3 1/4 in.)
 Materials Black aluminum and mixed metal box mounted vertically on a 4x4 foot aluminum plate. The box protects a precision framework of metal that constitutes an optical bench consisting of optical components, electronic detectors and baffles.
 Inventory Number A19990075000 Credit Line Transferred from NASA, Goddard Space Flight Center, Greenbelt, MD. Data Source National Air and Space Museum Restrictions & Rights Usage conditions apply
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