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

Backup for the gamma-ray detector installed in the "wheel" section on the OSO-1 satellite launched on 7 March 1962. The detector, built at the University of Rochester, includes two scintillators and a Cerenkov counter. Entering gamma-rays impinge on a thin lead sheet in the instrument; the collision converts the high energy photon to an electron-positron pair. Those charged particles then lead to a flash of light in the Lucite Cerenkov counter. The resulting flashes are amplified and counted by a photomultiplier tube. The scintillators form part of the anti-coincidence circuit that accepts only those signals that enter the detector from the front. The instrument on OSO-1 detected the cosmic ray background but did not provide clear evidence for high energy solar events. The detector was transferred to NASM from the Smithsonian Astrophysical Observatory in December 1982.

Display Status

This object is not on display at the National Air and Space Museum. It is either on loan or in storage.

Object Details
Country of Origin United States of America Type INSTRUMENTS-Scientific Manufacturer University of Rochester
Dimensions 3-D: 27.9 x 35.6 x 19.7cm (11 x 14 x 7 3/4 in.)
Materials Mixed metals
Lucite
Glass photomultipliers
Electronics
Inventory Number A19830087000 Credit Line Transferred from the Smithsonian Astrophysical Observatory Data Source National Air and Space Museum Restrictions & Rights Usage conditions apply
For more information, visit the Smithsonians Terms of Use.