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Wide Field and Planetary Camera for Space TelescopeThe Space Telescope's Wide Field and Planetary Camera instrument, presently under construction, will be used to map the observable universe and to study the outer planets. It will be able to see 1000 times farther than any previously employed instrument. The Wide Field system will be located in a radial bay, receiving its signals via a pick-off mirror centered on the optical axis of the telescope assembly. The external thermal radiator employed by the instrument for cooling will be part of the exterior surface of the Space Telescope. In addition to having a larger (1200-12,000 A) wavelength range than any of the other Space Telescope instruments, its data rate, at 1 Mb/sec, exceeds that of the other instruments. Attention is given to the operating modes and projected performance levels of the Wide Field Camera and Planetary Camera.
Document ID
19830050807
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lockhart, R. F.
(California Institute of Technology, Jet Propulsion Laboratory, Observational Systems Div., Pasadena CA, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: Instrumentation in astronomy IV; Fourth Conference
Location: Tucson, AZ
Start Date: March 8, 1982
End Date: March 10, 1982
Accession Number
83A32025
Distribution Limits
Public
Copyright
Other

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