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The Constellation-X Spectroscopy X-Ray TelescopeThe status of technology development for the Constellation-X Spectroscopy X-ray Telescope (SXT) mirror is presented. The SXT mirror combines a large (1.6 m) aperture with modest (12 arc sec half power diameter) angular resolution and low mass (750 kg). The overall collecting area, larger than 9,600 square cm at 0.25 keV, requires high throughput, and thus nesting of a substantial number of thin reflectors. A phased development program is underway to develop reflectors, mounting and alignment approaches, and metrology techniques for components and the mirror has a whole. The latest results in all these areas are summarized, along with an overview of results of optical testing of reflector performance.
Document ID
20040171448
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Petre, Robert
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Content, David
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Lehan, John
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
O'Dell, Stephen
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Owens, Scott
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Podgorsky, William
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Stewart, Jeff
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zhang, William
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2004
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: SPIE Meeting
Location: Glasgow, Scotland
Country: United Kingdom
Start Date: June 21, 2004
End Date: June 24, 2004
Sponsors: International Society for Optical Engineering
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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