Share Email Print
cover

Proceedings Paper

Constellation X-Ray Mission: recent developments for mission concept and technology development
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

The Constellation X-ray Mission is a high-throughput X-ray facility emphasizing observations at high spectral resolution (R ~ 300-3000) while covering a broad energy band (0.25-60 keV). The mission is intended to achieve a factor of 25-100 increase in sensitivity over current high resolution X-ray spectroscopy missions. Constellation-X is the X-ray astronomy equivalent of the Keck and the VLT, complementing the high spatial resolution capabilities of Changra. Constellation-X achieves its high-throughput and reduces mission risk by dividing the collecting area across four separate spacecraft launched two at a time into an L2 orbit. We describe the overall mission concept and also present a brief overview of alternate concepts which are under consideration. We discuss recent progress on the key technologies, including: lightweight, high-throughput X-ray optics, micro-caloriment spectrometer arrays, low-power and low-weight CCD arrays, lightweight gratings, multilayer coatings to enhance the hard X-ray performance of X-ray optics, and hard X-ray detectors.

Paper Details

Date Published: 11 October 2004
PDF: 13 pages
Proc. SPIE 5488, UV and Gamma-Ray Space Telescope Systems, (11 October 2004); doi: 10.1117/12.550481
Show Author Affiliations
Harvey Tananbaum, Smithsonian Astrophysical Observatory (United States)
Nicholas E. White, NASA Goddard Space Flight Ctr. (United States)
Jay A. Bookbinder, Smithsonian Astrophysical Observatory (United States)
Robert Petre, NASA Goddard Space Flight Ctr. (United States)
Kimberly Weaver, NASA Goddard Space Flight Ctr. (United States)


Published in SPIE Proceedings Vol. 5488:
UV and Gamma-Ray Space Telescope Systems
Guenther Hasinger; Martin J. L. Turner, Editor(s)

© SPIE. Terms of Use
Back to Top