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Space TelescopesExtended Abstract

Optics Requirements For The Generation-X X-Ray Telescope

20191 min read127 words
O'Dell, S. ., Elsner, R. F., Kolodziejczak, J. J., Ramsey, B. D., Weisskopf, M. C., Zhang, W. W., Content, D. A., Petre, R., Saha, T. T., Reid, P. B., Schwartz, D. A., Brissenden, R. J., Elvis, M., Freeman, M., Gaetz, T., Gorenstein, P., Jerius, D., Juda, M., Murray, S. S., Podgorski, W. A., Wolk, S. J., and Trolier-McKinstry, S.
Marshall Space Flight Center

US, European, and Japanese space agencies each now operate successful X-ray missions -- NASA s Chandra, ESA s XMM-Newton, and JAXA s Suzaku observatories. Recently these agencies began a collaboration to develop the next major X-ray astrophysics facility -- the International X-ray Observatory (IXO) -- for launch around 2020. IXO will provide an order-of-magnitude increase in effective area, while maintaining good (but not sub-arcsecond) angular resolution. X-ray astronomy beyond IXO will require optics with even larger aperture areas and much better angular resolution. We are currently conducting a NASA strategic mission concept study to identify technology issues and to formulate a technology roadmap for a mission -- Generation-X (Gen-X) -- to provide these capabilities. Achieving large X-ray collecting areas in a space observatory requires extremely lightweight mirrors.


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