The Chandra X-Ray Optics

Abstract

Significant advances in science always take place when the state of the art in instrumentation improves dramatically. NASA's Chandra X-Ray Observatory represents such an advance. Launched in July of 1999, Chandra is an observatory designed to study the x-ray emission from all categories of astronomical objects --- from comets, planets, and normal stars to quasars, galaxies, and clusters of galaxies. At the heart of this observatory is the precision X-Ray optic that has been vital for Chandra's outstanding success and which features an angular resolution improved by an order of magnitude compared to its forerunners. The Chandra mission is now entering its 13-th year of operation. Given that the Observatory was designed for a minimum of 3 years of operation testifies to its robust and carefully thought out design. We review the design and construction of the remarkable telescope, present examples of its usage for astronomy and astrophysics, and speculate upon the future.

14 pages, 11 figures, invited paper for Optical Engineering

References in corpus (4)

• Revealing the properties of dark matter in the merging cluster MACSJ0025.4-1222
• The Faintest X-ray Sources from z=0-8
• Cosmic ray diffusion near the Bohm limit in the Cassiopeia A supernova remnant
• No evidence of obscured, accreting black holes in most z=6 star-forming galaxies

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• 3D printing for astronomical mirrors
• X-Ray Optics for Astrophysics: a historical review
• Formation Flying Techniques for the Virtual Telescope for X-Ray Observations
• A Novel Optical Design for Wide-Field Imaging in X-ray Astronomy