Open Access Paper
20 November 2017 Active x-ray optics for high resolution space telescopes
Peter Doel, Carolyn Atkins, D. Brooks, Charlotte Feldman, Richard Willingale, Tim Button, Daniel Rodriguez Sanmartin, Carl Meggs, Ady James, Graham Willis, Andy Smith
Author Affiliations +
Proceedings Volume 10565, International Conference on Space Optics — ICSO 2010; 105652V (2017) https://doi.org/10.1117/12.2309202
Event: International Conference on Space Optics—ICSO 2010, 2010, Rhodes Island, Greece
Abstract
The Smart X-ray Optics (SXO) Basic Technology project started in April 2006 and will end in October 2010. The aim is to develop new technologies in the field of X-ray focusing, in particular the application of active and adaptive optics. While very major advances have been made in active/adaptive astronomical optics for visible light, little was previously achieved for X-ray optics where the technological challenges differ because of the much shorter wavelengths involved.

The field of X-ray astronomy has been characterized by the development and launch of ever larger observatories with the culmination in the European Space Agency’s XMM-Newton and NASA's Chandra missions which are currently operational. XMM-Newton uses a multi-nested structure to provide modest angular resolution (∼10 arcsec) but large effective area, while Chandra sacrifices effective area to achieve the optical stability necessary to provide sub-arc second resolution. Currently the European Space Agency (ESA) is engaged in studies of the next generation of X-ray space observatories, with the aim of producing telescopes with increased sensitivity and resolution. To achieve these aims several telescopes have been proposed, for example ESA and NASA’s combined International X-ray Observatory (IXO), aimed at spectroscopy, and NASA’s Generation-X. In the field of X-ray astronomy sub 0.2 arcsecond resolution with high efficiency would be very exciting. Such resolution is unlikely to be achieved by anything other than an active system. The benefits of a such a high resolution would be important for a range of astrophysics subjects, for example the potential angular resolution offered by active X-ray optics could provide unprecedented structural imaging detail of the Solar Wind bowshock interaction of comets, planets and similar objects and auroral phenomena throughout the Solar system using an observing platform in low Earth orbit.

A major aim of the SXO project was to investigate the production of thin actively controlled grazing incident optics for the next generation of X-ray space telescopes. Currently telescope systems are limited in the resolution and sensitivity by the optical quality of the thin shell optics used. As part of its research programme an actively controlled prototype X-ray thin shell telescope optic of dimensions 30x10cm has been developed to bench test the technology. The design is based on thin nickel shells bonded to shaped piezo-electric unimorph actuators made from lead zirconate titanate (PZT).
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Peter Doel, Carolyn Atkins, D. Brooks, Charlotte Feldman, Richard Willingale, Tim Button, Daniel Rodriguez Sanmartin, Carl Meggs, Ady James, Graham Willis, and Andy Smith "Active x-ray optics for high resolution space telescopes", Proc. SPIE 10565, International Conference on Space Optics — ICSO 2010, 105652V (20 November 2017); https://doi.org/10.1117/12.2309202
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Actuators

X-ray optics

X-rays

Space telescopes

Prototyping

Active optics

Ferroelectric materials

RELATED CONTENT

X-ray optic developments at NASA's MSFC
Proceedings of SPIE (May 03 2013)
Toward active x-ray telescopes
Proceedings of SPIE (October 12 2011)
Active x-ray mirror development at UCL: preliminary results
Proceedings of SPIE (November 21 2007)
Active x ray optics for the next generation of x...
Proceedings of SPIE (May 05 2009)

Back to Top