Paper
29 July 2010 Enhancing the International X-ray Observatory
Author Affiliations +
Abstract
Over the last two years, we have studied system concepts for the International X-ray Observatory (IXO) with the goal of increasing the science return of the mission and to reduce technical and cost risk. We have developed an optical bench concept that has the potential to increase the focal length from 20 to 25 m within the current mass and stability requirements. Our deployable bench is a tensegrity structure formed by two telescoping booms (compression) and a hexapod cable (tension) truss. This arrangement achieves the required stiffness for the optical bench at minimal mass while employing only high TRL components and flight proven elements. The concept is based on existing elements, can be fully tested on the ground and does not require new technology. Our design further features hinged, articulating solar panels, an optical bench fully enclosed in MLI and an instrument module with radially facing radiator panels. We find that our design can be used over a wide range of sun angles, thereby greatly increasing IXO's field of regard, without distorting the optical bench. This makes a much larger fraction of the sky instantaneously accessible to IXO.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Rolf Danner, Dean Dailey, Charles Lillie, and Connie Spittler "Enhancing the International X-ray Observatory", Proc. SPIE 7732, Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray, 77323V (29 July 2010); https://doi.org/10.1117/12.855968
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KEYWORDS
Mirrors

Sun

Observatories

Optical benches

X-rays

Space operations

Distortion

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