Mirror Technology Development for the International X-ray Observatory Mission
Abstract
The International X-ray Observatory (IXO) mission requires a large mirror assembly with an angular resolution of 5 arcseconds half-power diameter and an effective area of 3 square meters. We are developing a glass slumping technique that is coming close to meeting these requirements. In the last few years significant and steady progress has been made in mirror segment fabrication, metrology, and alignment and integration. In this paper, we will present a status update on the various components of the technology, including mirror fabrication, glass screening and strengthening, coating, mirror mount and metrology, alignment and integration. We will also present our plan and expectations for the next couple of years.
Document Details
- Document Type
- Technical Report
- Publication Date
- Jun 06, 2010
- Accession Number
- ADA536310
Entities
People
- William W. Zhang
Organizations
- National Aeronautics and Space Administration