Progress on precise grinding and polishing of thin glass monolithic shell (towards WFXT)

O. Citterio, M. M. Civitani, J. Arnold, S. Campana, H. Combrinck, P. Conconi, V. Cotroneo, R. Freeman, E. Mattaini, R. Morton, G. Motta, G. Pareschi, G. Parodi, L. Proserpio, S. Schuler, P. Simpson, G. Tagliaferri, D. Walker

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

14 Citations (Scopus)


The next generation wide-field X-ray telescope (WFXT) will require an angular resolution of ∼5-10 arcsec almost constant across a wide field of view (∼1 deg2 diameter). To achieve this goal, the design of the optical system has to be based on mirrors characterized by short length and polynomial profiles, as well as focal plane curvature and plate scale corrections. These concepts guarantee an improved angular resolution at large off-axis angle with respect to the normally used Wolter-I configuration. These telescopes are therefore optimal for survey purposes. A significant increase of effective area and grasp with respect to previous missions must also be achieved. This is possible with high precision but at the same time thin (2-3 mm thickness for mirror diameters of 30-110 cm) glass mirror shells. To achieve the goal of 5 arcsec and improve further the technology, we are considering different materials. Fused silica, a well-known material with good thermo-mechanical and polishability characteristics provide the best choice. To bring the mirror shells to the needed accuracy, we are adopting a deterministic direct polishing method (already used for past missions as Einstein, Rosat, Chandra). The technological challenge now is to apply it for almost ten times thinner shells.

Original languageEnglish
Title of host publicationOptics for EUV, X-Ray, and Gamma-Ray Astronomy V
Publication statusPublished - 8 Nov 2011
Externally publishedYes
EventOptics for EUV, X-Ray, and Gamma-Ray Astronomy V - San Diego, United States
Duration: 23 Aug 201125 Aug 2011
Conference number: V (Link to Conference Details )


ConferenceOptics for EUV, X-Ray, and Gamma-Ray Astronomy V
Country/TerritoryUnited States
CitySan Diego
Internet address


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