Paper
30 August 2005 Diamond turned, light weight, athermal, visible TMA telescope for the planned New Horizons mission to Pluto
M. J. Hegge, J. W. Baer, L. M. R. Hardaway, G. Taudien, D. S. Sabatke, S. R. Shidemantle, J. J. Santman, L. E. Comstock
Author Affiliations +
Proceedings Volume 5877, Optomechanics 2005; 58770K (2005) https://doi.org/10.1117/12.617018
Event: Optics and Photonics 2005, 2005, San Diego, California, United States
Abstract
Unpolished diamond turned mirrors are common for infrared systems. We report the successful use of unpolished mirrors in a visible spectrum, all aluminum telescope for the planned New Horizons mission to Pluto. The Ralph telescope is an F/8.7 Three Mirror Anastigmat with a 75mm aperture, a 5.7° by 1.0° field of view, and a mass of only 8kg. Key to the performance of the system are a process for reducing the micro-roughness of the off-axis aspheric surfaces to below 60 Ångstroms RMS, and the fabrication of precision diamond turned mounting features on the mirrors and one-piece, thin-walled housing. The telescope achieves nearly diffraction-limited performance with minimal post-assembly alignment, and maintains that performance, including focus, over a wide range about the operating temperature of 210K.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
M. J. Hegge, J. W. Baer, L. M. R. Hardaway, G. Taudien, D. S. Sabatke, S. R. Shidemantle, J. J. Santman, and L. E. Comstock "Diamond turned, light weight, athermal, visible TMA telescope for the planned New Horizons mission to Pluto", Proc. SPIE 5877, Optomechanics 2005, 58770K (30 August 2005); https://doi.org/10.1117/12.617018
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KEYWORDS
Mirrors

Diamond

Telescopes

Aluminum

Space telescopes

Pluto

Diamond turning

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