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Proceedings Paper • Open Access

Development of high precision and cryogenic lens holders
Author(s): A. Reutlinger; Anton Boesz; A. Mottaghibonab; P. Eckert; M. Dubowy; H. Gebler; F. Grupp; N. Geis; A. Bode; R. Katterloher; R. Bender

Paper Abstract

The optical system of the Near Infrared Spectrometer and Photometer (NISP) of the EUCLID mission consists mainly of a filter and grism wheel and 4 aspherical lenses with large diameters up to 170 mm. The single lenses require a high precision positioning at the operational temperature of 150 K. An additional design driver represents the CaF2 material of a lens, which is very sensitive wrt brittleness.

The technical maturity of the combination of single features such as CaF2, large diameter (and mass), high precision and cryogenic conditions is considered as low. Therefore, a dedicated pre-development program has been launched to design and develop a first prototype of lens holder and to demonstrate the functional performance at representative operational conditions.

The 4 lenses are divided into 3x lenses for the Camera Lens Assembly (CaLA) and 1x lens for the Corrector Lens Assembly (CoLA). Each lens is glue mounted onto solid state springs, part of an adaption ring. The adaption ring shall provide protection against vibration loads, high accuracy positioning, as well as quasi load free mounting of the lens under operational conditions. To reduce thermomechanical loads on the lens, the CTE of the adaption ring is adapted to that of the lens. The glue between lens and solid state spring has to withstand high tension loads during vibration. At the operational temperature the deviating CTE between glue and lens/adaption ring introduces shear loads into the glue interface, which are critical, in particular for the fragile CaF2 lens material. For the case of NISP the shear loads are controlled with the glue pad diameter and the glue thickness.

In the context of the development activity many technology aspects such as various solid state spring designs, glue selection and glue handling have been investigated. A parametric structural model was developed to derive the specific design feature of each ring, such as spring force, number of springs, eigenfrequency, etc.

This paper presents the design of the adaption ring in conjunction with test results from functional verification. These results are presented on behalf of the EUCLID consortium.

Paper Details

Date Published: 20 November 2017
PDF: 15 pages
Proc. SPIE 10564, International Conference on Space Optics — ICSO 2012, 105643T (20 November 2017); doi: 10.1117/12.2309023
Show Author Affiliations
A. Reutlinger, Kayser-Threde GmbH (Germany)
Anton Boesz, Kayser-Threde GmbH (Germany)
A. Mottaghibonab, Kayser-Threde GmbH (Germany)
P. Eckert, Kayser-Threde GmbH (Germany)
M. Dubowy, Kayser-Threde GmbH (Germany)
H. Gebler, Kayser-Threde GmbH (Germany)
F. Grupp, Max-Planck-Institut für extraterrestrische Physik (Germany)
Univ. Sternwarte München (Germany)
N. Geis, Max-Planck-Institut für extraterrestrische Physik (Germany)
A. Bode, Max-Planck-Institut für extraterrestrische Physik (Germany)
R. Katterloher, Max-Planck-Institut für extraterrestrische Physik (Germany)
R. Bender, Max-Planck-Institut für extraterrestrische Physik (Germany)
Univ. Sternwarte München (Germany)

Published in SPIE Proceedings Vol. 10564:
International Conference on Space Optics — ICSO 2012
Bruno Cugny; Errico Armandillo; Nikos Karafolas, Editor(s)

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