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Proceedings Paper • Open Access

The SPICA Telescope: design evolution and expected performance

Paper Abstract

The fairing of the launcher selected for the Space Infrared telescope for Cosmology and Astrophysics (SPICA) mission is not compatible with a primary mirror of 3.5m in diameter. Thus three alternative optical designs of the SPICA Telescope Assembly (STA) with a primary mirror of reduced size were defined and their theoretical optical performances assessed. The impact of the size reduction on the STA optical performances was then quantified. Based on the results of the study, we defined a STA optical design optimum in terms of optical performances and of accommodation of instruments in the STA focal surface.

Paper Details

Date Published: 11 January 2018
PDF: 6 pages
Proc. SPIE 10565, International Conference on Space Optics — ICSO 2010, 1056555 (11 January 2018); doi: 10.1117/12.2309162
Show Author Affiliations
L. M. Gaspar Venancio, European Space Agency, ESTEC (Netherlands)
D. Doyle, European Space Agency, ESTEC (Netherlands)
K. Isaak, European Space Agency, ESTEC (Netherlands)
T. Onaka, Univ. of Tokyo (Japan)
H. Kaneda, Nagoya Univ. (Japan)
T. Nakagawa, Japanese Aerospace Exploration Agency (Japan)
H. Matsuhara, Japanese Aerospace Exploration Agency (Japan)
N. Takahashi, Japanese Aerospace Exploration Agency (Japan)
T. Yamawaki, Japanese Aerospace Exploration Agency (Japan)


Published in SPIE Proceedings Vol. 10565:
International Conference on Space Optics — ICSO 2010
Errico Armandillo; Bruno Cugny; Nikos Karafolas, Editor(s)

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