Optical Design for a Cubesat: Unobscured Telescope, Using Freeform Mirrors and a Curved Detector


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Abstract

The possibility of constructing an optical scheme of a telescope for a small satellite based on mirrors with freeform surfaces and a curved photodetector is considered. It is shown that the use of a new element base allows the effective area of the main mirror to be maximized and the field of view up to 9.4 times to be increased in comparison with the classical scheme of the Ritchey–Chretien scheme in ensuring the high image quality.

About the authors

E. R. Muslimov

Aix Marseille Université, CNRS, LAM; Tupolev Kazan National Research Technical University

Email: nkpavlych@rambler.ru
France, 38 rue Frédéric Joliot-Curie, Marseille; ul. Karla Marksa 10, Kazan Tatarstan, 420111

E. Hugot

Aix Marseille Université, CNRS, LAM

Email: nkpavlych@rambler.ru
France, 38 rue Frédéric Joliot-Curie, Marseille

M. Ferrari

Aix Marseille Université, CNRS, LAM

Email: nkpavlych@rambler.ru
France, 38 rue Frédéric Joliot-Curie, Marseille

T. Behaghel

Aix Marseille Université, CNRS, LAM

Email: nkpavlych@rambler.ru
France, 38 rue Frédéric Joliot-Curie, Marseille

N. K. Pavlycheva

Tupolev Kazan National Research Technical University

Author for correspondence.
Email: nkpavlych@rambler.ru
Russian Federation, ul. Karla Marksa 10, Kazan Tatarstan, 420111

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