Poster + Paper
27 August 2022 6U CubeSat deployable telescope for optical Earth observation and astronomical optical imaging
Noah Schwartz, William Brzozowski, Zeshan Ali, Maria Milanova, Katherine Morris, Charlotte Bond, Jennifer Keogh, Douglas Harvey, Lawrence Bissell, Jean-François Sauvage, Maxime Dumont, Carlos Correia, Phil Rees, Heather Bruce
Author Affiliations +
Conference Poster
Abstract
Available volumes of nanosats such as CubeSats impose physical limits to the telescope diameter, limiting achievable spatial resolution and photometric capability. For example, a 12U CubeSat typically only has sufficient volume to host a 20 cm diameter monolithic telescope. In this paper, we present recent advances in deployable optics to host a 30 cm+ diameter telescope in a 6U CubeSat, with a volume of 4U dedicated to the payload and 2U to the satellite bus. To reach this high level of compactness, we fold the primary and secondary mirrors for launch, which are then unfolded and aligned in space. Diffraction-limited imaging quality in the visible part of the spectrum is achieved by controlling each mirror segment in piston, tip, and tilt. In this paper, we first describe overall satellite concept, we then report on the optomechanical design of the payload to deploy and adjust the mirrors. Finally, we discuss the automatic phasing of the primary to control the final optical quality of the telescope.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Noah Schwartz, William Brzozowski, Zeshan Ali, Maria Milanova, Katherine Morris, Charlotte Bond, Jennifer Keogh, Douglas Harvey, Lawrence Bissell, Jean-François Sauvage, Maxime Dumont, Carlos Correia, Phil Rees, and Heather Bruce "6U CubeSat deployable telescope for optical Earth observation and astronomical optical imaging", Proc. SPIE 12180, Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave, 1218031 (27 August 2022); https://doi.org/10.1117/12.2627248
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KEYWORDS
Telescopes

Mirrors

Tolerancing

Sensors

Active optics

Actuators

Wavefronts

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