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Laboratory Demonstration of an Active Optics System for High-Resolution Deployable CubeSat

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arxiv 1809.09097 v1 pith:JTN5IT74 submitted 2018-09-24 astro-ph.IM physics.optics

Laboratory Demonstration of an Active Optics System for High-Resolution Deployable CubeSat

classification astro-ph.IM physics.optics
keywords mirrordemonstrationlaboratoryco-phasingcubesatdeployabledesignhigh-resolution
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this paper we present HighRes: a laboratory demonstration of a 3U CubeSat with a deployable primary mirror that has the potential of achieving high-resolution imaging for Earth Observation. The system is based on a Cassegrain telescope with a segmented primary mirror composed of 4 petals that form an effective aperture of 300 mm. The design provides diffraction limited performance over the entire field-of-view and allows for a panchromatic ground-sampling distance of less than 1 m at an altitude of 350 km. The alignment and co-phasing of the mirror segments is performed by focal plane sharpening and is validated through rigorous numerical simulations. The opto-mechanical design of the prototype and its laboratory demonstration are described and measurements from the on-board metrology sensors are presented. This data verifies that the performance of the mirror deployment and manipulation systems is sufficient for co-phasing. In addition, it is shown that the mirrors can be driven to any target position with an accuracy of 25 nm using closed-loop feedback between the mirror motors and the on-board metrology.

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