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.
@article{arxiv.1809.09097,
title = {Laboratory Demonstration of an Active Optics System for High-Resolution Deployable CubeSat},
author = {Noah Schwartz and David Pearson and Stephen Todd and Maria Milanova and William Brzozowski and Andy Vick and David Lunney and Donald MacLeod and Steve Greenland and Jean-François Sauvage and Benjamin Gore},
journal= {arXiv preprint arXiv:1809.09097},
year = {2018}
}
Comments
15 pages, 19 figures, 4S Symposium, Conference Proceeding, Sorrento, Italy, May 28 - June 1, 2018