Optical modeling and testing of the Deformable Mirror Demonstration Mission (DeMi) CubeSat payload
Author
Morgan, Rachel E.Allan, Gregory
Douglas, Ewan
do Vale Pereira, Paula
Egan, Mark
Furesz, Gabor
Gubner, Jennifer
Haughwout, Christian
Holden, Bobby
Merk, John
Murphy, Thomas
Stein, Abigail
Xin, Yinzi
Cahoy, Kerri
Affiliation
Univ Arizona, Dept Astron, Steward ObservIssue Date
2019-09-09
Metadata
Show full item recordPublisher
SPIE-INT SOC OPTICAL ENGINEERINGCitation
Morgan, R., Allan, G., Douglas, E., do Vale Pereira, P., Egan, M., Furesz, G., ... & Cahoy, K. (2019, September). Optical modeling and testing of the Deformable Mirror Demonstration Mission (DeMi) CubeSat payload. In Astronomical Optics: Design, Manufacture, and Test of Space and Ground Systems II (Vol. 11116, p. 111160E). International Society for Optics and Photonics.Rights
© 2019 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Deformable Mirror Demonstration Mission (DeMi) is a 6U CubeSat that will characterize the on-orbit performance of a Microelectromechanical Systems (MEMS) deformable mirror (DM) with both an image plane wavefront sensor and a Shack-Hartmann wavefront sensor (SHWFS). Coronagraphs on future space telescopes will require precise wavefront control to detect and characterize Earth-like exoplanets. High-actuator count MEMS deformable mirrors can provide wavefront control with low size, weight, and power. The DeMi payload will characterize the on-orbit performance of a 140 actuator MEMS Deformable Mirror (DM) with 5.5 mu m maximum stroke, with a goal of measuring individual actuator wavefront displacement contributions to a precision of 12 nm. The payload will be able to measure low order aberrations to lambda/10 accuracy and lambda/50 precision, and will correct static and dynamic wavefront phase errors to less than 100 nm RMS. We present an overview of the payload design, the assembly, integration, and test process, and report on the development and validation of an optical diffraction model of the payload. Launch is planned for late 2019.ISSN
0277-786XVersion
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2529540
