Wavefront control in space with MEMS deformable mirrors

To meet the high contrast requirement of 1 × 10[superscript −10] to image an Earth-like planet around a Sun-like star, space telescopes equipped with coronagraphs require wavefront control systems. Deformable mirrors (DMs) are a key element of a wavefront control system, as they correct for imperfec...

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Main Authors: Cahoy, Kerri, Marinan, Anne D., Novak, Benjamin G., Kerr, Caitlin E., Webber, Matthew William
Other Authors: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
Format: Article
Language:en_US
Published: SPIE 2013
Online Access:http://hdl.handle.net/1721.1/81180
https://orcid.org/0000-0002-7791-5124
https://orcid.org/0000-0001-5391-9844
https://orcid.org/0000-0001-9005-2493
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author Cahoy, Kerri
Marinan, Anne D.
Novak, Benjamin G.
Kerr, Caitlin E.
Webber, Matthew William
author2 Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
author_facet Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
Cahoy, Kerri
Marinan, Anne D.
Novak, Benjamin G.
Kerr, Caitlin E.
Webber, Matthew William
author_sort Cahoy, Kerri
collection MIT
description To meet the high contrast requirement of 1 × 10[superscript −10] to image an Earth-like planet around a Sun-like star, space telescopes equipped with coronagraphs require wavefront control systems. Deformable mirrors (DMs) are a key element of a wavefront control system, as they correct for imperfections, thermal distortions, and diffraction that would otherwise corrupt the wavefront and ruin the contrast. The goal of the CubeSat Deformable Mirror technology demonstration mission is to test the ability of a microelectromechanical system (MEMS) deformable mirror to perform wavefront control on-orbit on a nanosatellite platform. In this paper, we consider two approaches for a MEMS deformable mirror technology demonstration payload that will fit within the mass, power, and volume constraints of a CubeSat: 1) a Michelson interferometer and 2) a Shack-Hartmann wavefront sensor. We clarify the constraints on the payload based on the resources required for supporting CubeSat subsystems drawn from subsystems that we have developed for a different CubeSat flight project. We discuss results from payload lab prototypes and their utility in defining mission requirements.
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spelling mit-1721.1/811802022-10-02T01:17:47Z Wavefront control in space with MEMS deformable mirrors Cahoy, Kerri Marinan, Anne D. Novak, Benjamin G. Kerr, Caitlin E. Webber, Matthew William Massachusetts Institute of Technology. Department of Aeronautics and Astronautics Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Cahoy, Kerri Marinan, Anne D. Novak, Benjamin G. Kerr, Caitlin E. Webber, Matthew William To meet the high contrast requirement of 1 × 10[superscript −10] to image an Earth-like planet around a Sun-like star, space telescopes equipped with coronagraphs require wavefront control systems. Deformable mirrors (DMs) are a key element of a wavefront control system, as they correct for imperfections, thermal distortions, and diffraction that would otherwise corrupt the wavefront and ruin the contrast. The goal of the CubeSat Deformable Mirror technology demonstration mission is to test the ability of a microelectromechanical system (MEMS) deformable mirror to perform wavefront control on-orbit on a nanosatellite platform. In this paper, we consider two approaches for a MEMS deformable mirror technology demonstration payload that will fit within the mass, power, and volume constraints of a CubeSat: 1) a Michelson interferometer and 2) a Shack-Hartmann wavefront sensor. We clarify the constraints on the payload based on the resources required for supporting CubeSat subsystems drawn from subsystems that we have developed for a different CubeSat flight project. We discuss results from payload lab prototypes and their utility in defining mission requirements. United States. National Aeronautics and Space Administration (Space Technology Research Fellowships OCT-NSTRF) Jeptha and Emily Wade Fund Massachusetts Institute of Technology. Undergraduate Research Opportunities Program 2013-09-25T19:33:39Z 2013-09-25T19:33:39Z 2013-03 Article http://purl.org/eprint/type/ConferencePaper 0277-786X http://hdl.handle.net/1721.1/81180 Cahoy, Kerri L., Anne D. Marinan, Benjamin Novak, Caitlin Kerr, and Matthew Webber. “Wavefront control in space with MEMS deformable mirrors.” In MEMS Adaptive Optics VII, edited by Scot S. Olivier, Thomas G. Bifano, and Joel Kubby, 861708-861708-16. SPIE - International Society for Optical Engineering, 2013. © (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE) https://orcid.org/0000-0002-7791-5124 https://orcid.org/0000-0001-5391-9844 https://orcid.org/0000-0001-9005-2493 en_US http://dx.doi.org/10.1117/12.2005685 Proceedings of SPIE--the International Society for Optical Engineering; v.8617 Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf SPIE SPIE
spellingShingle Cahoy, Kerri
Marinan, Anne D.
Novak, Benjamin G.
Kerr, Caitlin E.
Webber, Matthew William
Wavefront control in space with MEMS deformable mirrors
title Wavefront control in space with MEMS deformable mirrors
title_full Wavefront control in space with MEMS deformable mirrors
title_fullStr Wavefront control in space with MEMS deformable mirrors
title_full_unstemmed Wavefront control in space with MEMS deformable mirrors
title_short Wavefront control in space with MEMS deformable mirrors
title_sort wavefront control in space with mems deformable mirrors
url http://hdl.handle.net/1721.1/81180
https://orcid.org/0000-0002-7791-5124
https://orcid.org/0000-0001-5391-9844
https://orcid.org/0000-0001-9005-2493
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