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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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. |
first_indexed | 2024-09-23T15:12:09Z |
format | Article |
id | mit-1721.1/81180 |
institution | Massachusetts Institute of Technology |
language | en_US |
last_indexed | 2024-09-23T15:12:09Z |
publishDate | 2013 |
publisher | SPIE |
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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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