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dc.contributor.authorMerck, John
dc.contributor.authorSkouloudis, Nikolaos
dc.contributor.authorDouglas, Ewan S.
dc.contributor.authorCahoy, Kerri
dc.contributor.authorAllan, Gregory W.
dc.contributor.authorBarnes, Derek C.
dc.contributor.authorFigura, Joseph S.
dc.contributor.authorHaughwout, Christian Alexander
dc.contributor.authorGubner, Jennifer N.
dc.contributor.authorKnoedler, Alexander A.
dc.contributor.authorLeClair, Sarah
dc.contributor.authorMurphy, Thomas J.
dc.contributor.authorOpperman, Roedolph A
dc.date.accessioned2018-05-07T19:27:59Z
dc.date.available2018-05-07T19:27:59Z
dc.date.issued2017-08
dc.identifier.isbn9781510612570
dc.identifier.isbn9781510612587
dc.identifier.urihttp://hdl.handle.net/1721.1/115251
dc.description.abstractThe Deformable Mirror Demonstration Mission (DeMi) was recently selected by DARPA to demonstrate in-space operation of a wavefront sensor and Microelectromechanical system (MEMS) deformable mirror (DM) payload on a 6U CubeSat. Space telescopes designed to make high-contrast observations using internal coronagraphs for direct characterization of exoplanets require the use of high-actuator density deformable mirrors. These DMs can correct image plane aberrations and speckles caused by imperfections, thermal distortions, and diffraction in the telescope and optics that would otherwise corrupt the wavefront and allow leaking starlight to contaminate coronagraphic images. DeMi is provide on-orbit demonstration and performance characterization of a MEMS deformable mirror and closed loop wavefront sensing. The DeMi payload has two operational modes, one mode that images an internal light source and another mode which uses an external aperture to images stars. Both the internal and external modes include image plane and pupil plane wavefront sensing. The objectives of the internal measurement of the 140-actuator MEMS DM actuator displacement are characterization of the mirror performance and demonstration of closed-loop correction of aberrations in the optical path. Using the external aperture to observe stars of magnitude 2 or brighter, assuming 3-axis stability with less than 0.1 degree of attitude knowledge and jitter below 10 arcsec RMSE, per observation, DeMi will also demonstrate closed loop wavefront control on an astrophysical target. We present an updated payload design, results from simulations and laboratory optical prototyping, as well as present our design for accommodating high-voltage multichannel drive electronics for the DM on a CubeSat.en_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2274430en_US
dc.rightsArticle 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.en_US
dc.sourceSPIEen_US
dc.subjectUnited States. Defense Advanced Research Projects Agency (Aurora Flight Sciences)en_US
dc.titleDesign of the deformable mirror demonstration CubeSat (DeMi)en_US
dc.typeArticleen_US
dc.identifier.citationDouglas, Ewan S., et al. "Design of the Deformable Mirror Demonstration CubeSat (DeMi)." Proceedings Volume 10400, Techniques and Instrumentation for Detection of Exoplanets VIII, 6-10 August, 2017, San Diego, California, edited by Stuart Shaklan, SPIE, 2017, p. 37. © 2017 SPIE.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Aeronautics and Astronauticsen_US
dc.contributor.mitauthorDouglas, Ewan S.
dc.contributor.mitauthorCahoy, Kerri
dc.contributor.mitauthorAllan, Gregory W.
dc.contributor.mitauthorBarnes, Derek C.
dc.contributor.mitauthorFigura, Joseph S.
dc.contributor.mitauthorHaughwout, Christian Alexander
dc.contributor.mitauthorGubner, Jennifer N.
dc.contributor.mitauthorKnoedler, Alexander A.
dc.contributor.mitauthorLeClair, Sarah
dc.contributor.mitauthorMurphy, Thomas J.
dc.contributor.mitauthorOpperman, Roedolph A
dc.relation.journalProceedings Volume 10400, Techniques and Instrumentation for Detection of Exoplanets VIIIen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2018-03-15T18:13:30Z
dspace.orderedauthorsDouglas, Ewan S.; Cahoy, Kerri L.; Merck, John; Barnes, Derek; Allan, Gregory; Skouloudis, Nikolaos; LeClair, Sarah; Figura, Joseph S.; Haughwout, Christian A.; Gubner, Jennifer N.; Knoedler, Alex A.; Murphy, Thomas J.; Opperman, Roedolph A.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-0813-4308
dc.identifier.orcidhttps://orcid.org/0000-0002-7791-5124
dc.identifier.orcidhttps://orcid.org/0000-0002-7879-730X
dc.identifier.orcidhttps://orcid.org/0000-0001-7326-4654
mit.licensePUBLISHER_POLICYen_US


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