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dc.contributor.authorLawson, P. R.
dc.contributor.authorStapelfeldt, K.
dc.contributor.authorBrenner, M.
dc.contributor.authorLisman, D.
dc.contributor.authorSiegler, N.
dc.contributor.authorUnwin, S.
dc.contributor.authorWarfield, K.
dc.contributor.authorSeager, Sara
dc.date.accessioned2015-07-29T12:30:04Z
dc.date.available2015-07-29T12:30:04Z
dc.date.issued2014-08
dc.identifier.issn0277-786X
dc.identifier.urihttp://hdl.handle.net/1721.1/97914
dc.description.abstractThis paper provides a survey of the state-of-the-art in coronagraph and starshade technologies and highlights areas where advances are needed to enable future NASA exoplanet missions. An analysis is provided of the remaining technology gaps and the relative priorities of technology investments leading to a mission that could follow JWST. This work is being conducted in support of NASAs Astrophysics Division and the NASA Exoplanet Exploration Program (ExEP), who are in the process of assessing options for future missions. ExEP has funded Science and Technology Definition Teams to study coronagraphs and starshade mission concepts having a lifecycle cost cap of less than $1B. This paper provides a technology gap analysis for these concepts.en_US
dc.language.isoen_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2054939en_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.titleAn analysis of technology gaps and priorities in support of probe-scale coronagraph and starshade missionsen_US
dc.typeArticleen_US
dc.identifier.citationLawson, P. R., S. Seager, K. Stapelfeldt, M. Brenner, D. Lisman, N. Siegler, S. Unwin, and K. Warfield. “An Analysis of Technology Gaps and Priorities in Support of Probe-Scale Coronagraph and Starshade Missions.” Edited by Jacobus M. Oschmann, Mark Clampin, Giovanni G. Fazio, and Howard A. MacEwen. Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave (July 14, 2014). © 2014 Society of Photo-Optical Instrumentation Engineers (SPIE)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorSeager, Saraen_US
dc.relation.journalProceedings of SPIE--the International Society for Optical Engineeringen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dspace.orderedauthorsLawson, P. R.; Seager, S.; Stapelfeldt, K.; Brenner, M.; Lisman, D.; Siegler, N.; Unwin, S.; Warfield, K.en_US
dc.identifier.orcidhttps://orcid.org/0000-0002-6892-6948
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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