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dc.contributor.authorBuchanan, Weston P.
dc.contributor.authorde Jong, Maxim
dc.contributor.authorAgrawal, Rachana
dc.contributor.authorPetkowski, Janusz J.
dc.contributor.authorArora, Archit
dc.contributor.authorSaikia, Sarag J.
dc.contributor.authorSeager, Sara
dc.contributor.authorLonguski, James
dc.contributor.authoron behalf of the Venus Life Finder Mission Team,
dc.date.accessioned2022-07-11T14:31:09Z
dc.date.available2022-07-11T14:31:09Z
dc.date.issued2022-07-07
dc.identifier.urihttps://hdl.handle.net/1721.1/143635
dc.description.abstractMounting evidence of chemical disequilibria in the Venusian atmosphere has heightened interest in the search for life within the planet’s cloud decks. Balloon systems are currently considered to be the superior class of aerial platform for extended atmospheric sampling within the clouds, providing the highest ratio of science return to risk. Balloon-based aerial platform designs depend heavily on payload mass and target altitudes. We present options for constant- and variable-altitude balloon systems designed to carry out science operations inside the Venusian cloud decks. The Venus Life Finder (VLF) mission study proposes a series of missions that require extended in situ analysis of Venus cloud material. We provide an overview of a representative mission architecture, as well as gondola designs to accommodate a VLF instrument suite. Current architecture asserts a launch date of 30 July 2026, which would place an orbiter and entry vehicle at Venus as early as November 29 of that same year.en_US
dc.publisherMultidisciplinary Digital Publishing Instituteen_US
dc.relation.isversionofhttp://dx.doi.org/10.3390/aerospace9070363en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceMultidisciplinary Digital Publishing Instituteen_US
dc.titleAerial Platform Design Options for a Life-Finding Mission at Venusen_US
dc.typeArticleen_US
dc.identifier.citationAerospace 9 (7): 363 (2022)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
dc.identifier.mitlicensePUBLISHER_CC
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-07-08T11:55:14Z
dspace.date.submission2022-07-08T11:55:14Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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