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dc.contributor.authorLevison, Harold F
dc.contributor.authorOlkin, Catherine B
dc.contributor.authorNoll, Keith S
dc.contributor.authorMarchi, Simone
dc.contributor.authorBell III, James F
dc.contributor.authorBierhaus, Edward
dc.contributor.authorBinzel, Richard
dc.contributor.authorBottke, William
dc.contributor.authorBritt, Dan
dc.contributor.authorBrown, Michael
dc.contributor.authorBuie, Marc
dc.contributor.authorChristensen, Phil
dc.contributor.authorEmery, Joshua
dc.contributor.authorGrundy, Will
dc.contributor.authorHamilton, Victoria E
dc.contributor.authorHowett, Carly
dc.contributor.authorMottola, Stefano
dc.contributor.authorPätzold, Martin
dc.contributor.authorReuter, Dennis
dc.contributor.authorSpencer, John
dc.contributor.authorStatler, Thomas S
dc.contributor.authorStern, S Alan
dc.contributor.authorSunshine, Jessica
dc.contributor.authorWeaver, Harold
dc.contributor.authorWong, Ian
dc.date.accessioned2023-02-08T19:01:15Z
dc.date.available2023-02-08T19:01:15Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/147983
dc.description.abstract<jats:title>Abstract</jats:title> <jats:p>The Lucy Mission is a NASA Discovery-class mission to send a highly capable and robust spacecraft to investigate seven primitive bodies near both the L<jats:sub>4</jats:sub> and L<jats:sub>5</jats:sub> Lagrange points with Jupiter: the Jupiter Trojan asteroids. These planetesimals from the outer planetary system have been preserved since early in solar system history. The Lucy mission will fly by and extensively study a diverse selection of Trojan asteroids, including all the recognized taxonomic classes, a collisional family member, and a near equal-mass binary. It will visit objects with diameters ranging from roughly 1 km to 100 km. The payload suite consists of a color camera and infrared imaging spectrometer, a high-resolution panchromatic imager, and a thermal infrared spectrometer. Additionally, two spacecraft subsystems will also contribute to the science investigations: the terminal tracking cameras will supplement imaging during closest approach and the telecommunication subsystem will be used to measure the mass of the Trojans. The science goals are derived from the 2013 Planetary Decadal Survey and include determining the surface composition, assessing the geology, determining the bulk properties, and searching for satellites and rings.</jats:p>en_US
dc.language.isoen
dc.publisherAmerican Astronomical Societyen_US
dc.relation.isversionof10.3847/PSJ/ABF840en_US
dc.rightsCreative Commons Attribution 4.0 International licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceIOP Publishingen_US
dc.titleLucy Mission to the Trojan Asteroids: Science Goalsen_US
dc.typeArticleen_US
dc.identifier.citationLevison, Harold F, Olkin, Catherine B, Noll, Keith S, Marchi, Simone, Bell III, James F et al. 2021. "Lucy Mission to the Trojan Asteroids: Science Goals." The Planetary Science Journal, 2 (5).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.relation.journalThe Planetary Science Journalen_US
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.updated2023-02-08T18:53:16Z
dspace.orderedauthorsLevison, HF; Olkin, CB; Noll, KS; Marchi, S; Bell III, JF; Bierhaus, E; Binzel, R; Bottke, W; Britt, D; Brown, M; Buie, M; Christensen, P; Emery, J; Grundy, W; Hamilton, VE; Howett, C; Mottola, S; Pätzold, M; Reuter, D; Spencer, J; Statler, TS; Stern, SA; Sunshine, J; Weaver, H; Wong, Ien_US
dspace.date.submission2023-02-08T18:53:19Z
mit.journal.volume2en_US
mit.journal.issue5en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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