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dc.contributor.authorZuber, Maria T.
dc.contributor.authorPark, Ryan S.
dc.contributor.authorElkins-Tanton, Linda T.
dc.contributor.authorBell, J. F.
dc.contributor.authorBruvold, Kristoffer N.
dc.contributor.authorBercovici, David
dc.contributor.authorBills, Bruce G.
dc.contributor.authorBinzel, Richard P.
dc.contributor.authorJaumann, R.
dc.contributor.authorMarchi, Simone
dc.contributor.authorRaymond, Carol A.
dc.contributor.authorRoatsch, T.
dc.contributor.authorWang, Charles C.
dc.contributor.authorWeiss, Benjamin P.
dc.contributor.authorWenkert, Daniel
dc.contributor.authorWieczorek, Mark A.
dc.date.accessioned2022-10-24T12:28:07Z
dc.date.available2022-10-24T12:28:07Z
dc.date.issued2022-10-18
dc.identifier.urihttps://hdl.handle.net/1721.1/145937
dc.description.abstractAbstract The objective of the NASA Psyche mission gravity science investigation is to map the mass distribution within asteroid (16) Psyche to elucidate interior structure and to resolve the question of whether this metal-rich asteroid represents a remnant metal core or whether it is a primordial body that never melted. Measurements of gravity will be obtained via the X-band telecommunication system on the Psyche spacecraft, collected from progressively lower mapping altitudes. Orbital gravity will allow an estimate of G M $GM$ to better than 0.001 km3 s−2. A spherical harmonic model of gravity to degree and order 10 will be achievable and, in concert with spherical harmonic data sets from topography and magnetometry, as well as surface composition data, will provide information regarding the spatial and radial distribution of mass that will be used to constrain the origin and evolution of (16) Psyche.en_US
dc.publisherSpringer Netherlandsen_US
dc.relation.isversionofhttps://doi.org/10.1007/s11214-022-00905-3en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer Netherlandsen_US
dc.titleThe Psyche Gravity Investigationen_US
dc.typeArticleen_US
dc.identifier.citationSpace Science Reviews. 2022 Oct 18;218(8):57en_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.updated2022-10-23T03:20:36Z
dc.language.rfc3066en
dc.rights.holderThe Author(s)
dspace.embargo.termsN
dspace.date.submission2022-10-23T03:20:36Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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