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dc.contributor.authorGenova, Antonio
dc.contributor.authorGoossens, Sander
dc.contributor.authorMazarico, Erwan
dc.contributor.authorLemoine, Frank G.
dc.contributor.authorNeumann, Gregory A.
dc.contributor.authorKuang, Weijia
dc.contributor.authorSabaka, Terence J.
dc.contributor.authorHauck, Steven A. II
dc.contributor.authorSmith, David Edmund
dc.contributor.authorSolomon, Sean C.
dc.contributor.authorZuber, Maria
dc.date.accessioned2020-05-15T14:02:55Z
dc.date.available2020-05-15T14:02:55Z
dc.date.issued2019-04
dc.identifier.issn0094-8276
dc.identifier.issn1944-8007
dc.identifier.urihttps://hdl.handle.net/1721.1/125259
dc.description.abstractGeodetic analysis of radio tracking measurements of the MErcury Surface, Space ENvironment, GEochemistry, and Ranging spacecraft while in orbit about Mercury has yielded new estimates for the planet's gravity field, tidal Love number, and pole coordinates. The derived right ascension (α = 281.0082° ± 0.0009°; all uncertainties are 3 standard deviations) and declination (δ = 61.4164° ± 0.0003°) of the spin pole place Mercury in the Cassini state. Confirmation of the equilibrium state with an estimated mean (whole planet) obliquity ϵ of 1.968 ± 0.027 arcmin enables the confident determination of the planet's normalized polar moment of inertia (0.333 ± 0.005), which indicates a high degree of internal differentiation. Internal structure models generated by a Markov Chain Monte Carlo process and consistent with the geodetic constraints possess a solid inner core with a radius (ric) between 0.3 and 0.7 that of the outer core (roc).en_US
dc.language.isoen
dc.publisherAmerican Geophysical Union (AGU)en_US
dc.relation.isversionof10.1029/2018GL081135en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/en_US
dc.sourcePMCen_US
dc.titleGeodetic Evidence That Mercury Has A Solid Inner Coreen_US
dc.typeArticleen_US
dc.identifier.citationGenova, Antonio, et al. "Geodetic Evidence That Mercury Has A Solid Inner Core." Geophysical Research Letters 46:7(April 2019): 3625–3633 © 2019 Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.relation.journalGeophysical Research Lettersen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2020-05-08T15:43:19Z
dspace.date.submission2020-05-08T15:43:21Z
mit.journal.volume46en_US
mit.journal.issue7en_US
mit.licenseOPEN_ACCESS_POLICY
mit.metadata.statusComplete


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