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dc.contributor.authorMazarico, Erwan
dc.contributor.authorGoossens, Sander
dc.contributor.authorLemoine, Frank G.
dc.contributor.authorNeumann, Gregory A.
dc.contributor.authorGenova, Antonio
dc.contributor.authorZuber, Maria
dc.contributor.authorSmith, David Edmund
dc.date.accessioned2018-10-25T16:04:17Z
dc.date.available2018-10-25T16:04:17Z
dc.date.issued2018-01
dc.date.submitted2017-08
dc.identifier.issn2041-1723
dc.identifier.urihttp://hdl.handle.net/1721.1/118777
dc.description.abstractThe NASA MESSENGER mission explored the innermost planet of the solar system and obtained a rich data set of range measurements for the determination of Mercury's ephemeris. Here we use these precise data collected over 7 years to estimate parameters related to general relativity and the evolution of the Sun. These results confirm the validity of the strong equivalence principle with a significantly refined uncertainty of the Nordtvedt parameter η = (-6.6 ± 7.2) × 10⁻⁵. By assuming a metric theory of gravitation, we retrieved the post-Newtonian parameter β = 1 + (-1.6 ± 1.8) × 10⁻⁵ and the Sun's gravitational oblateness, J₂⊙ = (2.246 ± 0.022) × 10⁻⁷. Finally, we obtain an estimate of the time variation of the Sun gravitational parameter, GM⊙/ GM⊙ = (-6.13 ± 1.47) × 10⁻¹⁴, which is consistent with the expected solar mass loss due to the solar wind and interior processes. This measurement allows us to constrain |G'|G to be < 4 × 10⁻¹⁴ per year.en_US
dc.publisherNature Publishing Groupen_US
dc.relation.isversionofhttp://dx.doi.org/10.1038/S41467-017-02558-1en_US
dc.rightsCreative Commons Attribution 4.0 International Licenseen_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.sourceNatureen_US
dc.titleSolar system expansion and strong equivalence principle as seen by the NASA MESSENGER missionen_US
dc.typeArticleen_US
dc.identifier.citationGenova, Antonio et al. “Solar System Expansion and Strong Equivalence Principle as Seen by the NASA MESSENGER Mission.” Nature Communications 9, 1 (January 2018): 289 © 2018 The Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.contributor.mitauthorGenova, Antonio
dc.contributor.mitauthorSmith, David E.
dc.contributor.mitauthorZuber, Maria
dc.relation.journalNature Communicationsen_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.updated2018-10-05T14:01:02Z
dspace.orderedauthorsGenova, Antonio; Mazarico, Erwan; Goossens, Sander; Lemoine, Frank G.; Neumann, Gregory A.; Smith, David E.; Zuber, Maria T.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-5584-492X
dc.identifier.orcidhttps://orcid.org/0000-0003-2652-8017
mit.licensePUBLISHER_CCen_US


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