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dc.contributor.authorBanik, Indranil
dc.contributor.authorKroupa, Pavel
dc.date.accessioned2021-10-13T14:30:12Z
dc.date.available2021-10-13T14:30:12Z
dc.date.issued2019-08
dc.identifier.citationBanik , I & Kroupa , P 2019 , ' Effect of the Solar dark matter wake on planets ' , Monthly Notices of the Royal Astronomical Society , vol. 487 , no. 4 , pp. 4565-4570 . https://doi.org/10.1093/mnras/stz1601en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 276206349
dc.identifier.otherPURE UUID: 857966b9-8250-4e41-85d8-b841b73b969b
dc.identifier.otherScopus: 85070071849
dc.identifier.otherORCID: /0000-0002-4123-7325/work/101218064
dc.identifier.urihttp://hdl.handle.net/10023/24133
dc.descriptionFunding Information: IB is supported by an Alexander von Humboldt postdoctoral fellowship.en
dc.description.abstractThe Galaxy is conventionally thought to be surrounded by a massive dark matter (DM) halo. As the Sun goes through this halo, it excites a DM wake behind it. This local asymmetry in the DM distribution would gravitationally affect the motions of Solar System planets, potentially allowing the DM wake to be detected or ruled out. Hernandez (2019) recently calculated that the DM-induced perturbation to Saturn's position is 252 m net of the effect on the Sun. No such anomaly is seen in Saturn's motion despite very accurate tracking of the Cassini spacecraft, which orbited Saturn for >13 yr. Here, we revisit the calculation of how much Saturn would deviate from Keplerian motion if we fix its position and velocity at some particular time. The DM wake induces a nearly resonant perturbation whose amplitude grows almost linearly with time. We show that the Hernandez (2019) result applies only for an observing duration comparable to the ≈250 Myr period of the Sun's orbit around the Galaxy. Over a 100 yr period, the perturbation to Saturn's orbit amounts to <1 cm, which is quite consistent with existing observations. Even smaller perturbations are expected for the terrestrial planets.
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsCopyright 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.1093/mnras/stz1601.en
dc.subjectCelestial mechanicsen
dc.subjectDark matteren
dc.subjectEphemeridesen
dc.subjectGravitationen
dc.subjectPlanets and satellites: Dynamical evolution and stabilityen
dc.subjectSpace vehiclesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectSpace and Planetary Scienceen
dc.subjectAstronomy and Astrophysicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleEffect of the Solar dark matter wake on planetsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stz1601
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/1907.07130en


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