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dc.contributor.authorHercik, David
dc.contributor.authorAuster, Hans-Ulrich
dc.contributor.authorConstantinescu, Dragos
dc.contributor.authorBlum, Jürgen
dc.contributor.authorFornaçon, Karl-Heinz
dc.contributor.authorFujimoto, Masaki
dc.contributor.authorGebauer, Kathrin
dc.contributor.authorGrundmann, Jan-Thimo
dc.contributor.authorGüttler, Carsten
dc.contributor.authorHillenmaier, Olaf
dc.contributor.authorHo, Tra-Mi
dc.contributor.authorHördt, Andreas
dc.contributor.authorKrause, Christian
dc.contributor.authorKührt, Ekkehard
dc.contributor.authorLorda, Laurence
dc.contributor.authorMatsuoka, Ayako
dc.contributor.authorMotschmann, Uwe
dc.contributor.authorMoussi-Soffys, Aurélie
dc.contributor.authorRichter, Ingo
dc.contributor.authorSasaki, Kaname
dc.contributor.authorScholten, Frank
dc.contributor.authorStoll, Bernd
dc.contributor.authorWeiss, Benjamin P
dc.contributor.authorWolff, Friederike
dc.contributor.authorGlassmeier, Karl-Heinz
dc.date.accessioned2021-10-27T20:30:48Z
dc.date.available2021-10-27T20:30:48Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/136097
dc.description.abstract©2020. The Authors. Observations of the magnetization state of asteroids indicate diverse properties. Values between 1.9 × 10 -6Am2/kg (Eros) and 10-2 Am2/kg (Braille) have been reported. A more detailed understanding of asteroidal magnetic properties allows far-reaching conclusions of the magnetization mechanism as well as the strength of the magnetic field of the solar system regions the asteroid formed in. The Hayabusa2 mission with its lander Mobile Asteroid Surface Scout is equipped with a magnetometer experiment, MasMag. MasMag is a state-of-the-art three-axis fluxgate magnetometer, successfully operated also on Philae, the Rosetta mission lander. MasMag has enabled, after Eros for the second time ever, to determine the magnetic field of an asteroid during descent and on-surface operations. The new observations show that Ryugu, a low-albedo C-type asteroid, has no detectable global magnetization, and any local magnetization is either small (< 10−6 Am2/kg) or on very small (subcentimeter) scales. This implies, for example, that energetic solar wind particles could reach and alter the surface unimpeded by strong asteroidal magnetic fields, such as minimagnetospheres in case of the Moon.
dc.language.isoen
dc.publisherAmerican Geophysical Union (AGU)
dc.relation.isversionof10.1029/2019JE006035
dc.rightsCreative Commons Attribution NonCommercial License 4.0
dc.rights.urihttps://creativecommons.org/licenses/by-nc/4.0/
dc.sourceAmerican Geophysical Union (AGU)
dc.titleMagnetic Properties of Asteroid (162173) Ryugu
dc.typeArticle
dc.relation.journalJournal of Geophysical Research: Planets
dc.eprint.versionFinal published version
dc.type.urihttp://purl.org/eprint/type/JournalArticle
eprint.statushttp://purl.org/eprint/status/PeerReviewed
dc.date.updated2020-05-08T14:23:35Z
dspace.orderedauthorsHercik, D; Auster, H-U; Constantinescu, D; Blum, J; Fornaçon, K-H; Fujimoto, M; Gebauer, K; Grundmann, J-T; Güttler, C; Hillenmaier, O; Ho, T-M; Hördt, A; Krause, C; Kührt, E; Lorda, L; Matsuoka, A; Motschmann, U; Moussi-Soffys, A; Richter, I; Sasaki, K; Scholten, F; Stoll, B; Weiss, BP; Wolff, F; Glassmeier, K-H
dspace.date.submission2020-05-08T14:23:39Z
mit.journal.volume125
mit.journal.issue1
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Needed


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