Magnetic Properties of Asteroid (162173) Ryugu

Hercik, David ORCIDiD
Auster, Hans-Ulrich ORCIDiD
Constantinescu, Dragos ORCIDiD
Blum, Jürgen
Fornaçon, Karl-Heinz
Fujimoto, Masaki
Gebauer, Kathrin
Grundmann, Jan-Thimo ORCIDiD
Güttler, Carsten ORCIDiD
Hillenmaier, Olaf
Ho, Tra-Mi
Hördt, Andreas ORCIDiD
Krause, Christian
Kührt, Ekkehard
Lorda, Laurence
Matsuoka, Ayako ORCIDiD
Motschmann, Uwe ORCIDiD
Moussi-Soffys, Aurélie
Richter, Ingo ORCIDiD
Sasaki, Kaname ORCIDiD
Scholten, Frank ORCIDiD
Stoll, Bernd
Weiss, Benjamin P.
Wolff, Friederike ORCIDiD
Glassmeier, Karl-Heinz ORCIDiD

DOI: https://doi.org/10.1029/2019JE006035
Persistent URL: http://resolver.sub.uni-goettingen.de/purl?gldocs-11858/9475
Hercik, David; Auster, Hans-Ulrich; Constantinescu, Dragos; Blum, Jürgen; Fornaçon, Karl-Heinz; Fujimoto, Masaki; Gebauer, Kathrin; Grundmann, Jan-Thimo; Güttler, Carsten; Hillenmaier, Olaf; Ho, Tra-Mi; Hördt, Andreas; Krause, Christian; Kührt, Ekkehard; Lorda, Laurence; Matsuoka, Ayako; Motschmann, Uwe; Moussi-Soffys, Aurélie; Richter, Ingo; Sasaki, Kaname; Scholten, Frank; Stoll, Bernd; Weiss, Benjamin P.; Wolff, Friederike; Glassmeier, Karl-Heinz, 2020: Magnetic Properties of Asteroid (162173) Ryugu. In: Journal of Geophysical Research: Planets, 125, 1, DOI: https://doi.org/10.1029/2019JE006035. 

Abstract

Observations of the magnetization state of asteroids indicate diverse properties. Values between 1.9  × 10 −6 Am 2/kg (Eros) and 10 −2 Am 2/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 Am 2/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.