Back to Search Start Over

Magnetic Properties of Asteroid (162173) Ryugu

Authors :
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
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
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
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
Source :
American Geophysical Union (AGU)
Publication Year :
2022

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.

Details

Database :
OAIster
Journal :
American Geophysical Union (AGU)
Notes :
application/octet-stream, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1342472735
Document Type :
Electronic Resource