Nonmagnetic framboid and associated iron nanoparticles with a space-weathered feature from asteroid Ryugu

Author:

Kimura YukiORCID,Kato Takeharu,Anada SatoshiORCID,Yoshida Ryuji,Yamamoto KazuoORCID,Tanigaki ToshiakiORCID,Akashi Tetsuya,Kasai Hiroto,Kurosawa KosukeORCID,Nakamura Tomoki,Noguchi TakaakiORCID,Sato MasahikoORCID,Matsumoto ToruORCID,Morita Tomoyo,Kikuiri Mizuha,Amano KanaORCID,Kagawa Eiichi,Yada ToruORCID,Nishimura Masahiro,Nakato AikoORCID,Miyazaki AkikoORCID,Yogata KasumiORCID,Abe Masanao,Okada TatsuakiORCID,Usui TomohiroORCID,Yoshikawa Makoto,Saiki Takanao,Tanaka Satoshi,Terui Fuyuto,Nakazawa SatoruORCID,Yurimoto HisayoshiORCID,Okazaki Ryuji,Yabuta HikaruORCID,Naraoka Hiroshi,Sakamoto KanakoORCID,Watanabe Sei-ichiroORCID,Tsuda Yuichi,Tachibana ShogoORCID

Abstract

AbstractExtraterrestrial minerals on the surface of airless Solar System bodies undergo gradual alteration processes known as space weathering over long periods of time. The signatures of space weathering help us understand the phenomena occurring in the Solar System. However, meteorites rarely retain the signatures, making it impossible to study the space weathering processes precisely. Here, we examine samples retrieved from the asteroid Ryugu by the Hayabusa2 spacecraft and discover the presence of nonmagnetic framboids through electron holography measurements that can visualize magnetic flux. Magnetite particles, which normally provide a record of the nebular magnetic field, have lost their magnetic properties by reduction via a high-velocity (>5 km s–1) impact of a micrometeoroid with a diameter ranging from 2 to 20 μm after destruction of the parent body of Ryugu. Around these particles, thousands of metallic-iron nanoparticles with a vortex magnetic domain structure, which could have recorded a magnetic field in the impact event, are found. Through measuring the remanent magnetization of the iron nanoparticles, future studies are expected to elucidate the nature of the nebular/interplanetary magnetic fields after the termination of aqueous alteration in an asteroid.

Funder

MEXT | Japan Society for the Promotion of Science

Publisher

Springer Science and Business Media LLC

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