Characteristics of natural remanence records in fine-grained particles returned from asteroid Ryugu
Masahiko Sato, Yuki Kimura, Tadahiro Hatakeyama, Tomoki Nakamura, Satoshi Okuzumi, Sei-ichiro Watanabe, Seiji Sugita, Satoshi Tanaka, Shogo Tachibana, Hisayoshi Yurimoto, Takaaki Noguchi, Ryuji Okazaki, Hikaru Yabuta, Hiroshi Naraoka, Kanako Sakamoto, Toru Yada

TL;DR
This study analyzed the magnetic remanence in 28 particles from asteroid Ryugu, revealing stable and unstable NRM components, and suggesting aqueous alteration as a key process in remanence acquisition, enhancing understanding of primitive solar system materials.
Contribution
It significantly expands the sample size for NRM analysis in Ryugu particles and provides new insights into the mechanisms of remanence acquisition in asteroid materials.
Findings
Some particles show stable NRM components, others do not.
NRM directions are spatially inhomogeneous within particles.
Remanence likely acquired before solidification via aqueous alteration.
Abstract
Particles collected from the asteroid Ryugu by the Hayabusa2 spacecraft offer a unique opportunity to investigate the magnetic record of the primitive solar system, as any terrestrial magnetic contamination is minimal and can be accounted for. In previous studies, stepwise alternating field demagnetization (AFD) measurements of natural remanent magnetization (NRM) records have been conducted on seven Ryugu particles. However, due to the limited number of samples, there is no consensus regarding the interpretation of the results of these measurements. To address this problem, we performed stepwise AFD measurements of the NRM on 28 Ryugu particles. Twenty-three of the particles exhibited one or two stable NRM components, whereas the remaining five did not. Isothermal remanent magnetization-based paleointensity values derived from stable NRM components varied by more than one order of…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Astro and Planetary Science · Planetary Science and Exploration
