Journal of Evolving Space Activities
Online ISSN : 2758-1802
Crack Orientation of Boulders on Ryugu: Meridional Preference and Exfoliation
Sho SASAKI, Shiho KANDA, Hiroshi KIKUCHI, Tatsuhiro MICHIKAMI, Tomokatsu MOROTA, Chikatoshi HONDA, Hideaki MIYAMOTO, Ryodo HEMMI, Seiji SUGITA, Eri TATSUMI, Masanori KANAMARU, Sei-ichiro WATANABE, Noriyuki NAMIKI, Patrick MICHEL, Masatoshi HIRABAYASHI, Naru HIRATA, Tomoki NAKAMURA, Takaaki NOGUCHI, Takahiro HIROI, Naoya SAKATANI, Koji MATSUMOTO, Hirotomo NODA, Shingo KAMEDA, Tohru KOUYAMA, Hidehiko SUZUKI, Manabu YAMADA, Rie HONDA, Yuichiro CHO, Kazuo YOSHIOKA, Masahiko HAYAKAWA, Moe MATSUOKA, Rina NOGUCHI, Hirotaka SAWADA, Yasuhiro YOKOTA, Makoto YOSHIKAWA
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2023 Volume 1 Article ID: 89

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Abstract

Hayabusa 2 spacecraft revealed that a small carbonaceous asteroid 162173 Ryugu is a rubble pile and that its surface is covered with various sizes of boulders. A few percent of surface boulders have cracks. They are classified into straight cracks, sinuous cracks, arrested (incomplete) cracks, and complex (branched) cracks. We analyzed 538 boulders (777 cracks) and found 60% of their cracks have the meridional direction (±15deg from N-S) except complex cracks. Impacts or surface mass movement cannot have produced this preferred crack orientation. Thermal stress from solar heating would have grown cracks to meridional direction. Another feature of thermal stress – exfoliation – is also observed on the surface of small boulders of Ryugu as of Bennu.

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