- 著者
-
Eizo NAKAMURA
Katsura KOBAYASHI
Ryoji TANAKA
Tak KUNIHIRO
Hiroshi KITAGAWA
Christian POTISZIL
Tsutomu OTA
Chie SAKAGUCHI
Masahiro YAMANAKA
Dilan M. RATNAYAKE
Havishk TRIPATHI
Rahul KUMAR
Maya-Liliana AVRAMESCU
Hidehisa TSUCHIDA
Yusuke YACHI
Hitoshi MIURA
Masanao ABE
Ryota FUKAI
Shizuho FURUYA
Kentaro HATAKEDA
Tasuku HAYASHI
Yuya HITOMI
Kazuya KUMAGAI
Akiko MIYAZAKI
Aiko NAKATO
Masahiro NISHIMURA
Tatsuaki OKADA
Hiromichi SOEJIMA
Seiji SUGITA
Ayako SUZUKI
Tomohiro USUI
Toru YADA
Daiki YAMAMOTO
Kasumi YOGATA
Miwa YOSHITAKE
Masahiko ARAKAWA
Atsushi FUJII
Masahiko HAYAKAWA
Naoyuki HIRATA
Naru HIRATA
Rie HONDA
Chikatoshi HONDA
Satoshi HOSODA
Yu-ichi IIJIMA
Hitoshi IKEDA
Masateru ISHIGURO
Yoshiaki ISHIHARA
Takahiro IWATA
Kosuke KAWAHARA
Shota KIKUCHI
Kohei KITAZATO
Koji MATSUMOTO
Moe MATSUOKA
Tatsuhiro MICHIKAMI
Yuya MIMASU
Akira MIURA
Tomokatsu MOROTA
Satoru NAKAZAWA
Noriyuki NAMIKI
Hirotomo NODA
Rina NOGUCHI
Naoko OGAWA
Kazunori OGAWA
Chisato OKAMOTO
Go ONO
Masanobu OZAKI
Takanao SAIKI
Naoya SAKATANI
Hirotaka SAWADA
Hiroki SENSHU
Yuri SHIMAKI
Kei SHIRAI
Yuto TAKEI
Hiroshi TAKEUCHI
Satoshi TANAKA
Eri TATSUMI
Fuyuto TERUI
Ryudo TSUKIZAKI
Koji WADA
Manabu YAMADA
Tetsuya YAMADA
Yukio YAMAMOTO
Hajime YANO
Yasuhiro YOKOTA
Keisuke YOSHIHARA
Makoto YOSHIKAWA
Kent YOSHIKAWA
Masaki FUJIMOTO
Sei-ichiro WATANABE
Yuichi TSUDA
- 出版者
- The Japan Academy
- 雑誌
- Proceedings of the Japan Academy, Series B (ISSN:03862208)
- 巻号頁・発行日
- vol.98, no.6, pp.227-282, 2022-06-10 (Released:2022-06-10)
- 参考文献数
- 245
- 被引用文献数
-
90
Presented here are the observations and interpretations from a comprehensive analysis of 16 representative particles returned from the C-type asteroid Ryugu by the Hayabusa2 mission. On average Ryugu particles consist of 50% phyllosilicate matrix, 41% porosity and 9% minor phases, including organic matter. The abundances of 70 elements from the particles are in close agreement with those of CI chondrites. Bulk Ryugu particles show higher δ18O, Δ17O, and ε54Cr values than CI chondrites. As such, Ryugu sampled the most primitive and least-thermally processed protosolar nebula reservoirs. Such a finding is consistent with multi-scale H-C-N isotopic compositions that are compatible with an origin for Ryugu organic matter within both the protosolar nebula and the interstellar medium. The analytical data obtained here, suggests that complex soluble organic matter formed during aqueous alteration on the Ryugu progenitor planetesimal (several 10’s of km), <2.6 Myr after CAI formation. Subsequently, the Ryugu progenitor planetesimal was fragmented and evolved into the current asteroid Ryugu through sublimation.