TY - JOUR
T1 - Ryugu particles found outside the Hayabusa2 sample container
AU - Nakato, Aiko
AU - Inada, Shiori
AU - Furuya, Shizuho
AU - Nishimura, Masahiro
AU - Yada, Toru
AU - Abe, Masanao
AU - Usui, Tomohiro
AU - Yoshida, Hideto
AU - Mikouchi, Takashi
AU - Sakamoto, Kanako
AU - Yano, Hajime
AU - Miura, Yayoi N.
AU - Takano, Yoshinori
AU - Yamanouchi, Shinji
AU - Okazaki, Ryuji
AU - Sawada, Hirotaka
AU - Tachibana, Shogo
N1 - Funding Information:
The authors express our gratitude to Trevor Ireland (University of Queensland) for helping the reentry capsule retrieval operation team as an international witness at Woomera, Australia. The authors thank Takuma Maruyama and Kentaro Hatakeda for their assistance during the sample container transportation from Australia to Japan and the preparation of the sample container opening. Valuable comments and suggestions from Makoto Kimura and Michael Zolensky, which improved the manuscript significantly, and the editorial handling by Kentaro Terada are deeply appreciated. This work was partly supported by JSPS Kakenhi grant (20H05846 for ST and RO).
Funding Information:
Acknowledgments The authors express our gratitude to Trevor Ireland (University of Queensland) for helping the reentry capsule retrieval operation team as an international witness at Woomera, ?ustralia. The authors thank Takuma Maruyama and Kentaro Hatakeda for their assistance during the sample container transportation from ?ustralia to Japan and the preparation of the sample container opening. Valuable comments and suggestions from Makoto Kimura and Michael Zolensky, which improved the manuscript significantly, and the editorial handling by Kentaro Terada are deeply appreciated. This work was partly supported by JSPS Kakenhi grant (20H05846 for ST and RO).
Publisher Copyright:
Copyright © 2022 The Geochemical Society of Japan.
PY - 2022
Y1 - 2022
N2 - The Hayabusa2 spacecraft explored C-type near-Earth asteroid (162173) Ryugu and returned asteroidal materials, collected during two touchdown operations, to the Earth as the first sample from carbonaceous-type asteroid. The sample container, in which ~5 g of Ryugu sample was enclosed, was safely opened in the clean chamber system with no severe exposure to the terrestrial atmosphere. In the course of preparation operation of the sample container, two dark-colored millimeter- to sub-millimeter-sized particles were found outside the sealing part of the sample container. Because they look similar to the Ryugu particles inside the sample container, the particles were named as Q particles (Q from questionable). In this study, we investigated Q particles (Q001 and Q002) mineralogically and petrographically to compare them with potential contaminants (the ablator material of the reentry capsule and fine sand particles at the capsule landing site), Ryugu sample, and CI chondrites. The Q particles show close resemblance to Ryugu sample and CI chondrites, but have no evidence of terrestrial weathering that CI chondrites experienced. We therefore conclude that the Q particles are originated from Ryugu and were expelled from the sample catcher (sample storage canister) in space prior to the enclosure operation of the sample catcher in the sample container. The most likely scenario is that the Q particles escaped from the sample catcher during the retrieval of the sample collection reflector, which was the necessary operation for the sample container closing.
AB - The Hayabusa2 spacecraft explored C-type near-Earth asteroid (162173) Ryugu and returned asteroidal materials, collected during two touchdown operations, to the Earth as the first sample from carbonaceous-type asteroid. The sample container, in which ~5 g of Ryugu sample was enclosed, was safely opened in the clean chamber system with no severe exposure to the terrestrial atmosphere. In the course of preparation operation of the sample container, two dark-colored millimeter- to sub-millimeter-sized particles were found outside the sealing part of the sample container. Because they look similar to the Ryugu particles inside the sample container, the particles were named as Q particles (Q from questionable). In this study, we investigated Q particles (Q001 and Q002) mineralogically and petrographically to compare them with potential contaminants (the ablator material of the reentry capsule and fine sand particles at the capsule landing site), Ryugu sample, and CI chondrites. The Q particles show close resemblance to Ryugu sample and CI chondrites, but have no evidence of terrestrial weathering that CI chondrites experienced. We therefore conclude that the Q particles are originated from Ryugu and were expelled from the sample catcher (sample storage canister) in space prior to the enclosure operation of the sample catcher in the sample container. The most likely scenario is that the Q particles escaped from the sample catcher during the retrieval of the sample collection reflector, which was the necessary operation for the sample container closing.
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U2 - 10.2343/geochemj.GJ22017
DO - 10.2343/geochemj.GJ22017
M3 - Article
AN - SCOPUS:85144771881
VL - 56
SP - 197
EP - 222
JO - Geochemical Journal
JF - Geochemical Journal
SN - 0016-7002
IS - 6
ER -