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dc.contributor.authorSchönbächler, Mariaen
dc.contributor.authorFehr, Manuela A.en
dc.contributor.authorYokoyama, Tetsuyaen
dc.contributor.authorGautam, Ikshuen
dc.contributor.authorNakanishi, Naoen
dc.contributor.authorAbe, Yoshinarien
dc.contributor.authorAléon, Jérômeen
dc.contributor.authorAlexander, Conelen
dc.contributor.authorAmari, Sachikoen
dc.contributor.authorAmelin, Yurien
dc.contributor.authorBajo, Ken-ichien
dc.contributor.authorBizzarro, Martinen
dc.contributor.authorBouvier, Audreyen
dc.contributor.authorCarlson, Richard W.en
dc.contributor.authorChaussidon, Marcen
dc.contributor.authorChoi, Byeon-Gaken
dc.contributor.authorDauphas, Nicolasen
dc.contributor.authorDavis, Andrew M.en
dc.contributor.authorDi Rocco, Tommasoen
dc.contributor.authorFujiya, Wataruen
dc.contributor.authorFukai, Ryotaen
dc.contributor.authorHaba, Makiko K.en
dc.contributor.authorHibiya, Yukien
dc.contributor.authorHidaka, Hiroshien
dc.contributor.authorHomma, Hisashien
dc.contributor.authorHoppe, Peteren
dc.contributor.authorHuss, Gary R.en
dc.contributor.authorIchida, Kiyohiroen
dc.contributor.authorIizuka, Tsuyoshien
dc.contributor.authorIreland, Trevoren
dc.contributor.authorIshikawa, Akiraen
dc.contributor.authorItoh, Shoichien
dc.contributor.authorKawasaki, Noriyukien
dc.contributor.authorKita, Noriko T.en
dc.contributor.authorKitajima, Kokien
dc.contributor.authorKleine, Thorstenen
dc.contributor.authorKomatani, Shintaroen
dc.contributor.authorKrot, Alexander N.en
dc.contributor.authorLiu, Ming-Changen
dc.contributor.authorMasuda, Yukien
dc.contributor.authorMorita, Mayuen
dc.contributor.authorMotomura, Kazukoen
dc.contributor.authorMoynier, Frédéricen
dc.contributor.authorNakai, Izumien
dc.contributor.authorNagashima, Kazuhideen
dc.contributor.authorNguyen, Annen
dc.contributor.authorNittler, Larryen
dc.contributor.authorOnose, Morihikoen
dc.contributor.authorPack, Andreasen
dc.contributor.authorPark, Changkunen
dc.contributor.authorPiani, Lauretteen
dc.contributor.authorQin, Lipingen
dc.contributor.authorRussell, Saraen
dc.contributor.authorSakamoto, Naoyaen
dc.contributor.authorTafla, Laurenen
dc.contributor.authorTang, Haolanen
dc.contributor.authorTerada, Kentaroen
dc.contributor.authorTerada, Yasukoen
dc.contributor.authorUsui, Tomohiroen
dc.contributor.authorWada, Soheien
dc.contributor.authorWadhwa, Meenakshien
dc.contributor.authorWalker, Richard J.en
dc.contributor.authorYamashita, Katsuyukien
dc.contributor.authorYin, Qing-Zhuen
dc.contributor.authorYoneda, Shigekazuen
dc.contributor.authorYoung, Edward D.en
dc.contributor.authorYui, Hiroharuen
dc.contributor.authorZhang, Ai-Chengen
dc.contributor.authorNakamura, Tomokien
dc.contributor.authorNaraoka, Hiroshien
dc.contributor.authorNoguchi, Takaakien
dc.contributor.authorOkazaki, Ryujien
dc.contributor.authorSakamoto, Kanakoen
dc.contributor.authorYabuta, Hikaruen
dc.contributor.authorAbe, Masanaoen
dc.contributor.authorMiyazaki, Akikoen
dc.contributor.authorNakato, Aikoen
dc.contributor.authorNishimura, Masahiroen
dc.contributor.authorOkada, Tatsuakien
dc.contributor.authorYada, Toruen
dc.contributor.authorYogata, Kasumien
dc.contributor.authorNakazawa, Satoruen
dc.contributor.authorSaiki, Takanaoen
dc.contributor.authorTanaka, Satoshien
dc.contributor.authorTerui, Fuyutoen
dc.contributor.authorTsuda, Yuichien
dc.contributor.authorWatanabe, Sei-ichiroen
dc.contributor.authorYoshikawa, Makotoen
dc.contributor.authorTachibana, Shogoen
dc.contributor.authorYurimoto, Hisayoshien
dc.contributor.alternative伊藤, 正一ja
dc.contributor.alternative野口, 高明ja
dc.date.accessioned2025-04-25T00:25:32Z-
dc.date.available2025-04-25T00:25:32Z-
dc.date.issued2025-01-
dc.identifier.urihttp://hdl.handle.net/2433/293543-
dc.description.abstractNucleosynthetic isotope variations are powerful tracers to determine genetic relationships between meteorites and planetary bodies. They can help to link material collected by space missions to known meteorite groups. The Hayabusa 2 mission returned samples from the Cb-type asteroid (162173) Ryugu. The mineralogical, chemical, and isotopic characteristics of these samples show strong similarities to carbonaceous chondrites and in particular CI chondrites. The nucleosynthetic isotope compositions of Ryugu overlap with CI chondrites for several elements (e.g., Cr, Ti, Fe, and Zn). In contrast to these isotopes, which are of predominately supernovae origin, s-process variations in Mo isotope data are similar to those of carbonaceous chondrites, but even more s-process depleted. To further constrain the origin of this depletion and test whether this signature is also present for other s-process elements, we report Zr isotope compositions for three bulk Ryugu samples (A0106, A0106-A0107, C0108) collected from the Hayabusa 2 mission. The data are complemented with that of terrestrial rock reference materials, eucrites, and carbonaceous chondrites. The Ryugu samples are characterized by distinct ⁹⁶Zr enrichment relative to Earth, indicative of a s-process depletion. Such depletion is also observed for carbonaceous chondrites and eucrites, in line with previous Zr isotope work, but it is more extreme in Ryugu, as observed for Mo isotopes. Since s-process Zr and Mo are coupled in mainstream SiC grains, these distinct s-process variations might be due to SiC grain depletion in the analyzed materials, potentially caused by incomplete sample digestion, because the Ryugu samples were dissolved on a hotplate only to avoid high blank levels for other elements (e.g., Cr). However, local depletion of SiC grains cannot be excluded. An alternative, equally possible scenario is that aqueous alteration redistributed anomalous, s-process-depleted, Zr on a local scale, for example, into Ca-phosphates or phyllosilicates.en
dc.language.isoeng-
dc.publisherWileyen
dc.rights© 2024 The Author(s). Meteoritics & Planetary Science published by Wiley Periodicals LLC on behalf of The Meteoritical Society.en
dc.rightsThis is an open access article under the terms of the Creative Commons Attribution-NonCommercial License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.en
dc.rights.urihttp://creativecommons.org/licenses/by-nc/4.0/-
dc.titleZirconium isotope composition indicates 𝘴-process depletion in samples returned from asteroid Ryuguen
dc.typejournal article-
dc.type.niitypeJournal Article-
dc.identifier.jtitleMeteoritics & Planetary Scienceen
dc.identifier.volume60-
dc.identifier.issue1-
dc.identifier.spage3-
dc.identifier.epage16-
dc.relation.doi10.1111/maps.14279-
dc.textversionpublisher-
dc.relation.urlhttps://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.14279-
dcterms.accessRightsopen access-
dc.identifier.pissn1086-9379-
dc.identifier.eissn1945-5100-
出現コレクション:学術雑誌掲載論文等

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