从小行星“龙宫”返回的样品中,锆石同位素组成表明存在s过程损耗

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Maria Schönbächler, Manuela A. Fehr, Tetsuya Yokoyama, Ikshu Gautam, Nao Nakanishi, Yoshinari Abe, Jérôme Aléon, Conel Alexander, Sachiko Amari, Yuri Amelin, Ken-ichi Bajo, Martin Bizzarro, Audrey Bouvier, Richard W. Carlson, Marc Chaussidon, Byeon-Gak Choi, Nicolas Dauphas, Andrew M. Davis, Tommaso Di Rocco, Wataru Fujiya, Ryota Fukai, Makiko K. Haba, Yuki Hibiya, Hiroshi Hidaka, Hisashi Homma, Peter Hoppe, Gary R. Huss, Kiyohiro Ichida, Tsuyoshi Iizuka, Trevor Ireland, Akira Ishikawa, Shoichi Itoh, Noriyuki Kawasaki, Noriko T. Kita, Koki Kitajima, Thorsten Kleine, Shintaro Komatani, Alexander N. Krot, Ming-Chang Liu, Yuki Masuda, Mayu Morita, Kazuko Motomura, Frédéric Moynier, Izumi Nakai, Kazuhide Nagashima, Ann Nguyen, Larry Nittler, Morihiko Onose, Andreas Pack, Changkun Park, Laurette Piani, Liping Qin, Sara Russell, Naoya Sakamoto, Lauren Tafla, Haolan Tang, Kentaro Terada, Yasuko Terada, Tomohiro Usui, Sohei Wada, Meenakshi Wadhwa, Richard J. Walker, Katsuyuki Yamashita, Qing-Zhu Yin, Shigekazu Yoneda, Edward D. Young, Hiroharu Yui, Ai-Cheng Zhang, Tomoki Nakamura, Hiroshi Naraoka, Takaaki Noguchi, Ryuji Okazaki, Kanako Sakamoto, Hikaru Yabuta, Masanao Abe, Akiko Miyazaki, Aiko Nakato, Masahiro Nishimura, Tatsuaki Okada, Toru Yada, Kasumi Yogata, Satoru Nakazawa, Takanao Saiki, Satoshi Tanaka, Fuyuto Terui, Yuichi Tsuda, Sei-ichiro Watanabe, Makoto Yoshikawa, Shogo Tachibana, Hisayoshi Yurimoto
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引用次数: 0

摘要

核合成同位素变化是确定陨石和行星体之间遗传关系的有力示踪剂。它们可以帮助将太空任务收集的材料与已知的陨石群联系起来。隼鸟2号任务从b型小行星(162173)龙宫带回了样本。这些样品的矿物学、化学和同位素特征与碳质球粒陨石,特别是CI球粒陨石具有很强的相似性。Ryugu的核合成同位素组成与CI球粒陨石在Cr、Ti、Fe和Zn等元素上有重叠。与这些主要来自超新星的同位素相比,Mo同位素数据中的s过程变化与碳质球粒陨石的s过程变化相似,但s过程更少。为了进一步确定这种耗尽的来源,并测试这种特征是否也存在于其他s过程元素中,我们报告了从隼鸟2号任务中收集的三个龙宫样品(A0106, A0106- a0107, C0108)的Zr同位素组成。这些数据与陆相岩石参考物质、绿长岩和碳质球粒陨石的数据相辅相成。Ryugu样品的特征是相对于地球具有明显的96Zr富集,表明s过程耗尽。在碳质球粒陨石和绿长岩中也观察到这种耗尽,与之前的Zr同位素工作一致,但在龙宫中更为极端,正如在Mo同位素中观察到的那样。由于s-process Zr和Mo在主流SiC晶粒中耦合,这些明显的s-process变化可能是由于分析材料中的SiC晶粒耗尽,可能是由于样品消化不完全引起的,因为Ryugu样品在热板上溶解只是为了避免其他元素(例如Cr)的高空白水平。然而,不能排除SiC颗粒的局部耗竭。另一种同样可能的情况是,含水蚀变在局部范围内将异常的、s过程耗尽的Zr重新分配为钙磷酸盐或层状硅酸盐。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Zirconium isotope composition indicates s-process depletion in samples returned from asteroid Ryugu

Zirconium isotope composition indicates s-process depletion in samples returned from asteroid Ryugu

Nucleosynthetic 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.

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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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