Japan Geoscience Union Meeting 2021

Presentation information

[J] Oral

M (Multidisciplinary and Interdisciplinary) » M-IS Intersection

[M-IS14] Aqua planetology

Sat. Jun 5, 2021 10:45 AM - 12:15 PM Ch.02 (Zoom Room 02)

convener:Yasuhito Sekine(Earth-Life Science Insitute, Tokyo Institute of Technology), Takazo Shibuya(Japan Agency for Marine-Earth Science and Technology), Hidenori Genda(Earth-Life Science Institute, Tokyo Institute of Technology), Keisuke Fukushi(Institute of Nature & Environmental Technology, Kanazawa University), Chairperson:Takazo Shibuya(Japan Agency for Marine-Earth Science and Technology), Yasuhito Sekine(Earth-Life Science Insitute, Tokyo Institute of Technology), Keisuke Fukushi(Institute of Nature & Environmental Technology, Kanazawa University), Tomohiro Usui(Japan Aerospace Exploration Agency), Hidenori Genda(Earth-Life Science Institute, Tokyo Institute of Technology)

12:00 PM - 12:15 PM

[MIS14-06] Development of a technique for a multi-isotopic analyses of asteroid materials (small amount samples ~ 30 mg) returned by the Hayabusa2 mission

*Tetsuya Yokoyama1, Ikshu Gautam1, Yusuke Ohkuma1, Tsuyoshi Iizuka2, The Hayabusa2 initial analysis team “Isotopes and Chemistry” (1.Department of Earth and Planetary Sciences, School of Science, Tokyo Institute of Technology, 2.Department of Earth and Planetary Science, School of Science, The University of Tokyo)

Keywords:Hayabusa2, Ryugu, initial analysis, multi-isotope analysis

The sample-return mission Hayabusa2 conducted two sampling sequences that collected the surface and sub-surface materials from a C-type asteroid, Ryugu in 2019. The Sample Return Capsule (SRC) containing the collected materials was brought back to the Earth on Dec 6th of 2020. The curation team opened the SRC in a clean chamber at the curation facility of JAXA at Sagamihara, and found black chunks of rocks and dust from Ryugu, of which the total weight reached >5 g. Although the retrieved sample mass was far more than that was expected at the planning stage (0.1–1 g), each of the initial analysis team can use only limited amount of the samples (< 0.1 g) to obtain scientific data that characterize the asteroidal materials. We have developed a technique for a multi-isotopic analysis that uses ~ 30 mg of the Ryugu sample. Two terrestrial basalts (BCR-2, BHVO-2) and two CM chondrites (Murchison, Jbilet Winselwan) were chosen as the analog samples to evaluate the performance of the developed technique. The powdered sample was decomposed by a mixture of HF + HNO3 in a Teflon vessel. The sample was conditioned with HBr for the separation of Pb by anion exchange chromatography (Column-1; AG1-X8). The major element fraction of the Column-1 was dried and conditioned with 0.4 M HCl-0.5 M HF for the separation of Ti+Zr+Hf, W, and Mo (Column-2; AG1-X8). The major element fraction of the Column-2 was dried and conditioned with 6 M HCl for the separation of Fe and U (Column-3; AG1-X8), followed by the separation of Sr and Ba (Column-4; Sr-Resin), REEs (Column-5; RE-Resin), Ca (Column-6; DGA-n Resin), and Cr (Column-7; 1:1 mixture of AG50W-X8 and AG50W-X12). Finally, Mg and Ni were separated using Ni Resin (Column-8). The recovery yields of individual target elements are generally >90% during each step of the chromatography. However, these loss are not unique to our method and is always associated during any chemical separation procedures. Although extreme care was taken for handling samples but a certain loss are unavoidable such as during sample drying, pipetting and sample sticking to the Teflon beaker. The isotopic compositions of these analog samples, especially for Cr and Ti, will be reported in the presentation.