Earth, Planets and Space (Nov 2022)

Trace-element analysis of mineral grains in Ryugu rock fragment sections by synchrotron-based confocal X-ray fluorescence

  • Benjamin Bazi,
  • Pieter Tack,
  • Miles Lindner,
  • Bart Vekemans,
  • Ella De Pauw,
  • Beverley Tkalcec,
  • Frank E. Brenker,
  • Jan Garrevoet,
  • Gerald Falkenberg,
  • Hikaru Yabuta,
  • Hisayoshi Yurimoto,
  • Tomoki Nakamura,
  • Kana Amano,
  • Megumi Matsumoto,
  • Yuri Fujioka,
  • Yuma Enokido,
  • Daisuke Nakashima,
  • Masayuki Uesugi,
  • Hiroshi Naraoka,
  • Takaaki Noguchi,
  • Ryuji Okazaki,
  • Kanako Sakamoto,
  • Toru Yada,
  • Masahiro Nishimura,
  • Aiko Nakato,
  • Akiko Miyazaki,
  • Kasumi Yogata,
  • Masanao Abe,
  • Tatsuaki Okada,
  • Tomohiro Usui,
  • Makoto Yoshikawa,
  • Takanao Saiki,
  • Satoshi Tanaka,
  • Fuyuto Terui,
  • Satoru Nakazawa,
  • Shogo Tachibana,
  • Sei-ichiro Watanabe,
  • Yuichi Tsuda,
  • Laszlo Vincze

DOI
https://doi.org/10.1186/s40623-022-01726-y
Journal volume & issue
Vol. 74, no. 1
pp. 1 – 17

Abstract

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Abstract A fundamental parameter-based quantification scheme for confocal XRF was applied to sub-micron synchrotron radiation X-ray fluorescence (SR-XRF) data obtained at the beamline P06 of the Deutsches Elektronen-Synchrotron (DESY, Hamburg, Germany) from two sections C0033-01 and C0033-04 that were wet cut from rock fragment C0033 collected from Cb-type asteroid (162173) Ryugu by JAXA’s Hayabusa2 mission. Trace-element quantifications show that C0033 bulk matrix is CI-like, whereas individual mineral grains (i.e., magnetite, pyrrhotite, dolomite, apatite and breunnerite) show, depending on the respective phase, minor to strong deviations. The non-destructive nature of SR-XRF coupled with a new PyMca (a Python toolkit for XRF data analysis)-based quantification approach, performed in parallel with the synchrotron experiments, proves to be an attractive tool for the initial analysis of samples from return missions, such as Hayabusa2 and OSIRIS-REx, the latter returning material from a B-type asteroid (101955) Bennu in 2023. Graphical Abstract

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