月の表面に輝くガラスビーズの謎を解明(Why the moon shimmers with shiny glass beads)

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2025-06-11 ワシントン大学セントルイス校

月の表面に輝くガラスビーズの謎を解明(Why the moon shimmers with shiny glass beads)
Microscopic views of lunar volcanic glass. (Image: Katharine Robinson and G. Jeffrey Taylor, Nature Geoscience, 2014)

ワシントン大学などの研究チームは、アポロ計画で回収された月の微細ガラスビーズを分析し、約33〜36億年前の爆発的火山活動によって形成されたことを明らかにしました。ビーズは月面の火山噴火で溶岩が真空中で急冷してできたもので、NanoSIMSや電子顕微鏡による分析で、色や成分から当時の噴火様式やマグマの性質が判明しました。これは月の内部環境の変遷を示す貴重な証拠であり、月試料の科学的価値を再認識させる成果です。

<関連情報>

月の火山ガス雲の化学的性質: ガラスビーズ表面の昇華物からの制約 Lunar volcanic gas cloud chemistry: Constraints from glass bead surface sublimates

T.A. Williams, S.W. Parman, A.E. Saal, A.J. Akey, J.A. Gardener, R.C. Ogliore
Icarus  Available online: 24 April 2025
DOI:https://doi.org/10.1016/j.icarus.2025.116607

Highlights

  • Pristine 74,001 lunar glass bead surfaces host diverse vapour-deposited nanominerals.
  • The deposits primarily consist of nanopolycrystalline sphalerite ((Zn,Fe)S).
  • Thermochemical modelling supports current lunar volcanic gas composition estimates.

Abstract

Lunar pyroclastic glass beads preserve a record of physical and chemical conditions within volcanic gas clouds in the form of nanoscale minerals vapour-deposited onto their surfaces. However, the scale of these mineral deposits – less than 100 nm – has presented challenges for detailed analysis. Using SEM, TEM, APT, and NanoSIMS, we analysed pristine black glass beads from Apollo drive tube 74001 and found a sequence of sulfide deposition that directly evidences lunar gas cloud evolution. The deposits are predominantly micromound structures of nanopolycrystalline sphalerite ((Zn,Fe)S), with iron enrichment at the bead-micromound interface. Thermochemical modelling indicates that hydrogen and sulfur were major elements within the volcanic plume and ties the iron gradient to decreasing gas pressure during deposition. This pressure drop may also be consistent with our observed trend of potential δ34S depletion. Finally, Apollo 17 74220 orange beads, deposited higher in the Shorty Crater sequence, appear to lack abundant ZnS nanocrystals (Liu and Ma, 2024a), suggesting a change in vapour deposition between orange- and black-glass bead deposition. Together, our results suggest a change in eruption style over the course of a pyroclastic volcanic eruption in the Taurus-Littrow Valley.

1702地球物理及び地球化学
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