Chemical Composition of Metallic Iron Spherules in the Chang'e-5 Lunar Soil.

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Title: Chemical Composition of Metallic Iron Spherules in the Chang'e-5 Lunar Soil.
Authors: Sorokin, E. M.1 (AUTHOR) egorgeohim@ya.ru, Gerasimov, M. V.2 (AUTHOR), Shklover, V. Ya.3 (AUTHOR), Bondarev, A. V.3 (AUTHOR)
Source: Geochemistry International. Mar2026, Vol. 64 Issue 3, p163-181. 19p.
Subject Terms: *Lunar soil, *Siderophile elements, *Metal nanoparticles, *Moon, *Electron microscopy
Abstract: Nanophase iron metal (npFe0) spherules ranging in size from a few to hundreds of nanometers are a significant component of the regolith of the Moon and other airless bodies affecting the spectrum of electromagnetic wave reflection. Electron microscopy was used to study nanospherules on the surface and within the volume of agglutinate particles from the lunar regolith of Rümker Mons returned to the Earth by the Chang'e-5 mission. The glass hosting the npFe0 spherules was characterized by a noticeable oxygen depletion compared with the surrounding unmelted minerals. The oxygen deficiency of the glass contributed to the formation of npFe0 and the reduction of elements with low affinity for oxygen, in particular, siderophile elements and sulfur. The spherules were enriched in siderophile elements, including Ni and P, and S relative to the host glass. It can be hypothesized that the increased contents of siderophile elements and sulfur are due to the sorption of their reduced species by iron spherules formed in the glass during active mixing of boiling melt produced by a high-speed impact. The feeding glass zone from which these elements were sorbed was estimated to be up to 3–4 radii of the spherules. Thus, npFe0 spherules can act as a kind of repository for siderophile elements and sulfur or as their carrier, when the spherules were ejected into the impact-related vapor cloud. [ABSTRACT FROM AUTHOR]
Database: Energy & Power Source
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DbLabel: Energy & Power Source
An: 192725277
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  Label: Title
  Group: Ti
  Data: Chemical Composition of Metallic Iron Spherules in the Chang'e-5 Lunar Soil.
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  Data: <searchLink fieldCode="AR" term="%22Sorokin%2C+E%2E+M%2E%22">Sorokin, E. M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> egorgeohim@ya.ru</i><br /><searchLink fieldCode="AR" term="%22Gerasimov%2C+M%2E+V%2E%22">Gerasimov, M. V.</searchLink><relatesTo>2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Shklover%2C+V%2E+Ya%2E%22">Shklover, V. Ya.</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Bondarev%2C+A%2E+V%2E%22">Bondarev, A. V.</searchLink><relatesTo>3</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22Geochemistry+International%22">Geochemistry International</searchLink>. Mar2026, Vol. 64 Issue 3, p163-181. 19p.
– Name: Subject
  Label: Subject Terms
  Group: Su
  Data: *<searchLink fieldCode="DE" term="%22Lunar+soil%22">Lunar soil</searchLink><br />*<searchLink fieldCode="DE" term="%22Siderophile+elements%22">Siderophile elements</searchLink><br />*<searchLink fieldCode="DE" term="%22Metal+nanoparticles%22">Metal nanoparticles</searchLink><br />*<searchLink fieldCode="DE" term="%22Moon%22">Moon</searchLink><br />*<searchLink fieldCode="DE" term="%22Electron+microscopy%22">Electron microscopy</searchLink>
– Name: Abstract
  Label: Abstract
  Group: Ab
  Data: Nanophase iron metal (npFe0) spherules ranging in size from a few to hundreds of nanometers are a significant component of the regolith of the Moon and other airless bodies affecting the spectrum of electromagnetic wave reflection. Electron microscopy was used to study nanospherules on the surface and within the volume of agglutinate particles from the lunar regolith of Rümker Mons returned to the Earth by the Chang'e-5 mission. The glass hosting the npFe0 spherules was characterized by a noticeable oxygen depletion compared with the surrounding unmelted minerals. The oxygen deficiency of the glass contributed to the formation of npFe0 and the reduction of elements with low affinity for oxygen, in particular, siderophile elements and sulfur. The spherules were enriched in siderophile elements, including Ni and P, and S relative to the host glass. It can be hypothesized that the increased contents of siderophile elements and sulfur are due to the sorption of their reduced species by iron spherules formed in the glass during active mixing of boiling melt produced by a high-speed impact. The feeding glass zone from which these elements were sorbed was estimated to be up to 3–4 radii of the spherules. Thus, npFe0 spherules can act as a kind of repository for siderophile elements and sulfur or as their carrier, when the spherules were ejected into the impact-related vapor cloud. [ABSTRACT FROM AUTHOR]
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RecordInfo BibRecord:
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    Identifiers:
      – Type: doi
        Value: 10.1134/S0016702925600968
    Languages:
      – Code: eng
        Text: English
    PhysicalDescription:
      Pagination:
        PageCount: 19
        StartPage: 163
    Subjects:
      – SubjectFull: Lunar soil
        Type: general
      – SubjectFull: Siderophile elements
        Type: general
      – SubjectFull: Metal nanoparticles
        Type: general
      – SubjectFull: Moon
        Type: general
      – SubjectFull: Electron microscopy
        Type: general
    Titles:
      – TitleFull: Chemical Composition of Metallic Iron Spherules in the Chang'e-5 Lunar Soil.
        Type: main
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            NameFull: Sorokin, E. M.
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            NameFull: Gerasimov, M. V.
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            NameFull: Shklover, V. Ya.
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            NameFull: Bondarev, A. V.
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          Dates:
            – D: 01
              M: 03
              Text: Mar2026
              Type: published
              Y: 2026
          Identifiers:
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              Value: 00167029
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              Value: 64
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              Value: 3
          Titles:
            – TitleFull: Geochemistry International
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