Near-infrared spectral variation in Ryugu particles and implication for rapid space weathering by solar UV radiation

The 2.7 µm absorption band, represented by OH groups, in the near-infrared reflectance spectra of primitive Solar System bodies could be an indicator of the cause and degree of space weathering. We compared the absorption bands of particles sampled from the surface (chamber A) and the excavated subsurface (chamber C) on the C-type asteroid Ryugu by the JAXA Hayabusa2 mission. We developed a fitting method using multiple Gaussians to precisely calculate the band's peak position and depth, providing more reliable information on space weathering effects. We found that the chamber A particles were divided into groups Aα with shorter peak position and deeper band depth (non or poorly space weathered) and Aβ with longer peak position and shallower band depth (rich in space weathering). Chamber C particles are partly show intermediate characteristics between Aα and Aβ, which might imply weak space weathering by solar UV radiation during three months between the excavation by impact experiment and sampling by Hayabusa2. Supplementally, our preliminary experiment of UV irradiation to Ivuna meteorite showed decrease of 2.7 µm band depth and longward shift of the peak position, and further study is needed to investigate the effect of short-term UV space weathering on carbonaceous asteroids.

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Publication Details

Journal
Scientific Reports
Published
2025-04-26
DOI
https://doi.org/10.1038/s41598-025-98179-6
Citations
4
Primary Topic
Geochemistry and Geologic Mapping
Type
article
Field-Weighted Citation Impact
9.92

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article

Near-infrared spectral variation in Ryugu particles and implication for rapid space weathering by solar UV radiation

Jean‐Pierre Bibring, Y. Sugiyama, T. Hiroi, T. Ojima et al.
4 citations
Scientific Reports
Geochemistry and Geologic Mapping
9.92
article

Near-infrared spectral variation in Ryugu particles and implication for rapid space weathering by solar UV radiation

Jean‐Pierre Bibring, Y. Sugiyama, T. Hiroi, T. Ojima, Tania Le Pivert-Jolivet, Vincent Hamm, Kazuhide Nagashima, Lucie Riu, M. Nishimura, H. Kaiden, Masanao Abe, Shuhei Furukawa, Tomohiro Usui, Yuya Hitomi, Toru Yada, Yoshiya Egashira, A. Miyazaki, Rui Tahara, Rei Kanemaru, D. Loizeau, Kentaro Hatakeda, Kasumi Yogata, K. Kumagai, Atsushi Nakano, R. Brunetto, C. Pilorget, T. Okada, S. Sasaki
article en
4 citations

Abstract

The 2.7 µm absorption band, represented by OH groups, in the near-infrared reflectance spectra of primitive Solar System bodies could be an indicator of the cause and degree of space weathering. We compared the absorption bands of particles sampled from the surface (chamber A) and the excavated subsurface (chamber C) on the C-type asteroid Ryugu by the JAXA Hayabusa2 mission. We developed a fitting method using multiple Gaussians to precisely calculate the band's peak position and depth, providing more reliable information on space weathering effects. We found that the chamber A particles were divided into groups Aα with shorter peak position and deeper band depth (non or poorly space weathered) and Aβ with longer peak position and shallower band depth (rich in space weathering). Chamber C particles are partly show intermediate characteristics between Aα and Aβ, which might imply weak space weathering by solar UV radiation during three months between the excavation by impact experiment and sampling by Hayabusa2. Supplementally, our preliminary experiment of UV irradiation to Ivuna meteorite showed decrease of 2.7 µm band depth and longward shift of the peak position, and further study is needed to investigate the effect of short-term UV space weathering on carbonaceous asteroids.

Scientific ReportsVol. 15(1)
Bunkyo University (JP), Institut Universitaire de France (FR), The Graduate University for Advanced Studies, SOKENDAI (JP), Brown University (US), Japan Aerospace Exploration Agency (JP), National Institute of Polar Research (JP), European Space Astronomy Centre (ES), Instituto de Astrofísica de Canarias (ES), Institute of Space and Astronautical Science (JP), Naval Hospital Yokosuka Japan (JP), The University of Tokyo (JP), The University of Osaka (JP)
Centre National d’Etudes Spatiales
Climate action
Openalex Percentile: Top 2%
Geochemistry and Geologic Mapping
9.92
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