Modeling of Cosmogenic Cr Isotopes Produced in Lunar Rocks Compared With Existing Calculations and Measurements Article Swipe
Bailiang Liu
,
Jingnan Guo
,
Mikhail Dobynde
,
Jia Liu
,
Yingnan Zhang
,
Liping Qin
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1029/2023je008069
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.1029/2023je008069
The nucleosynthetic Cr isotope anomalies provides useful information to trace the source and origin of extraterrestrial samples, but it is usually influenced by high‐energy cosmic rays, and evaluating such effect of cosmic rays in lunar samples is especially important. Those cosmic radiation particles (primary particles) can react with lunar materials, creating many secondary particles. Both primary and secondary particles can produce cosmogenic nuclides on the Moon. Radiation Environment and Dose at the Moon (REDMoon) is a novel GEANT4 Monte‐Carlo model built to simulate the interactions of space particles with the lunar surface and subsurface content. Using this model, we simulate the production of cosmogenic Cr isotopes ( 50 Cr, 52 Cr, 53 Cr, 54 Cr) at different depths of lunar surface, and compare the contribution of different reactions generating these nuclides. The results suggest that spallation reactions are the most important process producing cosmogenic Cr isotopes. We also analyze the relationship between 53 Cr/ 52 Cr and 54 Cr/ 52 Cr predicted by our model and compare it with different Apollo samples. As previously studied, we also find an approximate linear relationship between ɛ 53 Cr and ɛ 54 Cr, where ɛ 53 Cr (or ɛ 54 Cr) is the relative deviation from the standard 53 Cr/ 52 Cr ratio (or 54 Cr/ 52 Cr ratio), normalized to 1/10,000. Furthermore, we reveal a change of this linear relationship in different depths of lunar surface. Besides, we investigate how the slopes can be influenced by exposure age and the Fe/Cr ratio. With these additional factors carefully considered, the comparison between our modeled results and the measurements is better than previous studies.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1029/2023je008069
- https://onlinelibrary.wiley.com/doi/pdfdirect/10.1029/2023JE008069
- OA Status
- hybrid
- Cited By
- 2
- References
- 43
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4392080495
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- OpenAlex ID
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https://openalex.org/W4392080495Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1029/2023je008069Digital Object Identifier
- Title
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Modeling of Cosmogenic Cr Isotopes Produced in Lunar Rocks Compared With Existing Calculations and MeasurementsWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-02-01Full publication date if available
- Authors
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Bailiang Liu, Jingnan Guo, Mikhail Dobynde, Jia Liu, Yingnan Zhang, Liping QinList of authors in order
- Landing page
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https://doi.org/10.1029/2023je008069Publisher landing page
- PDF URL
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https://onlinelibrary.wiley.com/doi/pdfdirect/10.1029/2023JE008069Direct link to full text PDF
- Open access
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://onlinelibrary.wiley.com/doi/pdfdirect/10.1029/2023JE008069Direct OA link when available
- Concepts
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Cosmogenic nuclide, Cosmic ray, Spallation, Isotope, Cosmic ray spallation, Nuclide, Isotopes of calcium, Radiochemistry, Mineralogy, Geology, Materials science, Astrobiology, Physics, Chemistry, Nuclear physics, Neutron, Ultra-high-energy cosmic rayTop concepts (fields/topics) attached by OpenAlex
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2Total citation count in OpenAlex
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2025: 1, 2024: 1Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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