Abstract
The Moon provides a unique environment for investigating nearby astrophysical events such as supernovae. Lunar samples retain valuable information from these events, via detectable long-lived “fingerprint” radionuclides such as \({}^{60} \hbox{Fe}\). In this work, we stepped up the development of an accelerator mass spectrometry (AMS) method for detecting \({}^{60} \hbox{Fe}\) using the HI-13 tandem accelerator at the China Institute of Atomic Energy (CIAE). Since interferences could not be sufficiently removed solely with the existing magnetic systems of the tandem accelerator and the following Q3D magnetic spectrograph, a Wien filter with a maximum voltage of \(\pm\,60\,\text {kV}\) and a maximum magnetic field of 0.3 T was installed after the accelerator magnetic systems to lower the detection background for the low abundance nuclide \({}^{60} \hbox{Fe}\). A \(1\,\upmu \text {m}\) thick Si\(_{3}\)N\(_{4}\) foil was installed in front of the Q3D as an energy degrader. For particle detection, a multi-anode gas ionization chamber was mounted at the center of the focal plane of the spectrograph. Finally, an \({}^{60} \hbox{Fe}\) sample with an abundance of \(1.125 \times 10^{-10}\) was used to test the new AMS system. These results indicate that \({}^{60} \hbox{Fe}\) can be clearly distinguished from the isobar \({}^{60} \hbox{Ni}\). The sensitivity was assessed to be better than \(4.3 \times 10^{-14}\) based on blank sample measurements lasting \(5.8\) h, and the sensitivity could, in principle, be expected to be approximately \(2.5 \times 10^{-15}\) when the data were accumulated for 100 h, which is feasible for future lunar sample measurements because the main contaminants were sufficiently separated.
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Data availability
The data that support the findings of this study are openly available in Science Data Bank at https://cstr.cn/31253.11.sciencedb.j00186.00511 and https://doi.org/10.57760/sciencedb.j00186.00511.
References
J.F. Snape, A.A. Nemchin, M.J. Whitehouse et al., The timing of basaltic volcanism at the Apollo landing sites. Geochim. Cosmochim. Ac. 266, 29–53 (2019). https://doi.org/10.1016/j.gca.2019.07.042
D. Stöffler, G. Ryder, Stratigraphy and isotope ages of lunar geologic units: Chronological standard for the inner solar system. Space Sci. Rev. 96, 9–54 (2001). https://doi.org/10.1023/A:1011937020193
H. Hiesinger, J.W. Head III., New views of lunar geoscience: an introduction and overview. Rev. Mineral. Geochem. 60, 1–81 (2006). https://doi.org/10.2138/rmg.2006.60.1
L.E. Borg, J.N. Connelly, M. Boyet et al., Chronological evidence that the Moon is either young or did not have a global magma ocean. Nature 477, 70–72 (2011). https://doi.org/10.1038/nature10328
H.-C. Tian, C. Zhang, W. Yang et al., Surges in volcanic activity on the Moon about two billion years ago. Nat. Commun. 14, 3734 (2023). https://doi.org/10.1038/s41467-023-39418-0
C.L. Li, H. Hu, M.-F. Yang et al., Characteristics of the lunar samples returned by the Chang’E-5 mission. Nat. Sci. Rev. 9, nwab188 (2022). https://doi.org/10.1093/nsr/nwab188
A. Wallner, M. Bichler, K. Buczak et al., Settling the half-life of \(^{60}\hbox{Fe}\): fundamental for a versatile astrophysical chronometer. Phys. Rev. Lett. 114, 041101 (2015). https://doi.org/10.1103/PhysRevLett.114.041101
K.M. Ostdiek, T.S. Anderson, W.K. Bauder et al., Activity measurement of 60Fe through the decay of \(^{60m}\)Co and confirmation of its half-life. Phys. Rev. C 95, 055809 (2017). https://doi.org/10.1103/PhysRevC.95.055809
C. Domingo-Pardo, I. Dillmann, T. Faestermann et al., S-process nucleosynthesis in massive stars: new results on \(^{60}\hbox{Fe}\),\(^{62}\hbox{Ni}\) and \(^{64}\hbox{Ni}\). AIP Conf. Proc. 1090, 230–237 (2009). https://doi.org/10.1063/1.3087019
S.Q. Yan, X.Y. Li, K. Nishio et al., The 59Fe (n,\(\gamma\)) \(^{60}\hbox{Fe}\) cross section from the surrogate ratio method and its effect on the \(^{60}\hbox{Fe}\) nucleosynthesis. Astrophys. J. 919, 84 (2021). https://doi.org/10.3847/1538-4357/ac12ce
M. Limongi, A. Chieffi, The nucleosynthesis of \(^{26}\)Al and \(^{60}\)Fe in solar metallicity stars extending in mass from 11 to 120 M\(\odot\): The hydrostatic and explosive contributions. Astrophys. J. 647, 483 (2006). https://doi.org/10.1086/505164
L. Fimiani, D.L. Cook, T. Faestermann et al., Interstellar \(^{60}\)Fe on the surface of the moon. Phys. Rev. Lett. 116, 151104 (2016). https://doi.org/10.1103/PhysRevLett.116.151104
K. Knie, G. Korschinek, T. Faestermann et al., Indication for supernova produced \(^{60}\)Fe activity on earth. Phys. Rev. Lett. 83, 18–21 (1999). https://doi.org/10.1103/PhysRevLett.83.18
A. Wallner, J. Feige, N. Kinoshita et al., Recent near-earth supernovae probed by global deposition of interstellar radioactive \(^{60}\)Fe. Nature 532, 69–72 (2016). https://doi.org/10.1038/nature17196
C. Fitoussi, G.M. Raisbeck, K. Knie et al., Search for supernova-produced \(^{60}\)Fe in a marine sediment. Phys. Rev. Lett. 101, 121101 (2008). https://doi.org/10.1103/PhysRevLett.101.121101
D. Koll, G. Korschinek, T. Faestermann et al., Interstellar 60Fe in Antarctica. Phys. Rev. Lett. 123, 072701 (2019). https://doi.org/10.1103/PhysRevLett.123.072701
S. Hu, H. He, J. Ji et al., A dry lunar mantle reservoir for young mare basalts of Chang’e-5. Nature 600, 49–53 (2021). https://doi.org/10.1038/s41586-021-04107-9
Q.-L. Li, Q. Zhou, Y. Liu et al., Two-billion-year-old volcanism on the moon from Chang’e-5 basalts. Nature 600, 54–58 (2021). https://doi.org/10.1038/s41586-021-04100-2
H.-C. Tian, H. Wang, Y. Chen et al., Non-KREEP origin for Chang’e-5 basalts in the Procellarum KREEP Terrane. Nature 600, 59–63 (2021). https://doi.org/10.1038/s41586-021-04119-5
X. Zeng, X. Li, J. Liu, Exotic clasts in Chang’e-5 regolith indicative of unexplored terrane on the Moon. Nat. Astron. 7, 152–159 (2023). https://doi.org/10.1038/s41550-022-01840-7
Y. Yao, C. Xiao, P. Wang et al., Instrumental neutron activation analysis of Chang’E-5 lunar regolith samples. J. Am. Chem. Soc. 144, 5478–5484 (2022). https://doi.org/10.1021/jacs.1c13604
Y. Jiang, J. Kang, S. Liao et al., Fe and Mg isotope compositions indicate a hybrid mantle source for Young Chang’E 5 mare basalts. Astrophys. J. Lett. 945, L26 (2023). https://doi.org/10.3847/2041-8213/acbd31
Y. Yao, C. Xiao, L. Zhao et al., Determination of \(^{58}\)Fe/\(^{54}\)Fe isotope ratios in Chang’E-5 lunar regolith by instrumental neutron activation analysis. Nucl. Anal. 3, 100102 (2024). https://doi.org/10.1016/j.nucana.2024.100102
X. Lu, J. Chen, Z. Ling et al., Mature lunar soils from Fe-rich and young mare basalts in the Chang’e-5 regolith samples. Nat. Astron. 7, 142–151 (2023). https://doi.org/10.1038/s41550-022-01838-1
K.N. Li, C.X. Kan, X.F. Wang et al., Practice and innovation in the operation and maintenance of HI-13 tandem accelerator for 35 years. Nuclear Techniques (in Chinese) 46, 080005 (2023). https://doi.org/10.11889/j.0253-3219.2023.hjs.46.080005
W.P. Liu, Review of the development of tandem accelerator laboratory in 35 years. Nuclear Techniques (in Chinese) 46, 080022 (2023). https://doi.org/10.11889/j.0253-3219.2023.hjs.46.080022
M. He, S. Jiang, S. Jiang et al., Development of AMS measurements and applications at the CIAE. Nucl. Instrum. Meth. Phys. Res. Sect. B 172, 87–90 (2000). https://doi.org/10.1016/S0168-583X(00)00370-0
Y.L. Dou, M. Lin, M. He et al., AMS measurement of in-situ produced cosmogenic 10Be in Loess Quartz in Luochuan. Chinese Phys. C 32 279–283 (2008). http://csnsdoc.ihep.ac.cn/article/id/en/article/id/3152caed-097e-411e-8a82-c7c4e7ac8fb2
J. Gong, C. Li, W. Wang et al., 32Si AMS measurement with \(\Delta\)E-Q3D method. Nucl. Instrum. Meth. Phys. Res. Sect. B 269, 2745–2749 (2011). https://doi.org/10.1016/j.nimb.2011.08.026
C. Li, M. He, W. Zhang et al., AMS measurement of \(^{36}\)Cl with a Q3D magnetic spectrometer at CIAE. Plasma Sci. Technol 14, 543 (2012). https://doi.org/10.1088/1009-0630/14/6/25
K.J. Dong, M. He, S.Y. Wu et al., Application of \(^{41}\)Ca tracer and its AMS measurement in CIAE. Chinese Phys. Lett. 21, 51 (2004). https://doi.org/10.1088/0256-307X/21/1/015
Z.C. Li, Y.H. Cheng, Y. Chen et al., Beijing Q3D magnetic spectrometer and its applications. Nucl. Instrum. Meth. Phys. Res. Sect. A 336, 150–161 (1993). https://doi.org/10.1016/0168-9002(93)91091-Z
C. Li, M. He, S. Jiang et al., An isobar separation method with Q3D magnetic spectrometer for AMS. Nucl. Instrum. Meth. Phys. Res. Sect. A 622, 536–541 (2010). https://doi.org/10.1016/j.nima.2010.07.065
Y. Zhang, M. He, F. Wang et al., Developing the measurement of \(^{60}\)Fe with AMS at CIAE. Nucl. Instrum. Meth. Phys. Res. Sect. B 438, 156–161 (2019). https://doi.org/10.1016/j.nimb.2018.05.020
F.F. Wang, M. He, Y.X. Zhang et al., \(^{60}\)Fe Sample preparation and extraction method for measurement with accelerator mass spectrometry. J. Isotopes 32, 103 (2019). https://doi.org/10.7538/tws.2018.youxian.008. (in Chinese)
Acknowledgements
The authors thank the staff of the HI-13 tandem accelerator for smooth operation of the machine.
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All authors contributed to the study conception and design. Yong-Shou Chen, Wei-Ping Liu, Bing Guo, Sheng-Quan Yan, Yun-Ju Li, You-Bao Wang, Zhi-Hong Li, Yang-Ping Shen and Ming He contributed to the conceptualization and methodology. Material preparation, data collection and analysis were performed by Yang Zhang, Sheng-Quan Yan, Ming He, Qing-Zhang Zhao, Wen-Hui Zhang, Chao-Xin Kan, Jian-Ming Zhou, Kang-Ning Li, Xiao-Fei Wang, Jian-Cheng Liu, Zhao-Hua Peng, Zhuo Liang, Ai-Ling Li, Jian Zheng, Qi-Wen Fan, Ding Nan, Wei Nan, Yu-Qiang Zhang, Jia-Ying-Hao Li, Jun-Wen Tian, Jiang-Lin Hou, Chang-Xin Guo, Zhi-Cheng Zhang, Ming-Hao Zhu, Yu-Wen Chen, Yu-Chen Jiang, Tao Tian, Jin-Long Ma, Yi-Hui Liu, Jing-Yu Dong, Run-Long Liu and Mei-Yue-Nan Ma. The first draft of the manuscript was written by Yang Zhang and all authors commented on previous versions of the manuscript. All authors read and approved the final manuscript.
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This work was supported by the National Natural Science Foundation of China (Nos. 12125509, 12222514, 11961141003, and 12005304), National Key Research and Development Project (No. 2022YFA1602301), CAST Young Talent Support Plan, the CNNC Science Fund for Talented Young Scholars Continuous support for basic scientific research projects.
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Zhang, Y., Yan, SQ., He, M. et al. Stepped-up development of accelerator mass spectrometry method for the detection of 60Fe with the HI-13 tandem accelerator. NUCL SCI TECH 35, 77 (2024). https://doi.org/10.1007/s41365-024-01453-x
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DOI: https://doi.org/10.1007/s41365-024-01453-x