Abstract
Nanophase iron particles (npFe0) are generated on the surface of airless bodies by space weathering and can alter surficial optical properties substantially. However, the details of their formation pathways are still unclear. Here we use impact glasses returned from the Moon by Chang’e-5 to distinguish the relative contributions of solar wind irradiation and (micro)meteorites impacts to the production of different-sized npFe0. We show that solar wind irradiation can solely produce small npFe0, via implantation of solar wind ions into the topmost grain surfaces. On the other hand, (micro)meteorite impacts produce directly large npFe0 in melts, through impact-triggered disproportionation reaction or thermal decomposition. These nanoparticles are also capable to further coalesce into micrometre-sized Fe0 particles during impacts. These findings can help in predicting the space-weathering behaviour of regions exposed to different space environments.
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All data supporting this study are presented in the paper and its Supplementary Information. Source data for Figs. 1–4 are available via figshare at https://doi.org/10.6084/m9.figshare.25683804 (ref. 55).
References
Pieters, C. M. et al. Space weathering on airless bodies: resolving a mystery with lunar samples. Meteorit. Planet. Sci. 35, 1101–1107 (2000).
Taylor, L. A., Pieters, C. M., Keller, L. P., Morris, R. V. & McKay, D. S. Lunar mare soils: space weathering and the major effects of surface‐correlated nanophase Fe. J. Geophys. Res. Planets 106, 27985–27999 (2001).
Sasaki, S., Nakamura, K., Hamabe, Y., Kurahashi, E. & Hiroi, T. Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering. Nature 410, 555–557 (2001).
Hapke, B. Space weathering from Mercury to the asteroid belt. J. Geophys. Res. Planets 106, 10039–10073 (2001).
Pieters, C. M. & Noble, S. K. Space weathering on airless bodies. J. Geophys. Res. Planets 121, 1865–1884 (2016).
Noguchi, T. et al. Incipient space weathering observed on the surface of Itokawa dust particles. Science 333, 1121–1125 (2011).
Lucey, P. G. & Riner, M. A. The optical effects of small iron particles that darken but do not redden: evidence of intense space weathering on Mercury. Icarus 212, 451–462 (2011).
Noble, S. K., Pieters, C. M. & Keller, L. P. An experimental approach to understanding the optical effects of space weathering. Icarus 192, 629–642 (2007).
Chapman, C. R. Space weathering of asteroid surfaces. Annu. Rev. Earth Planet. Sci. 32, 539–567 (2004).
Pieters, C. M. et al. Distinctive space weathering on Vesta from regolith mixing processes. Nature 491, 79–82 (2012).
Li, C. et al. Impact-driven disproportionation origin of nanophase iron particles in Chang’e-5 lunar soil sample. Nat. Astron. 6, 1156–1162 (2022).
Lu, X. J. et al. Mature lunar soils from Fe-rich and young mare basalts in the Chang’e-5 regolith samples. Nat. Astron. 7, 142–151 (2022).
Tai Udovicic, C. J., Costello, E. S., Ghent, R. R. & Edwards, C. S. New constraints on the lunar optical space weathering rate. Geophys. Res. Lett. 48, e2020GL092198 (2021).
Keller, L. P. & McKay, D. S. Discovery of vapor deposits in the lunar regolith. Science 261, 1305–1307 (1993).
Keller, L. P. & McKay, D. S. The nature and origin of rims on lunar soil grains. Geochim. Cosmochim. Acta 61, 2331–2341 (1997).
Xian, H. Y. et al. Ubiquitous and progressively increasing ferric iron content on the lunar surfaces revealed by the Chang’e-5 sample. Nat. Astron. 7, 280–286 (2023).
Bindi, L., Shim, S. H., Sharp, T. G. & Xie, X. D. Evidence for the charge disproportionation of iron in extraterrestrial bridgmanite. Sci. Adv. 6, eaay7893 (2020).
Housley, R. M., Grant, R. W. & Paton, N. E. Origin and characteristics of excess Fe metal in lunar glass welded aggregates. Geochim. Cosmoschim. Acta 3, 2737–2749 (1973).
Blewett, D. T., Denevi, B. W., Cahill, J. T. S. & Klima, R. L. Near-UV and near-IR reflectance studies of lunar swirls: implications for nanosize iron content and the nature of anomalous space weathering. Icarus 364, 114472 (2021).
Glotch, T. D. et al. Formation of lunar swirls by magnetic field standoff of the solar wind. Nat. Commun. 6, 6189 (2015).
Vernazza, P., Binzel, R. P., Rossi, A., Fulchignoni, M. & Birlan, M. Solar wind as the origin of rapid reddening of asteroid surfaces. Nature 458, 993–995 (2009).
Sim, C. K., Kim, S. S., Lucey, P. G., Garrick‐Bethell, I. & Choi, Y. J. Asymmetric space weathering on lunar crater walls. Geophys. Res. Lett. 44, 11273–11281 (2017).
Hemingway, D. J., Garrick-Bethell, I. & Kreslavsky, M. A. Latitudinal variation in spectral properties of the lunar maria and implications for space weathering. Icarus 261, 66–79 (2015).
Trang, D. & Lucey, P. G. Improved space weathering maps of the lunar surface through radiative transfer modeling of Kaguya multiband imager data. Icarus 321, 307–323 (2019).
Li, Q. L. et al. Two billion-year-old volcanism on the Moon from Chang’e-5 basalts. Nature 600, 54–58 (2021).
Li, C. L. et al. Characteristics of the lunar samples returned by the Chang’E-5 mission. Natl Sci. Rev. 9, nwab188 (2022).
Heiken, G. H., Vaniman, D. T. & French, B. M. Lunar Sourcebook: A User’s Guide to the Moon 1–721 (Cambridge Univ. Press, 1991).
Zellner, N. E. B. Lunar impact glasses: probing the Moon’s surface and constraining its impact history. J. Geophys. Res. Planets 124, 2686–2702 (2019).
Bastin, J. A. Rotating lunar globules. Nature 283, 108–108 (1980).
Pugh, M. J. Rotation of lunar dumbbell-shaped globules during formation. Nature 237, 158–159 (1972).
Burgess, K. D. & Stroud, R. M. Coordinated nanoscale compositional and oxidation state measurements of lunar space‐weathered material. J. Geophys. Res. Planets 123, 2022–2037 (2018).
Thompson, M. S., Zega, T. J., Becerra, P., Keane, J. T. & Byrne, S. The oxidation state of nanophase Fe particles in lunar soil: implications for space weathering. Meteorit. Planet. Sci. 51, 1082–1095 (2016).
Brett, R. Reduction of mare basalts by sulfur loss. Geochim. Cosmochim. Acta 40, 997–1004 (1976).
Hu, G. L., Dam-Johansen, K., Wedel, S. & Hansen, J. P. Decomposition and oxidation of pyrite. Prog. Energy Combust. Sci. 32, 295–314 (2006).
Zolensky, M. E. et al. Mineralogy and petrology of comet 81P/Wild 2 nucleus samples. Science 314, 1735–1739 (2006).
Li, A. et al. Taking advantage of glass: capturing and retaining of the helium gas on the moon. Mater. Futures 1, 035101 (2022).
Bradley, J. P. et al. Detection of solar wind-produced water in irradiated rims on silicate minerals. Proc. Natl Acad. Sci. USA 111, 1732–1735 (2014).
Krishan, K. Ordering of voids and gas bubbles in radiation environments. Radiat. Eit. 66, 121–155 (1982).
Zhou, C. J. et al. Chang’E-5 samples reveal high water content in lunar minerals. Nat. Commun. 13, 5336 (2022).
Xu, Y. C. et al. High abundance of solar wind-derived water in lunar soils from the middle latitude. Proc. Natl Acad. Sci. USA 119, e2214395119 (2022).
Bibring, J. P. et al. Ultrathin amorphous coatings on lunar dust grains. Science 175, 753–755 (1972).
Kuhlman, K. R., Sridharan, K. & Kvit, A. Simulation of solar wind space weathering in orthopyroxene. Planet. Space Sci. 115, 110–114 (2015).
Weber, I. et al. Space weathering by simulated micrometeorite bombardment on natural olivine and pyroxene: a coordinated IR and TEM study. Earth Planet. Sci. Lett. 530, 115884 (2020).
Zhang, S. L. & Keller, L. P. Space weathering effects in lunar soils: the roles of surface exposure time and bulk chemical composition. In 42nd Lunar and Planetary Science Conference No. JSC-CN-22819 (2011).
Zhao, R. et al. Diverse glasses revealed from Chang’E-5 lunar regolith. Natl Sci. Rev. 10, nwad079 (2023).
Guo, Z. et al. Nanophase iron particles derived from fayalitic olivine decomposition in Chang’E‐5 lunar soil: implications for thermal effects during impacts. Geophys. Res. Lett. 49, e2021GL097323 (2022).
Matsumoto, T., Harries, D., Langenhorst, F., Miyake, A. & Noguchi, T. Iron whiskers on asteroid Itokawa indicate sulfide destruction by space weathering. Nat. Commun. 11, 1117 (2020).
Loeffler, M., Dukes, C. & Baragiola, R. Irradiation of olivine by 4 keV He+: Simulation of space weathering by the solar wind. J. Geophys. Res. Planets 114, E03003 (2009).
Dukes, C. A., Baragiola, R. A. & McFadden, L. A. Surface modification of olivine by H+ and He+ bombardment. J. Geophys. Res. Planets 104, 1865–1872 (1999).
Liu, Y. et al. Direct measurement of hydroxyl in the lunar regolith and the origin of lunar surface water. Nat. Geosci. 5, 779–782 (2012).
Keller, L. P., Berger, E. L., Zhang, S. & Christoffersen, R. Solar energetic particle tracks in lunar samples: a transmission electron microscope calibration and implications for lunar space weathering. Meteorit. Planet. Sci. 56, 1685–1707 (2021).
Strazzulla, G. et al. Spectral alteration of the Meteorite Epinal (H5) induced by heavy ion irradiation: a simulation of space weathering effects on near-Earth asteroids. Icarus 174, 31–35 (2005).
Costello, E. S., Ghent, R. R., Hirabayashi, M. & Lucey, P. G. Impact gardening as a constraint on the age, source, and evolution of ice on Mercury and the Moon. J. Geophys. Res. Planets 125, e2019JE006172 (2020).
Costello, E. S., Ghent, R. R. & Lucey, P. G. Secondary impact burial and excavation gardening on the Moon and the depth to ice in permanent shadow. J. Geophys. Res. Planets 126, e2021JE006933 (2021).
Shen, L. & Chang, C. Distinguishing the effects of irradiation and impacts on lunar metallic iron formation. figshare https://doi.org/10.6084/m9.figshare.25683804 (2024).
Acknowledgements
We are indebted to the China National Space Administration (CNSA) for providing the lunar samples. We thank all the staff of China’s CE-5 project for their brilliant work returning lunar samples. This work was supported by the National Natural Science Foundation of China (T2322029, 52301225, 52192600, 52001220, 11790291 and 61888102), the Strategic Priority Research Program of the Chinese Academy of Sciences (XDB30000000), the Special Research Assistant Funding Program of the Chinese Academy of Sciences and Guangdong Major Project of Basic and Applied Basic Research, China (2019B030302010).
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W.W., H.B., M.Y. and Z.Z. led the project. H.B. and L.S. supervised the research. L.S., R.Z., C.C., H.B. and W.W. conceived this work and wrote the manuscript. L.S. designed the experiments and performed the SEM measurements. D.X. and L.S performed the STEM measurements. L.S., R.Z. and C.C. analysed the experimental data. J.Y. assisted in data collection. All authors contributed to comment on the manuscript writing and the result discussions.
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Shen, L., Zhao, R., Chang, C. et al. Separate effects of irradiation and impacts on lunar metallic iron formation observed in Chang’e-5 samples. Nat Astron (2024). https://doi.org/10.1038/s41550-024-02300-0
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DOI: https://doi.org/10.1038/s41550-024-02300-0