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Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering

Abstract

‘Space weathering’ is the term applied to the darkening and reddening of planetary surface materials with time, along with the changes to the depths of absorption bands in their optical spectra. It has been invoked to explain the mismatched spectra of lunar rocks and regolith, and between those of asteroids and meteorites1,2,3,4,5,6. The formation of nanophase iron particles on regolith grains as a result of micrometeorite impacts or irradiation by the solar wind has been proposed as the main cause of the change in the optical properties7,8. But laboratory simulations9,10,11,12,13,14 have not revealed the presence of these particles, although nano-second-pulse laser irradiation did reproduce the optical changes12. Here we report observations by transmission electron microscopy of olivine samples subjected to pulse laser irradiation. We find within the amorphous vapour-deposited rims of olivine grains nanophase iron particles similar to those observed in the rims of space-weathered lunar regolith grains15,16. Reduction by hydrogen atoms implanted by the solar wind is therefore not necessary to form the particles. Moreover, the results support the idea that ordinary chondrites came from S-type asteroids5, and thereby provides some constraints on the surface exposure ages of those asteroids.

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Figure 1: Bidirectional reflectance spectra of olivine pellet samples before and after pulse laser irradiation.
Figure 2: Nanophase iron particles in bright-field TEM images of the rim of laser-irradiated olivine grains.
Figure 3: A nanophase particle in the rim of an olivine grain irradiated 20 times at 30 mJ.

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References

  1. Adams, J. B. & McCord, T. B. Alteration of lunar optical properties: age and composition effects. Science 171, 567–571 (1971).

    Article  ADS  CAS  Google Scholar 

  2. Chapman, C. R. & Salisbury, J. W. Comparison of meteorite and asteroid spectral reflectivities. Icarus 19, 507–522 (1973).

    Article  ADS  CAS  Google Scholar 

  3. Gaffey, M. J. & McCord, T. B. Asteroid surface materials: Mineralogical characterizations from reflectance spectra. Space Sci. Rev. 21, 555–628 (1978).

    Article  ADS  Google Scholar 

  4. Wetherill, G. W. & Chapman, C. R. in Meteorites and the Early Solar System (eds Kerridge, J. F. & Matthews, M. S.) 35–67 (Univ. Arizona Press, Tucson, 1988).

    Google Scholar 

  5. Chapman, C. R. S-type asteroids, ordinary chondrites, and space weathering: The evidence from Galileo's fly-bys of Gaspra and Ida. Meteor. Planet. Sci. 31, 699–725 (1996).

    Article  ADS  CAS  Google Scholar 

  6. Pieters, C. M. et al. Space weathering on airless bodies: Resolving a mystery with lunar samples. Meteor. Planet. Sci. 35, 1101–1107 (2000).

    Article  ADS  CAS  Google Scholar 

  7. Hapke, B., Cassidy, W. & Wells, E. Effects of vapor-phase deposition processes on the optical, chemical and magnetic properties of the lunar regolith. Moon 13, 339–353 (1975).

    Article  ADS  CAS  Google Scholar 

  8. Hapke, B. Space weathering in the asteroid belt. Lunar Planet. Sci. 31, 1087 (2000).

    ADS  Google Scholar 

  9. Clark, B. E., Fanale, F. P. & Salisbury, J. W. Meteorite-asteroid spectral comparison: The effects of comminution, melting, and recrystallization. Icarus 97, 288–297 (1992).

    Article  ADS  CAS  Google Scholar 

  10. Moroz, L. V., Fisenko, A. V., Semjonova, L. F., Pieters, C. M. & Korotaeva, N. N. Optical effects of regolith processes on S-asteroids as simulated by laser shots on ordinary chondrite and other mafic materials. Icarus 122, 366–382 (1996).

    Article  ADS  CAS  Google Scholar 

  11. Yamada, M. et al. in Antarctic Meteorites Vol. 23, 173–176 (National Inst. Polar Res., Tokyo, 1998).

    Google Scholar 

  12. Yamada, M. et al. Simulation of space weathering of planet-forming materials: Nanosecond pulse laser irradiation and proton implantation on olivine and pyroxene samples. Earth Planets Space 51, 1255–1265 (1999).

    Article  ADS  CAS  Google Scholar 

  13. Hiroi, T. & Sasaki, S. Importance of olivine in S-asteroid space weathering. Lunar Planet. Sci. 30, 1444 (1999).

    ADS  Google Scholar 

  14. Hiroi, T. & Sasaki, S. First successful simulation of the asteroid space weathering using reflectance spectra of pulse laser irradiated olivine and pyroxene samples—Possible compositional dependency of S-asteroid space weathering. Meteor. Planet. Sci. (submitted).

  15. Keller, L. P. & McKay, D. S. Discovery of vapor deposits in the lunar regolith. Science 261, 1305–1307 (1993).

    Article  ADS  CAS  Google Scholar 

  16. Keller, L. P. & McKay, D. S. The nature and origin of rims on lunar soil grains. Geochim. Cosmochim. Acta. 61, 2331–2341 (1997).

    Article  ADS  CAS  Google Scholar 

  17. Gaffey, M. J. et al. Mineralogical variations within the S-type asteroid class. Icarus 106, 573–602 (1993).

    Article  ADS  CAS  Google Scholar 

  18. Clark, B. E. & Hiroi, T. S-type asteroid spectral continua: Redness and Fe, Ni metal. Bull. Am. Astron. Soc. 26, 1172 (1994).

    ADS  Google Scholar 

  19. Clark, B. E. Spectral mixing models of S-type asteroids. J. Geophys. Res. 100, 14443–14456 (1995).

    Article  ADS  Google Scholar 

  20. Allen, C. C., Morris, R. V., Lauer, H. V. Jr. & McKay, D. S. Microscopic iron metal on glass and minerals—A tool for studying regolith maturity. Icarus 104, 291–300 (1993).

    Article  ADS  CAS  Google Scholar 

  21. Binzel, R. P., Bus, S. J., Burbine, T. H. & Sunshine, J. M. Spectral properties of near-Earth asteroids: Evidence for sources of ordinary chondrite meteorites. Science 273, 946–948 (1996).

    Article  ADS  CAS  Google Scholar 

  22. Trombka, J. I. et al. The elemental composition of asteroid 433 Eros: Results of the NEAR-Shoemaker X-ray spectrometer. Science 289, 2101–2105 (2000).

    Article  ADS  CAS  Google Scholar 

  23. Grün, E. et al. in Origin and Evolution of Interplanetary Dust (eds Levasseur-Regourd, A. C. & Hasegawa, H.) 21–32 (Kluwer, Dordrecht, 1991).

    Book  Google Scholar 

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Acknowledgements

We thank M. Yamada for discussions and help in laser irradiation experiments, J. Owada and H. Akiyama for technical support during reflectance measurements, and H. Nagahara and K. Tomeoka for discussions and support. We thank T. Kogure for preliminary measurements by TEM and K. Akamatsu for technical advice during our TEM measurements. We also thank L. Keller for discussions on TEM analysis. We thank C. R. Chapman and B. E. Clark for their valuable comments. This work was partially supported by a Grant-in-Aid for Science Research from the Ministry of Education, Culture, Sports, Science and Technology, Japan and by a grant from the Inamori Foundation.

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Correspondence to Sho Sasaki.

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Sasaki, S., Nakamura, K., Hamabe, Y. et al. Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering. Nature 410, 555–557 (2001). https://doi.org/10.1038/35069013

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