• Infrared and Laser Engineering
  • Vol. 49, Issue 5, 20190460 (2020)
Zhenchao Wang1, Jiahang Liu1,*, Qinghong Sheng1, and Yunzhao Wu2
Author Affiliations
  • 1College of Astronautics, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, China
  • 2Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210034, China
  • show less
    DOI: 10.3788/IRLA20190460 Cite this Article
    Zhenchao Wang, Jiahang Liu, Qinghong Sheng, Yunzhao Wu. Study on space weathering of Chang′e-4 landing site by in situ spectra[J]. Infrared and Laser Engineering, 2020, 49(5): 20190460 Copy Citation Text show less
    References

    [1] Hapke B. They of Reflectance Emittance Spectroscopy[M]. 2nd ed. Cambridge: Cambridge University Press, 2012.

    [2] E M Fischer, C M Pieters. Remote determination of exposure degree and iron concentration of lunar soils using VIS-NIR spectroscopic methods. Icarus, 111, 475-488(1994).

    [3] P G Lucey, G J Taylor, E Malaret. Abundance and distribution of iron on the Moon. Science, 268, 1150-1153(1995).

    [4] B Hapke. Space weathering from Mercury to the asteroid belt. J Geophys Res, 106, 10039-10073(2001).

    [5] Mris R V. igins size distribution of metallic iron particles in the lunar regolith[C]Lunar Pla Sci Conf, 1980: 16971712.

    [6] Dawei Liu, Lin Li, Ying Sun. An improved radiative transfer model for estimating mineral abundance of immature and mature lunar soils. Icarus, 253, 40-50(2015).

    [7] Zhenchao Wang, Yunzhao Wu, D T Blewett. Submicroscopic metallic iron inlunar soils estimated from the in situ spectra of the Chang’E-3 mission. Geophys Res Lett, 44, 3492(2017).

    [8] Xiaohui Fu, Yongliao Zou, Yongchun Zheng. Space weathering processes and effects on the Moon. Chin J Space Sci, 31, 705-715(2011).

    [9] Zhe Zhao, Ping Zhou, Bokun Yan. Spectra simulation of lunar regolith based on the Hapke radiative transfer model. Front. Earth Sci, 23, 266-278(2016).

    [10] Chunlai Li, Zhendong Wang, Rui Xu. The scientific information model of Chang’e-4 visible and near-IR imaging spectrometer (VNIS) and in-flight verification. Sensors, 19, 2806(2019).

    [11] Yunzhao Wu, B Hapke. Spectroscopic observations of the Moon at the lunar surface. Earth Planet Sci Lett, 484, 145-153(2018).

    [12] Yunzhao Wu, Zhenchao Wang, Wei Cai. The absolute reflectance and new calibration site of the moon. The Astronomical Journal, 155, 213(2018).

    [13] B Hapke. Bidirectional reflectance spectroscopy: 1. Theory. J Geophys Res, 86, 3039-3054(1981).

    [14] Bowell E, Hapke B, Domingue D, et al. Applications of Photometric Models to Asteroids[M]. 2nd ed. Arizona: University of Arizona Press, 1989.

    [15] J Mustard, C Pieters. Photometric phase functions of common geologic minerals and applications to quantitative analysis of mineral mixture reflectance spectra. Geophys Res, 94, 619-634(1989).

    [16] Mckay D S, Cooper B L, Riofrio L M. New measurements of the particle size distribution of Apollo 11 lunar soil[C]Lunar Pla Sci Conf, 2009.

    [17] Paquin R A. Hbook of Optics[M]. New Yk: McGrawHill, Inc,1995.

    [18] Houston W N, Mitchell J K, Carrier III W D. Lunar soil density posity[C] Proc Lunar Pla Sci Conf, 1974: 23612364.

    [19] Askel D R, Phule P P. The Science Engineering of Materials[M]. 4 th ed. USA: BrooksCole PublishingThompson Learning, 2003.

    [20] Yunzhao Wu, Bin Xue, Baochang Zhao. Global estimates of lunar iron and titanium contents from the Chang’ E-1 IIM data. J Geophys Res, 117, E02001(2012).

    Zhenchao Wang, Jiahang Liu, Qinghong Sheng, Yunzhao Wu. Study on space weathering of Chang′e-4 landing site by in situ spectra[J]. Infrared and Laser Engineering, 2020, 49(5): 20190460
    Download Citation