Acta Photonica Sinica, Volume. 54, Issue 2, 0254110(2025)

Optical Design and Stray Light Analysis for Integrated Asteroid Detection and Imaging

Liguo BIAN1...2, Xuyang LI1,*, Qinfang CHEN1, Tongyu XU1,2, Zhixian LU1,2, and Li ZHANG12 |Show fewer author(s)
Author Affiliations
  • 1Space Optics Technology Lab, Xi'an Institute of Optics and Precision Mechanics of CAS, Xi'an 710119, China
  • 2University of Chinese Academy of Science, Beijing 100049, China
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    Figures & Tables(16)
    Schematic diagram of an R-C system structure
    Optical system layout diagram
    Spot diagram
    Modulation transfer function curves for different fields of view in the system
    Focus adjustments at different imaging distances
    Enclosed energy distribution in imaging mode
    Enclosed energy distribution in detecting mode
    Probability of MTF degradation in different directional fields of view
    M-C analysis of encircled energy
    System model for stray light analysis
    The PST curve of system
    • Table 1. Detector parameter details

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      Table 1. Detector parameter details

      ParameterValue
      Photon energy Ep/J3.61×10-19
      Non-suppressed stray radiation noise electron count Bn4
      Readout noise electron count Nr15
      Dark current noise electron count Nd6
      System transmittance τ070%
      Integration time t/s0.042
      Quantum efficiency QE50%
    • Table 2. Final structural parameters of the system

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      Table 2. Final structural parameters of the system

      SurfaceRadius/mmThickness/mmQuadratic coefficientMaterial
      Stop-818.53-306.73-1.093 6MIRROR
      1-285.03306.02-4.179 4MIRROR
      2100.6818.960SILICA_SPECIAL
      3395.2114.270
      4-86.117.870HQK3L_CDGM
      5113.2820.000
    • Table 3. Allocation of tolerances

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      Table 3. Allocation of tolerances

      TypeValue
      Lens thickness and air gap±0.02 mm
      Lens surface tilt±0.000 5 rad
      Lens surface decentering±0.02 mm
      Lens local aperture0.2
      Lens aperture2
      Lens refractive index±0.001
      Abbe number of lens±0.002
      Conic constant (quadric)±0.001
      Curvature radius (quadric)±0.02
    • Table 4. Distribution of surface roughness on optical surfaces and the resulting backscattered radiant flux

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      Table 4. Distribution of surface roughness on optical surfaces and the resulting backscattered radiant flux

      Optical surface numberRoughness/nmAngle of incidence/(°)Half-aperture/mmRadiant flux/W
      Mirror 11.52.940 151401.764 88×10-17
      Mirror 21.53.768 03387.612 6×10-17
      Surface 1 of lens 121.005 3215.54.301 3×10-17
      Surface 2 of lens 121.535 91145.272 39×10-17
      Surface 1 of lens 222.606 89128.111 84×10-17
      Surface 2 of lens 220.911 53128.111 84×10-17
    • Table 5. Structural parameters of the baffle

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      Table 5. Structural parameters of the baffle

      ParametersOuter bafflePrimary mirror baffleSecondary mirror baffle
      Largest outer diameter/mm319.8184.02120
      Length/mm475.58144.7591.09
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    Liguo BIAN, Xuyang LI, Qinfang CHEN, Tongyu XU, Zhixian LU, Li ZHANG. Optical Design and Stray Light Analysis for Integrated Asteroid Detection and Imaging[J]. Acta Photonica Sinica, 2025, 54(2): 0254110

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    Paper Information

    Category: Special Issue for Precise Beam Pointing for Space Gravitational Wave Detection

    Received: Jul. 12, 2024

    Accepted: Sep. 29, 2024

    Published Online: Mar. 25, 2025

    The Author Email: LI Xuyang (lixuyang2004@126.com)

    DOI:10.3788/gzxb20255402.0254110

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