Acta Optica Sinica, Volume. 45, Issue 18, 1828008(2025)

Performance Analysis of Near-Earth Asteroid Infrared Monitoring System Based on Earth-Leading Orbit (Invited)

Jiening Zhao1,2, Mingtao Li1,2、*, and Xintao Wang3
Author Affiliations
  • 1Key Laboratory of Electronics and Information Technology for Space System, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • 3DFH Satellite Co., Ltd., Beijing 100094, China
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    Figures & Tables(15)
    Cross-sectional views of guard zones for Earth-leading orbit telescope. (a) 45° guard zone; (b) 90° guard zone; (c) 180° guard zone
    Sky scanning strategy of Earth-leading orbit telescope
    Cross-sectional views of guard zones for Sun‒Earth L1 point orbit telescope
    Sky scanning strategy of Sun-Earth L1 point orbit telescope
    Cross-sectional views of guard zones for Earth-leading and Earth-trailing orbit telescopes. (a) 45° guard zone; (b) 90° guard zone
    Number of NEAs (NNEA) across different diameter ranges
    Reflected and thermal emission flux of asteroid across different wavelengths
    Reflected and thermal emission flux of asteroid across different albedos
    Minimum detectable diameters of asteroids at different positions for infrared telescope in Earth-leading orbit under different sensitivity levels. (a) 150 μJy; (b) 1000 μJy
    Minimum detectable diameters of asteroids at different positions for visible-light telescope in Earth-leading orbit under different limiting apparent magnitude. (a) 24 mag; (b) 22 mag
    Cumulative catalog completeness over time for NEAs with diameter not less than 50 m under different telescope systems
    • Table 1. Main parameters of telescope[24]

      View table

      Table 1. Main parameters of telescope[24]

      ParameterValue
      Telescope aperture /m0.5
      Wavelength /μm6‒10
      Dark current /electron200
      Read noise30
      Emissivity ε0.9
      Quantum efficiency /%70
      Point source sensitivity (5-σ)/ μJy150
    • Table 2. Monitoring and warning performance of Earth-leading orbit and Sun-Earth L1 point orbit telescope systems

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      Table 2. Monitoring and warning performance of Earth-leading orbit and Sun-Earth L1 point orbit telescope systems

      IndicatorEL 1EL 2EL 3L1
      Viewing zone (Earth longitude/solar longitude)-45°‒0°±45°±45° & ±(135°‒180°)±(45°‒135°)
      Viewing zone (ecliptic latitude)±45°±45°±45°±45°
      Point source sensitivity (5-σ) /μJy150150150150
      Finding effect29.67%37.97%41.58%54.73%
      Warning effect55.81%70.23%64.23%67.32%
      Warning effect (from Sun direction)86.88%75.83%67.02%72.93%
    • Table 3. Monitoring and warning performance of two-telescope system based on Earth-leading and Sun-Earth L1 point orbits

      View table

      Table 3. Monitoring and warning performance of two-telescope system based on Earth-leading and Sun-Earth L1 point orbits

      IndicatorEL 1+L1EL 2+L1EL 3+L1L1
      Finding effect56.13%56.53%56.60%54.73%
      Warning effect77.28%84.10%78.71%67.32%
      Warning effect (from Sun direction)91.02%86.52%81.32%72.93%
    • Table 4. Monitoring and warning performance of two-telescope system based on Earth-leading and Earth-trailing orbits

      View table

      Table 4. Monitoring and warning performance of two-telescope system based on Earth-leading and Earth-trailing orbits

      IndicatorEL 1EL 1+ETEL 2+ETL1
      Viewing zone (Earth longitude/solar longitude)-45°‒0°-45°‒0°±45°±(45°‒135°)
      Viewing zone (ecliptic latitude)±45°±45°±45°±45°
      Point source sensitivity (5-σ)/ μJy150150150150
      Finding effect29.67%43.56%52.77%54.73%
      Warning effect55.81%70.11%90.93%67.32%
      Warning effect (from Sun direction)86.88%92.08%91.50%72.93%
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    Jiening Zhao, Mingtao Li, Xintao Wang. Performance Analysis of Near-Earth Asteroid Infrared Monitoring System Based on Earth-Leading Orbit (Invited)[J]. Acta Optica Sinica, 2025, 45(18): 1828008

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    Paper Information

    Category: Remote Sensing and Sensors

    Received: Jun. 3, 2025

    Accepted: Jul. 29, 2025

    Published Online: Sep. 19, 2025

    The Author Email: Mingtao Li (limingtao@nssc.ac.cn)

    DOI:10.3788/AOS251203

    CSTR:32393.14.AOS251203

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