
Journal of Systems Engineering and Electronics ›› 2026, Vol. 37 ›› Issue (3): 933-951.doi: 10.23919/JSEE.2026.000127
• SYSTEMS ENGINEERING • Previous Articles Next Articles
Yaodong WANG1,2(
), Yue CAO3(
), Houman YU2(
), Yusheng LIU1,*(
)
Received:2024-07-31
Online:2026-06-18
Published:2026-06-29
Contact:
Yusheng LIU
E-mail:yaodong1217@163.com;ycao@zjut.edu.cn;htq501@139.com;ysliu@cad.zju.edu.cn
Supported by:Yaodong WANG, Yue CAO, Houman YU, Yusheng LIU. An MBPLE-enabled architecture design method for remote sensing satellites[J]. Journal of Systems Engineering and Electronics, 2026, 37(3): 933-951.
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Table 1
Typical configurations of RSS"
| Typical configuration | Application description |
| Low orbit stable | Applicable to satellites working in low orbit in steady state or with general attitude maneuvering/side swinging capability |
| Low orbit agile | Applicable to satellites with high requirements for low orbit attitude maneuvering capability |
| Medium and high orbit stable | Applicable to satellites working in medium and high orbit in steady state or with general attitude maneuvering/side swinging capability |
| Medium, high, and low orbit agile | Applicable to medium, high, and low orbits, with high system integration, high-precision measurement, pointing, and rapid maneuvering capability can be achieved through the optional three-supervision platform, achieving comprehensive performance improvement |
Table 2
List of available star sensor products"
| Number | Name | Product technical status | Application |
| 1 | High-precision star sensor APS VI type | Measurement accuracy (3σ): 3″(x/y), 25″(z) Optical axis thermal drift better than 0.3″/℃ Stray light suppression angle: 35° Dynamic performance: 3°/s Data update rate: 12 Hz Weight: probe 800g; line box 700g Power consumption: probe 1.8 W; line box 5W Power supply: 20−50 V, relay mode configurable Data interface: RS422, | Applicable to low, medium, and high orbits |
| 2 | High-precision star sensor APS II type | Measurement accuracy (3σ): When the absolute value of angular velocity is less than 0.1º/s, single head: x/y≤1"; z≤30" Two probes: When the installation angle is 90°, ≤0.7"(x/y); ≤0.7"(z) When the installation angle is 60°, ≤0.9"(x/y); ≤1.0"(z) Three probes: When the installation angle is 90°, ≤0.6"(x/y); ≤0.6"(z) When the installation angle is 60°, ≤0.8"(x/y); ≤1.0"(z) Optical axis thermal drift is better than 0.3″/℃ (15℃−25℃) Sunlight suppression angle 30° Earth-air light suppression angle 30° Dynamic performance: 2°/s Data update rate: 8 Hz Weight: Probe ≤3.7 kg, circuit box ≤7 kg Dimensions: Probe 156 mm×170 mm×392 mm Line box 144 mm×196 mm×258.5 mm Power consumption: Probe ≤4 W, Line box ≤45 W. Data interface: 1553B interface Power supply: +28−+42 V | Applicable to low, medium, and high orbits |
| 3 | Ultra-high precision star sensor APS I type | Field of view (°): 2×2; Sensitive magnitude (Mv): +10.5; Optical axis pointing accuracy (3σ): 0.3"; Update rate (Hz): 8; Dynamic performance (°/s): 0.2; Working temperature (℃): −30−+40; Sunlight suppression angle (°): 35; Body size (mm×mm×mm): Probe: 360×360 ×655; Line: 190×110 ×157; Weight (kg): Probe: to be determined; Line: to be determined; Electrical interface: RS422/1553B/LVDS; Power consumption (W): Probe: 2; Line: 10; Design life (a): 15; | Applicable to low, medium, and high orbits |
| 4 | Ultra-high precision star sensor APS II | Measurement accuracy (3σ): When angular velocity ≤0.1/s, better than 0.5″ (X/Y); Angular velocity 0.1−1 /s, better than 1″ (X/Y) Angular velocity 1−2/s, better than 2″ (X/Y) Angular velocity 2−5/s, better than 15″ (X/Y) Optical axis thermal drift is better than 0.1″/℃ (15℃−25℃) Sunlight suppression angle 30° Earth-air light suppression angle 30° Dynamic performance: 5°/s Data update rate: 8 Hz Weight: probe ≤5 kg, circuit box ≤10 kg Dimensions: probe 156 mm×170 mm×392 mm Circuit box 144 mm×196 mm×258.5 mm Power consumption: probe ≤4 W, circuit box ≤45 W. Data interface: 1553B interface Power supply: +28−+42 V | Applicable to low, medium orbits |
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