This invention provides a method and
system for high-fidelity physical modeling and
detection performance evaluation of space targets, relating to the field of
deep space exploration technology. The method first acquires the
relative motion parameters of the
spacecraft and the
asteroid, as well as camera parameters, and determines the static apparent magnitude based on observation geometry and the
asteroid's physical characteristics. Then, it calculates the
angular velocity modulus through
relative velocity, combines it with camera parameters to obtain
tail parameters, and quantifies the equivalent magnitude loss and effective apparent magnitude based on a piecewise model. Subsequently, it constructs a two-dimensional parameter grid of
focal length and
exposure time, calculates the effective
signal-to-
noise ratio and detection margin for each combination, and selects the optimal parameters using a heatmap. Finally, it generates a high-fidelity
simulation image and feeds back the observation values to the guidance, navigation, and
control system via a UDP asynchronous interface. This invention achieves
quantitative assessment of
tail loss and automated parameter optimization, balancing
high fidelity and real-time performance, and improving detection accuracy and
system reliability.