中国空间科学技术 ›› 2026, Vol. 46 ›› Issue (2): 118-125.doi: 10.16708/j.cnki.1000-758X.2026.0030

• 载人月球探测专刊 • 上一篇    下一篇

基于神经网络的地月转移中途修正脉冲快速估计方法

常笑宽1,2,李海阳1,2,*,李泽越1,2   

  1. 1.国防科技大学空天科学学院,长沙410073
    2.太空系统运行与控制全国重点实验室,长沙410073
  • 收稿日期:2025-09-27 修回日期:2025-11-10 录用日期:2025-11-20 发布日期:2026-03-20 出版日期:2026-03-31

A neural network approach for fast estimation of mid-correction in trans-lunar trajectory

CHANG Xiaokuan1,2,LI Haiyang1,2,*,LI Zeyue1,2   

  1. 1.College of Aerospace Science and Engineering, National University of Defense Technology, Changsha 410073, China
    2.State Key Laboratory of Space System Operation and Control, Changsha 410073, China
  • Received:2025-09-27 Revision received:2025-11-10 Accepted:2025-11-20 Online:2026-03-20 Published:2026-03-31

摘要: 在地月转移任务中,航天器入轨误差在强非线性动力学环境中迅速传播,影响终端精度。传统中途修正方法通常依赖“小偏差”假设与地面测控支持,难以满足未来任务对星上自主、实时执行的需求,且不适用于大偏差的情况。为此,提出一种适用于星上有限计算资源的轻量化神经网络方法,用于实现中途修正脉冲的快速估计。该方法首先通过高精度打靶仿真与理论分析,揭示了中途修正时刻速度偏差与所需修正脉冲之间存在近似线性关系;在此基础上,构建了一种轻量化全连接神经网络,建立了从标称轨道参数与修正时刻到脉冲比例系数的端到端智能映射。验证结果表明,该模型对脉冲比例系数的预测相对误差普遍低于3%。所提出的方法降低了对传统假设和地面支持的依赖,为在星上有限资源条件下实现自主中途修正提供了可行的技术途径。

关键词: 载人登月, 地月转移轨道, 中途修正, 偏差传播, 深度学习

Abstract: During Earth-Moon transfer, a spacecraft's orbit insertion errors propagate and amplify rapidly in a strong nonlinear dynamical environment, critically impacting mission success. Traditional mid-course correction methods, often reliant on the "small deviation" assumption and ground-based support, struggle to meet the demands for autonomous, real-time onboard execution. This study develops a lightweight neural network-based method for the rapid estimation of mid-course correction impulses, designed for limited onboard computational resources. The approach begins with high-fidelity shooting simulations and theoretical analysis, which reveal a near-linear relationship between initial velocity errors and the required correction impulses. Subsequently, a lightweight fully-connected network is constructed to establish a direct, end-to-end mapping from nominal orbital parameters and correction time to the corresponding impulse sensitivity coefficients. Validation results demonstrate that the relative error in predicting these coefficients remains below 3%. The proposed method reduces dependencies on traditional assumptions and ground support, offering a viable pathway for autonomous mid-course correction under stringent onboard resource constraints.

Key words: human lunar landing mission, trans-lunar trajectory, mid-correction, deviation propagation, DNN