Abstract
The problem of autonomous control of the translational motion of the spacecraft in the vicinity of the focus of the gravitational lens of the Sun is formulated. The problem is solved by a reinforcement machine learning method using contemporary stochastic numerical methods. The costs of the characteristic velocity for targeting the focal line of a remote extended source, the final accuracy of targeting and the quality of the control function are investigated. The results of the study are given for various forms of state and observation: 1) position and velocity, 2) noisy position and velocity, 3) image of the Einstein ring. The efficiency of control strategies when using recurrent layers and fully connected layers with an input in the form of a measurement stack is compared. The training of control models accounting for execution errors of maneuvers is also being explored.