I. Introduction
Small bodies, such as asteroids and comets, are likely to retain the conditions under which they were formed owing to the absence of atmospheric and crustal movements. Thus, they are expected to provide data that are useful for elucidating the conditions at the time of the birth of the solar system and the process of its evolution [1]–[5]. Flyby, which is one of the methods that is employed to explore celestial bodies entails spacecraft to collect various types of information while passing near the target body. Starting with the Halley's Comet flyby observation in 1986, many spacecraft have since succeeded in the flyby observation of small bodies. Generally, the quality of the image is proportional to the size of the telescope and in reverse proportion to the relative distance from the target body. Recently, the spacecraft tends to become smaller and the telescope size is limited under the resource constraints. Achieving precise observation with a small telescope means that the required relative distance becomes smaller and the importance of a precise navigation system becomes higher. At the same time, a target tracking system is required to enlarge the observation opportunities. In this regard, visual-based tracking systems are popular. Figure 1 shows an overview of the flyby imaging. The telescope's line-of-sight is controlled to track the target body direction during the flyby.
Target body tracking during the flyby.