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Question
what did you learn about star movement during this investigation?
Since no details of the investigation are given, a general answer could be that stars have both proper - motion across the celestial sphere and radial - motion towards or away from us. Proper - motion is due to the stars' own velocities in space relative to the Sun, and radial - motion can be detected through the Doppler effect in their spectral lines.
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Stars have proper - motion across the celestial sphere and radial - motion towards or away from us, with proper - motion being their motion relative to the Sun in the plane of the sky and radial - motion detectable via the Doppler effect in spectral lines.