Introduction

When observing the night sky, the stars appear as points of light on a great dome overhead. For centuries, humans have used these stars to track time, mark seasons, and find their way across oceans and deserts. To understand and predict the movements of celestial objects, astronomers have developed models and tools for mapping the sky. This chapter introduces the celestial sphere model and the key reference lines used to locate objects in the sky. It then discusses the recognition of star patterns and constellations, and concludes with basic techniques for using stars to determine direction and describe the position of objects in the night sky.
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Polaris (The North Star) appears stationary as the rest of the stars revolve around it. It is because The position of Polaris roughly aligns with Earth's rotational axis. Image - matt-molloy
Picture
The night sky at the equator clearly shows the counter clockwise and clockwise motion of stars at the North and South Poles, while stars at the equators moves from East to North.