in the sky daily and seasonally due to the motion of the Earth 2. Although we live in a 3D universe for convenience we define position of celestial objects as if they were on a sphere with the earth at the center. 3. Some basic trigonometric concepts are needed to understand “spherical astronomy” 4. We use several coordinate systems, some tied to the celestial body, some tied to the observer 6. The earth spin axis and orbit of the earth around the sun are used to define these coordinates 8. The 3 main coordinate system are RA/Dec, Alt/Az, and HA/Az