Early Discoveries, Page 7: [Previous Page] [Next Page] [Class Home Page] Textbook pages 10 - 16

The Celestial Sphere

Astronomers base their measurement of positions of objects on the concept of the celestial sphere upon which all objects are assumed to lie regardless of their true distances.
The meridian is the circle running from one pole to the other through a point directly overhead for an observer. The point directly overhead is called the zenith

The celestial poles and equator are the projections of the Earth's poles and equator onto the sky.
What stars you see passing through your zenith, depends on your latitude on the Earth. Consider standing on the top of the earth, the North Pole. At zenith, you will always see Polaris!
On the equator, then Polaris will be your furthest northern horizon point. Stars pass over you like you were inside a rolling barrel.

At our latitude, 39o, the celestial sphere rolls around us like a tilted barrel. Star Trails