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Table of Contents

View the Stars
Measuring Position
Important Points
The Earth's Tilt
Effects of Tilt
Sun's Motion
Stars' Motion
The North Star
Precession
Timekeeping
Sun as Timekeeper
Sideral Time
Ceasar's Calender
Ceasar's Solution
Does Earth Spin?

External Links

Now lets consider some of the star constellations that we can see fromnight_sky_anim.gif (27461 bytes) Bloomington.   Lets concentrate on the big dipper and the little dipper

stars keep the same position relative to each other. For example, the stars forming the lip of the Big Dipper always point toward the tail star of the Little Dipper (which is the star Polaris).

Thus we can consider the stars as attached to the celestial sphere. The fact that a star changes its position during the course of a night informs  us that the celestial sphere is not stationary. It is, in fact moving.  Do you know why the celestial sphere is moving?  Think of what causes day and night on the Earth and the answer will reveal itself.

The motion of the celestial sphere in the sky is actually quite simple. The fact that the motion is as simple as possible, was an attractive fact to the ancient Greek philosophers: it demonstrated design deserving an explanation.

In the picture to the right imagine you are facing north.  Can you determine which way the celestial sphere is rotating.  That is does the celestial sphere rotate west to east, east to west, north to south?  

back to top Astronomer Note:  Notice that the tail of the Little Dipper (the star Polaris) remained fixed while the other stars just rotated around it.  Why do you think this is the case?