This video attempts to demonstrate the path that the sun takes, in the Geocentric model, as the universe rotates about its center at a 23.5 degree angle.
The sun, as it moves in its own orbit, in a counter clockwise direction along the ecliptic plane (shown in white) will trace the path that is drawn in the video (shown in blue), showing how the sun, as it moves in its orbit, is found in the southern hemisphere and then gradually up into the northern hemisphere, always moving along the ecliptic path and within the rotation of the universe.
This path that the sun takes around the earth produces for us our seasons.
