Describe the annual motion of the Earth.
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Annual motion is the apparent yearly movement of the stars as observed from Earth as a direct effect of the Earth's revolution around the sun. The sun revolves 360 degrees a year around a path on the celestial sphere called the ecliptic. The sun moves eastward with respect to the stars on the celestial sphere.
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The earth also wobbles on its axis, which causes the seasons, and rotates on its own axis, which causes days. There is a ratio of 365.2498 rotations of its own axis to every rotation on the solar axis, leading to the amount of days in a year.
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