The document presents a modified equation for the moon's orbital motion, replacing the previous angle of 0.98562 degrees with a revised value of 1.6 degrees, leading to an accuracy of 96.12% in predicting the moon's position. It explains the relationship between the angle of motion (θ) and the moon's real displacement, emphasizing its effect on the moon's distance from Earth at perigee and apogee. The study includes calculations and data validation based on the moon's distance from Earth over a specified period.
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