Newton's Theory of Gravitation Development

Isaac Newton's development of the theory of gravitation began in the mid-17th century, specifically around 1665. During this period, he focused on understanding the forces that govern celestial bodies and their movements. His work laid the foundation for celestial mechanics, a branch of astronomy that deals with the motions of celestial objects under the influence of gravitational forces. By 1679, Newton intensified his research on gravitation, examining how it affects the orbits of planets. This exploration was crucial in establishing the laws of motion and universal gravitation, which would later be articulated in his seminal work, 'Philosophiæ Naturalis Principia Mathematica.' The impact of Newton's theory was profound, as it provided a comprehensive framework for understanding not only the motion of planets but also the behavior of objects on Earth. His insights into gravitational forces transformed the scientific community's approach to physics and astronomy, leading to advancements in various fields, including engineering and navigation. The principles he established remain fundamental to modern physics, influencing subsequent scientists and shaping our understanding of the universe.