Theory Of Orbital Motion

This book offers a thorough exploration of orbital mechanics, including Kepler's laws and Newton's gravitation, essential for understanding celestial motion.

The Theory Of Orbital Motion delves into the fundamental principles that govern the motions of celestial bodies. It begins by exploring Kepler's laws of planetary motion, which laid the groundwork for our understanding of how planets, moons, and other celestial objects move in space. Following this, the book examines Newton's law of gravitation, providing readers with a comprehensive overview of the forces that influence orbital dynamics. The author skillfully addresses the average and extremum values of dynamical variables, offering insights into the complexities of the central force problem.

As the narrative unfolds, the Theory Of Orbital Motion tackles the planetary problem using both Cartesian and complex coordinates. This approach not only enriches the reader's comprehension of orbital mechanics but also presents practical examples of Keplerian motion observed within our solar system. The text is designed to bridge the gap in existing literature, particularly at the elementary and intermediate levels, where such topics are often only briefly covered in broader mechanics courses.

In its final chapters, the book shifts focus to the motion of artificial Earth satellites, discussing how their orbits can be affected by various perturbing forces. This section highlights the relevance of orbital mechanics in today's space age, making it an essential resource for anyone engaged in space science, from students to seasoned professionals. Overall, the Theory Of Orbital Motion is both informative and accessible, making complex concepts understandable for a wide audience.