This book, in three parts, describes three phases in the development of
the modern theory and calculation of the Moon's motion. Part I explains
the crisis in lunar theory in the 1870s that led G.W. Hill to lay a new
foundation for an analytic solution, a preliminary orbit he called the
"variational curve." Part II is devoted to E.W. Brown's completion of
the new theory as a series of successive perturbations of Hill's
variational curve. Part III describes the revolutionary developments in
time-measurement and the determination of Earth-Moon and Earth-planet
distances that led to the replacement of the Hill-Brown theory in 1984.