Part B of Planetary Astronomy from the Renaissance to the Rise of Astrophysics is the sequel to Part A and continues the history of celestial mechanics and observational discovery through the eighteenth and nineteenth centuries. Twelve different authors have contributed their expertise in some eighteen chapters, each of them intended to be accessible to the interested layman. An initial section deals with stages in the reception of Newton's inverse square law as exact. In the remainder of the book a large place is given to the development of the mathematical theory of celestial mechanics from Clairaut and Euler to LeVerrier, Newcomb, Hill and Poincaré - a topic rarely treated, at once synoptically and in some detail. Lists of further reading provide entrée to the literature of these several topics.

Volume 4 of The General History of Astronomy, originally published in 1984, concerns the birth of modern astrophysics in the nineteenth century, the growth of astronomical institutions to around 1920, and the development of instrumentation. The volume commences in the 1850s, with the first astronomical applications of photography and spectral analysis. It closes in the 1950s, before the explosive growth made possible by new electronic devices and computers. In Part A, there are eleven chapters, written by an international panel of eighteen authors, on subjects such as observatories, large telescopes, astronomy in the southern hemisphere, and early radio astronomy. Intended for general readership, this book formed part of an in-depth synthesis of the development of astronomy from the earliest times.

Part B of Planetary Astronomy from the Renaissance to the Rise of Astrophysics is the sequel to Part A and continues the history of celestial mechanics and observational discovery through the eighteenth and nineteenth centuries. Twelve different authors have contributed their expertise in some eighteen chapters, each of them intended to be accessible to the interested layman. An initial section deals with stages in the reception of Newton's inverse square law as exact. In the remainder of the book a large place is given to the development of the mathematical theory of celestial mechanics from Clairaut and Euler to LeVerrier, Newcomb, Hill and Poincaré - a topic rarely treated, at once synoptically and in some detail. Lists of further reading provide entrée to the literature of these several topics.

Volume 4 of The General History of Astronomy, originally published in 1984, concerns the birth of modern astrophysics in the nineteenth century, the growth of astronomical institutions to around 1920, and the development of instrumentation. The volume commences in the 1850s, with the first astronomical applications of photography and spectral analysis. It closes in the 1950s, before the explosive growth made possible by new electronic devices and computers. In Part A, there are eleven chapters, written by an international panel of eighteen authors, on subjects such as observatories, large telescopes, astronomy in the southern hemisphere, and early radio astronomy. Intended for general readership, this book formed part of an in-depth synthesis of the development of astronomy from the earliest times.