The book describes the major physical theories of comets in the past two millennia. It describes the evolution of ideas about the nature, position, motion and constitution of comets. Unlike many works on the subject, this one focuses on details of each theory.

Although the development of ideas about the motion and trajectory of comets has been investigated piecemeal, we lack a comprehensive and detailed survey of ph- ical theories of comets. The available works either illustrate relatively short periods in the history of physical cometology or portray a landscape view without adequate details. The present study is an attempt to review with more details the major physical theories of comets in the past two millennia, from Aristotle to Whipple. My research, however, did not begin with antiquity. The basic question from which this project originated was a simple inquiry about the cosmic identity of comets at the dawn of the astronomical revolution: how did natural philosophers and astronomers define the nature and place of a new category of celestial objects comets after Brahe's estimation of cometary distances? It was from this turning point in the history of cometary theories that I expanded my studies in both the pre-modern and modern eras. A study starting merely from Brahe and ending with Newton, without covering classical and medieval thought about comets, would be incomplete and leave the fascinating achievements of post-Newtonian cometology unexplored.

A comprehensive history of physical theories of comets from 300 BC to the appearance of modern theory of comets in the1950s Discusses the details of major theories of comets based on primary sources Illustrates the interaction between observational and mathematical astronomy, and the physical sciences in defining the properties of comets

Inhalt
Aristotle's Theory of Comets.- After Aristotle.- From Brahe to Newton.- Comets in Newtonian Physics.- After Newton.- Non-Newtonian Theories of Comets.- Comets in the Laplacian Cosmos.- Comets in the Post-Laplacian Era.