Dialogue Concerning the Two Chief World Systems

“Dialogue Concerning the Two Chief World Systems” by Galileo is a pivotal work in the history of science, published by Random House Publishing Group on October 2, 2001. This new edition spans 640 pages and presents Galileo’s arguments in favor of the Copernican system, which posits that the Earth revolves around the Sun, contrasting it with the Ptolemaic model. Written in a dialogue format, this text reflects the classical philosophical tradition and is noted for its clarity and accessibility, making it a significant scientific treatise.
Readers will find that this edition utilizes the definitive text established by the University of California Press, featuring Stillman Drake’s translation. It includes a Foreword by Albert Einstein and a new Introduction by J. L. Heilbron, enriching the context of Galileo’s arguments. The book delves into themes of science, philosophy, and the history of ideas, providing insights into the life sciences and biology as they relate to the astronomical debates of Galileo’s time. This work continues to be relevant for those interested in the evolution of scientific thought and the philosophical implications of the heliocentric model.
Official synopsis Publisher
Galileo’s Dialogue Concerning the Two Chief World Systems, published in Florence in 1632, was the most proximate cause of his being brought to trial before the Inquisition. Using the dialogue form, a genre common in classical philosophical works, Galileo masterfully demonstrates the truth of the Copernican system over the Ptolemaic one, proving, for the first time, that the earth revolves around the sun. Its influence is incalculable. The Dialogue is not only one of the most important scientific treatises ever written, but a work of supreme clarity and accessibility, remaining as readable now as when it was first published. This edition uses the definitive text established by the University of California Press, in Stillman Drake’s translation, and includes a Foreword by Albert Einstein and a new Introduction by J. L. Heilbron.
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