Lazare Carnot was the unique example in the history of science of someone who inadvertently owed the scientific recognition he eventually achieved to earlier political prominence. He and his son Sadi produced work that derived from their training as engineering and went largely unnoticed by physicists for a generation or more, even though their respective work introduced concepts that proved fundamental when taken up later by other hands. There was, moreover, a filial as well as substantive relation between the work of father and son. Sadi applied to the functioning of heat engines the analysis that his father had developed in his study of the operation of ordinary machines. Specifically, Sadi's idea of a reversible process originated in the use his father made of geometric motions in the analysis of machines in general. This unique book shows how the two Carnots influenced each other in their work in the fields of mechanics and thermodynamics and how future generations of scientists have further benefited from their work.

Lazare Carnot was the unique example in the history of science of someone who inadvertently owed the scientific recognition he eventually achieved to earlier political prominence. He and his son Sadi producedwork that derived from their training as engineering and went largely unnoticed by physicists for a generation or more, even though their respective work introduced concepts that proved fundamental when taken up later by other hands. There was, moreover, a filial as well as substantive relation between the work of father and son. Sadi applied to the functioning of heat engines the analysis that his father had developed in his study of the operation of ordinary machines. Specifically, Sadi's idea of a reversible process originated in the use his father made of geometric motions in the analysis of machines in general.

This unique book shows how the two Carnots influenced each other in their work in the fields of mechanics and thermodynamicsand how future generations of scientists have further benefited from their work."

Originally published in 1960, The Edge of Objectivity helped to establish the history of science as a full-fledged academic discipline. In the mid-1950s, a young professor at Princeton named Charles Gillispie began teaching Humanities 304, one of the first undergraduate courses offered anywhere in the world on the history of science. From Galileo's analysis of motion to theories of evolution and relativity, Gillispie introduces key concepts, individuals, and themes. The Edge of Objectivity arose out of this course. It must have been a lively class. The Edge of Objectivity is pointed, opinionated, and selective. Even at six hundred pages, the book is, as the title suggests, an essay. Gillispie is unafraid to rate Mendel higher than Darwin, Maxwell above Faraday. Full of wry turns of phrase, the book effectively captures people and places. And throughout the book, Gillispie pushes an argument. He views science as the progressive development of more objective, detached, mathematical ways of viewing the world, and he orchestrates his characters and ideas around this theme. This edition of Charles Coulston Gillispie's landmark book introduces a new generation of readers to his provocative and enlightening account of the advancement of scientific thought over the course of four centuries. Since the original publication of The Edge of Objectivity, historians of science have focused increasingly on the social context of science rather than its internal dynamics, and they have frequently viewed science more as a threatening instance of power than as an accumulation of knowledge. Nevertheless, Gillispie's book remains a sophisticated, fast-moving, idiosyncratic account of the development of scientific ideas over four hundred years, by one of the founding intellects in the history of science. Featuring a new foreword by Theodore Porter, who places the work in its intellectual context and the development of the field, this edition of The Edge of Objectivity is a monumental work by one of the founding intellects of the history of science.

Pierre-Simon Laplace was among the most influential scientists in history. Often referred to as the lawgiver of French science, he is known for his technical contributions to exact science, for the philosophical point of view he developed in the presentation of his work, and for the leading part he took in forming the modern discipline of mathematical physics. His two most famous treatises were the five-volume" Traite de mecanique celeste" (1799-1825) and "Theorie analytique des probabilites" (1812). In the former he demonstrated mathematically the stability of the solar system in service to the universal Newtonian law of gravity. In the latter he developed probability from a set of miscellaneous problems concerning games, averages, mortality, and insurance risks into the branch of mathematics that permitted the quantification of estimates of error and the drawing of statistical inferences, wherever data warranted, in social, medical, and juridical matters, as well as in the physical sciences.

This book traces the development of Laplace's research program and of his participation in the Academy of Science during the last decades of the Old Regime into the early years of the French Revolution. A scientific biography by Charles Gillispie comprises the major portion of the book. Robert Fox contributes an account of Laplace's attempt to form a school of young physicists who would extend the Newtonian model from astronomy to physics, and Ivor Grattan-Guinness summarizes the history of the scientist's most important single mathematical contribution, the Laplace Transform."

First published in 1951, "Genesis and Geology" describes the background of social and theological ideas and the progress of scientific researches which, between them, produced the religious difficulties that afflicted the development of science in early industrial England. The book makes clear that the furor over "On the Origin of Species" was nothing new: earlier discoveries in science (particularly geology) had presented major challenges, not only to the literal interpretation of the Book of Genesis, but even more seriously to the traditional idea that Providence controls the order of nature with an eye to fulfilling divine purpose. A new Foreword by Nicolaas A. Rupke places this book in the context of the last forty-five years of scholarship in the social history of evolutionary thought.

This vividly illustrated book introduces the reader to the brothers Montgolfier, who launched the first hotair balloon in Annonay, France on 4 June 1783. Originally published in 1983. The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These editions preserve the original texts of these important books while presenting them in durable paperback and hardcover editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.

This vividly illustrated book introduces the reader to the brothers Montgolfier, who launched the first hotair balloon in Annonay, France on 4 June 1783.

Originally published in 1983.

The Princeton Legacy Library uses the latest print-on-demand technology to again make available previously out-of-print books from the distinguished backlist of Princeton University Press. These paperback editions preserve the original texts of these important books while presenting them in durable paperback editions. The goal of the Princeton Legacy Library is to vastly increase access to the rich scholarly heritage found in the thousands of books published by Princeton University Press since its founding in 1905.

From the 1770s through the 1820s the French scientific community predominated in the world to a degree that no other scientific establishment did in any period prior to the Second World War. In his classic "Science and Polity in France: The End of the Old Regime," Charles Gillispie analyzed the cultural, political, and technical factors that encouraged scientific productivity on the eve of the Revolution. In the present monumental and elegantly written sequel to that work, which Princeton is reissuing concurrently, he examines how the revolutionary and Napoleonic context contributed to modernization both of politics and science.

In politics, argues Gillispie, the central feature of this modernization was conversion of subjects of a monarchy into citizens of a republic in direct contact with a state enormously augmented in power. To the scientific community, attainment of professional status was what citizenship was to all Frenchmen in the republic proper, namely the license to self-governance and dignity within the respective contexts. Revolutionary circumstances set up a resonance between politics and science since practitioners of both were future oriented in their outlook and scornful of the past.

Among the creations of the First French Republic were institutions providing the earliest higher education in science. From them emerged rigorously trained people who constituted the founding generation in the disciplines of mathematical physics, positivistic biology, and clinical medicine. That scientists were able to achieve their ends was owing to the expertise they provided the revolutionary and imperial authorities in education, medicine, warfare, empire building, and industrial technology.

By the end of the eighteenth century, the French dominated the world of science. And although science and politics had little to do with each other directly, there were increasingly frequent intersections. This is a study of those transactions between science and state, knowledge and power--on the eve of the French Revolution. Charles Gillispie explores how the links between science and polity in France were related to governmental reform, modernization of the economy, and professionalization of science and engineering.