Stars and Atoms

'Stars and Atoms' is a seminal exploration of the profound connection between the microscopic world of subatomic particles and the vast mechanical workings of the cosmos. Written by the distinguished astrophysicist Arthur Stanley Eddington, this work bridge the gap between laboratory physics and celestial observation, arguing that the secrets of the heavens are written in the behavior of the smallest known particles. The text focuses on the physical constitution of stars, detailing how atomic energy and radiation pressure serve as the engines of the universe. Eddington masterfully explains complex phenomena such as stellar temperature, the internal density of suns, and the evolution of celestial bodies. By synthesizing the then-emerging fields of quantum mechanics and astronomy, the work provides a comprehensive look at how stars generate light and heat, and why they maintain their stability over eons. As a foundational text in modern astrophysics, 'Stars and Atoms' offers readers a fascinating glimpse into the intellectual rigor of early 20th-century science. It remains an essential read for anyone interested in the history of scientific discovery and the fundamental laws that govern our universe, presented with the clarity and insight for which Eddington was celebrated.This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you may see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work.This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work.As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.