The conservation of energy

audiobook

The conservation of energy

by Balfour Stewart

EN·~5 hours·14 chapters

Chapters

14 total
1

THE INTERNATIONAL SCIENTIFIC SERIES.

2:32
2

THE CONSERVATION OF ENERGY.

0:26
3

NOTE TO THE AMERICAN EDITION.

2:18
4

PREFACE.

1:57
5

CHAPTER I.WHAT IS ENERGY?

31:41
6

CHAPTER II.MECHANICAL ENERGY AND ITS CHANGE INTO HEAT.

34:49
7

CHAPTER III.THE FORCES AND ENERGIES OF NATURE: THE LAW OF CONSERVATION.

54:05
8

CHAPTER IV.TRANSMUTATIONS OF ENERGY.

1:03:12
9

CHAPTER V.HISTORICAL SKETCH: THE DISSIPATION OF ENERGY.

32:19
10

CHAPTER VI.THE POSITION OF LIFE.

18:56

Description

A clear‑headed guide to one of the most fundamental ideas in modern science, this work explains how energy—whether in heat, motion, electricity or chemistry—never disappears but merely changes form. Written in plain language and enriched with familiar illustrations, it walks readers through the history of the principle, the experiments that proved it, and the simple equations that describe its behaviour in everyday phenomena.

Beyond the physics, the book includes an appendix that explores how the same law can be seen at work in living organisms and the human mind. Essays by respected scholars connect the conservation of energy to physiology, mental processes and even broader philosophical questions, offering a thought‑provoking glimpse of how a single scientific insight can echo through many fields of study.

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Details

Language

en

Duration

~5 hours (323K characters)

Series

The international scientific series, volume 7.

Publisher of text edition

Project Gutenberg

Original publisher

United States: D. Appleton and Company, 1875.

Credits

Nina Akalis and the Online Distributed Proofreading Team at https://www.pgdp.net (This file was produced from images generously made available by The Internet Archive)

Release date

2022-09-27

Rights

Public domain in the USA.

About the author

Balfour Stewart

Balfour Stewart

1828–1887

A pioneering Scottish physicist and meteorologist, he helped lay the groundwork for modern ideas about heat radiation and energy exchange. He also led Kew Observatory and spent much of his career teaching physics in Manchester.

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