Worlds in the making: The evolution of the universe

audiobook

Worlds in the making: The evolution of the universe

by Svante Arrhenius

EN·~6 hours·12 chapters

Chapters

12 total
1

Transcriber’s Notes

0:16
2

WORLDS IN THE MAKING

5:24
3

ILLUSTRATIONS

3:27
4

PREFACE

6:32
5

I VOLCANIC PHENOMENA AND EARTHQUAKES

53:39
6

II THE CELESTIAL BODIES, IN PARTICULAR THE EARTH, AS ABODES OF ORGANISMS

44:27
7

III RADIATION AND CONSTITUTION OF THE SUN

44:53
8

IV THE RADIATION PRESSURE

38:10
9

V THE SOLAR DUST IN THE ATMOSPHERE—POLAR LIGHTS AND THE VARIATIONS OF TERRESTRIAL MAGNETISM

47:51
10

VI END OF THE SUN—ORIGIN OF NEBULÆ

58:52

Description

This volume takes listeners on a sweeping tour of the forces that have shaped our planet and the heavens. Beginning with the dramatic power of volcanoes and earthquakes, it explains how the Earth’s crust formed, cooled, and settled into a home for life. The narrative then lifts to the Sun, detailing its heat, spots, and the mysterious radiation pressure that influences comets and the solar corona.

Moving outward, the book explores the birth and evolution of nebulae, the mechanisms that turn clouds of gas into stars, and the delicate balance of entropy across the cosmos. It also ventures into early ideas about how life might travel beyond Earth, examining theories of spores hitching rides on solar dust and the possibility of panspermia. All of this is presented in a clear, thoughtful style that captures the wonder of early scientific discovery while remaining accessible to modern listeners.

Details

Language

en

Duration

~6 hours (360K characters)

Publisher of text edition

Project Gutenberg

Original publisher

United States: Harper & Brothers Publishers, 1908.

Credits

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

2022-09-21

Rights

Public domain in the USA.

Subjects

About the author

Svante Arrhenius

Svante Arrhenius

1859–1927

A pioneer of physical chemistry, this Swedish scientist helped explain why salts split into charged particles in solution and opened new ways of thinking about acids, bases, and reaction rates. He is also remembered for an early calculation showing how changes in carbon dioxide could affect Earth’s temperature.

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