
Stars and Atoms
PREFACE
LIST OF ILLUSTRATIONS
LECTURE I THE INTERIOR OF A STAR
Temperature in the Interior
Ionization of Atoms
Radiation Pressure and Mass
The Interior of a Star
Opacity of Stellar Matter
The Relation of Brightness to Mass
In this classic collection of three lectures, a pioneering astronomer invites listeners to travel from the heart of a star to the inner world of the atom, showing how the two realms echo each other. Using vivid analogies—a drop of water teeming with invisible atoms compared to a sun‑sized sphere populated by countless stars—he makes the immense and the infinitesimal feel equally tangible. The prose is clear enough for the curious layperson, yet it never shies away from the deep questions that drive modern physics.
The first lecture dives into the hidden furnace of a star, explaining temperature, ionization, and the pressure of radiation that balances gravity. Subsequent talks turn to recent astronomical discoveries, from the peculiar behavior of Algol and Sirius’s companion to the spectral fingerprints that reveal unknown elements in distant nebulae. Finally, the speaker explores how pulsating stars serve as cosmic mile‑markers and how the gradual aging of stars ties into the broader story of the universe’s evolution. Listeners will come away with a fresh sense of wonder at how the smallest particles and the brightest suns share a common language.
Language
en
Duration
~3 hours (206K characters)
Publisher of text edition
Project Gutenberg
Original publisher
New Haven: Yale University Press, 1927.
Credits
Laura Natal Rodrigues (Images generously made available by Hathi Trust Digital Library.)
Release date
2024-04-08
Rights
Public domain in the USA.

1882–1944
A pioneering astrophysicist who helped bring Einstein’s ideas to the English-speaking world, he wrote with unusual clarity about stars, space, and the deeper patterns of the universe. His books blend scientific insight with a calm, thoughtful sense of wonder.
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