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Astronomy 2e · The Sun: A Nuclear Powerhouse

Thinking Ahead

CC BY 4.0 · OpenStax · approximately 1 min read

Learning objectives

The Sun.

View original figure (external; image not reproduced in this text edition)

Original figure description: A photograph shows the sun low in the sky at sunset.

It takes an incredible amount of energy for the Sun to shine, as it has and will continue to do for billions of years. (credit: modification of work by Ed Dunens)

The Sun puts out an incomprehensible amount of energy—so much that its ultraviolet radiation can cause sunburns from 93 million miles away. It is also very old. As you learned earlier, evidence shows that the Sun formed about 4.5 billion years ago and has been shining ever since. How can the Sun produce so much energy for so long?

The Sun’s energy output is about 4×1026 watts. This is unimaginably bright: brighter than a trillion cities together each with a trillion 100-watt light bulbs. Most known methods of generating energy fall far short of the capacity of the Sun. The total amount of energy produced over the entire life of the Sun is staggering, since the Sun has been shining for billions of years. Scientists were unable to explain the seemingly unlimited energy of stars like the Sun prior to the twentieth century.

← Space WeatherSources of Sunshine: Thermal and Gravitational Energy →

Attribution. Astronomy 2e, OpenStax, Rice University, and the contributing authors credited in the book. Licensed under Creative Commons Attribution 4.0 International. Source revision 63157f370b of openstax/osbooks-astronomy (2026-02-02). CC BY 4.0. Original source ↗. Text edition of a pinned CC BY 4.0 source revision of the OpenStax book, converted from CNXML by the EvidenceHelix importer. Original prose, learning objectives, tables, exercises, glossary and captions are preserved; images are not copied (figures link to the original source and keep their credits). No new content was added. Later revisions of this book can carry different licence terms and are not used.

In this chapter Contents

  • Thinking Ahead
  • Sources of Sunshine: Thermal and Gravitational Energy
  • Mass, Energy, and the Theory of Relativity
  • The Solar Interior: Theory
  • The Solar Interior: Observations

Source

OpenStax source file ↗

Illustrated original ↗

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