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CHAPTER [strong]13[/strong]

RIVUXG This X-ray image of Tycho’s supernova, first seen as a visible light object by Tycho Brahe in 1572, was taken in 2003 by the Chandra X-ray Observatory. Gas and dust with temperatures in the millions of kelvins (shown in red and green) are expanding outward at about 10 million km/h, following a shell of high-energy electrons (blue).

The Deaths of Stars

WHAT DO YOU THINK?

  • Will the Sun someday cease to shine brightly? If so, how will this occur?
  • What is a nova? How does it differ from a supernova?
  • What are the origins of the carbon, silicon, oxygen, iron, uranium, and other heavy elements on Earth?
  • What are cosmic rays? Where do they come from?
  • What is a pulsar?

Answers to these questions appear in the text beside the corresponding numbers in the margins and at the end of the chapter.

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Most video and computer games have one thing in common: Players move through different levels, each progressively more difficult than the last. The biggest challenge comes at the final level, when you have to face the most powerful or evil entity. Stellar evolution is similar, with stars passing through different stages of stellar activity before they can move on to the next stage. There is one big difference—a game player can win the final level, but a star at the final stage of evolution always ceases to shine with the vigor that it had previously. In the end, stars more massive than red dwarfs eject vast quantities of gas and dust into interstellar space. In human terms, they die. In this chapter and in Chapter 14, we learn how the later stages of stellar evolution are significantly different for stars with different masses. Some of them stop evolving by relatively mild emissions of their outer layers, while others have spectacular finales.

In this chapter you will discover

  • what happens to stars when core helium fusion ceases
  • how heavy elements are created
  • the characteristics of the end of stellar evolution
  • why some stars go out relatively gently, and others go out with a bang
  • the incredible density of the matter in neutron stars and how these objects are observed