Explorations: Introduction to Astronomy (Arny), 6th Edition

Chapter 14: Stellar Evolution

<a onClick="window.open('/olcweb/cgi/pluginpop.cgi?it=jpg::::/sites/dl/free/0010202009/220722/chapter14.jpg','popWin', 'width=NaN,height=NaN,resizable,scrollbars');" href="#"><img valign="absmiddle" height="16" width="16" border="0" src="/olcweb/styles/shared/linkicons/image.gif"> (541.0K)</a>

  • When stars use up all their available nuclear fuel, they collapse.
  • Low-mass stars like the Sun turn into white dwarfs.
  • High-mass stars (ten or so times the Sun’s mass) may explode as supernova.
  • The core of a high-mass star may survive as either a neutron star or a black hole.
  • White dwarfs are about the size of the Earth but have a mass about that of the Sun.
  • Neutron stars have a mass about that of the Sun but are a mere 10 kilometers or so in diameter.
  • A black hole forms if the core of a massive star becomes so dense that the escape velocity at its surface reaches the speed of light.
  • Black holes emit no electromagnetic radiation but may be detected by observing gas that is heated as it falls into the hole.

Glencoe Online Learning CenterScience HomeProduct InfoSite MapContact Us

The McGraw-Hill CompaniesGlencoe