Stars and Nebulae

Stars and Nebulae — page 3
StarS and nebulae When a star goes supernova considerable amounts of its matter equaling the material of several Suns may be blasted into space with such a burst of energy as to enable the exploding star to outshine its entire home galaxy Supernovae are characterized by a tremendous rapid brightening lasting for a few weeks followed by a slow dimming A supernova explosion is a cataclysmic event for a star one that essentially ends its active i e energy-generating lifetime Supernovae release many of the heavier elements that make up the components of the solar system including Earth into the interstellar medium White dwarfs have a mass similar to that of the Sun but with a radius comparable to that of Earth making them extremely dense White dwarfs have average densities densities approaching 1,000,000 times that of water Neutron stars are any of a class of extremely dense compact stars thought to be composed primarily of neutrons neutrons Their masses range between 1 and 2 times that of the Sun Having so much mass packed within a ball on the order of 20 km 12 miles in diameter a neutron star has a density that can reach that of nuclear values which is roughly 100 trillion 1014 times the average density of solar matter or of water This approximates the density inside the atomic nucleus and in some ways a neutron star can be conceived of as a gigantic nucleus 8