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One Universe: At Home in the Cosmos







Matter | Pages 82-83 | (back to unlinked version)

Nearly 10,000 stars fill this portion of the Large Magellanic Cloud External Link: Learn more about this satellite galaxy of the Milky Way., a nearby galaxy gradually spiraling into the Milky Way. Despite the crowded appearance of the field, the stars themselves are so far apart that smash-ups between the two galaxies' stellar inhabitants are highly unlikely.

elements. The protons, nuclei, and electrons then waited for the universe to chill further, just as we might wait for our soup to cool at dinner. But whereas we wait a few minutes before sipping, the primordial matter waited another 300,000 years or so until the temperature dropped to a frosty 4,000 degrees. Only then was it cool enough for the electrons to join with the protons and the heavier nuclei to form atoms, an event called recombination External Link: A description of the era when atoms first formed in the universe..

This original Big Bang recipe for the cosmos yielded, by weight, about 75 percent hydrogen and 25 percent helium. There was a soupçon of other elements as well, including lithium External Link: Learn more about Element 3., beryllium External Link: Learn more about Element 4., and one one-thousandth of a percent deuterium External Link: Some information about the properties and chemistry of ''heavy hydrogen'' on Earth.. But the Big Bang produced not a single atom of carbon External Link: Learn more about Element 6., oxygen External Link: Learn more about Element 8., calcium External Link: Learn more about Element 20., iron External Link: Learn more about Element 26., or any other heavy element. Those ingredients for planets and life were generated by the second and ongoing phase of nucleosynthesis in the universe. The factories that churn out the heavy elements External Link: A detailed overview, with graphics, of the star formation process., astrophysicists realized during the twentieth century, are the stars in the sky.

The original set of cosmic ingredients spawned the first stars. Gravity pulled together pockets of matter that started with slightly higher densities, a slow process that probably took several million years. In time these prenatal stars became hot and dense enough at their cores to ignite the fires of thermonuclear fusion External Link: A Java-based interactive explanation of thermonuclear fusion in stars.. Hydrogen atoms in the cores fused into new atoms of helium, losing a tiny amount of mass along the way. That "lost" mass became energy in accordance with Einstein's famous equation, E = mc2. The energy flowed out from the cores of the newborn stars, providing the heat and pressure needed to balance any further contractions from the inward force of gravity. This continual balancing act of gravity versus nuclear fusion characterizes the lives of adult stars Internal Link:  .

All stars are large balls of electrically charged gas, called plasma External Link: Learn more about plasma, often (and somewhat incorrectly) referred to as a ''fourth state of matter.''. Perhaps because of science fiction­style plasma External Link: Learn more about plasma, often (and somewhat incorrectly) referred to as a ''fourth state of matter.'' ray guns, most people think of plasma External Link: Learn more about plasma, often (and somewhat incorrectly) referred to as a ''fourth state of matter.''s as exotic, energetic, and hot. That's true in a star, but in fact plasma External Link: Learn more about plasma, often (and somewhat incorrectly) referred to as a ''fourth state of matter.''s also are common on Earth. When we touch a metal doorknob after shuffling our feet across a carpet, that small spark we feel is an electrical charge running through a plasma External Link: Learn more about plasma, often (and somewhat incorrectly) referred to as a ''fourth state of matter.'' pathway in the air that arose milliseconds before the shock. The same process occurs with lightning, albeit on (continued)