Difference between revisions of "Star"

From OrbiterWiki
Jump to navigation Jump to search
m (Reverted edits by 74.231.24.2 (Talk); changed back to last version by Ozone)
Line 1: Line 1:
 +
bocdoms
 
A '''star''' is a massive body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. Unlike a planet, from which most light is reflected, a star emits light because of its intense heat. Scientifically, stars are defined as self-gravitating spheres of plasma in hydrostatic equilibrium, which generate their own energy through the process of nuclear fusion.
 
A '''star''' is a massive body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. Unlike a planet, from which most light is reflected, a star emits light because of its intense heat. Scientifically, stars are defined as self-gravitating spheres of plasma in hydrostatic equilibrium, which generate their own energy through the process of nuclear fusion.
  

Revision as of 23:19, 26 October 2007

bocdoms A star is a massive body of plasma in outer space that is currently producing or has produced energy through nuclear fusion. Unlike a planet, from which most light is reflected, a star emits light because of its intense heat. Scientifically, stars are defined as self-gravitating spheres of plasma in hydrostatic equilibrium, which generate their own energy through the process of nuclear fusion.

A longer definition at Wikipedia: [1]

This article is a stub. You can help Orbiterwiki by expanding it.