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Texto del Guión Gráfico

  • Hi! I represent hydrogen
  • we make matter in the form of elements using heat and light energy
  • Hi! I represent pressure
  • Hi I'm heat
  • The Bigger the star the more fuel the star burns causing it to live shorter
  • The sun is in the Main Sequence stage
  • The Sun's energy warms the Earth, causes wind and weather, and sustains plant and animal life.
  • Hey Ms.Earth, The force of gravity becomes greater than the force from internal pressure and the star begins to collapse.
  • Hey Mr. Moon, how does changes in the amount of hydrogen and helium in a star impact the remaining lifespan of the star?
  • the outward pressure produced by the heating of the gas by fusion energy balances gravity, a stable star is formed.
  • Once a star reaches equilibrium for the first time, it will start burning (fusing) hydrogen into helium.
  • The heaviest elements, like iron, however, are only formed in the massive stars which end their lives in supernova explosions.
  • The most common elements, like carbon and nitrogen, are created in the cores of most stars, fused from lighter elements like hydrogen and helium
  • The End.
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