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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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