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Evolution of Stars: Pressure, Temperature, and Fate Explained

Explore the journey of stars as they evolve through pressure and temperature changes, from normal to degenerate gases, leading to the red giant, horizontal branch, and asymptotic branch phases. Learn about the fate of the Sun, planetary nebulae, and the formation of white dwarfs.

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Evolution of Stars: Pressure, Temperature, and Fate Explained

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Presentation Transcript

    1. How Stars Evolve Pressure and temperature Normal gases Degenerate gases The fate of the Sun Red giant phase Horizontal branch Asymptotic branch Planetary nebula White dwarf

    2. Normal gas Pressure is the force exerted by atoms in a gas Temperature is how fast atoms in a gas move

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