LIFE OF A STAR What are the two main kinds of nebulae? Where in the life of a star would we find each of them? What type of star will the Sun turn into next? What will be happening inside the Sun that causes the change?
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Two main kinds of nebulae are emission nebulae and planetary nebulae. Emission nebulae are typically found in regions with newly formed stars, where energetic radiation excites surrounding gas, causing it to glow brightly. These impressive clouds often serve as the birthing grounds for new stars. On the other hand, planetary nebulae usually appear later in a star's life cycle, emerging after medium-sized stars like our Sun have exhausted their nuclear fuel, shedding outer layers to form a glowing shell of gas surrounding a white dwarf core. The Sun is set to evolve into a red giant after it runs out of hydrogen fuel in its core. As the hydrogen gets depleted, the core will contract and heat up, igniting helium fusion in a process called helium burning. This surge in energy will push the outer layers of the Sun outward, causing it to swell dramatically into a red giant before eventually shedding its outer layers to form a beautiful planetary nebula, leaving behind the hot core as a white dwarf. Exciting, isn’t it?
