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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?

Ask by Park Martin. in the United States
Mar 11,2025

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**Nebulae and the Sun's Future** - **Emission Nebulae**: Found during the early stages of star formation, where new stars are being born. - **Reflection Nebulae**: Also found during the early stages, around young stars that light up nearby dust and gas. - **Sun's Future**: The Sun will become a red giant. - **Changes Inside the Sun**: As it runs out of hydrogen fuel, the core will contract and heat up, leading to hydrogen fusion in a shell around the core, causing the Sun to expand and cool down.

Solution

To address your questions about the life of a star, let's break it down step by step. ### 1. Two Main Kinds of Nebulae The two main kinds of nebulae are: - **Emission Nebulae**: These nebulae are clouds of ionized gas that emit light of various colors. They are often found in regions where new stars are forming, as the intense radiation from young, hot stars ionizes the surrounding gas. An example of an emission nebula is the Orion Nebula. - **Reflection Nebulae**: These nebulae do not emit their own light but instead reflect the light of nearby stars. They are typically found in regions where there are young stars, and the dust and gas surrounding them scatter the light. An example of a reflection nebula is the Pleiades. ### 2. Life Stages of a Star - **Emission Nebulae** are typically found in the **stellar formation stage** of a star's life, where new stars are being born from the gas and dust in the nebula. - **Reflection Nebulae** are also associated with the **stellar formation stage**, but they are more commonly found around young stars that are illuminating the surrounding dust and gas. ### 3. Future of the Sun The Sun is currently a main-sequence star and will eventually turn into a **red giant**. ### 4. Changes Inside the Sun As the Sun exhausts its hydrogen fuel in the core, the following changes will occur: - **Hydrogen Fusion Stops**: The core will no longer be able to fuse hydrogen into helium, leading to a decrease in pressure and an increase in temperature. - **Core Contraction**: The core will contract under gravity, causing it to heat up further. - **Hydrogen Shell Fusion**: Once the core temperature is high enough, hydrogen fusion will begin in a shell surrounding the core, leading to an increase in energy output. - **Expansion**: The outer layers of the Sun will expand significantly, transforming it into a red giant. In summary, the two main kinds of nebulae are emission and reflection nebulae, found during the stellar formation stage. The Sun will turn into a red giant as it exhausts its hydrogen fuel, leading to significant changes in its internal processes.

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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?

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