un:evolution-of-single-stars
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| un:evolution-of-single-stars [2025/10/27 12:22] – created asad | un:evolution-of-single-stars [2025/10/27 12:24] (current) – asad | ||
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| The **evolution of single stars** traces how a star changes in structure, luminosity, and temperature over its lifetime. | The **evolution of single stars** traces how a star changes in structure, luminosity, and temperature over its lifetime. | ||
| These transformations are driven primarily by **nuclear fusion** in the core, the **loss of energy** through radiation, and the changing **balance between gravity and pressure**. | These transformations are driven primarily by **nuclear fusion** in the core, the **loss of energy** through radiation, and the changing **balance between gravity and pressure**. | ||
| - | The position of a star on the Hertzsprung–Russell (H-R) diagram changes as it evolves through successive stages. | ||
| - | {{: | + | The position of a star on the Hertzsprung–Russell (H-R) diagram changes as it evolves through successive stages. |
| ===== 1. Formation and pre-main-sequence stage ===== | ===== 1. Formation and pre-main-sequence stage ===== | ||
un/evolution-of-single-stars.1761589324.txt.gz · Last modified: by asad