Dark Matter refers to a mysterious and invisible substance that makes up approximately 27% of the universe's total mass-energy content. Unlike ordinary matter, which consists of atoms and can emit, absorb, or reflect light, dark matter does not interact with electromagnetic forces, making it undetectable by conventional means. Its presence is inferred through gravitational effects on visible matter, radiation, and the large-scale structure of the universe. For instance, the rotation curves of galaxies demonstrate that stars orbiting the outer regions of galaxies move at much higher speeds than would be expected based on the visible mass alone, suggesting the existence of additional unseen mass.
Despite extensive research, the precise nature of dark matter remains unknown, with several candidates proposed, including Weakly Interacting Massive Particles (WIMPs) and axions. Understanding dark matter is crucial for cosmology and could lead to new insights into the fundamental workings of the universe.
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