• 16 hours ago
The universe is vast and enigmatic, filled with wonders that challenge our understanding of reality. Among the many mysteries it holds, dark matter stands out as one of the most intriguing. Despite being invisible and undetectable by conventional means, dark matter is thought to comprise approximately 27% of the universe’s total mass-energy content. This essay explores the concept of dark matter, its evidence, and its significance in the cosmic landscape.

What is Dark Matter?

Dark matter is a hypothetical form of matter that does not emit, absorb, or reflect light, making it invisible to electromagnetic observations. Its presence is inferred through its gravitational effects on visible matter, such as galaxies and galaxy clusters. Unlike ordinary matter, which is composed of protons, neutrons, and electrons, dark matter is believed to consist of unknown particles that interact only weakly with electromagnetic forces.

Evidence for Dark Matter

The existence of dark matter is supported by several lines of evidence:

Galaxy Rotation Curves: Observations of spiral galaxies reveal that their outer regions rotate at nearly constant speeds, contrary to predictions based on visible matter alone. This discrepancy suggests the presence of an unseen mass providing additional gravitational pull.

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