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๐ Dark matter makes up about 27% of the universe's total mass-energy content.
๐ It does not emit, absorb, or reflect any electromagnetic radiation, making it invisible and undetectable by normal telescopes.
๐ซ Its presence is inferred through gravitational effects on visible matter, such as galaxies and galaxy clusters.
๐งช The particles that constitute dark matter remain unknown, with candidates including WIMPs and axions.
๐ญ Dark matter forms a halo around galaxies, influencing their rotation and maintaining their structure.
๐ It does not interact through the electromagnetic force, allowing it to pass through ordinary matter almost unhindered.
๐ฌ Scientists have been trying to directly detect dark matter particles through various experiments, but success has been elusive.
๐ The concept of dark matter was first proposed in the 1930s by physicist Fritz Zwicky.
๐ Dark matter's existence helps explain the discrepancy between the mass of large astronomical objects and the gravitational effects they exert.
๐ฝ It plays a crucial role in the formation and evolution of galaxies across the cosmos.
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