Dark matter is a hypothetical type of matter that accounts for approximately 85% of the matter in the universe but does not emit, absorb, or interact with electromagnetic radiation. It is believed to play a key role in the formation of galaxies and their structure. While its existence and properties are well-established through its gravitational effects, its exact nature remains unknown. Several experiments are attempting to directly detect dark matter particles through methods like observing signals produced when dark matter particles interact or are destroyed, but so far none have succeeded, and dark matter's composition remains one of the greatest unsolved mysteries in physics.