Dark matter is theorized to exist as a significant component of the universe, making up about 23% of its total mass-energy content, while ordinary matter constitutes only about 4%. It is believed to form dark haloes around galaxies, influencing their rotation and structure through gravitational effects, even though it cannot be directly observed. The discussion raises questions about whether dark matter could form structures like stars, but it is noted that if it did, it would no longer be "dark." The existence of dark matter remains a topic of debate, with some arguing that its properties, such as being collisionless and non-interactive, make it difficult to detect even in our solar system. Overall, while there is no definitive proof of dark matter's existence, many physicists consider it a reasonable extension of current models to explain observed phenomena.