Dark matter is a hypothetical form of matter that cannot be observed directly but is inferred from its gravitational effects on visible matter, particularly in galaxies. It is theorized to explain the constant high radial velocities of galaxies, which exceed expected values based on visible mass alone. The two main categories of dark matter candidates are WIMPs (Weakly Interacting Massive Particles) and MACHOs (Massive Compact Halo Objects), though MACHOs are often considered less viable due to insufficient baryonic matter. The discussion highlights the ongoing curiosity and research surrounding dark matter, emphasizing the need for further exploration of its properties and implications in astrophysics. Understanding dark matter remains a significant challenge in modern physics.