Dark matter is an invisible form of matter that constitutes about 30% of the universe, inferred from the gravitational effects on visible matter, such as the rapid motion of galaxies. It was initially overlooked due to its non-interaction with light and ordinary matter, leading to ongoing debates about its nature, including theories involving WIMPs and neutrinos. The existence of dark energy, which makes up about 60% of the universe, was proposed to explain the accelerated expansion of the cosmos. Discussions also touched on the distinction between baryonic and non-baryonic matter, with the latter being linked to dark matter. The implications of dark matter and energy are significant for the future of astronomy, as they challenge existing models of the universe.