This document discusses the history and current state of the dark matter problem in astrophysics. It summarizes that observations in the 1930s and 1970s found that galaxies and galaxy clusters contain far more mass than can be accounted for by the visible stars and gas, with the mass increasing farther from galaxy centers. This is known as the "missing mass" problem. The current favored model, called Lambda Cold Dark Matter (Lambda CDM), posits that dark matter makes up 85% of all matter in the universe and helps explain large scale structure formation. However, the nature of dark matter remains unknown, and alternative gravitational theories have not been ruled out. Future experiments aim to directly detect dark matter particles or test gravitational theories on larger scales