Dark matter is primarily influenced by gravity, with limited known properties. For mathematical equations related to dark matter, the derivation of galaxy rotation curves based on density profiles is essential, and graphical representations comparing Baryons and Dark Matter are recommended for clarity. Resources like Wikipedia provide useful graphs and information on rotation curves. Additionally, calculations using principles similar to Kepler's laws can estimate the amount of dark matter that can exist in the solar system without affecting planetary orbits. This foundational understanding will aid in the project on dark matter.