Task 1 uses paramaters from the solar system and selected exoplanet systems to verify kepler's third law. Kepler's third law states that the squares of the orbital periods of the planets are directly proportional to the cubes of the semi-major axes of their orbits, which was verified by plotting the Orbital period vs Orbital Semi-major axis^(3/2) for each planet in the system. As expected, for the solar system and many of the exoplanet systems, the constant of proportionality was shown to be close to unity, however the systems CoRoT–7, GJ 1061, GJ 163 and TOI-700 were far from unity. Due to it's simplicity, an error in the code is unlikely so it must be surmised that either the data used to calculate the plotted values is incorrect or these systems experience extrenous circumstances that influence the orbits of the planets within them.
