Our project aims to computationally evaluate the long-term evolution of exoplanet orbits around massive stars. These stars have high surface temperatures and strong stellar winds. The mass lost through these winds will have important effects on the development of their exoplanets' orbits and environments. We have performed a series of model calculations for a range of hot star properties. Each star is then assumed to have an initial collection of model planets orbiting them at a range of orbital radii. For the detailed modelling of the effects of stellar evolution, we use the open-source computer program Modules for Experiments in Stellar Astrophysics (MESA). We then run our own code in Python to calculate the effects on model planet orbits. This project should help in the interpretation of observations of exoplanets orbiting hot stars at various evolutionary stages.
