  Numerous numerical studies have been carried out in recent years that
simulate different aspects of exoplanets' magnetosphere and stellar winds.
These studies have focused primarily on hot Jupiters with sun-like stars. This
study addresses the challenges inherent in utilizing existing MHD codes to
model hot Jupiter-star systems. Due to the scaling of the system and the
assumption of a uniformly flowing stellar wind at the outer boundary of the
simulation, MHD codes necessitate a minimum distance of greater than 0.4 au for
a Jupiter-like planet orbiting a sun-like star to avoid substantial violations
of the code's assumptions. Additionally, employing the GAMERA (Grid Agnostic
MHD for Extended Research Applications) MHD code, we simulate star-planet
interactions considering various stellar types (Sun-like and M Dwarf stars)
with both Jupiter-like and Earth-like planets positioned at varying orbital
distances. Furthermore, we explore the impact of tidal locking on the total
power within the magnetosphere-ionosphere systems.
