ABSTRACT The interactions between stars and their orbiting planets, driven by forces such as stellar radiation and gravity, play an essential role in shaping exoplanetary atmospheres and gas‐rich debris discs. One way to look into the composition of these environments is to observe how they can contaminate the stellar photospheres. For that, we examine how stellar radiation pressure and gravity influence atomic species and analyze their effects across various stellar effective temperatures. Using the radiative‐to‐gravitational force ratio, we determined the atomic movement direction and assessed the velocity boost imparted to neutral atoms escaping from exoplanet atmospheres or debris discs. Incorporating the solar far ultraviolet/extreme ultraviolet spectrum to address flux discrepancies in the ATLAS9 model, we find that radiation affects atoms differently according to their ionization state, with highly ionized species less affected by stellar radiation. Our results conclude that the stars most suitable for observing stellar contamination are those between 6500 and 8000 K, with neutral noble gases and ionized iron‐peak elements as the most likely contaminants.