Exoplanets predominantly exhibit elliptical orbits, contrasting with the more defined orbits of planets in our solar system. The detection bias towards massive, close-in exoplanets is due to current observational limitations, which favor the identification of these types over smaller, distant planets. As observational techniques improve, astronomers are beginning to discover a wider variety of exoplanets, including those further from their stars. The challenges in detecting exoplanets stem from their lack of emitted light and the brightness of their parent stars, necessitating specialized detection methods. This ongoing research continues to reveal the diversity of planetary systems beyond our own.