
These mind-blowing exoplanets defy logic by whipping around their stars in mere hours—yet somehow avoid tidal destruction! Avonetics sleuths reveal the shocking truth: bloated stars, cosmic migration, and detection bias make these ultra-close orbits possible. Discover why current methods miss smaller, distant worlds and how gravitational chaos reshapes planetary fates. Will these planets eventually spiral into their stars? The answers will stun you. For advertising opportunities, visit Avonetics.com.