Why Falling Toward the Sun Is Almost Impossible

Contemplate the surprising physics of celestial orbital mechanics as we discover why sending a probe directly into the Sun requires more orbital energy than escaping the solar system entirely. Earth travels around our star at nearly 67,000 miles per hour, carrying an immense amount of sideways velocity that keeps us drifting safely in a permanent, stable orbit. To shed that momentum and fall inward toward the solar surface requires vast amounts of energy, making the heart of our solar system one of the most difficult destinations to reach. Let the eternal, harmonious balance of orbital motion soothe your mind and cradle you into a deep, peaceful sleep.