The Titius-Bode Law is a mathematical formula that predicts the distances of planets from the Sun in our solar system. It suggests that there is a pattern in the spacing of the planets, where each planet's distance from the Sun can be approximated using a simple equation. This law was first proposed by Johann Daniel Titius in 1766 and later popularized by Johan Elert Bode in 1772. While the Titius-Bode Law accurately describes the distances of some planets, such as Mercury, Venus, Earth, and Mars, it does not hold true for all celestial bodies. For example, it fails to predict the distance of Neptune accurately, leading scientists to view it as more of a curiosity than a strict rule in planetary formation.