Kepler's Second Law of Planetary Motion, also known as the Law of Equal Areas, states that:A line segment joining a planet and the Sun sweeps out equal areas in equal intervals of time.Relationship to Planetary Revolution:This law explains how a planet’s speed changes as it orbits the Sun:1. Faster Motion Near the Sun (Perihelion):- When a planet is closest to the Sun (perihelion), the gravitational pull is stronger, causing the planet to move faster.2. Slower Motion Far from the Sun (Aphelion):- When the planet is farther from the Sun (aphelion), the gravitational force weakens, making the planet move more slowly.3. Conservation of Angular Momentum:- Since angular momentum is conserved, the planet adjusts its speed so that the area covered in a given time remains constant.• Importance in Planetary Revolution:- This law helps explain why planets do not move at a constant speed in their orbits.- It supports the idea that planetary orbits are elliptical, not circular.- It is crucial for understanding orbital mechanics in space exploration.