Earth’s revolution, known as its orbital or translational motion, is the movement around the Sun.
Lasting approximately 365.25 days, this journey defines a year. Earth’s elliptical orbit contributes to seasonal variations, with axial tilt playing a role.
As our planet completes this orbit, different hemispheres experience varying sunlight intensity, leading to seasonal changes.
The constant, rhythmic pattern of Earth’s revolution is a fundamental astronomical phenomenon influencing climate and ecosystems, essential to understanding our planet’s relationship with the Sun and the cyclical nature of seasons.
