This page discusses seasons as a result of Earth's axial tilt of about 23.5 degrees, influencing weather and daylight changes during its orbit. It clarifies misconceptions about the sun's distance and...This page discusses seasons as a result of Earth's axial tilt of about 23.5 degrees, influencing weather and daylight changes during its orbit. It clarifies misconceptions about the sun's distance and introduces key terms like solstices and equinoxes that denote daylight changes. Furthermore, it explains how Earth's axial orientation changes over time due to precession, affecting seasonal timing over a 26,000-year cycle, with minor fluctuations caused by nutation.