The Earth-Sun relationship contributes to the seasons primarily through the tilt of the Earth's axis and its orbit around the Sun. As the Earth orbits, different hemispheres receive varying amounts of sunlight throughout the year due to this axial tilt, which is approximately 23.5 degrees. During summer, a hemisphere is tilted toward the Sun, resulting in longer days and more direct sunlight, while winter occurs when it's tilted away, leading to shorter days and less direct sunlight. This variation in sunlight and temperature is what creates the distinct seasons.
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