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  • Understanding Earth's Seasons: Tilt and Sunlight
    The Earth has seasons due to two main reasons:

    1. Earth's Tilt: The Earth is tilted on its axis at approximately 23.5 degrees. This tilt means that different parts of the Earth receive varying amounts of direct sunlight throughout the year.

    * Summer: When a hemisphere is tilted towards the Sun, it receives more direct sunlight, resulting in longer days and warmer temperatures.

    * Winter: When a hemisphere is tilted away from the Sun, it receives less direct sunlight, resulting in shorter days and colder temperatures.

    2. Earth's Orbit: The Earth orbits the Sun in an elliptical path, meaning it's not a perfect circle. This elliptical path causes the Earth to be closer to the Sun at certain times of the year and further away at other times.

    * Perihelion: The point in Earth's orbit where it's closest to the Sun (around January).

    * Aphelion: The point in Earth's orbit where it's furthest from the Sun (around July).

    * Impact on Seasons: While the distance from the Sun does affect the amount of solar radiation, it's a much smaller factor than Earth's tilt.

    Therefore, the combination of Earth's tilt and its orbit around the Sun creates the cycle of seasons we experience.

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