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Obliquity refers to the tilt of a planet's axis relative to its orbital plane. For Earth, this tilt is approximately 23.44 degrees and is not constant, varying over tens of thousands of years. This axial tilt is a primary driver of Earth's seasons, influencing how solar radiation is distributed across the planet throughout the year.123

The prevailing hypothesis for Earth's axial tilt suggests a massive collision with a celestial body named Theia early in its formation, which also contributed to the creation of the Moon. The gravitational pull of Earth's moon helps to stabilize this tilt. Obliquity is one of the orbital parameters that influence Earth's climate cycles, particularly over long timescales.12

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