Earth Systems Science
Milankovitch cycles are long-term variations in Earth's orbit and axial tilt that affect the distribution of solar energy received by the planet, leading to changes in climate over thousands of years. These cycles are primarily driven by three astronomical factors: eccentricity, axial tilt, and precession. They play a crucial role in explaining past glacial and interglacial periods and provide insight into the natural causes of climate change.
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