The Milankovitch Cycles are essential for explaining the glaciations during the Ice Age. These cycles are named after the Serbian scientist Milutin Milankovitch, who proposed that slow changes in Earth's orbit and tilt lead to significant alterations in climate.
- There are three main components: eccentricity, axial tilt, and precession.
- Eccentricity refers to the shape of Earth's orbit around the Sun, changing from more circular to more elliptical over a 100,000-year cycle.
- Axial tilt, occurring every 41,000 years, describes the angle between Earth's rotational axis and its orbital plane. Variations in tilt influence the severity of seasons.
- Precession involves the wobble in Earth's rotational axis and occurs over a 26,000-year cycle, affecting the timing of seasons.
These orbital changes influence the distribution of solar energy received by Earth, triggering cooling or warming phases, and hence, the advance or retreat of ice sheets. Understanding Milankovitch Cycles provides insight into the natural rhythms of Earth's climate system.