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Milankovitch
cycles are long-term, natural variations in Earth's orbit and axial
tilt that alter the amount of solar radiation reaching the planet,
influencing long-term climate changes like the onset and end of ice ages. These cycles include changes in the shape of Earth's orbit (eccentricity), the tilt of Earth's axis (obliquity), and the wobble of Earth's axis (precession). These
cycles operate over thousands to hundreds of thousands of years,
affecting climate patterns by influencing seasonal solar radiation, not
the total amount of solar radiation received.
Here are the three main cycles:
Role in Climate:
Distinguishing from Current Warming:
- It is important to note that Milankovitch cycles cannot explain the rapid global warming observed in recent times. The warming trend over the past century is far too fast to be driven by these slow orbital changes. The significant increase in atmospheric greenhouse gases from human activity is the primary driver of current warming, not the Sun or Earth's orbital position.
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Why Milankovitch (Orbital) Cycles Can't Explain Earth's Current Warming - NASA Science
Feb 27, 2020
NASA Science
Milankovitch Cycles, Paleoclimatic Change, and Hominin Evolution | Learn Science at Scitable
The
three elements of Milankovitch cycles are eccentricity, obliquity, and
precession (Figure 3). Eccentricity describes the degre...
Nature
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