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Climate Change

Milankovitch cycles and changes in solar output

  • 2 things to know
  • Component 03

Overview

Recall questions on eccentricity, obliquity and precession and their periods, summer insolation at 65° N and ice sheet growth, why orbital cycles need feedbacks, the sunspot cycle and solar irradiance, the Maunder Minimum, the faint young Sun paradox, and why solar output cannot explain recent warming.

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Answer each one before you reveal it.

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Key term

What is eccentricity, and what is its main period?

Key term

How does a greater axial tilt affect the seasons?

Questions from this subtopic

Each one with the model answer underneath.

  1. 1

    What are Milankovitch cycles?

    Model answer

    They are regular variations in the shape of Earth's orbit and the orientation of its axis that change how solar radiation is distributed across the planet and through the year.

  2. 2

    Name the three Milankovitch cycles.

    Model answer

    They are eccentricity, obliquity and precession.

  3. 3

    What is eccentricity, and what is its main period?

    Model answer

    Eccentricity is the degree to which Earth's orbit departs from a circle, and it varies mainly on a cycle of about 100,000 years.

  4. 4

    Define obliquity and state its period and range.

    Model answer

    Obliquity is the tilt of Earth's axis from the perpendicular to the plane of its orbit, and it swings between about 22.1° and 24.5° over roughly 41,000 years.

  5. 5

    How does a greater axial tilt affect the seasons?

    Model answer

    A larger tilt makes summers hotter and winters colder, especially at high latitudes, because the seasonal contrast in insolation increases.

  6. 6

    What is precession, and over what period does it operate?

    Model answer

    Precession is the slow wobble of Earth's axis, which changes the time of year at which the planet is closest to the Sun, on a cycle of roughly 19,000 to 23,000 years.

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