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Milankovitch Cycles (HL) (DP IB Environmental Systems & Societies (ESS)) : Revision Note

Alistair Marjot

Written by: Alistair Marjot

Reviewed by: Jacque Cartwright

Updated on

Milankovitch Cycles

  • Milankovitch cycles describe three long-term changes in Earth's position and movement relative to the Sun

    • These cycles impact the amount of solar radiation Earth receives

    • This influences the climate over very long timescales (tens to hundreds of thousands of years)

  • The cycles contribute to natural climate patterns such as:

    • Ice ages

    • Warmer interglacial periods

Three types of Milankovitch cycles

1. Eccentricity (shape of Earth’s orbit)

  • Eccentricity refers to the shape of Earth's orbit around the Sun

  • This orbit changes from a more circular shape to a more elliptical shape over a cycle of about 100,000 years

    • When the orbit is more elliptical, Earth’s distance from the Sun varies more

      • This creates larger differences in solar radiation received at different times of the year

    • When the orbit is more circular, the distance from the Sun remains more constant

      • This leads to smaller differences in seasonal temperatures

  • Climate impact:

    • Lower eccentricity (circular orbit) results in milder seasonal differences

    • This milder climate can allow ice sheets to slowly build up over time, especially in polar regions

    • If the Earth’s tilt is also smaller, the poles receive less direct sunlight, making it harder for ice to melt

    • As a result, snow and ice accumulate

    • This can lead to the onset of a glacial period or ice age

2. Obliquity (tilt of Earth's axis)

  • Axial tilt refers to the angle at which Earth's axis tilts in relation to its orbit around the Sun

    • The tilt angle changes from about 22.5° to 24.5° over a cycle of approximately 41,000 years

    • Greater tilt increases the intensity of seasons, making summers warmer and winters colder

  • Climate impact:

    • A higher tilt (closer to 24.5°) creates stronger seasonal contrasts

      • This can reduce the buildup of polar ice by making summers warmer

    • A lower tilt (closer to 22.1°) reduces seasonal contrasts

      • This allows ice to persist at the poles and contributes to glaciation

3. Precession (wobble of Earth's axis)

  • Axial precession is the wobble in Earth's rotational axis

    • This cycle takes approximately 26,000 years and causes the timing of seasons to shift

    • As Earth wobbles, the position of the North Star gradually changes

  • Climate impact:

    • Precession affects the seasonal distribution of solar radiation

    • This can lead to warmer or cooler summers and winters

      • This depends on where Earth is in its orbit when each season occurs

Diagram showing Milankovitch cycles: eccentricity (orbit shape), obliquity (Earth's tilt), and precession (wobble affecting star alignment).
The shape, tilt and wobble of Earth's movement, over thousands of years, affects long-term climate

Milankovitch cycles and climate change

  • The combined effects of eccentricity, obliquity, and precession drive long-term climate shifts, like the Ice Ages

    • Positive feedback loops amplify these climate shifts

      • For example, cooling from reduced solar radiation can lead to glaciation

        • This snow and ice reflect sunlight (albedo effect) and cause further cooling

      • Warming increases carbon dioxide, enhancing the greenhouse effect and leading to interglacial periods

  • Role of carbon dioxide:

    • Lower temperatures reduce carbon dioxide in the atmosphere, enhancing cooling

      • Cooler temperatures make the atmosphere less able to hold gases like carbon dioxide, which the oceans or soils then absorb

    • Higher temperatures release more carbon dioxide, enhancing warming

      • This occurs because warmer temperatures increase the rate at which carbon dioxide is released from sources like soils, oceans, and plant life

      • This increases atmospheric carbon dioxide levels

Real-world examples

  • Last glacial maximum:

    • It occurred approximately 20,000 years ago when eccentricity, axial tilt, and precession aligned to favour cooling

    • Resulted in extensive ice sheets covering parts of North America and Europe

  • Current interglacial period:

    • We are currently in a warmer interglacial period called the Holocene, which began around 11,700 years ago

    • This period has allowed the development of human civilisation due to the relatively stable and warmer climate

Examiner Tips and Tricks

Although Milankovitch cycles explain natural long-term climate patterns, they do not explain recent, rapid global warming, which is mainly due to human activities like fossil fuel burning.

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Alistair Marjot

Author: Alistair Marjot

Expertise: Biology & Environmental Systems and Societies Content Creator

Alistair graduated from Oxford University with a degree in Biological Sciences. He has taught GCSE/IGCSE Biology, as well as Biology and Environmental Systems & Societies for the International Baccalaureate Diploma Programme. While teaching in Oxford, Alistair completed his MA Education as Head of Department for Environmental Systems & Societies. Alistair has continued to pursue his interests in ecology and environmental science, recently gaining an MSc in Wildlife Biology & Conservation with Edinburgh Napier University.

Jacque Cartwright

Reviewer: Jacque Cartwright

Expertise: Geography Content Creator

Jacque graduated from the Open University with a BSc in Environmental Science and Geography before doing her PGCE with the University of St David’s, Swansea. Teaching is her passion and has taught across a wide range of specifications – GCSE/IGCSE and IB but particularly loves teaching the A-level Geography. For the past 5 years Jacque has been teaching online for international schools, and she knows what is needed to get the top scores on those pesky geography exams.

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