OCR A-Level Geography H481
Coastal Landscapes
Glaciated Landscapes
Dryland Landscapes
Earth’s Life Support Systems
Changing Spaces; Making Places
Trade in the Contemporary World
Global Migration
Human Rights
Power and Borders
Climate Change
Disease Dilemmas
Exploring Oceans
Future of Food
Hazardous Earth
Geographical Skills
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.
What you need to know
Answer each one before you reveal it.
How does a greater axial tilt affect the seasons?
Questions from this subtopic
Each one with the model answer underneath.
- 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
Name the three Milankovitch cycles.
Model answer
They are eccentricity, obliquity and precession.
- 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
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
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
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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