What Causes the Seasons?
Learning Target
The model of the solar system can explain that the seasons are a result of the tilt of the earth and are caused by the differing amounts of sunlight on different areas of Earth across the year.
Success Criteria
Using a model I can predict...
...the season on Earth, given the relative positions of Earth and the sun (including the orientation of the Earth’s axis) and a position on Earth.
...the relative positions of Earth and the sun when given a season and a relative position (e.g. far north, far south, equatorial) on Earth.
Questions to Ponder
In many different climates around the world, the different seasons bring very different weather.
What is your requirement for having a "perfect weather" day?
Why Do We Have Seasons?
Explore what causes seasons on Earth in this interactive adapted from NASA materials that features four cities at different latitudes.
Use this resource to view how Earth’s axial tilt causes seasons from different perspectives and to develop and use models of sunlight received at Earth’s surface.
Background Reading
Earth is in constant motion. Approximately every 365 days, Earth completes one revolution around the Sun, and approximately every 24 hours, Earth completes one rotation around its axis. Because Earth's axis of rotation is not perpendicular to the plane of Earth's orbit—it is tilted about 23.5 degrees—the way in which the Sun's light hits Earth's surface varies during the course of the orbit. The seasons—predictable patterns of temperature and precipitation over the course of each year that locations on Earth experience—are due to a combination of the tilt of Earth's axis and its place in its orbit.
The angle at which light strikes a surface greatly affects the amount of energy that the surface receives. For example, when a flashlight is positioned directly over a piece of paper, all the light is concentrated on a given circular area of the paper so that the paper receives direct, intense light from the source. However, if the paper is tilted and the same amount of light hits it at an angle, the light is spread out over a greater area and the intensity with which it hits that area is reduced. This idea also applies to the energy radiating from the Sun.
The orientation of Earth's axis relative to the Sun changes throughout the year. When the north pole of Earth's axis is pointed toward the Sun, it is summer in the Northern Hemisphere and winter in the Southern Hemisphere. During this time of year, the Northern Hemisphere receives more direct sunlight than the Southern Hemisphere. The Sun appears higher above the horizon, and its light takes a more direct path through the atmosphere. This results in less scattering of energy and a higher concentration of sunlight over the area—the most important factor for seasonal changes. In addition, daylight lasts longer, allowing more time for the radiation to warm the surface. Alternatively, when the north pole of Earth's axis is pointed away from the Sun, it is winter in the Northern Hemisphere and summer in the Southern Hemisphere.
Contrary to a popular misconception, variations in the distance of Earth from the Sun play a very minor role in temperature changes. Earth's orbit is nearly circular—our planet is always about 150 million kilometers (93 million miles) away from the Sun. In illustrations, Earth's orbit is commonly shown as an oval encircling the Sun—the noncircular shape is due to a perspective view of the nearly circular orbit. The change in distance between the Sun and Earth is minimal and has very little effect on the amount of energy that Earth receives.
Start Here...
Click on the link to right, read the introduction and then click LAUNCH to begin the simulation.
Follow the directions below as you make your way through the simulation:
Draw a diagram of the Sun/Earth System in your notebook. (be sure to include the Earth's tilt on its axis.)
Click on the points on Earth's orbit around the Sun to learn about that time of year.
Change the city location (New York, USA 41°N, Miami, USA 26°N, Singapore, 1°N, Melbourne, Australia 38°S) to see how they are similar and different as the Earth is in different positions in its orbit.
Read the tabs on the side (About Seasons, Earth's Orbit, Sun's Path In The Sky, Sun's Angle, Seasonal Lag) and add any notes to your science notebook.
Discussion Questions
How does the position of the Sun in the sky affect the intensity of sunlight striking Earth's surface?
Why is it winter in the southern hemisphere when it is summer in the northern hemisphere?
3 Minute Model
Using what you have learned about the cause of seasons, create a model to demonstrate that knowledge.
Remember! - A model can take many forms; physical, mental, etc.
Everybody must talk!
Seasons Animation
View this link to see another animation about seasons on Earth.
Why does the highlighted area change shape over time?
How does the animation relate to the seasons on Earth?
Individual Assessment
Answer the following questions by yourself. You may use your notes as you answer the questions.
Meteorology