Why Do We Have Seasons? Axial Tilt, Sunlight Angles, and the Earth-Sun-Moon System
Shared by A STEM Educator
Students will be able to explain that Earth's seasons result from axial tilt causing changes in the angle and duration of sunlight received at different latitudes, and will distinguish this from the common misconception that Earth's distance from the Sun drives seasonal temperature change.
Lesson Overview
Students investigate how Earth's 23.5° axial tilt — not its distance from the Sun — causes seasons by exploring how the angle of incoming sunlight affects energy concentration on Earth's surface. Real-world connections to solar panel optimization and agricultural planning anchor the learning.
Materials
- Foam globe (one per group of 3–4 students) with axis marked at 23.5°
- Bright flashlight or small LED lamp (one per group)
- Protractor (one per group)
- Graph paper (one sheet per student)
- Ruler (one per group)
- Dark construction paper (one sheet per group, for shadow/spread tracing)
- Colored pencils (red and blue)
- Printed lab recording sheet (one per student)
- Whiteboard markers and personal whiteboards or blank paper for VNPS
- Tape measure or meter stick
- Solar irradiance calculation worksheet (Elaborate phase)
- Exit slip cards (pre-printed, one per student)
Scaffolded Task Progression
[ Interactive graph / diagram — available in the full lesson ]
| Position | Hemisphere with More Direct Light | Season in N. Hemisphere | Season in S. Hemisphere |
|---|---|---|---|
| June Solstice (N. Pole toward Sun) | ? | ? | ? |
| December Solstice (N. Pole away from Sun) | ? | ? | ? |
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