Seasons and Sunlight

Change axial tilt, orbit position and latitude to compare noon sunlight and daylight duration.

Grades 3–5 · Earth Science

Explore one idea

Seasons and Sunlight

Your goal

Explore latitude 45° with 24° tilt at orbit position 90°. Compare the noon angle and daylight with the equator.

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Earth orbit location and Sun-facing axis projection with local sunlight comparisonSunOrbit position 0°Circular orbit keeps distance constantNSunlightNoon angle 90.0°Marked latitude 0° at noonDaylight 12.0 h

Reduced motion is on. The controls still update the scene.

At latitude 0°, noon Sun altitude is 90.0° and daylight lasts 12.0 hours. Solar declination is 0.0°.

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Axial tilt changes sunlight angle and day length. This circular orbit deliberately holds Sun distance constant. Earth sizes and orbit distances use independent drawing scales. The enlarged globe shows the Sun-facing projection of the axis; local angle and day length use spherical geometry without atmosphere. Real Earth tilts about 23.4°.

Learn with Seasons and Sunlight

Seasons and Sunlight lets elementary learners change the tilt of Earth, move around a circular orbit, and choose a latitude. Read the noon Sun angle and daylight hours as the northern and southern hemispheres take turns leaning toward sunlight. Compare a tilted Earth with zero tilt to see why changing distance from the Sun is unnecessary for this seasonal pattern. The diagram separates an orbit view from an enlarged globe, while numerical readings connect a local observation with the geometry of the whole planet.

What to look for

Keep distance fixed

Watch sunlight change even though the circular orbit keeps Sun distance constant.

Compare hemispheres

Switch latitude from positive to negative while keeping the same orbit position.

Remove the tilt

Set tilt to zero and compare daylight at several positions.

For teachers and curious learners

Explain how axial tilt changes sunlight angle and day length through a year. Ask students to predict what will happen, change one setting, and explain what they observe. Learn gives a starting point. Practice and Challenge offer new goals with the same scene.

Circular Earth orbit, a spherical surface and no atmospheric refraction. Sizes and orbital distances use separate drawing scales; real Earth tilt is about 23.4 degrees.

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