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See how Earth’s motion shapes day and night and the seasons. Explore the Moon’s phases and tides, or choose a location to check sunrise, sunset and Moon times.

Learning guide

What you’ll learn

Explain how Earth’s rotation, its tilted axis and the Moon’s motion affect daylight, seasons, Moon phases and tides.

What to change

Choose a date or location in one of the linked activities.

What to observe

Compare daylight duration, the Moon’s illuminated shape, or the timing and height of tides.

Why it happens

Earth’s rotation causes day and night. Its tilted axis changes seasonal sunlight as Earth orbits the Sun. The Moon’s orbit changes the amount of its sunlit half we can see. The Moon’s and Sun’s gravity cause tides.

Teacher notes

Learning objective: Describe one observed pattern and explain its cause using Earth’s motion, the Moon’s motion or gravity.

Suggested ages: 9–14. Adapt the activity to your group.

Suggested duration: 10–15 minutes for one activity.

Prerequisite knowledge: Earth rotates on its axis and orbits the Sun.

Common misconception: Earth’s shadow causes ordinary Moon phases. Phases arise because we see different amounts of the Moon’s sunlit half; Earth’s shadow causes a lunar eclipse.

Sources: NASA explains seasons and Moon phases. NOAA explains tides. Read our methods and data sources for individual tools.

Model limitations: Illustrations simplify sizes, distances and motion. The seasons diagram compares two solstice positions, viewed edge-on, with the same axis direction. Check each activity’s limitations before using it for measurements.

Lesson status: These are exploration activities. Ages and durations are suggestions, not classroom-tested results. Lesson development and unfinished drafts are separate.

Sunrise & Sunset

The cities below run north to south. The farther from the equator, the more day length swings with the season — long summer days, short winter ones.

Earth’s Tilt, the Sun & Seasons
Earth’s fixed axial tilt at the two solstices An edge-on view of Earth’s orbital plane. Both north poles point up and right. At the left position, the Northern Hemisphere tilts toward the Sun in June. At the right position, the Southern Hemisphere tilts toward the Sun in December. The axis is tilted 23.4 degrees from the perpendicular to the orbital plane. The axis keeps the same direction Sun 23.4° NS 23.4° NS June solsticeDecember solstice North tilts toward SunSouth tilts toward Sun

Two positions in Earth’s orbit, viewed edge-on. The horizontal line marks the orbital plane; the vertical guides are perpendicular to it. Sizes and distances are not to scale.

Earth carries the same 23.4° tilted axis around the Sun. That tilt changes the angle of sunlight and the hours of daylight, giving the hemispheres opposite seasons.

  • What is a solstice? A solstice marks the longest or shortest day of the year in each hemisphere.

  • What is an equinox? An equinox is the moment the Sun crosses Earth’s equator, around March and September.

Sun, Earth & Moon Simulator

Where the sun and moon are from your town, at any moment.

Keep exploring day and night, seasons, Moon phases and tides. Or jump across: All · Space · Time.