Measure the Earth
Materials: ★★☆ Available in most school laboratories or specialist stores
Difficulty: ★★☆ Can be done by science teachers
Safety: ★☆☆ Minimal safety procedures required
Categories: Astronomy and Space, Measurement and Units
Alternative titles: Eratosthenes Experiment
Summary
Using a stick, a measuring tape, and basic geometry, students can replicate Eratosthenes’ ancient experiment to measure the size of the Earth. By measuring the length of a stick’s shadow during the equinox, they calculate Earth’s circumference with surprising accuracy.
Procedure
- On a sunny day (ideally the equinox), place a straight stick vertically into flat ground.
- Measure the height of the stick.
- At local noon (when the Sun is highest), measure the length of the stick’s shadow.
- Use trigonometry to calculate the angle of the Sun above the horizon.
- Compare the angle measured at your location with data from another location at the same time (historically done between Alexandria and Syene by Eratosthenes).
- Use the difference in angles and the distance between the two locations to estimate the circumference of the Earth.
Links
Measure the Earth: An Easy, At-Home Science Experiment - Plateau Astro:
📄 The Eratosthenes experiment: calculating the Earth’s circumference - Science in School: https://scienceinschool.org/article/2023/calculating-earths-circumference/
Variations
- Collaborate with another school in a different city or country to share shadow data.
- Try the experiment on different days to compare results with equinox measurements.
- Use different stick lengths to check for accuracy and consistency.
Safety Precautions
- Do not look directly at the Sun during the experiment.
- Ensure the stick is firmly placed so it does not fall.
- Perform measurements in a safe, open area away from traffic.
Questions to Consider
- Why is the equinox the best time to perform this experiment? (The Sun is positioned such that shadow angles are easier to compare between different locations.)
- What assumptions did Eratosthenes make about the Earth when performing his experiment? (That Earth is spherical and the Sun’s rays are parallel.)
- How accurate do you expect this method to be compared with modern measurements? (Eratosthenes’ original estimate was within a few percent of today’s accepted value.)
- What are some potential sources of error in this experiment? (Uneven ground, incorrect measurement of shadow length, imprecise timing of local noon.)