5.4: Measuring the Earth with Eratosthenes (2024)

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    An ancient Greek astronomer named Eratosthenes was the first man to measure the size of the Earth accurately. His method was very simple: he measured the angle made by a shadow cast from a vertical stick in two different cities on the same day and time. With the help of another teacher, you can recreate Eratosthenes’ experiment and your students can measure the size of the Earth for themselves! All you will need is two yardsticks, a protractor, a magnetic compass, and a bit of string.

    Academic Standards

    Science and Engineering Practices

    • Asking questions and defining problems.
    • Planning and carrying out investigations.
    • Analyzing and interpreting data.
    • Using mathematics.
    • Constructing explanations.
    • Argument from evidence.
    • Obtain, evaluate, and communicate information.

    Crosscutting Concepts

    • Scale, proportion, and quantity.
    • Systems and system models.

    Next Generation Science Standards

    • Engineering and design (K-5, 6-8, 9-12).
    • The Earth-Moon system (6-8, 9-12).

    For the Educator

    Facts you need to know

    1. The Earth’s circumference was first accurately measured more than 2,200 years ago by a Greek astronomer named Eratosthenes.
    2. Eratosthenes method was very simple; he measured the length of a shadow from a vertical stick of a known height in two cities on the same day. The ratio between the north-south distance between the two cities and the angles measured gave a ratio which allowed Eratosthenes to calculate the size of the Earth.

    Teaching and Pedagogy

    This is a wonderful example of practical geometry and a powerful introduction into ancient cultures; the activity is not just STEM, but cross-curricular as well. It is a common misconception that just because cultures were ancient, they must have been primitive or simplistic. We often confuse technological sophistication for learning and knowledge. The activity where students actually work together with children from another school is living proof that this is not so.

    This activity is also another example of the practical application of mathematics. Math needn’t be complex or totally divorced from reality; children actually respond and learn better when mathematics are presented in a real-world concept. I can think of no more dramatic answer to the perennial question: “What are we gonna use this math junk for anyway?” than to say: “We’re going to measure the size of the Earth today!”

    Student Outcomes

    What will the student discover?

    1. This is a lovely project for many reasons; as with Activity #10 and #11, students are able to use simple methods to do amazing things, in this case to measure the entire Earth.
    2. Eratosthenes measured the Earth to within 2% of the modern measured value. Using a stick, protractor, and a piece of string you students can easily do as well.

    What will your students learn about science?

    1. Science is a cooperative venture. Without the help of student scientists at another school, this activity is not possible. Even though the activity itself is extremely simple (measure one angle at a specific time of day,) without cooperation nothing is gained.

    Conducting the Activity

    Materials

    1. A meter stick
    2. String or twine
    3. An accurate protractor

    Measuring the Earth with Eratosthenes

    1. The first step is to contact another teacher at your same grade level who lives at least 100 miles directly north or south of you – farther apart is better for this experiment. A direct north-south line between the cities is also important for this, you will need to know as exactly as possible how many miles north or south of you the other school is as opposed to the direct mileage between the cities. Look a map and select a likely city, research their schools on the internet and reach out to someone by email and send them an invitation to join your class in this exciting project. It may take one or two tries, but I bet you can find a partner without too much difficulty!
    2. When the big day arrives, send an email in the morning to be sure you have sunny weather in both cities. A few minutes before noon, set up the yard sticks in the playground area. One stick should be held vertically, (use a small carpenter’s level for this). Use the compass to lay out the second yardstick flat on the ground so that it points directly north. You have now made a simple sundial! Watch as the shadow moves clockwise; when the shadow lies directly along the flat yardstick, measure and record the position where the tip of the shadow falls. Depending on your location and the time of year, the shadow may extend past the end of the flat yardstick – that’s okay, just mark its position with some sidewalk chalk.
    3. Now that you’ve marked the tip of the shadow, stretch a piece of string from the top of the vertical yardstick down to where the tip of the shadow touched the ground. Measure the angle between the vertical stick and the string with a protractor as accurately as you can and record it. Email this information to each other – it will be the difference between the angles that will be important for this activity!
    4. Eratosthenes believed that the Earth was round, and so the angle of the Sun in the sky would be different depending on how far north you were from the equator – and he was right! By setting up a simple ratio and proportion between the difference in the two angles and the distance between the cities, he was able to accurately measure the circumference of the Earth for the first time about 2,300 years ago. Eratosthenes’ calculation for the size of the Earth was accurate to within about 2% of our modern value, how close can your students get? Set up your calculation as shown below!

    5.4: Measuring the Earth with Eratosthenes (2)

    5. The actual circumference of the Earth is 24,900 miles. The example above was done by my own students several years ago and shows a value within 4% of the true size of the Earth – pretty good for kids using some string and a protractor! How close will your students get!

    Discussion Questions

    1. Eratosthenes obviously didn’t have a telephone or the internet, how do you think he managed to do this activity in ancient Egypt? (Egypt was then part of the Greek/Macedonian empire.)
      • Answer: Eratosthenes did not take both measurements on the same day! The astronomer took a measure of the solar angle in the town of Syene in southern Egypt on the summer solstice. He then walked to the town of Alexandria in northern Egypt and carefully measured the distance along the way and measured the solar angle again on the summer solstice in the following year.
    2. We sometimes think of ancient peoples as ‘primitive’ or even ‘ignorant’. What do you think of the ancient Greek culture of Eratosthenes now that you know that people in this era were able to measure the size of the Earth and Moon, and even measure the distance between them accurately?
      • Answer: The ancient cultures were not all ignorant or primitive! Many cultures have had ‘dark ages’ where learning was not advanced, but ancient cultures were in many ways remarkably advanced!

    Supplemental Materials

    Going Deeper

    Understanding what is happening when we measure the solar angle at two different locations, and how this helps us measure the Earth, is a masterpiece of scientific thinking. Sometimes the power of a simple experiment or argument are difficult to grasp.

    One of the ways to comprehend the thinking of Eratosthenes is to draw the Earth and Sun, showing the angles between the Earth’s core and the lines representing the rays of the Sun. See if you can understand Eratosthenes ideas this way!

    There are many drawings of Eratosthenes ideas on the internet to help you!

    Being an Astronomer

    Measuring the solar angle with a stick, string, and protractor is another exercise that can show how the sky changes through the seasons. If your students can measure the solar angle once a week and keep a running record of the results, you will find that the solar angle changes measurably through the seasons.

    Can you find a relation between the solar angle and the season?

    Being a Scientist:

    Climatic change is a hot topic in research and political debate these days, but climate doesn’t just change slowly over centuries. The climatic change of the seasonal weather caused by the change in the solar angle is both powerful and measureable.

    If your students keep a running record of both the solar angle and the average high temperature for each week, and interesting relationship will be revealed.

    Create two graphs, one showing the solar angle over time, the other showing the weekly average high temperature over time. Compare the two graphs; what do you find?

    The Sun is the most powerful factor in our climatic change. By comparing solar angle to temperature fluctuations, we can find a powerful link between how much sunlight we receive and our local temperatures.

    Following Up

    Ancient scientists like Eratosthenes, Pythagoras, Aristotle, and many others contributed to our modern scientific knowledge. Look into some of the ideas and discoveries of these ancient masters and see what you can find!

    5.4: Measuring the Earth with Eratosthenes (2024)

    FAQs

    How Eratosthenes measure the Earth? ›

    Eratosthenes method was very simple; he measured the length of a shadow from a vertical stick of a known height in two cities on the same day. The ratio between the north-south distance between the two cities and the angles measured gave a ratio which allowed Eratosthenes to calculate the size of the Earth.

    How did Eratosthenes measure the Earth's tilt? ›

    Once he knew the circumference and diameter of the Earth, he could calculate the tilt using the maximum length of the same object's shadow throughout the year.

    What was the radius of the earth determined by Eratosthenes? ›

    (C = 2πr) With this information, Eratosthenes inferred that the Earth's radius was 6366 km. Both of these values are very close to the accepted modern values for the Earth's circumference and radius, 40,070 km and 6378 km respectively, which have since been measured by orbiting spacecraft.

    How to measure Earth's circumference? ›

    The distance between the north and south poles is approximately 7900 miles while the equatorial diameter is slightly larger at 7930 miles. The circumference of the Earth is just its average diameter, 7915 miles, times the number pi, where pi is 3.14159. This gives us about 25,000 miles for the Earth's circumference.

    How big did Eratosthenes say the Earth was? ›

    In the third century BCE , Eratosthenes, a Greek librarian in Alexandria , Egypt , determined the earth's circumference to be 40,250 to 45,900 kilometers (25,000 to 28,500 miles) by comparing the Sun's relative position at two different locations on the earth's surface.

    Who compared and arranged the 850 stars according to their brightness? ›

    Hipparchus (161 - 126 BC) had organised earlier Babylonian records together with his own observations to develop a catalogue of 850 stars. He plotted them on a celestial sphere and introduced the concept of comparing brightnesses on a magnitude scale that forms the basis of that still used today.

    How accurate was Eratosthenes calculation? ›

    We don't know which unit Eratosthenes used. If he used the Greek measure, his calculation would have been off by about 16 percent. If he used the Egyptian one, his error would have been less than 2 percent off the actual Earth's circumference of 24,860 miles (40,008 kilometers).

    How did Eratosthenes measure the size of the Earth Quizlet? ›

    How did Eratosthenes estimate the size of Earth? They measured the angle of the Sun above the horizon at midday in two places with different latitude and used the angle to estimate the circumference of Earth.

    How to calculate Earth's tilt? ›

    It is possible to estimate the tilt of the Earth, angle ε (epsilon), by measuring the maximum angular altitude of the Sun (angle alpha, α) during the summer and winter solstices at a particular location, subtracting the maximum angular altitude of the Sun during the summer solstice, angle αs, from the maximum angular ...

    How did Eratosthenes measure the shadow? ›

    He watched the shadow of the gnomon on the day in question, and measured the length of the shadow at noon. The height of the stick and the length of the shadow allowed him to calculate the angle between the vertical at Alexandria (as indicated by the gnomon) and the direction of the Sun's rays at noon.

    Who first measured the Earth? ›

    This illustration shows how Eratosthenes actually calculated the circumference of the Earth. At noon on the summer solstice, Eratosthenes measured the length of the shadow cast by a column of known height at Alexandria.

    What equation did Eratosthenes use? ›

    Eratosthenes divided 360° by 7.2° and got 50, which told him that the distance between Alexandria and Syene (500 miles) was 1/50 of the total distance around the Earth. So he multiplied 500 by 50 to arrive at his estimate of the Earth's circumference: 25,000 miles.

    How to calculate the Earth? ›

    How to Calculate the Circumference of the Earth? The circumference of the Earth can be calculated using the formula, Circumference = 2 πR or π D, where R is the radius of Earth and D is the diameter. By knowing the Equatorial diameter or the polar diameter of the Earth, the circumference can be found.

    What was the method of Eratosthenes? ›

    Eratosthenes sent a man to Syene from Alexandria on foot to measure the distance between Alexandria and Syene. Thus, Eratosthenes measured the distance between the two cities is 800 km. He multiplied by 800 km to 50 and calculated that the Earth's circumference is 40,000 km.

    How did the Egyptians measure the circumference of the Earth? ›

    The Ancient Egyptians did not calculate the circumference of the Earth. It is believed that the Greek mathematician Eratosthenes was the first to do so in the 3rd century BCE. He used the angles of shadows cast by the sun at two different locations to calculate the circumference of the Earth.

    What is the perimeter of the Earth? ›

    Earth's circumference (the distance all the way around the equator) is 24,901 miles (40,075 kilometers). Its diameter (the distance from one side to the other through Earth's center) is 7,926 miles (about 12,756 kilometers).

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