5.4: Measuring the Earth with Eratosthenes (2024)

  1. Last updated
  2. Save as PDF
  • Page ID
    31557
  • \( \newcommand{\vecs}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}}}\)

    \( \newcommand{\vecd}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash{#1}}} \)

    \( \newcommand{\id}{\mathrm{id}}\) \( \newcommand{\Span}{\mathrm{span}}\)

    ( \newcommand{\kernel}{\mathrm{null}\,}\) \( \newcommand{\range}{\mathrm{range}\,}\)

    \( \newcommand{\RealPart}{\mathrm{Re}}\) \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\)

    \( \newcommand{\Argument}{\mathrm{Arg}}\) \( \newcommand{\norm}[1]{\| #1 \|}\)

    \( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\)

    \( \newcommand{\Span}{\mathrm{span}}\)

    \( \newcommand{\id}{\mathrm{id}}\)

    \( \newcommand{\Span}{\mathrm{span}}\)

    \( \newcommand{\kernel}{\mathrm{null}\,}\)

    \( \newcommand{\range}{\mathrm{range}\,}\)

    \( \newcommand{\RealPart}{\mathrm{Re}}\)

    \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\)

    \( \newcommand{\Argument}{\mathrm{Arg}}\)

    \( \newcommand{\norm}[1]{\| #1 \|}\)

    \( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\)

    \( \newcommand{\Span}{\mathrm{span}}\) \( \newcommand{\AA}{\unicode[.8,0]{x212B}}\)

    \( \newcommand{\vectorA}[1]{\vec{#1}} % arrow\)

    \( \newcommand{\vectorAt}[1]{\vec{\text{#1}}} % arrow\)

    \( \newcommand{\vectorB}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}}}\)

    \( \newcommand{\vectorC}[1]{\textbf{#1}}\)

    \( \newcommand{\vectorD}[1]{\overrightarrow{#1}}\)

    \( \newcommand{\vectorDt}[1]{\overrightarrow{\text{#1}}}\)

    \( \newcommand{\vectE}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash{\mathbf {#1}}}} \)

    \( \newcommand{\vecs}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}}}\)

    \( \newcommand{\vecd}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash{#1}}} \)

    \(\newcommand{\avec}{\mathbf a}\)\(\newcommand{\bvec}{\mathbf b}\)\(\newcommand{\cvec}{\mathbf c}\)\(\newcommand{\dvec}{\mathbf d}\)\(\newcommand{\dtil}{\widetilde{\mathbf d}}\)\(\newcommand{\evec}{\mathbf e}\)\(\newcommand{\fvec}{\mathbf f}\)\(\newcommand{\nvec}{\mathbf n}\)\(\newcommand{\pvec}{\mathbf p}\)\(\newcommand{\qvec}{\mathbf q}\)\(\newcommand{\svec}{\mathbf s}\)\(\newcommand{\tvec}{\mathbf t}\)\(\newcommand{\uvec}{\mathbf u}\)\(\newcommand{\vvec}{\mathbf v}\)\(\newcommand{\wvec}{\mathbf w}\)\(\newcommand{\xvec}{\mathbf x}\)\(\newcommand{\yvec}{\mathbf y}\)\(\newcommand{\zvec}{\mathbf z}\)\(\newcommand{\rvec}{\mathbf r}\)\(\newcommand{\mvec}{\mathbf m}\)\(\newcommand{\zerovec}{\mathbf 0}\)\(\newcommand{\onevec}{\mathbf 1}\)\(\newcommand{\real}{\mathbb R}\)\(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\)\(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\)\(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\)\(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\)\(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\)\(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\)\(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\)\(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\)\(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\)\(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\)\(\newcommand{\bcal}{\cal B}\)\(\newcommand{\ccal}{\cal C}\)\(\newcommand{\scal}{\cal S}\)\(\newcommand{\wcal}{\cal W}\)\(\newcommand{\ecal}{\cal E}\)\(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\)\(\newcommand{\gray}[1]{\color{gray}{#1}}\)\(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\)\(\newcommand{\rank}{\operatorname{rank}}\)\(\newcommand{\row}{\text{Row}}\)\(\newcommand{\col}{\text{Col}}\)\(\renewcommand{\row}{\text{Row}}\)\(\newcommand{\nul}{\text{Nul}}\)\(\newcommand{\var}{\text{Var}}\)\(\newcommand{\corr}{\text{corr}}\)\(\newcommand{\len}[1]{\left|#1\right|}\)\(\newcommand{\bbar}{\overline{\bvec}}\)\(\newcommand{\bhat}{\widehat{\bvec}}\)\(\newcommand{\bperp}{\bvec^\perp}\)\(\newcommand{\xhat}{\widehat{\xvec}}\)\(\newcommand{\vhat}{\widehat{\vvec}}\)\(\newcommand{\uhat}{\widehat{\uvec}}\)\(\newcommand{\what}{\widehat{\wvec}}\)\(\newcommand{\Sighat}{\widehat{\Sigma}}\)\(\newcommand{\lt}{<}\)\(\newcommand{\gt}{>}\)\(\newcommand{\amp}{&}\)\(\definecolor{fillinmathshade}{gray}{0.9}\)

    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

    5.4: Measuring the Earth with Eratosthenes? ›

    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 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.

    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 did Eratosthenes measure the size of the Earth Quizlet? ›

    Eratosthenes measured the circumference of the earth by measuring the distance between two cities. Then he measured the angle of sunlight relative to the vertical on the summer solstice. The sun was overhead in Alexandria but seven degrees away from the vertical in Syene.

    How to calculate the size of the Earth? ›

    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 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.

    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.

    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.

    What did Eratosthenes mean by geography? ›

    In Greek, geo- means “earth” and -graphy means “to write.” Using geography, Eratosthenes and other Greeks developed an understanding of where their homeland was located in relation to other places, what their own and other places were like, and how people and environments were distributed.

    How long would it take to walk around the Earth? ›

    How long to walk around the Earth. If you were to walk around the world at an adult's average walking speed of 4.82 km/h (3 mph) it would take you roughly 8,313 hours and 20 minutes. That's just shy of a full year of non-stop walking.

    How did Eratosthenes measure the size of the Earth in 240? ›

    Eratosthenes estimated the size of the Earth in 240 BC by comparing the maximum altitude of the Sun in two cities located at different latitudes. He observed the angle of the Sun's rays at noon on the summer solstice at two different locations in Egypt: Alexandria and Syene (modern-day Aswan).

    What field of mathematics did Eratosthenes use to calculate the circumference of the earth? ›

    Eratosthenes knew the distance between two cities, he had the angle of the sun measured in each city at local noon on the same day. Using trigonometry he was able to calculate fairly closely the radius of the earth, which gives the diameter and distance around. This was about 250 BC.

    What is the circumference 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).

    How did we measure the size of Earth? ›

    Measurement of Earth's circumference has been important to navigation since ancient times. The first known scientific measurement and calculation was done by Eratosthenes, by comparing altitudes of the mid-day sun at two places a known north–south distance apart.

    What is Earth's real size? ›

    Therefore, the diameter of Earth through its center is 7,926 miles (12,756 km). Again, because of the equatorial bulge, the planet's diameter is slightly smaller when measured from pole to pole, where it is about 7,900 miles (12,712 km). The equatorial circumference of Earth is 24,901 miles (40,075 km).

    What did Eratosthenes think of the earth? ›

    Yet his most lasting achievement was his remarkably accurate calculation of the Earth's circumference (the distance around a circle or sphere). He computed this by using simple geometry and trigonometry and by recognizing Earth as a sphere in space.

    What is 250 000 stadia equal to? ›

    Answer: From his measurements, he computed the circumference of the Earth to be approximately 250 000 stadia (a stadium is a unit of measurement used to describe the size of a typical stadium at the time), about 40 000 kilometers.

    What is the diameter of the Earth? ›

    Its diameter (the distance from one side to the other through Earth's center) is 7,926 miles (about 12,756 kilometers). Earth is slightly smaller when measured between the North and South Poles which gives a diameter of 7,907 miles (12,725 kilometers).

    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.

    References

    Top Articles
    Aktivatours kortingscodes
    What Does the Bible Say About Church Triumphant?
    Netronline Taxes
    Maxtrack Live
    Top 11 Best Bloxburg House Ideas in Roblox - NeuralGamer
    Bild Poster Ikea
    Air Canada bullish about its prospects as recovery gains steam
    Encore Atlanta Cheer Competition
    Bluegabe Girlfriend
    Kentucky Downs Entries Today
    Slapstick Sound Effect Crossword
    1TamilMV.prof: Exploring the latest in Tamil entertainment - Ninewall
    Daniela Antury Telegram
    How Quickly Do I Lose My Bike Fitness?
    Mid90S Common Sense Media
    Craigslist Jobs Phoenix
    Blog:Vyond-styled rants -- List of nicknames (blog edition) (TouhouWonder version)
    Wisconsin Women's Volleyball Team Leaked Pictures
    Gmail Psu
    History of Osceola County
    Overton Funeral Home Waterloo Iowa
    Canvas Nthurston
    Craigslist Toy Hauler For Sale By Owner
    Grayling Purnell Net Worth
    Beryl forecast to become an 'extremely dangerous' Category 4 hurricane
    Lista trofeów | Jedi Upadły Zakon / Fallen Order - Star Wars Jedi Fallen Order - poradnik do gry | GRYOnline.pl
    Wsop Hunters Club
    Samantha Aufderheide
    Spn 520211
    Puretalkusa.com/Amac
    Ceramic tiles vs vitrified tiles: Which one should you choose? - Building And Interiors
    480-467-2273
    Churchill Downs Racing Entries
    Gen 50 Kjv
    Pulitzer And Tony Winning Play About A Mathematical Genius Crossword
    The Clapping Song Lyrics by Belle Stars
    Big Boobs Indian Photos
    Toonkor211
    Sinfuldeed Leaked
    Eegees Gift Card Balance
    Ravens 24X7 Forum
    Lucky Larry's Latina's
    Main Street Station Coshocton Menu
    Gold Dipping Vat Terraria
    Restored Republic June 6 2023
    Worcester County Circuit Court
    Kb Home The Overlook At Medio Creek
    'The Night Agent' Star Luciane Buchanan's Dating Life Is a Mystery
    Accident On 40 East Today
    Phunextra
    Ingersoll Greenwood Funeral Home Obituaries
    Electronics coupons, offers & promotions | The Los Angeles Times
    Latest Posts
    Article information

    Author: Neely Ledner

    Last Updated:

    Views: 5833

    Rating: 4.1 / 5 (62 voted)

    Reviews: 93% of readers found this page helpful

    Author information

    Name: Neely Ledner

    Birthday: 1998-06-09

    Address: 443 Barrows Terrace, New Jodyberg, CO 57462-5329

    Phone: +2433516856029

    Job: Central Legal Facilitator

    Hobby: Backpacking, Jogging, Magic, Driving, Macrame, Embroidery, Foraging

    Introduction: My name is Neely Ledner, I am a bright, determined, beautiful, adventurous, adventurous, spotless, calm person who loves writing and wants to share my knowledge and understanding with you.