A group of people are claiming that the Earth is flat. Meanwhile, much of humanity believes the Earth is round. Who is right, and who is wrong?
Folks: we live in the Internet age, which means we can test these ideas with an EXPERIMENT. To participate, all you need are three one-meter measuring sticks, a sunny day, some flat ground, and an Internet connection. I hereby declare October 24th, 2017 as the day we #MeasureEarth.
What to measure
The goal is to determine the length of shadow your stick creates when you hold it straight up on a specific date at a specific time of day. Then compare the length of shadow you measured with what people in other parts of the world measured.
Wait, why?
Do you expect people at other latitudes to measure the same length of shadow that you measure? Why or why not? What do you expect if the Earth is flat? What if the Earth is round? Discuss with your family, friends, classroom, or in the comments section!
Things you need
Three one-meter measuring sticks, flat ground, Internet connection. Recommended add-ons: a plumb-bob or other device to ensure your stick is vertical, a camera to take photos of your experimental setup, a social media account to post your photos with tag #MeasureEarth.
Procedure
On October. 24th at noon local time (1pm if your region is on Daylight Savings Time, noon otherwise), we #MeasureEarth!
- If it’s sunny, go outside to a location with flat ground.
- Position one measuring stick (henceforth the Shadow-casting stick) vertically. The stick’s entire shadow must fall on the ground for the experiment to work. Optional: use a plumb-bob or other device to keep the stick as close to truly vertical as you can.
- With the other measuring stick(s), measure the length of the shadow created by the Shadow-casting stick.
- Optional: Take photos of your setup! Post them to social media and tag your posts with #MeasureEarth.
- Record the following quantities in the #MeasureEarth Google form:
- your school/classroom/group/own name
- your location (city and country)
- your latitude*
- your longitude*
- the date of the experiment (should be Oct. 24, 2017)
- the clock time of the experiment (e.g., 1:02pm, if that is the time on the clock)
- the length of your Shadow-casting stick (should be 1.0 meters)
- the length of shadow you measured
- optional: the angle of incoming sunlight (see method of calculation below in the basic trigonometry section)
- any comments about what happened during your experiment that might have compromised its quality.
*You can find your latitude and longitude here https://mynasadata.larc.nasa.gov/latitudelongitude-finder/ or at a number of other websites.

Analysis
You did it! Look through the world-wide results to compare the length of shadow you measured to what people in other parts of the world measured. Especially focus on how the length of shadow relates to the experiment’s latitude. Do you notice a pattern? Describe the pattern in as much detail as you can. If you know basic trigonometry, try the analysis in the trig. section below to see if you can get an even clearer description of the pattern.
Conclusion
How does the pattern you observed relate to the pattern you predicted depending on whether Earth is flat or round?
Middle School and up: consider trying…
Basic Trigonometry:
Calculate the length of the shadow divided by the length of the Shadow-casting stick. This is the tangent of the angle between the incoming rays of sunlight and the vertical direction, and we call this quantity tan(θ) (pronounced “tan-theta”). Now take the arctan of tan(θ) to solve for θ, the angle of incoming rays of sunlight. Convert your answer from radians to degrees by multiplying 180/π.
Compare your calculation of θ to what people around the world measured. How does latitude relate to the angle θ? Can you write down a simple equation that describes this rule?
Seasons and Times:
If you did this experiment on a different date of the year or at a different time of day, how might the relationship between latitude and θ change? [NOTE: You can test these predictions by repeating the experiment on the same date a few hours after noon, and at local noon on a date months in the future! Feel free to record your results in the Google form if you do this.]
Circumference of Earth:
Look up the distance between two cities with similar longitudes but different latitudes. What was the difference in θ measured in these two cities? Use the difference in theta, dθ (pronounced “d-theta”), to estimate the circumference of Earth. There are 360 degrees in a circle, so the circumference of Earth is the distance between the two cities times 360 divided by dθ. Compare the circumference you calculated to what’s on the Internet: were you close? The ancient Greek scientist Eratosthenes did a very similar experiment in the third century B.C.

High School and up: Consider trying…
Data Science: Look for other patterns in the data. Compare the measured values of θ to the values of θ you predict in the Trigonometry section based on latitude. What is the difference between the measured and predicted value? Are there any locations around the world with particularly large differences between the predicted and measured values of θ? Why is this happening? What other patterns do you notice in the data, and why might they be there? You can get creative about which fields of the questionnaire you investigate!
Hi Lauren I love this type of approach. I live in the southern hemisphere and resent being lumped in with other “conspirators” like NASA, pilots…just for living on the wrong side of the equator. I have been looking at a modelling approach of near sun (flat Earth) vs far sun (spherical Earth) with location based regressions of solar/lunar behaviour. When you model the sun’s behaviour for a flat Earth in the southern hemisphere you get some really bizarre results.
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Hi Peter! Glad you’re thinking critically about solar system dynamics. As you mention, the flat Earth model requires the sun to be bizarrely close to the Earth to explain changes in the shadow lengths. The sun-Earth distance has been measured with triangulation of the transit of Venus https://rockyworlds.wordpress.com/2017/08/23/the-sun-the-moon-and-venus-oh-my/. At a distance of 93 million miles, the sun is too far away from Earth for changes in shadow length to be due to parallax. I would love to use another transit of Venus as a similar worldwide experiment, but the next one is a hundred years away… 🙂
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Hey Lauren! Great idea, totally going to put this through here in Chile (while I’m here!). I was thinking in creating a small video explaining the experiment… perhaps you would want to work on something similar (and perhaps we could create a common script?). Given this was your idea, I was thinking maybe you should do it and then I could translate it to Spanish. If you are too busy, I can create my own and then perhaps give you the translation ;-).
Cheers!
Néstor
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Hey Néstor, great to hear from you! I have a friend who I can hit up to film a video demonstration. I encourage you to either translate it to Spanish or make your own (or both)–whatever sounds fun to you. 😀
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This is great, I teach an intro Astronomy course atea university and it would make a fun lab!
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Today I’ll be teaching a trig class where we study Erotosthenes’ experiment. I just discovered this online experiment and am trying to set up a return to this idea on Oct 24 so that we can contribute to your data.
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I’m trying to get many children in Oklahoma involved! I believe this might spark some curiosity and wonder! If nothing else, at least I’ll get to go outside for a bit.
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This is a great idea, and I’m going to be participating with my college-level laboratory course. Hopefully there will be enough people that we’ll be able to get into some of the more interesting analysis – do you have any sense of what the level of participation will be?
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About a dozen people have told me they plan to participate. This post has more than 4k page views, so hopefully a few other people will also be inspired to join the fun!
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Reblogged this on Christopher Duston's Home and commented:
Just want to draw some attention to this cool world-side data collection project happening on Oct 24. I am hoping there will be a lot of involvement because I am planning on making this part of a laboratory class I teach here at Merrimack College. The more people who participate, the more data we will have to play with!
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I plan on having my students do this measurement, but one class will do it at 9:00 am, one class at 12:00 pm and one class at 1:00 pm local time (daylight savings time). Should I have all groups record their data in the Google Form? Or just the class that measures at 1:00?
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They should all record their data, and note in the comments section that they are doing the experiment at a different time. Anyone analyzing the results can choose to exclude those data, or to make a special study of how the shadow length changes as a function of the time of day!
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Still hoping to measure, but it’s wet and cloudy in Columbus, Ohio. Fingers crossed!
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