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Live From...the Hubble Space Telescope
Star Census Classroom Collaboratory

This activity was about students making data observations, analyzing the data locally and then sharing their results with one another.

To encourage students to observe the quality of the night sky and to determine the number of stars that can be seen from their local area.

Ask students how many stars there are outside at night. Accept all estimates and record them on the chalkboard. Ask how they could go beyond guesses and estimates. Tell students that they are going to devise a way to count the stars in the sky.

Ask students to explain the phrase "Twinkle, Twinkle, Little Star". Ask them what "twinkling" means. Explain to students that only stars twinkle--the moon and planets do not. As a group, make the predictions as suggested on the activity sheet below. Pick a time for students to make night-time observations of stars.


  • measuring activity sheet
  • empty paper towel or toilet paper tube (must be 3 times longer than the distance across the opening!)
  • scissors
  • ruler
  • a protractor
  • a compass (to determine North, etc.)

Plan a time for students to take a "Star Census". Review with students how to do the counting. If possible, it would be interesting to have students make these observations in different locations (near a city or out in the country) and at different times (when there's a bright moon and when there's no moon). For younger students, you can use fewer observations. Just remember that each observation represents 1/144th of the sky. If students make only 6 observations, they would multiply the total number of stars observed by 24 (which is 144 divided by 6).

Have your students try this experiment (at night at the agreed upon time) to measure the number of stars you can see.

  1. Make an "Observing Device" from a bathroom tissue or paper towel tube. Measure the diameter of your tube. Cut its length to be three times its diameter. Through the tube, you will see only a small portion of the sky. It would take 144 tubes to cover the whole sky.

    One by one, face in each of the 4 compass directions (North, South, East and West).

    Hold the tube 3/4 of the way up from the horizon in each direction and count the number of stars seen through the tube. Hold the tube half-way up from the horizon and repeat the count. Repeat the procedure again with the tube pointed a third of the way up. Repeat observations for the other directions.
    (To determine 3/4, 1/2 and 1/3, students can either use a protractor or they can simply estimate the angle)

  2. Add up the number of stars for all 12 sightings. If it takes 144 tubes to cover the sky, then you have observed 1/12th of the sky. Multiply your sub-total by 12 to estimate the total number of stars in the sky. Estimated total number of stars: (includes the stars above and below the horizon)

  3. Add up and compare the three measurements in each direction. Why do you see more stars in certain directions?

Remind students that they need to take RANDOM samples. That means that they need to use the samples where they see no stars at all, not drop that sample in favor of one where they see stars. In urban situations, kids are likely to have "blank" samples. That's what light pollution does to our skies. If kids in urban areas sample UNTIL they have 12 samples with stars, then they are going to have false high readings.

There were two parts to the online connection
1) a quick look at some simple data observed between March 15 - 22
2) a more detailed, longer time frame collaboration

Part 1:
For the quick look part, students counted the number of stars they saw as detailed above. As a class, come up with one number which is a good average of the count in your area. (Don't forget to multiply by 12 to estimate the total number of stars in the whole sky). Classrooms then sent that one number, along with their city, state (and country if not US), latitude and longitude to us.

Part 2:
We hope that teachers will also work with their students to prepare reports from their observations which better reflect the complexities of the task. For example, how do the following factors effect the numbers:
- weather
- proximity to surface lighting
- time of night that the observations were made
- size of the moon (if you take make observations over time)
- etc, etc

Hopefully the class can together produce a report that includes the original data and the conclusions that were derived from analyzing this data.

As an additional activity, classes examined other reports and 1) got ideas for improving their original report
2) derived new meaning by comparing data from other locations (for example, students may learn that students in the mountains see more stars then those closer to sea level).

The format of these reports was up to the individual teachers. Graphs and other visuals would make reports more attractive to others, if your class can find something meaningful to graph. Charts of the real data collected might be interesting to some. Students were incouraged to be as creative as they could, since their audience would be other engaged classrooms across the county and the world.

One related resource which you may find interesting is Dave Nash's discussion about light pollution.


Have you ever wondered what makes a star twinkle? On the next clear night look at a bright star.

  • How many blinks does it make in 10 seconds?
  • Look at the moon, an airplane or a bright planet at night. Do these objects twinkle?

A star is a point of light. It is so far away that even the largest telescope cannot show the star's disk. The atmosphere changing between the star and your eye causes starlight to twinkle.

Make these predictions about twinkling:

    a. Do stars lower in the sky or higher, twinkle more?
    b. Do stars twinkle more on a windy night, or a still night?
    c. Do stars twinkle more at sea level or on a mountain top?
    d. Do stars also change color as they twinkle?
Hint: Count star blink rates to answer the first question.

Share your data with students in other locations to answer the remaining questions.

"Seeing" is the term astronomers use to describe the steadiness of images. "Seeing" is best when the twinkling is least. When the seeing is good, astronomers can collect better data about the brightness and color of distant stars and galaxies.

  • Estimate how many stars you can see at night?
  • Do you see more stars in the city, or out in the country?
  • Do you see more stars on a moonless night or when there's a full moon?

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