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Classroom Activities

Activity: Time Travel to the Edge of the Universe and Back!

Instructional Objectives
Background Information
Time Needed for Activity
Target Grade Level
Web Resources

Instructional Objectives:

Students will -

  1. study the size of the universe,
  2. calculate the time to travel to near and distant destinations,
  3. construct a time scale model of the universe by using time travel distances.

Background Information:

When we observe the night sky, the planets, stars and galaxies appear to be close together. We know that some objects are closer to the Earth than others and that enormous distances separate us from other objects in the universe. As we gather information from the farthest reaches of the universe, we can learn about the history of the universe.

Distances to objects in the universe are measured indirectly and take advantage of the parallax effect. When an object is being measured against a stationary background, it appears to move when observed from two different points. The amount that an object appears to shift is determined by the distance to the object being observed and the distance between the two points of observation (the baseline). Because we have two eyes, we use parallax constantly to judge distances to objects.

To learn more about parallax, try the activities in Project Earth Science: Astronomy, P. Sean Smith, NSTA Publications, 1992.

Time Needed for Activity:

45-50 minutes

Target Grade Level:

High School (Note: Middle school extensions and advanced high school extensions are provided below.)



Distances to stars and celestial objects are immense. Cars travel at an average of 60 miles/hour, jets fly at about 600 miles/hour, and rockets travel through space at 25,000 miles/hour. Imagine that with new technolgy you can build a time machine that travels at light speed, or 186,000 miles/second. The unit used to express stellar distance is the light-year, which is the distance that light travels in a year (5.8 trillion miles or 9.46 x 1012 kilometers). With the unit of light-years, we can begin to make sense of the very great distances between objects in the universe and begin our time travel exploration.

1. Using the chart below, calculate the travel time from the Earth to the destinations given.

Planets & GalaxiesDestination Distance from Earth
Time at Light Speed
Moon 0.000000038 1.1991888 seconds
Sun 0.000016 8.41536 minutes
Mercury 0.0000095 4.99662 minutes
Venus 0.00000476 2.5035696 minutes
Mars 0.0000076 3.997296 minutes
Jupiter 0.0000666 35.028936 minutes
Saturn 0.000135 1.18341 hours
Uranus 0.000285 2.49831 hours
Neptune 0.00046 4.03236 hours
Pluto 0.0006183 5.4200178 hours
Alpha Centauri 4.27 4.27 years
Sirius (Dog star) 8.7 8.7 years
Arcturus 36 36 years
Pleiades Cluster 400 400 years
Betelgeuse 520 520 years
Deneb 1,600 1,600 years
Crab Nebula 4,000 4,000 years
Center of Milky Way 38,000 38,000 years
Magellanic Clouds 150,000 150,000 years
Andromeda Galaxy 2,200,000 2,200,000 years

2. Suspend the string or clothesline from the ceiling in your classroom or stretch it along the length of the hallway. Determine an appropriate scale, depending on whether you want to show the edge of the universe, approximately
15 billion light-years away, or the objects closer to the Earth, for which you will use a scale of 3 million light-years. Mark the scale on the string or clothesline.

3. Give each student a card. Have them record the name of the object that is their destination and the time distance to travel there. Use paper clips to attach the cards to the string at the appropriate distances on your scale. (Extension: Use the images from the Hubble Space Telescope and add artwork to each card. Select additional locations for students to add to their time line from the program and from the Hubble Space Telescope observations.)

4. The chart and travel time line represent a glimpse into the past. In a sense, our time travel is like a time machine. When we look at the history of the universe, what can we learn? What evidence have scientists gathered with new technologies and the Hubble Deep Field Project?

5. Because of the finite speed of light, we are restricted to studying our observable universe. Discuss with your class the question, "Are there other universes?" What hypotheses can they make?


Web Resources:

Amazing Space

SEDS Home Page

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PBS Online