Think about this for a moment: If the Universe is infinite, it has unlimited volume; if the Universe is finite, it has a limited, measurable volume. Remember now, we are not talking about boundaries, for this is another matter. A boundary is an edge of space. If we were to reach a boundary in space, we can go no farther.
In general, the human mind tends to have the following conception: if the size of something is finite, then it must have an edge or boundary of some sort. For it to have no edge or boundary, it must be infinite. So since we can't conceive of coming to the edge of space (after all, what would then be outside it?), space must be infinite.
We will explore this misconception in this exercise. In doing so, we will exercise our abilities in both deductive and inductive reasoning. Deductive reasoning is the process of demonstrating that if certain statements are true, then other statements can be shown to follow from them. Inductive reasoning stems from making conjectures based on observations and the patterns we see emerge from observations. Both forms of reasoning will be used in investigating the shape of our Universe.
We will see that there are shapes which are finite in size, but which have no boundaries. We will have to let go of many of the limitations put on us by our familiarity with the 3-dimensional world in which we live. Be prepared to think differently. Remember that in the following exercises we get to see more than we would see if we were confined to the surfaces we will investigate -- because we have another dimension or two available to us from which to look!
In this lesson, students will examine various "spaces" (including ones that are one-dimensional, two-dimensional, and three-dimensional). For each space, they will examine what it means to have or not have an edge, or to be finite or infinite.
Line segment: finite with boundary; Circumference of Circle: finite with no boundary; Ray: infinite with boundary; Line: infinite with no boundary
Interior of circle: finite with boundary; Surface of Sphere: finite with no boundary; Half plane: infinite with boundary; Plane: infinite with no boundary
Both are finite with no boundaries.
A 3-torus is finite with no boundary.
In this lesson, students will explore the concept of whether or not there is a "center" to the Universe. The lesson begins with an exercise in deductive reasoning and direct proof. This is followed by hands-on activities where they will observe for themselves that, when space is expanding, where the center is depends completely on from where you observe the expansion!
Answer Key and Instructions
If the Universe began with an explosion, then the Universe must be expanding. If the Universe is expanding, it has no center. Therefore, if the Universe began with an explosion, it has no center.
If the Universe began in an explosion and is expanding, is it or is it not required to have a center? No. Once the Universe began to expand, it became like an expanding surface. Space itself was expanding. Once objects began to appear in the Universe, we had some "markers", if you will, against which to establish coordinate locations. Try as we might, however, we have never been able to use these galaxies to establish a spatial preference in the Universe. There is no center, and all of space seems to be expanding away from all of the rest of space. No matter where you are.
Can we take all of the objects in the Universe, trace their motions backward in time to arrive at a single intersection point, i.e. at the point at which the big bang occurred? If so, this point would truly be the center of the Universe. However, such a point does not exist.
Let's Investigate Activities
Regardless of which galaxy they pick to be the center (and therefore measure all of the other galaxies relative to), all of the other galaxies will appear to be moving away from the selected center.
The same thing which occurred for the elastic band will happen for the balloon or ball.
You can now lead your students through a visualization of the ideas explored above, namely, every point sees itself as the center from which everything else is expanding. You will need to print the two images below on transparencies. If you don't have access to color, black and white will still work.
The transparency in blue shows what a portion of the Universe may have looked like about one billion years ago. The red transparency shows what that section would look like today. Place each sheet on the overhead projector one at a time. Look at each sheet. Is there an obvious "center" to the distribution? Now put the red sheet over the blue one, lining up the outer rims. Have students discuss and describe the pattern which emerges.
Shift the top sheet slightly to the right. Do not rotate the sheets relative to one another. What has happened to the distribution? Shift it up. Now, what do you see? Allow the students to discuss what is happening and how it relates to what they have learned about the Universe. They should record their thoughts on their worksheets.
Have the students try to figure out how to line up the overlays so that ANY dot can appear to be the center of the expansion. They should describe on their worksheets what would need to be done.
This activity has been adapted from one created by David Chandler, who also created the two simulation images.
One Billion Years Ago Full Size
Geometry: In grades 9 -12 all students should:
Origin and Evolution of the Universe: In grades 9 -12 all students should:
"Early in the history of the universe, matter, primarily in the form of hydrogen and helium, clumped together by gravitational attraction to form countless trillions of stars. Billions of galaxies, each of which is a gravitationally bound cluster of billions of stars, now form most of the visible mass of the universe; Stars produce energy from nuclear reactions, primarily the fusion of hydrogen to form helium. These and other processes in stars have led to the formation of all the other elements."