ISP 205, Section 3, Spring 1997

ACTIVITY: EXPANSION of the UNIVERSE


Work in groups of three. Each group needs one balloon and one ruler. One person handles the balloon, one person marks and measures, and one person records the results.

                                        Name: ________________________


                                        Student Number: ______________


                                        Name: ________________________


                                        Student Number: ______________


                                        Name: ________________________


                                        Student Number: ______________

In this activity we model the UNIVERSE as the TWO-DIMENSIONAL SURFACE of a balloon. Blow up the balloon to about a 4 inch diameter. Twist the neck and hold it closed so that no air escapes, but do NOT make a permanent knot because you will need to blow it up some more. Make SIX marks on its surface to represent clusters of galaxies and label them A-F. [Avoid placing any near the neck of the balloon.]

A. Measure and record the distances (in cm) from cluster A to each of the other 5 clusters.

B. Repeat step 1 measuring the distances (in cm) from cluster F to each of the other clusters.

C. Now blow up the balloon up more, to a diameter of about 8 inches. Measure the distances between the same clusters again and record them.

D. Calculate the increase in the distance and record that as well.

Use the chart provided on the other side of this page











                Clusters   Distance    Distance   Change in
                           (small)     (large)    Distance
                             (cm)        (cm)       (cm)


                A - B      --------    --------   --------


                A - C      --------    --------   --------


                A - D      --------    --------   --------


                A - E      --------    --------   --------


                A - F      --------    --------   --------


                Clusters   Distance    Distance   Change in
                           (small)     (large)    Distance
                             (cm)        (cm)       (cm)


                F - A      --------    --------   --------


                F - B      --------    --------   --------


                F - C      --------    --------   --------


                F - D      --------    --------   --------


                F - E      --------    --------   --------

  1. Are all the other clusters moving away from cluster A?
    YES _X___ NO ____

  2. Are all the other clusters moving away from cluster F?
    YES _X___ NO ____

  3. Is there a cluster that could be considered to be at the center of the universe as represented by the surface of the balloon?
    YES ____ NO _X___

    
    To conclude, just because it looks like all distant galaxies are
    receding from our Galaxy, doesn't necessarily mean that our Galaxy
    is the center of the Universe.  If the entire Universe itself were
    expanding, it would look as if all distant galaxies were moving 
    away no matter which galaxy you were located on.
    
    
    
    
    
    
    
  4. Finally, on the graph below plot the change in distance verses the initial distance for both sets of measurements. Use one symbol for the measurements from cluster A and another for the measurements from cluster F.
    Draw the best straight line you can that comes closest to the most points. Is a straight line a good representation of your measurements?
    YES _X___ NO ____ Some groups drew many lines in a "connect-the-dots" approach. The point of drawing a line is to help you see a general trend in the data, which are individual observations. Lots of lines connecting the dots will not help you do this, and none of the graphs in the book are drawn that way.

    
    
    
    
      
    
    
    
    

    Visions of the Universe
    Beth Hufnagel's home page, email: hufnage4@pilot.msu.edu
    Bob Stein's home page , email: steinr@pilot.msu.edu