R. W. Kershaw Middle School

Lab / The Expanding Balloon Universe

What is the age of my balloon universe after it has expanded?

 

Name: ________________________________________________

 


ySummary

In this exercise, you will use a two-dimensional analogy to explore the expansion of the Universe.

 

Hubble Deep Field NorthyBackground and Theory

The Hubble Law tells us that our Universe is expanding. We observe galaxies, find their distances and their velocities, and find that they are all moving away from us. The more distant the galaxy, the faster it is moving away. From this information, we can estimate the age of our Universe. Because we assume that the Universe has always been expanding at the same rate, we know how long distant galaxies have been traveling in order to get where they are today!

 

yProcedure

1.    Blow up your balloon to between ¼ and 1/3 its final size. Do NOT tie it shut!

2.    Draw and number ten (10) galaxies (G1–G10) on the balloon. Mark one more
galaxy (the 11th galaxy) as the reference galaxy (GR).

3.    Measure the distance between the reference galaxy and each of the numbered
galaxies. The easiest way to do this is to use a piece of string. Stretch it between the
two points on the balloon; then measure the string using your millimeter ruler.
Record these data in the table. Be sure to indicate the units you are using. (Hint: Use millimeters.)

4.    Now blow up the balloon fully (but not so big that it is in danger of popping). 
You can tie it shut this time if you like. Estimate the amount of time it took you to blow
up the balloon (in seconds). (Hint: Have several people time the “expansion” and take
the average of those times.)

5.    Measure the distance between the reference galaxy and each of the numbered
galaxies after this second expansion of your balloon universe. Record these data in the
table. (Again, use millimeters.)

6.    Subtract the first measurement (FM) from the second measurement (SM); record the difference in the data table.

7.    Divide the distance traveled (the difference SM – FM) by this time (T, in seconds) to get a velocity. 
Distance traveled (mm) / Time (s) = Velocity (mm/s)   or   d/t = v.

8.    Plot the velocity (v) versus the second measurement (SM, which is the expansion distance) to get the “Hubble Law for  Balloons.” Don't forget to label the units on your axes! (Note that velocity is plotted on the y-axis and distance on the x-axis.)

9.   You plot points on an x-y graph using ordered pairs of numbers: (x1, y1), (x2, y2), (x3, y3). Using numbers, we might plot ordered pairs on our velocity vs. distance graph
that have these values: (150, 4), (180, 6.5), (220, 8), (250, 13). Your values will depend on the distances you measure between the reference galaxy and your 10 galaxies
and the time it took to blow up your balloon.

10.     Fit a straight line to your data. About as many data points should be above the line as there are below the line. “Eyeballing” the position of your line is close enough.
This is called the “best-fit” line.

11.     Find the slope. (Remember that the slope is “the change in y over the change in x.”) This is exactly the way that we find the value of H from Hubble's Law.  Pick two
points that are relatively far apart that are on the best-fit line you have drawn.

12.     Find the age of your balloon universe from this slope by taking its reciprocal.


 

Galaxy Number

First Measurement

Second Measurement

SM – FM

(Difference)

Text Box: First measurement (FM) is the distance (in mm) between the reference galaxy, GR, and each numbered galaxy, G1 through G10.
 
Second measurement (SM) is the distance (in mm) between the reference galaxy, GR, and each numbered galaxy, G1 through G10. after the balloon has been inflated a second time. 
 
Difference = SM – FM mm
 
V = Difference/Time
V = mm/s
 
T = Time to blow up balloon from initial size to final size
 
T = _____________ s
 
 

 

Velocity

 

1

 

 

 

 

2

 

 

 

 

3

 

 

 

 

4

 

 

 

 

5

 

 

 

 

6

 

 

 

 

7

 

 

 

 

8

 

 

 

 

9

 

 

 

 

10

 

 

 

 

 

Plot the velocity versus the second measurement to get the “Hubble Law for Balloons.” Label the units on your axes.

Text Box: The current estimate for H0, the Hubble constant, is 72 km/s/Mpc or about 22 km/s/Mly
 
H0 is the slope of the line.
Text Box: Your graph should look similar to the one below.
Text Box: y-axis?
 

 

 

 

               

  

 

 

 

 

yQuestions

 

1.  You drew a “best-fit” straight line through your points. The line should go through (0,0) on your graph. Why?

 

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2.   Find the slope. (For full credit, you must show all the math steps!)

 

     Slope = ____________________

 

x1

y1

x2

y2

 

 

 

 

x2 x1

y2y1

 

 

 y2y1 /  x2 x1 =  ____________________

 

 

 

 

 

3.   Find the age of your balloon universe from this slope. (Show your calculations!)

The reciprocal of the slope is directly related to the age of your “universe.”

Slope of line = H0. Velocity/distance =

Age of “universe” =

 

Age of “universe” = ____________________  [Your balloon universe should be approximately between 5 and 15 seconds old.]

 

  

4.   How does this age compare to the time it took to blow up the balloon the second time (i.e., the expansion time)?
     What assumptions are you making by doing this? Are they sensible assumptions?

 

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5.   What are some of the practical limitations of your balloon universe and the way it was “expanded” that could affect the age you
     calculated  for it?

 

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6.   How would your results change if you used a different reference “galaxy” on the balloon? If you are not sure, try it!

 

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