Schlumberger
 
The Hubble Constant
Our Results

SEED
 

Here are our results for this experiment:

Data Sheet
Galaxy Initial Distance from Milky Way (cm) Stretched Distance from Milky Way (cm) Total Distance Moved (cm) Galaxy
Speed
(cm/s)
A

1.0

2.0

1.0

2.0

B

2.0

4.0

2.0

4.0

C

3.0

5.9

2.9

5.8

D

4.0

7.8

3.8

7.6

E

5.0

10.0

5.0

10.0

F

6.0

12.1

6.1

12.2

G

7.0

14.4

7.4

14.8


Results

 

 

Relative to the end of the ruler, the Milky Way did not move at all. This is because we used it as our reference. We are located there. However, the farther any other galaxy was initially from the Milky Way, the faster it moved away. This agrees with Hubble’s findings. You can see this in the plot of our data below.

By looking at the graph you can see that the trend appears to be linear. To compare this with Hubble’s findings and learn why this trend makes sense, check out Digging Deeper

Try This

Choose a different galaxy, such as Galaxy C, on the rubber band to represent your reference galaxy. Then, repeat the experiment. How does your new data compare with your original data? When you stretched the rubber band, were the other galaxies moving toward or away from your reference galaxy?

For a related experiment look at The Expanding Balloon.

 

  Digging Deeper  

Find out more about

 

 

the effect of distance on speed.

 

 

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Experiment  
Results  
The Expanding Universe
Digging Deeper  
Teacher's Notes 
Related Links 
PDF Version of Experiment
 
 

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