Explore 2.12 How Humanity Discovered the Big Bang

Learning Objectives

By the time you have completed the 2.12. Introduction & Exploration Activities, you should be able to:

  • Understand how Western Civilization perceived the Universe 1) before Copernicus, 2) between Copernicus and Newton, 3) between Newton and Hubble, and 4) today.
  • Describe what Hubble’s law is and whether it implies that galaxies are moving through the Universe or being carried by an expanding Universe.
  • Describe whether the concepts of ‘center’ and ‘edge’ apply to the Universe, or not.


Understanding the Universe

Answer the questions below.

How did western civilization perceive the universe before Copernicus? 



How did western civilization perceive the universe between Copernicus and Newton?



How did western civilization perceive the universe between Newton and Hubble?



How does western civilization perceive the universe today?




Hubble’s Law

Hubble’s law tells us that distant galaxies' speeds are proportional to their distance. We read about the rising dough analogy and the galaxies on an expanding balloon.

According to Hubble’s Law, are galaxies moving through, or being carried by an expanding universe? 



Based on what you know about the falsification of scientific explanations, what does Hubble’s Law indicate about the Newtonian Universe?



Raisin Bread UniverseRaisin Bread Expansion Law

Imagine that you live inside one of the raisins (or chocolate chips, if you prefer) in some rising bread dough—illustrated in the image above. From our perspective inside the ‘local’ raisin (our galaxy), we observe the effect of the dough rising on the motions of and distances to all other raisins in the dough.

To do this, we measure the distances between the raisins at 2 o’clock, as the dough begins to rise, and then again at 3 o’clock, once the dough has finished rising.

During that hour, the dough tripled in size, which caused the distances between raisins to triple: the nearest raisin was 1 cm away before rising and 3 cm away after rising, the next raisin moved from 2 to 6 cm, the third from 3 to 9 cm, the fourth from 4 to 12 cm, …. Thus, the nearest raisin moved 2 cm further away (from the local raisin) as the dough rose, the second raisin moved 4 cm further, the third raisin moved 6 cm, the fourth raisin moved 8 cm, …. Now, knowing the distance traveled by each raisin during the hour the dough rose allows us to calculate the speed of each raisin relative to the local raisin. As you know, speed is the distance traveled divided by the duration of the trip (e.g., 60 miles per hour means you traveled 60 miles in 1 hour). So, the raisins traveled at the following speeds as the bread rose: 2 cm/hour for raisin one, 4 cm/hour for raisin two, 6 cm/hour for raisin three, 8 cm/hour for raisin four, …. Okay, with the data in hand, let’s plot the distance to each raisin at the end of rising (on the x-axis) versus the speed traveled by each raisin during rising (on the y-axis). This graph is already plotted above.

Before interpreting our observations, let’s be clear: the raisins in the analogy are galaxies in the Universe and the dough is the fabric of spacetime. To help you think more deeply about how this analogy relates to Hubble’s Law, answer each of the questions below.

From our vantage point inside the ‘local raisin’ (local galaxy), are the rest of the raisins (galaxies) moving towards or away from us?

Look at the plot of raisin speed versus raisin distance. Do you recognize this pattern?

So, what is causing the raisins (galaxies) to move apart. In other words, what is the best explanation of ‘The Law of Raisin Bread Expansion’?

Are the raisins moving through the dough? If not, describe what is causing the observed motion.


Now, imagine a much larger loaf and consider that you move to another raisin (galaxy)—any other raisin, near or far. In fact, consider making distance and velocity measurements from many different raisins (galaxies). Would you observe the same ‘Hubble’s Law’ relationship from raisins (galaxies) other than the local raisin (Milky Way)? In other words, does it matter which raisin (galaxy) you observe from?




Ends of the Universe

The Stretching Balloon Surface Universe. This analogy is based on a partially inflated child’s balloon on which are drawn small galaxy-shaped dots, as shown in the image below. To appropriately understand this analogy, you must consider that nothing exists beyond the surface of the balloon. In other words, imagine that you are a two-dimensional being—a stick figure—that exists entirely within the surface of the balloon. You can move in any direction across the surface, but you cannot leave the surface. Now, locate yourself in one of the galaxies and observe what happens as the balloon is inflated to a larger size, as illustrated below.

Balloon Analogy

From your existence within the surface of the balloon, describe the motion of all other galaxies relative to your own as the balloon inflates.

In this analogy, are distant galaxies moving away from you because they are moving across the surface of the balloon? If not, what is causing the distances between galaxies to increase?

Again, from your existence within the surface of the balloon, describe which galaxies are traveling away from you more slowly and which are moving away more quickly. Also, describe why.

In this analogy, if you plotted the distance to galaxies against their speed (as they move away from you), would you recreate Hubble’s Law?


Okay, these are the last questions, and then we’ll summarize what these analogies teach us. Once again, answer each of the following questions from your existence within the surface of the balloon: Does the surface of the balloon have a center or an edge? In other words, can you place your finger on the balloon and say, “Here’s the center!” or, “Here’s the edge!”