Explore 2.6 The Scale of the Universe


Learning Objectives

By the time you have completed the 2.6. Introduction & Exploration Activities, you should be able to:

  • Understand the meaning of the following terms/concepts and be able to identify examples of each: Universe, Planet (rocky, gaseous, and icy), planetesimal, solar/planetary system, star, normal star, giant star, mini star, nebula(ae), galaxy (spiral, elliptical, & irregular), galaxy cluster, galactic voids.
  • Use a scale model of the Solar System (the Sun as a 12” ball) to describe 1) the relative sizes of the Sun, Mercury, Earth, & Jupiter, 2) the distances from the Sun to Mercury, Earth, & Jupiter, 3) the relative distance between the Sun and other nearby stars, and 4) the size of the Milky Way Galaxy.
  • Use a scale model of our galaxy (the Milky Way as a DVD) to identify the relative distance to the Andromeda galaxy, relative diameters of the largest and smallest galaxies, the size of the Universe, and the distribution of galaxies in the Universe.

Scientific Terms/Concepts

Terms: Universe, Planet (rocky, gaseous, and icy), Planetesimal, Solar/Planetary System, Star, Normal Star, Giant Star, Mini Star, Nebula(ae), Galaxy (spiral, elliptical, & irregular), Galaxy Cluster, Galactic Voids.

Define and give an example of each term:

Term:

Universe

Definition:

Example:


Term:

Planet

Definition:

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Term:

Rocky Planet

Definition:

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Term:

Gaseous Planet

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Term:

Icy Planet

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Term:

Planetesimal

Definition:

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Term:

Solar/Planetary System

Definition:

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Term:

Star

Definition:

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Term:

Normal Star

Definition:

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Term:

Giant Star

Definition:

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Term:

Mini Star

Definition:

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Term:

Nebula

Definition:

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Term:

Galaxy

Definition:

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Term:

Spiral Galaxy

Definition:

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Elliptical Galaxy

Definition:

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Term:

Irregular Galaxy

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Galaxy Cluster

Definition:

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Term:

Galactic Voids

Definition:

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Solar System Scale

Use a scale model of the Solar System (the Sun as a 12” ball) to describe 1) the relative sizes of the Sun, Mercury, Earth, & Jupiter, 2) the distances from the Sun to Mercury, Earth, & Jupiter, 3) the relative distance between the Sun and other nearby stars, and 4) the size of the Milky Way Galaxy.

Scale Model 1. The Sun as a 12" ball (30.5 cm)

The Sun is so large that is is hard for us to comprehend, so let's shrink it to something we do understand. Imagine making the Sun about 4.6 billion times smaller. If we did, the Sun would be about the size of a 12" ball (a little bigger than a basketball and nearly twice as big as a soccer ball). At this scale, what size would the planets be? ...and how far apart would they be?

The Size of the Planets

In the box below, enter estimates for the scaled sizes of 1) Mercury (the smallest planet in our solar system), 2) Earth (our home), and 3) Jupiter (the largest planet).

If you'd like, you can also estimate the sizes of the other planets. Remember, you're estimating the size these planets would be if they were 'scaled down' in the same way we scaled the Sun. Number your estimates (as above).



The Distances between the Planets

In the box below, enter estimates for the scale distances from the Sun to 1) Mercury, 2) Earth, and 3) Jupiter.

If you'd like, you can also estimate the distances to the other planets. Number your estimates (as above).



The Distances between Stars (Solar Systems)

In the box below, enter an estimate for the scale distance from the Sun to the nearest star, which is a little over 4 light years away.

The Size of the Milky Way Galaxy

With the scale size of a star (~0.02 in or 0.5 mm), scale width of a solar system (~4.3 in or 11 cm), and scale distance between stars (0.25 mi or 0.4 km) established, we are prepared to consider the size of a galaxy in this model.

In the box below, enter your estimate for the scale width of the Milky Way Galaxy.




Galaxy Scale

Use a scale model of our galaxy (the Milky Way as a DVD) to identify the relative distance to the Andromeda galaxy, relative diameters of the largest and smallest galaxies, the size of the Universe, and the distribution of galaxies in the Universe.

Scale Model 2. The Sun as a Candy Sprinkle

The Size of Our Solar System & The Distance between Stars

Our first scale model becomes unproductive if we try to extend it beyond the nearest stars. In order to understand distances in galaxies, we need a new scale. For our new model, we make the Sun even smaller: we scale it down to the size of a very small, round candy sprinkle (about 0.02 in or 0.5 mm across). At this scale, the solar system would be about the size of your palm (~4.3 in or 11 cm)—as shown in the image below. (FYI: The green dot representing the candy sprinkle is larger than the Sun would be. We made it that size so you could see it.)

A sprinkle on the palm of a hand.

At this new scale (Sun is a small candy sprinkle), where would you place the next star (solar system)? Enter your estimate below.



The Number of Stars in Our Galaxy

We mentioned above that there are several hundred billion stars—say 200 billion—in our Galaxy. Does the number 200 billion mean anything more than 'A FREAKIN LOT!' to you? It doesn't to most people. So, that's next on our list of things to understand. In order to do that, we want you to estimate how much space 200 billion small candy sprinkles would fill. Would it fill a bucket? a car? a bedroom? ... ?

In the space below, enter your estimate of the space that 200 billion small candy sprinkles would fill.




Scale Model 3. The Milky Way is the Size of a DVD

As we extend our view beyond galaxies, our second scale model also becomes unproductive. In order to understand distances between galaxies in the Universe, we need a new scale. Our new model is based on scaling the Milky Way down to the size of a DVD. In this model, the ~100,000 light year diameter of the Milky Way becomes the 5 inch (13 cm) diameter of a DVD.

How Big are Galaxies?

At this scale, the very smallest galaxies would be a little smaller than BBs, large galaxies such as the Milky Way and Andromeda would be about the size of a DVD, and the largest galaxies would be about the size of a car or merry-go-round (~8 feet or 2.5 m across). The scaled size range of galaxies in the Universe is illustrated by the images below. Small galaxies, which can contain as few as several hundred thousand stars, are far more abundant in the Universe than large galaxies. And the largest galaxies, which can contain as many as 1 trillion stars, are quite rare.

BB PelletsA merry-go-round

 

The Distances between Galaxies

Andromeda is the nearest large galaxy to the Milky Way. Using our current scale model, estimate the scaled distance to Andromeda.

Record your estimate in the box below.



On this same scale, where the sun is the size of a soccer ball, let’s look at how far the planets will be from the sun. Keep in mind that if the sun was about the size of a soccer, this would be how big Mercury, Earth, and Jupiter would be:

Size of Jupiter,Earth, and mercury when the Sun is compared to a soccer ball

But for the purposes of this next image, we are just looking at distance. Planets are not to scale. If the sun was about the size of a soccer ball, how far away would Mercury, Earth, and Jupiter be from the sun?

Distance from the Sun to Jupiter using 12 school buses or 555 feet

If we assume a standard size bus is about 45 feet, this would give us a rough idea of the distance between the Sun and Mercury, Earth, and Jupiter.

The Size of the Universe

The Universe contains all existing energy, matter, and space. As we'll discuss later in this unit, the Universe does not exist inside 'something else', like Earth exists inside our solar system and galaxy. As a result, it's inappropriate to think about the dimensions of the Universe in the same way we think about the size of objects that exist inside the Universe. For now, we'll leave this issue alone and simply provide an answer. Later, we'll explore some introductory ideas regarding how to think about the geometry of the Universe. At the scale of model three the Universe would be about 70 miles (113 km) in diameter. In southeast Idaho, where BYU-Idaho is located, the distance between Rexburg and Pocatello is about 70 miles. Can you think of a city or location that is about that distance from you? Now, image a 70-mile-wide sphere (that doesn't exist inside something larger) containing several hundred billion galaxies ranging in size from BBs to merry-go-rounds and spaced up to about 80 feet apart. Finally, consider that these galaxies and not evenly spread throughout the sphere but are instead concentrated at nodes and along sheets and filaments, as illustrated in the image below. Recognize that each dot of light in that image is a galaxy, galaxy cluster, or galaxy supercluster. In other words, each dot of light represents billions of stars. Note also the large voids that contain few, if any, galaxies. That's our Universe! It looks a little like foam, neuron networks, or cell boundaries, doesn't it?

The structure of the Universe