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Energy and Human Ambitions on a Finite Planet, 2021a

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4 Space Col<strong>on</strong>izati<strong>on</strong> 55<br />

Figure 4.1: Earth <str<strong>on</strong>g>and</str<strong>on</strong>g> Mo<strong>on</strong> (far right) to scale. On this scale, the sun would be larger than the page <str<strong>on</strong>g>and</str<strong>on</strong>g> about 400 pages away. Mars would<br />

be 160 to 1,100 pages away. Since 1972, humans have not traveled bey<strong>on</strong>d the black outline of the earth in this figure (600 km).<br />

Sun<br />

Earth (invisible)<br />

Figure 4.2: Proving the point that textbooks are not c<strong>on</strong>ducive to correctly-scaled graphics of objects in space, by the time the Earth-Sun<br />

distance spans the page, Earth (<strong>on</strong> far right) is too small to be visible in print, at less than 1% the diameter of the orange sun at far left. The<br />

Earth–Mo<strong>on</strong> distance is about the width of the arrow shaft pointing to Earth. <str<strong>on</strong>g>Human</str<strong>on</strong>g>s have never traveled more than the arrow shaft’s<br />

width from Earth, <str<strong>on</strong>g>and</str<strong>on</strong>g> have not even g<strong>on</strong>e 0.2% that far in about 50 years! Mars, <strong>on</strong> average, is farther from Earth than is the sun.<br />

Let us first lay out some basic ratios that can help build suitable mental<br />

models at whatever scale we choose.<br />

Definiti<strong>on</strong> 4.1.1 Scale models of the universe can be built based <strong>on</strong> these<br />

approximate relati<strong>on</strong>s, some of which appear in Table 4.1 <str<strong>on</strong>g>and</str<strong>on</strong>g> Table 4.2:<br />

Table 4.1: Progressi<strong>on</strong> of scale factors.<br />

Step<br />

Factor<br />

Earth diameter (start)<br />

Mo<strong>on</strong> distance 30×<br />

Sun distance 400×<br />

Neptune distance 30×<br />

Nearest Star 9,000×<br />

Milky Way Center 6,000×<br />

Andromeda Galaxy 100×<br />

Universe Edge 6,000×<br />

1. The mo<strong>on</strong>’s diameter is <strong>on</strong>e-quarter that of Earth, <str<strong>on</strong>g>and</str<strong>on</strong>g> located 30<br />

earth-diameters (60 Earth-radii) away from Earth, <strong>on</strong> average (see<br />

Figure 4.1).<br />

2. The sun’s diameter is about 100 times that of Earth, <str<strong>on</strong>g>and</str<strong>on</strong>g> 400 times as<br />

far as the mo<strong>on</strong> from Earth (see Figure 4.2).<br />

3. Mars’ diameter is about half that of Earth, <str<strong>on</strong>g>and</str<strong>on</strong>g> the distance from Earth<br />

ranges from 0.4 to 2.7 times the Earth–Sun distance.<br />

4. Jupiter’s diameter is about 10 times larger than Earth’s <str<strong>on</strong>g>and</str<strong>on</strong>g> 10 times<br />

smaller than the sun’s; it is about 5 times farther from the sun than is<br />

the earth.<br />

5. Neptune orbits the sun 30 times farther than does Earth.<br />

2: The Oort cloud marks the outer influence<br />

6. The Oort cloud 2 of comets ranges from about 2,000 to 100,000 times<br />

of the sun, gravitati<strong>on</strong>ally.<br />

the Earth–Sun distance from the sun.<br />

3: . . . Proxima Centauri<br />

7. The nearest star 3 is 4.2 light years from us, compared to 500 lightsec<strong>on</strong>ds<br />

from Earth to the sun—a ratio of 270,000.<br />

A light year is the distance light travels in a<br />

year.<br />

8. The Milky Way galaxy has its center about 25,000 light years away 4: That’s 6,000 times the distance to the<br />

away, 4 <str<strong>on</strong>g>and</str<strong>on</strong>g> is a disk about four times that size in diameter.<br />

closest star.<br />

9. The next large galaxy 5 is 2.5 milli<strong>on</strong> light years away, or about 25 5: ...theAndromeda galaxy<br />

Milky Way diameters away.<br />

6: The “edge” is limited by light travel<br />

10. The edge of the visible universe 6 is 13.8 billi<strong>on</strong> light years away, or<br />

time since the Big Bang (13.8 billi<strong>on</strong> years<br />

about 6,000 times the distance to the Andromeda galaxy.<br />

ago), <str<strong>on</strong>g>and</str<strong>on</strong>g> is called our cosmic horiz<strong>on</strong>. See<br />

Sec. D.1 (p. 392) for more.<br />

We will c<strong>on</strong>struct a model using the set of scale relati<strong>on</strong>s in Definiti<strong>on</strong><br />

4.1.1, starting local <strong>on</strong> a comfortable scale.<br />

We’ll make Earth the size of a grain of s<str<strong>on</strong>g>and</str<strong>on</strong>g> (about 1 mm diameter).<br />

The mo<strong>on</strong> is a smaller speck (dust?) <str<strong>on</strong>g>and</str<strong>on</strong>g> the diameter of its orbit would<br />

span the separati<strong>on</strong> of your eyes. On this scale, the sun is 100 mm in<br />

diameter (a grapefruit) <str<strong>on</strong>g>and</str<strong>on</strong>g> about 12 meters away (40 feet). Mars could<br />

As we build up our model, pause <strong>on</strong><br />

each step to lock in a sense of the<br />

model: visualize it or even recreate<br />

it using objects around you!<br />

© 2021 T. W. Murphy, Jr.; Creative Comm<strong>on</strong>s Attributi<strong>on</strong>-N<strong>on</strong>Commercial 4.0 Internati<strong>on</strong>al Lic.;<br />

Freely available at: https://escholarship.org/uc/energy_ambiti<strong>on</strong>s.

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