Energy and Human Ambitions on a Finite Planet, 2021a
Energy and Human Ambitions on a Finite Planet, 2021a
Energy and Human Ambitions on a Finite Planet, 2021a
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10 Renewable Overview 168<br />
Treating Earth as a sphere of radius R, it has surface area 4πR 2 , but<br />
the sun doesn’t “see” the whole surface at <strong>on</strong>ce. In fact, from the<br />
vantage point of the rays of sunlight intercepting Earth, what matters<br />
is the projecti<strong>on</strong> of Earth, 14 which just looks like a disk of area πR 2 .<br />
Averaging the solar input across the entire planet therefore reduces<br />
the 1,360 W/m 2 by a factor of 4 to 340 W/m 2 .<br />
Not all the sunlight arriving at the top of the atmosphere makes it to<br />
the surface, so in practice, a typical locati<strong>on</strong> will receive an average 15<br />
of about 200 W/m 2 . This is a number that comes up often as a typical<br />
insolati<strong>on</strong>, so is worth remembering.<br />
14: Imagine taking a picture of a sphere situated<br />
across the room. The area the sphere<br />
takes up <strong>on</strong> the photo is πR 2 ,notthetotal<br />
curved surface area of 4πR 2 . See also<br />
Fig. 9.6 (p. 144).<br />
15: ...averaging over day, night, sun angles,<br />
<str<strong>on</strong>g>and</str<strong>on</strong>g> weather c<strong>on</strong>diti<strong>on</strong>s.<br />
Clouds <str<strong>on</strong>g>and</str<strong>on</strong>g> ice (mostly) reflect almost 30% of incoming sunlight, leaving<br />
123,000 TW to be absorbed by l<str<strong>on</strong>g>and</str<strong>on</strong>g>, water, <str<strong>on</strong>g>and</str<strong>on</strong>g> atmosphere in various<br />
forms (see Table 10.2). Virtually all of the energy hitting the surface<br />
goes to direct thermal absorpti<strong>on</strong>, 16 much of which then flows into 16: That is, heating (see Example 10.3.2);<br />
evaporati<strong>on</strong> of water—the starting point of the hydrological cycle. A<br />
tiny porti<strong>on</strong> of the absorbed energy gives rise to wind, some of which<br />
will drive waves. An even smaller porti<strong>on</strong> c<strong>on</strong>tributes to photosynthesis<br />
<str<strong>on</strong>g>and</str<strong>on</strong>g> supports essentially all life (biology) <strong>on</strong> the planet. And finally, a<br />
tiny fragment of the absorbed energy drives ocean currents. Table 10.2<br />
tracks where the incoming solar energy goes, in several stages, also<br />
listing n<strong>on</strong>-solar geothermal <str<strong>on</strong>g>and</str<strong>on</strong>g> tidal c<strong>on</strong>tributi<strong>on</strong>s. For comparis<strong>on</strong>,<br />
the current energy scale of human activity is approximately 18 TW, while<br />
human metabolism, 17 is about 0.8 TW.<br />
note that solar panels could intercept part<br />
of this energy flow.<br />
17: Recall Ex. 5.5.2 (p. 74). 100 W per pers<strong>on</strong><br />
times 8 billi<strong>on</strong> people is 800 GW, or 0.8 TW.<br />
Table 10.2: Earth’s energy input budget. Symbols ⊙, ⊕, <str<strong>on</strong>g>and</str<strong>on</strong>g> ☾represent Sun, Earth, <str<strong>on</strong>g>and</str<strong>on</strong>g> Mo<strong>on</strong>, respectively. The sec<strong>on</strong>d group breaks out<br />
the solar input into three pieces that add to the total in the row above. The third group all comes from absorbed energy—mostly at Earth’s<br />
surface. The last group is not from radiant solar energy, so that percentages are in parentheses as they do not bel<strong>on</strong>g to the solar budget<br />
[63–65].<br />
Category Power (TW) % solar source Comments<br />
total solar input 174,000 100 ⊙ the next 3 inputs come from here<br />
surface absorpti<strong>on</strong> 83,000 47.9 ⊙ heats surface; evaporates H 2 O, powers life, wind, etc.<br />
reflecti<strong>on</strong> to space 51,000 29.3 ⊙ from clouds, ice; uncaptured energy<br />
atmos. absorpti<strong>on</strong> 40,000 22.6 ⊙ heats atmosphere, some to wind<br />
evaporati<strong>on</strong> 44,000 25.4 ⊙→⊕surf. from surface absorpti<strong>on</strong>; hydrological cycle<br />
wind 900 0.5 ⊙ absorp. from absorpti<strong>on</strong>s above, also makes waves<br />
photosynthesis 100 0.06 ⊙→⊕surf. fuels biology (life) <strong>on</strong> the planet<br />
ocean currents 5 0.003 ⊙→⊕surf. moves water around<br />
geothermal 44 (0.025) ⊕ half original heat, half radioactive decays<br />
tides 3 (0.0018) ☾, ⊙ gravitati<strong>on</strong>al; mostly from Mo<strong>on</strong>, some from Sun<br />
Example 10.3.2 Solar Heating: How much would a black table 18<br />
warm up sitting in full sun for ten minutes?<br />
18: . . . parameters defined below<br />
A nice round-number approximati<strong>on</strong> of full overhead sunlight is that<br />
it delivers 1,000 W/m 2 to the ground. If we situate a table whose top<br />
surface area is 1 m 2 , has a mass of 20 kg, <str<strong>on</strong>g>and</str<strong>on</strong>g> a specific heat capacity<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.