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Energy and Human Ambitions on a Finite Planet, 2021a

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D.5 <str<strong>on</strong>g>Human</str<strong>on</strong>g>ity’s L<strong>on</strong>g View 405<br />

In order for human civilizati<strong>on</strong> to be in its infancy, it would have to<br />

c<strong>on</strong>tinue for at least 10,000 years more, if not far l<strong>on</strong>ger. What would it<br />

mean for us to still be operating “successfully” 10,000 years from now?<br />

Our physics <str<strong>on</strong>g>and</str<strong>on</strong>g> math approach actually allows us to place c<strong>on</strong>straints!<br />

This discussi<strong>on</strong> is limited to living <strong>on</strong> Earth. Chapter 4 laid out reas<strong>on</strong>s<br />

why imagining a space-faring future may be misguided. But even<br />

ignoring these arguments, Chapter 1 illustrated that human growth<br />

ambiti<strong>on</strong>s would be brought to an end l<strong>on</strong>g before 10,000 years pass.<br />

In this light, it is most straightforward to c<strong>on</strong>centrate <strong>on</strong> what it would<br />

take to succeed <strong>on</strong> Earth itself. 46<br />

If we manage to carry our civilizati<strong>on</strong> into the far future, 47 we can<br />

comfortably call this success. If we d<strong>on</strong>’t, well, that would be failure.<br />

Can we sketch out what success looks like? One easy way to get there is<br />

to start enumerating the things that can’t be carried into the far future.<br />

1. Fossil fuels will not power civilizati<strong>on</strong>: a large fracti<strong>on</strong> of the initial<br />

inheritance has been spent in a short 200 years, 48 so that 10,000<br />

years in the future it is safe to say they will be l<strong>on</strong>g g<strong>on</strong>e.<br />

2. No steady annual decline of natural resources like forests, fisheries,<br />

fresh water, or species populati<strong>on</strong>s can be brooked. Allowing any<br />

comp<strong>on</strong>ent to decline would mean eventually losing that resource,<br />

which may be critical to our survival.<br />

3. <str<strong>on</strong>g>Human</str<strong>on</strong>g> populati<strong>on</strong> will not be allowed to grow. Even small growth<br />

rates will step up pressure <strong>on</strong> natural resources, <str<strong>on</strong>g>and</str<strong>on</strong>g> Earth can<br />

<strong>on</strong>ly support so much, l<strong>on</strong>g-term. Independent of what the “right”<br />

number is, 49 <strong>on</strong>ce settled, we will not be able to dial it up without<br />

imperiling the hard-w<strong>on</strong> success.<br />

4. Even under steady human populati<strong>on</strong>, any increase in resource<br />

use per pers<strong>on</strong> will also not be compatible. In general, growth<br />

leads to a dead end: to failure.<br />

5. Mining materials from the Earth will not c<strong>on</strong>tinue at anything near<br />

the current pace. In the last few hundred years, the best deposits<br />

of copper, gold, aluminum, etc. have been found <str<strong>on</strong>g>and</str<strong>on</strong>g> exploited.<br />

Even if <strong>on</strong>ly 10% of the attainable resource has been c<strong>on</strong>sumed<br />

thus far, 50 c<strong>on</strong>tinuing for tens of thous<str<strong>on</strong>g>and</str<strong>on</strong>g>s of years (<str<strong>on</strong>g>and</str<strong>on</strong>g> bey<strong>on</strong>d)<br />

cannot be expected.<br />

6. Ultimately, any activity that draws down a finite natural resource<br />

will be impossible to sustain if the extracti<strong>on</strong> rate is modest or high<br />

in relati<strong>on</strong> to the initial resource abundance. Anything that can’t<br />

last for well over 10,000 years is not a viable l<strong>on</strong>g-term soluti<strong>on</strong><br />

<str<strong>on</strong>g>and</str<strong>on</strong>g> should not be exploited if success is the goal. Likewise, any<br />

pollutant that can build up to dangerous levels <strong>on</strong> even these very<br />

l<strong>on</strong>g timescales cannot be tolerated, if failure is to be avoided.<br />

7. We can use the rule of 70 to say that anything having a doubling<br />

time (or halving-time in the case of depleti<strong>on</strong>) shorter than 10,000<br />

years is a no-go for success <strong>on</strong> these timescales, meaning that any<br />

activity impacting resources would have to be held to a growth rate<br />

46: Even if extending to other planets, the<br />

same logic will apply.<br />

47: A useful definiti<strong>on</strong> might be uninterrupted<br />

preservati<strong>on</strong> of the knowledge <str<strong>on</strong>g>and</str<strong>on</strong>g><br />

history gained thus far, without some apocalyptic<br />

collapse forcing a start-from-scratch<br />

revival—to the extent that’s even plausible.<br />

48: . . . most of this in the last 50 years<br />

49: . . . unlikely as high as 10 billi<strong>on</strong>, <str<strong>on</strong>g>and</str<strong>on</strong>g><br />

it could even be well less than a billi<strong>on</strong>,<br />

depending <strong>on</strong> living st<str<strong>on</strong>g>and</str<strong>on</strong>g>ards<br />

50: . . . author’s c<strong>on</strong>jecture; it could well be<br />

higher<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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