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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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.