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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18 <str<strong>on</strong>g>Human</str<strong>on</strong>g> Factors 312<br />
18.4 Fermi Paradox Explained?<br />
Having discussed some of the top-level challenges facing our technological<br />
society, it is too tempting to speculate <strong>on</strong> how universal our trajectory<br />
might be. We do so in the c<strong>on</strong>text of the Fermi Paradox [119], which asks:<br />
if the universe produces a reas<strong>on</strong>ably high probability of intelligent<br />
life developing, why have we seen no credible evidence 32 of advanced<br />
civilizati<strong>on</strong>s? Yes, this is a bit of a tangent, 33 but it could be interpreted<br />
as a relevant data point in the likelihood that we maintain an advanced<br />
civilizati<strong>on</strong> for a l<strong>on</strong>g durati<strong>on</strong>.<br />
The setup to the questi<strong>on</strong> is a “big if.” The usual approach to estimating<br />
the number of intelligent species in our galaxy 34 is via the Drake Equati<strong>on</strong><br />
[120]. The equati<strong>on</strong> is simple, just multiplying the number of stars by<br />
a chain of probabilities: that the star has planets at all; that <strong>on</strong>e of the<br />
star’s planets is “habitable;” that the envir<strong>on</strong>ment is benign <str<strong>on</strong>g>and</str<strong>on</strong>g> that life<br />
has had enough time to develop; <str<strong>on</strong>g>and</str<strong>on</strong>g> finally that the life develops into<br />
an intelligent form, capable of communicating. Also factored in is the<br />
likelihood that any such species would endeavor to reach out, <str<strong>on</strong>g>and</str<strong>on</strong>g> how<br />
l<strong>on</strong>g their civilizati<strong>on</strong> lasts in that state so that we might overlap 35 in<br />
time. For the Milky Way galaxy, 100 billi<strong>on</strong> stars—almost all of which<br />
we now know are likely to have planets—gives a huge start so that even<br />
if the chance of intelligent life arising is <strong>on</strong>e in a milli<strong>on</strong>, we’re left with<br />
quite a margin.<br />
But maybe our trajectory is pretty typical. By the time an intelligent<br />
species arises, the many milli<strong>on</strong>s or billi<strong>on</strong>s of years of life leading<br />
up to that event may ubiquitously lead to deposits of fossil fuels. 36<br />
The first species smart enough to utilize the planet’s fossil fuels does<br />
so with reckless ab<str<strong>on</strong>g>and</str<strong>on</strong>g><strong>on</strong>. Because evoluti<strong>on</strong> does not skip steps, we<br />
should not expect to find a species wise enough to refrain from rapid<br />
fossil fuel use emerging before a species who is just smart enough to<br />
use them, but not smart enough not to. So the “intelligent” species<br />
short-circuits the battery 37 in a blaze of glory that may even involve<br />
baby-step excursi<strong>on</strong>s into space before either climate change or other<br />
resource/planetary limitati<strong>on</strong>s removes the fossil fuel source that made<br />
it all possible. Lacking wisdom <str<strong>on</strong>g>and</str<strong>on</strong>g> foresight, solid plans are not in<br />
place to h<str<strong>on</strong>g>and</str<strong>on</strong>g>le the withdrawal, which does not go well <str<strong>on</strong>g>and</str<strong>on</strong>g> leaves the<br />
species in a crippled lower-tech state. Rebuilding from the ashes is then<br />
much less likely to explode without that <strong>on</strong>e-time elixir that made it all<br />
possible the first time. 38 A simple, <str<strong>on</strong>g>and</str<strong>on</strong>g> possibly quite satisfying life may<br />
await, but it may not involve traveling or communicating across space<br />
for others to learn of our existence.<br />
This noti<strong>on</strong> is, of course, highly speculative <str<strong>on</strong>g>and</str<strong>on</strong>g> of little practical value.<br />
Except it may allow us to think “bigger” than ourselves <str<strong>on</strong>g>and</str<strong>on</strong>g> p<strong>on</strong>der<br />
whether it is surprising that we might fail to achieve a Star Trek future.<br />
It is at least somewhat relevant to note that the universe we peer into<br />
does not have an evident intergalactic intelligent presence. Perhaps the<br />
32: ...in the form of communicati<strong>on</strong>s or<br />
alien visits<br />
33: Normally, this kind of tangent might go<br />
in a box, but it is big enough to be awkward<br />
in that format, thus a whole secti<strong>on</strong>.<br />
34: ...or the whole universe, if thinking<br />
more broadly<br />
35: The noti<strong>on</strong> of “overlap” is complicated<br />
here by the 100,000 light-year scale of the<br />
galaxy, so that by the time a signal arrives<br />
at Earth, the civilizati<strong>on</strong> may be l<strong>on</strong>g g<strong>on</strong>e<br />
already.<br />
36: . . . buried remnants of life<br />
37: Fossil fuels can be thought of as a solarcharged<br />
battery that we are discharging<br />
almost a milli<strong>on</strong> times faster than the time<br />
it took to charge it: see Box 10.2 (p. 169).<br />
38: Also, easily accessed surface metal deposits<br />
have l<strong>on</strong>g disappeared, bringing into<br />
questi<strong>on</strong> whether a Br<strong>on</strong>ze Age would be<br />
possible to replicate.<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.