Cross-posted from Sentient Developments.
I'm surprised how often the Drake Equation is still mentioned when people discuss such things as the search for extra terrestrial intelligence (SETI), astrobiology and problems like the Fermi Paradox.
Fairly
recent insights in such fields as cosmology, astrobiology and various
future studies have changed our perception of the cosmos and the ways
in which advanced life might develop.
Frank Drake's
equation, which he developed back in 1961, leaves much to be desired in
terms of what it's supposed to tell us about both the nature and
predominance of extraterrestrial life in our Galaxy.
The Drake Equation
The Drake equation states that:
where:
N is the number of civilizations in our galaxy with which we might hope to be able to communicate and:
R* is the average rate of star formation in our galaxy
fp is the fraction of those stars that have planets
ne is the average number of planets that can potentially support life per star that has planets
fl is the fraction of the above that actually go on to develop life at some point
fi is the fraction of the above that actually go on to develop intelligent life
fc is the fraction of civilizations that develop a technology that releases detectable signs of their existence into space
L is the length of time such civilizations release detectable signals into space.
Arbitrary at bestThe
integers that are plugged into this equation are often subject to wide
interpretation and can differ significantly from scientist to
scientist. Even the slightest change can result in vastly different
answers. Part of the problem is that our understanding of cosmology and
astrobiology is rapidly changing and there is often very little
consensus among specialists as to what the variables might be.
Consequently,
the Drake formula relies on 'stabs in the dark.' This makes it highly
imprecise and unscientific. The margin of error is far beyond what
should be considered acceptable or meaningful.
No accounting for cosmological development or time Another
major problem of the Drake Equation is that it does not account for two
rather important variables: cosmological developmental phases and time
(see Cirkovic, "
The Temporal Aspect of the Drake Equation and SETI").
More
specifically, it does not take into consideration such factors as the
age of the Galaxy, the time at which intelligence first emerged, or the
presence of physiochemical variables necessary for the presence of life
(such as metallicity required to form planets). The equation assumes a
sort of cosmological uniformity rather than a dynamic and ever changing
universe.
For example, the equation asks us to guess the number of Earth-like planets, but it does not ask us
when there were Earth-like planets. And intelligence itself may have been present as long as
2 to 4.5 billion years ago.
The
Galaxy's extreme age and the potential for intelligence to have emerged
at disparate points in time leaves an absurdly narrow window for
detecting radio signals. The distances and time-scales in question are
mind-boggingly vast. SETI, under its current model, is conducting an
incredibly futile search.
Detecting ETI'sWhich
leads to the next problem, that of quantifying the number of radio
emitting civilizations. I'm sure that back in the 1960's it made a lot
of sense to think of radio capability as a fairly advanced and
ubiquitous means of communication, and by consequence, an excellent way
to detect the presence and frequency of extraterrestrial civilizations.
But
time has proven this assumption wrong. Our radio window is quickly
closing and it will only be a matter of time before Earth stops
transmitting these types of signals -- at least unintentionally (
active SETI is a proactive attempt to contact ETI's with radio signals).
Due
to this revelation, the entire equation as a means to both classify and
quantify certain types of civilizations becomes quite meaningless and
arbitrary. At best, it's a way of searching for a very narrow class of
civilizations under very specific and constrained conditions.
Rather,
SETI should continue to redefine the ways in which ETI's could be
detected. They should try to predict future means of communication
(like quantum communication schemes) and ways to identify these
signals. They should also look for artificial objects such as
megascale engineering and artificial calling cards (see Arnold, "
Transit Lightcurve Signatures of Artificial Objects").
The future of advanced intelligenceAlthough
possibly outside the auspices of this discussion, the Drake Equation
does not account for the presence of post-radio capable civilizations,
particularly
post-Singularity machine intelligences. This is a problem because of what these types of civilizations might be capable of.
The
equation is used to determine the number of radio capable civilizations
as they conduct their business on their home planet. Again, this is a
vary narrow view of ETI's and the space of all possible advanced
civilizational types. Moreover, it does not account for any migratory
tendency that advanced civs may have.
The Drake Equation does not tell us about exponential civilizational growth on account of
Von Neumann probe
disbursement. It does not tell us where advanced ETI's may be dwelling
or what they're up to (e.g. Are they outside the Galaxy? Do they live
inside
Jupiter Brains?
Do they phase shift outside of what we regard as habitable space?
etc.). This is a serious shortcoming because the answers to these
questions should help us determine not just where we should be looking,
but they can also provide us with insight as to the makeup of advanced
intelligence life and our own potential trajectory.
In other
words, post-Singularity ETI's may represent the most common mode of
existence for late-stage civilizations. And that's who we should be
looking for rather than radio transmitting civs.
Are we alone?Michael Crichton
once put out a very weak argument against the Drake Equation. He
claimed that SETI was a religious endeavor because it was a search for
imaginary entities. He is wrong, of course; we should most certainly
search for data where we think we might find it. I believe, despite the
low odds, that it is reasonable to assume that our search for life on
other planets is warranted. Even a negative result can be meaningful.
Consequently, SETI should keep listening, but
expect to
hear nothing. If we should suddenly hear something from the depths of
space, then we will have to seriously re-evaluate our assumptions.
At
the same time we should find better ways to detect advanced life and
tweak the Drake Equation in such a way as to account for the missing
variables and factors I mentioned earlier.
Again, and more
generally, we should probably adopt the contact pessimist's frame. Back
in the 60's and 70's, when the contact optimists like Sagan, Shklovskii
and Drake ruled the Earth, it was not uncommon to think that
N in the equation fell somewhere between 10x6 to 10x9.
These days, in the post
Tipler and
Hart era of
astrosociobiology, cosmologists and astrobiologists have to take such factors into consideration as Von Neumann probes, the Fermi Paradox, the
Rare Earth Hypothesis, stronger variants of the
anthropic principle and
catastrophism.
Put
another way, as we continue to search for advanced ETI's, and as we
come to discover the absurdity of our isolation here on Earth, we may
have no choice but to accept the hypothesis that advanced life does not
venture out into space for whatever reason (the most likely being
self-destruction).
Our other option is to cross our fingers and
hope that something radical and completely unpredictable lies on the
other side of the technological Singularity.