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Defense Intelligence Reference Document An Introduction To The Statistical Drake Equation

Defense Intelligence Agency · 55 pages · text from the file's own layer

This Defense Intelligence Agency reference document, dated 11 March 2010, is one of the advanced technology reports produced in FY 2009 under the Advanced Aerospace Weapon System Applications (AAWSA) program. It introduces the Statistical Drake Equation, which replaces each factor of Frank Drake's 1961 equation with a uniform random variable to estimate how far away the nearest extraterrestrial civilization is. In the worked example, there is a 75% probability that the nearest civilization lies between 1,361 and 3,979 light years from Earth.

  • p. 2 …a series of advanced technology reports produced in FY 2009 under the Defense Intelligence Agency, gb…
  • p. 4 …in the universe, how far from us they exist, and possibly how much more advanced than…
  • p. 7 …that the galaxy is pulsing and humming with advanced societies, and, therefore, that the nearest such…
  • p. 8 …Perhaps the evolution of advanced life forms is improbable. Or it may be that complex life…
  • p. 9 …On the other hand, there must be quite different pathways to an advanced civilization of specified…
  • p. 11 …In other words, we have transformed the classical and simplistic Drake equation (7) into an advanced…
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' 6 R" I. • ) c;,,,,,,-,. l C
Ef_Dtstance(N)= ifN • ifN
where the positive constant C is defined by
C = -' 6 Rl,,1<rn he;""'-" c:c 28845 light years.
Equations (5) and (6) are the starting point to understand the origin of the Drake
equation that we discuss in detail in Section 3 of this paper.
Let us just complete this section by pointing out three different numerical cases of the
distance law (5):
( 5)
(6)
• We know that we exist, so N may not be smaller than 1, i.e., N z I. Suppose then
that we are alone in the galaxy, i.e., that N=l. Then the distance law (5) yields as
distance to the nearest civilization from us just the constant C, i.e., 28,845 light
years. This is about the distance in between ourselves and the center of the galaxy
(i.e. the Galactic Bulge). Thus, this result seems to suggest that, if we do not find
any extraterrestrial civilization around us in these outskirts of the galaxy where we
live, we should look around the Galactic Center first. And this is indeed what is
happening, i.e., many SETI searches are actually pointing the antennas towards the
Galactic Center, looking for beacons (see, for instance ref. [1]).
• Suppose next that N=l000, i.e. there are about a thousand extraterrestrial
communicating civilizations in the whole galaxy right now. Then the distance law (5)
yields an average distance of 2,885 light years. This is a distance that most
radiotelescopes in Earth may not reach for SETI searches right now: hence the need
to build larger radiotelescopes, like ALMA, LOFAR and the SKA.
• Suppose finally that N=l000000, i.e., there are a million communicating civilizations
now in the galaxy. Then the distance law (5) yields an average distance of 288 light
years. This is within the (upper) range of distances that our current radiotelescopes
may reach for SETI searches, and that justifies all SETI searches that have been
done so far in the first fifty years of SETI (1960-2010).
In conclusion, interpolating the above three special cases of N, we may say that the
distance law (5) yields the following key diagram of the average ET distance vs. the
assumed number of communicating civilizations, N, in the galaxy right now (Figure 1):
6
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Report, from the dia collection. The PDF is mirrored here; the original link is above. 55 pages are in the text index: search them above, or from the library's search.