Drake Equation

From A+ Club Lesson Planner & Study Guide

The Drake Equation is a probability (possibility) measurement of the existence of extraterrestrial life

  • formulated in 1961 by Dr. Frank Drake

N = R* • ƒp • ne • ƒ1 • ƒi • ƒc • L

R* = the average rate of star formation in our Galaxy

ƒp = the fraction of those stars that have planets

ne = the average number of planets that can potentially support life per star that has planets

ƒ1 = the fraction of planets that could support life that actually develop life at some point

ƒi = the fraction of planets with life that actually go on to develop intelligent life (civilizations)

ƒc = the fraction of civilizations that develop a technology that releases detectable signs of their existence into space

L = the length of time for which such civilizations release detectable signals into space

from Drake Equation (wikipedia)

  • Drake's estimate:

R = 1 yr−1 (1 star formed per year, on the average over the life of the galaxy; this was regarded as conservative)

fp = 0.2 to 0.5 (one fifth to one half of all stars formed will have planets)

ne = 1 to 5 (stars with planets will have between 1 and 5 planets capable of developing life)

fl = 1 (100% of these planets will develop life)

fi = 1 (100% of which will develop intelligent life)

fc = 0.1 to 0.2 (10–20% of which will be able to communicate)

L = 1000 to 100,000,000 communicative civilizations (which will last somewhere between 1000 and 100,000,000 years)

= between 1000 and 100,000,000 planets with civilizations in the Milky Way Galaxy

  • Fermi paradox
    • in 1950, physicist Enrico Fermi casually thought up the paradox that, if extraterrestrial life is so probable (likely), then we would have encountered it by now
      • "But where is everybody?" Fermi asked
  • a 2018 paper called, "Dissolving the Fermi Paradox" concluded that the probability of intelligent life outside of earth is unlikely
    • the authors incorporated additional models of chemical and genetic transitions into life
      • thus we should not be surprised by Fermi's conclusion, "But where is everybody?"