Lecture 35: Intelligent Life in the Universe
Astronomy 101/103
Terry Herter, Cornell University
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Lecture
Topics
  • Probabilities
  • Rates and totals
  • The Drake equation
    • Computes the expected number of technical civilizations in the galaxy

Are we Alone?
  • Do other civilizations exist in the galaxy or elsewhere?
  • How might we estimate this statistically and what are the uncertainties?
  • We would like to quantify whether life and other civilizations, in particular, might exist in the galaxy.

Probabilities
  • How many dates might a guy get in this class?



Probablities
(cont'd)

Suppose Nw = 100

 


Rates and
Totals
  • Suppose
    • Rstar = Rate at which stars are born
      tl = Average lifetime of a star
  • How many stars are alive at a given time?
  • The number of stars is:
    • N = Rstar x tl (Rate times time)

Total Number
of
Stars alive
  • Suppose: Rstar = 1 star/year (represented by spikes above) and stars live only 10 years.
  • 10 stars would be alive at any given time.

Number of
Civilizations
  • Suppose that each star developed a civilization.
  • If the lifetime of the civilization is tl then the total number of civilizations alive is:

  • But this isn't the whole story ....

 


The Drake
Equation
  • Attempts to quantify the number of civilizations that might exist in the galaxy.
  • Named after Frank Drake



We now go over each of the terms in the Drake equation make some (optimistic?) estimates.

Rate
of Star
Formation

Rstar = Rate at which stars are born, averaged over the lifetime of the galaxy. (Stars/year)

  • There are ~100 billion stars in the galaxy today.
  • And the galaxy is about 10 billion years old.
    • R* ~ 10 stars/year

Fraction
of Stars
having
Planets

fp = Fraction having planetary systems.

  • If our understanding of star formation is correct, then planets are a natural consequence.
  • All stars could have planets, so we take:
    • fp ~ 1
  • However, only 3% of the sun-like stars in solar neighborhood have giant planets

Fraction
of Planets
Suitable
for Life

fh = Average number of life-suitable (habitable) planets within those systems having planets.

  • The ecosphere size varies with stellar type, but we might expect the odds to be similar to our solar system, so we choose
    • fh ~ 1/10
  • Accept only F, G and K stars.

Galactic
Habitable
Zone

To be discussed in class -

There are specific regions in the galaxy which may be more suitable to the formation of terrestrial worlds and survivability of life.


Simple Life

fs = Fraction of habitable planets on which at least simple life arises.

  • How likely is it for life to form? Is life rare?
  • It is certainly complex!

Laboratory experiments show that complex organic molecules can be formed in an atmosphere similar to that expected on the early earth.


Urey-Miller
Experiment
  • Harold Urey and Stanley Miller (1953)
  • Made "primordial soup" mixture
    • water, methane, carbon dioxide, ammonia
  • Passed simulated lightning through it.
  • Produced "gunk" containing many of the amino acids found in life today.

Cyril
Ponnamperuma
  • About a decade later constructed nucleotide bases in a similar manner.
  • Both experiments did not closely resemble the early atmosphere.
    • But showed biological molecules can be synthesized by nonbiological methods.

Creating
Organics
is easy
  • Using better knowledge of the primordial ocean and atmosphere.
  • Various energy sources can produce amino acids and nucleotide bases.
  • Possible energy sources: solar UV radiation, lightning, volcanic heat, natural radioactivity, and atmospheric shock waves produced by meteorites.

Fraction
on which
Simple Life
Arises

fs = Fraction of habitable planets on which at least simple life arises.

  • Making organics is easy as demonstrated by experiments, but creating life may not be. Some argue that life happens only under the right conditions.
  • Most optimistic case:
    • fs ~ 1

Fraction
which evolve
Intelligence

fi = Fraction of life-bearing planets on which intelligence evolves.

  • The appearance of a well-developed brain might not happen if left to random chance.
  • But, natural selection tends to single out the more adaptable, more intelligent species.
  • The optimistic view takes intelligence as inevitable:
    • fi ~ 1

Dinosaurs
and
Extinction
  • Dinosaurs "ruled" the world for ~100 million years, but were pretty stupid.
  • Was the mass extinction of the dinosaurs necessary for Homo Sapiens to evolve?

Meteor
Impacts

The Sky is Falling: Meteor Impacts

  • A 1 km rock, traveling at 30 km/sec:
    • Equivalent to 170,000 Megatons TNT.
    • Not a global effect
    • A 10 km object releases 1000 times more energy
    • One hits every 10-50 million years.
    • 5 x 109 people/ 10 x 106 yrs = 500 people/yr
      (higher probability than a plane crash)

Fraction
which develop
Technology

ft = Fraction of those intelligent life planets that develop a technological society.

  • It is hard to imagine an intelligent species avoiding technology.
  • Technical civilizations arose independently in many areas of the world.
  • Taking technological development to be inevitable,
    • ft ~ 1

Average
Lifetime
of Technical
Civilization

tl = Average lifetime of a technological civilization. (years)

  • How long does a technical civilization last?
  • We've had one for ~100 years.
  • There are many unknowns to our own future, let alone predicting how long another civilization might last.
  • Suppose the average lifetime of a technical civilization is 1 million years
    • 1% of the reign of the dinosaurs
    • 100 times longer than human civilization has existed!

      1 million civilizations in our galaxy.

Uncertainties!
  • Important - each term in the Drake equation (probably) gets more uncertain when proceeding from left to right.
  • For lack of a better example we have adopted an Earth/human bias when estimating various terms.
  • We do not know the uncertainties.

Neighbors:
How far?
  • For 1,000,000 civilizations in the galaxy
    • the average distance between them will be ~ 150 ly!!!
    • two-way communication will take at least 300 years!
  • If the lifetime of a technical civilization is less than 3000 years
    • Average distance is so large that civilizations will die, on average, before two-way communications can be established!
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