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Lecture
35: Intelligent Life in the Universe
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| Astronomy
101/103 |
Terry
Herter, Cornell University
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Lecture
Topics
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- Probabilities
- Rates
and totals
- The
Drake equation
- Computes
the expected number of technical civilizations in
the galaxy
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Are we Alone?
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- 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.
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Probabilities
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Probablities
(cont'd)
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Suppose
Nw = 100
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Rates and
Totals
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- 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)
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Total Number
of
Stars alive
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- Suppose:
Rstar = 1 star/year (represented by spikes
above) and stars live only 10 years.
- 10
stars would be alive at any given time.
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Number of
Civilizations
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- Suppose
that each star developed a civilization.
- If
the lifetime of the civilization is tl then
the total number of civilizations alive is:
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The Drake
Equation
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- Attempts
to quantify the number of civilizations that might exist
in the galaxy.
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Named
after Frank Drake
We
now go over each of the terms in the Drake equation make
some (optimistic?) estimates.
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Rate
of Star
Formation
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Rstar = Rate at which stars
are born, averaged over the lifetime of the galaxy. (Stars/year)
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Fraction
of Stars
having
Planets
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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:
- However,
only 3% of the sun-like stars in solar neighborhood
have giant planets
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Fraction
of Planets
Suitable
for Life
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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
- Accept
only F, G and K stars.
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Galactic
Habitable
Zone
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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.
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Simple Life
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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.
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Urey-Miller
Experiment
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- 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.
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Cyril
Ponnamperuma
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- 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.
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Creating
Organics
is easy
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- 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.
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Fraction
on which
Simple Life
Arises
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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:
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Fraction
which evolve
Intelligence
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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:
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Dinosaurs
and
Extinction
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- 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?
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Meteor
Impacts
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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)
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Fraction
which develop
Technology
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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,
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Average
Lifetime
of Technical
Civilization
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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.
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Uncertainties!
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- 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.
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Neighbors:
How far?
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- For
1,000,000 civilizations in the galaxy
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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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