Lecture 41: Science Fact or
Science Fiction?
Intelligent Life in the
Universe
Four Opinions:
1. It is highly likely that
intelligent life has arisen elsewhere in the Universe.
2. There is no evidence of
extraterrestrial visits to the Earth, now or in the past.
3. Lack of visits may be
explained by the extreme difficulty of interstellar travel.
4. If we do make contact, it
will be by receiving radio signals.
Basic Requirements for Life
Energy
Warmth to permit
liquid water (liquid methane?)
Energy to fuel
chemical reactions
Complex chemistry
Elements heavier
than H and He
Carbon as building
blocks for complex molecules
Protection from harmful UV
light
Mutations inhibit
emergence of complex life
Ozone layer,
underwater, or underground
Extreme Life on Earth
Dark Life
Bacteria
that thrive many kilometers beneath the Earth or deep in polar ice.
Hot Life
Microbes
surviving in boiling geysers, pools and deep ocean thermal vents
On the Moon:
Strep bacteria
survived 3 years on the lunar surface!
Life in the Solar System?
Mars
May have liquid
water and a thicker atmosphere in the past
Europa
Liquid water ocean
warmed by tides
Protected by outer
shell of ice
Titan
Methane chemistry
Complex molecules
present
Each may satisfy the basic
requirements for life to develop
What do we mean by
ÒIntelligentÓ
This usually means:
A highly advanced
technological civilization
Capable of
communicating across interstellar distances
Capable of
interstellar travel by spacecraft
Interested in
finding and communicating with other intelligences.
In other words: life like
us.
Do we qualify as
ÒIntelligentÓ?
Just barely:
Only had radio
communications technology for ~100 years
Only had limited
(short-duration) manned spaceflight for ~40 years.
Only
sent robotic spacecraft to the edges of our Solar System in the last decade
May
or may not yet have sufficiently sensitive radio reception technology
Sheer Weight of Numbers
The primary reason I think
life must have arisen elsewhere is the sheer number of stars in the visible
Universe:
~200 billion
galaxies in the visible Universe
~100 billion stars
per galaxy
Total of ~2x1022
(20 billion trillion) stars
Even
one chance in a trillion would yield more than 20 billion possible sites for
life.
Planetary Requirements for Life
Long-lived, stable star
Good: F, G, &K
stars: last > 3 Gyr
Bad:
O, B & A stars: short-lived, high UV output (damaging to organic molecules)
Bad:
M stars: small & dim, powerful flaring
Stable orbital environment
Excludes more binary
star systems
Metals=chemically evolved
environment
Need metals to make
rocky planets
Need carbon for
complex molecules
The Drake Equation
N=number of advanced civilizations in the Galaxy
R*=rate at which Sun-like stars form
fp=fraction of stars with planetary systems
ne=number of Earth-like planets per system
fl=fraction of Earth-like planets with life
fi=fraction where intelligent life has evolved
fc=fraction with communication technology
L=lifetime of an advanced civilization
Measurement and Conjecture
Only the first 3 terms of the
Drake Equation can be measured by astronomers:
Star formation rate:
R*~ 1 per
year (F, G, & K stars)
Fraction of Stars with
Planets
fp~
0.1-0.2 from recent planet searches
ne
number of Earth-like planets per system may be measurable in the next few years
The rest are purely
conjectural
Shameless Optimism
One very optimistic view:
ne=0.1 (1
in 10 solar systems have earths)
fl=1 (if earth-like, life is inevitable)
fi= (if
life, intelligence is inevitable)
fc= (if
intelligence, technology is inevitable)
L=100 years (we made
it this farÉ.so farÉ.)
Extraterrestrial Visitations?
No.
ÒExtraordinary claims require
extraordinary proofÓ
No extraordinary proof has
been offered:
Fuzzy photographs
Anecdotal accounts
of visits & abductions
Claims of government
conspiracies
These do not count
There are unexplained
sightings, but failure to explain them does not justify a leap to a truly wild
explanations.
Where are they?
The extreme difficulty of
interstellar travel is a plausible explanation of a lack of visits.
The distances between stars
are enormous:
Need very large
amounts of time or
Extremely large
amounts of energy
The fastest spacecraft:
Voyager 1&2
Outward bound at 15
km/sec (0.005% c)
Need 80,000 years to
reach the nearest stars
Relativistic Starships
Accelerate a starship to
near-light speeds
Need 0.1c to reach
nearest star in 50 years
Energy costs are enormous
Amount
of fuel increases exponentially with the acceleration time (use more fuel at
first)
50% max efficiency
for matter/anti-matter fuel
But the production
efficiency is extremely low
Possible given a sufficiently
advanced technology?
Talk is Cheap! (and travels
at the speed of light)
If you really want to bridge
interstellar distances, use light to send messages.
Messages travel at
the speed of light
Very low energy cost
per message
What wavelengths to use?
Microwaves
1000-10000 MHz is a region of relatively low cosmic background ÒnoiseÓ
Lasers
at visible to IR wavelengths: very few natural lasers in the sky to cause
confusion
Earth is already on-the-air
We have been inadvertently
beaming radio signals into space for the last 80 years:
Radio broadcasts
from the 1920s onward
Television
broadcasts from the 1950s onward
We could detect
these with current technology
Episodes of ÒI Love LucyÓ
will have already reached most solar neighborhood stars (~40 light years)É is
this a good thing?
Increasing radio silence
EarthÕs radio brightness has
been decreasing
Introduction &
spread of cable TV
Increased
use of ÒdirectedÓ communication (e.g., fiber optics, beamed satellite, etc.)
Sufficiently advanced
civilizations may emit less Òwaste radioÓ & become radio quiet:
If a
civilization wants to be found, it may have to deliberately broadcast its
presence.
The SearchÉ
SETI:
Search for
Extra-Terrestrial Intelligence
A relatively inexpensive
search strategy to look for radio signals from extraterrestrial civilizations.
Phoenix project of
the SETI Institute
Optical & Microwave
SETI at Harvard
Various smaller
projects
What are we looking for?
Signals that appear
ÒartificialÓ
Very
narrow ÒbandwidthÓ (<300 Hz, the narrowest natural maser sources)
Pulsed signals
(common way to encode information)
Highly polarized
signals (another encoding scheme)
Very little
frequency ÒdriftÓ
So far, no detectionsÉ
Pioneer 10 detected. Nice to
know we can detect our own artificial signals from deep space.
What if we detect something?