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Life in the Universe

Date post: 01-Jan-2016
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Life in the Universe. What We Want to Know. There is intelligent life on Earth Could it have happened elsewhere? Alien Spacecraft/UFO’s? Evidence is unconvincing Can we calculate probabilities? No - PowerPoint PPT Presentation
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Life in the Universe What We Want to Know •There is intelligent life on Earth •Could it have happened elsewhere? •Alien Spacecraft/UFO’s? •Evidence is unconvincing •Can we calculate probabilities? •No •Drake’s Equation is a way to estimate how many intelligent civilizations (besides ours) are in the galaxy
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Page 1: Life in the Universe

Life in the UniverseWhat We Want to Know

•There is intelligent life on Earth•Could it have happened elsewhere?

•Alien Spacecraft/UFO’s?•Evidence is unconvincing

•Can we calculate probabilities?•No•Drake’s Equation is a way to estimate how many intelligent civilizations (besides ours) are in the galaxy

Page 2: Life in the Universe

Drake’s Equation

N = number of civilizations in our galaxy

R* = rate at which solar-type stars form

fP = fraction of those stars with planets

nPM= number of suitable planets and moons

fl = probability of getting life

fi = probability of life evolving intelligence

L = lifetime of intelligent species

N = R* fP nPM fl fi L

Page 3: Life in the Universe

Stars, Planets, and Moons

N = R* fP nPM fl fi L

R* = rate at which solar-type stars form = 1/year

fP = fraction of those stars with planets = 0.1 – 0.5

Page 4: Life in the Universe

The right temperatureN = R* fP nPM fl fi L

nPM = number of suitable planets and moons

= 0.1 - 1 Too hot

Too cold

Just right

Page 5: Life in the Universe

Getting Life StartedN = R* fP nPM fl fi L

fl = probability of getting life started = ?? – 1

•The basic building blocks of life (elements, amino acids) are common•Life started fairly quickly on Earth

•But even very simple life is extremely complicated/unlikely

Page 6: Life in the Universe

Getting Advanced CivilizationN = R* fP nPM fl fi L

fi = probability of life evolving intelligence = ?? – 0.5

•Evolution follows naturally from physical laws

•Evolution naturally leads to some complexity•Intelligence is a very useful kind of complexity

•Catastrophes could wipe out advanced life•Evolution may sometimes lead to dead ends

Page 7: Life in the Universe

Keeping Civilization AliveN = R* fP nPM fl fi L

L = Mean lifetime of intelligent life = 100 – 109 years

•We have the ability to destroy civilization•We are also damaging our environment•We are using up non-renewable resources

•Civilizations may “mature” – some evidence•Sustainable civilizations is technically possible

Page 8: Life in the Universe

Are We Alone?N = R* fP nPM fl fi L

•Intelligent life could be rare•Intelligent life could be common

R*= 1/yr fP = 0.1 – 0.5nPM = 0.1 - 1 fl = ?? – 1 fi = ?? – 0.5 L = 100 – 109 yr

= 0 - billions

My opinion:•We are first in the galaxy, and possibly the visible universe•Ultimately, this is an experimental question

Page 9: Life in the Universe

Searching Stars for Life

How can we know if intelligent life exists around other stars?•Visitors from outer space?

•Fermi paradox – If they exist, why aren’t they here?•Travel to distant stars?•Search for signals from space?

Page 10: Life in the Universe

Traveling Between the Stars

How Best to do it?•Best chemical rockets: 10-4c – 10-3c

•Millenia to nearest star•Nuclear rockets, solar sails, ion engines

•10-2c – 10-1c•Decades – centuries to nearest star

•Solutions:•Unmanned missions•Generation ships – parents have children•Long life span/hibernation

Page 11: Life in the Universe

Signals From Space

•We can send/receive electromagnetic signals throughout the universe at c

•The universe is a noisy place•Dust/gas/etc. blocks many wavelengths•Some radiation can penetrate gas and dust•In radio waves, the Earth outshines the Sun

Page 12: Life in the Universe

Signals From Space•We send accidental and intentional signals into space•We also look for signals from alien civilizations

•Nothing found so far

Page 13: Life in the Universe

Final Exam Equations

sin2 2

l

d

P2 = a3

F = ma

2

GMmF

r

(M + m)P2 = a3 c = f c = m/s

shift rest rad

rest

v

c

E = hfP = knT

maxT = 2900 Km

4 H + 2e - He + 2 neutrino + energy

L = 4d2B

3.26 lyd

p

4 2L T R

L T R

v = H0d H0 = 22 km/s/Mly

Page 14: Life in the Universe

End of Material for Test 4

Questions?


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