Things to consider:
Formulas were developed to calculate the number of communicating civilizations. The number of communicating civilizations (N) can be calculated by the following formulas:
N=N*fpneflfifc
N=R*fpneflfifcL
Note: 2nd letters below are subscripts.
Where
N*= Number of stars in the observable universe.
R*= Rate of star formation.
fp= Fraction of stars with planets.
ne= Mean number of planets per star with environments suitable for life.
fl= Fraction of these planets on which life does not arise.
fi= Fraction of life-bearing planets on which intelligent life evolves.
fc= Fraction of these planets which develop the technology needed to use radio
communication.
L= Mean life of communicating civilizations.
The first formula assumes that a communicating civilization, once formed, survives as long as the planet. The second takes account of the destruction of civilizations.
Note: Numbers below separated by a dash mark are superscripts.
In 1958, Shapley first calculated in “Of Stars And Men,� that there are:
10-20 stars in the universe.
10-11stars in galaxy.
10-9 galaxies.
10-17 stars with planets.
10-14 planets at a suitable distance for life to arise.
10-11 planets with a suitable atmosphere.
10-8 planets on which life arose.
10-5 planets with intelligent life.
10-2 planets with communicating civilizations.
Shapley did not consider the rate of star formation or the rate of destruction of civilizations and came up with a relatively conservative estimate of 10-2 communicating civilizations in the universe. He used low values to present the least favorable scenario.
Sagan and Drake later came up with a much more optimistic estimate of 10-10 to 10-16 communicating civilizations in the universe. They also gave a “high� and “low� optimistic estimate for communicating civilizations per universe and per galaxy.
Low Optimistic: 10-10 per universe.
0.1 per galaxy.
High Optimistic: 10-18 per universe.
10-7 per galaxy (this would give us a pretty good chance of finding life within our galaxy)!
Other Factors:
Most stars are double or triple and are inappropriate places to look for life due to unstable planetary systems.
Large and hot stars have short life times. Our Sun is a Type G2.
Small stars are not suitable because they have a smaller habitable zone.
The distance from a star is very constrained. For example, if the Earth were 1% closer to the Sun there would be a runaway “greenhouse effect.�
How are we going to find extraterrestrial life?
Spacecraft-No good. With our present understanding of physics it would take too long.
Robots-Possibly. At this point not realistic.
Radio Communication-Our best shot right now; however there is the problem of what frequency to transmit and receive at. SETI.
Formulas were developed to calculate the number of communicating civilizations. The number of communicating civilizations (N) can be calculated by the following formulas:
N=N*fpneflfifc
N=R*fpneflfifcL
Note: 2nd letters below are subscripts.
Where
N*= Number of stars in the observable universe.
R*= Rate of star formation.
fp= Fraction of stars with planets.
ne= Mean number of planets per star with environments suitable for life.
fl= Fraction of these planets on which life does not arise.
fi= Fraction of life-bearing planets on which intelligent life evolves.
fc= Fraction of these planets which develop the technology needed to use radio
communication.
L= Mean life of communicating civilizations.
The first formula assumes that a communicating civilization, once formed, survives as long as the planet. The second takes account of the destruction of civilizations.
Note: Numbers below separated by a dash mark are superscripts.
In 1958, Shapley first calculated in “Of Stars And Men,� that there are:
10-20 stars in the universe.
10-11stars in galaxy.
10-9 galaxies.
10-17 stars with planets.
10-14 planets at a suitable distance for life to arise.
10-11 planets with a suitable atmosphere.
10-8 planets on which life arose.
10-5 planets with intelligent life.
10-2 planets with communicating civilizations.
Shapley did not consider the rate of star formation or the rate of destruction of civilizations and came up with a relatively conservative estimate of 10-2 communicating civilizations in the universe. He used low values to present the least favorable scenario.
Sagan and Drake later came up with a much more optimistic estimate of 10-10 to 10-16 communicating civilizations in the universe. They also gave a “high� and “low� optimistic estimate for communicating civilizations per universe and per galaxy.
Low Optimistic: 10-10 per universe.
0.1 per galaxy.
High Optimistic: 10-18 per universe.
10-7 per galaxy (this would give us a pretty good chance of finding life within our galaxy)!
Other Factors:
Most stars are double or triple and are inappropriate places to look for life due to unstable planetary systems.
Large and hot stars have short life times. Our Sun is a Type G2.
Small stars are not suitable because they have a smaller habitable zone.
The distance from a star is very constrained. For example, if the Earth were 1% closer to the Sun there would be a runaway “greenhouse effect.�
How are we going to find extraterrestrial life?
Spacecraft-No good. With our present understanding of physics it would take too long.
Robots-Possibly. At this point not realistic.
Radio Communication-Our best shot right now; however there is the problem of what frequency to transmit and receive at. SETI.
Comment