The ManDrake equation: Answer to the Fermi Paradox.

Answer to the Fermi Paradox

Where is everybody?

Everybody is having a party at Proxima Centauri, MCXIII Century

But you cannot go because you are still a kid.

In remastering the Drake equation (aka ManDrake EQUATION for the shake of pure joy) we are asking a different question.

How long will take to the planet earth to populate the solar system and the galaxy? Which is the population critical mass to do it?

We are considering that life thrives in the planet earth and the earth-moon system could make several attemps to generate intelligent life, which means the Homo Sapiens could be one of the multiple options to populate the solar system with intelligent life.

We are also considering a population limit for the planet as an important factor for the equation.

As a matter of fact we are considering a population cap for every celestial body colonized as well as a population cap for the High Earth Orbit Habitat.

PT = MP+MIQ+LP+HEOP+SPP+BAIP+IPP+SSSPL

PT= Base Population and time to populate two solar systems

MP= Mother planet population limit

MIQ= Mother planet attemps to create intelligent creatures

LP= Lunar population limit

HEOP= High Earth Orbit Population

SPP= Second Planet Population limit

SSP= Solar System Population Limit

BAIP= Biomechanoids Population

IPP= Interstellar Reverse Panspermia Population

SSSPL= Second Solar System Population Limit

The population critical mass is 1.5 x 10^20 people and the time is 11,113 centuries to populate two star systems in the galaxy.