# Use the sliders below to enter your estimates:

Average number of new stars formed in our galaxy annually (NASA estimates about 7):
Proportion of stars which have one or more planets (observations suggest 30+ percent):
Average number of planets/moons per solar system where basic life could potentially arise:
Percentage of life-compatible planets where basic life eventually does arise:
Percentage of basic-life planets where intelligent life eventually evolves:
Percentage of civilizations which eventually send signals into space (TV, radio, radar, etc.):
Average number of years that an advanced civilization will send such signals:
Probable communicating civilizations in the Milky Way:
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# The Drake Equation

From Wikipedia:

The Drake equation is a famous result in the fields of exobiology and the search for extraterrestrial intelligence (SETI). This equation was devised by Dr. Frank Drake (now Professor Emeritus of Astronomy and Astrophysics at the University of California, Santa Cruz) in 1960, in an attempt to estimate the number of extraterrestrial civilizations in our galaxy with which we might come in contact.

The main purpose of the equation is to allow scientists to quantify the uncertainty of the factors which determine the number of such extraterrestrial civilizations.

N= R*x fpx nex flx fix fcx L

• N is the number of civilizations in our galaxy with which we might hope to be able to communicate.
• R* is the average rate of star formation in our galaxy.
• fp is the fraction of those stars that have planets.
• ne is the average number of planets that can potentially support life per star that has planets.
• fl is the fraction of the above that actually go on to develop life at some point.
• fi is the fraction of the above that actually go on to develop intelligent life.
• fc is the fraction of civilizations that develop a technology that releases detectable signs of their existence into space.
• L is the length of time such civilizations release detectable signals into space.