Will this technical marvel vindicate the “Drake Equation” ?
How many alien societies exist, and are detectable? This famous formula gives us an idea. The Drake Equation, which was the agenda for a meeting of experts held in West Virginia in 1961, estimates N, the number of transmitting societies in the Milky Way galaxy. The terms are defined as follows:
N : The number of civilizations in the Milky Way galaxy whose electromagnetic emissions are detectable.
R* : The rate of formation of stars suitable for the development of intelligent life (number per year).
fp : The fraction of those stars with planetary systems.
ne : The number of planets, per solar system, with an environment suitable for life.
fl : The fraction of suitable planets on which life actually appears.
fi : The fraction of life bearing planets on which intelligent life emerges.
fc : The fraction of civilizations that develop a technology that produces detectable signs of their existence.
L : The average length of time such civilizations produce such signs (years).
Where Is Webb? NASA/Webb
'WhereIsWebb' shows the status of Webb on its journey to L2 orbit. The page constantly updates as Webb travels, deploys, and cools to operating temperature. The most recently completed deployment step for Webb is displayed along a timeline that also indicates the major deployment phases. Note...
jwst.nasa.gov
How many alien societies exist, and are detectable? This famous formula gives us an idea. The Drake Equation, which was the agenda for a meeting of experts held in West Virginia in 1961, estimates N, the number of transmitting societies in the Milky Way galaxy. The terms are defined as follows:
N : The number of civilizations in the Milky Way galaxy whose electromagnetic emissions are detectable.
R* : The rate of formation of stars suitable for the development of intelligent life (number per year).
fp : The fraction of those stars with planetary systems.
ne : The number of planets, per solar system, with an environment suitable for life.
fl : The fraction of suitable planets on which life actually appears.
fi : The fraction of life bearing planets on which intelligent life emerges.
fc : The fraction of civilizations that develop a technology that produces detectable signs of their existence.
L : The average length of time such civilizations produce such signs (years).