Matteo Cantiello edited Ne.tex  about 10 years ago

Commit id: 3c9f6977f27e253790d10cb1a33e0b1c3299b2a9

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$n_e$ Is the \textbf{fraction of Earth-like planets}. A measure of how common are planets that can likely support biological life as we know it.   The definition is a little lose, but the idea is having a rocky planet in the so called Goldilocks or habitable zone, a range of distances from the host star where temperature at the surface is just about right for liquid water to be present. This might well be a restrictive definition of habitability, as life forms might thrive in very different environments As  fromwhat we are used to. But one has to start somewhere, and liquid water seems to have played a decisive role as a catalyst for biological life on Earth.   The news came up just in the  last few months: year we also know this factor!  Earth-like planets are very common. Statistically speaking at least  1 in 5 planets around Sun-like stars could potentially support life \cite{Petigura_Howard_Marcy_2013}.And Sun-like stars are extremely common, resulting in about 10 billion of habitable planets just in the Galaxy and the closest to us potentially within 12 light years.\\  $n_e \approx$ 0.2