seager {extraterrestrial} | R Documentation |
The Seager 2013 equation
Description
An alternative to the Drake 1961 equation. The Seager equation considers the detection biogenic gases in the estimation of planets harboring life.
Usage
seager(Ns, fQ, fHZ, fo, fL, fS)
Arguments
Ns |
number of stars |
fQ |
fraction of quiet stars |
fHZ |
fraction with rocky planets within the habitable zone. |
fo |
fraction of observable planets. |
fL |
fraction of planets with life. |
fS |
fraction of planets with detectable gaseous signatures. |
Value
N number of planets with signs of life.
References
https://www.cfa.harvard.edu/events/2013/postkepler/Exoplanets_in_the_Post_Kepler_Era/Program_files/Seager.pdf
The Drake Equation Revisited: Interview with Planet Hunter Sara Seager Devin Powell, Astrobiology Magazine 4 September 2013.
Examples
seager(Ns=.45, fQ=0.5, fHZ=0.2, fo=0.05, fL=0.5, fS=500)
[Package extraterrestrial version 0.1.0 Index]