Description Usage Arguments Value References Examples
An alternative to the Drake 1961 equation. The Seager equation considers the detection biogenic gases in the estimation of planets harboring life.
1 | seager(Ns, fQ, fHZ, fo, fL, fS)
|
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. |
N number of planets with signs of life.
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.
1 | seager(Ns=.45, fQ=0.5, fHZ=0.2, fo=0.05, fL=0.5, fS=500)
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