The Indigenous Perspective on the Drake Equation express

Original: "Indigenizing the Drake Equation: how Indigenous methods can help us understand life in the Milky Way Galaxy"
· Hilding R. Neilson
arXiv:2606.26296 · 2026-06-24 · CC BY 4.0 · 1 min
Traditional knowledge flips the equation, and the Galaxy turns out to be densely populated.

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The Drake Equation is an attempt to guess the number of intelligent civilizations in our Galaxy. It’s like counting finished cakes in an unknown bakery: you know the ovens (stars), the baking sheets (planets), and the baking time. But were eggs added to the batter? Western science, relying on a single earthly recipe, considers them a rare ingredient. Indigenous knowledge flips the script: eggs are the basis of any cosmic dough, life is not an exception but the rule.

Suddenly, there aren't just a couple of cakes, but a whole pantry full.

Civilizations in such a universe aren’t flash-in-the-pan quickbreads but sourdough loaves — living for millennia. The equation spits out staggering numbers, and the search for intelligence turns from eavesdropping on radio noise into a communal meal. The irony is that Drake himself later considered the parameters of life and intelligence to be the stumbling block — precisely the factors that traditional cultures would never have taken for zero.

Frank Drake devised the equation for a 1961 conference, hoping to organize thoughts rather than get a number. Today it's less a calculator and more a mirror of our assumptions.

Sci-fi movies like 'Contact' build on the assumptions of the Drake Equation, but what if it was solved not by an astronomer, but by a bearer of traditional knowledge?

N = R_* \times f_p \times n_e \times f_l \times f_i \times f_c \times L
N — number of civilizations ready for contact; R* — star formation rate; fp — fraction of stars with planets; ne — number of habitable planets per star; fl — fraction of planets with life; fi — fraction where life becomes intelligent; fc — fraction of civilizations that release detectable signs; L — lifetime of a technological civilization.
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
origin of life biology prebiotic chemistry biosignature detection abiogenesis milky way technosignature search earth dwarf galaxy Price equation red dwarf habitability evolution drug discovery abundance rocky planet consciousness navigation genomics galactic evolution terrestrial exoplanet