A New Empirical Constraint on the Prevalence of Technological Species in the Universe

TL;DR

This paper uses recent exoplanet data and modifications to the Drake Equation to establish a lower bound on the likelihood of technological species existing elsewhere in the universe, suggesting humanity is not unique if this probability exceeds 10^-24.

Contribution

It introduces a new empirical constraint on the prevalence of technological species by refining the Drake Equation with current astrophysical data.

Findings

Probability > 10^-24 implies multiple technological species exist

Provides a firm lower bound on the likelihood of extraterrestrial technological life

Implications for scientific understanding and philosophical perspectives on extraterrestrial intelligence

Abstract

In this paper we address the cosmic frequency of technological species. Recent advances in exoplanet studies provide strong constraints on all astrophysical terms in the Drake Equation. Using these and modifying the form and intent of the Drake equation we show that we can set a firm lower bound on the probability that one or more additional technological species have evolved anywhere and at any time in the history of the observable Universe. We find that as long as the probability that a habitable zone planet develops a technological species is larger than ~$10^{-24}$, then humanity is not the only time technological intelligence has evolved. This constraint has important scientific and philosophical consequences.