A New Empirical Constraint on the Prevalence of Technological Species in the Universe
To cite this article:
Frank A. and Sullivan W.T. III. Astrobiology . May 2016, 16( 5): 359-362. https://doi.org/10.1089/ast.2015.1418
Published in Volume: 16 Issue 5: May 13, 2016
Online Ahead of Print: April 22, 2016
A. Frank1 and W.T. Sullivan III2
1Department of Physics and Astronomy, University of Rochester, Rochester, New York.
2Department of Astronomy and Astrobiology Program, University of Washington, Seattle, Washington.
Address correspondence to:
A. Frank
Department of Physics and Astronomy
University of Rochester
Rochester, NY 14620
E-mail: afrank@pas.rochester.edu
Submitted 5 October 2015
Accepted 16 February 2016
Abstract
Abstract
In this article, 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 set a firm lower bound on the probability that one or more 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, humanity is not the only time technological intelligence has evolved. This constraint has important scientific and philosophical consequences.
Key Words: Life—Intelligence—Extraterrestrial life.
Astrobiology 2016, 359–362.
FREE PDF GRATIS: Astrobiology
Key Words: Life—Intelligence—Extraterrestrial life.
FREE PDF GRATIS: Astrobiology