Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-28T14:24:55.963Z Has data issue: false hasContentIssue false
  • English
  • Français

Spatial dispersion of interstellar civilizations: a probabilistic site percolation model in three dimensions

Published online by Cambridge University Press:  02 October 2012

Thomas W. Hair  and
Andrew D. Hedman
Thomas W. Hair*
Affiliation:
College of Arts and Sciences, Florida Gulf Coast University, 10501 FGCU Blvd, South, Fort Myers, FL 33965, USA
Andrew D. Hedman
Affiliation:
College of Arts and Sciences, Florida Gulf Coast University, 10501 FGCU Blvd, South, Fort Myers, FL 33965, USA
*
e-mail: twhair@fgcu.edu
Get access Rights & Permissions [Opens in a new window]

Abstract

A model of the spatial emergence of an interstellar civilization into a uniform distribution of habitable systems is presented. The process of emigration is modelled as a three-dimensional probabilistic cellular automaton. An algorithm is presented which defines both the daughter colonies of the original seed vertex and all subsequent connected vertices, and the probability of a connection between any two vertices. The automaton is analysed over a wide set of parameters for iterations that represent up to 250 000 years within the model's assumptions. Emigration patterns are characterized and used to evaluate two hypotheses that aim to explain the Fermi Paradox. The first hypothesis states that interstellar emigration takes too long for any civilization to have yet come within a detectable distance, and the second states that large volumes of habitable space may be left uninhabited by an interstellar civilization and Earth is located in one of these voids.

Keywords

astrobiologyextraterrestrial intelligenceFermi paradoxpercolation theoryspatial dispersion
Type
Research Article
Information
International Journal of Astrobiology , Volume 12 , Issue 1 , January 2013 , pp. 45 - 52
Copyright
Copyright © Cambridge University Press 2012

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Brin, D. (1983). Q. J. R. Astron. Soc. 24, 287.Google Scholar
Broadbent, S. & Hammersley, J. (1957). Proc. Camb. Phil. Soc. 53, 629.CrossRefGoogle Scholar
Freitas, R. (1980). J. Br. Interplanet Soc. 33, 251.Google Scholar
Gros, C. (2005). J. Br. Interplanet Soc. 58, 108.Google Scholar
Hair, T. (2011). Int. J. Astrobiol. 10, 131.CrossRefGoogle Scholar
Jones, E.M. (1981). Icarus 46, 328.CrossRefGoogle Scholar
Landis, G. (1998). J. Br. Interplanet Soc. 51, 163.Google Scholar
Lineweaver, C.H. (2001). Icarus 151, 307.Google Scholar
Long, K.F. (2011). Deep Space Propulsion: A Roadmap to Interstellar Flight. Springer, Berlin.Google Scholar
Newman, W. & Sagan, C. (1981). Icarus 46, 293.CrossRefGoogle Scholar
Science: ‘Project Ozma’ Time, April 18, 1960 (web version accessed 17 April 2011).Google Scholar
Webb, C.S. (2002). If the Universe is Teeming with Aliens – Where is Everybody?: Fifty Solutions to the Fermi Paradox and the Problem of Extraterrestrial Life. Springer, Berlin.Google Scholar
Wesson, P. (1990). Q. J. R. Astron. Soc. 31, 161.Google Scholar