Description

Book Synopsis
Exploring the astronomical, biological, and cultural factors that determine whether extraterrestrial life is abundant or rare, leading scientists and historians use the Drake Equation as a springboard to identify essential topics and guide their assumptions. An accessible overview of the field of astrobiology for both established and incoming researchers.

Trade Review
'Now, over a half century after Drake's original formulation, Douglas Vakoch and Matthew Dowd have brought together a group of scholars to assess the equation's place in the history of astrobiology … the Drake equation may reveal as much about the historical epistemology of science as it does about the ongoing search for a way to communicate with intelligent life in the universe.' Greg Eghigian, Isis

Table of Contents
List of contributors; Foreword Frank Drake; Preface; Acknowledgements; Introduction Steven Dick; 1. Rate of formation of stars suitable for the development of intelligent life, R*, pre-1961 David DeVorkin; 2. Rate of formation of stars suitable for the development of intelligent life, R*, 1961 to the present Patrick François and Danielle Briot; 3. Fraction of stars with planetary systems, fp, pre-1961 Matthew F. Dowd; 4. Fraction of stars with planetary systems, fp, 1961 to the present Chris Impey; 5. Number of planets, per solar system, with an environment suitable for life, ne, pre-1961 Florence Raulin Cerceau; 6. Number of planets, per solar system, with an environment suitable for life, ne, 1961 to the present Danielle Briot and Jean Schneider; 7. Fraction of suitable planets on which life actually appears, fl, pre-1961 Stephané Tirard; 8. Fraction of suitable planets on which life actually appears, fl, 1961 to the present David J. Des Marais; 9. Fraction of life-bearing planets on which intelligent life emerges, fl, pre-1961 Michael Crowe; 10. Fraction of life-bearing planets on which intelligent life emerges, fl, 1961 to the present Lori Marino; 11. Fraction of civilizations that develop a technology that releases detectable signs of their existence into space, fc, pre-1961 Florence Raulin Cerceau; 12. Fraction of civilizations that develop a technology that releases detectable signs of their existence into space, fc, 1961 to the present Seth Shostak; 13. Length of time such civilizations release detectable signals into space, L, pre-1961 David Dunér; 14. Length of time such civilizations release detectable signals into space, L, 1961 to the present Garry Chick; Afterword Paul Davies; Index.

The Drake Equation Estimating the Prevalence of Extraterrestrial Life through the Ages 8 Cambridge Astrobiology Series Number 8

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    A Hardback by Douglas A. Vakoch, Matthew F. Dowd, Frank Drake

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      View other formats and editions of The Drake Equation Estimating the Prevalence of Extraterrestrial Life through the Ages 8 Cambridge Astrobiology Series Number 8 by Douglas A. Vakoch

      Publisher: Cambridge University Press
      Publication Date: 7/2/2015 12:00:00 AM
      ISBN13: 9781107073654, 978-1107073654
      ISBN10: 1107073650
      Also in:
      Astrology

      Description

      Book Synopsis
      Exploring the astronomical, biological, and cultural factors that determine whether extraterrestrial life is abundant or rare, leading scientists and historians use the Drake Equation as a springboard to identify essential topics and guide their assumptions. An accessible overview of the field of astrobiology for both established and incoming researchers.

      Trade Review
      'Now, over a half century after Drake's original formulation, Douglas Vakoch and Matthew Dowd have brought together a group of scholars to assess the equation's place in the history of astrobiology … the Drake equation may reveal as much about the historical epistemology of science as it does about the ongoing search for a way to communicate with intelligent life in the universe.' Greg Eghigian, Isis

      Table of Contents
      List of contributors; Foreword Frank Drake; Preface; Acknowledgements; Introduction Steven Dick; 1. Rate of formation of stars suitable for the development of intelligent life, R*, pre-1961 David DeVorkin; 2. Rate of formation of stars suitable for the development of intelligent life, R*, 1961 to the present Patrick François and Danielle Briot; 3. Fraction of stars with planetary systems, fp, pre-1961 Matthew F. Dowd; 4. Fraction of stars with planetary systems, fp, 1961 to the present Chris Impey; 5. Number of planets, per solar system, with an environment suitable for life, ne, pre-1961 Florence Raulin Cerceau; 6. Number of planets, per solar system, with an environment suitable for life, ne, 1961 to the present Danielle Briot and Jean Schneider; 7. Fraction of suitable planets on which life actually appears, fl, pre-1961 Stephané Tirard; 8. Fraction of suitable planets on which life actually appears, fl, 1961 to the present David J. Des Marais; 9. Fraction of life-bearing planets on which intelligent life emerges, fl, pre-1961 Michael Crowe; 10. Fraction of life-bearing planets on which intelligent life emerges, fl, 1961 to the present Lori Marino; 11. Fraction of civilizations that develop a technology that releases detectable signs of their existence into space, fc, pre-1961 Florence Raulin Cerceau; 12. Fraction of civilizations that develop a technology that releases detectable signs of their existence into space, fc, 1961 to the present Seth Shostak; 13. Length of time such civilizations release detectable signals into space, L, pre-1961 David Dunér; 14. Length of time such civilizations release detectable signals into space, L, 1961 to the present Garry Chick; Afterword Paul Davies; Index.

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