Towards a Theory of Life

doi:10.1017/CBO9780511902574.005

2 - Towards a Theory of Life

from Part II - Origin of Planets and Life

Published online by Cambridge University Press: 05 December 2012

Steven Benner and

Edited by

Jonathan Lunine and

Chris Impey: Affiliation:
University of Arizona
Jonathan Lunine: Affiliation:
Cornell University, New York
José Funes: Affiliation:
Vatican Observatory, Vatican City

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Summary

Introduction

What is this thing called “life” that seems to interest everyone? And why are we looking for it so hard? Why, for example, are we seeking “Earth-like planets” in “habitable zones,” or the spectroscopic signatures of amino acids and carbohydrates in the interstellar dust? Why not just accept the perspective of Dr. Manhattan from The Watchmen: most of the universe appears uninhabitable, yet seems to get along quite well.

Certainly, it is easy to understand the motivation of SETI astronomers who seek intelligent life. They seek someone to talk to, someone who can teach us something, if it does not consume us, or destabilize our society with technological wizardry. If we physically encounter life of the type that SETI seeks, we will almost certainly recognize it as life. SETI-style life will have the attributes that we most value in life, whether it explains the secrets of dark matter or simply applies 40 of us to a recipe for Rigelian stew. But the higher probability seems now that we will not find anything so complex. The life that we seem most likely to encounter will be “primitive,” single-celled organisms visible only under the microscope. And the life that we now seem most likely to encounter will be detectable only by its chemical signatures, no longer able to grow after its first encounter with us.

Type: Chapter
Information: Frontiers of Astrobiology , pp. 25 - 47

DOI: https://doi.org/10.1017/CBO9780511902574.005 [Opens in a new window]

Publisher: Cambridge University Press

Print publication year: 2012

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