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2 - Revisiting The Fitness of the Environment

Published online by Cambridge University Press:  18 December 2009

Owen Gingerich
Affiliation:
Harvard-Smithsonian Center for Astrophysics
John D. Barrow
Affiliation:
University of Cambridge
Simon Conway Morris
Affiliation:
University of Cambridge
Stephen J. Freeland
Affiliation:
University of Maryland, Baltimore
Charles L. Harper, Jr
Affiliation:
John Templeton Foundation
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Summary

In 1913, long after Charles Darwin had argued for the fitness of organisms for their environment, the Harvard chemist Lawrence J. Henderson pointed out that the organisms would not exist at all except for the fitness of the environment itself. “Fitness there must be, in environment as well as in organism,” he declared near the outset of his classic work, The Fitness of the Environment (1913, p. 6). While most of Henderson's contemporaries ignored the philosophical implications of this work, as John Barrow and Frank Tipler have noted, it “still comprises the foundation of the Anthropic Principle as applied to biochemical systems” (1986, p. 143).

Henderson pointed out the uniqueness of hydrogen, carbon, and oxygen in the chemistry of living organisms. Another two decades would pass before astronomers would establish that these were three of the four most abundant elements in the cosmos; but Henderson was at least aware that these atoms were commonly found in the stars and planets. In his treatise, he began with the properties of water, just as William Whewell had done eight decades earlier in his far more teleologically oriented Bridgewater Treatise (1833).

Henderson grouped the notable qualities of water under two headings: (1) thermal properties and (2) interaction with other substances. As far as he was concerned, these were empirical, observed properties with minimal theoretical explanation. (Remember that Rutherford's nuclear atom was still a future concept, while quantum mechanics and the nature of the hydrogen bond lay many more years ahead.)

Type
Chapter
Information
Fitness of the Cosmos for Life
Biochemistry and Fine-Tuning
, pp. 20 - 30
Publisher: Cambridge University Press
Print publication year: 2007

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References

Barrow, J. D. and Tipler, F. J. (1986). The Anthropic Cosmological Principle. Oxford: Oxford University Press.Google Scholar
Denton, M. (1998). Nature's Destiny. New York, NY: The Free Press.Google Scholar
Gamow, G. (1970). My World Line: An Informal Biography. New York, NY: Viking Press.Google Scholar
Henderson, L. J. (1913). The Fitness of the Environment: An Inquiry into the Biological Significance of the Properties of Matter. New York: Macmillan. Repr. (1958) Boston, MP: Beacon Press; (1970) Gloucester, MA: Peter Smith.Google Scholar
Hoyle, F. (1981). The Universe: past and present reflections. Engineering and Science, XLV, no. 2, November.Google Scholar
Pauling, L. (1939). The Nature of the Chemical Bond. Ithaca, NY: Cornell University Press.Google Scholar
Salpeter, E. (1952). Nuclear reactions in stars without hydrogen. Astrophysical Journal, 115, 326–8. Repr. (1979) in A Source Book in Astronomy and Astrophysics, 1900–1975, ed. K. R. Lang and O. Gingerich. Cambridge, MA: Harvard University Press.CrossRefGoogle Scholar
Whewell, W. (1833). Astronomy and General Physics Considered with Reference to Natural Theology. (Bridgewater Treatise, III.) London: William Pickering.Google Scholar

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