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Optical Lasers for CETI

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Bioastronomy — The Next Steps

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 144))

Abstract

Present research supporting SETI and CETI is entirely focused upon microwave wavelengths and technologies. This paper demonstrates that there are compelling reasons why the search should be broadened to optical wavelengths. New perceptions regarding the feasibility of optical laser technologies, together with reassessments of signal-to-noise considerations, indicate both the feasibility and desirability of interstellar transmissions at infrared, visible, and ultraviolet wavelengths. Implicit in the rationale for SETI/CETI is the question of ultimate motivations. It is shown that use of the large bandwidths available at optical wavelengths greatly enhances the utility of such endeavors. Present astronomical equipment and methods are adequate for the initial detection, although specially constructed receiving equipment would be required for full decoding of the signals.

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References

  1. R.N. Schwartz and C.H. Townes, “Interstellar and Interplanetary Communication by Optical Lasers”, Natur., 190,. 205, (1961).

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  3. B.M. Oliver, “The Rationale for the Waterhole”. Technical Memorandum, Hewlett Packard Corp., Palo Alto CA. (1976).

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  4. B.M. Oliver, “Linear Amplification vs. Photon Detection In the Search for Interstellar Signals”, Technical Memorandum, Hewlett Packard Corp., Palo Alto, CA. (1976).

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© 1988 Kluwer Academic Publishers

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Rather, J.D.G. (1988). Optical Lasers for CETI. In: Marx, G. (eds) Bioastronomy — The Next Steps. Astrophysics and Space Science Library, vol 144. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2959-3_57

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  • DOI: https://doi.org/10.1007/978-94-009-2959-3_57

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-7830-6

  • Online ISBN: 978-94-009-2959-3

  • eBook Packages: Springer Book Archive

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