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7 September 2010 The Drake Equation in an astrobiological context
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Abstract
The Drake Equation was originally composed as an attempt to quantify the potential number of extraterrestrial civilizations in our Galaxy which we might be able to detect using a radio telescope. Since this equation was first formulated, nearly 50 years ago, we have discovered that life on Earth arose very early in its history, and has filled virtually every habitable, potentially extreme, niche available. This suggests that simple forms of life might be plentiful where possible, and can be observed remotely by atmospheric biosignatures in the host planet. We consider modifications to the Drake Equation to reflect this new understanding.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gregory A. Konesky "The Drake Equation in an astrobiological context", Proc. SPIE 7819, Instruments, Methods, and Missions for Astrobiology XIII, 781916 (7 September 2010); https://doi.org/10.1117/12.860757
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KEYWORDS
Planets

Exoplanets

Radio telescopes

Oxygen

Stars

Earth's atmosphere

Atmospheric sensing

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