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Reassessing the Possibility of Life on Venus: Proposal for an Astrobiology Mission

To cite this article:
Dirk Schulze-Makuch and Louis N. Irwin. Astrobiology. July 2004, 2(2): 197-202. doi:10.1089/15311070260192264.

Published in Volume: 2 Issue 2: July 5, 2004

Author information

Dirk Schulze-Makuch
Department of Geological Sciences, University of Texas at El Paso, El Paso, TX
Louis N. Irwin
Department of Biological Sciences, University of Texas at El Paso, El Paso, TX

ABSTRACT

With their similar size, chemical composition, and distance from the Sun, Venus and Earth may have shared a similar early history. Though surface conditions on Venus are now too extreme for life as we know it, it likely had abundant water and favorable conditions for life when the Sun was fainter early in the Solar System. Given the persistence of life under stabilizing selection in static environments, it is possible that life could exist in restricted environmental niches, where it may have retreated after conditions on the surface became untenable. High-pressure subsurface habitats with water in the supercritical liquid state could be a potential refugium, as could be the zone of dense cloud cover where thermoacidophilic life might have retreated. Technology based on the Stardust Mission to collect comet particles could readily be adapted for a pass through the appropriate cloud layer for sample collection and return to Earth.

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