Impact constraints on the environment for chemical evolution and the continuity of life.
The Moon and the Earth were bombarded heavily by planetesimals and asteroids that were capable of interfering with chemical evolution and the origin of life.  In this paper, we explore the frequency of giant terrestrial impacts able to stop prebiotic chemistry in the probable regions of chemical evolution.  The limited time available between impacts disruptive to prebiotic chemistry at the time of the oldest evidence of life suggests the need for a rapid process for chemical evolution of life.  The classical hypothesis for the origin of life through the slow accumulation of prebiotic reactants in the primordial soup in the entire ocean may not be consistent with constraints imposed by the impact history of Earth.  On the other hand, rapid chemical evolution in cloud systems and lakes or other  shallow evaporating water bodies would have been possible because reactants could have been concentrated and polymerized rapidly in this environment.  Thus, life probably could have originated near the surface between frequent surface sterilizing impacts.  There may not have been continuity of life depending on sunlight because there is evidence that life, existing as early as 3.8 Gyr ago, may have been destroyed by giant impacts.  The first such organisms on Earth were probably not the ancestors of present life.
Oberbeck
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VR
NASA Ames Research Center, Moffett Field, CA 94035, USA.
Fogleman
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G
D018534:Earth, Planet; D019418:Evolution, Chemical; D018535:Mars; D018543:Minor Planets; D015233:Models, Statistical; D016081:Moon; D000069497:Origin of Life; D011336:Probability