title: The origin and emergence of life under impact bombardment.
abstract: Craters formed by asteroids and comets offer a number of possibilities as sites for prebiotic chemistry, and they invite a literal application of Darwin's 'warm little pond'. Some of these attributes, such as prolonged circulation of heated water, are found in deep-ocean hydrothermal vent systems, previously proposed as sites for prebiotic chemistry. However, impact craters host important characteristics in a single location, which include the formation of diverse metal sulphides, clays and zeolites as secondary hydrothermal minerals (which can act as templates or catalysts for prebiotic syntheses), fracturing of rock during impact (creating a large surface area for reactions), the delivery of iron in the case of the impact of iron-containing meteorites (which might itself act as a substrate for prebiotic reactions), diverse impact energies resulting in different rates of hydrothermal cooling and thus organic syntheses, and the indiscriminate nature of impacts into every available lithology-generating large numbers of 'experiments' in the origin of life. Following the evolution of life, craters provide cryptoendolithic and chasmoendolithic habitats, particularly in non-sedimentary lithologies, where limited pore space would otherwise restrict colonization. In impact melt sheets, shattered, mixed rocks ultimately provided diverse geochemical gradients, which in present-day craters support the growth of microbial communities.
authors.affiliation: Centre for Earth, Planetary, Space and Astronomical Research, Open University, Milton Keynes MK7 6AA, UK. c.s.cockell@open.ac.uk
authors.forename: Charles S
authors.initials: CS
authors.lastname: Cockell
mesh_terms: D005075:Biological Evolution; D018534:Earth, Planet; D004777:Environment; D049690:History, Ancient; D019110:Meteoroids; D018543:Minor Planets; D000069497:Origin of Life