Energy for biologic sulfate reduction in a hydrothermally formed ocean on Europa
نویسندگان
چکیده
[1] Formation of a sulfate-bearing ocean on Jupiter’s satellite Europa by quenched hydrothermal fluids provides a source of metabolic energy for low-temperature sulfatereducing organisms that use dissolved H2 as an electron donor. Inhibition of thermodynamically favorable sulfate reduction in cooled hydrothermal fluids creates the potential for biologic reduction. Both high temperature and reduced conditions of oceanforming hydrothermal solutions favor sulfate reduction in quenched fluids. The maximum amount of energy available to support autotrophic sulfate reduction is on the order of a few kilojoules per kilogram of water and is limited by the low abundances of either H2 or sulfate in ocean-forming fluids. Although this irreplaceable energy source might have supported early life on Europa, maintenance of biologic sulfate reduction throughout the ocean’s history would require a supply of organic compounds from endogenic sources or from the satellite’s surface.
منابع مشابه
A model for low-temperature biogeochemistry of sulfur, carbon, and iron on Europa
[1] Galileo spacecraft data obtained from Jupiter’s ice-covered satellite Europa suggest the existence of a subsurface water ocean. The formation of this ocean is a direct consequence of early igneous and hydrothermal processes that may have facilitated oxidation through H2 and CH4 escape. These processes could have led to a moderately alkaline sulfate-carbonate ocean and a moderately oxidized ...
متن کاملSulfate content of Europa's ocean and shell: evolutionary considerations and some geological and astrobiological implications.
Recent models for the origin of Jupiter indicate that the Galilean satellites were mostly derived from largely unprocessed solar nebula solids and planetesimals. In the jovian subnebula the solids that built Europa were first heated and then cooled, but the major effect was most likely partial or total devolatilization, and less likely to have been wholesale thermochemical reprocessing of rock ...
متن کاملEnergy, chemical disequilibrium, and geological constraints on Europa.
Europa is a prime target for astrobiology. The presence of a global subsurface liquid water ocean and a composition likely to contain a suite of biogenic elements make it a compelling world in the search for a second origin of life. Critical to these factors, however, may be the availability of energy for biological processes on Europa. We have examined the production and availability of oxidan...
متن کاملChemistry of a Primordial Ocean on Europa
Introduction: Jupiter’s moon Europa is a differentiated body that consists of a Fe-rich core, a silicate mantle, and a water shell, which could contain an ocean [1]. The presence of sulfate-bearing compounds on the moon’s icy surface has been interpreted in terms of frozen oceanic water [2]. However, evaluations of oceanic chemistry from surface observations are limited because of radiolysis [3...
متن کاملSalts and Radiation Products on the Surface of Europa
The surface of Europa could contain the compositional imprint of a underlying interior ocean, but competing hypotheses differ over whether spectral observations from the Galileo spacecraft show the signature of ocean evaporates or simply surface radiation products unrelated to the interior. Using adaptive optics at the W.M. Keck Observatory, we have obtained spatially resolved spectra of most o...
متن کامل