Europa - The prospects for an oceanTidal dissipation in the satellites of a giant planet may provide sufficient heating to maintain a liquid water ocean below a thin ice layer. In the solar system, Europa, one of the Galilean satellites of Jupiter, may have such an ocean. Both theoretical calculations and certain observations support its existence, although proof is lacking. The putative ocean would probably have temperatures, pressures, and chemistry conducive to biologic activity. However, the environment would be severely energy limited. Possible energy sources include transient transmission of sunlight through fractures in the ice and hydrothermal activity on the ocean floor. While temporary conditions could exist that are within the range of adaptation of certain terrestrial organisms, origin of life under such conditions seems unlikely. In other solar systems, however, larger satellites with more significant heat flow could provide environments that are stable over an order of aeons and in which life could perhaps evolve.
Document ID
19880067977
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Reynolds, R. T. (NASA Ames Research Center Moffett Field, CA, United States)
Mckay, C. P. (NASA Ames Research Center Moffett Field, CA, United States)
Kasting, J. F. (NASA Ames Research Center Moffett Field, CA, United States)
Squires, S. W. (Cornell University Ithaca, NY, United States)