Jupiter's icy moon Europa is a major target of astrobiology research as it offers a possible habitable environment. Under its 10 km-thick icy crust is an ocean of liquid water over 100 km deep. Energy deriving from the moon's gravitational interaction with Jupiter keeps this ocean warm.
Theoretical research to evaluate the microbial habitability of Europa using data collected from analogous environments on Earth has been conducted by a group of Brazilian researchers linked to the University of São Paulo (USP). They've published their report in Scientific Reports.
"We studied the possible effects of a biologically usable energy source on Europa based on information obtained from an analogous environment on Earth," said Douglas Galante, a researcher at Brazil's National Synchrotron Light Laboratory (LNLS) and the Astrobiology Research Center (NAP-Astrobio) of the University of São Paulo's Institute of Astronomy, Geophysics & Atmospheric Sciences (IAG-USP).
Galante coordinates the study, which aims at investigating places in Brazil and Africa with possible vestiges of geochemical and isotopical transformations related to the emergence of multicelular life in Neoproterozoic Age.
In the Mponeng gold mine near Johannesburg, South Africa, at a depth of 2.8 km, the researchers found traces of major changes linked to the history of life on Earth, and a terrestrial context analogous to Europa. They discovered that the bacterium Candidatus desulforudis audaxviator survives inside the mine without sunlight by means of water radiolysis, the dissociation of water molecules by ionizing radiation.
"This very deep subterranean mine has water leaking through cracks that contain radioactive uranium," Galante said. "The uranium breaks down the water molecules to produce free radicals (H+, OH-, and others), which attack the surrounding rocks, especially pyrite (iron disulfide, FeS2), producing sulfate. The bacteria use the sulfate to synthesize ATP [adenosine triphosphate], the nucleotide responsible for energy storage in cells. This is the first time an ecosystem has been found to survive directly on the basis of nuclear energy."
According to Galante and colleagues, the environment colonized by bacteria in the Mponeng mine is an excellent analogue of the environment assumed to exist at the bottom of Europa's ocean.
Although the temperature in Europa's surface is next to absolute zero, there is an enormous amount of thermal energy in its core, as an effect of Europa's interaction with Jupiter's powerful gravity, which causes the satellite's orbit to be extremely elliptical. Thus, Europa orbits either extremely close or quite far from the gas giant. The moon experiences geometrical deformation as a result of Jupiter's immense tidal force. The energy released by the alternating states of elongation and relaxation makes Europa's subsurface capable of hosting an ocean of liquid water.
"However, it's not enough for there to be heated liquid water," said Galante. According to the researcher, biological activity is based on differences in the concentrations of molecules, ions or electrons in distinct regions that produce a flow in a certain direction, allowing the occurrence of cellular respiration, photosynthesis, ATP production and other processes common to living beings.
"Hydrothermal emanations—of molecular hydrogen [H2], hydrogen sulfide [H2S], sulfuric acid [H2SO4], methane [CH4] and so on—are important sources of chemical imbalance and potential factors of biological transduction, i.e., transformation of the imbalance into biologically useful energy," Galante said. "These hydrothermal sources are the most plausible scenario for the origin of life on Earth."
Investigating conditions in Europa for ATP production
The group evaluated how chemical imbalances in Europa could be initiated through the emanation of water leading to chain reactions between water and chemical elements found in Europa's crust—however, there is a total lack of supporting empirical data. "That's why we looked for a more universal physical effect that was highly likely to occur. That effect was the action of radioactivity," Galante said.
Celestial bodies in the solar system with rocky cores share the same radioactive materials, ejected into space by supernova explosions that originated the sun and the planets. The researchers considered the concentrations of uranium, thorium and potassium on Europa based on the quantities already observed and measured on Earth, in meteorites and on Mars.
"From these amounts, we were able to estimate the energy released, how this energy interacts with the surrounding water, and the efficiency of the water radiolysis resulting from this interaction in generating free radicals," Galante said.
According to the study, along with radionuclides, pyrite is a crucial ingredient whose presence is indispensable for life in Europa. "One of the proposals deriving from our study is that traces of pyrite should be looked for as part of any assessment of the habitability of a celestial body," said Galante. Chances for finding pyrite in a hypothetical mission to Europa are good, since sulfur (S) and iron (Fe) are elements found in abundance across the solar system.
"The ocean bed on Europa appears to offer very similar conditions to those that existed on primitive Earth during its first billion years. So studying Europa today is to some extent like looking back at our own planet in the past. In addition to the intrinsic interest of Europa's habitability and the existence of biological activity there, the study is also a gateway to understanding the origin and evolution of life in the universe."
More information: Thiago Altair et al, Microbial habitability of Europa sustained by radioactive sources, Scientific Reports (2018). DOI: 10.1038/s41598-017-18470-z
Journal reference: Scientific Reports
Provided by: FAPESP