Saturn’s moon Enceladus has been a subject of scientific intrigue due to its massive water plumes, which were initially believed to be linked to an underground ocean beneath its icy crust. The idea that this ocean could sustain microbial life made it a prime target for astrobiological studies. However, new research suggests that the source of these geysers may not be the deep subsurface ocean, but rather a mushy layer within the ice shell itself. This finding challenges previous assumptions about the habitability of Enceladus and raises new questions about the mechanisms behind the moon’s plumes.
New Theory on Enceladus’ Geysers
According to a study published in Geophysical Research Letters, researchers from Dartmouth College propose that the plumes erupting from Enceladus may not require fractures that extend entirely through the ice shell to the underground ocean. Instead, they suggest that a slushy, salt-laden layer within the ice could act as the source of the water vapor and ice particles seen in the plumes. This theory is based on the observation that the moon’s icy surface contains salts, which lower the melting point of ice, allowing it to form a semi-liquid state in certain regions.
Shear Heating and Fractures in the Ice
Scientists have pointed to “tiger stripe” fractures in the moon’s southern hemisphere as key locations where these eruptions occur. The study suggests that friction between ice layers, known as shear heating, could generate enough warmth to maintain a slushy state within the ice shell. This would create a reservoir of briny water close to the surface, supplying the plumes without requiring a direct connection to the deep ocean.
Gases and Plume Composition
As per the reports, the composition of the plumes observed by NASA’s Cassini spacecraft could be explained by the melting of gas-rich ice structures called clathrates. These formations trap molecular hydrogen, carbon dioxide, and methane within the ice. Partial melting of these structures could release hydrogen while retaining other gases, potentially accounting for the chemical composition detected in the plumes.
Future Investigations
While this study provides an alternative explanation for Enceladus’ geysers, further research is required to determine how the slushy zone replenishes itself over time. Scientists continue to analyse Cassini’s data to refine their understanding of the processes shaping the moon’s icy surface and its potential for sustaining life.
