Using data provided by the Cassini-Huygens spacecraft scientists have pinpointed 101 geysers on Enceladus, one of Saturn’s icy moons. Issued in a press release by NASA, July 28th, 2014, the findings are helping scientists understand the geological processes that may allow for liquid water to exist on the moon’s surface.
The first geysers were spotted nearly ten years ago on the moon. Since then scientists have been able to resolve not only where they were being formed, but also how. Early hypothesis’ suggested that pressure built up by the flexing of the small moon’s surface was heating ice into vapor; once an enough tidal friction melted an opening on the surface, a geyser would erupt allowing the pressure to be released.
Using Cassini scientists were able to triangulate the locations of 101 fountains and have found the south pole of the moon to be a breeding ground for the geysers. Tiger stripe fractures run across the terrain of Enceladus in this area. Measurements taken over the last seven years have indicated that the geysers are erupting from hot spots along these striped fractures. This is a great clue for the scientists because it offers a possible origin for the water that spews from these vents.
Scientists have been able to correlate the intensity of the jets to thermal radiation as well as tidal stressors. It was apparent that higher temperatures were associated with the vents, however, it was unknown if increased temperatures were causing the geysers or vice versa. By analyzing high-resolution data gathered by Cassini’s heat-sensing technology in 2010 and 2012, the scientists could say definitively which came first, the chicken or the egg. In this case, it is the geysers that are causing the increased temperatures on the surface of Enceladus. Carolyn Porco, leader of the Cassini image team said in a report published in the Astronomical Journal, “[The results] told us the geysers are not a near-surface phenomenon, but have much deeper roots.”
Scientists now believe that the underground sea that resides on the moon is the most plausible source of these watery fountains. “They also found that narrow pathways through the ice shell can remain open from the sea all the way to the surface, if filled with liquid water.” Enceladus’ sea is believed to be nearly 10 kilometers deep, covered by 30-40 kilometers of ice near its south pole. It is still unclear why much of the moon’s water appears to be concentrated in this region. Porco had long suspected that Enceladus was releasing heat from within. Small silica particles have been spotted in the plumes, this combined with the newest evidence of deep channels connecting the moon’s surface with its underground sea gives scientists more hope of possibly finding life here.
In an article published in the journal Nature, in April, 2014, it states, “At the bottom of the Enceladus ocean, the water presumably comes in contact with the moon’s rocky core. “What matters about the new result is they say they have evidence for the ocean contacting rock,” says Christopher McKay, an astrobiologist at NASA’s Ames Research Center in Moffett Field, California. “That’s very important because pure water is not interesting biologically — the water needs to interact with rock in order to put in the stuff that’s useful for life.”
Hydrothermal vents on Earth act as transmitters of heat and chemicals from within the planet’s interior and they have been found to harbor the most extreme forms of life. Only further research will tell if similar underwater outlets are heating Enceladus, and whether or not biological life may be hiding there.