For the first time, images from NASA’s Cassini spacecraft have enabled scientists to
correlate the spraying of jets of water vapor from fissures on Saturn’s moon Enceladus with the way Saturn’s gravity stretches and stresses the fissures. As said Terry Hurford, a Cassini associate based at NASA Goddard Space Flight Center in Greenbelt, Md. this new work gives scientists insight into the mechanics of these picturesque jets at Enceladus and shows that Saturn really stresses Enceladus. Enceladus is unique in the Saturn system in having jets of water vapor and organic particles spray from long fissures in its south polar region. The long fissures have been nicknamed the tiger stripes. Hurford and colleagues suggested a few years ago that tidal pulls from Saturn’s gravity could explain the existence of the jets, but they had not been able to correlate specific jets with calculated stresses until now. They studied the jets emerging from the warmest regions within the tiger stripes Baghdad Sulcus and Damascus Sulcus. The scientists found that the greatest stresses pulling apart the tiger stripes, occurred right after Enceladus made its closest approach to Saturn in its orbit. The scientists found that Saturn’s gravitational pull could also deform the fissure by making one side move relative to the other side. That kind of deformation seemed to occur quite often during Enceladus’ orbit around the planet, even when Enceladus was very far away. The finding suggests that a large reservoir of liquid water would be necessary to allow Enceladus to flex enough to generate stresses great enough to deform the surface. That process would control the timing of the jet eruptions. The finding also suggests that Saturn’s tides create an enormous amount of heat in the area.