News / Space News |
Icy Tendrils Reaching into Saturn Ring Traced to Their Source
NASA | APRIL 16, 2015
Long, sinuous, tendril-like structures seen in the vicinity of Saturn's icy moon Enceladus originate directly from geysers erupting from its surface, according to scientists studying images from NASA's Cassini spacecraft.
Each unique tendril structure can be reproduced by particular sets of geysers on the moon's surface. The geysers, which were discovered by Cassini in 2005, are jets of tiny water ice particles, water vapor and simple organic compounds.
Under certain lighting conditions, Cassini's wide-view images showing icy material erupting from Enceladus reveal faint, finger-like features, dubbed "tendrils" by the imaging team. The tendrils reach into Saturn's E ring -- the ring in which Enceladus orbits -- extending tens of thousands of miles (or kilometers) away from the moon.
The tendrils are composed of particles with diameters no smaller than about a hundred thousandth of an inch, a size consistent with the measurements of E-ring particles. They give a way to ascertain how much mass is leaving Enceladus and making its way into Saturn orbit. another important step is to determine how much mass is involved, and thus estimate how much longer the moon's sub-surface ocean may last.