 
 
 
 
 A tiny moon 
  of Saturn, no larger than England, is changing researchers notions about 
  which celestial bodies can support geologic activity. New, closer images of 
  Enceladus have confirmed that a plume, noticed in previous images, is indeed 
  an enormous geyser emanating from visible cracks in the moons surface.
A tiny moon 
  of Saturn, no larger than England, is changing researchers notions about 
  which celestial bodies can support geologic activity. New, closer images of 
  Enceladus have confirmed that a plume, noticed in previous images, is indeed 
  an enormous geyser emanating from visible cracks in the moons surface. 
  
In this color-enhanced image, an enormous 
  plume emanating from fractures on Saturns moon Enceladus appears backlit 
  by the sun. Astronomers were surprised to find geologic activity on the small 
  moon, which is seven times smaller than Earths moon. Image courtesy of 
  NASA/JPL/Space Science Institute. 
  
  NASAs Cassini spacecraft first revealed the plume-like feature in images 
  taken in January and February last year. But according to Carolyn Porco, Cassini 
  imaging team leader at the Space Science Institute in Boulder, Colo., speculation 
  remained that the feature was an artifact of the camera. Following a special 
  Cassini mission in November to take a closer look, however, the images confirmed 
  it without question, Porco says. 
  
  The moon and its plume look similar to a comet and its tail, which forms from 
  vapor created when sunlight warms the icy body. Enceladus, however, does not 
  receive much sunlight. Instead, pressurized vapor on Enceladus emanates from 
  below the surface and shoots out like a jet through vents the team 
  calls tiger stripes, Porco says. She describes the vapors composition 
  of small icy particles to be like the finest powder you might ski on in 
  Utah. The cause of the pressurized geyser, Porco says, is due to an internal 
  source of heat on the moon, either from flexing tides or from radioactive material. 
  
  
  Small bodies such as Earths moon, which is 3,476 kilometers in diameter, 
  typically lose their internal heat shortly after formation, rendering them geologically 
  dead. Porco says that even though she was not surprised to find geologic activity 
  on Enceladus, she finds it thrilling to see geologic activity on 
  another body  especially a moon only 480 kilometers in diameter, with 
  a geyser as tall as the moon is wide. Finding activity on such a small body, 
  Porco says, has torqued our ideas around about how geologic activity can 
  come about. 
Kathryn Hansen
  
 
 
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