
NASA image of Enceladus within the E-ring in orbit around Saturn, where it is possible that the methanol detection could originate further out in the E-ring. Credit: NASA / JPL-Caltech / Space Science Institute. Click for a larger image


NASA image of Enceladus within the E-ring in orbit around Saturn, where it is possible that the methanol detection could originate further out in the E-ring. Credit: NASA / JPL-Caltech / Space Science Institute. Click for a larger image

This graphic illustrates how Cassini scientists think water interacts with rock at the bottom of the ocean of Saturn’s icy moon Enceladus, producing hydrogen gas. Credit: NASA/JPL-Caltech/Southwest Research Institute
Two veteran NASA missions are providing new details about icy, ocean-bearing moons of Jupiter and Saturn, further heightening the scientific interest of these and other “ocean worlds” in our solar system and beyond. Cassini scientists announce that a form of chemical energy that life can feed on appears to exist on Saturn’s moon Enceladus, and Hubble reports additional evidence of plumes erupting from Jupiter’s moon Europa.
“This is the closest we’ve come, so far, to identifying a place with some of the ingredients needed for a habitable environment,” said Thomas Zurbuchen, as...
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Image showing the thickness of Enceladus’s ice shell, which reaches 35 kilometers in the cratered equatorial regions (shown in yellow) and less than 5 kilometers in the active south polar region (shown in blue). Credit: © LPG-CNRS-U. Nantes/U. Charles, Prague
With eruptions of ice and water vapor, and an ocean covered by an ice shell, Saturn’s moon Enceladus is one of the most fascinating in the Solar System, especially as interpretations of data provided by the Cassini spacecraft have been contradictory until now. An international team recently proposed a new model that reconciles different data sets and shows that the ice shell at Enceladus’s south pole may be only a few kilometers thick...
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Three of Saturn’s moons, Tethys, Enceladus and Mimas, taken in visible light with the Cassini spacecraft narrow-angle camera on December 3, 2015 is shown in this NASA image released on February 22, 2016. © NASA / JPL-Caltech / Space Science Institute / Reuters
Tethys (660 miles or 1,062 kilometers across) appears above the rings, while Enceladus (313 miles or 504 kilometers across) sits just below center. Mimas (246 miles or 396 kilometers across) hangs below and to the left of Enceladus. This view looks toward the sunlit side of the rings from about 0.4 degrees above the ring plane. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on Dec. 3, 2015.
The view was acquired at a distance of ~837,000 miles from Enceladus, with an image scale of 5 miles per ...
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