Enceladus tagged posts

An Ocean Lies a few kilometers beneath Saturn’s Moon Enceladus’s Icy Surface

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

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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Cassini Captures Group Photo of Tethys, Enceladus, Mimas

Image: Cassini captures group photo of Tethys, Enceladus and Mimas

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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Saturn and Enceladus produce the same amount of Plasma

Saturn

A false-color composite image, constructed from data obtained by NASA’s Cassini spacecraft showing the glow the aurora about 1,000 km above the cloud tops of Saturn’s south pole (credit NASA/JPL/University of Arizona/ University of Leicester)

The evidence that Saturn’s upper atmosphere may, when buffeted by the solar wind, emit the same total amount of mass per second into its magnetosphere as its moon, Enceladus, has been found by UCL scientists working on the Cassini mission. Magnetospheres are regions of space that are heavily influenced by the magnetic field of a nearby planet and can contain charged particles in the form of plasma from both external and internal sources.

In the case of Saturn, its moon Enceladus ejects water from its icy plumes which is ionised into H2O+, O+, OH+ ...

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