Cassini tagged posts

Geysers on Saturn’s icy moon Enceladus may form from a ‘mushy zone’

Geysers on Saturn's icy moon Enceladus may form from a 'mushy zone'
Saturn’s moon Enceladus captured by the Cassini spacecraft’s orbit in 2008. Credit: NASA/JPL/Space Science Institute.

Searching for life on other celestial bodies, or at the very least the necessary components to support it, has been fascinating scientists and enthusiasts for centuries. While planets are the obvious choice, their moons can also harbor the chemical ingredients for life.

Saturn is orbited by 146 moons, with Enceladus being the sixth largest at approximately 500km in diameter. This small, icy moon is characterized by its highly reflective white surface and geyser-like jets releasing ice and water vapor hundreds of kilometers into space from its south pole.

NASA’s Cassini spacecraft identified these jets in 2005, before going on to sample them in 2008, 2009 and 2015...

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Webb Telescope finds Towering Plume of Water escaping from one of Saturn’s Moons

Courtesy of NASA/ESA/CSA/Alyssa Pagan (STScI)/Geronimo Villanueva (NASA-GSFC) SwRI contributed to new Cycle 1 JWST findings that show the plume of water escaping from Saturn’s moon Enceladus extends 6,000 miles or more than 40 times the moon’s size. In light of this discovery, SwRI’s Dr. Christopher Glein was awarded a NASA JWST Cycle 2 allocation to study the plume as well as the icy surface of Enceladus, to better understand the potential habitability of this ocean world.

Two Southwest Research Institute scientists were part of a James Webb Space Telescope (JWST) team that observed a towering plume of water vapor more than 6,000 miles long—roughly the distance from the U.S. to Japan—spewing from the surface of Saturn’s moon, Enceladus...

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Theoretical Model suggests Saltiness of Enceladus’s Oceans may be right to Sustain Life

Considered heat sources/sinks and salinity/temperature forcings in our Enceladus experiments

A team of researchers at MIT has found via theoretical modeling that the saltiness of the oceans on Saturn’s moon, Enceladus, may be the right level to sustain life. In their paper published in the journal Science Advances, the group describes the factors that went into building their model and the features of Enceladus that were used to measure the saltiness of its oceans.

The combined data from the Cassini and Galileo missions showed that Saturn’s moon Enceladus and Jupiter’s moon Europa both hold potential for satisfying three of the main features believed to be necessary for supporting life on other celestial bodies: they have a source of energy, they have liquid water and they have a mi...

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Possible Detection of Hydrazine on Saturn’s moon Rhea

Possible detection of hydrazine on Saturn’s moon Rhea
Cassini grand finale. Credit: The European Space Agency

In a new report on Science Advances, Mark Elowitz, and a team of scientists in physical sciences, optical physics, planetary science and radiation research in the U.S., U.K., India, and Taiwan, presented the first analysis of far-ultraviolet reflectance spectra of regions on Rhea’s leading and trailing hemispheres—as collected by the Cassini ultraviolet imaging spectrograph during targeted flybys. In this work, they specifically aimed to explain the unidentified broad absorption feature centered near 184 nanometers of the resulting spectra. Using laboratory measurements of the UV spectroscopy of a set of molecules, Elowitz et al...

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