Water plumes erupting from the `tiger stripe’ features on the south pole of Enceladus are thought to connect to a global subsurface ocean. Proposed origins for the initial stress necessary […]
Enceladus
New Models Reveal The Inner Complexity Of Enceladus
A Southwest Research Institute team developed a new geochemical model that reveals that carbon dioxide (CO2) from within Enceladus, an ocean-harboring moon of Saturn, may be controlled by chemical reactions […]
Spontaneous Formation of Geysers At Only One Pole On Enceladus' Ice Shell
The ice shell on Enceladus, an icy moon of Saturn, exhibits strong asymmetry between the northern and southern hemispheres, with all geysers compacted over the south pole, even though the […]
How Saturn's Moon Enceladus Got Its Stripes
Saturn’s icy moon Enceladus is of great interest to scientists due to its subsurface ocean, making it a prime target for those searching for life elsewhere. New research led by […]
New Organic Compounds Found in Enceladus Ice Grains
New kinds of organic compounds, the ingredients of amino acids, have been detected in the plumes bursting from Saturn’s moon Enceladus. The findings are the result of the ongoing deep […]
'Snow-Cannon' Enceladus Shines Up Saturn's Super-Reflective Moons
Radar observations of Saturn’s moons, Mimas, Enceladus and Tethys, show that Enceladus is acting as a ‘snow-cannon,’ coating itself and its neighbours with fresh water-ice particles to make them dazzlingly […]
Enceladus and Titan: Emerging Worlds of the Solar System (ESA Voyage 2050 White Paper)
Some of the major discoveries of the recent Cassini-Huygens mission have put Titan and Enceladus firmly on the Solar System map. The mission has revolutionised our view of Solar System […]
Abundance of Gases in Enceladus's Ocean Are A Potential Fuel For Life
The subsurface ocean of Saturn’s moon Enceladus probably has higher than previously known concentrations of carbon dioxide and hydrogen and a more Earthlike pH level, possibly providing conditions favorable to […]
Enceladus's Crust As A Non-uniform Thin Shell: II Tidal Dissipation
Tidal heating is the prime suspect behind Enceladus’s south polar heating anomaly and global subsurface ocean. No model of internal tidal dissipation, however, can explain at the same time the […]
Evidence of Complex Organic Molecules In Plumes From Enceladus
Using mass spectrometry data from NASA’s Cassini spacecraft, scientists found that large, carbon-rich organic molecules are ejected from cracks in the icy surface of Saturn’s moon Enceladus. Southwest Research Institute […]
