New theory sheds light on space enigmaFebruary 25, 2008An enormous plume of dust and water spurts violently into space from the south pole of Enceladus, Saturn's sixth-largest moon. This raging eruption has intrigued scientists ever since the Cassini spacecraft provided dramatic images of the phenomenon. Now, physicist Nikolai Brilliantov, at the University of Leicester, and colleagues in Germany, have revealed why the dust particles in the plume emerge more slowly than the water vapour escaping from the moon's icy crust. Enceladus orbits in Saturn's outermost "E" ring. It is one of only three outer solar system bodies that produce active eruptions of dust and water vapour. Moreover, aside from the Earth, Mars, and Jupiter's moon Europa, it is one of the only places in the solar system for which astronomers have direct evidence of the presence of water. The erupting plume on Enceladus is ejected by geyser-like volcanic eruptions from deep, "tiger-stripe" cracks within the moon's south pole. Some astronomers have suggested that the myriad tiny grains of dust from these eruptions could be the actual source of Saturn's E-ring. However, the dynamics and the origin of the plume itself have remained a mystery. Now, Brilliantov, who is also on the faculty at the University of Potsdam, Germany and Moscow State University, working with Juergen Schmidt and Frank Spahn of Potsdam and Sascha Kempf of the Max Planck Institute for Nuclear Physics in Heidelberg, and the Technical University of Braunschweig, Germany have developed a new theory to explain the formation of these dust particles and to explain why they are ejected into space. The researchers point out that once ejected the dust particles, which are in fact icy grains, and water vapour are too dilute to interact with each other and so the water vapour cannot be the cause of the dusty slowdown. Instead, the team suggests that the shift in speed must occur below the moon's surface before ejection. The numerous cracks through which the plume material escapes from the moon's icy surface, and which can be hundreds of metres deep, are narrower at some points along their length. At these points temperature and pressure of vapour drop drastically down, causing condensation of vapour into icy grains and hence to formation of the dust-vapour mixture. The required vapour density to accelerate the grains to the observed speeds implies temperatures where liquid water can exist in equilibrium with solid ice and water vapour within the moon's frozen crust. These peculiar conditions allow the water vapour to erupt rapidly carrying with it the dust particles. However, these particles undergo countless frequent collisions with the inside of the channel walls which causes friction that slows them down before final ejection. The larger the particle the slower the ejection speed. This effect, quantified by the new theory, explains the structure of the plume and eventually the particle size distribution of the E-ring of Saturn. The existence of liquid water is a prerequisite for life and, while not suggesting there is life on Enceladus, offers another extraterrestrial place that might be searched. University of Leicester |
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| Related Enceladus Current Events and Enceladus News Articles How the moon got its stripes A new study has revealed the origins of tiger stripes and a subsurface ocean on Enceladus- one of Saturn's many moons. These geological features are believed to be the result of the moon's unusual chemical composition and not a hot core, shedding light on the evolution of planets and guiding future space exploration. New cleaning protocol for future 'search for life' missions Scientists have developed a new cleaning protocol for space hardware, such as the scoops of Mars rovers, which could be used on future "Search for Life" missions on other planets. Four of Saturn's moons parade by their parent On 24 February 2009, the NASA/ESA Hubble Space Telescope captured a photo sequence of four moons of Saturn passing in front of their parent planet. NASA Scientists Find Clues to a Secret of Life NASA scientists analyzing the dust of meteorites have discovered new clues to a long-standing mystery about how life works on its most basic, molecular level. Montana State team finds Yellowstone alga that detoxifies arsenic Arsenic may be tough, but scientists have found a Yellowstone National Park alga that's tougher. Cassini flyby of Saturn moon offers insight into solar system history NASA's Cassini spacecraft is scheduled to fly within 16 miles of Saturn's moon Enceladus on Oct. 9 and measure molecules in its space environment that could give insight into the history of the solar system. Hot spot on Enceladus causes plumes Enceladus, the tiny satellite of Saturn, is colder than ice, but data gathered by the Cassini-Huygens Mission to Saturn and Titan has detected a hot spot that could mean there is life in the old moon after all. In fact, for researchers of the outer planets, Enceladus is so intellectually hot, it's smokin'. Frigid Enceladus: An unlikely harbor for life A new model of Saturn's icy moon Enceladus may quell hopes of finding life there. Developed by researchers at the University of Illinois, the model explains the most salient observations on Enceladus without requiring the presence of liquid water. Charon: An Ice Machine in the Ultimate Deep Freeze Frigid geysers spewing material up through cracks in the crust of Pluto's companion Charon and recoating parts of its surface in ice crystals could be making this distant world into the equivalent of an outer solar system ice machine. Life elsewhere in Solar System could be different from life as we know it The search for life elsewhere in the solar system and beyond should include efforts to detect what scientists sometimes refer to as "weird" life -- that is, life with an alternative biochemistry to that of life on Earth -- says a new report from the National Research Council. More Enceladus Current Events and Enceladus News Articles |
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