News on Jupiter
- First detailed mapping of Jovian-moon Io
- NASA and European amateur astronomers spy on Jupiter
- Vulcanism causes changes in Jupiters aurora
- Evidence for subsurface 'Great Lake' on Europa
- Giant planet ejected from the solar system
- Jupiter on the move
- Io subsurface molten ocean
- Ripples in planetary rings caused by comet-impacts
- A revisit with Jupiters lost belt
- Jupiter hit by asteroid, not comet
- Jupiters lost cloud-belt is re-appearing
- Quantum simulations uncover hydrogen’s phase transitions in gas planets
- Jupiter impact: Mystery of the missing debris
- The atmosphere of Io
- Asteroid impact on Jupiter
- Jupiters southern belt has disappeared
- Juno space probe taking shape
- Helium rain on Jupiter blocks Neon
- Jupiters spot is glowing
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The atmosphere of Io
Tuesday, 15 June 2010 15:24
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| Solar system - Jupiter |
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Io is one of the four moons of Jupiter that Galileo discovered after he turned his new telescope heavenward. They shocked him and his contemporaries because they demonstrated that heavenly bodies can orbit objects other than the earth. Io in particular continues to amaze scientists. It orbits closer to the cloud tops of Jupiter than our moon does to the earth, and is strongly subjected to Jupiter's powerful gravitational field and its intense radiation belts. One consequence is that Io is the most volcanic object known anywhere, with lava flows, erupting with plumes of sulfurous material, and a changing atmosphere of noxious gases. The 1979 Voyager flyby observations revealed many of these details, but many puzzles remain. It is estimated, for example, that one ton of material needs to be ejected into Io's atmosphere every second in order to replenish the gases that escape from its atmosphere, but it is not known whether it all comes from volcanic gas or perhaps from the evaporation of surface ices. CfA astronomers Arielle Moullet and Mark Gurwell, together with two colleagues, used the Submillimeter Array to image the surface of Io in key diagnostic lines of sulfur dioxide and, for the first time, in sulfur monoxide and sodium chloride. They write in the latest issue of the journal Icarus that these three species of gases appear to be concentrated on the anti-jovian side of Io, although with different spatial distributions. The scientists conclude that ice sublimation is most probably the origin of the sulfur dioxide, while the sulfur monoxide may in turn be a product of the sulfur dioxide interacting with radiation. The sodium chloride, on the other hand, most likely comes from volcanoes. The group also derives temperature and density information for the gas. The new results help to sort out competing models of this bizarre satellite, and highlight the disruptive role that volcanoes can play in other solar system bodies besides the earth. Source: Harvard Univsersity |




A new studyof the Jupitermoon Io with radiotelescopes from Earth, reveals new information on the origin of Io's atmosphere