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Is Titan a saturnian Europa/Ganymede?
Just watched the Cassini Team news briefing today, Friday 2. of July.
They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim |
#2
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Is Titan a saturnian Europa/Ganymede?
Just to be more clear, I of course know the theories and hopes that Titan
may have liquid oceans of ethane/methane (that are liquid even at the low temperatures at this distance). But gravitational heating might come up with a somewhat different story, as well... Bjørn Sørheim "Bjørn Sørheim" skrev i melding ... Just watched the Cassini Team news briefing today, Friday 2. of July. They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim |
#3
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Is Titan a saturnian Europa/Ganymede?
Just to be more clear, I of course know the theories and hopes that Titan
may have liquid oceans of ethane/methane (that are liquid even at the low temperatures at this distance). But gravitational heating might come up with a somewhat different story, as well... Bjørn Sørheim "Bjørn Sørheim" skrev i melding ... Just watched the Cassini Team news briefing today, Friday 2. of July. They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim |
#4
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Is Titan a saturnian Europa/Ganymede?
Bjørn Sørheim wrote:
Just watched the Cassini Team news briefing today, Friday 2. of July. They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. Of course, if life were doing it, it would be so much more interesting! Jack |
#5
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Is Titan a saturnian Europa/Ganymede?
Bjørn Sørheim wrote:
Just watched the Cassini Team news briefing today, Friday 2. of July. They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. Of course, if life were doing it, it would be so much more interesting! Jack |
#6
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Is Titan a saturnian Europa/Ganymede?
Jack wrote:
Bjørn Sørheim wrote: It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. I wouldn't think it likely. Titan's orbit is nearly a circle (e=0.03) and is not in resonant relationship to anything except a moon Hyperion which is about 1/1000th of Titan's mass. Got this off of http://www.nineplanets.org/data.html So it would seem that Titan doesn't see much gravitational variation as it orbits Saturn. And the Sun is way too far away to make any variation of significance. |
#7
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Is Titan a saturnian Europa/Ganymede?
Jack wrote:
Bjørn Sørheim wrote: It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. I wouldn't think it likely. Titan's orbit is nearly a circle (e=0.03) and is not in resonant relationship to anything except a moon Hyperion which is about 1/1000th of Titan's mass. Got this off of http://www.nineplanets.org/data.html So it would seem that Titan doesn't see much gravitational variation as it orbits Saturn. And the Sun is way too far away to make any variation of significance. |
#8
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Is Titan a saturnian Europa/Ganymede?
"Jack" wrote in message news:B1oFc.15098$%_6.2360@attbi_s01... Bjørn Sørheim wrote: Just watched the Cassini Team news briefing today, Friday 2. of July. They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. Of course, if life were doing it, it would be so much more interesting! Jack I don't know much about bio-chemistry or life sciences, but I think there is ammonia based life on Titan... (This of course has nothing to do with the fact that I have just finished reading Stephen Baxter's fine sci-fi novel "Titan". : ) |
#9
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Is Titan a saturnian Europa/Ganymede?
"Jack" wrote in message news:B1oFc.15098$%_6.2360@attbi_s01... Bjørn Sørheim wrote: Just watched the Cassini Team news briefing today, Friday 2. of July. They gave out the information that in the best images sofar they had of Titan - better very soon coming up - that there is visible linear crisscrossing features at some parts of Titan, and called them tectonic linear features... It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Of course it might be possible that the ice is the frozen result of not water, but a mix of several ingredients, I don't know much different liquids might seperate at this temperature and environment or not. Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? Bjørn Sørheim I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. Of course, if life were doing it, it would be so much more interesting! Jack I don't know much about bio-chemistry or life sciences, but I think there is ammonia based life on Titan... (This of course has nothing to do with the fact that I have just finished reading Stephen Baxter's fine sci-fi novel "Titan". : ) |
#10
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Is Titan a saturnian Europa/Ganymede?
Robert Casey wrote:
Jack wrote: Bjørn Sørheim wrote: It occurred to me that if crisscrossing linear features are seen, they might be linear cracks of an ice-covered body, just like the two (or three) of thr galilean moons of Jupiter. We haven't heard much about water ice on Titan in its history of exploration, but then Titan has a thick atmosphere (1.5 of the earth's). Is it possible that Titan to a not neglectable degree experiences gravitational heating just like Io, Europa, Ganymede (and Callisto) of Jupiter that warms up its interior to make water and other compounds liquid under a thick ice cover? I think it may be more like Io. There is plenty of methane in the atmosphere, and that is a non-equilibrium condition (like oxygen in our atomosphere). Something must be pumping methane into the atmosphere, and assuming it's not life, then it could be due to tidal squeezing of the planet which forces frozen methane out of the planet and into the atmosphere, like sulfur is forced out of Io. I wouldn't think it likely. Titan's orbit is nearly a circle (e=0.03) and is not in resonant relationship to anything except a moon Hyperion which is about 1/1000th of Titan's mass. Got this off of http://www.nineplanets.org/data.html So it would seem that Titan doesn't see much gravitational variation as it orbits Saturn. And the Sun is way too far away to make any variation of significance. Well, there is a bright plume of methane viewed by Cassini in the southern hemisphe http://saturn.jpl.nasa.gov/cgi-bin/g...jpg&type=image so there is *something* releasing methane into the air. My guess would be some kind of volcano that spews methane, like the sulfur spewing volcanoes on Io. Orbital eccentricity has nothing to do with it. Io's eccentricity is less than Titan's (0.00 vs. 0.03). The heat is generated by the steep gravity gradient between the planet facing side of the moon and its far side, which "kneads" the moon. Jack |
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