#1
|
|||
|
|||
Titan/tides
Darn good question. I would like to know this also. It would depend on the
rotation time of Titan and the eccentricity of its orbit, and the exact time. I have no idea. "Pierre Vandevennne" wrote in message ... Assuming there are "seas" on Titan, whatever they are made of, does anyone knows if the tides were high or low at the location Huygens touched down? I saw some amateur speculation that the altitude pics looked a lot like the tide weathered dutch coastal areas, and at the same time ESA mentions the possibility of erosion at the foot of the stones/ice cubes. That's fun to imagine that Huygens landed on a beach, at a time where the tides were low and that the erosion seen at the bottom of the stones/ice cubes is what we can observe at the base of round stones on a sand beach here. Also, a fun site (thanks for the link JMB!) http://anthony.liekens.net/index.php/Main/Huygens |
#2
|
|||
|
|||
On 15 Jan 2005 16:31:24 GMT, Pierre Vandevennne
wrote: Assuming there are "seas" on Titan, whatever they are made of, does anyone knows if the tides were high or low at the location Huygens touched down? That's a very good point. Some quick math using mean masses and distances for Saturn and Titan would suggest the tidal forces are some 50 times stronger than between the Earth and Moon. That would suggest tidal activity might be significant on Titan. --- Michael McCulloch |
#3
|
|||
|
|||
"Pierre Vandevennne" wrote in message ... Assuming there are "seas" on Titan, whatever they are made of, does anyone knows if the tides were high or low at the location Huygens touched down? I saw some amateur speculation that the altitude pics looked a lot like the tide weathered dutch coastal areas, and at the same time ESA mentions the possibility of erosion at the foot of the stones/ice cubes. That's fun to imagine that Huygens landed on a beach, at a time where the tides were low and that the erosion seen at the bottom of the stones/ice cubes is what we can observe at the base of round stones on a sand beach here. Also, a fun site (thanks for the link JMB!) http://anthony.liekens.net/index.php/Main/Huygens I think I read somewhere that Titan is gravitationally locked to Saturn - hence no tides; or rather a permanent high tide at sub-saturnian point and its antipode. see para 6 in this article http://www.csmonitor.com/2002/1212/p25s02-stss.html |
#4
|
|||
|
|||
Tides of what? Obviously not enough to wipe out all the impact
craters Isee. Michael McCulloch wrote: On 15 Jan 2005 16:31:24 GMT, Pierre Vandevennne wrote: Assuming there are "seas" on Titan, whatever they are made of, does anyone knows if the tides were high or low at the location Huygens touched down? That's a very good point. Some quick math using mean masses and distances for Saturn and Titan would suggest the tidal forces are some 50 times stronger than between the Earth and Moon. That would suggest tidal activity might be significant on Titan. --- Michael McCulloch |
#5
|
|||
|
|||
Assuming there are "seas" on Titan, whatever they are made of, does anyone knows if the tides were high or low at the location Huygens touched down? That's a very good point. Some quick math using mean masses and distances for Saturn and Titan would suggest the tidal forces are some 50 times stronger than between the Earth and Moon. That would suggest tidal activity might be significant on Titan. Actually, from a distance of many km from the surface, they remaind me of the seas on the Moon. Image 3 on the Cassini site seems to very clearly show craters throughout. I would have trouble imagining ripples or tides that large. The image info claims there is a "shoreline", but it looks a lot more to me like crater boundaries, as would be seen on the Moon. Dominic |
#6
|
|||
|
|||
Dominic-Luc Webb wrote in
: of the seas on the Moon. Image 3 on the Cassini site seems to very clearly show craters throughout. I would have trouble imagining ripples or tides that large. The image info claims there is a "shoreline", but it looks a lot more to me like crater boundaries, as would be seen on the Moon. Well, see the other thread he I guess we aren't sure there are small craters there. Some probably very dumb questions and possibly dumb answers. What is the density of liquid or solid ethane at Titan's temperature? Finding the density at 20C is easy enough, but ethane ice? Ethane is flammable. I guess that means it can be violently oxydized. I've read also that there was propane and acetylene. How does one safely introduce oxygen in such a system? -- Pierre Vandevenne - DataRescue sa/nv - www.datarescue.com The IDA Pro Disassembler & Debugger - world leader in hostile code analysis PhotoRescue - advanced data recovery for digital photographic media latest review: http://www.pcmag.com/article2/0,1759,1590497,00.asp |
Thread Tools | |
Display Modes | |
|
|