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Saturn has a visitor.

 
 
smorgs
 
  1  
Reply Sat 7 Oct, 2006 01:30 pm
Fantastic photos - thank you!

x
0 Replies
 
Steve 41oo
 
  1  
Reply Sat 7 Oct, 2006 01:40 pm
smorgs wrote:
Fantastic photos - thank you!

x
what you doin here smorshissimus? you suppost to be on planet earth somewhere near blackpool.
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smorgs
 
  1  
Reply Sat 7 Oct, 2006 02:39 pm
And you're supposed to be watching football...

Besides, I like astro... astronomik...

SPACE FINGS...

x
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Walter Hinteler
 
  1  
Reply Thu 1 Mar, 2007 04:27 pm
http://i9.tinypic.com/29pvtk7.jpg

This image of Saturn released on March 1, 2007 taken by the Cassini spacecraft's wide-angle camera on February 4, 2007, at a distance of approximately 1.2 million kilometers (700,000 miles) shows dark and sharply defined ring shadows. Scientist are not yet sure about the precise cause of the color changes form north to south. REUTERS/NASA/JPL/Space Science Institute/Handout
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satt fs
 
  1  
Reply Thu 1 Mar, 2007 05:30 pm
Very mysterious color changes are seen there. Exclamation
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Steve 41oo
 
  1  
Reply Fri 2 Mar, 2007 05:21 am
Todays Independent has some spectaclar pictures of Saturn's rings. Interesting that Saturn itself is flattened at the poles due to its rotation.
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rosborne979
 
  1  
Reply Fri 2 Mar, 2007 07:46 am
Steve 41oo wrote:
Interesting that Saturn itself is flattened at the poles due to its rotation.


Saturn's mean density is lighter than water. It's a relatively 'fluid' planet.
0 Replies
 
Steve 41oo
 
  1  
Reply Fri 2 Mar, 2007 10:44 am
rosborne979 wrote:
Steve 41oo wrote:
Interesting that Saturn itself is flattened at the poles due to its rotation.


Saturn's mean density is lighter than water. It's a relatively 'fluid' planet.
Is it gaseous all the way down? If not is there any sort of boundary between dense gas/liquid or solid?
0 Replies
 
rosborne979
 
  1  
Reply Fri 2 Mar, 2007 11:01 am
Steve 41oo wrote:
rosborne979 wrote:
Steve 41oo wrote:
Interesting that Saturn itself is flattened at the poles due to its rotation.


Saturn's mean density is lighter than water. It's a relatively 'fluid' planet.
Is it gaseous all the way down? If not is there any sort of boundary between dense gas/liquid or solid?


Due to the pressures, I assume it has a 'solid' core, and even the gasses in the middle layers are probably very viscous. But I don't know the density threholds at various levels.

None of the planets are really solid all the way down. Most are fluid to some degree or another. Even Earth is molten rock and metal most of the way down. Then we have a thin layer of crust and a thin layer of atmosphere.

Saturn is probably more like a big thick atmosphere surrounding a kernel of relatively solid compressed gas.

Saturn Info
0 Replies
 
Steve 41oo
 
  1  
Reply Fri 2 Mar, 2007 11:36 am
Thanks

I was just idly musing to myself that if its gaseous at the "surface" and for a long way down, but solid or liquid further down then there might be an "interior surface" but I dont think so. Its just gets more dense until its effectively solid...or liquid. How about glassy?
0 Replies
 
 

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