Difference between revisions of "Talk:Planet"

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: - [[User:Maksim-Smelchak|Maksim-Smelchak]] ([[User talk:Maksim-Smelchak|talk]]) 11:34, 31 July 2017 (EDT)
 
: - [[User:Maksim-Smelchak|Maksim-Smelchak]] ([[User talk:Maksim-Smelchak|talk]]) 11:34, 31 July 2017 (EDT)
  
== Additional classification of Planets ==
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== Additional classification of Planets (2017) ==
 
 
 
There is a finer division of the composition of planets. From GT: First In,p 57:  
 
There is a finer division of the composition of planets. From GT: First In,p 57:  
 
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* A planet with a density of 1.3 to 3.0 is a ''silicate world'', with a density 3.1 to 4.5 is a ''low-iron'' world, with density 4.6 to 6.0 is a ''medium-iron'' world, with a density 6.1 to 7.0 is a ''high-iron'' world, and with a density 7.1 and up is a ''metallic'' world.  
A planet with a density of 1.3 to 3.0 is a ''silicate world'', with a density 3.1 to 4.5 is a ''low-iron'' world, with density 4.6 to 6.0 is a ''medium-iron'' world, with a density 6.1 to 7.0 is a ''high-iron'' world, and with a density 7.1 and up is a ''metallic'' world.  
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* Values are in grams per cubic centimeter (gm/cc^3). Earth has a density of 5.5, a medium-iron world. Worlds consisting entirely of water (or ice) would be a ''silicate world''.  
 
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* Icy bodies too small to be planets (i.e. have the gravity to be self-rounding) may have densities in the range of 0.8 to 1.3 range.  
Values are in grams per cubic centimeter (gm/cc^3). Earth has a density of 5.5, a medium-iron world. Worlds consisting entirely of water (or ice) would be a ''silicate world''.  
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* From GT:First In, p 58:  
 
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: G = 0.0228 x K x D , where K is the density given above, and D is the diameter of the world in thousands of miles, and the result G is the gravity of the world in Gs.  
Icy bodies too small to be planets (i.e. have the gravity to be self-rounding) may have densities in the range of 0.8 to 1.3 range.  
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: - [[User:Tjoneslo|Tjoneslo]] ([[User talk:Tjoneslo|talk]]) 11:25, 27 August 2017 (EDT)
 
 
From GT:First In, p 58:  
 
 
 
G = 0.0228 x K x D , where K is the density given above, and D is the diameter of the world in thousands of miles, and the result G is the gravity of the world in Gs.  
 
 
 
[[User:Tjoneslo|Tjoneslo]] ([[User talk:Tjoneslo|talk]]) 11:25, 27 August 2017 (EDT)
 
  
 
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Revision as of 13:19, 16 September 2017

Notes (2017)

  1. External Link: T5 World Mapping Tool
  2. External Link: Unbelievably Strange Planets in Space
  3. External Link: HI. I'm have a question: What are the planet types in 2300 AD? Can others be added?
- Maksim-Smelchak (talk) 11:34, 31 July 2017 (EDT)

Additional classification of Planets (2017)

There is a finer division of the composition of planets. From GT: First In,p 57:

  • A planet with a density of 1.3 to 3.0 is a silicate world, with a density 3.1 to 4.5 is a low-iron world, with density 4.6 to 6.0 is a medium-iron world, with a density 6.1 to 7.0 is a high-iron world, and with a density 7.1 and up is a metallic world.
  • Values are in grams per cubic centimeter (gm/cc^3). Earth has a density of 5.5, a medium-iron world. Worlds consisting entirely of water (or ice) would be a silicate world.
  • Icy bodies too small to be planets (i.e. have the gravity to be self-rounding) may have densities in the range of 0.8 to 1.3 range.
  • From GT:First In, p 58:
G = 0.0228 x K x D , where K is the density given above, and D is the diameter of the world in thousands of miles, and the result G is the gravity of the world in Gs.
- Tjoneslo (talk) 11:25, 27 August 2017 (EDT)

Let's make a nonfunctional blank entry in the UWP and record it for future use. Great point.

I didn't participate in the GURPS products like you, but I have read through all of them and love the work.
I have already been deriving climate codes from the GURPS data.
Let's brainstorm it sometime, please, and see what we can come up with.
- Maksim-Smelchak (talk) 11:30, 27 August 2017 (EDT)

Thomas, I like it. Well done.

Please go over Jupiter if you get a chance.
- Maksim-Smelchak (talk) 21:59, 27 August 2017 (EDT)