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Planets: Difference between revisions

From EVE University Wiki
Vordel (talk | contribs)
test for planet icon placement
Vordel (talk | contribs)
Undo revision 8994 by Vordel (Talk)
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[[File:BarrenLarge.png]]<br/>
Barren planets are archetypical "dead terrestrials": dry, rocky worlds with a minimal atmosphere and an unremarkable composition. They are commonly etched with flood channels, which are often broad enough to be visible from orbit; most such worlds have accumulated significant quantities of ice over their lifetimes, but cannot retain it on their surface. Generally surface liquid evaporates rapidly, contributing to the thin atmosphere, but occasionally it will seep back into the ground and refreeze, ready for another breakout in future when the local temperature rises.
Barren planets are archetypical "dead terrestrials": dry, rocky worlds with a minimal atmosphere and an unremarkable composition. They are commonly etched with flood channels, which are often broad enough to be visible from orbit; most such worlds have accumulated significant quantities of ice over their lifetimes, but cannot retain it on their surface. Generally surface liquid evaporates rapidly, contributing to the thin atmosphere, but occasionally it will seep back into the ground and refreeze, ready for another breakout in future when the local temperature rises.


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*Noble Metals
*Noble Metals


 
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Gas planets are characterized by a deep, opaque upper atmosphere, usually composed primarily of light elements such as hydrogen or helium. Simple chemicals can add a range of hues and shades in the visual spectrum, and the interaction between upwellings and rapidly circulating pressure bands result in a huge variety of visible surface structures. A similar level of diversity can be found beneath the cloud-tops: the inner composition of a given gas planet might belong to any one of a dozen broad groups, with no two planets entirely alike in this regard.
Gas planets are characterized by a deep, opaque upper atmosphere, usually composed primarily of light elements such as hydrogen or helium. Simple chemicals can add a range of hues and shades in the visual spectrum, and the interaction between upwellings and rapidly circulating pressure bands result in a huge variety of visible surface structures. A similar level of diversity can be found beneath the cloud-tops: the inner composition of a given gas planet might belong to any one of a dozen broad groups, with no two planets entirely alike in this regard.
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'''Resources'''
'''Resources'''
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Resources on a Gas planet will typically be found in narrow bands running east-west at various latitudes.  Base metals are generally in bands around the equator, Aqueous Liquids and Ionic Solutions in mid-latitudes bands, with the Noble Gas near the poles.  Reactive Gas will be found in small pockets at all latitudes.
Resources on a Gas planet will typically be found in narrow bands running east-west at various latitudes.  Base metals are generally in bands around the equator, Aqueous Liquids and Ionic Solutions in mid-latitudes bands, with the Noble Gas near the poles.  Reactive Gas will be found in small pockets at all latitudes.


 
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