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Planets: Difference between revisions

From EVE University Wiki
Dys novus (talk | contribs)
Created page with 'Planets are present in every solar system in EVE. The vast majority are uninhabited. Planetary Interaction introduced in the Tyrannis expansion allows players to utilize the plan…'
 
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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.


===Resources===
'''Resources'''
*Aqueous Liquids
*Aqueous Liquids
*Base Metals
*Base Metals