There are three main categories of planets: Solid planets, water giants and gas giants. Even moons are considered as planets.

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Terrestrial planet

Image Class Color Exploration Value (with detailed surface scanner?) Rarity In game description
File:Icy-180px.png
Icy Planet
Icy planete White - Grey ~500cr Very common Ice world composed mainly of water ice. Worlds like this will not have much heating in the past, forming in the cooler regions of a star system and have retained many volatiles as solids withing their crust.
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Rocky Planets

Rocky planete

White - Grey - Light blue - Light brown - Yellow ~500cr Common Rocky world with little or no surface metal content. Worlds like this have lost most of their volatiles due to past heating, and any metallic content will form a small central core.
File:Rocky ice.png
Rocky ice planete
Rocky ice planete White - Grey - Light blue - Light brown  ~500cr Uncommon Rocky ice world. Typically formed in the cooler regions of star system these worlds have a small metal core and thick rocky mantle with a crust of very deep ice. Geological activity is common in these worlds because of the large quantities of volatiles in the crust, often creating a thin, sometimes seasonal atmosphere.
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Variety of High Metal Content Planets
High metal content planete Brown - Dark brown - Beige 2,500cr Uncommon Meta-rich world with a metallic core. Worlds like this can have metallic ores near the sruface in places, especially around areas of past volcanism.
Metal rich planete Brown - Black (sometime with visible lava) ~5,000cr Rare
File:Water-World-180px.png
Water World
Water world Blue with green, brown and white unknown (guess ~10,000cr) very rare
Earth-like world Blue with green, brown and white ~10,000cr

Extremely rare

File:Ammonia-World-180px.png
Ammonia World
Ammonia world Light brown unknown (guess ~10,000cr) Very rare

Water Giants

Water Giant

  • Very rare.
  • Color: Blue
  • Exploration value: unknown

Gas Giants

Image Class Exploration Value (with detailed surface scanner?) Rarity  In game description
File:Gas-Giant-Class-I.png
Class I Gas Giant
I 1,000 - 1,500cr Rare Class I or Jovian gas giants have primarily hydrogen and helium atmospheres. Coloration comes from clouds in the upper atmosphere of ammonia, water vapour, hydrogen sulphide, phosphine and sulphur. The temperature at the top of their upper cloud layers is typically less than 150 K.
II 5,000cr Very rare
File:Gas-Giant-Class-III-180px.png
Class III Gas Giant
III 1,000 - 1,500cr Rare Class III gas giants have primarily hydrogen and helium atmospheres without distinctive cloud layers. Their surface temperature typically ranges between 350 K and 800 K. They are primarily blue in colour because of optical scattering in the armosphere - with the chance of wispy cloud layers from sulphides and chlorides.
IV 1,000 - 1,500cr Rare
File:Gas giant with ammonia based life.png
Gas giant with ammonia based life
Gas giant with ammonia-based life 1,000 - 1,500cr ? Very rare Gas giant with ammonia-based life. This is primarily a hydrogen and helium-based atmospheric gas giant, but a little below the surface cloud layers,life exists based in the ammonia-cloud layer. The chemistry of this gaseous region is far from equilibrium, with a surprising excess of oxygen and many carbon-based compounds giving it some vivid colours. As with many such gaseous living systems, it is underpinned by vast quantities of free-floating radioplankton - tiny carbon-based algae, each retaining small quantity of liquid ammonia, extracting their energy from the intese radiation flux.
File:Water based life gas giant.png
Gas giant with water-based life. 1,000 - 1,500cr ? Very rare Gas giant with water-based life. This is primarily a hydrogen and helium based atmospheric gas giant, but not far below the surface exists life based in the water-cloud layer just below the atmospheric surface. The chemistry of this gaseous region is far from equilibrium, with a surprising excess of oxygen and many carbon-based compounds giving it some vivid colours. As with many such gaseous living systems, it is underpinned by vast quantities of free-floating radioplankton - tiny carbon-based algae, each retaining small quantity of liquid water, extracting their energy from the intese radiation flux.