Desert Planet (Class-G)

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{{Infobox-Planets  
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|        Planet image=[[Image:Desert.gif]]
|        Planet image=[[Image:Desert.gif]]
|    Image description=Orbital view
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|      Terrain images=[[Image:Desertplain.gif|Desert]] [[Image:Rockfield.gif|Rock]] [[Image:Space.gif|Space]]
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|      Terrain images=[[Image:Desertplain.gif|link=Desert|Desert]] [[Image:Rockfield.gif|link=Rock|Rock]] [[Image:Space.gif|link=Space|Space]]
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|  Atmospheric density=5
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|              Sorium=n/a
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'''Class G''' or '''Desert Planets''' are best suited for solar power for obvious reasons, both in orbit and in desert sections (see properties). Although not the best location for Nitrium mining, but there are only 2 planet classes that you can mine Nitrium on.  
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'''Desert''' or '''Class G Planets''' are one of the most sought-after planet types because you can produce massive energy very cheaply using [[Solar Satellite]]s and [[Solar Array]]s on them. This makes them ideal for energy-intensive uses, such as [[Antimatter]] production or [[Isolinear Chips|Isolinear Chip]] production using Jupiter stations.  However, they can also produce nitrium (although less efficiently than [[Class-La|Lavas]]).
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Class G planets are ideal for power generation to aid in ISO-Chip production.
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Latest revision as of 11:51, 6 September 2016

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Starmap Legend

Colonisable Sectors

Other Sectors

Artificia Sectors
Desert.gif

Orbital view

Desert Planet
Terrain characteristics
Desert Rock Space

General characteristics
Atmospheric density: 5
Attractiveness: 15
Orbital solar power: 7
Desert solar power: 9
Raw material deposits
Iridium Ore: 4
Nitrium: 2
Dilithium: n/a
Sorium: n/a
Planet class overview


Desert or Class G Planets are one of the most sought-after planet types because you can produce massive energy very cheaply using Solar Satellites and Solar Arrays on them. This makes them ideal for energy-intensive uses, such as Antimatter production or Isolinear Chip production using Jupiter stations. However, they can also produce nitrium (although less efficiently than Lavas).


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