Difference between revisions of "Maurasi VIII"

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{{quote|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.}}<br/><br/>
 
{{quote|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.}}<br/><br/>
  
'''The following data is extracted from the Caldari Research & Science Hall of Records concerning the specifics of Kisogo VIII & Maurasi VIII.''<br/><br/>
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'''The following data is extracted from the Caldari Research & Science Hall of Records concerning the specifics of Maurasi VIII.''<br/><br/>
  
 
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Revision as of 19:33, 21 May 2012



Maurasi VIII is 1 of several Gas class planets in a system of 12 known within the Maurasi system. It lays within the Kimotoro constellation of The Forge deep within the heart of Caldari State.




"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."



'The following data is extracted from the Caldari Research & Science Hall of Records concerning the specifics of Maurasi VIII.

Maurasi VIII
Temperature 90 K
Orbit Radius 3.913 AU
Eccentricity 0.084
Mass 4.9e+26 kg
Density 698.2 g/cm3
Surface gravity 10.8 m/s^2
Escape velocity 34.5 km/s
Orbit period 278 days
Pressure 525.60 kPa
Radius 55.190 km
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