Verse:Sel/ZE-1: Difference between revisions

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'''ZE-1''', also known as '''Izh''', is a [[:w:F-type main-sequence star|F-type main-sequence star]] with a mass of approximately  1.27''M''<sub>☉</sub> (1.269Mim''M''<sub>J</sub>) and a spectral type of F8V. This star is central to the main solar system in the Sel universe, in which is hosted the most complex life of this universe known to date. The designation of 1 for the first star-scale object to be conceived of in this universe; all star-scale objects in Sel are designated as ZE-the number in order it was conceived.  
'''ZE-1''', also known as '''Izh''' (Periodan: {{term|iž#Periodan|iž}}), is a [[:w:F-type main-sequence star|F-type main-sequence star]] with a mass of approximately  1.27''M''<sub>☉</sub> (1.269Mim''M''<sub>J</sub>) and a spectral type of F8V. This star is central to the main solar system in the Sel universe, in which is hosted the most complex life of this universe known to date. The designation of 1 for the first star-scale object to be conceived of in this universe; all star-scale objects in Sel are designated as ZE-the number in order it was conceived.  


The star is known to radiate high levels of [[Verse:Sel#Magical force|magical radiation]], as is expected of most stars within Sel's physics, forcing many magic-negative organisms on its planets, such as [[Verse:Sel/ZE-1b/Valsatbat/Elves|elves]], to be nocturnal in order to not overload or render useless their abilities. As a result, this radiation is the cause of the observed discrepancy between the star's relatively high mass and relatively low spectral subtype if judging by our universe's physics.
The star is known to radiate high levels of [[Verse:Sel#Magical force|magical radiation]], as is expected of most stars within Sel's physics, forcing many magic-negative organisms on its planets, such as [[Verse:Sel/ZE-1b/Valsatbat/Elves|elves]], to be nocturnal in order to not overload or render useless their abilities. As a result, this radiation is the cause of the observed discrepancy between the star's relatively high mass and relatively low spectral subtype if judging by our universe's physics.
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