Sun O1 (Divine Immanence) (not published)
Sun O1 (Divine Immanence)
Description:
This was originally a luminous blue stellar body of a star class of considerable interest to the Triglavian Collective. Manipulation of this star by a Triglavian Dazh Porevitium Transmuter has caused profound changes in this stellar body, and throughout the system surrounding it.
More typical members of this relatively rare class of main-sequence stars are often large and massive. Such stars very quickly burn through their core hydrogen fuel supply and therefore have short lifetimes on the main sequence. These stars emit a tremendous amount of ultraviolet radiation and the largest among them will typically go nova after only a few million years. Smaller stars of this type can cool sufficiently that they will turn into rapidly-rotating stars dominated by carbon-nitrogen-oxygen (CNO) cycle nuclear fusion.
More typical members of this relatively rare class of main-sequence stars are often large and massive. Such stars very quickly burn through their core hydrogen fuel supply and therefore have short lifetimes on the main sequence. These stars emit a tremendous amount of ultraviolet radiation and the largest among them will typically go nova after only a few million years. Smaller stars of this type can cool sufficiently that they will turn into rapidly-rotating stars dominated by carbon-nitrogen-oxygen (CNO) cycle nuclear fusion.
Structure and speed:
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Mass: 1e18 kg
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Volume: 1 m3
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Cargo capacity: 0 m3
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