Carbon Detonation: Difference between revisions
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== Requirements == | == Requirements == | ||
{| cellpadding="5" border="1" style="border-collapse: collapse; text-align: center" class="colortable-Eve" | {| cellpadding="5" border="1" style="border-collapse: collapse; text-align: center" class="colortable-Eve" | ||
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| {{PvE}} || 1164% || 10125% || 951% || 4050% || rowspan=2 | 6 || rowspan=2 | 1 || rowspan=2 | 22 || rowspan=2 | 1 || rowspan=2 | 300 MP || rowspan=2 | 180 Seconds || rowspan=2 | [[File:ElWater.png|link=El's Essence]] x1 | | {{PvE}} || 1164% || 10125% || 951% || 4050% || rowspan=2 | 6 || rowspan=2 | 1 || rowspan=2 | 22 || rowspan=2 | 1 || rowspan=2 | 300 MP || rowspan=2 | 180 Seconds || rowspan=2 | [[File:ElWater.png|link=El's Essence]] x1 | ||
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| | | {{PvP}} || 139% || 1215% || 114% || 486% | ||
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== Trivia == | == Trivia == | ||
*The name refers to the [https://en.wikipedia.org/wiki/Carbon_detonation process] by which a white dwarf star undergoes a runaway thermonuclear reaction and explodes as a bright [https://en.wikipedia.org/wiki/Type_Ia_supernova Type Ia supernova]. | *The name refers to the [https://en.wikipedia.org/wiki/Carbon_detonation process] by which a white dwarf star undergoes a runaway thermonuclear reaction and explodes as a bright [https://en.wikipedia.org/wiki/Type_Ia_supernova Type Ia supernova]. | ||
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==Updates== | ==Updates== | ||