About: Nebula Manipulation   Sponge Permalink

An Entity of Type : dbkwik:resource/xoykDFxJFBgF02W_HRnEzw==, within Data Space : 134.155.108.49:8890 associated with source dataset(s)

The user is able to create, shape and manipulate nebula; an interstellar cloud of dust, hydrogen, helium and other ionized gases, with some being formed from supernova. Most nebulae are of vast size, even hundreds of light years in diameter. Although denser than the space surrounding them, most nebulae are far less dense than any vacuum created in an Earthen environment - a nebular cloud the size of the Earth would have a total mass of only a few kilograms.

AttributesValues
rdf:type
rdfs:label
  • Nebula Manipulation
rdfs:comment
  • The user is able to create, shape and manipulate nebula; an interstellar cloud of dust, hydrogen, helium and other ionized gases, with some being formed from supernova. Most nebulae are of vast size, even hundreds of light years in diameter. Although denser than the space surrounding them, most nebulae are far less dense than any vacuum created in an Earthen environment - a nebular cloud the size of the Earth would have a total mass of only a few kilograms.
dcterms:subject
Row 1 info
  • Manipulate nebulas
Row 1 title
  • Power/Ability to:
Box Title
  • Nebula Manipulation
Caption
  • A living nebula manipulating its own form into that of a dragon.
dbkwik:powerlistin...iPageUsesTemplate
imagewidth
  • 450(xsd:integer)
BGCOLOR
  • black
abstract
  • The user is able to create, shape and manipulate nebula; an interstellar cloud of dust, hydrogen, helium and other ionized gases, with some being formed from supernova. Most nebulae are of vast size, even hundreds of light years in diameter. Although denser than the space surrounding them, most nebulae are far less dense than any vacuum created in an Earthen environment - a nebular cloud the size of the Earth would have a total mass of only a few kilograms. Nebulae are often star-forming regions, such as in the "Pillars of Creation" in the Eagle Nebula. In these regions the formations of gas, dust, and other materials "clump" together to form larger masses, which attract further matter, and eventually will become massive enough to form stars. The remaining materials are then believed to form planets and other planetary system objects.
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