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Orion complex: Difference between revisions
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The '''Orion complex''' is a large nebular complex in the [[Orion Arm]] of the [[Milky Way Galaxy]]. The nebula was once the nexus of [[Forerunner]] activity as the core of their [[ecumene]]. It was home to the Forerunner homeworld [[Ghibalb]],<ref name="c222">''Halo: Cryptum'', page 222</ref> located at the outer edges of the nebula, the triple star system housing [[Bornstellar's homeworld|the homeworld]] of [[IsoDidact|Bornstellar Makes Eternal Lasting]] and his family,<ref>''Halo: Cryptum'', page 220</ref> and the [[Capital]], the seat of the [[Ecumene Council]]. The cloud itself is situated between 1,500 and 1,600 light-years away from the [[Sol system]] and is hundreds of light-years across. The complex contains several smaller nebulae, and many protoplanetary discs and young stars.<ref>[[Wikipedia:Orion Molecular Cloud Complex|''Orion Molecular Cloud Complex'' on Wikipedia]]</ref> | The '''Orion complex''' is a large nebular complex in the [[Orion Arm]] of the [[Milky Way Galaxy]]. The nebula was once the nexus of [[Forerunner]] activity as the core of their [[ecumene]]. It was home to the Forerunner homeworld [[Ghibalb]],<ref name="c222">''Halo: Cryptum'', page 222</ref> located at the outer edges of the nebula, the triple star system housing [[Bornstellar's homeworld|the homeworld]] of [[IsoDidact|Bornstellar Makes Eternal Lasting]] and his family,<ref>''Halo: Cryptum'', page 220</ref> and the [[Capital]], the seat of the [[Ecumene Council]]. The cloud itself is situated between 1,500 and 1,600 light-years away from the [[Sol system]] and is hundreds of light-years across. The complex contains several smaller nebulae, and many protoplanetary discs and young stars.<ref>[[Wikipedia:Orion Molecular Cloud Complex|''Orion Molecular Cloud Complex'' on Wikipedia]]</ref> | ||