Basilisk Nebula
The Basilisk Nebula is an emission nebula located in the heart of Tarchon Sector, within the Where The Stars End region of the Empty Stars.
- It is an astrographic feature and a nebula.
Description (Specifications)[edit]
The Basilisk Nebula is a group of bright nebulae and dark clouds measuring around 10 parsecs coreward-rimward by 13 parsecs spinward-trailing. The Basilisk's Eye system lies at its core.
- It is classified as an emission nebula and is primarily formed of ionized gases, thrown off by the supergiant primary star of the Basilisk's Eye system many millennia ago.
- The gases consist of about 90% hydrogen (H2), with the remainder made up of helium (He), oxygen (O2), nitrogen (N2), and other elements. The clouds have a mean density of 102–106 particles/cm³.
- The gases primarily emit red light, though other colors can be seen: the source of ionization is high-energy photons emitted from the Basilisk's Eye supergiant star.
A quaternary star system lies at the heart of the nebula:
Hex Location: 1723 Tarchon Sector. 3 Gas Giants.
History & Background (Dossier)[edit]
The positions and types of the stars present within the Basilisk Nebula have been cataloged as part of the University of Tal Varisa Deep Sky Program.
Image Repository[edit]
Worlds & Sectors (Astrography)[edit]
This astrographic feature is primarily found in the following areas:
Charted Space:
World Listing: 1105[edit]
The following systems and worlds are associated with this astrographic feature:
References & Contributors (Sources)[edit]
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- Traveller Wiki Editorial Team
- Author & Contributor: Lord (Marquis) and Master Scout Emeritus Adie Alegoric Stewart of the IISS
- Author & Contributor: Lord (Marquis) and Master of Sophontology Maksim-Smelchak of the Ministry of Science
