Difference between revisions of "RSS LB2133"
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== Details / Specifications == | == Details / Specifications == | ||
| − | An anomalous signal originating from a quaternary system containing a blue giant star, a red subdwarf star, a yellow main sequence star, and a brown dwarf. The signal is periodic, | + | An anomalous signal originating from a quaternary system containing a blue giant star, a red subdwarf star, a yellow main sequence star, and a brown dwarf. The signal is periodic, modulated, and in the 2.5-3.5 GHz range. |
== History == | == History == | ||
Revision as of 07:16, 30 October 2017
RSS LB2133 Received Signal Source Lon Beon Sector 2133.
Details / Specifications
An anomalous signal originating from a quaternary system containing a blue giant star, a red subdwarf star, a yellow main sequence star, and a brown dwarf. The signal is periodic, modulated, and in the 2.5-3.5 GHz range.
History
RSS LB1937 was detected by the University of Selasia Spinward Survey. It became public knowledge following publication of the "Stars of The Rim" Astrographic Survey in 5570AD. The signal may be a false positive, it may be being transmitted by a currently unknown advanced sophont NIL, it may be evidence of the existence of Lon Beon, or it may simply be a natural phenomenon.
References & Contributors / Sources
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- 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