We are proud to host CMDR Urania Minora’s study of the Spectral Class Distribution of Galactic Phenomena, which aims to bring an understanding of the relationship between the Harvard Stellar Classification of a primary star, and what phenomena may be discovered in a system, as a help to guide exploration efforts. The research paper examines the specifics for phenomena of specific interest to Canonn scientists establishing potential patterns and biases from a detailed analysis of available data from 3.28×10^7 known explored systems
Bark Mounds
Mahon Research Base
As with the nearby Mic Turner Base, this facility on HIP 18077 6 C is administered by the Alliance’s Turner Research Group. Clearly fungal growths are of great interest to the…
Mic Turner Base
Constructed in 3302 by the Alliance, despite accusations that they were attempting to lay claim to the organic structures in the area, this base on California Sector BA-A e6 4 serves…
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