This system is the closest known star system in the Milky Way to the Large Cloud of Magellan, located on the outer edge of the Perseus Arm and 40,554.46 LY from Sagittarius A*.

A jump range of at least 128.45 LY is required to reach this system (the closest system is 70.50 LY away but the closest to that, also the second closest system to Cloud One, is 128.45 LY distant). For a 77LY-capable ship, as used for this visit, it is highly recommended to have the capability to carry out a minimum of six standard FSD boosts and twelve basic FSD boosts in addition to the two premium FSD boosts to reach the nearest star. The star density is low in this region and careful fuel management is essential, potentially saving the need for more powerful FSD boosts.

More FSD boosting may be needed at times to traverse the tail end of the Perseus Arm, so a reserve of materials or the means to gather more is essential.

The Nyoijaa QD-K d8-0 system itself is a binary, with a G0 VAB primary and a M1 VA secondary. Only the secondary star has planets, six in total and three of the icy worlds have a single icy moon. The innermost planet is a high metal content type, the others are icy.

The most significant feature is the presence of two biological signals on the surface of the third planet. The life forms found there are Fonticulua Campestris - Amethyst and Bacterium Vesicula - Gold, the latter being hard to find, having a similar colour to much of the surface. The surface temperature of about 40K-78K is unsafe for prolonged on-foot exploration but the surface gravity of 0.20 g makes for straightforward manoeuvring on foot and in a SRV.

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