Hyponia AA-A g2 (Hyponia) [#145095254]

Coordinates

This system is located at: -23174.875 / -206.90625 / 23643.0625

Galactic coordinates: R: 33,107.583 / l: 44.427 / b: -0.358
Equatorial coordinates: Right ascension: 19h 13m 55.120s / Declination: 10° 3'0.067''


Traffic report

It was named by the Galactic Mapping Project with the name of: Hyponia

There is no traffic report for Hyponia AA-A g2.

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This sector is one of several anomalies found throughout the galaxy. For reasons unknown, hyperdrives refuse to lock on to the stars in this area of space, effectively making it impassable to deep space travellers. Pilots are thus required to either avoid this area or to plot a course above, below or around it. What may be found within this restricted area remains a mystery for the time being.

In 3301 the Daedalus Wing set out to map the borders of this region; this mission was cut short due to developments in the Formidine Rift. In 3303 a second attempt was made with the Hyponia Horizon Mission, which was finished with a complete different crew than that with which the mission was started.

In late October 3303 the Aronnax Expedition arrived at the borders of Hyponia and conducted a survey for signs of spacefaring activity, as well as outdoor worlds and systems with all the materials needed for FSD boosting ('green' systems). A suitable location for a 'Forward Base' was discovered just under 1 KLY from the border: Wembuia HD-Z d1-39 hosts an Earth-like World and has several 'green' systems nearby, including its nearest neighbour. Notable findings included an Earth-like World with one of the densest atmospheres known, with 4.32 bars of pressure, Pha Flaae QZ-N c20-76 5. Detailed findings on the region are given in the expedition journal.

The Hyponia permit locked sector is generally spherical in shape, the region intersects the Galactic Plane, and extends roughly 500 LY above and below the plane, encompassing a volume of roughly 1000 LY in diameter. No astronomical anomalies were encountered during the survey, however it has been noted that inside the upper spherical region the stars appear to be more dense than in the lower part.

Links:

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