NGC 6188 Sector LC-V c2-28 (Morgan's Rock / NGC 6188) [#7783319541250]

Informacje o układzie

Sojusz:

Niezależny

Rząd:

Korporacja

Ekonomia:

Extraction

Bezpieczeństwo:

Low

 

Populacja:

26 515

Frakcja kontrolująca:

Interstellar Mining Corp
(Niepokój cywilny)

Współrzędne

This system is located at: 1706.1875 / -87.625 / 4057.15625

Współrzędne galaktyczne R: 4 402,189 / l: 337,191 / b: -1,141
Współrzędne równikowe Rektascensja: 16h 41m 17,297s / Deklinacja: -48° 6'59,033''


Poziom rezerwy: Dziewiczy

Strefa mieszkalna:
Metal-rich body (2 to 7 ls), Earth-like world (111 to 167 ls), Water world (91 to 353 ls), Ammonia world (231 to 628 ls), Terraformable (87 to 173 ls)

Szacowana wartość: 278 458 cr

In this system you can find all the materials for FSD Injections. This is a GREEN system.
Raport ruchu

This system was visited for the first time on EDSM by Majkl.

Został nazwany w Projekcie Mapowania Galaktyki nazwą: Morgan's Rock / NGC 6188

2306 ships passed through NGC 6188 Sector LC-V c2-28 space, including 9 ships in the last 7 days.

0 ship passed through NGC 6188 Sector LC-V c2-28 space in the last 24 hours.

Pomniejsze frakcje.
Interstellar Mining Corp (Civil unrest) 94,000 %
The Consortium (None) 6,000 %
Wpis Projektu Mapowania Galaktyki

enter image description here

Astrophotography by by CMDR Sahb

Morgan's Rock is an asteroid base inside the small NGC 6188 nebula. It is controlled by the Interstellar Mining Corporation, with 26,000 staff on site. All concourse and ship services are available except for outfitting and a shipyard. This is the closest station to Hawking's Gap and the last stop for those going to Eta Carina Nebula 4000ly away. The identity of the station's namesake, 'Morgan,' is unknown.

Reference: Link

NGC 6188 is an emission nebula in the southern constellation Ara, located about four thousand light years coreward of Sol. It also has reflection nebulosity due to the associated open cluster, NGC 6193. It is an active, star forming nebula, with some recently formed stars that are only a few million years in age. These stars continue to sculpt the nebula and contribute to the glow with intense solar ultraviolet radiation. The recent star formation was probably triggered by supernova explosions from previous generations of massive stars within.

enter image description here Astrophotography by CMDR IkerzTheMage