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

Informace o systému

Příslušnost

Nezávislý

Státní zřízení

Korporace

Ekonomika:

Extraction

Úroveň zabezpečení

Low

 

Populace:

26 515

Kontrolující frakce:

Interstellar Mining Corp
(Občanské nepokoje)

Souřadnice

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

Galaktické souřadnice R: 4 402,189 / l: 337,191 / b: -1,141
Rovníkové koordináty: Stoupání 16h 41m 17,297s / Deklinace: -48° 6'59,033''


Reserve level: Nedotčené

Obyvatelná zóna:
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)

Předpokládaná hodnota: 278 458 CR

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

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

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

Frakce
Interstellar Mining Corp (Civil unrest) 94,000 %
The Consortium (None) 6,000 %
Galactic Mapping Project entry

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