NGC 6188 Sector LC-V c2-28 (Morgan's Rock / NGC 6188) [#7783319541250]
Příslušnost
Nezávislý
Státní zřízení
Korporace
Ekonomika:
Extraction
Úroveň zabezpečení
Low
Populace:
26 515
Kontrolující frakce:
Interstellar Mining Corp
(Občanské nepokoje)
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
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
2309 ships passed through NGC 6188 Sector LC-V c2-28 space, including 10 ships in the last 7 days.
4 ships passed through NGC 6188 Sector LC-V c2-28 space in the last 24 hours.
Breakdown:
Diamondback Explorer - 1
Krait Phantom - 1
Interstellar Mining Corp (Civil unrest) | 99,000 % | ||
The Consortium (None) | 1,000 % |
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.
Astrophotography by CMDR IkerzTheMage