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

Информация о системе

Принадлежность:

Независимые

Форма правления:

Анархия

Экономика:

Extraction

Безопасность:

Anarchy

 

Население:

26 515

Контролирующая фракция:

The Consortium
(Инвестирование)

Координаты

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

Галактические координаты: R: 4 402,189 / l: 337,191 / b: -1,141
Экваториальные координаты: прямое восхождение: 16h 41m 17,297s / склонение: -48° 6'59,033''


Объем ресурсов: Обилие

Обитаемая зона:
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)

Прибл. стоимость данных сканирования: 278 458 кр.

In this system you can find all the materials for FSD Injections. This is a GREEN system.
Отчёт о передвижениях

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

Название, присвоенное Galactic Mapping Project: Morgan's Rock / NGC 6188

2313 ships passed through NGC 6188 Sector LC-V c2-28 space, including 6 ships in the last 7 days.

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

Breakdown:
Asp Explorer - 2

Фракции
The Consortium (Investment) 85,900 %
Interstellar Mining Corp (None) 14,100 %

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