T Tauri (Hind Mine / Hind Nebula (T Tauri)) [#182276016435]

星系资讯

拥护:

独立

政府:

企业

经济:

Extraction

安保等级:

Medium

 

人口:

21,264

控制派系：

Azimuth Biotech
(投资)

坐标

This system is located at: -32.96875 / -206.40625 / -557.3125

银河系坐标 R: 595.221 / l: 176.615 / b: -20.290
赤道坐标 赤经 4h 24m 54.588s / 赤纬 19° 38'59.813''


货物储备等级 储量未经开发

可居住区域：
Metal-rich body (2 to 33 ls), Earth-like world (515 to 773 ls), Water world (423 to 1,637 ls), Ammonia world (1,069 to 2,910 ls), Terraformable (401 to 801 ls)

预计价值： 5,785 cr

交通报告

This system was visited for the first time on EDSM by AndySpawn on 2015年1月11日 上午1:18:41.

它被银星系地图团队命名为:Hind Mine / Hind Nebula (T Tauri)

4531 ships passed through T Tauri space, including 2 ships in the last 7 days.

1 ship passed through T Tauri space in the last 24 hours.

Breakdown:
Imperial Cutter - 1

1 ships were destroyed in this system in the last 24 hours.
次要派系
Azimuth Biotech (Investment) 82.700 %
Hind Co-Operative (None) 17.300 %
Children of the Sun (None) 0.000 %
Taurus Mining Ventures (None) 0.000 %
Aegis Defense (None) 0.000 %
星系地图团队条目

enter image description here

Astrophotography by Mienamoo

The Hind Mine asteroid base was constructed in 3303 by Taurus Mining Ventures. It is in the T Tauri system - orbiting the star that illuminates the Hind's Variable Nebula.

This base was used as a supply depot for the Premonition Allied Coordination in the hours leading up to their mission to defend Salomé.

Reference: Link

enter image description here

NGC 1555, sometimes known as Hind's Nebula, is a variable nebula, illuminated by the star T Tauri, located in the constellation Taurus. The nebula was discovered on October 11, 1852 by John Russell Hind. It is a yellowish/orange nebula and when viewed from within the T Tauri system, part of the nebula resembles the shape of a bird in flight (large image).

T Tauri itself is a very young pre-main-sequence star in the process of contracting to the main sequence. It is the prototype of the T Tauri stars. These young stars have surface temperatures similar to those of main-sequence stars of the same mass, but they are significantly more luminous because their radii are larger. Their central temperatures are too low for hydrogen fusion. Instead, they are powered by gravitational energy released as the stars contract, while moving towards the main sequence, which they reach after about 100 million years. [Note: In Elite Dangerous T-Tauri is depicted as a G-class main sequence star. It is unkown why this is so.] (Source)

The Hind Nebula was the destination of one of the early research voyages organized by the First Great Expedition - making it one of the first nebulae to be surveyed by group exploration (source).