Bleethue KR-A b15-0 (Beetle Nebula) [#574582907009]
This system is located at:
-7171.15625
/ -992.84375
/ 37657.8125
Coordonnées galactiques:
R: 38 347,387 / l: 10,782 / b: -1,484
Coordonnées équatoriales:
Ascension droite: 18h 14m 54,762s /
Déclinaison: -20° 19'9,324''
Zone habitable :
Metal-rich body (1 to 3 ls), Earth-like world (47 to 70 ls), Water world (38 to 149 ls), Ammonia world (97 to 264 ls), Terraformable (36 to 73 ls)
Crédits estimés : 5 208 cr
This system was visited for the first time on EDSM by Guy De Lombard on 12 déc. 2017 17:11:47.
Cela a été nommé par le Projet Cartographie Galactique avec le nom de : Beetle Nebula
47 ships passed through Bleethue KR-A b15-0 space, including 0 ship in the last 7 days.
0 ship passed through Bleethue KR-A b15-0 space in the last 24 hours.
Beetle Nebula is located in the Perseus Stem over 38,000 LYs from Sol and around 1,000 LYs below the galactic plane. Its colours range from deep purples to bright orange, with half of the nebula obscured in dark clouds of dust.
Most stars inside the nebula are cool K and M class stars - indicating that it could possibly have been a birthplace for many of the red giants and Carbon Stars nearby in the 'Beetle Burial Grounds'. The nebula also has a high concentration of Neutron Stars, White Dwarfs, and Black Holes. Most of these stellar remnants are older generation, roughly 13 billion years old.
There tends to be younger stars at the top of the nebula - including many T-Tauri stars. This age pattern is not limited to star type, but actual star age, as systems toward the top of the nebula are much younger than their counterparts near the bottom. This indicates that the nebula is growing upwards like the famed pillars of creation formations we remember from the ancient Hubble Telescope.
Within the nebula, many extremely large Gas Giant planets has been found, and surprisingly, almost all of these large exoplanets orbited DC White Dwarfs.
Links:
Beetle Nebula served as a basecamp and was extensively surveyed during the SHEPARD Mission in early 3303.
Vera’s Last Jump Landing Site
- Orbital Body: BLEETHUE FL-Y E396 2B
- Surface Coordinates: 38.4910 // -113.3502
- Surface Gravity: 0.06
Named after recently decreased astronomer Vera Rubin, Vera was a part of a binary pair of metallic moons orbiting a metal-rich lava planet - itself bearing a long and thin ring system and orbiting only 1000ls from a B-Class Subgiant star. Vera was the smaller of the two moons, and in fact was so close to its brother that another moon of the same size could not fit in between them. The planet has active silicate vapor volcanism and is rich in jumpnium materials and low g (0.06). The site was used as a basecamp for the Shepard Mission for SRV canyon jumping.
