Revision for Hermes' Acolyte | ||
Previous Revision, by CMDR Marx [2022-09-11 15:53:34] | → | Selected revision, by CMDR Sheehy [2022-09-11 16:46:56] |
DISCOVERER | ||
CMDR Sheehy | → | CMDR Sheehy |
NAME | ||
due 001 - Hermes' Acolyte | → | Hermes' Acolyte |
SYSTEMNAME | ||
Gludgae RM-W d1-29 | → | Gludgae RM-W d1-29 |
CATEGORY | ||
Sights and Scenery | → | Sights and Scenery |
CATEGORY 2 | ||
→ | ||
REGION | ||
Sanguineous Rim | → | Sanguineous Rim |
LATITUDE | ||
→ | ||
LONGITUDE | ||
→ | ||
CALLSIGN | ||
→ | ||
SUMMARY | ||
A Class V Gas Giant which orbits an L-type star every ~5 hours. | → | A Class V Gas Giant which orbits an L-type star every ~5 hours. |
DESCRIPTION | ||
→ | ||
This star system, discovered during the Deeply Uninteresting Expedition (due) of the Sanguineous Rim, houses a Class V gas giant with a fast and close orbit around an L class dwarf star. It completes an orbit in about five hours. The system's stars consist of one each of a A, F, K, M, and L type stars. The F class star is in a fast orbit around the A Class primary. The others are clustered together in a trinary cluster at a short distance from the primary. The K and M types orbit the barycenter closely, while the L Class circles them. Around the class L dwarf star is a Class V gas giant with a fast and close orbit - a little under 5 hours. A short video demonstrating the positioning can be seen here. | → | This star system, discovered during the Deeply Uninteresting Expedition (due) of the Sanguineous Rim, houses a Class V gas giant with a fast and close orbit around an L class dwarf star. It completes an orbit in about five hours. The system's stars consist of one each of a A, F, K, M, and L type stars. The F class star is in a fast orbit around the A Class primary. The others are clustered together in a trinary cluster at a short distance from the primary. The K and M types orbit the barycenter closely, while the L Class circles them. Around the class L dwarf star is a Class V gas giant with a fast and close orbit - a little under 5 hours. A short video demonstrating the positioning can be seen here. |
JOURNAL | ||
→ | ||
OBSERVATORY | ||
→ |