| Revision for Hermes' Acolyte | ||
| Previous Revision, by CMDR Sheehy [2022-09-11 07:15:22] | → | Selected revision, by CMDR Sheehy [2022-09-11 15:13:46] |
| DISCOVERER | ||
| CMDR Sheehy | → | CMDR Sheehy |
| NAME | ||
| Hot, Fast Class V Gas Giant | → | 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 orbits an L-type star every ~5 hours. | → | A Class V Gas Giant orbits an L-type star every ~5 hours. |
| DESCRIPTION | ||
| → | ||
The star system contains one each of a Type-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 closely, while the L Class circles them.
Around the L Class dwarf is a Class V gas giant with a fast and close orbit - a little under 5 hours. A short video demonstrates the positioning: | → | The star system contains one each of a Type-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 closely, while the L Class circles them.
Around the L Class dwarf is a Class V gas giant with a fast and close orbit - a little under 5 hours. A short video demonstrates the positioning: |
| JOURNAL | ||
| → | ||
| OBSERVATORY | ||
| → | ||
