Revision for Hermes' Acolyte | ||
Previous Revision, by CMDR Sheehy [2022-09-11 15:13:46] | → | Selected revision, by CMDR Sheehy [2022-09-11 15:15:49] |
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 | ||
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REGION | ||
Sanguineous Rim | → | Sanguineous Rim |
LATITUDE | ||
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LONGITUDE | ||
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CALLSIGN | ||
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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 | ||
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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: | → | Discovered during the Deeply Uninteresting Expedition (due) of the Sanguineous Rim. 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 | ||
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OBSERVATORY | ||
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