| Revision for Aryabhata's Shadow | ||
| Previous Revision, by CMDR Sheehy [2022-12-14 06:08:56] | → | Selected revision, by CMDR Sheehy [2022-12-14 07:28:43] |
| DISCOVERER | ||
| CMDR Sheehy | → | CMDR Sheehy |
| NAME | ||
| Aryabhata's Shadow | → | Aryabhata's Shadow |
| SYSTEMNAME | ||
| Byae Aip GW-N d6-10 | → | Byae Aip GW-N d6-10 |
| CATEGORY | ||
| Planetary Features | → | Planetary Features |
| CATEGORY 2 | ||
| → | ||
| REGION | ||
| Dryman's Point | → | Dryman's Point |
| LATITUDE | ||
| → | ||
| LONGITUDE | ||
| → | ||
| CALLSIGN | ||
| → | ||
| SUMMARY | ||
| A close-orbiting moon with ring proximity experiencing regular eclipses | → | A close-orbiting moon with ring proximity experiencing regular eclipses |
| DESCRIPTION | ||
| → | ||
Aryabhata (476–550) was an Indian mathematician who explained eclipses and posited that planetary albedo was the reflecting of the sun's light. Byae Aip GW-N d6-10 5 a orbits a mere 1,349 km from it's parent gas giant, and is only 110 km from it's ring. The lack of inclination of the parent Class III gas giant guarantees a spectacular eclipse every 0.8 days.
A video of this system can be viewed here. This star system sports 44 bodies that includes:
| → | Aryabhata (476–550) was an Indian mathematician who explained eclipses and posited that planetary albedo was the reflecting of the sun's light. Byae Aip GW-N d6-10 5 a orbits a mere 1,349 km from it's parent gas giant, and is only 110 km from it's ring. The lack of inclination of the parent Class III gas giant guarantees a spectacular eclipse every 0.8 days.
A video of this system can be viewed here. This star system sports 44 bodies that includes:
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| JOURNAL | ||
| → | ||
| OBSERVATORY | ||
| → | ||
