| Revision for Aryabhata's Shadow | ||
| Previous Revision, by CMDR Sheehy [2022-12-14 07:28:43] | → | Selected revision, by CMDR Marx [2022-12-14 12:17:51] |
| 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:
| → | Byae Aip GW-N d6-10 5 a orbits a mere 1,349 km from its parent gas giant, and is only 110 km from its ring. The lack of inclination of the parent Class III gas giant guarantees a spectacular eclipse every 0.8 days. The moon was named after Aryabhata (476–550), an Indian mathematician who explained eclipses and posited that the light of the Moon and the other planets was from them reflecting the Sun's light.
A video of this system can be viewed here. This star system sports 44 bodies, which include:
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| JOURNAL | ||
| → | ||
| OBSERVATORY | ||
| → | ||
