| Original submission for Aryabhata's Shadow | ||
| Original submission, by CMDR Sheehy [2022-12-13 21:03:18] | ||
| DISCOVERER | ||
| → | CMDR Sheehy | |
| NAME | ||
| → | Aryabhata's Shadow | |
| SYSTEMNAME | ||
| → | Byae Aip GW-N d6-10 | |
| CATEGORY | ||
| → | Planetary Features | |
| CATEGORY 2 | ||
| → | ||
| REGION | ||
| → | Dryman's Point | |
| LATITUDE | ||
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| LONGITUDE | ||
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| CALLSIGN | ||
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| SUMMARY | ||
| → | 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:
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| JOURNAL | ||
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| OBSERVATORY | ||
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