Revision for Shards of Perdition | ||
Previous Revision, by Richard Fluiraniz M. [2022-10-24 04:50:40] | → | Selected revision, by Richard Fluiraniz M. [2022-10-24 04:54:54] |
DISCOVERER | ||
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NAME | ||
Neon Shards | → | Shards of Perdition |
SYSTEMNAME | ||
Slegaa AR-I c11-0 | → | Slegaa AR-I c11-0 |
CATEGORY | ||
Planetary Features | → | Planetary Features |
CATEGORY 2 | ||
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REGION | ||
Errant Marches | → | Errant Marches |
LATITUDE | ||
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LONGITUDE | ||
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CALLSIGN | ||
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SUMMARY | ||
This system features two rare atmospheric bodies (B3 and B6) that have crystalline shards: a very rare combination to have in a single system. | → | This system features two rare atmospheric bodies (B3 and B6) that have crystalline shards: a very rare combination to have in a single system. |
DESCRIPTION | ||
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Firstly, body B 3 located roughly 150,000 light-seconds from the main star, features Technetium crystalline shard formations in the following coordinates: Lat: 52.5163 Long: 13.3373. Crystalline shards lined with yttrium also are featured surface of planet B 6, in the following coordinates; LAT: 53.6022 LONG: 167.6930 Yttrium and Technetium are crucial element in premium FSD injections. With very thin neon and neon rich atmospheres, visitors would need to descend upon the planets to be able to visualize the visual features. The Canonn database has determined, at the time of writing, that only a handful of thin atmospheric planets with crystalline shards have been found; with this being a textbook example of them. | → |
Firstly, body B 3 located roughly 150,000 light-seconds from the main star, features Technetium microorganism crystalline shard formations in the following coordinates: Lat: 52.5163 Long: 13.3373. Crystalline shards lined with yttrium also are featured surface of planet B 6, in the following coordinates; LAT: 53.6022 LONG: 167.6930 Yttrium and Technetium are crucial elements in synthesizing premium FSD injections, necessary to navigate the sparse area. Body B6 "ultra thin" atmosphereWith very thin neon and neon rich atmospheres, visitors would need to descend upon the planets to be able to visualize the visual features. The Canonn database has determined, at the time of writing, that only a handful of thin atmospheric planets with crystalline shards have been found; with this being a textbook example of them. |
JOURNAL | ||
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OBSERVATORY | ||
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