| Revision for Evaporating Giant | ||
| Previous Revision, by Just_ [2023-01-11 19:50:35] | → | Selected revision, by Just_ [2023-01-11 19:53:33] |
| DISCOVERER | ||
| CMDR Just_ | → | CMDR Just_ |
| NAME | ||
| Evaporating Giant | → | Evaporating Giant |
| SYSTEMNAME | ||
| Thailoea TE-V c4-1 | → | Thailoea TE-V c4-1 |
| CATEGORY | ||
| Planetary Features | → | Planetary Features |
| CATEGORY 2 | ||
| → | ||
| REGION | ||
| Inner Orion Spur | → | Inner Orion Spur |
| LATITUDE | ||
| → | ||
| LONGITUDE | ||
| → | ||
| CALLSIGN | ||
| → | ||
| SUMMARY | ||
| Class V gas giant only 5ls from main star. | → | Class V gas giant only 5ls from main star. |
| DESCRIPTION | ||
| → | ||
There are 3 stars in this system and only one planet - a class V gas giant. The distance from the main star is only 5 ls (1,503,798 km from the center of the star). It is quite hot - 2,217 K. In real life, a gas giant so close to the star would certainly not survive for long, and would soon evaporate, but here, in the elite, it can be observed indefinitely.
| → | There are 3 stars in this system and only one planet - a class V gas giant. The distance from the main star is only 5 ls (1,503,798 km from the center of the star). It is quite hot - 2,217 K. In real life, a gas giant so close to the star would certainly not survive for long, and would soon evaporate, but here, in the elite, it can be observed indefinitely.
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| JOURNAL | ||
| → | ||
| OBSERVATORY | ||
| → | ||
