Revision for Evaporating Giant | ||
Previous Revision, by Just_ [2023-01-11 20:16:15] | → | Selected revision, by CMDR Marx [2023-01-12 20:59:02] |
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. | → | A Class V Gas Giant 5 ls from the 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 infinitely. | → | There are three stars in this system and only one planet, a class V gas giant. Like other such gas giants, it orbits its parent star close: its distance from the main star is only 5 ls (1,503,798 km from the center of the star). It is also quite hot - 2,217 K. |
JOURNAL | ||
→ | ||
OBSERVATORY | ||
→ |