G-794

Prior to the End War, this system was colonized by the Korlan Remnant (also known as Korlan Empire). Due to the isolationist nature of the Remnant, not much data had been acquired on the system prior to its fall to the Scourge. The system was visited and surveyed by the Jenolan Alliance ship, USS *Intrepid*, as part of post-End War expedition to the Korlan systems.

## G-794/I

K-class

Diameter: 13 000 km

Estimated age: 6.4 billion years

Ecliptic tilt: 10°

Magnetic axis tilt: 7°

Once an M-class world, this planet has been devastated by the Scourge Harvester ship in September 2419, as it was calculated from Scourge's Dark Energy (DE) weapon residual signal. It is very difficult to sort the planet into any specific category as it shares properties with many different standard types. However, as it still has the tectonic activity as M-class planet, lacks atmosphere, and it is a barren world which could be re-inhabited, it is the opinion of Science Department of the surveying vessel the planet be designated as K-class. It should be noted, however, that this is K-class at its extreme. Any attempts of terraforming will be met with difficulties.

Apart from the lack of atmosphere, one potential hazard is the unsual effect akin to ball lightning - isolated pockets of ionic discharges, occupying volumes in range of 50 cm2 - 1.4 m2. These discharge pockets are more-less evenly spread across the planet, most notably in areas which seemed to be densely populated by the Korlans. Detailed scans by the away teams indicated a correlation with higher concentrations of (DE) residue. It would seem that the diffusion of the residue interacts with what ever remaining atmosphere or gases there is. While the DE residue itself is not active, its presence acts as the catalyst for the longer lifetime of the ionic discharges.

Unless there is some interaction between the DE residue and normal matter on the subspace level, beyond our current level of detection, this would be one of the few recorded instances of DE/DM influence on standard, baryonic matter. Aside from the possible high voltage electric shock, no other hazards from these discharges can be noted.

## Asteroid field

A dense asteroid field stretches between the two planets. Several mining outposts, with different degrees of damage, have been located, with no signs of recent activity. The average mass and distribution of the bodies indicates there is enough material to form a planet, at least of Class D, estimated diameter - 6000 km. It is very likely that the formation of a larger planetary body was disturbed by the presence of the supergiant.

## G-794/II

S-class

Diameter: 14 million km

Estimated age: 7.1 billion years

Ecliptic tilt: 3°

Magnetic axis tilt: 11°-23°

 File:Super+giant.png
A supergiant, possessing a double rings' system, at roughly 10 milion and and 114 million kilometers away from the the planet's ionosphere. The supergiant's surface is very dynamic, with storm winds up to 600 km/h. It is consisting mostly of hydrogen, helium and, to small degree, heavier inert gases. The planet has at least 12 moons, ranging in size 800 - 1200 km. The magnetic field, while unstable, reaches far out from the planet. Five more moons are suspected to exist. None of the moons deemed habitable.