Meeting aboard Barrier

[Morosz]

"Oh. I thought that you..never mind then." He said as he internally cursed at his own stupid impatient self. In any case what was done was done. He might as well salvage as much as he can. He did get some information out which he could later use to further refine his now growing theory. Dropping the cigarette in the ashtray he picked up the datapad activating its screen and inserting the acces codes for it to make the file on it available. He slid the pad across the table to Doctor Genda.

"Well. I'm sure that you are interested in this. So I'm not going to keep you waiting. I'll give you some time to read through it. And then tell me your thoughts. Untill then i'Ll go get myself another drink." As he stood up he forgot to keep his coat tight to his body and if one was looking it at him they could make out the unmistakeable shape of a gunholster and a gun.

Survey Report P3X-234

The system is a binary one with an M8 type dwarf and a G2 type main sequence star. The red dwarf we designated P3X-234/Alpha has the following specifications: Luminosity Ib, Color: Red, it has a Temperature of 3000K, Mass: 1.59 x 10e33 kg, Diameter: 8.02 x 10e9 km. The G2 type main sequence was designated: P3X-234/Beta. It has the following specifications: Luminosity: V, Color: Yellow, Temperature: 5000K, Mass: 1.99 x 10e30 kg, Diameter: 1.39 x 10e7 km.
Arround theese stars we found two gas giants that are in orbit. Designated P3X-234/1 and P3X-234/2. P3X-234/1 had three moons orbiting it. We designated them M7G-451, M7G-452, M7G-453.

P3X-234/1:
Diameter: 120 535 km
Mass: 5,6846 × 10e26 kg
Temperature: N/A
Terrian: N/A
Escape velocity: 35,49 km/sec
Initial scanns of the planet's atmosphere concluded that it is comprised of hydrogen and helium. In detail the outer atmosphere contains 96,3% hydrogen and 3,25% helium. Trace ammounts of ammonia, acetylene propane, ethane and phosphine along with methane have been detected in the atmosphere as well. The upper clouds are composed of ammonia crystals while the lower clouds appear to consist of either ammonium hydrosulfide or water. Ultraviolet radiation from the stars it orbits causes methane photolysis in the upper atmosphere, leading to a series of hydrocarbon chemical reactions with the resulting products being carried downward by eddies and diffusion. Similar to other gas giants it exhibits a banded pattern in its atmosphere. The bands are fainter and wider near the equator. We also observed extremely strong winds in the atmosphere with a peak velocity of 500 m/s.

M7G-451 and M7G-452 are extremely small asteroids that consist mostly of nikel and iron. And M7G-452 is on an extremely low orbit and after anylizing it's behaviour we came to the conclusion that it will collide with P3X-234/1 within the next 200 years.

M7G-453 on the other hand was more interesting to survey. The moon itself is mostly comprised of silicate rock similar to rocky planets and it has large ammount of water on it in the form of a thick lair of Ice. We also suspect form the scans that it has liquid water below said ice wich surrounds the rocky silicate crust. The moon also has a thin atmosphere comprised mainly of molecular oxigen and water vapor.
Diameter: 3 121 km
Mass: 4,80 x 10^22 kg
Temperature: 50K to 125K
Terrian: See above.
Escape Velocity: 2,025 km/s

Moving on further we later examined P3X-234/2. After entering orbit we sent probes to the planet and determined that it consists largely of hydrogen with a minimal ammount of helium and methane. To be precise the upper atmosphere consists of arround 91% hydrogen, 5% helium and 4% methane. It also contains trace ammounts of ammonia, water and silicon. We also detected carbon ethan hydrogen-sulfid, neon, oxigen and sulfur in various ammounts. The upper atmosphere also contains frozen ammonia in a crystalized state. Infrared and ultraviolet scans also detected Benzene among other hydrocarbons.
Diameter: 142 984 km
Mass: 1,989 × 10e27 kg
Terrain: N/A
Temperature: N/A
Escape Velocity: 59,60 km/sec

After finishing up the surveys of the planets and their moons. We moved further away from the system's center to an asteroid belt. Preliminary scans showed nothing extraordinary as the asteroids were comprised mostly of rocky silicates with any noteworthy traces of metals being iron and nickel. After sampling multiple rocks however we found high concentration of platinum in one particularly large rock and it's surroundings. Further research required.

The system also contained a small gas cloud. Scans indicated large concentration of explosive gas pockets making surveys difficult but we believe it consists mostly of methane.

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