Genesis Research Group- Internal Communication

[Morosz]

- - - - : Incoming Transmission : - - -
- - - -: ID: Dr. Evan Chandler : - - - -

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- - - - : Secure Channel Open/Close : - - - -
- - - - : Encryption Level L3-74-O-THETA-F9 : - - - -
- - - - : Initializing... : - - - -
- - - - : To: GRG Directorate : - - - -
- - - - : Location: Livadia Shipyard, Omicron Kappa : - - - -
- - - - : Subject: Deep Space Survey report : - - - -



- - - - : Beginning Message : - - - -

Greetings.
It has been some time but The Neumann is finally back in populated space form the deep space journey. Now that the pleasantries are aside i wish to make my report on our findings. As we know we departed from Freeport 11 and then headed for deep space. Our journey was long and we encountered some minor issues but nothing we could not handle. We discovered a new jumphole wich took us beyond the edge nebula. We discovered a new star system wich we designated P3X-234. The following is the report of the systems initial survey.

P3X-234 Preliminary report

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: 26 216 km
Mass: 9.89 x 10e24 kg
Temperature: N/A
Terrian: N/A
Escape velocity: 15.42 km/sec
Initial scanns of the planet's atmosphere concluded that it is comprised of hydrogen and helium.

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.

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/sec


Moving on further we later examined P3X-234/2. This gas giant had no moons nor any indication that it ever had one. It's atmosphere consist primarily of hydrogen, helium and methane. And it is the largest planet within this system.
Diameter: 27,992 km
Mass: 15.76 x 10e24 kg
Terrain: N/A
Temperature: N/A
Escape Velocity: 24.78 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.

Unfortunatly we had to abandon the system when our scanners detected the jumphole is destabilizing. This means that further research within this system is currently not possible.

Down below I attached the system's map as well as the photo from our initial arrival. On the photo unfortunatly you cannot see the asteroid belt nor the nebula.

Attachment 1

Attachment 2