02-23-2017, 12:09 PM
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Miss Raven
Per your request the HS-Marama entered the Omega-11 system and we have concluded our tests on both the Red Giant in that system and the radiation that it emits. We composed a report on our findings, which i now send to you. We also have rock and diamond samples that were recovered if your own people wish to examine them.
I hope this is what you were looking for.
Regards: Dr J. Steiner
Observations on Red Giants and Radioactivity in Omega-11 (pg. 834-836)
Dr J. Steiner, et al (824 A.S.) Excerpt of Report as requested by Auxesia regarding spacial travel in radioactive systems
However in order to understand the level of radioactivity found in the Omega-11 system , and to accuratly predict whether or not the radioactivity will increase within the average Human lifespan, we must first examine the cause. Our focus therefore is the Red Giant that lies at the heart of the system. First charted and mapped by the famed Rheinland explorer, Von Rohe, and later confirmed by the Sirius Meterological Institute (SMI) the giant's data is as follows:
TYPE: M8
LUMINOSITY: Ib
COLOR: Red
TEMPERATURE: 3K
MASS: 1.59 x 10e33 kg
DIAMETER: 8.02 x 10e9 km
Given that stars age over millions if not billions of years it is safe to presume that the star has changed little since Von Rohe first mapped the system.
We can see, according to the above data, that the giant's surface temparture sits around 3000 Kelvin (Roughly 2726.85 degrees celsius). Given the star's mass, this is not an uncommon red giant, if anything it is still a young star. The levels of radiation (Which are confirmed to be Gammar photons) that are produced are perfectly normal for a star this old and of this size. To support this theory, the field team conducted a series of test. At roughly 25 Killometers from the surface of the star, teams were instructed to drop their ship sheilds and for a period of 5 minutes. The resulting damage to the hull was insignificant. The test was repeated with sheilds up with the same results. However at 15.6 Killiometers, the tests were concluded early due to significant hull damage. As such it is not reccomended for pilots to fly within the 16KM mark of the star. It should be noted that the test was conducted without armour, in order to accuratly assess the damage done.
Considering this temprature and the star's mass (as mentioned above) and the radioactivity it is producing we aboard the HS-Marma argue that the star is perfectly normal and healthy for its age, the background radiaction is an example of Nuclear fusion, meaning the star has exhusted its supply of Hydrogen and is now burning Helium. (Crowther, P. A. (797 A.S.). "Physical Properties of Wolf-Rayet Stars". Annual Review of Astronomy and Astrophysics. 177–219) Thus the star is expected to increase over time and eventually from a diamond planet, a nebula or possibly a white dwarf or supergiant at which point the possibility of a supernova is signifcantly higher than what it is now (Zeilik, Michael A.; Gregory, Stephan A. (793 A.S.)Introductory Astronomy & Astrophysics (4th ed.).
Regardless, with sheilds maintained and pilots flying an acceptable distance away from the star, the background radiation poses little to no threats to ships or people.
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