Neutron Star (Omega-41)
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Revision as of 09:31, 2 February 2016 by Silverleaf81 (talk | contribs) (Created page with "<div style="font-size:40px; line-height:60px; color:red;">'''WARNING, NAVIGATIONAL HAZARD! '''</div> The Neutron Star found at the center is the most commonly seen one i...")
WARNING, NAVIGATIONAL HAZARD!
The Neutron Star found at the center is the most commonly seen one in Sirius due to the many system connections present. It is one of only 2 Neutron Stars to emit visible radiation, a characteristic it shares with a Neutron Star in a nearby system. It also has a visible ring system, a distinction it shares with the Puerto Rican Neutron Star.
Long before humans discovered Omega-41, the star at the center of the system went supernova, shattering all the planets into a massive asteroid field, and then causing the star to collapse into the Stellar Remnant seen today.
