Qubar and Ixonic Double dwarf planet Binary system

The Qubar and Ixonic double dwarf planet system orbit NY-Beta in the extreme regions of the Beta system. Discovered by Luamer Vitch, it has a extremely low magnitude of +11.6 and with a albedo of 41%. It also has a average surface temperature of -340c, due to it's extreme distance form Beta. The system is currently one of the 2 only known planetary bodies to be binaries, the other being XG25A and XG25B in a planetary system 56 light years away. There were also some evidence that Qubar and Ixonic were used to be slightly closer to Beta, as evidence by the Montri trojans.

Orbit
The binary system orbits NY-Beta at roughly 43 AU with a eccentricity of 0.42 and a inclination of 0.18. Due to it's orbit being in an vulnerable location, gas giants and other dwarf planets in the vicinity, the eccentricity can vary between 0.38 to 0.49, though it's inclination remains largely the same with usually a 0.5 difference. Interactions with neighboring dwarf planet Jasperion-SPS-A and Qilkon-SPS-A also will encourage such effect. Regularly inspections are preformed on the binary system to investigate the " effect " further via the Uriland Space Program ( USP )