Capstone
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- Feb 14, 2012
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[1608.01808] Discovery of A New Retrograde Trans-Neptunian Object: Hint of A Common Orbital Plane for Low Semi-Major Axis, High Inclination TNOs and Centaurs
The gist of it:
". . . Comparing similar high inclination TNOs and Centaurs (q>10 AU, a<100 AU andi>60∘), we find that these objects exhibit a surprising clustering of ascending node, and occupy a common orbital plane. This orbital configuration has high statistical significance: 3.8-σ. An unknown mechanism is required to explain the observed clustering. This discovery may provide a pathway to investigate a possible reservoir of high-inclination objects."
It seems a minor planetary body has broken the ecliptic plane on the far side of Neptune. This object has a highly inclined retrograde orbit that cannot be explained by anything in the observable solar system. I think what we have here may be our first visual confirmation of one of the far-flung orbitals in the Nibiru system. Accordingly, the "reservoir" mentioned above would be the ecliptic plane for our Sun's couterpart in a binary system.
More to come.
Discovery of A New Retrograde Trans-Neptunian Object: Hint of A Common Orbital Plane for Low Semi-Major Axis, High Inclination TNOs and Centaurs
Ying-Tung Chen,Hsing Wen Lin,Matthew J. Holman, Matthew J. Payne, Wesley C. Fraser, Pedro Lacerda, Wing-Huen Ip, Wen-Ping Chen, Rolf-Peter Kudritzki, Robert Jedicke, Richard J. Wainscoat,John L. Tonry,Eugene A. Magnier,Christopher Waters, Nick Kaiser, Shiang-Yu Wang, Matthew Lehner
(Submitted on 5 Aug 2016)
Although the majority of Centaurs are thought to have originated in the scattered disk, with the high-inclination members coming from the Oort cloud, the origin of the high inclination component of trans-Neptunian objects (TNOs) remains uncertain. We report the discovery of a retrograde TNO, which we nickname "Niku", detected by the Pan-STARRS 1 Outer Solar System Survey. Our numerical integrations show that the orbital dynamics of Niku are very similar to that of 2008 KV42(Drac), with a half-life of ∼500 Myr. Comparing similar high inclination TNOs and Centaurs (q>10 AU, a<100 AU andi>60∘), we find that these objects exhibit a surprising clustering of ascending node, and occupy a common orbital plane. This orbital configuration has high statistical significance: 3.8-σ. An unknown mechanism is required to explain the observed clustering. This discovery may provide a pathway to investigate a possible reservoir of high-inclination objects.
The gist of it:
". . . Comparing similar high inclination TNOs and Centaurs (q>10 AU, a<100 AU andi>60∘), we find that these objects exhibit a surprising clustering of ascending node, and occupy a common orbital plane. This orbital configuration has high statistical significance: 3.8-σ. An unknown mechanism is required to explain the observed clustering. This discovery may provide a pathway to investigate a possible reservoir of high-inclination objects."
It seems a minor planetary body has broken the ecliptic plane on the far side of Neptune. This object has a highly inclined retrograde orbit that cannot be explained by anything in the observable solar system. I think what we have here may be our first visual confirmation of one of the far-flung orbitals in the Nibiru system. Accordingly, the "reservoir" mentioned above would be the ecliptic plane for our Sun's couterpart in a binary system.
More to come.