Your Gateway to Understanding Black Holes
The Rupture of Black Holes and the Formation of Magnetic Strings
The sets of parallel magnetic strings observed between our SMBH and a point approximately 150 light-years from it are the remnants of the rupture of black holes.
Once a black hole of sufficient mass breaches that distance from the edge of the SMBH, much of it bursts into two equal but opposite magnetic rotating masses, which this theory refers to as Right and Left Swirls.
- The Right Swirl has a positive inner core and a negative outer shell, spacing it from the Left Swirl.
- The Left Swirl has a negative inner core and a positive outer shell.
- Centrifugal force secures each Swirl in place.
A pictorial cross-section of a mature black hole attempts to show the Swirls, which might comprise a larger proportion of the black hole’s matter than depicted.
Other remnants of the rupture act as additional fuel for the already enhanced journey of the Left and Right Swirl’s trails into our SMBH.
Three spinning entities—both Swirls and the black hole itself—combine to present an interesting gyroscopic entity.
Other remnants of the rupture act as additional fuel for the already enhanced journey of the Left and Right Swirl’s trails into our SMBH.
Three spinning entities—both Swirls and the black hole itself—combine to present an interesting gyroscopic entity.
Summarizing:
The same force that holds the Swirls separated before the black hole bursts continues to exist after the burst.
Anomaly and Movement
In Search of Movement
Along with the sets of parallel magnetic strings, a brightly shining anomaly has been observed, and its trajectory deserves attention (forthcoming picture).
While primarily seeking movement, even the slightest change in other aspects of the anomaly could be significant, including but not limited to: Radiation levels, absorption properties, shape and size variations, color shifts and polar activity.
While primarily seeking movement, even the slightest change in other aspects of the anomaly could be significant, including but not limited to: Radiation levels, absorption properties, shape and size variations, color shifts and polar activity.
With decades of data available, if movement is confirmed, trajectories and timelines can be established. Possible paths include:
- A slingshot past our SMBH
- Entry into the SMBH
Contributors
George Scheber – TheoristJeff Sadowski – Illustrator
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