Two 48 and 29 approximate Solar Masses equivalent Black Holes collided and merged, and approximately 3 Solar Masses of Black Hole equivalent Energy was lost, some 3.26 light-years years away, then the only way the Gravity Energy Wave can travel Earth if following equation is satisfied.

Gradient of "g" = Density of Mass. When the unit probe mass has density of the surrounding Big Mass, there is no Gravitational Force exerted, things float and merge at that distance like clouds or Ionosphere. Gravitation is property of Mass and Space-Time. Mass is Energy and there are all kinds of Energy.

So the only other model that can explain this Space Energy Bubble of Wave reaching Earth is when the Energy density of this Space-Time Ripple is more than the approaching Space Energy Density.

So what is the Energy density of a Black Hole and what is the Energy density of Vacuum of Space - minus all Galactics, Stars, Planets and Sun Mass, Cosmic Particles, and Radiations.

How much distance it has to travel in space to match up the Energy Density of the Vacuum of Space and if it would cover 3.26 light years of Sphere made of Vacuum of Space.

To reach Earth's surface, the Energy Density has to match "n" times that of the Surface Energy Density. This "n" has to be qualified, e.g. 10 factor would be better than factor of :>1, and so on.

So is LIGO sensitive enough to measure this Energy Density Ripple?

We also need to calculate the total Energy of 3 Solar Mass Black Hole and Vacuum Sphere of 3 .26 Billion Light Years. And see if it would be large or small enough to contain the disturbance in Space-Time Fabric.

If it is small, then it becomes easier to detect with LIGO. If it becomes big enough to contain, then it should not have reached Earth.

I think this approach would help look at different angle.

In my calculations, they had to calculate a disturbance in Space-Time Fabric of 420 (no pun intended) Joules differential (spread on the surface of the Vacuum Sphere). When it comes to the area used by LIGO in two LEGS, it comes to a very small small small.. number.

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