Two three body simulations are implemented: 2 Black holes and planet Mercury simulation.
Control Display |
The Control Display contains the following parameters which can be changed:
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Time Evolution Display |
Observe the right hand side of this display. You will observe a wobbly black line and three wobblied coloured lines. The three coloured lines are stacked. One above each other. They are shifted to the right compared to the black lines. |
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Time Evolution Display |
The overal impression is that the trajectories of the third planet will be highly influenced by the speed and the common direction of the gravitational field which will make it very difficult to perform a realistic simulation based on actual observations when Black holes are involved.
In order to test the program:
Simulation Display
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Time Evolution Display
The red dots represent a running average value of the angle. The function calculated is f(t) = a + b*t. The parameter a is the initial angle. The parameter b is the forward angle per time unit. |
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Part of the problem is that the Black holes are there already during the start of the observations which makes it extremely difficult to calculate the the initial conditions of the simulations based on actual observations (which are partly invisible). This is a difficult problem when your system is stable but extremely complex when your system is unstable i.e when the black holes will collide.
The reason why they are not completely black is because they can be detected by means of the gravitational field or better the emission of gravitons which influences the behaviour of rotating objects
When you have two rotating Black holes this dynamic field causes what are called gravitational waves and the wobbling of the trajectories of the rotating objects.
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