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Invutil said:I guess I'm dealing with planetary scales so radius comes into effect. Is there a formula I can use? Is there anything special that happens at negative radius, like, a Kerr black hole, using a Newtonian equation? Would the constant-acceleration formula generally be correct, as it is a Taylor expansion? If so, how do you interpret the trajectory after r < 0?
A Gravitational Plot is a visual representation of the gravitational forces between two or more objects. It is typically a graph that plots the distance between the objects on the x-axis and the strength of the gravitational force on the y-axis.
The accuracy of a Gravitational Plot is checked by comparing it to theoretical calculations or experimental measurements. This can be done by calculating the force of gravity using the Universal Law of Gravitation or by conducting experiments with objects of known mass and distance.
Several factors can affect the accuracy of a Gravitational Plot, including errors in measurement of distance and mass, the presence of external forces, and the shape and composition of the objects involved. It is important to carefully control and account for these factors when creating a Gravitational Plot.
Checking the accuracy of a Gravitational Plot is important because it allows us to validate the laws and theories of gravity and understand the behavior of objects in space. It also helps us to identify any discrepancies or errors in our measurements and improve our understanding of the forces at work in the universe.
A Gravitational Plot can be used in scientific research to study the behavior of objects in space and to test the accuracy of theories and laws of gravity. It can also be used to make predictions about the movement and interactions of celestial bodies, such as planets, stars, and galaxies. Additionally, Gravitational Plots can be used to analyze and understand the effects of gravity on systems on Earth, such as tides and orbits.