Hi Our teacher told us the following:F = m * v² / r = m * 4 pi² /

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The discussion revolves around the formulas related to gravitational forces and orbital mechanics, specifically focusing on the relationship between force, mass, and radius. The teacher's equations illustrate how gravitational force can be expressed in different forms, including the role of constants like k and c. The mention of 1/r² indicates the inverse square law, which is fundamental in gravitational interactions, particularly in the context of celestial bodies like Earth and the Sun. The formula T = 2π√(r³/GM) is introduced to explain the time taken for an orbit, linking orbital radius and mass. Understanding these concepts is crucial for grasping the dynamics of objects in orbit.
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hi

Our teacher told us the following:

F = m * v² / r = m * 4 pi² / T² * r

= m * 4 pi² / k * 1 / r²

= c * m / r²

F = y * mM / r2

Why is there the k and 1 / r² and later the c?
 
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Did this have to do with one object orbiting another?
 


Yes, it's about the Earth around the Sun for example.

PS: I now understand the c but still not k (is it the same?) and 1 / r² :S
 


Are you familiar with the following formula?
T = 2\pi\sqrt{\frac{r^3}{GM}}where T is the time taken for one orbit, r is the radius of the orbit, G is the gravitational constant, and M is the mass of the body being orbited.
 
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