Aceleration/Velocity and Integration help

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SUMMARY

The discussion focuses on deriving the velocity expression of a planet in orbit based on its acceleration, which is influenced by gravitational forces. The gravitational force is defined by the equation F=(-G.m1.m2/r^3) * position_vector. The participants debate the validity of using the formula a = (Vf - Vi) / (tf - ti) for each axis and explore integration methods to derive velocity, emphasizing that acceleration is not constant in elliptical orbits. The conversation highlights the need for understanding Newtonian mechanics and the properties of elliptical orbits.

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  • Understanding of Newton's laws of motion
  • Familiarity with gravitational force equations
  • Knowledge of calculus, specifically integration techniques
  • Concept of elliptical orbits in celestial mechanics
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  • Study Newtonian central force theory
  • Learn about the properties of elliptical orbits and Kepler's laws
  • Explore advanced integration techniques in physics
  • Investigate the relationship between acceleration and velocity in non-constant acceleration scenarios
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Physics students, astrophysicists, and anyone interested in celestial mechanics and orbital dynamics will benefit from this discussion.

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Hello, I have expression for the aceleration of a planet in the orbit of another planet and need to get the expression for it's velocity. The aceleration expression came from the Gravitacional Force within the gravitacional field of the planets.

F=ma
F=(-G.m1.m2/r^3) * position_vector

Where r is the scalar value of the position_vector. From here we can get ax and ay.

For the velocity:

1) Is it ok to do it Using
a= Vf-Vi/tf-ti
for each axis (ax ay).?

2) How would it be done using the intergration rules.?

Thanks.
 
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If I'm understanding correctly, you want an expression for the speed of the planet as it orbits. is that not simply [tex]\frac{m_2v^2}{r} = \frac{Gm_1m_2}{r^2}[/tex] canceled down, because that seems far too simple.
 
finchie_88 said:
If I'm understanding correctly, you want an expression for the speed of the planet as it orbits. is that not simply [tex]\frac{m_2v^2}{r} = \frac{Gm_1m_2}{r^2}[/tex] canceled down, because that seems far too simple.

That assumes the orbit is circular. In general they are ellipses.

In general you can't set [tex]\mathbf{a}=\frac{\mathbf{\Delta v}}{\Delta t}[/tex] because this implicitly assumes that the acceleration is constant. You need to use [tex]\mathbf{v}= \int \mathbf{a(r)} \, dt[/tex] the problem being here that you are integrating over the "wrong" variable. Without dragging the whole Newtonian central force theory into it, I'm not sure what to do to fix that at this point. Off the top of my head I would suggest that perhaps using the facts that the orbit is an ellipse and that equal areas are swept out by the orbit in equal times might be useful.

What subject does this question pertain to? (i.e. is this a Math question or Physics?)

-Dan
 

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