The Binet equation, derived by Jacques Philippe Marie Binet, provides the form of a central force given the shape of the orbital motion in plane polar coordinates. The equation can also be used to derive the shape of the orbit for a given force law, but this usually involves the solution to a second order nonlinear ordinary differential equation. A unique solution is impossible in the case of circular motion about the center of force.
The shape of an orbit is often conveniently described in terms of relative distance as a function of angle . For the Binet equation, the orbital shape is instead more concisely described by the reciprocal as a function of . Define the specific angular momentum as where is the angular momentum and is the mass. The Binet equation is
Newton's Second Law for a purely central force is
The conservation of angular momentum requires that
Derivatives of with respect to time may be rewritten as derivatives of with respect to angle.
Combine all of the above and we have
If the angle is measured from the periapsis, then the general solution for the orbit expressed in (reciprocal) polar coordinates is
Inverse Kepler problem
Differentiating twice the above polar equation for an ellipse gives
The force law is therefore
The effective force for Schwarzschild coordinates is
In the parameterized post-Newtonian formalism we will obtain
where for the general relativity and in the classical case.
An inverse cube force law has the form
The shapes of the orbits of an inverse cube law are known as Cotes spirals. The Binet equation shows that the orbits must be solutions to the equation
The differential equation has three kinds of solutions, in analogy to the different conic sections of the Kepler problem. When , the solution is the epispiral, including the pathological case of a straight line when . When , the solution is the hyperbolic spiral. When the solution is Poinsot's spiral.
Off-axis circular motion
Although the Binet equation fails to give a unique force law for circular motion about the center of force, the equation can provide a force law when the circle's center and the center of force do not coincide. Consider for example a circular orbit that passes directly through the center of force. A (reciprocal) polar equation for such a circular orbit of diameter is
Differentiating twice and making use of the Pythagorean identity gives
The force law is thus
Note that solving the general inverse problem, i.e. constructing the orbits of an attractive force law, is a considerably more difficult problem because it is equivalent to solving
which is a second order nonlinear differential equation.
- Bohr–Sommerfeld quantization#Relativistic orbit
- Classical central-force problem
- General relativity
- Two-body problem in general relativity
- Bertrand theorem
- "Fyta12:1 – Motion in a Central Force Field". Retrieved 2010-10-05.
- http://chaos.swarthmore.edu/courses/PDG07/AJP/AJP000352.pdf - The first-order orbital equation
- http://arxiv.org/pdf/astro-ph/0306611.pdf - A flat space-time relativistic explanation for the perihelion advance of Mercury
- Yan Kun. General form of Binet’s equation (2007)