The general equation of orbit describes the path of a particle moving under a central force in a plane. By using the conservation of angular momentum and Newton’s second law in polar coordinates, we can derive a differential equation that determines the orbit shape.
Conservation of Angular Momentum
From conservation of angular momentum per unit mass:
where is a constant.
This allows us to write:
Change of Variables
To simplify the radial equation, we introduce:
Differentiating with respect to :
Further derivatives yield:
However, a standard and simpler result from the chain rule gives:
The General Orbit Differential Equation
The derived form of the orbit equation is:
where:
is the reciprocal of the radius.
is the central force as a function of
.
is the specific angular momentum.
This second-order differential equation governs the shape of the orbit.
Example: Inverse-Square Law
For gravitational attraction:
Substituting:
The orbit equation becomes:
The general solution is:
where:
is the orbital eccentricity.
is the orientation constant.
This solution represents a conic section (circle, ellipse, parabola, or hyperbola), depending on .
Significance
The general equation of orbit links the nature of the central force to the trajectory’s geometric shape. For any given central force law , solving this differential equation determines the path of the particle in space.