A central force is characterized by its dependence on the radial distance from a fixed point and by its direction being always along the radius vector. The general mathematical expression for a central force acting on a particle at position r is:
where:
is a scalar function that depends only on the distance
.
is the unit vector pointing from the center toward the particle.
This form ensures that the force has no component perpendicular to . It acts purely in the radial direction.
Scalar Form
In scalar notation, the magnitude of the force is:
where:
is a constant (positive or negative depending on the nature of the force),
is the exponent defining how the force varies with distance.
Examples:
- Gravitational force:
- Electrostatic force:
Vector Form in Polar Coordinates
In polar (planar) coordinates , the position vector is:
The force vector becomes:
with no component:
Conservative Nature and Potential Energy
If the central force is conservative, it can be derived from a potential energy function :
For inverse-square law forces:
This relationship links force and potential energy, simplifying the analysis of orbital motion.
Summary of Mathematical Properties
- Direction: Always along
- Magnitude: Function only of
- Conservative: Can be expressed as gradient of a potential
- Example forms:
(gravitational, electrostatic)
(harmonic oscillator)
These properties make central forces fundamental in describing planetary and satellite motion.