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of Particles Moving in a Central Force Field |
The Astronomer Johannes Kepler found laws followed by the orbits of the planets of the solar system. Isaac Newton explained those laws as a result of the gravitation attraction between the Sun and the planets that obeyed an inverse distance squared formula. Some of Kepler's laws however are the result of a more general force formula. This material is to derive those properties of the trajectories of particles moving in a force field that depend only on the force acting centrally.
If the force on a particle depends only upon the distance r from the center of the force field then there is spherical symmentry to the system and angular momentum is conserved. Let r and v denote the radial vector and velocity vector, respectively, of the particle. (In the following vectors are depicted in red.) If m is the mass of the particle then its momentum p is equal to mv. The angular momentum M of the particle with respect to the center of the force field is given by
Since
r and p must always be perpendicular to M. If M≠0 then r and p must lie in the plane whose normals are parallel to M and passes through the center of the force field.
This means the analysis can be restricted to the plane. The origin of the coordinate system may be taken to be at the center of the force field. The trajectory of the particle can be represented by the radial vectors and these are completely described by their magnitude r and an angle θ.
Let r^ and θ^ be the unit vectors in the increasing r and θ directions, respectively. The velocity of the paricle is then
Since r^ and θ^ are perpendicular the squared magnitude of velocity is
This means that the kinetic energy K of the particle is
If the potential energy of the particle is denoted as V(r) then the total energy E of the particle is
The angular momentum of the particle with respect to the center of the force field is mr²(dθ/dt) and this remains constant; i.e.,
Since the mass m is constant this means that r²(dθ/dt) is also constant.
Now consider the area swept out by the radial vector as the particle moves, as shown below
Thus the rate at which area is swept by the radial vector is equal to r²(dθ/dt) which was found to be constant as a result of the conservation of angular moment. Therefore the rate at which area is swept out is everywhere constant along the trajectory of the particle as a result of the conservation of its angular momentum moving in a central force field. This is Kepler's Second Law of planetary motion.
The angular momnetum of the particle with respect to the center of the force field is constant. Let this constant be denoted as q. Thus
This latter equation can be solved for (dr/dt); i.e.,
Since (dθ/dt) = q/(mr²) this means (dt/dθ) = mr²/q. Therefore
Given the formula for V(r) the above equation may be integrated to give θ in terms of r and hence, in principle, r in terms of θ. This would be the equation of the orbit of the particle.
The integration can be carried out only over the range in which the expression in the denominator is positive. The limits of integration are given as the solutions to the equation
The coordinate system can be oriented so that θ=0 corresponds to the smallest root of the above equation.
(To be continued.)
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