Monday, January 16, 2012

Lesson 22 The Kepler Problem

Kepler's three laws describe the motion of the planets, but Isaac Newton's explanation of these laws was the culmination of the Scientific Revolution.

Isaac Newton hypothesized that the force of gravity gave rise to elliptical orbits:

F = -D/r^2(r^) - inverse square law of gravity

F = m a

m a = -D/r^2(r^)

a = -D/Mr^2 (r^)

d^2r/dt^2 = -D/Mr^2 (r^) - differential equation of any orbit because the solution is the algebraic equation of any conic section.

r = L^2/DM/ 1+ecos(theta)
Twist or torque cannot be applied by gravity rxF =0

F= m a

r x m a = 0

m r x a = 0

m r x dv/dt = 0

d(r x v) = dr/dt x v + r x dv/dt
dt

=v x v + r x dv/dt

d(r x v) = r x dv/dt
dt

m d(r x v) = 0
    dt

Zero torque, together with Newton's second law leads to a differential equation to be integrated.

integral(d(mr x v)) = 0
             dt
mr x v = L

When there is no torque a certain quantity is constant called angular momentum.

A planet orbiting with constant angular momentum stays in a single plane with orbital speed varying in a precisely determined way. The area swept out by its radius vector changes at a constant rate (Kepler's second law).

da/dt = (1/2) r x v

This is easily determined in polar coordinates where da/dt = 1/2r^2 d(theta)/dt k^ including planets moving in an ellipse under Newton's Universal Law of Gravity.


F = -G M M(o)/r^2 (r^)
   = -D/r^2 (r^)

F = m a

a = -D/Mr^2 (r^)
                                                    >Cross these vectors
L = Mr^2 d(theta)/dt (k^)

a x L = -D/Mr^2 (r^) x Mr^2 d(theta)/dt (k^)

d(v x L) = D dr^
dt                  dt

v x L = D (r^ + e)

The orbit of heavens described by the perfect circle of underlying geometry. Product of these events:

r . v x L = Dr1 (r^ + e)

r x v . L = D r . (r^ + e)

Once order is exchanged, and mass allowed its play

L^2/M = Dr . (r^ + e)

L^2/DM = r . (r^ + e)

L^2/DM = (r . r^ + r . e)
               = (r + recos(theta))

r = L^2/DM                     -conic section algebraic equation.
      1 + ecos(theta)

The force of gravity moves all heavenly bodies along conic sections.

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