Physics 101- Introduction to Mechanics
|April 19- Angular Momentum II|
of Conservation of Angular Momentum
Ice Skating/ Dancing
Bicycles & Gyroscopes
Why is it so easy to maintain your balance on a moving
bicycle, but not on a stationary one?
Second law is simply conservation of angular momentum. That's it.
This can be restated in terms of the area
swept out (dA) in some time interval (dt).
The area of the triangle can be found by taking 1/2 of the parallelogram's area-
dA= 1/2 R * v dt
By using the definition of angular momentum (of a point particle) we can rewrite the triangle's area as-
dA= L/ 2m dt
dA/ dt= L/ 2m= constant
Angular momentum has to be conserved as
we only have a central force acting on the orbitting body (it cannot exert
a torque), so the body sweeps out equal areas in equal time intervals.
Kepler's second law implies that as a planet's distance from the sun increases in an elliptical orbit, its orbital speed
When the density of matter gets cosmically extreme, weird stuff happens. One place where matter can get this compressed is in the interior of dying highly massive stars. As heavier and heavier elements fuse in the compacted cores of old red supergiants, the core begins to collaspe and eventually falls in on itself, exploding violently in a supernova. Often, the core remaining after the explosion can be so extremely compacted that it is completely made of neutrons. These insanely dense neutron stars pack the mass of our Sun into a diameter of 30 km, the size of San Diego. One Dixie cup full of neutron star stuff would weigh around 200 million tons on Earth.
These stars also have intense magnetic fields which
accelerate the electrons which remain in the surrounding gas. Once
the electrons reach a speed near that of light, they must radiate off some
of their energy, usually as radio waves or X-rays. These radio waves
are emitted only near the magnetic poles of the star, essentially as two
beams in opposite directions. But,... these stars are rotating at
very high rates, so what we see are pulses of the waves, just like a lighthouse's
beam that is swept around in circle leaving us to only see pulses of light.
About the Course
Homework- assignments & solutions
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