That requirement brings us back to Mr.
Newton. The story goes that he observed an apple falling from a
tree and at the same time noticed the moon, also up in sky but
not falling to Earth. The difference, he might have decided, was
that the moon had some sideways (tangential) velocity whereas the
apple did not.
The apple orbit, at least that part of it which was observable, appears to be a straight line. We know that in the case of simple harmonic motion a linear "orbit" is possible. Just look at the combined SHM display with the x and y parameters identical. It turns out that a linear orbit is also possible with an inverse square type central force. Unfortunately in the apple situation the orbit was interrupted by a collision with the surface of the planet. If it were possible for a hole to be drilled through the entire earth, an apple or anything else falling into that hole would oscillate back and forth along a diameter of the planet.
One of Newton's major contributions to science was to come up with one law of nature which could explain the behavior of both the apple and the moon. By the way, he had to invent calculus along the way to accomplish this feat. What he concluded was that any two bodies are attracted to each other in a way which is quantified by a simple law called the law of "universal gravitation". That law says that the attractive force between a pair of objects is proportional to the product of their masses divided by the square of the distance between their centers of mass. The force on the two objects is an action-reaction pair in that they are equal and directed oppositely.
The law of universal gravitation is writtenFor convenience let's replace G * m1 * m2, with a constant k since for a given system they are all constant. So
Obviously as r increases, the force gets weaker and weaker, dropping to zero at infinite r. As r approaches zero the force approaches infinity but this is not a problem since all real masses have some size to them so that the particles will collide before the distance between centers can get too small. In fact if it were possible for objects to pass through one another, the force drops off once the one object penetrates the other since the mass outside the distance between the two centers can be shown to make no contribution to the force. {Think about this one a bit!}
Of course, the y component of force
behaves the same way along its dimension as the x does along its.
So we find that the motion component along the x and y axes are
oscillatory, but certainly not SHM since the magnitude of the
force is not directly proportional to the displacement but to the
reciprocal of displacement squared. To see how a simple harmonic
oscillator's position vs time graph compares to one of an
object subject to an inverse square type central force, run the
Gravity and SHM display. In the
inverse square law part of this display, we assume that the
moving object can pass through the object creating the central
force so that a linear orbit is possible, allowing a direct
comparison with the linear SHM.
Notice that the inverse square central force produces a waveform that is generally broader near the peaks and steeper at the crossing of the axis than that produced by the directly proportional force. The mathematical form of the spring like force waveform is just the cosine function. The mathematical form of the inverse square force waveform is an infinite series of sine and cosine terms.
One way to model the motion of a particle subject to a central force like gravity might be to treat the x and y components as separate oscillators as we did in converting SHM to circular motion. This idea has two drawbacks. First, since the oscillatory motion is not simple harmonic, initial conditions affect not only the phase angle but the frequency. Second, the model is very sensitive to the magnitude of the time increment, D t and becomes unstable if D t is not small enough. Besides these technical difficulties, our everyday experience with gravity makes it feel like a force so we will go back to Newton's second law to model gravitational attraction.
First we will look at a strictly made up situation. We want to predict the future of a something the mass of a hamburger in orbit around something the mass of a sports car in a universe where the gravitational constant is 1.0. This is essentially the situation set up in the next display called Orbital Vibrations. Here we will see a relatively light object interacting with an object of more mass but still movable. The display is a three dimensional one but looking at the (x,y) plane edgewise along the x axis.
We will consider our objects in this
model to be spherical so the force of gravity is spherically
symmetric. Otherwise the math is too hard for me. With a
spherically symmetric force, the orbits will lie in a plane
determined by the initial position and velocities. I chose the
initial conditions so the (x,y) plane contains the orbit. Due to
this symmetry property of the gravitational field, later we will
often use two dimensional displays for two-body interactions.
The size of the objects on the display is somewhat related to mass but the smaller object is kept big enough so you can see it. Notice that motion of our quarter pounder sort of fits the description of vibration which we discussed in the previous section. It dithers around in the vicinity of the heavier mass. The blue mass by the way appears transparent to the green one in this display. Notice that the oscillations while symmetrical in space are not symmetrical in time. The green mass goes faster when moving to the left than when to the right. Run the Orbital Vibrations display.
Unlike the uniform circular motion we observed in combining simple harmonic vibrations, the orbital speed in a gravitational field changes noticeably in different parts of the orbit. Remember the conservation of angular momentum? Angular momentum, L, was defined as rXp where r was the position vector of the object and p was the linear momentum vector. But p is the mass times the velocity v so
Now let's take a look at an example
with more realistic values. We will show in the Satellite Orbit display, the Earth with its
true radius and mass, and give you an opportunity to place a
satellite in orbit at any altitude and with a velocity you set.
Then you can observe the orbit produced by your choices. The
distances will be in kilometers and the velocities will be in
meters per second in this display.
Next we will look at the work and energy aspects of gravity. In the section on work and kinetic energy we introduced the notion of work done against the force of gravity and in the section on potential energy and fields we described a scalar potential field due to gravity. In that case we were talking about the approximation where the force of gravity was constant in space. Now we know more about how gravity depends on position so let's work out what the scalar potential field would be like in the vicinity of a large object, like the Earth.
Remember that we can only
assign a specific potential energy to each point in space if the
forces involved are
conservative in nature. To demonstrate that the force of
gravity is conservative consider two points out in space and a
small test mass moving from one to the other along some arbitrary
path. Any point on that path may be reached from any other point
by a combination of motion along a circular arc centered on the
origin, and motion along a radius from the origin. Look at the Conservative Central Force display for an
illustration.
Pay close attention to the accumulation of minus sign in the discussion above. We got one because the change in pe is the negative of the work done by gravity. We got one because the gravitational force is directed opposite to the radius vector. And we got one because the anti-derivative required dividing by minus one.
There is an implicit assumption in taking the potential energy to be the negative of the work done by gravity and that is that the zero of potential energy is at infinite displacement. That makes intuitive sense since the force goes to zero at that distance. Remember that we can make an arbitrary choice where we want potential energy zero to be since we always deal in changes. Customarily the for gravitational potential energy, it is in fact chosen to be at infinity.
Notice that the gravitational potential energy goes to -infinity as the distance to the center goes to zero. This makes physicists nervous. We do not like our natural laws to have singularities (blow up) unless it happens way out at infinity where it is not going to bother anyone. For ordinary sized objects, we found a way to wiggle out of this difficulty by noticing that objects will collide before the distance between their centers goes to zero and a different force law applies in a collision. Suppose however we have a planet sized object with a hole drilled through its center. The center of mass of that object will lie in the middle of this drilled passage and thus be accessible to another object dropped into the hole. Under this scenario, the centers of mass of the drilled object and the dropped object could coincide.
What is the potential energy of our
system when one of the objects gets inside the other? Without
spending a lot of time on this I will give what is called a
plausibility argument that the gravitational force exerted on a
mass inside a spherical shell by the shell itself is zero.
Consider a situation where the mass is at the center of the shell
centered on the origin of our reference frame. The force exerted
by every little D m of mass in the
shell would be exactly cancelled by the same amount of mass on
the opposite side of the shell, so in the case of a centered
object the gravitational force from the spherical shell is
clearly zero. For the next part of the discussion refer to the Spherical Shell display.
While we are dealing
with this little make believe two body system, we should also look at the kinetic
energy and total energy of the system as the red object goes along its path. Remember
that kinetic energy is 1/2 * m v2. If both objects were moving in the
reference frame the kinetic energy of the system would be the sum of that expression
for each object. In our system only one object is moving. The total energy then
is
The
potential energy field goes to zero at infinity and produces a
force that attracts the moving object to the origin of the
reference frame. The kinetic energy is a measure of the moving
object's ability to overcome this attractive force. As the
object becomes more distant from the origin, the potential energy
increases (becomes less negative) and the kinetic energy
decreases. If we run out of kinetic energy before the potential
energy gets up to zero, the object is held captive by the
gravitational force and will return to its starting point,
producing a closed orbit. If there is more than enough kinetic
energy to compensate for the negative potential energy, the
object will not be held captive by the gravitational force so the
orbit will be open. Look at the Open
Orbit display to see this.
In the next section of this course we will move on to the study of mechanical waves.