AN INTRODUCTION TO
NEWTONIAN MECHANICS by Edward Kluk Dickinson State University, Dickinson ND |
NEWTON SECOND LAW
Definition of gravitational mass and how to
compare forces
This time we are facing a
very formidable task to analyse and truly understand
Newton laws of motion. In a process of doing it a few new ideas
and related to them operational definitions must be established.
These definitions will enable us to measure magnitudes which are
characterizing quantitatively mentioned ideas.
Long before Newton people
were measuring, with help of simple two plate symmetric or
spring balances, gravity forces that are pulling bodies down
toward the center of Earth . Such measurements were mostly done
for commercial purposes to compare amounts of
matter, scientifically called masses, with
certain standards. In 1790 Paris Academy of Science established a
standard of mass called 1 kilogram (1 kg) which is still
used in International System of Units (SI). If a certain body
placed on one plate of the balance needs to be equilibrated by
two copies of 1 kg standard placed on the other plate, its mass
is 2 kg. Moreover, the gravity force acting on this body is
two times greater than the gravity force acting on 1 kg standard
mass. In every day language these forces are called weights
and the measuring process is called weighing. In this
scheme masses and weights are evidently proportional. But exact
relation between them (a coefficient of proportionality) is still
missing. There is one more interesting thing. If an object is
moved from the surface of Earth to the surface of another planet
its weight will be different because a gravity force exerted by
the planet on the object will be different. Its mass, however,
will stay the same. For example, 2 kg object on the other planet
must still be equilibrated on the two plate balance by two copies
of 1 kg mass standard. This is why the idea of mass is more
generic than the idea of weight. But comparing masses of other
bodies with use of balances we are always employing gravitational
forces. This is why such masses should be called gravitational
masses. Later on you will learn why we do not use the added
adjective too often. Now, try to figure out on your own why all
these ideas are still working if a good spring balance is used.
The good spring balance must have the spring which elongates
proportionally to the applied force. Notice that using springs we
can compare magnitudes of other forces to magnitudes of
gravitational forces. For example, attach one end of an exercise
spring to the ceiling and stretch it 0.2 m by pulling it down
with your arm. Now, instead of stretching it yourself, hang on it
such amount of mass which will stretch it 0.2 m. The gravity
force acting on this mass must than be equal to the force you
were exerting on the spring.
Newtonian calculus
Our investigation of
rectilinear motion on a horizontal frictionless plane let us
conclude that if a body is left alone (no a net force is acting
upon the body) it moves with constant velocity. If the body stays
at rest this constant velocity is equal to zero . So far we have
learned how to compare forces and we can measure their relative
magnitudes. We also know that forces are influencing body's
motion. But we do not know any quantitative relations between the
body's motion and applied forces. This situation will change as
soon as Newton second law is introduced. A meaningfull
introduction of it, however, is not possible without a little bit
more sophisticated algebra. Limiting our discussion to 1D motion
of a point like body along x axis we can mark a
current position of the body at time t as x(t).
Traditionally a small change of any variable is denoted with help
of capital greek letter "delta" which looks like an
equilateral triangle. Unfortunately HTML in its current form does
not allow this kind of letter. Therefore it will be replaced by D.
Consequently Dt will represent a small change of
time and Dx(t) = x(t) - x(t - Dt) a small change of
x that takes place in the time interval (t, t - Dt).
The same kind of notation will be applied to other variables
which are dependent on time. Right now it is not difficult to
notice that Dx(t) / Dt represents a
rate of change of body's position or a body's velocity. Assuming Dt
positive, if Dx(t) is positive the
velocity is positive too, and the body at this particular instant
t moves in the positive direction of
x axis. If Dx(t) is negative
then the velocity is negative too and body moves in the negative
direction of x axis. Understanding of this
kind of math is very important for our further discussion.
Formulation of the second law and problem of
inertial mass
As we already have noticed
a change of body's velocity demands application of a force.
More massive is the body more force is needed to induce the same
change in its velocity. The resistance of the body against a
change of its velocity is called the body's inertia. Notice that
the body's inertia may have nothing to do with body's
gravitational mass. The last demonstrates itself and can be
measured only if the body is under influence of a gravitational
force. The body's inertia demonstrates itself always in this
senese that body's velocity cannot be changed without application
of a force or inducting a change of its inertia. For sake of
simplicity we will discuss here only bodies with constant
inertia. Following Newton let introduce another idea which he
called an amount of body's motion. Now it is known as a
body's momentum p(t) and defined as
a product of body's inertial mass mI
and its velocity v(t). Thus we may write
p(t) = mI v(t) .
Newton proposed that a rate of change of momentum Dp(t)/Dt should be equal to the force F(t) acting upon the body which we can write as
Dp(t)/Dt = F(t) .
This formula represents Newton second law in its original formulation. In most of practical cases an inertial mass of the body is constant then it does not depend on time. Consequently
Dp(t) = p(t) - p(t - Dt) = mI v(t) - mI v(t - Dt) = mI [v(t) - v(t - Dt)] = mI Dv(t)
which leads to more popular form of Newton second law
mI Dv(t)/Dt = F(t) or mI a(t) = F(t)
where a(t) is a rate of change of velocity or a body's acceleration. It is very important to realize that the second law does not define force or inertial mass. But it makes possible to predict the motion if the force, inertial mass and some initial conditions for this motion are known. Another important and unsolved yet problem represents inertial mass. Formally at this stage we do not know how to measure it.
Solution of the inertial mass
problem
Historically verification
of Newton second law took many years because of lack of proper
technologies and enough advanced mathematics. Remember that to
formulate the second law Newton was forced to invent a calculus
similar to what we are using in our lectures. Latter developed
advanced mathematics helped to confront Newtons second law with
astronomical data and confirm its correctness. In our
verification we will rely mostly on unusual properties of our
fictitious planet like its very low gravity acceleration and lack
of friction. The second law describes correctly motion of a body
if a net force acting upon this body is equal to zero. A zero
force implies a zero acceleration which in turn implies a
constant velocity. In a case of free fall motions
experiments show a constant and equal for everybody acceleration
g. On Earth g is about 9.8 m / s2
and on our strange planet about 0.01 m / s2.
In both cases the second law implies a constant force F =
mI g. On the other
hand we know that this case F is
a gravitational force and then it must be proportional to
the gravitational mass of the body. Consequently for everybody
inertial mass is proportional to its gravitational mass.
Because there are not other constrains on inertial mass it is
very convenient to choose for a proportionality coefficient the
plain number 1. Thus both masses will have the same
units and the same values, but not necessary the same nature.
Additionally, from now on we will skip subscript I used
with inertial mass.
The verifying
"experiment"
Now we know enough about
the second law to verify it "experimentally". The
"experimental" set contains (see the applet above):
the block of mass mB which can slide on the frictionless horizontal surface
the hanger of mass mH connected with the block with help of massless string running through the pulley
the pulley which will not rotate because there is not friction between the pulley and the string.
We will investigate motion of the
system containing the block, hanger and string. A total mass of
the system m = mB +
mH will be
kept constant. If we let it go, the system will move with a
constant acceleration caused by a constant gravitational force
F acting on the hanger. Knowing the hanger mass we can
find this force as F = mH g
. Remember you are on the surface of the strange planet,
not Earth. Timing the block or hanger every two meters and making
the graph of the travelled distance versus t2
we can find the system acceleration exactly the same way as we
did it for the free fall motion. Remember to include into your
graph the point t = 0 with the travelled
distance also equal to zero.
If you are already
convinced about constant acceleration of the system the
"experiment" could be simplified. Just measuring only
a flight time of the block from 0 m to 8 m and using an
appropriate formula we could calculate an acceleration. Please
avoid this simplification and time the block or hanger every two
meters because the collected data will be used again for the
study of system mechanical energy.
For each consecutive run a
portion of mass should be moved from the block to the hanger. It
will increase the force F running the system ,
without changing the total mass of the system. When enough data
pairs force - acceleration are collected than a graph
force vs. acceleration can be made. As the total mass of the
system was kept constant, then according to the second law this
graph should be a straight line through (0,0) point and its slope
should be equal to the total mass of the system. If you
understand the idea of this "experiment " go ahead find
a partner and make it. It is easier for two people to make the
"experiment". One person shall observe the block or
hanger and signal when to read the time, whereas the other person
shall read and record the time. Make all graphing and
calculations needed to verify the second law. Compare the
inertial mass of the system recovered from the slope on the graph
force vs. acceleration with the real mass of the system. They
should not differ more than 5%. Any discrepancy between them is
related to both experimental errors in time and distance
measurements and imperfectness of graphing.
Please save all the data related to this "experiment" because they will be used again in conjunction with mechanical energy problems.
Short epilogue
Laws formulated by
scientists have their limitations. That means they apply only
under certain conditions and if these conditions are not met they
do not work. To make them work with less restrictive conditions
they have to be generalized. If Newton second law were exact for
bodies on and around Earth we would not have stationary
satellites nor hurricanes. Shortly you will learn about the
second law limitations.
Evaluation
If at this point you can
solve the following problems:
the objectives of this lesson are fully achieved. If you have doubts try to read it once more concentrating on them, but do not try to memorize this text. Physics is not about memorizing, it is about understanding.
Last update: Jan 10, 1997 | E - mail to Edward Kluk |
Copyright (c) 1996 Edward Kluk |