| The Physics of "s is one half 
            gt 2" This song contains five important 
            equations from first-semester physics. The title equation, s 
            = 1/2 gt 2, gives the distance 
            s fallen by an object in a time t, assuming the 
            object starts at rest and that air resistance is negligible; g 
            is the acceleration of gravity, which is about 9.8 m/s2 
            on the surface of the Earth. (Note: for medium to small objects, the 
            force of air resistance becomes important after a drop of 10 meters 
            or less. You might be interested in my answer to the question, "What 
            would happen if you dropped a superball off the Empire State Building".) 
             
              | The second equation in the song, PV= 
                nRT is the "ideal gas law". It gives the relationship 
                between the pressure P, the volume V, the number 
                of moles n, and the temperature (measured from absolute 
                zero) T of any gas, with the assumptions that the gas 
                molecules only interact with each other in very short collisions, 
                and that the volume of the gas molecules themselves is negligible 
                compared to the total volume occupied by the gas. The constant 
                R  is the "ideal gas constant", which equals 
                8.31 J/mol K. The equation says that, if you start with a given 
                container filled with gas, you can increase the pressure either 
                by 1) adding more gas (increasing n), 2) heating the 
                gas (increasing T), or 3) squeezing the container to 
                a smaller volume (decreasing V). (Note: the "number 
                of moles" is equal to the number of gas molecules divided 
                by Avogadro's number, 6.02 x 1023.) Perhaps the most 
                remarkable thing about this equation is that the gas pressure 
                doesn't depend on the type of gas -- you would get the same pressure 
                for a given number of oxygen molecules as you would for the same 
                number of helium atoms.) Click the image at right to open a Java 
                applet from Ohio State University that nicely illustrates this 
                law. |  |   
              | The third equation 
                  gives the expression for kinetic energy: KE = 1/2 mv 
                  2, where m is the mass of a moving object and 
                  v is its velocity. Although the idea of energy is so 
                  central to our current understanding of physics, and indeed 
                  the way we think about everyday life and geopolitics, it is 
                  a relatively recent notion. The law of conservation of energy, 
                  i.e. that energy can never be destroyed, but only transformed 
                  from one form to another, was initially obscured by the common 
                  observation that things that move usually eventually come to 
                  rest, so that their energy of motion seems to disappear. We 
                  now understand that, when this happens, the kinetic energy is 
                  transformed into thermal energy through friction. However, it 
                  was not until experiments performed by the brewer James P. Joule 
                  in the early 1840s that this really became clear, and it took 
                  many years after that for the idea of energy conservation to 
                  be widely accepted in the scientific community. Read 
                  more about the history of energy here. 
 |  |   
              | The fourth equation 
                  in the song gives the formula for the period (the time for a 
                  complete swing back and forth) of a pendulum:  . 
                  Here L is the length of the pendulum, and g 
                  is the acceleration of gravity, which is about 9.8 m/s2 
                  on the surface of the Earth. There are two astonishing things 
                  about this equation: 1) The period of the pendulum doesn't depend 
                  on the mass of the pendulum bob (the weight at the end of the 
                  pendulum)! 2) The period doesn't depend on the amplitude of 
                  swinging. In other words, the period is the same when the pendulum 
                  is swinging back and forth only a tiny amount as when its swinging 
                  more vigorously. (In fact, this equation only works well for 
                  moderate or small amplitude swings, say less than 30 degrees 
                  back and forth.) There is a wonderful 
                  legend (apocryphal, but so what) of how Galileo discovered the 
                  lack of dependence on amplitude: "Galileo was bored. As 
                  he listened to a Mass in the drafty cathedral of Pisa in 1581, 
                  the 17-year-old student noticed something interesting. A chandelier 
                  high overhead was swaying in the breeze, sometimes barely moving 
                  and other times swinging in a wide arc. His curiosity aroused, 
                  he timed the swings with his pulse. To his surprise, it took 
                  the same number of pulse beats for the chandelier to complete 
                  one swing no matter how far it moved. The wider the swing, the 
                  faster the motion, but always in the same amount of time. So 
                  time could be measured by the swing of a pendulum -- the basis 
                  for the pendulum clock."1  The pendulum, of course, 
                  was then used to construct the first accurate clocks, which 
                  were eventually adapted for use at sea, allowing accurate navigation. |  Galileo
 1564-1642
 
 |  
              | The last equation in the song is 
                  Newton's second law, "force is mass times acceleration", 
                  or F = ma. This equation is really the definition 
                  of force: a force is something that, when applied to a body 
                  of mass m produces an acceleration a.  In one of the best parts of the song, 
                  the professor goes on to say, "or more precisely the time 
                  derivative of the linear momentum". In fact, this is the 
                  way Newton originally stated the law -- his wording was, "The 
                  net force acting on a body is equal to the rate at which the 
                  body's quantity of motion is changing." What he called 
                  "quantity of motion" is what we now call "linear 
                  momentum" (linear as opposed to angular momentum); it is 
                  usually assigned the symbol p, and is given by p 
                  = mv.  We can easily see that the two ways 
                  of stating Newton's second law are equivalent. ("There 
                  he goes again!") The "rate of change of " (equivalently 
                  "time derivative of") the momentum is written  , 
                  so that Newton's second law in his original version would be  . 
                  Since, for most situations, the mass of the accelerating object 
                  doesn't change, we can rewrite this as  . 
                  Finally, the acceleration 
                  is the time derivative (i.e. the rate of change) of the velocity:  , 
                  so  . Usually, the familiar F = 
                  ma form is more convenient. However, the original form, 
                   is important for developing the idea of "impulse", 
                  which is useful for analyzing collisions. --WFS 8/28/05 |  |  References: 1 
            - Prof. Roger Newton, author of Galileo's Pendulum (Harvard 
            University Press, 2004) Back to "s 
            is one half gt 2"main page Back to "The 
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