Michael Fowler

*University of Virginia*

Index of Lectures and Overview of the Course

Link to Previous Lecture

Let us consider first the simple case of a car moving at a *steady speed down a straight road*. Once we've agreed on the units we are using to measure speed---such as miles per hour or meters per second, or whatever---a simple number, such as 55 (mph), tells us all there is to say in describing steady speed motion. Well, actually, this is not quite all---it doesn't tell us which way (east or west, say) the car is moving. For some purposes, such as figuring gas consumption, this is irrelevant, but if the aim of the trip is to get somewhere, as opposed to just driving around, it is useful to know the direction as well as the speed.

To convey the *direction* as well as the speed, physicists make a distinction between two words that mean the same thing in everyday life: *speed* and *velocity*.

*Speed*, in physics jargon, keeps its ordinary meaning---it is simply a measure of *how fast something's moving*, and gives *no clue about* which *direction* it's moving in.

*Velocity*, on the other hand, in physics jargon *includes direction*. For motion along a straight line, velocity can be positive or negative. For a given situation, such as Charlottesville to Richmond, we have to agree beforehand that one particular direction, such as away from Charlottesville, counts as positive, so motion towards Charlottesville would then always be at a *negative* velocity (but, of course, a positive *speed*, since speed is always positive, or zero).

Now think about how you would describe quantitatively the motion of a smooth ball rolling steadily on a flat smooth tabletop (so frictional effects are negligible, and we can take the speed to be constant). Obviously, the first thing to specify is the speed---how fast is it moving, say in meters per second? But next, we have to tackle how to give its *direction* of motion, and just positive or negative won't do, since it could be moving at any angle to the table edge.

One approach to describing uniform motion in the plane is a sort of simplified version of Galileo's "compound motion" analysis of projectiles. One can think of the motion of the ball rolling steadily across the table as being compounded of two motions, one a steady rolling parallel to the *length* of the table, the other a steady rolling parallel to the *width* of the table. For example, one could say that in its steady motion the ball is proceeding at a steady four meters per second along the length of the table, and, at the same time, it is proceeding at a speed of three meters per second parallel to the width of the table (this is a big table!). To visualize what this means, think about where the ball is at some instant, then where it is one second later. It will have moved four meters along the length of the table, and also three meters along the width. How far did it actually move? And in what direction?

We can see that if the ball's uniform motion is compounded of a steady velocity of 4 meters per second parallel to the length of the table and a steady velocity of 3 meters per second parallel to the width, as shown above, the actual distance the ball moves in one second is 5 meters (remembering Pythagoras' theorem, and in particular that a right angled triangle with the two shorter sides 3 and 4 has the longest side 5---we chose these numbers to make it easy). That is to say, the *speed *of the ball is 5 meters per second.

What, exactly, is its *velocity*? As stated above, the velocity includes both *speed* and *direction* of motion. *The simplest and most natural way to represent direction is with an arrow*. So, we represent velocity by drawing an arrow in the plane indicating the direction the ball is rolling in. We can see on the above representation of a table that this is the direction of the slanting line arrow, which showed from where to where the ball moved in one second, obviously in the direction of its velocity. Hence, we represent the direction of the velocity by drawing an arrow pointing in that direction.

We can make the arrow represent the speed, as well, by agreeing on a rule for its length, such as an arrow 1 cm long corresponds to a speed of 1 meter per second, one 2 cm long represents 2 meters per second, etc. These arrows are usually called *vectors*.

Let us agree that we represent velocities for the moment by arrows pointing in the direction of motion, and an arrow 2 cm long corresponds to a speed of 1 meter per second. Then the velocity of the ball, which is 5 meters per second in the direction of the slanting arrow above, is in fact represented quantitatively by that arrow, since it has the right length---10 cms. Recalling that we began by saying the ball had a velocity 4 meters per second parallel to the length of the table, and 3 meters per second parallel to the width, we notice from the figure that these individual velocities, which have to be added together to give the total velocity, can themselves be represented by arrows (or vectors), and, in fact, are represented by the horizontal and vertical arrows in the figure. All we are saying here is that the arrows showing how far the ball moves in a given direction in one second also represent its velocity in that direction, because for uniform motion velocity just means how far something moves in one second.

The total velocity of 5 meters per second in the direction of the dashed arrow can then be thought of as the sum of the two velocities of 4 meters per second parallel to the length and 3 meters per second parallel to the width. Of course, the *speeds* don't add.

Staring at the figure, we see *the way to add these vectors is to place the tail of one of them at the head of the other, then the sum is given by the vector from the other tail to the other head*. In other words, putting the two vectors together to form two sides of a triangle with the arrows pointing around the triangle the same way, the sum of them is represented by the third side of the triangle, but with the arrow pointing the other way.

As we shall see, relative velocities play an important role in relativity, so it is important to have a clear understanding of this concept. As an example, consider a child running at 3 meters per second (about 6 mph) in a train. The child is running parallel to the length of the train, towards the front, and the train is moving down the track at 30 meters per second. What is the child's velocity relative to the ground? It is 33 meters per second in the direction the train is moving along the track (notice we always specify *direction* for a velocity). To really nail this down, you should think through just how far the child moves relative to the ground in one second---three meters closer to the front of the train, and the train has covered 30 meters of ground.

A trickier point arises if the child is running across the train, from one side to the other. (This run will only last about one second!) Again, the way to find the child's velocity relative to the ground is to visualize how much ground the child covers in one second---three meters in the direction across the track, from one side to the other, plus thirty meters in the direction along the track. To find the total velocity, we now have to add two velocities at right angles, using the "head to tail" rule for adding vectors. This is just the same problem as the ball rolling across the table at an angle discussed above, and we need to use Pythagoras' theorem to find the child's speed relative to the ground.

Here is another example of vector addition, this time the two vectors to be added are not perpendicular to each other, but the same rules apply:

So in the diagram above, the two vectors on the left add to give the vector on the right. (We are just using a dashed line for one of them so you can see what's going on in the middle, usually all vectors are represented by solid lines.) To get a bit less abstract, this could represent relative velocity in the following way: the big arrow on the left might be the speed at which a person is swimming relative to water in a river, the little arrow is the velocity at which the river water is moving over the river bed. then the vector sum of these two represents the velocity of our swimmer relative to the river bed, which is what counts for actually getting somewhere!

We restrict our considerations here to an object, such as an oxcart, moving in a horizontal plane. Aristotle would say (with some justification) that it moves in the direction it's being pushed (or pulled), and with a speed proportional to the force being applied. Let us think about that in terms of vectors. He is saying that the magnitude of the velocity of the object is proportional to the applied force, and the direction of the velocity is the direction of the applied force. We see right away that not only is the velocity a vector, but so is the applied force! Of course, this is obvious really---the applied force certainly has magnitude (how hard are we pushing?) and direction, and can be represented by an arrow (we would have to figure out some units of force if we want the length to represent force quantitatively---we will come back to this later).

So **Aristotle's rule for horizontal motion** is: *velocity is proportional to applied force*, where *both are vectors*.

This rule seems to work well for oxcarts, but doesn't make much sense for our ball rolling across a smooth table, where, after the initial shove, there is* no* applied force in the direction of motion.

Galileo's Law of Horizontal Motion can be deduced from his statement near the beginning of Fourth day in Two New Sciences,

*Imagine any particle projected along a horizontal plane without friction; then we know ... that this particle will move along this same plane with a motion which is uniform and perpetual, provided the plane has no limits.*

So **Galileo's rule for horizontal motion** is: *velocity = constant*, provided* no force*, including friction, acts on the body.

The big advance from Aristotle here is Galileo's realization that* friction is an important part of what's going on*. He knows that if there were no friction, the ball would keep at a steady velocity. The reason Aristotle thought it was necessary to apply a force to maintain constant velocity was that he failed to identify the role of friction, and to realize that the force applied to maintain constant velocity was just balancing the frictional loss. In contrast, Galileo realized the friction acted as a drag force on the ball, and the external force necessary to maintain constant motion just balanced this frictional drag force, so there was no *total *horizontal force on the ball.

As we have already discussed at length, Galileo's Law of Vertical Motion is:

For **vertical motion**: acceleration = constant (neglecting air resistance, etc.)

As an exercise in using vectors to represent velocities, consider the velocity of a cannonball shot horizontally at 100 meters per second from the top of a cliff: what is the velocity after 1, 2, 3 seconds? As usual, neglect air resistance.

The initial velocity is represented by a horizontal arrow, which we take to be 10 cms long, for convenience:

------------------------------------------------------------------->

After one second, the downward velocity will have increased from zero to 10 meters per second, as usual for a falling body. Thus, to find the total velocity after one second, we need to add to the initial velocity, the vector above, a vertically downward vector of length 1 cm, to give the right scale:

It is worth noting that although the velocity has visibly changed in this first second, the speed has hardly changed at all---remember the speed is represented by the length of the slanting vector, which from Pythagoras' theorem is the square root of 101 cms long, or about 10.05 cms, a very tiny change. The velocity after two seconds would be given by adding two of the dashed downward arrows head-to-tail to the initial horizontal arrow, and so on, so that after ten seconds, if the cliff were high enough, the velocity would be pointing downwards at an angle of 45 degrees, and the speed by this point would have increased substantially.

Galileo defined naturally accelerated motion as downward motion in which speed increased at a steady rate, giving rise to units for acceleration that look like a misprint, such as 10 meters per second per second.

In everyday life, this is just what acceleration means---how fast something's picking up speed.

However, in physics jargon, acceleration (like velocity) has a more subtle meaning: *the acceleration of an object is its rate of change of velocity*. From now on, this is what we mean when we say acceleration.

At first this might seem to you a nitpicking change of definition---but it isn't. Remember velocity is a *vector*. *It can change without its length changing*---it could just swing around and point in a different direction. This means a body can accelerate *without *changing speed!

Why would we want to define acceleration in such a nonintuitive way? It almost seems as if we are trying to make things difficult! It turns out that our new definition is what Galileo might call the *natural* definition of acceleration. In the true laws of motion that describe things that happen in the universe, as we shall discuss below, if a body has a net force acting on it, it accelerates. But it doesn't necessarily change speed---it might just swing its velocity around, in other words veer off in a different direction. Therefore, as we shall see, this new definition of acceleration is what we need to describe the real world.

For motion in a straight line, our definition is the same as Galileo's---we agree, for example, that the acceleration of a falling body is 10 meters per second per second downwards.

Written material Copyright © Michael Fowler 1995 except where otherwise noted.

**NOTE**: the next topics covered in the course are the contributions of two very colorful characters, Tycho Brahe and Johannes Kepler. I gave a more complete account of these two and their works in an earlier version of this course. If you would like to read the more complete (and more interesting) version, click on Tycho Brahe.