Galileo was probably the first to look closely at the way objects fell down to Earth. Legend has it that he climbed to the top of the leaning tower of Pisa and from there dropped simultaneously heavy and light balls, noting that they hit the ground at the same time. He thus demonstrated, contrary to some ancient claims, that heavy and light objects ("bodies") fell at the same rate. Galileo's studies created great interest, because they applied not only to simple falls--such as the fall of an apple from a tree, said to have inspired Newton--but were also relevant to the very practical subject of the trajectory of cannonballs.

## Acceleration

A dropped object starts its fall quite slowly, but then steadily increases its velocity--**accelerates**--as
time goes on. Galileo showed that (ignoring air resistance) heavy and
light objects **accelerated** at the same constant rate as they
fell, that is, their speed (or "**velocity**") increased at a
constant rate. The velocity of a ball dropped from a high place increases
each second by a constant amount, usually denoted by the small letter *g*
(for gravity). In modern units (using the convention of algebra,
that symbols or numbers standing next to each other are understood to
be multiplied) its velocity is

at the start-- **0** (zero)

after 1 second-- **g** meters/second

after 2 seconds-- **2g** meters/second

after 3 seconds-- **3g** meters/second

and so on. This is modified by the resistance of the air, which becomes important
at higher speeds and usually sets an upper limit ("terminal velocity") to the
fall velocity--a much smaller limit for someone using a parachute than one
falling without.

The number **g** is close to 10--more precisely,
9.79 at the equator, 9.83 at the pole, and intermediate
values in between--and
is known as "**the acceleration due to gravity**." If
the velocity increases by 9.81 m/s each second (a good average value),
**g** is said to equal "9.81 meters per second per second" or in
short 9.81 m/s^{2}.

## Adding an Initial Velocity

Suppose the ball was given an **initial velocity ***u *upwards
or **downwards**. If distances **down** are chosen as positive,
the velocity due to gravity will always be positive, while *u*
will be positive if directed downwards, negative if upwards.

With this provision, observations show that *u* must be
added everywhere to the velocity due to gravity, making the velocity in
consecutive seconds (as in the list above)

**u, u+g, u+2g, u+3g** . . .

and
in general, after *t* seconds, with **gt** meaning
**g** times **t**" **u + gt**.
## The Distance Covered

The distance covered by the ball can be shown to be the same as the
one covered if the ball has a constant "*mean*" velocity **v**_{
(mean)}, equal to **half the sum** of the velocities at the
**start** and at the **finish**. For the falling ball in the
preceding example, after *t* seconds that would be

**v**_{(mean)} = (1*/*2)[u + (u+gt)]

making the distance covered

**distance = t v**_{(mean)} = ut + (1*/*2)
gt^{2}

## Galileo's Experiment

The book "The God Particle" by Nobel prize winner Leon Lederman
with Dick Teresi (a good book, if you tolerate its irreverent
attitude and corny humor) tells how Galileo showed that the
downward motion of a ball due to gravity had a constant acceleration,
and that starting from rest (*u = 0*) it covered distances which
increased (as shown in the formula above) in proportion to the
**square** of the time that has passed.

Since a vertical fall was too fast for Galileo to measure
accurately, he slowed it down by making the ball roll down an
inclined board. Across the board, along to its surface, he
strung a number of taut horizontal wires, making the ball sound a click whenever it jumped over one of them. Galileo then moved the wires up and down the board, until the clicks sounded evenly spaced.

If the acceleration now was *a* (much less than *g*) and the time *t* was measured in clicks, by the formula above, starting with the ball at rest (*u*= 0) one gets for the distance S covered

After one click **S = (a***/*2) 1^{2}= a*/* 2

After two **S = (a***/*2) 2^{2}= 2a

After three **S = (a***/*2) 3^{2}= 4.5 a

and so forth. The ratio between the distances should be that of the square numbers 1, 4, 9, 16, 25. . . and that was what Galileo confirmed. If one could convert the clicks into seconds, take into account the angle of the board and also the fact that the ball was **rolling** (a theory that was not available in Galileo's day), one could even in principle calculate *g* from *a*.

## Waterfalls and Baseballs

If in addition the ball is also given at the start a **horizontal**
velocity *w*, its horizontal motion continues unimpeded, advancing a
distance *w* each second, even while the ball is falling
(air resistance is now ignored). The two motions take place
simultaneously, making the ball follow a curve, which gradually
becomes steeper because the downward velocity keeps increasing
while the horizontal one does not. That is how droplets move in a
waterfall, which gives the cross-section of a waterfall its
characteristic shape (left).

The situation one sees again and again in "Road Runner" cartoon films,
where Wily Coyote runs past the edge of a cliff, hangs motionless in space
(as the realization dawns on him), then plummets down--that is a fanciful
invention, quite contrary to the laws of physics. Actually two motions
like that always take place simultaneously. Likewise, a bullet fired from
a rifle at a target range begins falling the moment it leaves the
muzzle. Adjusting the sights on the rifle for the distance shifts
the aim to a point above the bull's eye, calculated so that at the
appropriate distance, the fall of the bullet brings it down to the
level of the target.

For a stone thrown upwards, *u*
is negative, as are any vertical distances above the
throwing point. In that case, let **û = -u**
be a **positive number**. Then after *t* seconds

**velocity = (-û + gt) m/s**

At first *t* is small and the velocity is
negative, showing the stone travels upwards. At the time when

**gt = û**

the sum is zero and for the briefest instant the stone
is at rest, at the top of its trajectory. At that time

**t = û***/*g

and if that value is used in the formula for the distance,
the height at which this happens is found. And finally, if one
adds to this motion a constant horizontal speed *w*, the
motion of a baseball or cannonball is derived.

## About air resistance

The above formulas only hold for ideal cannonballs
that experience no air resistance. In actual practice,
air resistance modifies the motion and may have to be
taken into account, especially in the fall of a light
object, such as a feather. A science demonstration popular
for centuries had a coin and a feather dropped simultaneously
inside a glass tube, from which air had been pumped: the two
are always seen to drop equally fast.

Such a demonstration was also made on the surface of the
Moon by David Scott, one of the Apollo astronauts. Not only
has the Moon no atmosphere, but its gravity is several times
weaker, making the fall slower and easier to observe. In front
of a TV camera, the astronaut simultaneously let go of his
geology hammer and a feather, and his audience on Earth,
watching their TV screen, observed the two falling together.

Later word (or legend?) had it, though, that he first tried
his experiment out of camera view, just to make sure it worked.