# Newton's universal law of gravity

### Galileo's Law of Falling

What might the arrows at left represent? Which of these are equal (not equal) for the feather and the rock?

- Acceleration,
- Force of gravity,
- Mass.

But according to our equation for acceleration, $a=f/m$, a more massive object requires a bigger force to accelerate it at the same rate as a lighter object, no??

Yes, exactly! The force of gravity near the surface of the earth is called "weight"

$$W=mg$$

Since the weight is proportional to the mass of an object, this is exactly what is needed to produce the Law of Falling, so that all objects have the same acceleration.

### What about force pairs?

A force results from an interaction between two bodies. If the earth pulls on a rock, isn't the rock pulling on the earth too?

So, it seems reasonable that the gravitational force $F_g$
is proportional to the masses of **both** bodies involved in the interaction.
There's nothing so special about one or the other.

### Newton's equation for gravity

Newton's full equation for the gravitational force between two bodies of mass $m_1$ and $m_2$ does indeed depend on the masses of both:

With masses in kilograms and distances in meters:

$F_g = 6.7 \times 10^{-11}\frac{m_1 m_2}{d^2}$

Distances from where to where? Surface to surface?

Distances are measured from the center of mass of one body to the center of mass of the other.

**Materialism** of Newton's day: A body can only exert a force on another body when the two are *touching*...

### Elliptical orbits

Sir Isaac Newton, 1642-1727

- born in year of Galileo's death,
- wrote more about theology and occult studies than science,
- Invented calculus (so did Leibniz),
- Came up with a formula for the gravitational force $F_g$ between two bodies,
- Used calculus to show that his $F_g$
**leads to elliptical orbits of the planets**(confirming Kepler's observations).

With this force law and the just-invented *calculus*, Newton was able to show that planetary orbits around a massive body, like the sun, ought to be **ellipses**, just as Kepler had observed (but never explained).

## Weight

Newton's equation for gravity means that the force of gravity at the surface of the earth on some object of mass $m$ is:

$$F_g \approx 6.7 \times 10^{-11} \frac{m_E \cdot m}{r_E^2} = 6.7 \times 10^{-11}\frac{5.97 \times 10^{24} {\rm kg}\cdot m}{(6.38 \times 10^6 m)^2} = 9.8 (m/sec^2) * m (kg)$$

Talk about how this changes even on the earth, but certainly on different planets.

### The nature of gravity on Earth.

According to the **law of falling**, all objects near Earth's surface fall
(are accelerated at...) the same rate. That rate is called $g$, "the acceleration
of gravity". $g=$

- 22 mph increase in velocity every second, or
- 32 feet per second increase every second, or
- 9.8 (~10) meters per second increase every second

### g-factor

This
dragster accelerates from 0 to 100 mph in ~0.9 sec. 100 mph in one second ~
5 *(22 mph increase in one second) = **5g**.

There is a formula for** **that relates distance and time (starting from rest) to acceleration. It is...

$$d = \frac{1}{2}at^2.$$

Solve it for $a$:

$$\frac{2 d}{t^2}= a.$$

World class sprinter:
40 m dash in 4.4 seconds:

$a = (2*40)/(4.4^2) \approx 4 $m / sec / sec = 0.4
* 10 m / sec / sec = **0.4 g**.

John Stapp survived *horizontal* acceleration of $\approx 22g$ for more than a second (1954 USAF sled trial).

The human body can withstand only about $5g$ *vertically* before blood flow away from the head leaves you unconscious. The space shuttle is designed to limit accelerations to $3g$.

Conceptual Exercises in Chapter 5: 3, 4, 11, 12, 18, 22.

Problems in Chapter 5: 2, 3, 4