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Secondary 6 · Physics
Interaction · Gravitation

The Law of Universal Gravitation

Before you start, make sure you know: Scientific notation and significant figures (Secondary Year 3 (first cycle))
Before you start, make sure you know: Third law: action and reaction (Secondary Year 3 (first cycle))

When you look at the sea from the Malecón in Santo Domingo, you see the water level rise and fall during the day. And the pencil that drops to the floor, does it have anything to do with that? Isaac Newton wondered whether the force that makes an apple fall is the same one that keeps the Moon in orbit. His answer was a single equation that explains why objects fall, why the planets orbit the Sun, and why the tides rise and fall.

The statement of the law

An apple falls to the ground, the sea rises as the Moon passes, and the Moon circles the Earth without escaping: what law explains all of these attractions at once?

In SI units: $F$ in newtons (N), $M$ and $m$ in kilograms (kg), and $r$ in meters (m). Notice that $r$ is measured between the centers of the bodies.

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Two steel balls of $1\ \text{kg}$ each are placed so that their centers are $1\ \text{m}$ apart, as shown in the diagram. Apply the law of universal gravitation,…

Two steel balls of $1\ \text{kg}$ each are placed so that their centers are $1\ \text{m}$ apart, as shown in the diagram.

m = 1 kg m = 1 kg F = ? F = ? r = 1 m

Apply the law of universal gravitation, $F = G\times\frac{M\times m}{r^2}$, with $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$, and calculate the gravitational force attracting them. Does this seem like a large or small force? Comment on it.

Solve
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In the law of universal gravitation, $F = G\times\frac{M\times m}{r^2}$: a) State what each letter represents ($F$, $G$, $M$, $m$ and $r$) and its SI unit of…

In the law of universal gravitation, $F = G\times\frac{M\times m}{r^2}$:

  1. a) State what each letter represents ($F$, $G$, $M$, $m$ and $r$) and its SI unit of measurement.
  2. b) The value of $G$ is $6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$, a very small number. Explain the consequence of this for the force between objects of ordinary mass.
Solve

Dependence on the masses

Two students sitting next to each other at school feel no attraction at all, but with a planet the effect is obvious. How does the force change when the masses change?

Two spheres of masses M and m attracting each other with forces of equal magnitude F and opposite directions, separated by a distance r between their centers. attract each other with the same force F M m F F r (center to center)
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Two classmates, with masses of $60\ \text{kg}$ and $70\ \text{kg}$, are sitting such that their bodies are on average $1\ \text{m}$ apart. Calculate the gravitational…

Two classmates, with masses of $60\ \text{kg}$ and $70\ \text{kg}$, are sitting such that their bodies are on average $1\ \text{m}$ apart. Calculate the gravitational force of attraction between them ($G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$) and express it in standard form.

Solve
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Two asteroids attract each other with a force $F$. a) If one of them had twice the mass, what would the new force be? b) What if both of them had twice the mass? Reason…

Two asteroids attract each other with a force $F$.

  1. a) If one of them had twice the mass, what would the new force be?
  2. b) What if both of them had twice the mass?

Reason both answers using the formula for universal gravitation.

Solve
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When you drop a pen, the Earth attracts it downwards; but, according to the law of universal gravitation, the pen also attracts the Earth with a force of equal…

When you drop a pen, the Earth attracts it downwards; but, according to the law of universal gravitation, the pen also attracts the Earth with a force of equal magnitude.

  1. a) Why do we only see the pen moving and not the Earth rising to meet it?
  2. b) Reason this taking into account the masses of both bodies and the acceleration that the same force produces in each.
Solve
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The Sun keeps the Earth in orbit by attracting it. Calculate this force using the following data: mass of the Sun $M_S = 1.99\times10^{30}\ \text{kg}$, mass of the Earth…

The Sun keeps the Earth in orbit by attracting it. Calculate this force using the following data: mass of the Sun $M_S = 1.99\times10^{30}\ \text{kg}$, mass of the Earth $M_T = 5.97\times10^{24}\ \text{kg}$, mean distance between their centers $r = 1.5\times10^{11}\ \text{m}$ and $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$. Then, compare the result with the Earth–Moon force, of about $2\times10^{20}\ \text{N}$: how many times larger is it?

Solve

Dependence on the square of the distance

At a distance r between two masses the force is F; when the distance doubles to 2r, the force is reduced to F/4. M m F r r → F M m F/4 2r 2r → F/4

The Moon and the tides

The Moon attracts the ocean water, and it attracts it more strongly on the side near it than on the far side, because the force depends on $1/r^2$. That difference stretches the water and produces the tides: on coasts like those of Puerto Plata or Samaná the water level rises and falls twice a day. The same law, applied to the solid Earth, also produces small "Earth tides."

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Two bodies attract each other with a force $F$, as shown in the graph of force against distance. Without changing the masses, we move them further apart until the…

Two bodies attract each other with a force $F$, as shown in the graph of force against distance.

r F 2r ?

Without changing the masses, we move them further apart until the distance between them is doubled. Looking at the formula $F = G\times\frac{M\times m}{r^2}$, what will the force be now? Justify your answer.

Solve
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Calculate the gravitational force of attraction between the Earth and the Moon, as shown in the diagram. Given: mass of the Earth $M_T = 5.97\times10^{24}\ \text{kg}$,…

Calculate the gravitational force of attraction between the Earth and the Moon, as shown in the diagram.

Earth M = 5.97·10²⁴ kg Moon M = 7.35·10²² kg F = ? F = ? r = 3.84·10⁸ m

Given: mass of the Earth $M_T = 5.97\times10^{24}\ \text{kg}$, mass of the Moon $M_L = 7.35\times10^{22}\ \text{kg}$, mean distance between their centers $r = 3.84\times10^{8}\ \text{m}$ and $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$. Express the result in standard form, rounded to two decimal places.

Solve
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At what distance from the center of the Earth is the gravitational force on a body reduced to half of that felt on the surface? a) Set up the equality using the fact…

At what distance from the center of the Earth is the gravitational force on a body reduced to half of that felt on the surface?

  1. a) Set up the equality using the fact that the force decreases with $\frac{1}{r^2}$.
  2. b) Rearrange for $r$ in terms of the Earth's radius $R_T$ (a $\sqrt{2}$ will appear).
  3. c) Using $R_T = 6370\ \text{km}$, calculate at what height above the surface one must ascend, in kilometers. Do you think a commercial airplane, flying at a height of about $10\ \text{km}$, notices this decrease? Give reasons for your answer.
Solve

From the law of gravitation to surface gravity

The value of $g$ is not a fixed number of the universe: it is derived from the law of gravitation by equating two ways of writing weight.

A body of mass m on a planet of mass M and radius r: its weight points toward the center and equals m·g or G·M·m/r², so g = G·M/r². r planet: mass M m F = m·g F = G·M·m/r²
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Calculate the force with which the Earth attracts a person of $50\ \text{kg}$ located on its surface, as shown in the diagram. Given: mass of the Earth…

Calculate the force with which the Earth attracts a person of $50\ \text{kg}$ located on its surface, as shown in the diagram.

Earth M = 5.97·10²⁴ kg r = 6.37·10⁶ m m = 50 kg F = ?

Given: mass of the Earth $M = 5.97\times10^{24}\ \text{kg}$, Earth's radius $r = 6.37\times10^{6}\ \text{m}$ and $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$. Compare the result with their weight, $P = m\times g$ with $g = 9.8\ \text{m/s}^2$: what do you observe?

Solve
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Let us deduce the value of $g$ on the surface of the Earth from the law of universal gravitation. a) Write the force exerted by the Earth on a body of mass $m$ in two…

Let us deduce the value of $g$ on the surface of the Earth from the law of universal gravitation.

  1. a) Write the force exerted by the Earth on a body of mass $m$ in two ways: as $F = m\times g$ and as $F = G\times\frac{M\times m}{r^2}$.
  2. b) Equate the two expressions, cancel the mass $m$ and rearrange for $g$.
  3. c) Calculate its value with $M = 5.97\times10^{24}\ \text{kg}$, $r = 6.37\times10^{6}\ \text{m}$ and $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$. What well-known value do you obtain?
Solve
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A rocky exoplanet has four times the mass of the Earth and twice the radius, as shown in the figure. a) Using $g = \frac{G\times M}{R^2}$, reason by what factor gravity…

A rocky exoplanet has four times the mass of the Earth and twice the radius, as shown in the figure.

R Earth mass M g = 9.8 m/s² 2R exoplanet mass 4 · M g = ?
  1. a) Using $g = \frac{G\times M}{R^2}$, reason by what factor gravity changes on its surface relative to Earth's gravity.
  2. b) How much would a $60\ \text{kg}$ astronaut weigh there (take Earth's gravity as $9.8\ \text{m/s}^2$)?
  3. c) What if the planet had four times the mass but the same radius as the Earth? Calculate the astronaut's new weight.
Solve

The Moon also "falls"

Newton didn't stop at the formula: he put it to the test by comparing the fall of an apple with the motion of the Moon. To understand the comparison you need an idea from circular motion.

A body that moves along a circle of radius $r$ at constant speed $v$ is continuously changing direction. That is an acceleration, directed toward the center: the centripetal acceleration. Its value is $$a_c = \frac{v^2}{r}$$ Since $v = \dfrac{2\pi r}{T}$, where $T$ is the period of one revolution, it can also be written as $$a_c = \frac{4\pi^2\, r}{T^2}$$

Why toward the center? The force that bends the path must point toward the inside of the curve. In the case of the Moon, that force is the Earth's gravitational attraction. By Newton's second law, the Moon's acceleration is $a_c = F/m_M$.

That coincidence was Newton's proof: if gravity decreases with $1/r^2$, at a distance 60 times greater it must be $60^2 = 3{,}600$ times smaller. The force pulling on the apple and the force holding the Moon are the same.

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A geostationary satellite of $1000\ \text{kg}$ orbits at a distance of $r = 4.22\times10^{7}\ \text{m}$ from the center of the Earth, as shown in the diagram. a)…

A geostationary satellite of $1000\ \text{kg}$ orbits at a distance of $r = 4.22\times10^{7}\ \text{m}$ from the center of the Earth, as shown in the diagram.

Earth r = 4.22·10⁷ m satellite · m = 1000 kg F = ?
  1. a) Calculate the force with which the Earth attracts it (mass of the Earth $M_T = 5.97\times10^{24}\ \text{kg}$, $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$).
  2. b) Compare this force with the satellite's weight when it was on the surface, $P = m\times g$ with $g = 9.8\ \text{m/s}^2$: approximately how many times smaller is it?
Solve
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Newton tested his law by comparing the fall of objects at the surface with the motion of the Moon. a) Calculate the force that the Earth exerts on a body of…

Newton tested his law by comparing the fall of objects at the surface with the motion of the Moon.

  1. a) Calculate the force that the Earth exerts on a body of $1\ \text{kg}$ on its surface ($r = 6.37\times10^{6}\ \text{m}$, $M_T = 5.97\times10^{24}\ \text{kg}$, $G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$).
  2. b) Calculate the force it would exert on that same body if it were at the Moon's distance ($r = 3.84\times10^{8}\ \text{m}$).
  3. c) Verify that the second force is about $3600$ times smaller and relate that number to the ratio between the two distances, which is about $60$. What law is confirmed?
Solve

Applications and problems

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A book and the bookshelf on which it rests attract each other gravitationally, just like the Earth and the Moon. However, we never see the book move towards the shelf.…

A book and the bookshelf on which it rests attract each other gravitationally, just like the Earth and the Moon. However, we never see the book move towards the shelf. Considering the value of $G$, the masses of the objects and the formula $F = G\times\frac{M\times m}{r^2}$, explain why we do not notice the gravitational attraction between everyday objects.

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Two identical metal spheres, placed with their centers $2\ \text{m}$ apart, attract each other with a force of $6.67\times10^{-5}\ \text{N}$. a) Write the law of…

Two identical metal spheres, placed with their centers $2\ \text{m}$ apart, attract each other with a force of $6.67\times10^{-5}\ \text{N}$.

  1. a) Write the law of universal gravitation letting $m$ be the mass of each sphere (they are both equal!).
  2. b) Rearrange the formula for $m$ and calculate the mass of each sphere ($G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$).
Solve
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Calculate the gravitational force between a person of $80\ \text{kg}$ and a lorry of $5000\ \text{kg}$ parked $10\ \text{m}$ away (…

Calculate the gravitational force between a person of $80\ \text{kg}$ and a lorry of $5000\ \text{kg}$ parked $10\ \text{m}$ away ($G = 6.67\times10^{-11}\ \text{N}\times\text{m}^2/\text{kg}^2$). Then, calculate the weight of a mosquito of mass $2\ \text{mg}$ ($P = m\times g$, with $g = 9.8\ \text{m/s}^2$; be careful with the units) and compare both forces. What conclusion do you draw regarding the gravitational attraction between everyday objects?

Solve
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Two fixed masses, of $100\ \text{kg}$ and $400\ \text{kg}$, are $3\ \text{m}$ apart. We want to place a third mass on the line joining them, between the two, such that…

Two fixed masses, of $100\ \text{kg}$ and $400\ \text{kg}$, are $3\ \text{m}$ apart. We want to place a third mass on the line joining them, between the two, such that the net gravitational force on it is zero, as shown in the diagram.

100 kg 400 kg m F₁ F₂ x 3 m − x
  1. a) If $x$ is the distance from the third mass to that of $100\ \text{kg}$, write down the equality between the two forces acting on it.
  2. b) Solve the equation and calculate $x$ (hint: first simplify $G$ and the third mass, and then take square roots).
  3. c) Does the result depend on the value of the third mass? What about $G$? Comment on this.
Solve

Back to the beginning: the apple falls straight down because it starts from rest; the Moon has a large sideways velocity and Earth's gravity continuously curves its path, so it "falls" around the Earth without crashing into it. And the same lunar attraction, which depends on $1/r^2$, is what raises the tides you see at the Malecón.

Summary

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