The law of universal gravitation
Isaac Newton wondered whether the force that makes an apple fall is the same one that keeps the Moon circling without flying away. The answer, a single equation, explains at once why things fall, why planets orbit and why we weigh less on the Moon.
The statement of the law
An apple falls to the ground and the Moon stays in orbit around the Earth without moving away or crashing into it: what common rule governs both the fall of everyday objects and the motion of the heavenly bodies at the same time?
Two steel balls of $1\ \text{kg}$ each are placed so that their centres 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 centres are $1\ \text{m}$ apart, as shown in the diagram.
Apply the law of universal gravitation, $F = G\cdot\frac{M\cdot m}{r^2}$, with $G = 6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$, and calculate the gravitational force attracting them. Does this seem like a large or small force? Comment on it.
In the law of universal gravitation, $F = G\cdot\frac{M\cdot m}{r^2}$: a) State what each letter represents ($F$, $G$, $M$, $m$ and $r$) and its SI unit of measurement.…
In the law of universal gravitation, $F = G\cdot\frac{M\cdot m}{r^2}$:
- a) State what each letter represents ($F$, $G$, $M$, $m$ and $r$) and its SI unit of measurement.
- b) The value of $G$ is $6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$, a very small number. Explain the consequence of this for the force between objects of ordinary mass.
What the force depends on: the masses
Two small magnets attract each other visibly on a table, but two people sitting in a classroom feel no force between them: why is gravitational attraction only obvious when enormous masses such as planets are involved?
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 ($G = 6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$) and express it in standard form.
The Sun keeps the Earth in orbit by attracting it. Calculate this force using the following data: mass of the Sun $M_S = 1,99\cdot10^{30}\ \text{kg}$, 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 $M_S = 1,99\cdot10^{30}\ \text{kg}$, mass of the Earth $M_T = 5,97\cdot10^{24}\ \text{kg}$, mean distance between their centres $r = 1,5\cdot10^{11}\ \text{m}$ and $G = 6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$. Then, compare the result with the Earth–Moon force, of about $2\cdot10^{20}\ \text{N}$: how many times larger is it?
What the force depends on: the square of the distance
Calculate the gravitational force of attraction between the Earth and the Moon, as shown in the diagram. Given: mass of the Earth $M_T = 5,97\cdot10^{24}\ \text{kg}$,…
Calculate the gravitational force of attraction between the Earth and the Moon, as shown in the diagram.
Given: mass of the Earth $M_T = 5,97\cdot10^{24}\ \text{kg}$, mass of the Moon $M_L = 7,35\cdot10^{22}\ \text{kg}$, mean distance between their centres $r = 3,84\cdot10^{8}\ \text{m}$ and $G = 6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$. Express the result in standard form, rounded to two decimal places.
Two twin oil tankers, each with a mass of $10^{6}\ \text{kg}$, are anchored with their centres of mass separated by $100\ \text{m}$. a) Calculate the gravitational force…
Two twin oil tankers, each with a mass of $10^{6}\ \text{kg}$, are anchored with their centres of mass separated by $100\ \text{m}$.
- a) Calculate the gravitational force attracting them ($G = 6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$).
- b) Compare this force with that needed to drag a sheet of paper across a table, of the order of $0,01\ \text{N}$. Will the ships notice this attraction? Justify your answer.
From the law of gravitation to gravity on the surface
The acceleration due to gravity $g$ on the surface of a planet is not a fixed number of the universe: it can be deduced from the law of universal gravitation by equating the two ways of writing weight.
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.
- a) Write the force exerted by the Earth on a body of mass $m$ in two ways: as $F = m\cdot g$ and as $F = G\cdot\frac{M\cdot m}{r^2}$.
- b) Equate the two expressions, cancel the mass $m$ and rearrange for $g$.
- c) Calculate its value with $M = 5,97\cdot10^{24}\ \text{kg}$, $r = 6,37\cdot10^{6}\ \text{m}$ and $G = 6,67\cdot10^{-11}\ \text{N}\cdot\text{m}^2/\text{kg}^2$. What well-known value do you obtain?
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.
- 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.
- b) Solve the equation and calculate $x$ (hint: first simplify $G$ and the third mass, and then take square roots).
- c) Does the result depend on the value of the third mass? What about $G$? Comment on this.
Back to the beginning: We weigh less on the Moon because its mass is about 81 times smaller than that of the Earth and, when we apply $g = G \cdot M / r^2$ with its measurements, its surface gravity is only $1{,}6\ \text{m/s}^2$ compared with the Earth's $9{,}8\ \text{m/s}^2$.