Advertisements
Advertisements
Question
Derive the expression for gravitational potential energy.
Advertisements
Solution
Consider two masses m1 and m2 are initially separated by a distance r’. m1 is assumed to be fixed in its position.


Two distant masses changing the linear distance
To move the mass m2 through an infinitesimal displacement `"d"vec"r"` from `vec"r"` to `vec"r" + "d"vec"r"` (shown in the Figure above), work has to be done externally. This infinitesimal work is given by
dW = `vec"F"_"ext"."d"vec"r"` ......(1)
The work is done against the gravitational force, therefore,
`|vec"F"_"ext"| = |vec"F"_"G"| = ("Gm"_1"m"_2)/"r"^2` .........(2)
Substituting Equation (2) in (1) we get,
dW = `("Gm"_1"m"_2)/"r"^2 hat"r" . "d"vec"r"` ....(3)
And `"d"vec"r" = "dr"hat"r"` ....(4)
dW = `("Gm"_1"m"_2)/"r"^2hat"r".("dr"hat"r")` ......(5)
`hat"r".hat"r"` = 1 (since both are unit vectors)
∴ dW = `("Gm"_1"m"_2)/"r"^2 "dr"` ....(6)
Hence the total work done for displacing the particle from r’ to r is
W = `int_"r′"^"r""dW" = int_"r′"^"r"("Gm"_1"m"_2)/"r"^2 "dr"` ....(7)
W = `-(("Gm"_1"m"_2)/"r")_"r’"^"r"`
W = `-("Gm"_1"m"_2)/"r" + ("Gm"_1"m"_2)/"r’"` .....(8)
W = U(r) − U(r’)
where U(r) = `(-"Gm"_1"m"_2)/"r"`
This work done W gives the gravitational potential energy difference of the system of masses m1 and m2 when the separation between them is r and r’ respectively.


Cases for calculation of work done by gravity
Case 1:
If r < r’ - Since the gravitational force is attractive, m2 is attracted by m1. Then m2 can move from r’ to r without any external Work. Here work is done by the system spending its internal energy and hence the work done is said to be negative.
Case 2:
If r > r’ - Work has to be done against gravity to move the object from r’ to r. Therefore work is done on the body by external force and hence work done is positive.
APPEARS IN
RELATED QUESTIONS
If the masses of the Earth and Sun suddenly double, the gravitational force between them will ___________.
A planet moving along an elliptical orbit is closest to the Sun at distance r1 and farthest away at a distance of r2. If v1 and v2 are linear speeds at these points respectively. Then the ratio `"v"_1/"v"_2` is
The gravitational potential energy of the Moon with respect to Earth is ____________.
Define the gravitational field.
Write unit of the gravitational field.
Define gravitational potential.
The work done by Sun on Earth in one year will be
The work done by Sun on Earth at any finite interval of time is
If the Earth’s pull on the Moon suddenly disappears, what will happen to the Moon?
What is the gravitational potential energy of the Earth and Sun? The Earth to Sun distance is around 150 million km. The mass of the Earth is 5.9 × 1024 kg and the mass of the Sun is 1.9 × 1030 kg.
