Newton's Law of Gravitation - NEET Physics Questions
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Newton's Law of Gravitation

Question 11: easy

The acceleration due to gravity (on earth) depends upon

1. size of the body
2. gravitational mass of the body
3. gravitational mass of the earth
4. none of the above factors
View Answer

The acceleration due to gravity is \(g = \frac{GM_e}{R_e^2}\). This depends on the mass of the Earth, not on the properties of the body itself.

Question 12: easy

A thin rod of length \(L\) is bent to form a circle. Its mass is \(M\). What force will act on the mass \(m\) placed at the centre of the circle?

1. \(\frac{4\pi^2 GMm}{L^2}\)
2. \(\frac{GMm}{4\pi^2 L^2}\)
3. \(\frac{2\pi GMm}{L^2}\)
4. zero
View Answer

Due to the symmetrical distribution of mass in a circular ring, the gravitational field at the center is zero. Therefore, the force on any mass placed at the center is zero.

Question 13:

Suppose the gravitational force varies inversely as the \(n^{\text{th}}\) power of distance. Then, the time period of a planet in circular orbit of radius \(R\) around the sun will be proportional to

1. \(R^n\)
2. \(R^{\frac{n+1}{2}}\)
3. \(R^{\frac{n-1}{2}}\)
4. \(R^{-n}\)
View Answer

The centripetal force is provided by the gravitational force: \(m \omega^2 R = \frac{k}{R^n} ⇒ \omega^2 \propto \frac{1}{R^{n+1}}\). Since \(T = \frac{2\pi}{\omega}\), we get \(T^2 \propto R^{n+1} ⇒ T \propto R^{\frac{n+1}{2}}\).

Question 14: easy

A thin rod of length \(L\) is bent to form a circle. Its mass is \(M\). What force will act on the mass \(m\) placed at the centre of the circle ?

1. \(\frac{4 \pi^2 GMm}{L^2}\)
2. \(\frac{GMm}{4 \pi^2 L^2}\)
3. \(\frac{2 \pi GMm}{L^2}\)
4. zero
View Answer

Due to symmetry, the gravitational forces exerted by all symmetric parts of the ring at the center cancel each other out, resulting in a net force of zero.

Question 15: easy

A spherical shell has mass \(M\) and radius \(R\). A point mass \(m/2\) kept inside the shell at a distance \(R/2\) from centre. Then force of attraction on the mass is:

1. \(\frac{2Gm^2}{R^2}\)
2. \(\frac{Gm^2}{R^2}\)
3. \(\frac{Gm^2}{2R}\)
4. zero
View Answer

The gravitational field inside a uniform spherical shell is zero everywhere. Therefore, the gravitational force on any mass kept inside the shell is zero.

Question 16: easy

The gravitational force of attraction between two bodies is \(F\) newtons. If the mass of each body and the distance between them are doubled, then the gravitational force between them in newton is

1. \(16 F\)
2. \(F/16\)
3. \(F/4\)
4. \(F\)
View Answer

Formula of gravitational force is \(F = \frac{G m_1 m_2}{r^2}\). If masses and distance are doubled: \(F' = \frac{G(2m_1)(2m_2)}{(2r)^2} = \frac{4 G m_1 m_2}{4 r^2} = F\). Thus, the force remains unchanged.

Question 17: moderate

Two identical particles of combined mass \(M\), placed in space with certain separation, are released. Interaction between the particles is only of gravitational in nature and there is no external force present. Acceleration of one particle with respect to the other when separation between them is \(R\), has a magnitude :

1. \(\frac{GM}{2R^2}\)
2. \(\frac{GM}{R^2}\)
3. \(\frac{2GM}{R^2}\)
4. not possible to calculate due to lack of information
View Answer

Each particle has mass \(m = M/2\). The force is \(F = \frac{G m^2}{R^2} = \frac{GM^2}{4R^2}\). Acceleration of each is \(a = \frac{F}{m} = \frac{GM}{2R^2}\). Relative acceleration is \(a_{\text{rel}} = 2a = \frac{GM}{R^2}\).

Question 18: easy

If three uniform spheres, each having mass \(M\) and radius \(R\), are kept in such a way that each touches the other two, the magnitude of the gravitational force on any sphere due to the other two is

1. \(\frac{GM^2}{4r^2}\)
2. \(\frac{2GM^2}{r^2}\)
3. \(\frac{2GM^2}{4r^2}\)
4. \(\frac{\sqrt{3}GM^2}{4r^2}\)
View Answer

The distance between the centers of any two touching spheres is \(2R\). The gravitational force between any two is \(F = \frac{GM^2}{(2R)^2} = \frac{GM^2}{4R^2}\). The angle between the two forces acting on one sphere is \(60^\circ\). Net force is \(F_{\text{net}} = \sqrt{3}F = \frac{\sqrt{3}GM^2}{4R^2}\).

Question 19: easy

Imagine a light planet revolving around a very massive star in a circular orbit of radius \(r\) with a period of revolution T. If the gravitational force of attraction between the planet and the star is proportional to \(r^{-5/2}\), then the square of the time period will be proportional to

1. \(r^3\)
2. \(r^2\)
3. \(r^{2.5}\)
4. \(r^{3.5}\)
View Answer

The centripetal force is \(F = m\omega^2 r = m\frac{4\pi^2}{T^2} r \propto \frac{r}{T^2}\). Given \(F \propto r^{-5/2}\), we get \(\frac{r}{T^2} \propto r^{-5/2} \Rightarrow T^2 \propto r^{3.5}\).

Question 20: easy

Assertion (A): The gravitational force between two finite bodies is necessarily along the line joining their centre of mass.


Reason (R): The gravitational force between two particles is not central.


 

1. Both (A) & (R) are true and the (R) is the correct explanation of the (A)
2. Both (A) & (R) are true but the (R) is not the correct explanation of the (A)
3. (A) is true but (R) is false
4. Both (A) and (R) are false
View Answer

Assertion (A) is false.


The gravitational force between two finite bodies is generally not directed along the line joining their centers of mass.


Reason (R) is also false. The gravitational force between two point particles is always central, acting along the line connecting them. Therefore, both (A) and (R) are false.