Gravitational Field Intensity — JEE Main Physics MCQs with Solutions
Free JEE Main Physics Gravitational Field Intensity MCQs with step-by-step solutions (15 questions). Part of Gravitation. Practise online on Prepizo — no login needed.
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Questions with solutions
Q1 — Gravitational Field Intensity · easy · numerical
If the gravitational field intensity on the surface of the Earth is $I_0$, what is the magnitude of the gravitational field intensity at a distance of $2R$ from the surface of the Earth? ($R$ = radius of the Earth)
A. $\dfrac{I_0}{4}$
B. $\dfrac{I_0}{9}$ ✓ Correct
C. $\dfrac{I_0}{3}$
D. $\dfrac{I_0}{2}$
Solution: Distance from the centre of the Earth: $r = R + 2R = 3R$.
Outside the Earth ($r \ge R$): $$I(r) = \frac{GM}{r^2} = \frac{GM}{(3R)^2} = \frac{GM}{9R^2} = \frac{I_0}{9}$$
Q2 — Gravitational Field Intensity · easy · numerical
At what height $h$ above the surface of the Earth will the gravitational field intensity reduce to $16\%$ of its value on the surface? ($R$ = radius of the Earth)
A. $1.5\,R$ ✓ Correct
B. $2.0\,R$
C. $2.5\,R$
D. $4.0\,R$
Solution: Given $I(h) = 0.16\,I_0 = \dfrac{4}{25}\,I_0$.
Using $I(h) = I_0\left(\dfrac{R}{R+h}\right)^2$: $$\left(\frac{R}{R+h}\right)^2 = \frac{4}{25} \implies \frac{R}{R+h} = \frac{2}{5} \implies 5R = 2R + 2h \implies h = 1.5\,R$$
Q3 — Gravitational Field Intensity · easy · numerical
Two satellites $A$ and $B$ are orbiting the Earth (radius $R$) in circular orbits at heights $h_A = R$ and $h_B = 3R$ above the surface, respectively. What is the ratio of the gravitational field intensity experienced by satellite $A$ to that by satellite $B$, $\dfrac{I_A}{I_B}$?
A. $2 : 1$
B. $4 : 1$ ✓ Correct
C. $9 : 4$
D. $16 : 1$
Solution: Distance of $A$ from the centre: $r_A = R + R = 2R$.
Distance of $B$ from the centre: $r_B = R + 3R = 4R$.
Since $I \propto \dfrac{1}{r^2}$: $$\frac{I_A}{I_B} = \left(\frac{r_B}{r_A}\right)^2 = \left(\frac{4R}{2R}\right)^2 = 4 : 1$$
Q4 — Gravitational Field Intensity · easy · numerical
If a body is moved radially outward from a distance $r_1 = 2R$ to $r_2 = 4R$ measured from the centre of the Earth (radius $R$), the percentage decrease in the gravitational field intensity is:
A. $50\%$
B. $75\%$ ✓ Correct
C. $66.7\%$
D. $25\%$
Solution: Field at $r_1 = 2R$: $I_1 = \dfrac{GM}{(2R)^2} = \dfrac{I_0}{4}$.
Field at $r_2 = 4R$: $I_2 = \dfrac{GM}{(4R)^2} = \dfrac{I_0}{16}$.
Percentage decrease: $$\frac{I_1 - I_2}{I_1} \times 100\% = \frac{\frac{1}{4} - \frac{1}{16}}{\frac{1}{4}} \times 100\% = 75\%$$
Q5 — Gravitational Field Intensity · easy · numerical
The gravitational field intensity on the surface of the Earth (radius $R$, assumed a uniform solid sphere) is $I_0$. What is the magnitude of the gravitational field intensity inside the Earth at a depth of $d = \dfrac{R}{2}$ from the surface?
A. $\dfrac{I_0}{4}$
B. $\dfrac{I_0}{2}$ ✓ Correct
C. $\dfrac{3I_0}{4}$
D. $\dfrac{I_0}{\sqrt{2}}$
Solution: Distance from the centre: $r = R - \dfrac{R}{2} = \dfrac{R}{2}$.
Inside a uniform solid sphere ($r \le R$): $I(r) = \dfrac{GM}{R^3}\,r = I_0\left(\dfrac{r}{R}\right)$ $$I = I_0\left(\frac{R/2}{R}\right) = \frac{I_0}{2}$$
Q6 — Gravitational Field Intensity · easy · numerical
A straight mine shaft is drilled deep into the Earth (radius $R$, assumed a uniform solid sphere, surface field intensity $I_0$). At what depth $d$ below the surface does the gravitational field intensity become $\dfrac{1}{3}I_0$?
A. $\dfrac{R}{3}$
B. $\dfrac{2R}{3}$ ✓ Correct
C. $\dfrac{\sqrt{3}-1}{\sqrt{3}}R$
D. $\dfrac{R}{6}$
Solution: Inside the Earth: $I(d) = I_0\left(1 - \dfrac{d}{R}\right)$.
Setting $I(d) = \dfrac{1}{3}I_0$: $$1 - \frac{d}{R} = \frac{1}{3} \implies \frac{d}{R} = \frac{2}{3} \implies d = \frac{2R}{3}$$
Q7 — Gravitational Field Intensity · easy · numerical
Consider two points $P_1$ and $P_2$: $P_1$ is located at a depth of $\dfrac{R}{4}$ below the surface of the Earth, and $P_2$ is at an altitude of $\dfrac{R}{4}$ above the surface ($R$ = radius of the Earth, assumed a uniform solid sphere). The ratio of the magnitude of gravitational field intensity at $P_1$ to that at $P_2$ is:
A. $1 : 1$
B. $75 : 64$ ✓ Correct
C. $16 : 15$
D. $25 : 16$
Solution: At $P_1$ (inside, depth $R/4$): $I_1 = I_0\left(1 - \dfrac{1}{4}\right) = \dfrac{3}{4}I_0$.
At $P_2$ (outside, height $R/4$): $I_2 = I_0\left(\dfrac{R}{R + R/4}\right)^2 = I_0\left(\dfrac{4}{5}\right)^2 = \dfrac{16}{25}I_0$.
Ratio: $$\frac{I_1}{I_2} = \frac{3/4}{16/25} = \frac{3 \times 25}{4 \times 16} = \frac{75}{64}$$
Q8 — Gravitational Field Intensity · easy · theory
A thin, uniform spherical shell of mass $M$ and radius $R$ is centred at the origin. Let $r$ be the radial distance from the centre. Which of the following statements is CORRECT regarding the gravitational field intensity $\vec{I}$ and its magnitude $I(r)$?
A. Inside the shell ($r < R$), $\vec{I} = \vec{0}$; outside the shell ($r > R$), the magnitude $I(r) = \dfrac{GM}{r^2}$ ✓ Correct
B. Inside the shell ($r < R$), $I(r) = \dfrac{GM}{R^2}$; outside the shell ($r > R$), $I(r)$ increases linearly with $r$
C. Inside the shell ($r < R$), $\vec{I} = -\dfrac{GM}{R^3}\vec{r}$; outside the shell, the field is zero
D. Both inside and outside the shell, the gravitational field intensity remains non-zero and constant
Solution: By Newton's shell theorem:
• Inside ($r < R$): the pulls of symmetric mass elements cancel in pairs, so $\vec{I}_{\text{in}} = \vec{0}$.
• Outside ($r > R$): the shell acts as if all its mass were at the centre, so $\vec{I}_{\text{out}} = -\dfrac{GM}{r^2}\hat{r}$, with magnitude $I = \dfrac{GM}{r^2}$.
Q9 — Gravitational Field Intensity · easy · numerical
A thin, uniform circular ring of mass $M$ and radius $R$ lies in the $y$-$z$ plane centred at the origin. What is the magnitude of the gravitational field intensity at an axial distance $x = \sqrt{2}R$ from the centre of the ring?
A. $\dfrac{\sqrt{2}}{3\sqrt{3}}\,\dfrac{GM}{R^2}$ ✓ Correct
B. $\dfrac{2}{3\sqrt{3}}\,\dfrac{GM}{R^2}$
C. $\dfrac{1}{3\sqrt{3}}\,\dfrac{GM}{R^2}$
D. $\dfrac{\sqrt{2}}{27}\,\dfrac{GM}{R^2}$
Solution: On the axis of a ring: $I(x) = \dfrac{GMx}{(R^2 + x^2)^{3/2}}$.
With $x = \sqrt{2}R$: $R^2 + x^2 = 3R^2$, so $(3R^2)^{3/2} = 3\sqrt{3}\,R^3$. $$I = \frac{GM(\sqrt{2}R)}{3\sqrt{3}\,R^3} = \frac{\sqrt{2}}{3\sqrt{3}}\,\frac{GM}{R^2}$$
Q10 — Gravitational Field Intensity · easy · numerical
The gravitational field intensity at a distance $\dfrac{R}{2}$ from the centre of the Earth is $I_0$. What will be the magnitude of the gravitational field intensity at a distance $2R$ from the centre? (Assume the Earth is a uniform solid sphere of radius $R$)
A. $\dfrac{I_0}{2}$ ✓ Correct
B. $\dfrac{I_0}{4}$
C. $I_0$
D. $2I_0$
Solution: Inside a uniform solid sphere ($r \le R$): $I(r) = \dfrac{GM}{R^3}\,r$.
At $r = \dfrac{R}{2}$: $I_0 = \dfrac{GM}{2R^2} \implies \dfrac{GM}{R^2} = 2I_0$.
Outside ($r \ge R$): $I(r) = \dfrac{GM}{r^2}$, so at $r = 2R$: $$I(2R) = \frac{GM}{4R^2} = \frac{1}{4}(2I_0) = \frac{I_0}{2}$$
Q11 — Gravitational Field Intensity · easy · numerical
What will be the gravitational field intensity on the surface of a planet whose mass is $4$ times and radius is half that of the Earth? ($I_e$ = gravitational field intensity on the surface of the Earth)
A. $2\,I_e$
B. $8\,I_e$
C. $16\,I_e$ ✓ Correct
D. $4\,I_e$
Solution: On the Earth: $I_e = \dfrac{GM_e}{R_e^2}$.
For the planet, $M_p = 4M_e$ and $R_p = \dfrac{R_e}{2}$: $$I_p = \frac{G(4M_e)}{(R_e/2)^2} = 16\,\frac{GM_e}{R_e^2} = 16\,I_e$$
Q12 — Gravitational Field Intensity · easy · numerical
A hypothetical celestial body has a mass $81$ times that of the Earth, and the distance between their centres is $4\times 10^5\text{ km}$. Find the distance from the Earth where the net gravitational field intensity due to the two is zero.
A. $40{,}000\text{ km}$ ✓ Correct
B. $44{,}444\text{ km}$
C. $36{,}000\text{ km}$
D. $80{,}000\text{ km}$
Solution: Let the neutral point be at distance $x$ from the Earth; its distance from the other body is $d - x$, with $d = 4\times 10^5$ km.
$$\frac{GM_E}{x^2} = \frac{G(81M_E)}{(d - x)^2} \implies \frac{1}{x} = \frac{9}{d - x} \implies d = 10x$$ $$x = \frac{d}{10} = 40{,}000\text{ km}$$
Q13 — Gravitational Field Intensity · easy · numerical
The gravitational field intensity on the surface of the Earth (radius $R$, assumed a uniform solid sphere) is $I_s$. At what distances $r$ from the centre of the Earth (one inside and one outside) is the magnitude of the field intensity equal to $\dfrac{I_s}{4}$?
A. Inside: $\dfrac{R}{4}$, Outside: $2R$ ✓ Correct
B. Inside: $\dfrac{R}{2}$, Outside: $4R$
C. Inside: $\dfrac{R}{4}$, Outside: $4R$
D. Inside: $\dfrac{R}{16}$, Outside: $2R$
Solution: Inside ($r < R$): $I(r) = I_s\left(\dfrac{r}{R}\right) = \dfrac{I_s}{4} \implies r = \dfrac{R}{4}$.
Outside ($r > R$): $I(r) = I_s\left(\dfrac{R}{r}\right)^2 = \dfrac{I_s}{4} \implies \dfrac{R}{r} = \dfrac{1}{2} \implies r = 2R$.
Q14 — Gravitational Field Intensity · easy · numerical
A spherical planet has the same average mass density as the Earth, but its radius is $3$ times that of the Earth. If the gravitational field intensity on the Earth's surface is $I_e$, what is the field intensity on the surface of this planet?
A. $\dfrac{I_e}{3}$
B. $3\,I_e$ ✓ Correct
C. $9\,I_e$
D. $27\,I_e$
Solution: In terms of density $\rho$: $$I = \frac{GM}{R^2} = \frac{G\left(\frac{4}{3}\pi R^3\rho\right)}{R^2} = \frac{4}{3}\pi G\rho R$$ With $\rho$ the same, $I \propto R$, so $I_p = 3\,I_e$.
Q15 — Gravitational Field Intensity · easy · numerical
Two point masses $M_1 = 4M$ and $M_2 = 16M$ are held at a fixed separation $L$. At what distance from $M_1$ along the line joining the two masses is the net gravitational field intensity equal to zero?
A. $\dfrac{L}{2}$
B. $\dfrac{L}{4}$
C. $\dfrac{L}{3}$ ✓ Correct
D. $\dfrac{2L}{3}$
Solution: Let the point be at distance $x$ from $M_1$; its distance from $M_2$ is $L - x$.
$$\frac{G(4M)}{x^2} = \frac{G(16M)}{(L - x)^2} \implies \frac{2}{x} = \frac{4}{L - x} \implies L - x = 2x \implies x = \frac{L}{3}$$