Mechanics

227 questions

Question 21Question

Two point masses are separated by a distance rr and exert a gravitational force FF on each other. If the distance between them is doubled while keeping their masses constant, what is the new gravitational force between them?

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Answer: F4\frac{F}{4}

Answer

The new gravitational force between the two masses is F4\frac{F}{4}.
Gravitational force obeys an inverse-square law with respect to distance (F1r2F \propto \frac{1}{r^2}). When separation distance is multiplied by 2, the force decreases by a factor of 22=42^2 = 4, yielding F4\frac{F}{4}.

Step-by-Step Solution

1
Write down Newton's Law of Universal Gravitation
F=Gm1m2r2F = \frac{G m_1 m_2}{r^2}
Establish the mathematical relationship governing gravitational force and separation distance.
2
Substitute the new distance r=2rr' = 2r into the gravitational force equation
F=Gm1m2(2r)2=Gm1m24r2F' = \frac{G m_1 m_2}{(2r)^2} = \frac{G m_1 m_2}{4r^2}
Evaluate how doubling the separation distance affects the magnitude of the force.
3
Express the new force FF' in terms of the initial force FF
F=14(Gm1m2r2)=F4F' = \frac{1}{4}\left(\frac{G m_1 m_2}{r^2}\right) = \frac{F}{4}
Relate the calculated force directly to the original force FF.

Key Concept

Inverse-Square Law of Gravitation
Estimated Time:45s
Question 22Question

A simple pendulum suspended in a terrestrial laboratory has a period of oscillation TT when fitted with a bob of mass mm. If the bob is replaced by another bob of mass 4m4m and the entire setup is moved to a high-altitude station where the acceleration due to gravity is g4\frac{g}{4}, what is the new period of oscillation of the pendulum?

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Answer: 2T2T

Answer

The new period of oscillation is 2T2T.
The period of a simple pendulum is given by T=2πLgT = 2\pi \sqrt{\frac{L}{g}}. It depends strictly on the length of the string LL and the local gravitational acceleration gg, making it independent of the bob's mass mm. Replacing mass mm with 4m4m does not alter the period. When gravity decreases to g=g4g' = \frac{g}{4}, the new period becomes T=2πLg/4=2(2πLg)=2TT' = 2\pi \sqrt{\frac{L}{g/4}} = 2 \left(2\pi \sqrt{\frac{L}{g}}\right) = 2T.

Step-by-Step Solution

1
Identify the formula for the period of a simple pendulum
The period TT of a simple pendulum is given by T=2πLgT = 2\pi \sqrt{\frac{L}{g}}, where LL is the pendulum length and gg is the acceleration due to gravity.
This formula defines how physical parameters affect the oscillatory period of a pendulum under simple harmonic motion.
2
Analyze the effect of changing the bob's mass
Changing the mass of the bob from mm to 4m4m has no effect on the period.
The equation for the period of a simple pendulum contains no mass term, demonstrating that mass does not influence the period of small-angle oscillations.
3
Calculate the new period TT' under the altered gravitational field g=g4g' = \frac{g}{4}
T=2πLg/4=2π4Lg=2×(2πLg)=2TT' = 2\pi \sqrt{\frac{L}{g/4}} = 2\pi \sqrt{\frac{4L}{g}} = 2 \times \left(2\pi \sqrt{\frac{L}{g}}\right) = 2T.
Reducing the gravitational acceleration to one-fourth increases the square-root term 11/4=2\sqrt{\frac{1}{1/4}} = 2, thereby doubling the period.

Key Concept

Mass Independence and Gravity Dependence of Simple Pendulum Period
Question 23Question

A particle executes simple harmonic motion along a straight line with an amplitude of 0.10 m0.10\text{ m}. At what displacement from the equilibrium position is the kinetic energy of the particle equal to three times its potential energy?

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Answer: 0.05 m0.05\text{ m}

Answer

The displacement from the equilibrium position is 0.05 m0.05\text{ m}.
In simple harmonic motion, potential energy is U=12kx2U = \frac{1}{2}kx^2 and kinetic energy is K=12k(A2x2)K = \frac{1}{2}k(A^2 - x^2). Equating K=3UK = 3U yields A2x2=3x2A^2 - x^2 = 3x^2, which simplifies to 4x2=A24x^2 = A^2 or x=A2x = \frac{A}{2}. For an amplitude of 0.10 m0.10\text{ m}, the displacement is 0.05 m0.05\text{ m}.

Step-by-Step Solution

1
Write the expressions for kinetic energy KK and potential energy UU in simple harmonic motion.
U=12kx2U = \frac{1}{2} k x^2 and K=12k(A2x2)K = \frac{1}{2} k (A^2 - x^2), where AA is amplitude and xx is displacement.
These equations express the energy distribution at any displacement xx.
2
Set up the condition given in the problem, K=3UK = 3U.
12k(A2x2)=3×(12kx2)    A2x2=3x2\frac{1}{2} k (A^2 - x^2) = 3 \times \left(\frac{1}{2} k x^2\right) \implies A^2 - x^2 = 3x^2.
Canceling common factor 12k\frac{1}{2} k simplifies the relationship between amplitude and displacement.
3
Solve for displacement xx in terms of amplitude AA.
A2=4x2    x=A2A^2 = 4x^2 \implies x = \frac{A}{2}.
Taking the square root of both sides gives the position where kinetic energy is three times potential energy.
4
Substitute the given amplitude A=0.10 mA = 0.10\text{ m} to find xx.
x=0.10 m2=0.05 mx = \frac{0.10\text{ m}}{2} = 0.05\text{ m}.
Carrying out the calculation yields the final numerical displacement.

Key Concept

Conservation of Energy in Simple Harmonic Motion
Estimated Time:1m 15s
Question 24Question

A body accelerates uniformly from rest at a rate of 4 m/s24\text{ m/s}^2 for 6 s6\text{ s}. What is the distance covered by the body during this time interval?

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Answer: 72 m72\text{ m}

Answer

The distance covered by the body is 72 m72\text{ m}.
Applying the equation of motion s=ut+12at2s = ut + \frac{1}{2}at^2 with u=0 m/su = 0\text{ m/s}, a=4 m/s2a = 4\text{ m/s}^2, and t=6 st = 6\text{ s} yields s=0+12(4)(62)=72 ms = 0 + \frac{1}{2}(4)(6^2) = 72\text{ m}.

Step-by-Step Solution

1
Identify the given kinematic parameters
Initial velocity u=0 m/su = 0\text{ m/s}, acceleration a=4 m/s2a = 4\text{ m/s}^2, and time interval t=6 st = 6\text{ s}.
Since the body starts from rest, its initial velocity is zero.
2
Select and set up the equation of motion for displacement
s=ut+12at2=(0)(6)+12(4)(6)2s = ut + \frac{1}{2}at^2 = (0)(6) + \frac{1}{2}(4)(6)^2
This formula directly relates displacement to initial velocity, acceleration, and time under constant acceleration.
3
Calculate the total distance
s=12×4×36=72 ms = \frac{1}{2} \times 4 \times 36 = 72\text{ m}
Squaring 6 s6\text{ s} yields 36 s236\text{ s}^2, and multiplying by 2 m/s22\text{ m/s}^2 gives 72 m72\text{ m}.

Key Concept

Linear motion under uniform acceleration
Estimated Time:45s
Question 25Question

A body is released from rest from the top of a cliff of height hh. If it covers a distance equal to 716h\frac{7}{16}h in the final second of its motion before hitting the ground, what is the total height hh of the cliff? (Take acceleration due to gravity g=10 m s2g = 10\text{ m s}^{-2})

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Answer: 80 m80\text{ m}

Answer

80 m80\text{ m}
Using the equation of motion under constant acceleration, the total distance fallen from rest in time tt is h=12gt2h = \frac{1}{2}gt^2. The distance fallen up to time (t1)(t-1) is ht1=12g(t1)2h_{t-1} = \frac{1}{2}g(t-1)^2. The distance traveled during the final second is Δh=hht1=12g(2t1)\Delta h = h - h_{t-1} = \frac{1}{2}g(2t-1). Equating this to 716h\frac{7}{16}h yields 12g(2t1)=716(12gt2)\frac{1}{2}g(2t-1) = \frac{7}{16}\left(\frac{1}{2}gt^2\right), which simplifies to 7t232t+16=07t^2 - 32t + 16 = 0. Factoring gives t=4 st = 4\text{ s} (rejecting t=47 st = \frac{4}{7}\text{ s} since time must exceed 1 s1\text{ s}). Substituting t=4 st = 4\text{ s} into h=12(10)(4)2h = \frac{1}{2}(10)(4)^2 gives 80 m80\text{ m}.

Step-by-Step Solution

1
Express total height hh in terms of total fall time tt.
h=12gt2=5t2h = \frac{1}{2} g t^2 = 5t^2
Since the body starts from rest (u=0 m s1u = 0\text{ m s}^{-1}), displacement under uniform acceleration g=10 m s2g = 10\text{ m s}^{-2} is given by h=12gt2h = \frac{1}{2}gt^2.
2
Express the height fallen in the first (t1)(t - 1) seconds.
h=12g(t1)2=5(t1)2h' = \frac{1}{2} g (t - 1)^2 = 5(t - 1)^2
The distance covered up to one second before impact is the total distance fallen minus the distance covered in the final second.
3
Calculate the distance fallen in the final second and set up the equation.
Δh=hh=5t25(t1)2=5(2t1)\Delta h = h - h' = 5t^2 - 5(t - 1)^2 = 5(2t - 1). Given Δh=716h\Delta h = \frac{7}{16}h, we have 5(2t1)=716(5t2)5(2t - 1) = \frac{7}{16}(5t^2).
The distance fallen during the last second is the difference between total height and height fallen up to (t1)(t-1) seconds.
4
Solve the quadratic equation for tt.
7t232t+16=0    (7t4)(t4)=0    t=4 s7t^2 - 32t + 16 = 0 \implies (7t - 4)(t - 4) = 0 \implies t = 4\text{ s} (since t>1 st > 1\text{ s}).
Simplifying 2t1=716t22t - 1 = \frac{7}{16}t^2 gives 7t232t+16=07t^2 - 32t + 16 = 0. The root t=4/7 st = 4/7\text{ s} is discarded as tt must be greater than 1 s1\text{ s}.
5
Substitute t=4 st = 4\text{ s} back into the total height formula.
h=5(4)2=80 mh = 5(4)^2 = 80\text{ m}.
Calculating total height using h=5t2h = 5t^2 for t=4 st = 4\text{ s} gives 80 m80\text{ m}.

Key Concept

Free Fall under Gravity and Motion in the nn-th Second
Question 26Question

A solid object of volume 0.002 m30.002\text{ m}^3 is completely immersed in water of density 1000 kg/m31000\text{ kg/m}^3. What is the magnitude of the upthrust exerted on the object by the water? [Take g=10 m/s2g = 10\text{ m/s}^2]

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Answer: 20

Answer

The magnitude of the upthrust exerted on the object is 20 N20\text{ N}.
According to Archimedes' principle, any body completely or partially submerged in a fluid experiences an upward force (upthrust) equal to the weight of the fluid displaced. The weight of the displaced fluid is calculated using U=VρgU = V \cdot \rho \cdot g. Substituting V=0.002 m3V = 0.002\text{ m}^3, ρ=1000 kg/m3\rho = 1000\text{ kg/m}^3, and g=10 m/s2g = 10\text{ m/s}^2 yields U=0.002×1000×10=20 NU = 0.002 \times 1000 \times 10 = 20\text{ N}.

Step-by-Step Solution

1
Identify the given quantities from the problem statement.
V=0.002 m3V = 0.002\text{ m}^3, ρ=1000 kg/m3\rho = 1000\text{ kg/m}^3, and g=10 m/s2g = 10\text{ m/s}^2.
These are the essential inputs required to calculate the weight of the displaced liquid.
2
Apply Archimedes' principle to find upthrust force.
U=Vρg=0.002×1000×10=20 NU = V \rho g = 0.002 \times 1000 \times 10 = 20\text{ N}.
Archimedes' principle states that the upthrust force equals the weight of the fluid displaced by the object.

Key Concept

Archimedes' Principle and Upthrust
Question 27Question
The volume flow rate QQ of a viscous liquid flowing through a pipe of radius rr under a pressure gradient ΔPl\frac{\Delta P}{l} is modeled by the equation:
Q=kηxry(ΔPl)zQ = k \eta^x r^y \left(\frac{\Delta P}{l}\right)^z
where η\eta is the coefficient of dynamic viscosity and kk is a dimensionless constant. What are the values of the exponents xx, yy, and zz respectively?
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Answer: x=1,y=4,z=1x = -1, y = 4, z = 1

Answer

x=1x = -1, y=4y = 4, and z=1z = 1
The dimensional representation of volume flow rate is [L3T1][L^3 T^{-1}], dynamic viscosity is [ML1T1][M L^{-1} T^{-1}], radius is [L][L], and pressure gradient is [ML2T2][M L^{-2} T^{-2}]. Equating the powers of MM, LL, and TT gives x+z=0x + z = 0, x2z=1-x - 2z = -1, and x+y2z=3-x + y - 2z = 3. Solving these simultaneously yields x=1x = -1, y=4y = 4, and z=1z = 1.

Step-by-Step Solution

1
Determine the fundamental dimensions of each physical quantity
Volume flow rate Q=VolumeTime=[L3T1]Q = \frac{\text{Volume}}{\text{Time}} = [L^3 T^{-1}];
Dynamic viscosity η=[ML1T1]\eta = [M L^{-1} T^{-1}];
Radius r=[L]r = [L];
Pressure gradient ΔPl=PressureLength=[ML1T2][L]=[ML2T2]\frac{\Delta P}{l} = \frac{\text{Pressure}}{\text{Length}} = \frac{[M L^{-1} T^{-2}]}{[L]} = [M L^{-2} T^{-2}].
Correct base dimensions are required for dimensional analysis.
2
Set up the dimensional equation by substituting the base dimensions into the formula
[L3T1]=[ML1T1]x[L]y[ML2T2]z=Mx+zLx+y2zTx2z[L^3 T^{-1}] = [M L^{-1} T^{-1}]^x [L]^y [M L^{-2} T^{-2}]^z = M^{x+z} L^{-x + y - 2z} T^{-x - 2z}.
The principle of dimensional homogeneity requires both sides of the equation to have matching exponents for MM, LL, and TT.
3
Equate exponents for MM, TT, and LL to form algebraic equations
For MM: x+z=0    z=xx + z = 0 \implies z = -x
For TT: x2z=1-x - 2z = -1
For LL: x+y2z=3-x + y - 2z = 3.
This creates a linear system of equations for the exponents xx, yy, and zz.
4
Solve the system of linear equations
Substituting z=xz = -x into the TT equation: x2(x)=1    x=1-x - 2(-x) = -1 \implies x = -1.
Hence z=(1)=1z = -(-1) = 1.
Substituting x=1x = -1 and z=1z = 1 into the LL equation: (1)+y2(1)=3    1+y2=3    y=4-(-1) + y - 2(1) = 3 \implies 1 + y - 2 = 3 \implies y = 4.
Yields the unique set of exponents x=1,y=4,z=1x = -1, y = 4, z = 1.

Key Concept

Dimensional Analysis and Homogeneity
Estimated Time:2m 0s
Question 28Question

A 0.50 kg0.50\text{ kg} mass attached to a horizontal spring undergoes simple harmonic motion on a frictionless surface. The total mechanical energy of the system is 0.16 J0.16\text{ J} and the force constant of the spring is 32 N/m32\text{ N/m}. What is the speed of the mass, in m/s\text{m/s}, at the instant when the magnitude of its acceleration is 3.84 m/s23.84\text{ m/s}^2?

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Answer: 0.64

Answer

The speed of the mass at that instant is 0.64 m/s0.64\text{ m/s}.
Using the relation for total mechanical energy E=12kA2E = \frac{1}{2}kA^2, the amplitude is A=0.10 mA = 0.10\text{ m}. The angular frequency is ω=k/m=8.0 rad/s\omega = \sqrt{k/m} = 8.0\text{ rad/s}. From a=ω2x|a| = \omega^2 |x|, the displacement magnitude when acceleration is 3.84 m/s23.84\text{ m/s}^2 is x=0.06 m|x| = 0.06\text{ m}. Substituting these values into v=ωA2x2v = \omega \sqrt{A^2 - x^2} yields v=8.00.1020.062=0.64 m/sv = 8.0 \sqrt{0.10^2 - 0.06^2} = 0.64\text{ m/s}.

Step-by-Step Solution

1
Calculate the angular frequency of the simple harmonic motion
ω=8.0 rad/s\omega = 8.0\text{ rad/s}
The angular frequency depends on the stiffness constant and the mass according to \omega = \sqrt{k/m}.
2
Calculate the amplitude of oscillation from total energy
A = 0.10\text{ m}
The total mechanical energy in SHM is given by E = \frac{1}{2}kA^2.
3
Find the magnitude of displacement corresponding to the given acceleration
|x| = 0.06\text{ m}
In SHM, acceleration magnitude is related to displacement magnitude by |a| = \omega^2 |x|.
4
Calculate the speed at this displacement using the SHM velocity-displacement relation
v = 0.64\text{ m/s}
Velocity in SHM is calculated using v = \omega \sqrt{A^2 - x^2}.

Key Concept

Interdependence of energy, angular frequency, acceleration, and velocity in Simple Harmonic Motion
Question 29Question

Match each vector scenario on the left with its correct resultant magnitude or value on the right.

Click a left item, then click its matching right item

Items

Resultant of two perpendicular forces of magnitudes 6 N6\text{ N} and 8 N8\text{ N}
Minimum possible magnitude of the resultant of two forces of 7 N7\text{ N} and 12 N12\text{ N}
Resultant magnitude of two equal forces of 15 N15\text{ N} inclined at an angle of 120120^\circ to each other
Magnitude of a 3D displacement vector given by r=(3i+4j+12k) m\mathbf{r} = (3\mathbf{i} + 4\mathbf{j} + 12\mathbf{k})\text{ m}

Matches

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Answer

Match perpendicular forces of 6 N and 8 N to 10 N; minimum resultant of 7 N and 12 N forces to 5 N; two 15 N forces at 120 degrees to 15 N; and 3D displacement vector to 13 m.
Each vector calculation correctly applies the geometric or algebraic properties of vectors: orthogonal vector resolution, opposite-direction subtraction, law of cosines for equal magnitudes at 120 degrees, and 3D component magnitude synthesis.

Step-by-Step Solution

1
Calculate the magnitude of perpendicular vectors
R=62+82=10 NR = \sqrt{6^2 + 8^2} = 10\text{ N}
Perpendicular vectors form a right-angled triangle, so the Pythagorean theorem applies.
2
Find the minimum resultant magnitude of two vectors
Rmin=12 N7 N=5 NR_{\text{min}} = 12\text{ N} - 7\text{ N} = 5\text{ N}
Minimum resultant occurs when vectors act collinear in opposite directions.
3
Determine the resultant of two equal vectors at 120120^\circ
R=15 NR = 15\text{ N}
Using the cosine rule R=F2+F2+2F2cos120R = \sqrt{F^2 + F^2 + 2F^2\cos 120^\circ}, since cos120=0.5\cos 120^\circ = -0.5, R=FR = F.
4
Compute the magnitude of the 3D displacement vector
r=32+42+122=13 m|\mathbf{r}| = \sqrt{3^2 + 4^2 + 12^2} = 13\text{ m}
3D magnitude is calculated using the square root of the sum of squared orthogonal components.

Key Concept

Vector Addition, Resolution, and Magnitude Evaluation
Question 30Question

A projectile is launched from ground level over flat terrain. At time t=2 st = 2\text{ s} after launch, the projectile passes through a point located 60 m60\text{ m} horizontally and 60 m60\text{ m} vertically from its launch point. Taking the acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2 and neglecting air resistance, what is the total horizontal range of the projectile in meters?

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Answer: 240

Answer

The total horizontal range of the projectile is 240 m240\text{ m}.
The horizontal motion occurs at a constant velocity of 30 m/s30\text{ m/s} calculated from 60 m2 s\frac{60\text{ m}}{2\text{ s}}. Substituting the vertical position (60 m60\text{ m}) and time (2 s2\text{ s}) into y=uyt5t2y = u_y t - 5t^2 yields an initial vertical velocity of 40 m/s40\text{ m/s}. The total duration in the air is T=2(40)10=8 sT = \frac{2(40)}{10} = 8\text{ s}. The total horizontal range is therefore 30 m/s×8 s=240 m30\text{ m/s} \times 8\text{ s} = 240\text{ m}.

Step-by-Step Solution

1
Determine the horizontal component of velocity
vx=30 m/sv_x = 30\text{ m/s}
Horizontal velocity remains constant throughout flight because there is no horizontal acceleration.
2
Determine the initial vertical component of velocity
uy=40 m/su_y = 40\text{ m/s}
Applying the vertical displacement equation y=uyt12gt2y = u_y t - \frac{1}{2}g t^2 with y=60 my = 60\text{ m}, t=2 st = 2\text{ s}, and g=10 m/s2g = 10\text{ m/s}^2.
3
Calculate the total time of flight
T=8 sT = 8\text{ s}
The projectile completes its full parabolic trajectory when vertical displacement returns to zero, given by T=2uygT = \frac{2 u_y}{g}.
4
Calculate the total horizontal range
R=240 mR = 240\text{ m}
The total range is the product of the constant horizontal velocity component and total time of flight (R=vx×TR = v_x \times T).

Key Concept

Independence of horizontal and vertical components of projectile motion
Question 31Question

A train accelerates uniformly along a straight track from an initial velocity of 10 m/s10\text{ m/s} to a final velocity of 30 m/s30\text{ m/s} over a distance of 100 m100\text{ m}. What is the magnitude of the acceleration of the train?

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Answer: 4 m/s24\text{ m/s}^2

Answer

4 m/s24\text{ m/s}^2
Using the equation of motion v2=u2+2asv^2 = u^2 + 2as, substitute u=10 m/su = 10\text{ m/s}, v=30 m/sv = 30\text{ m/s}, and s=100 ms = 100\text{ m}. This gives 302=102+2(a)(100)30^2 = 10^2 + 2(a)(100), which simplifies to 900100=200a900 - 100 = 200a, or 800=200a800 = 200a. Solving for acceleration yields a=4 m/s2a = 4\text{ m/s}^2.

Step-by-Step Solution

1
Identify the given kinematic values from the problem statement.
Initial velocity u=10 m/su = 10\text{ m/s}, final velocity v=30 m/sv = 30\text{ m/s}, and displacement s=100 ms = 100\text{ m}.
Listing known values helps in selecting the appropriate equation of motion.
2
Select the linear motion formula relating uu, vv, ss, and acceleration aa.
v2=u2+2asv^2 = u^2 + 2as
This formula connects initial velocity, final velocity, distance, and acceleration without requiring time tt.
3
Substitute the values into the equation and solve for aa.
302=102+2(a)(100)    900=100+200a    800=200a    a=4 m/s230^2 = 10^2 + 2(a)(100) \implies 900 = 100 + 200a \implies 800 = 200a \implies a = 4\text{ m/s}^2
Algebraic rearrangement yields the magnitude of acceleration.

Key Concept

Equations of Uniformly Accelerated Motion
Estimated Time:45s
Question 32Question

A water pump driven by an engine with an efficiency of 80%80\% raises water from an underground tank of depth 20 m20\text{ m} and discharges it through a nozzle of cross-sectional area 10 cm210\text{ cm}^2 at a steady speed of 10 m/s10\text{ m/s}. Taking the density of water as 1000 kg/m31000\text{ kg/m}^3 and acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2, what is the minimum input power rating (in W\text{W}) required for the engine?

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Answer: 3125

Answer

The minimum input power rating required for the engine is 3125 W3125\text{ W}.
The engine must supply power to lift 10 kg10\text{ kg} of water per second through a vertical height of 20 m20\text{ m} while accelerating it to 10 m/s10\text{ m/s}. The useful power output is 2000 W2000\text{ W} (potential) +500 W+ 500\text{ W} (kinetic) =2500 W= 2500\text{ W}. Accounting for an engine efficiency of 80%80\%, the total input power is 25000.80=3125 W\frac{2500}{0.80} = 3125\text{ W}.

Step-by-Step Solution

1
Determine the mass of water discharged per unit time (mass flow rate).
dmdt=ρ×A×v=1000 kg/m3×(10×104 m2)×10 m/s=10 kg/s\frac{dm}{dt} = \rho \times A \times v = 1000\text{ kg/m}^3 \times (10 \times 10^{-4}\text{ m}^2) \times 10\text{ m/s} = 10\text{ kg/s}
Water is moving through a cross-sectional area at a constant velocity.
2
Calculate the useful output power required to lift the water and impart kinetic energy.
Pout=dmdtgh+12dmdtv2=(10×10×20)+(12×10×102)=2000 W+500 W=2500 WP_{\text{out}} = \frac{dm}{dt} g h + \frac{1}{2} \frac{dm}{dt} v^2 = (10 \times 10 \times 20) + \left(\frac{1}{2} \times 10 \times 10^2\right) = 2000\text{ W} + 500\text{ W} = 2500\text{ W}
The engine must perform work against gravity to raise the water depth and provide kinetic energy for exit velocity.
3
Calculate the total input power using engine efficiency.
Pin=PoutEfficiency=2500 W0.80=3125 WP_{\text{in}} = \frac{P_{\text{out}}}{\text{Efficiency}} = \frac{2500\text{ W}}{0.80} = 3125\text{ W}
Efficiency is the ratio of useful power output to total power input.

Key Concept

Work-Energy Theorem applied to fluid flow and Power-Efficiency relations
Question 33Question

An object of mass 0.20 kg0.20\text{ kg} executes simple harmonic motion with an amplitude of 0.05 m0.05\text{ m} and a maximum acceleration of 20 m/s220\text{ m/s}^2. What is the speed of the object when its displacement from the equilibrium position is 0.03 m0.03\text{ m}?

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Answer: 0.80 m/s0.80\text{ m/s}

Answer

The speed of the object at a displacement of 0.03 m0.03\text{ m} is 0.80 m/s0.80\text{ m/s}.
The maximum acceleration in simple harmonic motion is given by amax=ω2Aa_{\text{max}} = \omega^2 A. Substituting amax=20 m/s2a_{\text{max}} = 20\text{ m/s}^2 and A=0.05 mA = 0.05\text{ m} gives ω2=400 rad2/s2\omega^2 = 400\text{ rad}^2/\text{s}^2, so ω=20 rad/s\omega = 20\text{ rad/s}. The speed at any displacement xx is given by v=ωA2x2v = \omega \sqrt{A^2 - x^2}. For x=0.03 mx = 0.03\text{ m}, v=200.0520.032=20×0.04=0.80 m/sv = 20 \sqrt{0.05^2 - 0.03^2} = 20 \times 0.04 = 0.80\text{ m/s}.

Step-by-Step Solution

1
Determine the angular frequency (ω\omega) of the simple harmonic motion from the maximum acceleration formula.
ω=20 rad/s\omega = 20\text{ rad/s}
Maximum acceleration is given by amax=ω2Aa_{\text{max}} = \omega^2 A. Rearranging gives ω2=amaxA=200.05=400 rad2/s2\omega^2 = \frac{a_{\text{max}}}{A} = \frac{20}{0.05} = 400\text{ rad}^2/\text{s}^2, so ω=20 rad/s\omega = 20\text{ rad/s}.
2
Calculate the speed (vv) at the given displacement (x=0.03 mx = 0.03\text{ m}) using the SHM velocity formula.
v=0.80 m/sv = 0.80\text{ m/s}
The speed at displacement xx is v=ωA2x2=20×0.0520.032=20×0.0016=20×0.04=0.80 m/sv = \omega \sqrt{A^2 - x^2} = 20 \times \sqrt{0.05^2 - 0.03^2} = 20 \times \sqrt{0.0016} = 20 \times 0.04 = 0.80\text{ m/s}.

Key Concept

Simple Harmonic Motion Velocity and Acceleration Relationships
Estimated Time:1m 30s
Question 34Question

A body AA of mass 4.0 kg4.0\text{ kg} moving due east at a velocity of 6.0 m s16.0\text{ m s}^{-1} collides head-on with a body BB of mass 2.0 kg2.0\text{ kg} moving due west at 3.0 m s13.0\text{ m s}^{-1}. If body AA continues to move due east after the collision with a speed of 1.0 m s11.0\text{ m s}^{-1}, what is the velocity of body BB after the collision?

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Answer: 7.0 m s17.0\text{ m s}^{-1} due East

Answer

7.0 m s17.0\text{ m s}^{-1} due East
According to the principle of conservation of linear momentum, the total momentum before collision equals the total momentum after collision. Assigning positive to East and negative to West, total initial momentum is 4(6)+2(3)=18 kg m s14(6) + 2(-3) = 18\text{ kg m s}^{-1}. Equating this to final momentum 4(1)+2vB4(1) + 2v_B gives 2vB=142v_B = 14, resulting in vB=+7.0 m s1v_B = +7.0\text{ m s}^{-1}, which represents 7.0 m s17.0\text{ m s}^{-1} due East.

Step-by-Step Solution

1
Define a reference direction for 1D momentum vectors
Let East be positive (+) and West be negative (-).
Linear momentum is a vector quantity, so opposite directions must have opposite algebraic signs.
2
Calculate the total initial momentum before collision (pip_i)
pi=mAuA+mBuB=(4.0 kg)(+6.0 m s1)+(2.0 kg)(3.0 m s1)=24.06.0=18.0 kg m s1p_i = m_A u_A + m_B u_B = (4.0\text{ kg})(+6.0\text{ m s}^{-1}) + (2.0\text{ kg})(-3.0\text{ m s}^{-1}) = 24.0 - 6.0 = 18.0\text{ kg m s}^{-1}.
Body B moves west, so its initial velocity is 3.0 m s1-3.0\text{ m s}^{-1}.
3
Formulate the total final momentum after collision (pfp_f)
pf=mAvA+mBvB=(4.0 kg)(+1.0 m s1)+(2.0 kg)vB=4.0+2.0vBp_f = m_A v_A + m_B v_B = (4.0\text{ kg})(+1.0\text{ m s}^{-1}) + (2.0\text{ kg})v_B = 4.0 + 2.0 v_B.
Body A moves east after collision, so its final velocity is +1.0 m s1+1.0\text{ m s}^{-1}.
4
Apply the Law of Conservation of Linear Momentum (pi=pfp_i = p_f)
18.0=4.0+2.0vB    2.0vB=14.0    vB=+7.0 m s118.0 = 4.0 + 2.0 v_B \implies 2.0 v_B = 14.0 \implies v_B = +7.0\text{ m s}^{-1}.
Since total initial momentum equals total final momentum in an isolated system.
5
Interpret the sign of the calculated velocity
Since vBv_B is positive (+7.0 m s1+7.0\text{ m s}^{-1}), body B moves at 7.0 m s17.0\text{ m s}^{-1} due East.
Positive values correspond to the defined East direction.

Key Concept

Principle of Conservation of Linear Momentum in 1D head-on collisions
Question 35Question

A stone is projected from ground level with an initial velocity of 40 m/s40\text{ m/s} at an angle of 3030^\circ to the horizontal. What is the total time of flight of the stone, in seconds? (Take g=10 m/s2g = 10\text{ m/s}^2)

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Answer: 4

Answer

The total time of flight of the stone is 4 s4\text{ s}.
The total time of flight TT for a projectile launched over level ground is calculated using T=2usinθgT = \frac{2 u \sin \theta}{g}. Substituting u=40 m/su = 40\text{ m/s}, θ=30\theta = 30^\circ, and g=10 m/s2g = 10\text{ m/s}^2 yields T=2×40×0.510=4 sT = \frac{2 \times 40 \times 0.5}{10} = 4\text{ s}.

Step-by-Step Solution

1
Find the vertical component of the launch velocity
uy=20 m/su_y = 20\text{ m/s}
The vertical motion determines the time the projectile remains in the air.
2
Calculate the total time of flight
T=4 sT = 4\text{ s}
Applying T=2usinθg=2×2010=4 sT = \frac{2 u \sin \theta}{g} = \frac{2 \times 20}{10} = 4\text{ s} gives the total duration before landing back at ground level.

Key Concept

Time of Flight in Projectile Motion
Estimated Time:45s
Question 36Question

A satellite of mass mm moves in a circular orbit around a uniform spherical planet of radius RR. If the height of the satellite above the planet's surface is h=2Rh = 2R and the acceleration due to gravity at the planet's surface is gg, which of the following expressions represents the orbital speed of the satellite?

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Answer: gR3\sqrt{\frac{gR}{3}}

Answer

The orbital speed of the satellite is gR3\sqrt{\frac{gR}{3}}.
The total orbital radius from the center of the planet is r=R+h=R+2R=3Rr = R + h = R + 2R = 3R. Since surface gravity is g=GMR2g = \frac{GM}{R^2}, we have GM=gR2GM = gR^2. Substituting these into the orbital velocity expression v=GMrv = \sqrt{\frac{GM}{r}} yields v=gR23R=gR3v = \sqrt{\frac{gR^2}{3R}} = \sqrt{\frac{gR}{3}}, which makes the expression gR3\sqrt{\frac{gR}{3}} correct.

Step-by-Step Solution

1
Determine the total orbital radius from the center of the planet.
r=R+h=R+2R=3Rr = R + h = R + 2R = 3R
Gravitational attraction and circular orbital radii are always measured from the center of mass of the primary body, not its surface.
2
Relate the gravitational constant GG and planet mass MM to surface gravity gg.
g=GMR2    GM=gR2g = \frac{GM}{R^2} \implies GM = gR^2
At the surface of a spherical planet of radius RR, the gravitational field strength is gg.
3
Substitute r=3Rr = 3R and GM=gR2GM = gR^2 into the circular orbital velocity equation v=GMrv = \sqrt{\frac{GM}{r}}.
v=gR23R=gR3v = \sqrt{\frac{gR^2}{3R}} = \sqrt{\frac{gR}{3}}
Equating centripetal force to gravitational force mv2r=GMmr2\frac{m v^2}{r} = \frac{G M m}{r^2} yields v=GMrv = \sqrt{\frac{GM}{r}}.

Key Concept

Orbital velocity of a satellite in terms of surface gravitational acceleration and orbital radius
Question 37Question

A motorist traveling along a straight highway at a constant speed of 30 m/s30\text{ m/s} observes a road hazard ahead. The driver experiences a reaction delay of 0.5 s0.5\text{ s} before applying the brakes, after which the vehicle decelerates uniformly at a rate of 5 m/s25\text{ m/s}^2. What is the total distance traveled by the vehicle from the instant the hazard is observed until the vehicle comes to a complete stop?

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Answer: 105 m105\text{ m}

Answer

The total distance traveled by the vehicle before coming to a stop is 105 m105\text{ m}.
The motion consists of two distinct stages: a constant-speed phase during the 0.5 s0.5\text{ s} reaction time (15 m15\text{ m}) and a uniformly decelerating phase until rest (90 m90\text{ m}). Summing both components yields 105 m105\text{ m}.

Step-by-Step Solution

1
Calculate the reaction distance (s1s_1) covered during the driver's reaction delay.
s1=u×tr=30 m/s×0.5 s=15 ms_1 = u \times t_r = 30\text{ m/s} \times 0.5\text{ s} = 15\text{ m}
Before the brakes are applied, the vehicle continues moving at its initial constant speed of 30 m/s30\text{ m/s}.
2
Calculate the braking distance (s2s_2) using the third equation of motion.
v2=u2+2as2    02=302+2(5)s2    10s2=900    s2=90 mv^2 = u^2 + 2as_2 \implies 0^2 = 30^2 + 2(-5)s_2 \implies 10s_2 = 900 \implies s_2 = 90\text{ m}
The vehicle decelerates from 30 m/s30\text{ m/s} to a final velocity of 0 m/s0\text{ m/s} at a uniform deceleration rate of a=5 m/s2a = -5\text{ m/s}^2.
3
Sum the reaction distance and the braking distance to find the total stopping distance.
stotal=s1+s2=15 m+90 m=105 ms_{\text{total}} = s_1 + s_2 = 15\text{ m} + 90\text{ m} = 105\text{ m}
The total stopping distance is the sum of the distance covered before braking begins and the distance covered while braking.

Key Concept

Two-phase linear motion combining constant velocity reaction distance and uniform deceleration braking distance.
Question 38Question

A metallic sphere weighs 5.0 N5.0\text{ N} in air. When completely immersed in water, its apparent weight is 3.0 N3.0\text{ N}. When completely immersed in an unknown liquid XX, its apparent weight is 3.4 N3.4\text{ N}. What is the density of liquid XX in kg/m3\text{kg/m}^3? (Take the density of water as 1000 kg/m31000\text{ kg/m}^3 and acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2).

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Answer: 800

Answer

The density of liquid XX is 800 kg/m3800\text{ kg/m}^3.
The upthrust in water (2.0 N2.0\text{ N}) gives the volume of the sphere as 2.0×104 m32.0 \times 10^{-4}\text{ m}^3. Using the upthrust in liquid X (1.6 N1.6\text{ N}), the density of liquid X is calculated as ρX=1.6(2.0×104)(10)=800 kg/m3\rho_X = \frac{1.6}{(2.0 \times 10^{-4})(10)} = 800\text{ kg/m}^3.

Step-by-Step Solution

1
Calculate upthrust in water
Uw=5.0 N3.0 N=2.0 NU_w = 5.0\text{ N} - 3.0\text{ N} = 2.0\text{ N}
Upthrust equals the loss in weight of the submerged body in water.
2
Determine the volume of the metallic sphere
V=Uwρwg=2.01000×10=2.0×104 m3V = \frac{U_w}{\rho_w g} = \frac{2.0}{1000 \times 10} = 2.0 \times 10^{-4}\text{ m}^3
According to Archimedes' principle, upthrust in water equals the weight of displaced water.
3
Calculate upthrust in liquid X
UX=5.0 N3.4 N=1.6 NU_X = 5.0\text{ N} - 3.4\text{ N} = 1.6\text{ N}
Loss of weight in liquid X gives the upthrust exerted by liquid X.
4
Calculate the density of liquid X
ρX=UXVg=1.6(2.0×104)×10=800 kg/m3\rho_X = \frac{U_X}{V g} = \frac{1.6}{(2.0 \times 10^{-4}) \times 10} = 800\text{ kg/m}^3
Rearranging UX=ρXVgU_X = \rho_X V g allows solving for the unknown fluid density.

Key Concept

Archimedes' Principle and Apparent Weight
Estimated Time:2m 0s
Question 39Question

The maximum acceleration of a body oscillating in simple harmonic motion is 8 m/s28\text{ m/s}^2. If the period of oscillation is π s\pi\text{ s}, calculate the amplitude of the oscillation in meters.

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Answer: 2

Answer

The amplitude of the oscillation is 2.0 m2.0\text{ m}.
The correct answer of 2.0 m2.0\text{ m} is obtained by first deriving the angular frequency ω=2πT=2 rad/s\omega = \frac{2\pi}{T} = 2\text{ rad/s}, and then using the relation amax=ω2Aa_{\text{max}} = \omega^2 A to solve for amplitude: A=822=2.0 mA = \frac{8}{2^2} = 2.0\text{ m}.

Step-by-Step Solution

1
Calculate angular frequency (ω\omega) from the given period (TT).
ω=2πT=2ππ=2 rad/s\omega = \frac{2\pi}{T} = \frac{2\pi}{\pi} = 2\text{ rad/s}
Angular frequency specifies the rate of phase change in oscillations.
2
Apply the maximum acceleration formula for simple harmonic motion to determine amplitude (AA).
amax=ω2A    8=22×A    A=2.0 ma_{\text{max}} = \omega^2 A \implies 8 = 2^2 \times A \implies A = 2.0\text{ m}
In simple harmonic motion, maximum acceleration occurs at the extreme position and equals ω2A\omega^2 A.

Key Concept

Simple Harmonic Motion Acceleration and Period Relationship
Question 40Question

A stone is projected vertically upwards from the top edge of a cliff 80 m80\text{ m} high with an initial speed of 30 m/s30\text{ m/s}. Taking acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2, calculate the total time, in seconds, taken by the stone to reach the ground at the base of the cliff.

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Answer: 8

Answer

The total time taken by the stone to reach the ground at the base of the cliff is 8 s8\text{ s}.
Using the equation of motion s=ut12gt2s = ut - \frac{1}{2}gt^2 with s=80 ms = -80\text{ m}, u=30 m/su = 30\text{ m/s}, and g=10 m/s2g = 10\text{ m/s}^2 yields the quadratic equation t26t16=0t^2 - 6t - 16 = 0. Solving gives t=8 st = 8\text{ s} (ignoring the unphysical negative root t=2 st = -2\text{ s}). Alternatively, breaking the motion into two parts: time to reach maximum height (30 m/s/10 m/s2=3 s30\text{ m/s} / 10\text{ m/s}^2 = 3\text{ s}, covering 45 m45\text{ m}) plus time to fall from maximum height of 125 m125\text{ m} to the ground (t=2(125)/10=5 st = \sqrt{2(125)/10} = 5\text{ s}), giving a total time of 3+5=8 s3 + 5 = 8\text{ s}.

Step-by-Step Solution

1
Set up the kinematic equation with appropriate vector signs
Displacement s=80 ms = -80\text{ m}, initial velocity u=+30 m/su = +30\text{ m/s}, acceleration a=g=10 m/s2a = -g = -10\text{ m/s}^2
Since the ground is below the release point, displacement is negative when taking the upward direction as positive.
2
Substitute values into s=ut+12at2s = ut + \frac{1}{2}at^2
80=30t5t2-80 = 30t - 5t^2
Relates displacement, initial speed, time, and constant gravitational acceleration.
3
Form and solve the quadratic equation
5t230t80=0    t26t16=0    (t8)(t+2)=05t^2 - 30t - 80 = 0 \implies t^2 - 6t - 16 = 0 \implies (t - 8)(t + 2) = 0
Simplifies the algebraic expression to find the time roots.
4
Select the physical root
t=8 st = 8\text{ s}
Time elapsed must be a positive quantity.

Key Concept

Kinematics of Vertical Motion under Gravity with Displacement from Elevation
Estimated Time:2m 0s
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