Mechanics

227 questions

Question 41Question

A projectile is launched from ground level with a horizontal velocity component of 15 m/s15\text{ m/s} and a vertical velocity component of 20 m/s20\text{ m/s}. Neglecting air resistance, what is the magnitude of the velocity of the projectile at its maximum height?

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Answer: 15 m/s15\text{ m/s}

Answer

The magnitude of the velocity of the projectile at its maximum height is 15 m/s15\text{ m/s}.
In projectile motion under gravity without air resistance, the horizontal component of velocity remains constant throughout flight (vx=15 m/sv_x = 15\text{ m/s}). At the highest point (apex), the vertical component of velocity momentarily becomes zero (vy=0 m/sv_y = 0\text{ m/s}). Therefore, the magnitude of the velocity at the maximum height is equal to the horizontal component, which is 15 m/s15\text{ m/s}.

Step-by-Step Solution

1
Identify the velocity components at the maximum height of a projectile
Vertical component vy=0 m/sv_y = 0\text{ m/s} and horizontal component vx=ux=15 m/sv_x = u_x = 15\text{ m/s}.
Gravity acts vertically, reducing vertical velocity to zero at the peak, while horizontal velocity remains constant in the absence of air resistance.
2
Calculate the total magnitude of velocity at maximum height
v=vx2+vy2=152+02=15 m/sv = \sqrt{v_x^2 + v_y^2} = \sqrt{15^2 + 0^2} = 15\text{ m/s}.
The magnitude of the resultant velocity vector is derived using the Pythagorean theorem.

Key Concept

Velocity at Maximum Height in Projectile Motion
Question 42Question

A spherical particle of radius 3.0×103 m3.0 \times 10^{-3}\text{ m} and density 8.0×103 kg/m38.0 \times 10^3\text{ kg/m}^3 is released from rest and falls vertically through a tall column of a viscous liquid of density 2.0×103 kg/m32.0 \times 10^3\text{ kg/m}^3. If the coefficient of viscosity of the fluid is 0.40 Pas0.40\text{ Pa}\cdot\text{s} and the acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2, calculate the magnitude of its terminal velocity in m/s\text{m/s}.

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Answer: 0.3

Answer

The magnitude of the terminal velocity of the falling sphere is 0.3 m/s0.3\text{ m/s}.
When a body falls at terminal velocity through a viscous medium, its weight is balanced by the sum of buoyancy upthrust and Stokes' viscous drag force. Applying vt=2r2(ρsρf)g9ηv_t = \frac{2 r^2 (\rho_s - \rho_f) g}{9 \eta} with sphere radius r=0.003 mr = 0.003\text{ m}, sphere density ρs=8000 kg/m3\rho_s = 8000\text{ kg/m}^3, fluid density ρf=2000 kg/m3\rho_f = 2000\text{ kg/m}^3, viscosity η=0.40 Pas\eta = 0.40\text{ Pa}\cdot\text{s}, and g=10 m/s2g = 10\text{ m/s}^2 yields vt=0.3 m/sv_t = 0.3\text{ m/s}.

Step-by-Step Solution

1
Formulate the dynamic equilibrium condition at terminal velocity.
At terminal velocity, the net acceleration is zero, leading to the force balance equation W=U+FvW = U + F_v, where WW is the gravitational weight of the sphere, UU is the buoyant upthrust, and FvF_v is the retarding viscous force.
Terminal velocity occurs when the downward force of gravity is precisely balanced by the sum of upward resistive and buoyancy forces.
2
Substitute algebraic expressions for weight, upthrust, and Stokes' viscous drag.
W=43πr3ρsgW = \frac{4}{3}\pi r^3 \rho_s g, U=43πr3ρfgU = \frac{4}{3}\pi r^3 \rho_f g, and Fv=6πηrvtF_v = 6\pi \eta r v_t.
Archimedes' principle defines the upthrust force equal to the weight of displaced liquid, while Stokes' law governs viscous resistance on spherical bodies.
3
Solve the equilibrium equation for terminal velocity vtv_t.
vt=2r2(ρsρf)g9ηv_t = \frac{2 r^2 (\rho_s - \rho_f) g}{9 \eta}.
Equating 43πr3(ρsρf)g=6πηrvt\frac{4}{3}\pi r^3 (\rho_s - \rho_f) g = 6\pi \eta r v_t and simplifying cancels common factors of π\pi and rr.
4
Substitute the specified numerical parameters into the derived expression.
vt=2×(3.0×103)2×(80002000)×109×0.40=2×9.0×106×6000×103.6=1.083.6=0.3 m/sv_t = \frac{2 \times (3.0 \times 10^{-3})^2 \times (8000 - 2000) \times 10}{9 \times 0.40} = \frac{2 \times 9.0 \times 10^{-6} \times 6000 \times 10}{3.6} = \frac{1.08}{3.6} = 0.3\text{ m/s}.
Direct calculation yields the exact value of terminal velocity.

Key Concept

Terminal Velocity, Stokes' Law, and Archimedes' Principle
Question 43Question

A uniform spherical planet has twice the mass and twice the radius of the Earth. If the acceleration due to gravity at the Earth's surface is gg, what is the acceleration due to gravity at the surface of this planet?

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Answer: 0.5g0.5g

Answer

The acceleration due to gravity at the surface of the planet is 0.5g0.5g.
The acceleration due to gravity at a planet's surface is given by g=GMR2g = \frac{GM}{R^2}. Doubling the mass doubles the field strength, but doubling the radius reduces the field strength by a factor of 22=42^2 = 4 due to the inverse-square law. Combining these changes results in 24g=0.5g\frac{2}{4}g = 0.5g.

Step-by-Step Solution

1
Write the general expression for surface acceleration due to gravity.
g=GMR2g = \frac{GM}{R^2}, where GG is the gravitational constant, MM is planetary mass, and RR is planetary radius.
Establishes the fundamental formula relating gravity to mass and radius.
2
Substitute the given parameters for the new planet (Mp=2MM_p = 2M and Rp=2RR_p = 2R).
gp=G(2M)(2R)2=2GM4R2g_p = \frac{G(2M)}{(2R)^2} = \frac{2GM}{4R^2}.
Applies the proportional changes to mass and radius into the formula.
3
Simplify the expression to find gpg_p in terms of gg.
gp=24(GMR2)=0.5gg_p = \frac{2}{4} \left(\frac{GM}{R^2}\right) = 0.5g.
Evaluates the fractional change relative to Earth's surface gravity.

Key Concept

Dependence of surface gravitational field strength on planetary mass and radius via the inverse-square law.
Estimated Time:1m 15s
Question 44Question

The speed vv of a transverse wave traveling along a stretched string under tension TT with mass per unit length μ\mu is given by v=kTxμyv = k T^x \mu^y, where kk is a dimensionless constant. What is the numerical value of the exponent xx?

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Answer: 0.5

Answer

The numerical value of the exponent xx is 0.5.
Applying the principle of dimensional homogeneity, the dimensions on both sides must match. Speed [v]=LT1[v] = L T^{-1}, tension force [T]=MLT2[T] = M L T^{-2}, and mass per unit length [μ]=ML1[\mu] = M L^{-1}. Substituting these into v=kTxμyv = k T^x \mu^y yields M0L1T1=Mx+yLxyT2xM^0 L^1 T^{-1} = M^{x+y} L^{x-y} T^{-2x}. Comparing the exponents of TT gives 2x=1-2x = -1, leading to x=0.5x = 0.5.

Step-by-Step Solution

1
Determine the dimensions of speed vv, tension force TT, and linear density μ\mu.
[v]=LT1[v] = L T^{-1}, [T]=MLT2[T] = M L T^{-2}, [μ]=ML1[\mu] = M L^{-1}
Tension is a force (F=maF=ma) with dimensions [MLT2][M L T^{-2}], and μ\mu is mass per unit length (m/lm/l) with dimensions [ML1][M L^{-1}].
2
Substitute the dimensional formulas into the equation v=kTxμyv = k T^x \mu^y and collect powers of base dimensions.
M0L1T1=Mx+yLxyT2xM^0 L^1 T^{-1} = M^{x+y} L^{x-y} T^{-2x}
Combining exponents for base dimensions MM, LL, and TT allows applying the principle of dimensional homogeneity.
3
Equate the exponent of TT on both sides to solve for xx.
2x=1    x=0.5-2x = -1 \implies x = 0.5
The exponent of TT on the left side is 1-1 and on the right side is 2x-2x.

Key Concept

Dimensional Analysis and Determination of Exponents
Estimated Time:1m 30s
Question 45Question

A solid cylinder of length 10 cm10\text{ cm} floats vertically at the interface of two immiscible liquids: oil of density 800 kg/m3800\text{ kg/m}^3 and water of density 1000 kg/m31000\text{ kg/m}^3. If 4 cm4\text{ cm} of its length is submerged in water while the remaining 6 cm6\text{ cm} is submerged in oil, what is the density of the cylinder?

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Answer: 880 kg/m3880\text{ kg/m}^3

Answer

The density of the cylinder is 880 kg/m3880\text{ kg/m}^3.
According to the Law of Flotation, a floating body displaces its own weight of the fluids in which it floats. For a body submerged across two immiscible liquids, the total buoyant force is the sum of the upthrusts from both fluids: U=(ρwVw+ρoVo)gU = (\rho_w V_w + \rho_o V_o)g. Equating this to the total weight W=ρcVtotalgW = \rho_c V_{total} g yields ρc(0.10 m)=1000(0.04 m)+800(0.06 m)=88\rho_c (0.10\text{ m}) = 1000(0.04\text{ m}) + 800(0.06\text{ m}) = 88, which gives ρc=880 kg/m3\rho_c = 880\text{ kg/m}^3.

Step-by-Step Solution

1
Set up the condition for flotation.
Weight of the cylinder = Total upthrust exerted by both liquids.
For a body floating in equilibrium, its total weight is balanced by the sum of buoyant forces from all surrounding fluids.
2
Express the weight and upthrusts in terms of density, cross-sectional area AA, length LL, and acceleration due to gravity gg.
ρcALg=(ρwAhw+ρoAho)g\rho_c A L g = (\rho_w A h_w + \rho_o A h_o) g
The weight of the cylinder is ρcVtotalg\rho_c V_{total} g and upthrust from each liquid is ρliquidVsubmergedg\rho_{liquid} V_{submerged} g.
3
Cancel common factors AA and gg from both sides.
ρcL=ρwhw+ρoho\rho_c L = \rho_w h_w + \rho_o h_o
Since the cylinder has a uniform cross-sectional area, volume ratio simplifies to length ratio.
4
Substitute the given values (L=0.10 mL = 0.10\text{ m}, hw=0.04 mh_w = 0.04\text{ m}, ho=0.06 mh_o = 0.06\text{ m}, ρw=1000 kg/m3\rho_w = 1000\text{ kg/m}^3, ρo=800 kg/m3\rho_o = 800\text{ kg/m}^3).
ρc(0.10)=1000(0.04)+800(0.06)=40+48=88 kg/m2\rho_c (0.10) = 1000(0.04) + 800(0.06) = 40 + 48 = 88\text{ kg/m}^2
Evaluating the weighted contribution of buoyancy from each fluid.
5
Solve for the density of the cylinder ρc\rho_c.
ρc=880.10=880 kg/m3\rho_c = \frac{88}{0.10} = 880\text{ kg/m}^3
Dividing both sides by the total length of 0.10 m0.10\text{ m} gives the density.

Key Concept

Archimedes' Principle for Floating Bodies in Immiscible Liquids
Question 46Question

A screw jack with a thread pitch of 0.5 cm0.5\text{ cm} is operated using a Tommy bar of length 35 cm35\text{ cm}. If the machine has an efficiency of 40%40\%, what is the minimum effort force required to raise a load of mass 880 kg880\text{ kg}? (Take g=10 m/s2g = 10\text{ m/s}^2 and π=227\pi = \frac{22}{7})

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Answer: 50 N50\text{ N}

Answer

The minimum effort force required is 50 N50\text{ N}.
The effort distance per turn is the circumference 2πr=2×227×35 cm=220 cm2\pi r = 2 \times \frac{22}{7} \times 35\text{ cm} = 220\text{ cm}. Dividing by the pitch (0.5 cm0.5\text{ cm}) yields a Velocity Ratio of 440440. Applying the 40%40\% efficiency gives a Mechanical Advantage of MA=0.40×440=176\text{MA} = 0.40 \times 440 = 176. Finally, dividing the load force (8800 N8800\text{ N}) by MA\text{MA} gives an effort force of 50 N50\text{ N}.

Step-by-Step Solution

1
Calculate the total load force in Newtons
L=mg=880 kg×10 m/s2=8800 NL = m \cdot g = 880\text{ kg} \times 10\text{ m/s}^2 = 8800\text{ N}
Effort overcomes weight force, which is mass multiplied by gravitational acceleration.
2
Calculate the Velocity Ratio (VR) of the screw jack
VR=2πrp=2×227×35 cm0.5 cm=220 cm0.5 cm=440\text{VR} = \frac{2 \pi r}{p} = \frac{2 \times \frac{22}{7} \times 35\text{ cm}}{0.5\text{ cm}} = \frac{220\text{ cm}}{0.5\text{ cm}} = 440
The effort travels around the circumference of a circle of radius rr, while the load moves vertically by one pitch length pp per revolution.
3
Determine the Mechanical Advantage (MA) from efficiency
MA=η×VR=0.40×440=176\text{MA} = \eta \times \text{VR} = 0.40 \times 440 = 176
Efficiency is defined as η=MAVR\eta = \frac{\text{MA}}{\text{VR}}, so MA=ηVR\text{MA} = \eta \cdot \text{VR}.
4
Calculate the effort force E
E=LMA=8800 N176=50 NE = \frac{L}{\text{MA}} = \frac{8800\text{ N}}{176} = 50\text{ N}
Mechanical advantage is the ratio of load to effort force (MA=LE)(\text{MA} = \frac{L}{E}).

Key Concept

Relationship between Velocity Ratio, Mechanical Advantage, Efficiency, and Pitch in a Screw Jack
Question 47Question

A constant net force of 20 N20\text{ N} acts on an object of mass 4 kg4\text{ kg} that is initially at rest on a frictionless horizontal surface. What is the magnitude of the linear momentum of the object after 3 s3\text{ s}?

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Answer: 60

Answer

The magnitude of the linear momentum of the object after 3 s3\text{ s} is 60 kg m s160\text{ kg m s}^{-1}.
According to Newton's Second Law in terms of momentum, force is the rate of change of linear momentum (F=ΔpΔtF = \frac{\Delta p}{\Delta t}). Rearranging gives Δp=FΔt\Delta p = F \Delta t. Since the object is initially at rest (pi=0 kg m s1p_i = 0\text{ kg m s}^{-1}), the final momentum is pf=FΔt=20 N×3 s=60 kg m s1p_f = F \Delta t = 20\text{ N} \times 3\text{ s} = 60\text{ kg m s}^{-1}.

Step-by-Step Solution

1
Apply the impulse-momentum theorem.
J=FΔt=ΔpJ = F \Delta t = \Delta p
The impulse of the net force acting on an object equals the change in its linear momentum.
2
Calculate the final linear momentum.
pf=20 N×3 s=60 kg m s1p_f = 20\text{ N} \times 3\text{ s} = 60\text{ kg m s}^{-1}
Since the object starts from rest, its initial momentum is zero (pi=0p_i = 0), so the final momentum is equal to the total impulse supplied.

Key Concept

Impulse-Momentum Theorem
Question 48Question

The viscous drag force FF acting on a spherical body moving through a fluid at speed vv is given by Stokes' law, F=6πηrvF = 6 \pi \eta r v, where rr is the radius of the sphere and η\eta is the coefficient of viscosity. What is the dimensional formula of the coefficient of viscosity η\eta?

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Answer: M L1T1\text{M L}^{-1} \text{T}^{-1}

Answer

The dimensional formula of the coefficient of viscosity is M L1T1\text{M L}^{-1} \text{T}^{-1}.
Isolating the coefficient of viscosity from Stokes' law yields η=F6πrv\eta = \frac{F}{6\pi r v}. Substituting the dimensions [F]=M L T2[F] = \text{M L T}^{-2}, [r]=L[r] = \text{L}, and [v]=L T1[v] = \text{L T}^{-1} gives [η]=M L T2L2T1=M L1T1[\eta] = \frac{\text{M L T}^{-2}}{\text{L}^2 \text{T}^{-1}} = \text{M L}^{-1} \text{T}^{-1}.

Step-by-Step Solution

1
Identify the dimensional formulas for force, radius, and velocity.
[F]=M L T2[F] = \text{M L T}^{-2}, [r]=L[r] = \text{L}, and [v]=L T1[v] = \text{L T}^{-1}.
Base physical quantities must be represented by their fundamental dimensions.
2
Rearrange Stokes' law to express η\eta in terms of the other variables, treating 6π6\pi as a dimensionless constant.
[η]=[F][r][v][\eta] = \frac{[F]}{[r][v]}.
Numerical constants do not carry physical dimensions.
3
Substitute the base dimensions into the formula and simplify using index rules.
[η]=M L T2LL T1=M L T2L2T1=M L1T1[\eta] = \frac{\text{M L T}^{-2}}{\text{L} \cdot \text{L T}^{-1}} = \frac{\text{M L T}^{-2}}{\text{L}^2 \text{T}^{-1}} = \text{M L}^{-1} \text{T}^{-1}.
Subtracting denominator indices from numerator indices yields the final dimensional expression.

Key Concept

Dimensional analysis of physical constants and equations
Question 49Question

An electric train starts from rest and accelerates uniformly at 2 m/s22\text{ m/s}^2 for a time interval tt. It then maintains the maximum velocity attained for a time interval of tt. Finally, it decelerates uniformly at 4 m/s24\text{ m/s}^2 until it comes to a complete stop. If the total distance covered during the entire journey is 350 m350\text{ m}, what is the value of tt?

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Answer: 10 s10\text{ s}

Answer

10 s10\text{ s}
The motion consists of three stages: acceleration from rest (s1=t2s_1 = t^2), uniform velocity (s2=2t2s_2 = 2t^2), and deceleration to rest (s3=0.5t2s_3 = 0.5t^2). Adding these gives a total distance of S=3.5t2S = 3.5t^2. Setting 3.5t2=350 m3.5t^2 = 350\text{ m} yields t2=100t^2 = 100, so t=10 st = 10\text{ s}.

Step-by-Step Solution

1
Analyze Stage 1 (Acceleration phase)
Maximum velocity v=2tv = 2t, displacement s1=12(2)t2=t2s_1 = \frac{1}{2}(2)t^2 = t^2
Starting from rest (u=0u = 0) with acceleration a1=2 m/s2a_1 = 2\text{ m/s}^2 for duration tt, v=u+a1t=2tv = u + a_1 t = 2t and s1=12a1t2=t2s_1 = \frac{1}{2} a_1 t^2 = t^2.
2
Analyze Stage 2 (Constant velocity phase)
Displacement s2=(2t)(t)=2t2s_2 = (2t)(t) = 2t^2
The train moves at constant velocity v=2tv = 2t for duration tt, so distance is velocity multiplied by time.
3
Analyze Stage 3 (Deceleration phase)
Deceleration time t3=0.5tt_3 = 0.5t, displacement s3=0.5t2s_3 = 0.5t^2
Decelerating from v=2tv = 2t to 00 at a2=4 m/s2a_2 = 4\text{ m/s}^2 takes time t3=va2=2t4=0.5tt_3 = \frac{v}{a_2} = \frac{2t}{4} = 0.5t. Distance s3=12vt3=12(2t)(0.5t)=0.5t2s_3 = \frac{1}{2} v t_3 = \frac{1}{2} (2t)(0.5t) = 0.5t^2.
4
Calculate total displacement and solve for tt
Total distance S=3.5t2=350    t2=100    t=10 sS = 3.5t^2 = 350 \implies t^2 = 100 \implies t = 10\text{ s}
Summing the displacements: S=t2+2t2+0.5t2=3.5t2S = t^2 + 2t^2 + 0.5t^2 = 3.5t^2. Equating to 350 m350\text{ m} gives 3.5t2=3503.5t^2 = 350, so t2=100t^2 = 100, giving t=10 st = 10\text{ s}.

Key Concept

Multi-stage linear motion and displacement calculation
Estimated Time:2m 0s
Question 50Question

A spherical planet has a radius of 7.2×106 m7.2 \times 10^{6} \text{ m} and an acceleration due to gravity of 10 m/s210 \text{ m/s}^2 at its surface. What is the escape velocity for an object launched from the surface of this planet, in km/s\text{km/s}?

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Answer: 12

Answer

The escape velocity from the surface of the planet is 12 km/s.
The escape velocity vev_e from the surface of a spherical planet of radius RR with surface gravity gg is given by ve=2gRv_e = \sqrt{2gR}. Substituting g=10 m/s2g = 10 \text{ m/s}^2 and R=7.2×106 mR = 7.2 \times 10^6 \text{ m} yields ve=2×10×7.2×106=1.44×108=12000 m/sv_e = \sqrt{2 \times 10 \times 7.2 \times 10^6} = \sqrt{1.44 \times 10^8} = 12000 \text{ m/s}, which equals 12 km/s12 \text{ km/s}.

Step-by-Step Solution

1
Identify the relationship between surface gravity, planetary radius, and escape velocity
The escape velocity formula is ve=2gRv_e = \sqrt{2gR}.
Escape velocity is the minimum initial speed required for an object to overcome the gravitational pull of a celestial body.
2
Substitute the given numerical values into the formula
ve=2×10 m/s2×7.2×106 m=144×106 m/sv_e = \sqrt{2 \times 10 \text{ m/s}^2 \times 7.2 \times 10^6 \text{ m}} = \sqrt{144 \times 10^6} \text{ m/s}.
Plugging in the given values allows direct calculation of the velocity in standard SI units.
3
Simplify the square root and convert units to km/s
ve=12000 m/s=12 km/sv_e = 12000 \text{ m/s} = 12 \text{ km/s}.
Taking the square root of 144×106144 \times 10^6 gives 12000 m/s12000 \text{ m/s}, which corresponds to 12 km/s12 \text{ km/s}.

Key Concept

Escape Velocity from a Planet's Surface
Question 51Question

A toy truck of mass 2.5 kg2.5\text{ kg} moving at a velocity of 6.0 m s16.0\text{ m s}^{-1} collides head-on with a toy car of mass 1.5 kg1.5\text{ kg} moving in the opposite direction at 2.0 m s12.0\text{ m s}^{-1}. If the two vehicles stick together upon impact, what is their combined velocity immediately after the collision?

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Answer: 3.0 m s13.0\text{ m s}^{-1}

Answer

3.0 m s13.0\text{ m s}^{-1} in the direction of the initial motion of the truck
According to the principle of conservation of linear momentum, total initial momentum equals total final momentum. Taking the direction of the toy truck as positive gives an initial momentum of (2.5 kg×6.0 m s1)+(1.5 kg×2.0 m s1)=15.03.0=12.0 kg m s1(2.5\text{ kg} \times 6.0\text{ m s}^{-1}) + (1.5\text{ kg} \times -2.0\text{ m s}^{-1}) = 15.0 - 3.0 = 12.0\text{ kg m s}^{-1}. Dividing this net momentum by the combined mass (2.5 kg+1.5 kg=4.0 kg)(2.5\text{ kg} + 1.5\text{ kg} = 4.0\text{ kg}) yields a common final velocity of 3.0 m s13.0\text{ m s}^{-1}.

Step-by-Step Solution

1
Assign direction signs to the velocity vectors
Let the initial direction of the truck be positive (u1=+6.0 m s1u_1 = +6.0\text{ m s}^{-1}). The car moves in the opposite direction, so its velocity is negative (u2=2.0 m s1u_2 = -2.0\text{ m s}^{-1}).
Linear momentum is a vector quantity, so direction must be accounted for in one-dimensional motion.
2
Calculate the total initial momentum of the system
pinitial=m1u1+m2u2=(2.5×6.0)+(1.5×2.0)=15.03.0=12.0 kg m s1p_{\text{initial}} = m_1 u_1 + m_2 u_2 = (2.5 \times 6.0) + (1.5 \times -2.0) = 15.0 - 3.0 = 12.0\text{ kg m s}^{-1}
The total momentum before collision is the vector sum of individual momenta.
3
Apply the law of conservation of linear momentum to solve for common final velocity vv
pfinal=(m1+m2)v=(2.5+1.5)v=4.0vp_{\text{final}} = (m_1 + m_2) v = (2.5 + 1.5) v = 4.0 v. Setting pfinal=pinitial4.0v=12.0v=3.0 m s1p_{\text{final}} = p_{\text{initial}} \Rightarrow 4.0 v = 12.0 \Rightarrow v = 3.0\text{ m s}^{-1}.
Since the vehicles stick together, they move as a single combined mass.

Key Concept

Conservation of Linear Momentum in Inelastic Collisions
Estimated Time:50s
Question 52Question

An aircraft flies due East at a velocity of 120 m/s120\text{ m/s} while a crosswind blows due North at 50 m/s50\text{ m/s}. What is the magnitude of the resultant velocity of the aircraft?

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Answer: 130 m/s130\text{ m/s}

Answer

The magnitude of the resultant velocity of the aircraft is 130 m/s130\text{ m/s}.
Because the aircraft's velocity and the wind's velocity are perpendicular to each other, their vector sum is found using the Pythagorean theorem R=v12+v22R = \sqrt{v_1^2 + v_2^2}. Substituting 120 m/s120\text{ m/s} and 50 m/s50\text{ m/s} gives R=1202+502=16900=130 m/sR = \sqrt{120^2 + 50^2} = \sqrt{16900} = 130\text{ m/s}.

Step-by-Step Solution

1
Identify the given velocity vectors and their relative direction.
Velocity due East ve=120 m/s\vec{v}_e = 120\text{ m/s} and velocity due North vn=50 m/s\vec{v}_n = 50\text{ m/s} are perpendicular to each other (9090^\circ angle).
East and North directions are orthogonal to each other.
2
Apply the Pythagorean theorem to calculate the magnitude of the resultant vector RR.
R=ve2+vn2=1202+502=14400+2500=16900=130 m/sR = \sqrt{v_e^2 + v_n^2} = \sqrt{120^2 + 50^2} = \sqrt{14400 + 2500} = \sqrt{16900} = 130\text{ m/s}.
The resultant of two perpendicular vectors forms the hypotenuse of a right-angled triangle.

Key Concept

Vector Addition of Perpendicular Vectors
Estimated Time:1m 0s
Question 53Question

A projectile is launched from ground level over flat terrain with a constant horizontal velocity component of 10 m/s10\text{ m/s}. At a height of 40 m40\text{ m} above the ground, the magnitude of its vertical velocity component is equal to its horizontal velocity component. Taking g=10 m/s2g = 10\text{ m/s}^2, calculate the maximum height reached by the projectile in meters.

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Answer: 45

Answer

The maximum height reached by the projectile is 45 m45\text{ m}.
At the height of 40 m40\text{ m}, the vertical velocity is equal to the horizontal velocity of 10 m/s10\text{ m/s}. Applying the vertical kinematic relation vy2=uy22ghv_y^2 = u_y^2 - 2gh yields 102=uy22(10)(40)10^2 = u_y^2 - 2(10)(40), which gives uy2=900 m2/s2u_y^2 = 900\text{ m}^2/\text{s}^2. The maximum height attained above ground level occurs when vy=0v_y = 0, calculated as Hmax=uy22g=90020=45 mH_{\text{max}} = \frac{u_y^2}{2g} = \frac{900}{20} = 45\text{ m}.

Step-by-Step Solution

1
Identify the vertical component of velocity at the given height
vy=10 m/sv_y = 10\text{ m/s} at h=40 mh = 40\text{ m}
The problem states that at h=40 mh = 40\text{ m}, the vertical velocity component equals the constant horizontal component ux=10 m/su_x = 10\text{ m/s}.
2
Determine the initial vertical launch velocity component uyu_y
uy2=900 m2/s2    uy=30 m/su_y^2 = 900\text{ m}^2/\text{s}^2 \implies u_y = 30\text{ m/s}
Applying the vertical motion equation vy2=uy22ghv_y^2 = u_y^2 - 2gh gives 102=uy22(10)(40)    uy2=100+800=90010^2 = u_y^2 - 2(10)(40) \implies u_y^2 = 100 + 800 = 900.
3
Calculate the maximum height HmaxH_{\text{max}}
Hmax=45 mH_{\text{max}} = 45\text{ m}
At maximum height, the vertical velocity becomes zero. Using Hmax=uy22g=90020=45 mH_{\text{max}} = \frac{u_y^2}{2g} = \frac{900}{20} = 45\text{ m}.

Key Concept

Vertical Kinematics and Maximum Height of a Projectile
Question 54Question

A satellite orbits the Earth at an altitude equal to three times the radius of the Earth, RR. If the acceleration due to gravity at the Earth's surface is gg, what is the gravitational field strength experienced by the satellite at its orbit?

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Answer: g16\frac{g}{16}

Answer

The gravitational field strength at the orbital position is g16\frac{g}{16}.
The total distance from the center of the Earth to the satellite is r=R+3R=4Rr = R + 3R = 4R. Since gravitational field strength is inversely proportional to the square of the distance from the center of mass, increasing the distance by a factor of 44 reduces the field strength by a factor of 42=164^2 = 16, giving g16\frac{g}{16}.

Step-by-Step Solution

1
Determine the total distance from the center of the Earth to the satellite.
The orbital radius is r=R+h=R+3R=4Rr = R + h = R + 3R = 4R.
Gravitational calculations must be measured from the center of mass of the attracting body, not its surface.
2
Apply Newton's law of universal gravitation for gravitational field strength.
At the surface (r=Rr = R), g=GMR2g = \frac{GM}{R^2}. At orbit (r=4Rr = 4R), g=GM(4R)2=GM16R2g' = \frac{GM}{(4R)^2} = \frac{GM}{16R^2}.
Gravitational field strength follows an inverse-square law with respect to distance from the center of mass.
3
Express the orbital gravitational field strength in terms of the surface gravity gg.
g=116(GMR2)=g16g' = \frac{1}{16} \left(\frac{GM}{R^2}\right) = \frac{g}{16}.
Substituting the surface value g=GMR2g = \frac{GM}{R^2} yields the simplified ratio.

Key Concept

Gravitational Field Strength and Inverse-Square Law
Question 55Question

A body of mass 4 kg4\text{ kg} moves with a constant velocity of 5 m s15\text{ m s}^{-1}. Calculate the kinetic energy of the body in Joules.

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Answer: 50

Answer

The kinetic energy of the body is 50 J50\text{ J}.
The kinetic energy of an object in linear motion is calculated using Ek=12mv2E_k = \frac{1}{2} m v^2. Substituting m=4 kgm = 4\text{ kg} and v=5 m s1v = 5\text{ m s}^{-1} gives Ek=12×4×52=50 JE_k = \frac{1}{2} \times 4 \times 5^2 = 50\text{ J}.

Step-by-Step Solution

1
Identify the given physical quantities
Mass m=4 kgm = 4\text{ kg} and velocity v=5 m s1v = 5\text{ m s}^{-1}
Extract values provided in the problem statement.
2
Apply the formula for kinetic energy
Ek=12mv2E_k = \frac{1}{2} m v^2
Kinetic energy is defined as half the product of mass and the square of velocity.
3
Substitute values and solve
Ek=12×4×(5)2=50 JE_k = \frac{1}{2} \times 4 \times (5)^2 = 50\text{ J}
Perform arithmetic evaluation to get the final energy in Joules.

Key Concept

Kinetic Energy
Question 56Question

A particle is projected from horizontal ground at an initial angle θ\theta to the horizontal. At its maximum height H=20 mH = 20\text{ m}, its kinetic energy is exactly half of its initial kinetic energy at launch. Taking acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2, what is the horizontal range of the projectile?

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Answer: 80 m80\text{ m}

Answer

The horizontal range of the projectile is 80 m80\text{ m}.
At the trajectory's highest point, the vertical component of velocity becomes zero while the horizontal component ucosθu\cos\theta remains unchanged. The kinetic energy at the apex is therefore 12m(ucosθ)2=Ek,icos2θ\frac{1}{2}m(u\cos\theta)^2 = E_{k,i}\cos^2\theta. Setting cos2θ=12\cos^2\theta = \frac{1}{2} gives θ=45\theta = 45^\circ. For a 4545^\circ launch angle, the horizontal range R=u2gR = \frac{u^2}{g} is related to the maximum height H=u24gH = \frac{u^2}{4g} by R=4HR = 4H. Substituting H=20 mH = 20\text{ m} yields R=80 mR = 80\text{ m}.

Step-by-Step Solution

1
Relate kinetic energy at maximum height to initial kinetic energy.
Initial kinetic energy Ek(0)=12mu2E_k(0) = \frac{1}{2}m u^2. At peak height, vertical velocity component vy=0v_y = 0, so velocity is vx=ucosθv_x = u\cos\theta. Thus, Ek(peak)=12m(ucosθ)2=Ek(0)cos2θE_k(\text{peak}) = \frac{1}{2}m (u\cos\theta)^2 = E_k(0)\cos^2\theta.
At maximum height, only the horizontal component of velocity remains.
2
Calculate the launch angle θ\theta.
Given Ek(peak)=12Ek(0)E_k(\text{peak}) = \frac{1}{2} E_k(0), we have cos2θ=12\cos^2\theta = \frac{1}{2}, giving θ=45\theta = 45^\circ.
Setting the energy expression equal to the given condition enables solving for the angle.
3
Relate maximum height HH to horizontal range RR for θ=45\theta = 45^\circ.
For θ=45\theta = 45^\circ, H=u2sin2(45)2g=u24gH = \frac{u^2 \sin^2(45^\circ)}{2g} = \frac{u^2}{4g} and R=u2sin(90)g=u2gR = \frac{u^2 \sin(90^\circ)}{g} = \frac{u^2}{g}. Therefore, R=4HR = 4H.
Standard formulas for maximum height and range express both quantities in terms of launch speed uu and acceleration due to gravity gg.
4
Substitute the maximum height value into the range formula.
R=4×20 m=80 mR = 4 \times 20\text{ m} = 80\text{ m}.
Multiplying the given peak height of 20 m20\text{ m} by 44 yields the exact horizontal range.

Key Concept

Kinetic Energy Conservation and Range-Height Relationship in Projectile Motion
Estimated Time:2m 0s
Question 57Question

A uniform wooden cube of edge length 0.20 m0.20\text{ m} floats in water of density 1000 kg/m31000\text{ kg/m}^3 with 0.15 m0.15\text{ m} of its vertical height submerged. Taking acceleration due to gravity g=10 m/s2g = 10\text{ m/s}^2, what minimum mass, in kilograms, must be placed on the top surface of the cube so that its upper face becomes just flush with the water surface?

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Answer: 2

Answer

The minimum mass required to submerge the cube completely flush with the water surface is 2.0 kg2.0\text{ kg}.
By the Law of Flotation, a floating body displaces its own weight of fluid. Initially, the cube displaces a volume of 0.20 m×0.20 m×0.15 m=0.006 m30.20\text{ m} \times 0.20\text{ m} \times 0.15\text{ m} = 0.006\text{ m}^3 of water, corresponding to an upthrust of 60 N60\text{ N} (or mass of 6.0 kg6.0\text{ kg}). When completely submerged, the total volume displaced is 0.203=0.008 m30.20^3 = 0.008\text{ m}^3, providing a total upthrust of 80 N80\text{ N} (or mass equivalent of 8.0 kg8.0\text{ kg}). The additional mass required on top is therefore the difference: 8.0 kg6.0 kg=2.0 kg8.0\text{ kg} - 6.0\text{ kg} = 2.0\text{ kg}.

Step-by-Step Solution

1
Calculate the cross-sectional area of the cube
A=(0.20 m)2=0.04 m2A = (0.20\text{ m})^2 = 0.04\text{ m}^2
The base area is needed to find the volume of the block submerged and unsubmerged.
2
Calculate the volume of the cube above the water surface
Vabove=0.04 m2×(0.20 m0.15 m)=0.002 m3V_{\text{above}} = 0.04\text{ m}^2 \times (0.20\text{ m} - 0.15\text{ m}) = 0.002\text{ m}^3
To push the cube level with the surface, the additional weight added on top must balance the extra upthrust created by submerging this remaining volume.
3
Calculate the additional mass required
m=ρwater×Vabove=1000 kg/m3×0.002 m3=2.0 kgm = \rho_{\text{water}} \times V_{\text{above}} = 1000\text{ kg/m}^3 \times 0.002\text{ m}^3 = 2.0\text{ kg}
By Archimedes' principle, the additional downward mass must equal the mass of the extra water displaced when fully submerged.

Key Concept

Archimedes' Principle and Law of Flotation
Question 58Question

A shell of total mass 5.0 kg5.0\text{ kg} is moving horizontally with a velocity of 20 m s120\text{ m s}^{-1} when an internal explosion splits it into two fragments. One fragment of mass 2.0 kg2.0\text{ kg} is propelled backward along the original path at a speed of 10 m s110\text{ m s}^{-1}. What is the magnitude of the velocity, in m s1\text{m s}^{-1}, of the second fragment immediately after the explosion?

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Answer: 40

Answer

The magnitude of the velocity of the second fragment immediately after the explosion is 40 m s140\text{ m s}^{-1}.
According to the Law of Conservation of Linear Momentum, the total momentum of a system remains constant when no net external horizontal force acts on it. Taking the original direction of motion as positive, the initial momentum is 100 kg m s1100\text{ kg m s}^{-1}. Since the 2.0 kg2.0\text{ kg} fragment moves backward at 10 m s110\text{ m s}^{-1}, its momentum is 20 kg m s1-20\text{ kg m s}^{-1}. For total momentum to remain +100 kg m s1+100\text{ kg m s}^{-1}, the remaining 3.0 kg3.0\text{ kg} fragment must carry a momentum of +120 kg m s1+120\text{ kg m s}^{-1}, which corresponds to a velocity of 40 m s140\text{ m s}^{-1}.

Step-by-Step Solution

1
Calculate the initial momentum of the shell prior to the explosion.
pi=5.0 kg×20 m s1=100 kg m s1p_i = 5.0\text{ kg} \times 20\text{ m s}^{-1} = 100\text{ kg m s}^{-1} in the initial forward direction.
Before the internal explosion, the system consists of a single mass moving with a constant velocity.
2
Apply the Law of Conservation of Linear Momentum taking vector direction into account.
pi=m1v1+m2v2    100=2.0(10)+3.0v2p_i = m_1 v_1 + m_2 v_2 \implies 100 = 2.0(-10) + 3.0 v_2
In the absence of external forces, total momentum is conserved. The fragment propelled backward takes a negative sign relative to the initial forward motion.
3
Solve the algebraic equation for the unknown velocity v2v_2.
100+20=3.0v2    120=3.0v2    v2=40 m s1100 + 20 = 3.0 v_2 \implies 120 = 3.0 v_2 \implies v_2 = 40\text{ m s}^{-1}
Isolating v2v_2 gives the forward velocity magnitude of the remaining 3.0 kg3.0\text{ kg} piece.

Key Concept

Conservation of Linear Momentum in Explosions (1D Vector Sign Convention)
Question 59Question

A block is pulled along a smooth horizontal table by a horizontal force of 30 N30\text{ N} through a displacement of 4 m4\text{ m}. At the same time, a vertical upward force of 40 N40\text{ N} acts on the block as it moves. What is the total work done on the block?

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Answer: 120 J120\text{ J}

Answer

The total work done on the block is 120 J120\text{ J}.
Work done is given by W=FdcosθW = F d \cos\theta. The horizontal force acts along the line of motion (θ=0\theta = 0^\circ), performing 30 N×4 m=120 J30\text{ N} \times 4\text{ m} = 120\text{ J} of work. The vertical force acts at an angle of 9090^\circ to the horizontal displacement, performing zero work because cos(90)=0\cos(90^\circ) = 0. Thus, the total work done is 120 J120\text{ J}.

Step-by-Step Solution

1
Identify the formula for work done by a constant force
W=Fdcos(θ)W = F \cdot d \cdot \cos(\theta)
Work is defined as the scalar product of force and displacement vectors.
2
Calculate work done by the horizontal force
Whorizontal=30 N×4 m×cos(0)=120 JW_{\text{horizontal}} = 30\text{ N} \times 4\text{ m} \times \cos(0^\circ) = 120\text{ J}
The horizontal force is in the exact direction of motion (θ=0\theta = 0^\circ).
3
Calculate work done by the vertical force
Wvertical=40 N×4 m×cos(90)=0 JW_{\text{vertical}} = 40\text{ N} \times 4\text{ m} \times \cos(90^\circ) = 0\text{ J}
The vertical force is perpendicular to the horizontal displacement (θ=90\theta = 90^\circ), so cos(90)=0\cos(90^\circ) = 0.
4
Sum the work done by all forces
Wtotal=120 J+0 J=120 JW_{\text{total}} = 120\text{ J} + 0\text{ J} = 120\text{ J}
Work is a scalar quantity, so total work is the algebraic sum of individual work values.

Key Concept

Work done by perpendicular forces is zero
Estimated Time:45s
Question 60Question

Match each displacement vector combination on the left with its corresponding resultant displacement magnitude or vector on the right.

Click a left item, then click its matching right item

Items

A walk of 3 m3\text{ m} East followed by 4 m4\text{ m} North
A walk of 5 m5\text{ m} East followed by 12 m12\text{ m} South
A walk of 8 m8\text{ m} East followed by 6 m6\text{ m} West
A walk of 9 m9\text{ m} North followed by 12 m12\text{ m} East

Matches

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Answer

The correct pairs correspond as follows: 3 m3\text{ m} East and 4 m4\text{ m} North matches a resultant magnitude of 5 m5\text{ m}; 5 m5\text{ m} East and 12 m12\text{ m} South matches a resultant magnitude of 13 m13\text{ m}; 8 m8\text{ m} East and 6 m6\text{ m} West matches a resultant displacement of 2 m2\text{ m} East; and 9 m9\text{ m} North and 12 m12\text{ m} East matches a resultant magnitude of 15 m15\text{ m}.
Each vector combination is resolved according to its directional alignment: perpendicular displacements require the Pythagorean theorem (R=A2+B2R = \sqrt{A^2 + B^2}), whereas anti-parallel collinear displacements require vector subtraction.

Step-by-Step Solution

1
Identify orthogonal vector scenarios
Perpendicular displacement vectors form right-angled triangles.
Directions such as East-North, East-South, and North-East are at 9090^\circ relative to one another.
2
Calculate magnitudes for orthogonal pairs using the Pythagorean theorem
For 3 m3\text{ m} and 4 m4\text{ m}: 32+42=5 m\sqrt{3^2 + 4^2} = 5\text{ m}. For 5 m5\text{ m} and 12 m12\text{ m}: 52+122=13 m\sqrt{5^2 + 12^2} = 13\text{ m}. For 9 m9\text{ m} and 12 m12\text{ m}: 92+122=15 m\sqrt{9^2 + 12^2} = 15\text{ m}.
The magnitude of two perpendicular vectors A\vec{A} and B\vec{B} is given by R=A2+B2R = \sqrt{A^2 + B^2}.
3
Calculate net displacement for opposite collinear vectors
For 8 m8\text{ m} East and 6 m6\text{ m} West: 86=2 m8 - 6 = 2\text{ m} East.
Vectors pointing in opposite directions along the same axis subtract algebraically, retaining the direction of the vector with the greater magnitude.

Key Concept

Addition of Perpendicular and Collinear Displacement Vectors
Estimated Time:1m 30s
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