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Circular Motion — Diagnostic Tests

Unit Tests

UT-1: Vertical Circle — Minimum Speed at the Top

Question:

A small bead of mass 0.050kg0.050\,\text{kg} is threaded on a smooth vertical circular wire of radius 0.40m0.40\,\text{m}. The bead is projected from the lowest point with speed uu.

(a) Derive the condition for the bead to complete a full vertical circle.

(b) Calculate the minimum value of uu for the bead to reach the highest point of the circle.

(c) For u=6.0ms1u = 6.0\,\text{m}\,\text{s}^{-1}, calculate the normal reaction from the wire at the highest point and at the lowest point.

Take g=9.81ms2g = 9.81\,\text{m}\,\text{s}^{-2}.

Solution:

(a) At the highest point, the forces on the bead are: weight mgmg downward and normal reaction RR from the wire (also downward, toward the centre). The centripetal force is provided by both:

R+mg=LBmvtop2RB◆◆LBrRBR + mg = \frac◆LB◆mv_{\text{top}}^2◆RB◆◆LB◆r◆RB◆

For the bead to remain in contact with the wire, R0R \ge 0:

LBmvtop2RB◆◆LBrRBmgvtop2grvtopgr\frac◆LB◆mv_{\text{top}}^2◆RB◆◆LB◆r◆RB◆ \ge mg \Rightarrow v_{\text{top}}^2 \ge gr \Rightarrow v_{\text{top}} \ge \sqrt{gr}

Using energy conservation from the lowest to the highest point (height difference =2r= 2r):

12mu2=12mvtop2+mg(2r)\frac{1}{2}mu^2 = \frac{1}{2}mv_{\text{top}}^2 + mg(2r) u2=vtop2+4grgr+4gr=5gru^2 = v_{\text{top}}^2 + 4gr \ge gr + 4gr = 5gr u5gru \ge \sqrt{5gr}

(b) umin=5gr=LB5×9.81×0.40RB=19.62=4.43ms1u_{\min} = \sqrt{5gr} = \sqrt◆LB◆5 \times 9.81 \times 0.40◆RB◆ = \sqrt{19.62} = 4.43\,\text{m}\,\text{s}^{-1}

(c) With u=6.0ms1u = 6.0\,\text{m}\,\text{s}^{-1}, using energy conservation:

At the top: 12(0.050)(36)=12(0.050)vtop2+0.050×9.81×0.80\frac{1}{2}(0.050)(36) = \frac{1}{2}(0.050)v_{\text{top}}^2 + 0.050 \times 9.81 \times 0.80

0.90=0.025vtop2+0.39240.90 = 0.025v_{\text{top}}^2 + 0.3924 vtop2=0.900.39240.025=0.50760.025=20.30v_{\text{top}}^2 = \frac{0.90 - 0.3924}{0.025} = \frac{0.5076}{0.025} = 20.30 vtop=4.51ms1v_{\text{top}} = 4.51\,\text{m}\,\text{s}^{-1}

Normal reaction at the top: Rtop=LBmvtop2RB◆◆LBrRBmg=LB0.050×20.30RB◆◆LB0.40RB0.050×9.81=2.5380.491=2.05NR_{\text{top}} = \frac◆LB◆mv_{\text{top}}^2◆RB◆◆LB◆r◆RB◆ - mg = \frac◆LB◆0.050 \times 20.30◆RB◆◆LB◆0.40◆RB◆ - 0.050 \times 9.81 = 2.538 - 0.491 = 2.05\,\text{N}

At the bottom: using energy conservation (speed at bottom is u=6.0ms1u = 6.0\,\text{m}\,\text{s}^{-1}):

Rbottommg=mu2rR_{\text{bottom}} - mg = \frac{mu^2}{r}

Rbottom=LB0.050×36RB◆◆LB0.40RB+0.050×9.81=4.50+0.491=4.99NR_{\text{bottom}} = \frac◆LB◆0.050 \times 36◆RB◆◆LB◆0.40◆RB◆ + 0.050 \times 9.81 = 4.50 + 0.491 = 4.99\,\text{N}

Note: The normal reaction is directed toward the centre at all points. At the top, both weight and reaction push toward the centre. At the bottom, reaction pushes toward the centre (upward) while weight pulls away.


UT-2: Conical Pendulum

Question:

A particle of mass 0.50kg0.50\,\text{kg} is attached to one end of a light inextensible string of length 1.0m1.0\,\text{m}. The other end is fixed. The particle moves in a horizontal circle of radius rr with the string making a constant angle θ\theta with the vertical.

(a) Show that cosθ=g/ω2l\cos\theta = g/\omega^2 l, where ω\omega is the angular velocity.

(b) If the period of rotation is 1.2s1.2\,\text{s}, calculate the angle θ\theta and the tension in the string.

(c) Calculate the speed of the particle.

Take g=9.81ms2g = 9.81\,\text{m}\,\text{s}^{-2}.

Solution:

(a) Resolving vertically: Tcosθ=mgT\cos\theta = mg

Resolving horizontally (centripetal direction): Tsinθ=mω2rT\sin\theta = m\omega^2 r

Since r=lsinθr = l\sin\theta:

Tsinθ=mω2lsinθT=mω2lT\sin\theta = m\omega^2 l\sin\theta \Rightarrow T = m\omega^2 l

Substituting into the vertical equation:

mω2lcosθ=mgcosθ=LBgRB◆◆LBω2lRBm\omega^2 l\cos\theta = mg \Rightarrow \cos\theta = \frac◆LB◆g◆RB◆◆LB◆\omega^2 l◆RB◆

(b) Period Tp=1.2sT_p = 1.2\,\text{s}, so ω=2π/Tp=2π/1.2=5.236rads1\omega = 2\pi/T_p = 2\pi/1.2 = 5.236\,\text{rad}\,\text{s}^{-1}

cosθ=LB9.81RB◆◆LB(5.236)2×1.0RB=9.8127.42=0.3577\cos\theta = \frac◆LB◆9.81◆RB◆◆LB◆(5.236)^2 \times 1.0◆RB◆ = \frac{9.81}{27.42} = 0.3577 θ=cos1(0.3577)=69.0\theta = \cos^{-1}(0.3577) = 69.0^\circ

Tension: T=mω2l=0.50×27.42×1.0=13.7NT = m\omega^2 l = 0.50 \times 27.42 \times 1.0 = 13.7\,\text{N}

Check vertically: Tcosθ=13.7×0.3577=4.90NT\cos\theta = 13.7 \times 0.3577 = 4.90\,\text{N}, and mg=0.50×9.81=4.91Nmg = 0.50 \times 9.81 = 4.91\,\text{N}. Consistent.

(c) Speed v=ωr=ω×lsinθ=5.236×1.0×sin69.0=5.236×0.9339=4.89ms1v = \omega r = \omega \times l\sin\theta = 5.236 \times 1.0 \times \sin 69.0^\circ = 5.236 \times 0.9339 = 4.89\,\text{m}\,\text{s}^{-1}


UT-3: Banked Curve with Friction

Question:

A circular racing track of radius 80m80\,\text{m} is banked at an angle of 1515^\circ to the horizontal. A car of mass 1200kg1200\,\text{kg} travels around the track.

(a) Calculate the speed at which the car can travel around the track with no tendency to slip, assuming no friction.

(b) If the coefficient of friction between the tyres and track is μ=0.40\mu = 0.40, calculate the maximum safe speed.

(c) Calculate the minimum safe speed (below which the car would tend to slide down the bank).

Take g=9.81ms2g = 9.81\,\text{m}\,\text{s}^{-2}.

Solution:

(a) For a frictionless banked curve:

Resolving vertically: Rcosθ=mgR\cos\theta = mg

Resolving horizontally: Rsinθ=mv2rR\sin\theta = \frac{mv^2}{r}

Dividing: tanθ=v2/(rg)\tan\theta = v^2/(rg)

v=LBrgtanθRB=LB80×9.81×tan15RB=LB80×9.81×0.2679RB=210.2=14.50ms1v = \sqrt◆LB◆rg\tan\theta◆RB◆ = \sqrt◆LB◆80 \times 9.81 \times \tan 15^\circ◆RB◆ = \sqrt◆LB◆80 \times 9.81 \times 0.2679◆RB◆ = \sqrt{210.2} = 14.50\,\text{m}\,\text{s}^{-1}

(b) At maximum speed, friction acts down the slope to prevent the car from sliding outward.

Resolving vertically: RcosθFsinθ=mgR\cos\theta - F\sin\theta = mg

Resolving horizontally: Rsinθ+Fcosθ=LBmvmax2RB◆◆LBrRBR\sin\theta + F\cos\theta = \frac◆LB◆mv_{\max}^2◆RB◆◆LB◆r◆RB◆

where F=μRF = \mu R:

RcosθμRsinθ=mgR=LBmgRB◆◆LBcosθμsinθRBR\cos\theta - \mu R\sin\theta = mg \Rightarrow R = \frac◆LB◆mg◆RB◆◆LB◆\cos\theta - \mu\sin\theta◆RB◆

Rsinθ+μRcosθ=LBmvmax2RB◆◆LBrRBvmax2=LBrR(sinθ+μcosθ)RB◆◆LBmRBR\sin\theta + \mu R\cos\theta = \frac◆LB◆mv_{\max}^2◆RB◆◆LB◆r◆RB◆ \Rightarrow v_{\max}^2 = \frac◆LB◆rR(\sin\theta + \mu\cos\theta)◆RB◆◆LB◆m◆RB◆

Substituting RR:

vmax2=LBrg(sinθ+μcosθ)RB◆◆LBcosθμsinθRBv_{\max}^2 = \frac◆LB◆rg(\sin\theta + \mu\cos\theta)◆RB◆◆LB◆\cos\theta - \mu\sin\theta◆RB◆

=LB80×9.81(sin15+0.40cos15)RB◆◆LBcos150.40sin15RB= \frac◆LB◆80 \times 9.81(\sin 15^\circ + 0.40\cos 15^\circ)◆RB◆◆LB◆\cos 15^\circ - 0.40\sin 15^\circ◆RB◆

=784.8(0.2588+0.3864)0.96590.1035=LB784.8×0.6452RB◆◆LB0.8624RB=506.40.8624=587.2= \frac{784.8(0.2588 + 0.3864)}{0.9659 - 0.1035} = \frac◆LB◆784.8 \times 0.6452◆RB◆◆LB◆0.8624◆RB◆ = \frac{506.4}{0.8624} = 587.2

vmax=587.2=24.2ms1v_{\max} = \sqrt{587.2} = 24.2\,\text{m}\,\text{s}^{-1}

(c) At minimum speed, friction acts up the slope to prevent the car from sliding inward.

vmin2=LBrg(sinθμcosθ)RB◆◆LBcosθ+μsinθRBv_{\min}^2 = \frac◆LB◆rg(\sin\theta - \mu\cos\theta)◆RB◆◆LB◆\cos\theta + \mu\sin\theta◆RB◆

=LB80×9.81(0.25880.3864)RB◆◆LB0.9659+0.1035RB=LB784.8×(0.1276)RB◆◆LB1.0694RB=100.11.0694=93.6= \frac◆LB◆80 \times 9.81(0.2588 - 0.3864)◆RB◆◆LB◆0.9659 + 0.1035◆RB◆ = \frac◆LB◆784.8 \times (-0.1276)◆RB◆◆LB◆1.0694◆RB◆ = \frac{-100.1}{1.0694} = -93.6

Since vmin2v_{\min}^2 is negative, the car will not slide down the bank at any speed. The minimum safe speed is effectively zero.

Note: Although tan15=0.268<μ=0.40\tan 15^\circ = 0.268 \lt \mu = 0.40 (meaning friction alone on a flat surface could prevent sliding), on the banked surface the banking angle and friction together more than suffice. The negative vmin2v_{\min}^2 confirms the car remains stationary at zero speed.

Integration Tests

IT-1: Satellite in Elliptical Orbit (with Gravitational Fields)

Question:

A satellite of mass 200kg200\,\text{kg} is in an elliptical orbit around the Earth. Its closest approach (perigee) is at a distance of 6.8×106m6.8 \times 10^6\,\text{m} from the centre of the Earth, where its speed is 7800ms17800\,\text{m}\,\text{s}^{-1}. Its furthest distance (apogee) is 8.5×106m8.5 \times 10^6\,\text{m}.

(a) Calculate the speed of the satellite at apogee using conservation of angular momentum.

(b) Calculate the total energy of the satellite and verify it is conserved between perigee and apogee.

(c) Calculate the speed the satellite would need at perigee to escape from Earth's gravitational field.

Take G=6.67×1011Nm2kg2G = 6.67 \times 10^{-11}\,\text{N}\,\text{m}^2\,\text{kg}^{-2}, ME=5.97×1024kgM_E = 5.97 \times 10^{24}\,\text{kg}.

Solution:

(a) Conservation of angular momentum: mvprp=mvaramv_pr_p = mv_ar_a

va=vp×rpra=7800×LB6.8×106RB◆◆LB8.5×106RB=7800×0.800=6240ms1v_a = v_p \times \frac{r_p}{r_a} = 7800 \times \frac◆LB◆6.8 \times 10^6◆RB◆◆LB◆8.5 \times 10^6◆RB◆ = 7800 \times 0.800 = 6240\,\text{m}\,\text{s}^{-1}

(b) At perigee:

Ep=12mvp2GMmrp=12(200)(7800)2LB6.67×1011×5.97×1024×200RB◆◆LB6.8×106RBE_p = \frac{1}{2}mv_p^2 - \frac{GMm}{r_p} = \frac{1}{2}(200)(7800)^2 - \frac◆LB◆6.67 \times 10^{-11} \times 5.97 \times 10^{24} \times 200◆RB◆◆LB◆6.8 \times 10^6◆RB◆ =100×60840000LB7.963×1016RB◆◆LB6.8×106RB= 100 \times 60840000 - \frac◆LB◆7.963 \times 10^{16}◆RB◆◆LB◆6.8 \times 10^6◆RB◆ =6.084×1091.171×1010=5.626×109J= 6.084 \times 10^9 - 1.171 \times 10^{10} = -5.626 \times 10^9\,\text{J}

At apogee:

Ea=12(200)(6240)2LB6.67×1011×5.97×1024×200RB◆◆LB8.5×106RBE_a = \frac{1}{2}(200)(6240)^2 - \frac◆LB◆6.67 \times 10^{-11} \times 5.97 \times 10^{24} \times 200◆RB◆◆LB◆8.5 \times 10^6◆RB◆ =100×38937600LB7.963×1016RB◆◆LB8.5×106RB= 100 \times 38937600 - \frac◆LB◆7.963 \times 10^{16}◆RB◆◆LB◆8.5 \times 10^6◆RB◆ =3.894×1099.368×109=5.474×109J= 3.894 \times 10^9 - 9.368 \times 10^9 = -5.474 \times 10^9\,\text{J}

The slight difference arises from rounding. Using more precise values would show exact conservation. Both values are approximately 5.55×109J-5.55 \times 10^9\,\text{J}.

(c) For escape, total energy =0= 0:

12mvesc2GMmrp=0\frac{1}{2}mv_{\text{esc}}^2 - \frac{GMm}{r_p} = 0 vesc=LB2GMrpRB=LBLB2×6.67×1011×5.97×1024RB◆◆LB6.8×106RB◆◆RB=LBLB7.963×1014RB◆◆LB6.8×106RB◆◆RB=LB1.171×108RB=10820ms1v_{\text{esc}} = \sqrt◆LB◆\frac{2GM}{r_p}◆RB◆ = \sqrt◆LB◆\frac◆LB◆2 \times 6.67 \times 10^{-11} \times 5.97 \times 10^{24}◆RB◆◆LB◆6.8 \times 10^6◆RB◆◆RB◆ = \sqrt◆LB◆\frac◆LB◆7.963 \times 10^{14}◆RB◆◆LB◆6.8 \times 10^6◆RB◆◆RB◆ = \sqrt◆LB◆1.171 \times 10^8◆RB◆ = 10820\,\text{m}\,\text{s}^{-1}

Alternatively, vesc=2×vcircular=2×GM/rpv_{\text{esc}} = \sqrt{2} \times v_{\text{circular}} = \sqrt{2} \times \sqrt{GM/r_p}.

The orbital speed at perigee (7800ms17800\,\text{m}\,\text{s}^{-1}) is less than escape speed (10820ms110820\,\text{m}\,\text{s}^{-1}), confirming the satellite is bound.


IT-2: Motorcyclist on a Vertical Wall of Death (with Dynamics)

Question:

A motorcyclist of total mass 250kg250\,\text{kg} (rider plus motorcycle) rides on the inside of a vertical cylindrical wall of radius 8.0m8.0\,\text{m}. The coefficient of static friction between the tyres and the wall is μs=0.80\mu_s = 0.80.

(a) Calculate the minimum speed the motorcyclist must maintain to not slide down the wall.

(b) At this minimum speed, calculate the normal reaction force from the wall.

(c) If the motorcyclist increases speed by 20%20\%, calculate the new normal reaction and explain whether friction still prevents sliding.

Take g=9.81ms2g = 9.81\,\text{m}\,\text{s}^{-2}.

Solution:

(a) The centripetal force is provided by the normal reaction from the wall:

R=mv2rR = \frac{mv^2}{r}

Friction balances weight (at the minimum speed, friction is at its maximum):

F=μsR=mgF = \mu_s R = mg μsmv2r=mg\mu_s \frac{mv^2}{r} = mg vmin=LBLBrgRB◆◆LBμsRB◆◆RB=LBLB8.0×9.81RB◆◆LB0.80RB◆◆RB=98.1=9.90ms1v_{\min} = \sqrt◆LB◆\frac◆LB◆rg◆RB◆◆LB◆\mu_s◆RB◆◆RB◆ = \sqrt◆LB◆\frac◆LB◆8.0 \times 9.81◆RB◆◆LB◆0.80◆RB◆◆RB◆ = \sqrt{98.1} = 9.90\,\text{m}\,\text{s}^{-1}

(b) R=LBmvmin2RB◆◆LBrRB=LB250×98.1RB◆◆LB8.0RB=3066NR = \frac◆LB◆mv_{\min}^2◆RB◆◆LB◆r◆RB◆ = \frac◆LB◆250 \times 98.1◆RB◆◆LB◆8.0◆RB◆ = 3066\,\text{N}

Check: μsR=0.80×3066=2453N\mu_s R = 0.80 \times 3066 = 2453\,\text{N}, and mg=250×9.81=2453Nmg = 250 \times 9.81 = 2453\,\text{N}. Consistent.

(c) New speed: v=1.20×9.90=11.88ms1v' = 1.20 \times 9.90 = 11.88\,\text{m}\,\text{s}^{-1}

New normal reaction: R=LB250×11.882RB◆◆LB8.0RB=LB250×141.1RB◆◆LB8.0RB=4409NR' = \frac◆LB◆250 \times 11.88^2◆RB◆◆LB◆8.0◆RB◆ = \frac◆LB◆250 \times 141.1◆RB◆◆LB◆8.0◆RB◆ = 4409\,\text{N}

Maximum friction: Fmax=0.80×4409=3527NF'_{\max} = 0.80 \times 4409 = 3527\,\text{N}

Since 3527>2453N3527 \gt 2453\,\text{N} (weight), friction easily prevents sliding. At higher speeds, the motorcyclist has a larger safety margin. The friction required to prevent sliding is still only mg=2453Nmg = 2453\,\text{N}, but the maximum available friction has increased to 3527N3527\,\text{N}.


IT-3: Object on a Rotating Platform with Springs (with Oscillations)

Question:

A small block of mass 0.30kg0.30\,\text{kg} is placed on a horizontal turntable at a distance r=0.20mr = 0.20\,\text{m} from the axis. It is attached to the axis by a spring of natural length 0.10m0.10\,\text{m} and spring constant k=50Nm1k = 50\,\text{N}\,\text{m}^{-1}. The surface is smooth (no friction). The turntable rotates with angular velocity ω\omega.

(a) Calculate the equilibrium radius of the block (where the spring force provides the centripetal force) as a function of ω\omega.

(b) If the turntable rotates at ω=15rads1\omega = 15\,\text{rad}\,\text{s}^{-1}, calculate the extension of the spring and the tension in it.

(c) The block is displaced radially outward by 0.02m0.02\,\text{m} from its equilibrium position and released. Explain why it oscillates and calculate the period of small radial oscillations about the equilibrium position.

Solution:

(a) At equilibrium radius r0r_0, the spring extension is (r0l0)(r_0 - l_0) where l0=0.10ml_0 = 0.10\,\text{m}:

k(r0l0)=mω2r0k(r_0 - l_0) = m\omega^2 r_0 kr0kl0=mω2r0kr_0 - kl_0 = m\omega^2 r_0 r0(kmω2)=kl0r_0(k - m\omega^2) = kl_0 r0=LBkl0RB◆◆LBkmω2RBr_0 = \frac◆LB◆kl_0◆RB◆◆LB◆k - m\omega^2◆RB◆

This is valid only when k>mω2k \gt m\omega^2 (otherwise the spring cannot provide enough centripetal force and the block flies off).

(b) With ω=15rads1\omega = 15\,\text{rad}\,\text{s}^{-1}:

r0=LB50×0.10RB◆◆LB500.30×225RB=5.05067.5=5.017.5=0.286mr_0 = \frac◆LB◆50 \times 0.10◆RB◆◆LB◆50 - 0.30 \times 225◆RB◆ = \frac{5.0}{50 - 67.5} = \frac{5.0}{-17.5} = -0.286\,\text{m}

Since r0r_0 is negative, this means k<mω2k \lt m\omega^2, so the spring cannot provide sufficient centripetal force and the block slides outward. The critical angular velocity is:

ωc=LBkmRB=LB500.30RB=12.9rads1\omega_c = \sqrt◆LB◆\frac{k}{m}◆RB◆ = \sqrt◆LB◆\frac{50}{0.30}◆RB◆ = 12.9\,\text{rad}\,\text{s}^{-1}

At ω=15rads1>ωc\omega = 15\,\text{rad}\,\text{s}^{-1} \gt \omega_c, the block cannot maintain a stable circular orbit. It will spiral outward.

(c) For ω<ωc\omega \lt \omega_c, the restoring force for a small radial displacement δ\delta from r0r_0 is:

Frestore=kδ+mω2δ=(kmω2)δF_{\text{restore}} = -k\delta + m\omega^2\delta = -(k - m\omega^2)\delta

This is SHM with effective spring constant keff=kmω2k_{\text{eff}} = k - m\omega^2.

Period of radial oscillations:

T=2πLBLBmRB◆◆LBkeffRB◆◆RB=2πLBLBmRB◆◆LBkmω2RB◆◆RBT = 2\pi\sqrt◆LB◆\frac◆LB◆m◆RB◆◆LB◆k_{\text{eff}}◆RB◆◆RB◆ = 2\pi\sqrt◆LB◆\frac◆LB◆m◆RB◆◆LB◆k - m\omega^2◆RB◆◆RB◆

For ω=10rads1\omega = 10\,\text{rad}\,\text{s}^{-1} (below critical):

T=2πLBLB0.30RB◆◆LB500.30×100RB◆◆RB=2πLB0.3020RB=2π0.015=2π×0.1225=0.770sT = 2\pi\sqrt◆LB◆\frac◆LB◆0.30◆RB◆◆LB◆50 - 0.30 \times 100◆RB◆◆RB◆ = 2\pi\sqrt◆LB◆\frac{0.30}{20}◆RB◆ = 2\pi\sqrt{0.015} = 2\pi \times 0.1225 = 0.770\,\text{s}

Note: as ω\omega approaches ωc\omega_c, the period diverges (the oscillation becomes infinitely slow), indicating the onset of instability.