Unit M3: Mechanics 3

Syllabus
2019
Section
—
Level
A2

M3.1 - Further kinematics

Syllabus
2019
Topic
M3.1
Level
A2

Choose and solve a variable-acceleration equation

For motion along a straight line, displacement xx, signed velocity vv and signed acceleration aa are linked by derivatives. Choose the form whose independent variable matches the information given; this avoids introducing an unnecessary unknown function.

v=dxdt,a=dvdt=vdvdxv=\frac{\mathrm dx}{\mathrm dt},\qquad a=\frac{\mathrm dv}{\mathrm dt}=v\frac{\mathrm dv}{\mathrm dx}

Information given Equation to set up First result after integration
a=f(t)a=f(t) dvdt=f(t)\dfrac{\mathrm dv}{\mathrm dt}=f(t) vv as a function of tt
a=f(x)a=f(x) vdvdx=f(x)v\dfrac{\mathrm dv}{\mathrm dx}=f(x) 12v2\dfrac12v^2 as a function of xx
v=f(x)v=f(x) dxdt=f(x)\dfrac{\mathrm dx}{\mathrm dt}=f(x), so dt=dxf(x)\mathrm dt=\dfrac{\mathrm dx}{f(x)} tt as a function of xx
v=f(t)v=f(t) dxdt=f(t)\dfrac{\mathrm dx}{\mathrm dt}=f(t) xx as a function of tt

The displacement form of acceleration follows from the chain rule:dvdt=dvdxdxdt=vdvdx.\frac{\mathrm dv}{\mathrm dt}=\frac{\mathrm dv}{\mathrm dx}\frac{\mathrm dx}{\mathrm dt}=v\frac{\mathrm dv}{\mathrm dx}.Use it when acceleration or velocity is expressed in terms of xx. If the required quantity is time and v=f(x)v=f(x), separate variables instead: dt=dx/v(x)\mathrm dt=\mathrm dx/v(x).

Every indefinite integration needs a constant. Apply a stated condition such as x=x0x=x_0 and v=v0v=v_0 at t=t0t=t_0 only after integrating, or use definite integrals with those values as limits. Keep vv signed: a negative velocity represents motion in the negative xx-direction, while speed is ∣v∣|v|.

Suppose v=12/(x+2)v=12/(x+2) metres per second and x=1x=1 when t=0t=0. First,a=vdvdx=12x+2(−12(x+2)2)=−144(x+2)3.a=v\frac{\mathrm dv}{\mathrm dx}=\frac{12}{x+2}\left(-\frac{12}{(x+2)^2}\right)=-\frac{144}{(x+2)^3}.At x=4x=4, a=−2/3 m s−2a=-2/3\,\mathrm{m\,s^{-2}}. For the elapsed time to reach x=4x=4,t=∫14dxv=∫14x+212 dx=[x224+x6]14=98 s.t=\int_1^4\frac{\mathrm dx}{v}=\int_1^4\frac{x+2}{12}\,\mathrm dx=\left[\frac{x^2}{24}+\frac{x}{6}\right]_1^4=\frac98\text{ s}.The negative acceleration means velocity is decreasing here; the deceleration magnitude is 2/3 m s−22/3\,\mathrm{m\,s^{-2}}.

Check that the final variable matches the question, substitute the initial condition back into the integrated relation, and verify units: vv has units m s−1\mathrm{m\,s^{-1}} and aa has units m s−2\mathrm{m\,s^{-2}}. If a derivation divides by vv or by another expression that can be zero, solve on intervals where that division is valid and inspect the zero case separately.

Do not use constant-acceleration formulae when aa varies, replace aa by dv/dx\mathrm dv/\mathrm dx without the factor vv, discard an integration constant, or report a negative acceleration automatically as a positive deceleration. Acceleration and velocity signs must be interpreted together.

M3.2 - Elastic strings and springs

Syllabus
2019
Topic
M3.2
Level
A2

Model elastic tension with Hooke's law

An elastic element has natural length ll, the length at which it is undeformed. If its current length is LL, its extension is x=L−lx=L-l. Under Hooke's law, the elastic-force magnitude is proportional to this extension.

T=λxlT=\frac{\lambda x}{l}

Here TT is tension in newtons and λ\lambda is the modulus of elasticity, also measured in newtons. The ratio x/lx/l is dimensionless. When a spring is described using stiffness kk instead, the equivalent form is T=kxT=kx, with k=λ/lk=\lambda/l and unit N m−1\mathrm{N\,m^{-1}}.

Model When the elastic force acts Direction
light elastic string only while stretched, L>lL>l tension pulls each attached object along the string
string at or below natural length it is slack, so T=0T=0 no push is possible
elastic spring when stretched or compressed within the Hooke-law model restoring force points towards natural length

First calculate extension from the actual geometry, not from the total length alone. Apply Hooke's law to find tension, then place that force on the free-body diagram and resolve it in the chosen direction. If two equal sections pull symmetrically, include both resolved tensions; do not replace them by one tension.

A particle of mass 1.51.5 kg hangs from a vertical light elastic string with natural length 0.80.8 m and modulus 4040 N. At an instant the string has length 1.11.1 m, so x=0.3x=0.3 m andT=40(0.3)0.8=15 N.T=\frac{40(0.3)}{0.8}=15\text{ N}.Taking upward as positive, the particle's acceleration at that instant isa=T−mgm=15−1.5(9.8)1.5=0.20 m s−2.a=\frac{T-mg}{m}=\frac{15-1.5(9.8)}{1.5}=0.20\,\mathrm{m\,s^{-2}}.Hooke's law supplies the force; Newton's second law supplies the acceleration.

Do not substitute the current length for the extension, treat the modulus as a spring constant with unit N m−1\mathrm{N\,m^{-1}}, or let an elastic string push when slack. Hooke's law describes the stated ideal elastic model; geometry and force resolution remain separate steps.

Use elastic energy in a work-energy balance

Stretching an elastic string or deforming a spring stores elastic potential energy (EPE). For a Hooke-law element, the force rises linearly from zero, so the stored energy is the area under the force-extension relation.

Ee=λx22l=12Tx=12kx2E_{\mathrm e}=\frac{\lambda x^2}{2l}=\frac12Tx=\frac12kx^2

Use the extension x=L−lx=L-l at the particular state being considered. For an elastic string, Ee=0E_{\mathrm e}=0 whenever the string is slack; for a spring, x2x^2 gives positive stored energy for either extension or compression. Elastic energy is measured in joules.

Energy term Expression What changes it
kinetic energy 12mv2\tfrac12mv^2 the particle's speed
gravitational potential energy mghmgh vertical height relative to one fixed datum
elastic potential energy λx2/(2l)\lambda x^2/(2l) the element's extension or compression
external work force component ×\times displacement, or an integral a non-conservative applied force

Choose initial and final states, calculate the elastic extension separately at each state, and use one consistent height datum. If only gravity and ideal elastic forces do work,Ki+Ug,i+Ee,i=Kf+Ug,f+Ee,f.K_i+U_{g,i}+E_{\mathrm e,i}=K_f+U_{g,f}+E_{\mathrm e,f}.Otherwise add the work of any other force with its correct sign. Energy equations compare states; they do not require the acceleration to be constant.

A 11 kg particle is attached below a vertical elastic string of natural length 11 m and modulus 2020 N. It is released from rest with extension 0.100.10 m and falls 0.200.20 m, so the final extension is 0.300.30 m. The initial and final EPE values are 0.100.10 J and 0.900.90 J. Conservation of mechanical energy gives0+0.10+1(9.8)(0.20)=12v2+0.90,0+0.10+1(9.8)(0.20)=\frac12v^2+0.90,hence 12v2=1.16\tfrac12v^2=1.16 and v=1.52 m s−1v=1.52\,\mathrm{m\,s^{-1}} to three significant figures.

Do not use the same extension at both endpoints, omit elastic energy when the element remains stretched, or write EPE as TxTx: because tension changes during deformation, the factor 1/21/2 is essential. When a string becomes slack, stop using the stretched-string formula beyond that event.

M3.3 - Further dynamics

Syllabus
2019
Topic
M3.3
Level
A2

Solve one-dimensional motion under a variable force

For motion along one signed axis, first write the resultant force with its direction, then choose the acceleration form that matches the variable in the force law. A varying force produces a differential equation rather than a constant-acceleration problem.

Fresultant=ma,a=dvdt=vdvdxF_{\mathrm{resultant}}=ma,\qquad a=\frac{\mathrm dv}{\mathrm dt}=v\frac{\mathrm dv}{\mathrm dx}

Force information Useful equation Typical result
F=f(t)F=f(t) m dv/dt=f(t)m\,\mathrm dv/\mathrm dt=f(t) integrate for v(t)v(t), then for x(t)x(t) if needed
F=f(x)F=f(x) mv dv/dx=f(x)mv\,\mathrm dv/\mathrm dx=f(x) integrate for v2v^2 as a function of xx
work is simpler ∫x0xF(s) ds=12m(v2−v02)\int_{x_0}^{x}F(s)\,\mathrm ds=\tfrac12m(v^2-v_0^2) compare two positions directly
inverse-square attraction choose outward positive, so F=−k/x2F=-k/x^2 preserve the negative force sign before integrating

Define the coordinate origin and positive direction before inserting a force. Include every force component in the resultant. Separate variables or integrate with limits, use the supplied motion condition to determine the constant, and accept only positions for which v2≥0v^2\ge0 and the force model is defined.

A 22 kg particle moves in the positive xx-direction under resultant force F=12−2xF=12-2x N. At x=0x=0, its speed is 1 m s−11\,\mathrm{m\,s^{-1}}. Since2vdvdx=12−2x,2v\frac{\mathrm dv}{\mathrm dx}=12-2x,integration between the initial position and xx givesv2=1+12x−x2.v^2=1+12x-x^2.At x=3x=3 m, v=28=27 m s−1v=\sqrt{28}=2\sqrt7\,\mathrm{m\,s^{-1}}. A turning point requires v=0v=0; the positive solution is x=6+37x=6+\sqrt{37} m.

For an attractive inverse-square force with outward coordinate x>0x>0, F=−k/x2F=-k/x^2. Thenmvdvdx=−kx2mv\frac{\mathrm dv}{\mathrm dx}=-\frac{k}{x^2}integrates to 12mv2=k/x+C\tfrac12mv^2=k/x+C. The plus sign on k/xk/x after integration is consistent with differentiating k/xk/x to recover −k/x2-k/x^2.

Do not use constant-acceleration formulae, omit a force from the resultant, drop the factor vv in a=v dv/dxa=v\,\mathrm dv/\mathrm dx, or remove the sign from an attractive inverse-square force. A negative value of v2v^2 signals an inaccessible region, not an imaginary physical speed.

Recognise and calculate with simple harmonic motion

Motion is simple harmonic when acceleration is proportional to displacement from a fixed equilibrium point and always directed back towards that point. With signed displacement xx from equilibrium, the defining equation is

x¨=−ω2x\ddot x=-\omega^2x

To prove SHM in a mechanical system, write a signed equation of motion and simplify it in terms of displacement from equilibrium. Constant force terms must cancel at equilibrium. Reaching x¨=−cx\ddot x=-c x with c>0c>0 proves SHM and identifies ω=c\omega=\sqrt c; merely obtaining a periodic-looking expression is not the required force-law proof.

Quantity SHM relation
displacement x=Acos⁡(ωt+ϕ)x=A\cos(\omega t+\phi), equivalently a sine form
speed at displacement xx v2=ω2(A2−x2)v^2=\omega^2(A^2-x^2)
period T=2π/ωT=2\pi/\omega
maximum speed, at equilibrium vmax⁡=ωAv_{\max}=\omega A
maximum acceleration, at an endpoint ∣a∣max⁡=ω2A|a|_{\max}=\omega^2A

Choose the phase from the initial state. Release from rest at x=Ax=A allows x=Acos⁡ωtx=A\cos\omega t; starting at equilibrium in the positive direction allows x=Asin⁡ωtx=A\sin\omega t. For time spent in a region, solve the boundary displacement within one cycle and use the symmetry of the cosine or sine curve without double-counting endpoints.

If x=0.12cos⁡(5t)x=0.12\cos(5t) metres, then A=0.12A=0.12 m, ω=5 rad s−1\omega=5\,\mathrm{rad\,s^{-1}} and T=2π/5T=2\pi/5 s. The maximum speed is 0.60 m s−10.60\,\mathrm{m\,s^{-1}}. Starting at the positive endpoint, the first time the particle reaches x=0.06x=0.06 m satisfies cos⁡(5t)=1/2\cos(5t)=1/2, so t=π/15t=\pi/15 s.

Displacement must be measured from equilibrium, not an arbitrary origin. The minus sign is essential: x¨=+ω2x\ddot x=+\omega^2x drives motion away from equilibrium and is not SHM. Amplitude is a non-negative distance, whereas xx, vv and acceleration are signed.

Model elastic oscillations about equilibrium

A particle attached to an ideal spring or taut elastic string can perform SHM along the element's direction. Measure displacement from the equilibrium position: doing so makes the constant weight term cancel and exposes the restoring force.

mx¨=−kx,ω=km,k=λlm\ddot x=-kx,\qquad \omega=\sqrt{\frac{k}{m}},\qquad k=\frac{\lambda}{l}

For a vertical element, let its equilibrium extension be ee. Equilibrium gives ke=mgke=mg. If downward displacement from equilibrium is xx, the extension is e+xe+x andmx¨=mg−k(e+x)=−kx.m\ddot x=mg-k(e+x)=-kx.Gravity shifts the equilibrium position but does not appear in ω\omega after this cancellation.

Arrangement Condition for the SHM model to remain valid
spring deformation stays within the stated Hooke-law model
one elastic string its extension never becomes negative; for equilibrium extension ee and amplitude AA, require e−A≥0e-A\ge0
particle between two elastic strings calculate both extensions at each extreme and require both strings to remain taut
string reaches natural length tension becomes zero; subsequent motion is not governed by the same SHM equation

A 0.50.5 kg particle oscillates vertically on an elastic element with stiffness 18 N m−118\,\mathrm{N\,m^{-1}}. Then ω=18/0.5=6 rad s−1\omega=\sqrt{18/0.5}=6\,\mathrm{rad\,s^{-1}} and T=π/3T=\pi/3 s. If its amplitude is 0.080.08 m, its speed at displacement 0.040.04 m isv=60.082−0.042=0.416 m s−1.v=6\sqrt{0.08^2-0.04^2}=0.416\,\mathrm{m\,s^{-1}}.If the element is a string, this calculation applies for the whole oscillation only after checking that the minimum extension remains non-negative.

Do not measure elastic extension and SHM displacement from the same origin without defining both, leave the equilibrium weight term in the final restoring equation, or claim one continuous SHM cycle after a string goes slack. The specified oscillation is along the string or spring, not transverse to it.

M3.4 - Motion in a circle

Syllabus
2019
Topic
M3.4
Level
A2

Connect angular speed to period and linear speed

Angular speed ω\omega measures the rate at which angular position changes. Angles in circular-motion formulae are measured in radians, so one complete revolution is 2π2\pi radians.

ω=dθdt,ω=2πT=2πf\omega=\frac{\mathrm d\theta}{\mathrm dt},\qquad \omega=\frac{2\pi}{T}=2\pi f

For a point at radius rr, arc length is s=rθs=r\theta. Differentiating gives tangential speed v=rωv=r\omega. All points on one rigid rotating body have the same angular speed, but a point farther from the axis has a larger linear speed.

Quantity Meaning Unit
θ\theta angular displacement radians
ω\omega angular speed rad s−1\mathrm{rad\,s^{-1}}
TT time for one revolution seconds
ff revolutions per second hertz, s−1\mathrm{s^{-1}}
vv distance travelled per second along the circle m s−1\mathrm{m\,s^{-1}}

A wheel completes 1515 revolutions in 66 minutes. Its period is 360/15=24360/15=24 s andω=2π24=π12 rad s−1.\omega=\frac{2\pi}{24}=\frac{\pi}{12}\,\mathrm{rad\,s^{-1}}.A point 88 m from the axis therefore moves at v=8(π/12)=2π/3 m s−1v=8(\pi/12)=2\pi/3\,\mathrm{m\,s^{-1}}.

Do not insert degrees into s=rθs=r\theta or v=rωv=r\omega, confuse revolutions per minute with radians per second, or assume equal angular speed means equal tangential speed at different radii.

Use inward radial acceleration

A particle moving in a circle accelerates even when its speed is constant, because its velocity direction changes. The acceleration points radially inward, towards the centre of the circle.

ar=v2r=rω2a_r=\frac{v^2}{r}=r\omega^2

The inward acceleration is not an extra force. Choose inward as the positive radial direction and resolve the actual forces:∑Finward=mv2r=mrω2.\sum F_{\mathrm{inward}}=m\frac{v^2}{r}=mr\omega^2.Forces pointing away from the centre enter with a negative sign.

Component Direction What changes it describes
radial acceleration towards the centre direction of velocity
tangential acceleration along or opposite the motion magnitude of speed
uniform circular motion radial component present, tangential component zero constant speed but changing velocity

A 0.400.40 kg particle moves at 3.0 m s−13.0\,\mathrm{m\,s^{-1}} in a circle of radius 1.51.5 m. Thenar=3.021.5=6.0 m s−2,a_r=\frac{3.0^2}{1.5}=6.0\,\mathrm{m\,s^{-2}},so the resultant inward force must be 0.40(6.0)=2.40.40(6.0)=2.4 N. Individual forces need not each equal 2.42.4 N; their inward components must have that resultant.

Do not draw radial acceleration tangentially, call mv2/rmv^2/r a separate 'centripetal force', or write a radial force balance without defining which direction is inward. The speed may be constant while velocity and acceleration are not zero.

Resolve forces in a horizontal circle

For uniform motion in a horizontal circle, vertical acceleration is zero while the horizontal resultant towards the centre is mrω2mr\omega^2. Draw every real force, resolve vertically for equilibrium, and resolve horizontally inwards for circular motion.

∑Fvertical=0,∑Finward=mrω2\sum F_{\mathrm{vertical}}=0,\qquad \sum F_{\mathrm{inward}}=mr\omega^2

Context Forces and modelling decision
conical pendulum tension has vertical and inward components; r=lsin⁡θr=l\sin\theta if θ\theta is from the vertical
smooth banked surface normal reaction supplies vertical and inward components
rough banked surface friction acts along the surface; choose its direction from the tendency to slip and use ∣F∣≤μR|F|\le\mu R
elastic string calculate extension and tension with Hooke's law before resolving
contact with a floor require normal reaction R≥0R\ge0; at loss of contact, R=0R=0

Mark the circle's horizontal radius before resolving. Geometry determines rr and the angles of strings or reactions. Use limiting friction only when the speed is at a limiting value; otherwise the friction magnitude is an unknown no greater than μR\mu R. Check that every tension and reaction is non-negative.

A 0.500.50 kg particle is a conical pendulum on a string of length 1.21.2 m at 30∘30^\circ to the vertical. Its circle has radius r=1.2sin⁡30∘=0.60r=1.2\sin30^\circ=0.60 m. FromTcos⁡30∘=mg,Tsin⁡30∘=mrω2,T\cos30^\circ=mg,\qquad T\sin30^\circ=mr\omega^2,division gives tan⁡30∘=rω2/g\tan30^\circ=r\omega^2/g. Hence ω=3.07 rad s−1\omega=3.07\,\mathrm{rad\,s^{-1}} and T=mg/cos⁡30∘=5.66T=mg/\cos30^\circ=5.66 N using g=9.8 m s−2g=9.8\,\mathrm{m\,s^{-2}}.

Do not put mrω2mr\omega^2 into the vertical balance, use the sloping string length as the circle radius, assume friction has magnitude μR\mu R away from limiting motion, or ignore the non-negative contact/tension conditions that restrict possible angular speeds.

Combine energy and radial force in a vertical circle

In a vertical circle, speed changes with height while the required inward resultant remains mv2/rmv^2/r. Use conservation of energy to find speed at a position, then use a separate radial equation to find tension or reaction.

Let θ\theta be measured from the lowest point and let the bottom speed be uu. The height above the bottom is r(1−cos⁡θ)r(1-\cos\theta). With no non-conservative work,v2=u2−2gr(1−cos⁡θ).v^2=u^2-2gr(1-\cos\theta).For a particle on a taut string, resolving inward gives

T−mgcos⁡θ=mv2rT-mg\cos\theta=\frac{mv^2}{r}

Position θ\theta Radial equation for a string
bottom 00 T−mg=mv2/rT-mg=mv^2/r
side π/2\pi/2 T=mv2/rT=mv^2/r
top π\pi T+mg=mv2/rT+mg=mv^2/r

A string must satisfy T≥0T\ge0; a smooth contact must satisfy reaction R≥0R\ge0. At the first loss of constraint, set the relevant force to zero. For a string to complete a full vertical circle, the limiting top condition is vtop2=grv_{\mathrm{top}}^2=gr, which with energy gives the minimum bottom speed u=5gru=\sqrt{5gr}. A rigid rod can push as well as pull, so it does not use the string-tension condition.

A particle on a string enters the bottom with u2=6gru^2=6gr. At the top, energy gives v2=6gr−4gr=2grv^2=6gr-4gr=2gr, soT+mg=2mg⇒T=mg>0.T+mg=2mg\quad\Rightarrow\quad T=mg>0.The string remains taut there. At the bottom, T−mg=6mgT-mg=6mg, so T=7mgT=7mg; the larger bottom tension supplies both the inward acceleration and opposition to the downward weight.

Do not use one constant speed around a vertical circle, mix the energy equation with the radial force equation, reverse the inward weight component, or continue constrained circular motion after tension/reaction becomes negative. After a string goes slack, the particle follows unconstrained projectile motion until another interaction.

M3.5 - Statics of rigid bodies

Syllabus
2019
Topic
M3.5
Level
A2

Find the centre of mass of a rigid body

The centre of mass is the point at which the body's total mass may be treated as concentrated when calculating moments. For a uniform body, symmetry locates every coordinate that lies on an axis or plane of symmetry; integration is needed for a remaining coordinate when the shape varies.

xˉ=1M∫x dm,yˉ=1M∫y dm,M=∫dm\bar x=\frac{1}{M}\int x\,\mathrm dm,\qquad \bar y=\frac{1}{M}\int y\,\mathrm dm,\qquad M=\int\mathrm dm

Uniform body Suitable mass element
thin rod or wire dm=λ ds\mathrm dm=\lambda\,\mathrm ds
lamina dm=ρA dA\mathrm dm=\rho_A\,\mathrm dA
solid dm=ρV dV\mathrm dm=\rho_V\,\mathrm dV
solid of revolution about the xx-axis dV=πy2 dx\mathrm dV=\pi y^2\,\mathrm dx

Choose axes that exploit symmetry. Write both the total mass and its first moment using the same density model and limits, then divide first moment by total mass. For a simple composite body, treat each part as a point mass at its own centre of mass:xˉ=∑mixi∑mi,yˉ=∑miyi∑mi.\bar x=\frac{\sum m_i x_i}{\sum m_i},\qquad \bar y=\frac{\sum m_i y_i}{\sum m_i}.A removed piece is entered with negative mass (or negative area or volume when density is common).

A uniform 6×46\times4 rectangular lamina has a 2×22\times2 square removed from its top-right corner. Taking the lower-left corner as the origin, use the full rectangle minus the hole:xˉ=24(3)−4(5)24−4=2.6,yˉ=24(2)−4(3)24−4=1.8.\bar x=\frac{24(3)-4(5)}{24-4}=2.6,\qquad \bar y=\frac{24(2)-4(3)}{24-4}=1.8.The centre shifts left and down, away from the removed mass, which checks the result.

Use mass, not geometric area or volume, unless uniform density makes them proportional. Keep every coordinate relative to one origin, use the perpendicular distance required by the chosen moment, and never assume that the centre of mass lies inside a hollow or concave body.

Test equilibrium, suspension and toppling

A rigid body is in equilibrium only when the resultant force is zero and the resultant moment about any point is zero. Its weight acts vertically through its centre of mass, so the position of that vertical line controls suspension and toppling.

∑F=0,∑MP=0\sum \mathbf F=\mathbf0,\qquad \sum M_P=0

Situation Equilibrium condition
freely suspended from a fixed point the centre of mass lies vertically below the suspension point in stable equilibrium, so the weight has zero moment about the point
body on a horizontal plane the vertical through the centre of mass must meet the contact base; at limiting toppling it passes through an edge
body on an inclined plane provided sliding is prevented, the same vertical line must meet the contact base; increasing inclination moves its intersection towards the downhill edge

First find the centre of mass in body-fixed coordinates. For suspension, rotate the body until the line joining the suspension point to the centre of mass is vertical. For a supported body, identify the possible pivot edge and take moments about it. At the instant of toppling the reaction at the opposite side has fallen to zero and the resultant contact force acts through the pivot edge.

A uniform rectangular block has base length bb measured up the line of greatest slope and its centre of mass is a perpendicular distance hh above the plane. On a rough plane inclined at θ\theta, the vertical through the centre of mass meets the plane htan⁡θh\tan\theta downhill from the middle of the base. It is stable against toppling whilehtan⁡θ<b2,h\tan\theta<\frac b2,and is on the point of toppling when htan⁡θ=b/2h\tan\theta=b/2. This test assumes the available friction prevents sliding first.

Do not align the centre of mass with the plane's normal: weight is vertical. Do not set friction equal to μR\mu R unless sliding is limiting, and do not assume toppling occurs before sliding; both conditions must be checked when the friction information is available.