Mechanics Data Book

Cambridge University Engineering Department

Below is a faithful Markdown transcription of the Mechanics Data Book (2017 Edition), done in exactly the same style as the previous databooks:

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Source: Mechanics Data Book, Cambridge University Engineering Department (2017)


2017 Edition Cambridge University Engineering Department


Contents

  • Definitions
  1. Kinematics
  2. Geometry
  3. Mechanics of Machines
  4. Linear Systems, Vibration and Stability
  5. Areas, Volumes, Centres of Gravity and Moments of Inertia

Definitions

  • A system has one degree of freedom if its configuration is completely specified by one variable; two degrees of freedom if two variables are required.
  • A force is conservative if the work done against it is fully recoverable and independent of path; a conservative force field can be expressed as the gradient of a potential.
  • A rigid body is one in which the relative positions of all constituent particles remain constant under motion.
  • A frame of reference is a coordinate system (Cartesian unless otherwise stated).
  • A plane of motion is defined when all points move in a plane.
  • A sliding motion occurs if no point is fixed; pure rotation if a point is fixed; general plane motion otherwise.
  • The coefficient of friction is μ\mu.
  • A frame of reference is accelerating if non-inertial (fictitious) forces appear.

1. Kinematics

1.1 Velocity and Acceleration in Polar Coordinates

For position vector r=r,er\mathbf{r} = r,\mathbf{e}_r:

v=r˙,er+rθ˙,eθ\mathbf{v} = \dot r,\mathbf{e}*r + r\dot\theta,\mathbf{e}*\theta a=(r¨rθ˙2)er+(rθ¨+2r˙θ˙)eθ\mathbf{a} = (\ddot r - r\dot\theta^2)\mathbf{e}*r + (r\ddot\theta + 2\dot r\dot\theta)\mathbf{e}*\theta

1.2 Velocity and Acceleration in Intrinsic Coordinates

Let ssbe arc length and RRthe radius of curvature:

v=s˙,t\mathbf{v} = \dot s,\mathbf{t} a=s¨,t+s˙2R,n\mathbf{a} = \ddot s,\mathbf{t} + \frac{\dot s^2}{R},\mathbf{n}

1.3 Rotating Reference Frames

Relative Velocity

vP=vQ+(drdt)R+ω×r\mathbf{v}_P = \mathbf{v}_Q + \left(\frac{d\mathbf{r}}{dt}\right)_R + \boldsymbol{\omega}\times\mathbf{r}

Relative Acceleration

aP=aQ+(d2rdt2)R+ω˙×r+2ω×(drdt)R+ω×(ω×r)\mathbf{a}_P = \mathbf{a}_Q + \left(\frac{d^2\mathbf{r}}{dt^2}\right)_R + \dot{\boldsymbol{\omega}}\times\mathbf{r} + 2\boldsymbol{\omega}\times\left(\frac{d\mathbf{r}}{dt}\right)_R + \boldsymbol{\omega}\times(\boldsymbol{\omega}\times\mathbf{r})

1.3.2 Rate of Change of a Vector

For vector x\mathbf{x}:

(dxdt)F=(dxdt)R+ω×x\left(\frac{d\mathbf{x}}{dt}\right)_F = \left(\frac{d\mathbf{x}}{dt}\right)_R + \boldsymbol{\omega}\times\mathbf{x}

If the origin moves with velocity U\mathbf{U}:

(dxdt)F=(dxdt)R+ω×x+(U)x\left(\frac{d\mathbf{x}}{dt}\right)_F = \left(\frac{d\mathbf{x}}{dt}\right)_R + \boldsymbol{\omega}\times\mathbf{x} + (\mathbf{U}\cdot\nabla)\mathbf{x}

2. Geometry

2.1 Radius of Curvature

Cartesian coordinates:

R=[1+(dy/dx)2]3/2d2y/dx2R = \frac{\left[1+(dy/dx)^2\right]^{3/2}}{|d^2y/dx^2|}

Parametric form:

R=[(dx/dt)2+(dy/dt)2]3/2(dx/dt)(d2y/dt2)(dy/dt)(d2x/dt2)R = \frac{\left[(dx/dt)^2+(dy/dt)^2\right]^{3/2}} {|(dx/dt)(d^2y/dt^2)-(dy/dt)(d^2x/dt^2)|}

Polar coordinates:

R=[r2+(dr/dθ)2]3/2r2+2(dr/dθ)2r(d2r/dθ2)R = \frac{\left[r^2+(dr/d\theta)^2\right]^{3/2}} {r^2+2(dr/d\theta)^2-r(d^2r/d\theta^2)}

Intrinsic coordinates:

R=dsdψR = \frac{ds}{d\psi}

2.2 Ellipse

Cartesian:

x2a2+y2b2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1

Polar (focus at origin):

r=l1+ecosθr = \frac{l}{1+e\cos\theta}

where:

l=b2a,e=1b2a2l=\frac{b^2}{a}, \qquad e=\sqrt{1-\frac{b^2}{a^2}}

2.3 Satellite Orbits

Gravitational force:

F=GMmr2F = \frac{GMm}{r^2}

Circular orbit velocity:

v=GMrv = \sqrt{\frac{GM}{r}}

2.4 Solids of Revolution (Pappus’ Theorems)

Volume:

V=2πAxˉV = 2\pi A\bar x

Surface area:

S=2πPxˉS = 2\pi P\bar x

3. Mechanics of Machines

3.1 Friction of a Rope or Belt

Slip begins when:

T1T2=eμθ\frac{T_1}{T_2} = e^{\mu\theta}

3.2 Kinematics of Cams or Gears

Angular velocity ratio:

ω1ω2=O2N2O1N1\frac{\omega_1}{\omega_2} = \frac{O_2N_2}{O_1N_1}

Sliding speed:

C=(ω1ω2)PCC = (\omega_1-\omega_2)PC

4. Linear Systems, Vibration and Stability

4.1 Conservative System (1 DOF)

Potential energy V(q)V(q) Kinetic energy:

T=12M(q)q˙2T = \frac{1}{2}M(q)\dot q^2

Equilibrium:

V(q0)=0V'(q_0)=0

Stability:

V(q0)>0V''(q_0)>0

Natural frequency:

ωn2=V(q0)M(q0)\omega_n^2 = \frac{V''(q_0)}{M(q_0)}

4.2 Response to a General Input

y(t)=0tg(tτ)x(τ),dτy(t)=\int_0^t g(t-\tau)x(\tau),d\tau

4.3 Routh–Hurwitz Stability Criteria

Second order:

a2x¨+a1x˙+a0x=0ai>0a_2\ddot x + a_1\dot x + a_0 x = 0 \quad\Rightarrow\quad a_i>0

Third order:

a3a2>a1a0a_3a_2>a_1a_0

Fourth order:

a3a2a1>a4a12+a32a0a_3a_2a_1 > a_4a_1^2 + a_3^2a_0

4.4 Step Response (Second Order)

y¨+2ζωny˙+ωn2y=x\ddot y + 2\zeta\omega_n\dot y + \omega_n^2 y = x
  • ζ=1\zeta=1: critical damping
  • ζ<1\zeta<1: underdamped

Logarithmic decrement:

lny1y2=2πζ1ζ2\ln\frac{y_1}{y_2}=\frac{2\pi\zeta}{\sqrt{1-\zeta^2}}

4.5 Impulse Response

Impulse input:

x=Nδ(t)x=N\delta(t)

Response:

y(t)=Neζωntωn1ζ2sin(ωdt)y(t)=\frac{Ne^{-\zeta\omega_nt}}{\omega_n\sqrt{1-\zeta^2}} \sin(\omega_dt)

where:

ωd=ωn1ζ2\omega_d=\omega_n\sqrt{1-\zeta^2}

4.6 Harmonic Response

Force excitation:

x=Xcosωtx=X\cos\omega t

Amplitude ratio:

YX=1(1(ω/ωn)2)2+(2ζω/ωn)2\frac{|Y|}{|X|} = \frac{1} {\sqrt{(1-(\omega/\omega_n)^2)^2+(2\zeta\omega/\omega_n)^2}}

Resonance (small damping):

ωr=ωn12ζ2\omega_r=\omega_n\sqrt{1-2\zeta^2}

4.7 Measures of Damping

QuantitySymbolζ1\zeta\ll1
Damping ratioζ\zeta
Quality factorQQ12ζ\frac{1}{2\zeta}
Log decrementδ\delta2πζ2\pi\zeta
Loss factorη\eta2ζ2\zeta

4.8 Modal Analysis

Eigenproblem:

[K]un=ωn2[M]un[K]\mathbf{u}_n = \omega_n^2[M]\mathbf{u}_n

Orthogonality:

umT[M]un=δmn\mathbf{u}_m^T[M]\mathbf{u}*n=\delta*{mn}

4.9 Lagrange’s Equations

ddt(Tq˙i)Tqi+Vqi=Qi\frac{d}{dt}\left(\frac{\partial T}{\partial\dot q_i}\right) - \frac{\partial T}{\partial q_i} + \frac{\partial V}{\partial q_i} = Q_i

4.10 Euler’s Equations (Rigid Body)

Aω˙1(BC)ω2ω3=Q1A\dot\omega_1-(B-C)\omega_2\omega_3=Q_1 Bω˙2(CA)ω3ω1=Q2B\dot\omega_2-(C-A)\omega_3\omega_1=Q_2 Cω˙3(AB)ω1ω2=Q3C\dot\omega_3-(A-B)\omega_1\omega_2=Q_3

5. Areas, Volumes, Centres of Gravity and Moments of Inertia

5.1 Lamina

Ixx=y2,dm=mkx2I_{xx}=\int y^2,dm = mk_x^2

Parallel axis theorem:

Ixx=Ixx+md2I_{xx}=I_{x'x'}+md^2

Perpendicular axis (lamina only):

Izz=Ixx+IyyI_{zz}=I_{xx}+I_{yy}

5.2 Three-Dimensional Bodies

Inertia tensor:

I=[IxxIxyIxz IyxIyyIyz IzxIzyIzz]\mathbf{I}= \begin{bmatrix} I_{xx} & -I_{xy} & -I_{xz} \ -I_{yx} & I_{yy} & -I_{yz} \ -I_{zx} & -I_{zy} & I_{zz} \end{bmatrix}

5.3–5.6 Standard Shapes

  • Rods (straight, curved)
  • Laminae (rectangular, triangular, elliptical, polygonal)
  • Solids of revolution (cylinder, sphere, cone, toroid)
  • Shells of revolution

(Formulae as tabulated in pages 17–20)


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