The forces acting on rigid bodies can be divided into two groups:
Internal: Fint : (either for translation or rotation)
External: Fext
Concept of system is in mechanical equilibrium.
p is a constant of motion
∑i=1nFi=0 Translational Equilibium
∑yFix=0,∑yFiy=0,∑iFiz=0
∑iτi=0 Rotational Equilibrium
∑iτix=0,∑iτiy=0,∑iτiz=0
Let us say that the system is under equilibrium.
∑Fi = 0 : 2 Conditions
τ about an axis perpendicular to F1 and F2 vanishes.
∑iτi = 0 (Rotational equilibrium) does it remain valid, if the origin is changed.
Moment of the coplanar =r1×(−F)+(r2×F) =(r2−r1)×F = AB×F
"Rotational equilibrium" is independent to the location of the origin.
Case: 1 τ =0, ∑Fi = Ftotal=0
∑Fi =2 F
Under rotational equilibrium, but not translational equilibrium.
Case: 2 ∑Fi = Ftotal = 0
∑τi=τtotal=0
It is under translational equilibrium but not in the rotational equilibrium.
For translation equilibrium : R=F1+F2
Moment about 0 : F1d2=F2d2 rotational equilibrium.
F2F1=l1d2 known as mechanical advantage.
The center of gravity of a body is the point around which the resultant torque due to gravity forces vanishes.
R=Mg of the book.
Centre of gravity(CG)
τ=∑iri×mig=0
∑imiri=0
CM = CG in a uniform gravitational field.
AB=70cm, AG=35cm, AP=30cm, and PG=5cm
AK1=3,K2=10 cm
K1G=K2G=25 cm
TE⇒R1+R2=W1+W
R1+R2=10g
RE⇒−R1(K1G)+R2(K2G)+W1(PG)=0
R1−R2=1.2g
R1 = 54.88N,and R2 = 43.12N
TE⇒∑F=0
∑Fx=0⇒f=N2
∑Fy=0⇒N1=Mg
RE⇒∑τi=0
Mg(2Lcosθ)−N2Lsinθ=0
N2=f=2Mgcotθ
∣F∣=N12+f2=N12+N22
=(Mg)2(1+4cot2θ)
∣F∣=2(Mg)4+cot2θ
The direction of the reaction R is ∠OBE.
TE: ∑F⇒
f=Mg sinθ
N=Mgcosθ
RE: ∣∑τ∣c=0 ⇒Nx=f×2h