Engineering Sciences · Study · FE Chemical · FE → PE Prep
Engineering Sciences
4% of exam
Basic dynamics (friction, force, mass, acceleration, momentum), work, energy, and power for particles and rigid bodies, and electricity fundamentals (charge, current, voltage, power, Ohm's law, and Kirchhoff's laws).
2 concepts
A. Basic dynamics
Newtonian Dynamics, Work, Energy and Power
Newton's second law with friction, the work-energy theorem, and impulse-momentum for particles — the three bookkeeping methods that solve almost every FE dynamics question.
Dynamics rewards the engineer who picks the right bookkeeping tool before touching a number. Three laws cover the entire FE Engineering Sciences dynamics set: Newton's second law ∑F=ma when you want an instantaneous acceleration or force, the work-energy theorem when a problem links force and distance to a change in speed, and the impulse-momentum theorem when force and time govern a change in velocity — especially across impacts. The NCEES FE Reference Handbook collects all three under Dynamics (Particle Kinetics), and the points are lost not in the physics but in the setup: a missing friction term, a velocity squared that should not be squared, or a USCS mass that forgot the
gc
factor. This concept builds the reflex of naming the method first, drawing one clean free-body diagram, and carrying units the whole way.
Newton's second law and the free-body diagram
For a particle of constant mass, Newton's second law is the vector statement that the net force equals mass times acceleration. Everything starts with a free-body diagram: isolate the body, draw every external force (weight, normal, applied, friction, tension), choose axes, and write one scalar equation per axis. On an incline it almost always pays to align one axis with the surface so the normal direction has zero acceleration. Acceleration is shared by all forces on the body — it is not a force you add to the diagram.
∑F=ma=mdtdv
Friction: the force that is an inequality
Dry (Coulomb) friction acts along the contact surface, opposing relative sliding or its tendency. The handbook states it as F≤μsN: below impending motion the friction force is whatever static value the other equations require, capped at μsN; once sliding begins it takes the fixed kinetic value F=μkN, usually with μk<μs. The normal force N is whatever the surface actually pushes with — on a flat floor N=mg, but on an incline N=mgcosθ, and any vertical component of an applied force changes it. Friction is never μmg by reflex; it is μN with N from the perpendicular equilibrium.
Ff=μkN(sliding),Ff≤μsN(static)
The mass-force relation and the gc factor
In SI, ∑F=ma with force in newtons, mass in kilograms, and acceleration in m/s2 — no conversion constant appears. USCS is the trap: with mass in lbm, force in lbf, and acceleration in ft/s2, the handbook writes F=ma/gc where gc=32.174lbm⋅ft/(lbf⋅s2). The constant exists only to reconcile the pound-mass and pound-force, which were defined so that one pound-mass weighs one pound-force at standard gravity. A body of m lbm weighs W=mg/gc lbf; at standard g that is numerically W=m, which is exactly why people forget gc when an acceleration is not g.
F=gcma,gc=32.174lbf⋅s2lbm⋅ft
Work, kinetic energy, and the work-energy theorem
Work is the line integral of force along the path, U=∫F⋅dr; for a constant force at angle θ to the displacement it is U=Fscosθ. The principle of work and energy states that the net work done on a particle equals its change in kinetic energy, T=21mv2. This is the fastest route whenever a problem gives forces and distances and asks for a speed, because time never enters. Forces perpendicular to motion (a normal force, the tension on a body moving along a level path) do no work, which is what makes the method clean.
U1→2=T2−T1=21mv22−21mv12
Potential energy and conservation
When only conservative forces act — gravity and ideal springs — mechanical energy is conserved: T2+V2=T1+V1. Gravitational potential energy is Vg=mgh relative to a chosen datum, and a linear spring stores Ve=tfrac12ks2 where s is the deflection from the free length. When a nonconservative force such as friction is present, add its work as a separate term, T2+V2=T1+V1+U1to2nc, where U1to2nc is the work of the nonconservative forces only (negative for a dissipative force) and explicitly excludes the gravity and spring work already carried in V. Note this differs from the work-energy theorem, where U1to2 is the net work of ALL forces; mixing the two double-counts gravity or spring work. Choosing the right datum and a consistent sign convention removes most arithmetic errors.
T1+V1+U1to2nc=T2+V2,qquadV=mgh+tfrac12ks2
Impulse, momentum, and impact
Linear momentum is p=mv, and integrating Newton's law over time gives the impulse-momentum theorem: the impulse of the net force equals the change in momentum. For a collision with no external impulse, total momentum is conserved, m1v1+m2v2=m1v1′+m2v2′. Kinetic energy is conserved only in a perfectly elastic impact (e=1); a perfectly plastic impact (e=0) has the bodies move off together and dissipates the most energy. The coefficient of restitution e relates the relative separation and approach speeds along the line of impact.
mv2=mv1+∫t1t2Fdt,e=(v1−v2)n(v2′−v1′)n
Power and efficiency
Power is the time rate of doing work, P=dU/dt, and for a force moving a body at velocity v it is the dot product P=F⋅v. Mechanical efficiency is the ratio of useful output power to input power, η=Pout/Pin. These appear in FE problems as pump, motor, and hoist questions — watch the unit families (1hp=550ft⋅lbf/s=746W) and keep force and velocity collinear before multiplying.
P=dtdU=F⋅v,η=PinPout
Exam strategy
Name the method before you compute. If the question pairs force with distance and asks for speed, use work-energy and avoid solving for acceleration. If it pairs force with time, or involves a collision, use impulse-momentum or conservation of momentum. If it asks for an instantaneous acceleration or a force at one instant, use ∑F=ma with a free-body diagram. Always resolve forces on the incline before computing N, write friction as μN (never μmg blindly), and in USCS insert gc the moment you see lbm with a non-g acceleration. A quick units check on the final number — N, J, or W — catches most slips.
Key equations
Newton's second law (particle)∑F=ma=mdtdv
Net external force equals mass times acceleration. SI: F in N, m in kg, a in m/s2. Apply per axis from a free-body diagram.
Newton's law in USCS (gc form)F=gcma,gc=32.174lbf⋅s2lbm⋅ft
Energy of motion of a particle. v = speed (m/s), result in J. Note v
Work of a forceU=∫F⋅dr=Fscosθ(constant F)
θ = angle between force and displacement; forces perpendicular to motion do zero work.
Work-energy theoremU1→2=21mv22−21mv12
Conservation of energyT1+V1+U1to2nc=T2+V2
Linear impulse-momentummv2=mv1+∫t1t2Fdt
Conservation of momentum (impact)m1v1+m2v2=m1v1′+m2v2′
Coefficient of restitutione=(v1−v2)n(v2′−v1′)n,0≤e≤1
Power and efficiencyP=F⋅v,η=PinPout
Worked examples
Acceleration of a dragged box (Newton's second law with friction)
Problem. A 25kg box rests on a level floor with kinetic friction coefficient μk=0.30. A horizontal force of 120N is applied. Find the acceleration. Use g=9.81m/s2.
Solution. Vertical equilibrium gives the normal force: N=mg=25×9.81=245.25N.
Kinetic friction opposes motion: Ff=μkN=0.30×245.25=73.6N
a=mFap−μkmg=25120−(0.30)(25)(9.81)=1.86m/s2
Speed at the bottom of an incline (work-energy theorem)
Problem. A 12kg block is released from rest and slides 5.0m down a 30∘ incline with kinetic friction coefficient μk=0.25
Perfectly plastic collision (conservation of momentum)
Problem. A 2000kg truck moving at 15m/s strikes a stationary 1000kg car; the two lock together. Find the common velocity after impact and the kinetic energy lost.
Solution. No significant external impulse acts during the brief impact, so momentum is conserved. Bodies stick (perfectly plastic, e=0
USCS force with the gc factor
Problem. A 50lbm casting on a frictionless conveyor must be accelerated at 8.0ft/s2. What horizontal force in lbf is required?
Solution. In USCS, Newton's second law carries the conversion constant gc
Common pitfalls
•Writing friction as μmg on an incline. The normal force there is N=mgcosθ, so Ff=μmgcosθ; using μmg overestimates friction.
•Dropping the gc factor in USCS. With lbm and lbf you must use F=ma/gc; it only 'disappears' when the acceleration happens to equal g
•Treating kinetic energy as linear in v. T=21mv2 — doubling speed quadruples kinetic energy; a missing square is the most common work-energy mistake.
•Using work-energy when force and time are given (or impulse-momentum when force and distance are given). Match the theorem to what the problem supplies before computing.
•Assuming kinetic energy is conserved in every collision. Momentum is always conserved (no external impulse), but KE is conserved only for a perfectly elastic impact (e=1); plastic impacts dissipate energy.
•Forgetting that a normal force and a perpendicular tension do no work. Including them in ∫F⋅dr corrupts the energy balance.
•Mixing power units: 1hp=550ft⋅lbf/s=746W. Multiplying a force in lbf by a velocity in ft/s gives ft·lbf/s, not hp.
References
NCEES FE Reference Handbook — Dynamics
NCEES FE Reference Handbook — Dynamics (Laws of Friction) — Laws of Friction: $F \\le \\mu N$; below impending motion $F < \\mu_s N$ (no slip), at impending motion $F = \\mu_s N$, while sliding $F = \\mu_k N$. Printed in the Dynamics section, consistent with section 1.
Hibbeler, Engineering Mechanics: Dynamics — Work-energy and impulse-momentum methods; source of the handbook's notation.
C. Electricity, current, and voltage laws
Electricity: Charge, Ohm’s and Kirchhoff’s Laws
Charge, current, voltage and power, Ohm's law, series and parallel resistance, and Kirchhoff's two laws — the toolkit for any resistive DC circuit on the FE.
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Required whenever mass is in lbm and force in lbf; gc reconciles the two. Weight W=mg/gc.
Friction opposes relative motion. N = actual normal force (mgcosθ on an incline). μs,μk dimensionless.
Links velocity, acceleration, time, and displacement for constant a. Use with ∑F=ma to bridge force and motion.
is squared — never linear.
Net work equals change in kinetic energy. Time-free — ideal for force-and-distance to speed problems.
V=mgh+tfrac12ks2. U1to2nc = work of nonconservative forces only (negative for friction; zero for conservative systems). Distinct from the work-energy theorem U1to2, which is the net work of all forces — do not equate the two.
Impulse of net force equals change in momentum. For constant F: FΔt=mΔv.
Holds when external impulse is negligible during impact. KE conserved only if e=1.
e=1 perfectly elastic, e=0 perfectly plastic (bodies stick). Applied along the line of impact.
Power in W (or ft·lbf/s); 1hp=746W. Force and velocity must be collinear.
.
Apply
∑Fx=ma
along the floor:
120−73.6=25a
, so
a=25120−73.575=2546.43=1.86m/s2.
Sanity check: with no friction the acceleration would be
120/25=4.80m/s2
, so friction must reduce it —
1.86m/s2
is appropriately smaller. Final answer:
a=1.86m/s2
in the direction of the applied force.
. Find its speed at the bottom. Use
g=9.81m/s2
.
Solution. Forces along the 5m path: gravity component mgsinθ aids motion; friction μkN=μkmgcosθ opposes it. The normal force is N=mgcosθ.
Net work over distance d:
U1→2=mgd(sinθ−μkcosθ)=(12)(9.81)(5)(sin30∘−0.25cos30∘).U1→2=588.6(0.5−0.2165)=588.6×0.2835=167J.
Work-energy theorem from rest: U1→2=21mv2, so
v=m2U1→2=122(166.86)=27.81=5.27m/s.
Sanity check: a frictionless drop of the same vertical height h=5sin30∘=2.5m gives v=2gh=7.00m/s; friction must lower this, and 5.27m/s is correctly less. Final answer: v=5.27m/s.