Every key Laws of Motion formula, definition and theorem for JEE Main Physics in one place — with common examiner traps and worked examples. Free to read; blurt from memory, then check your gaps.
Syllabus — topics coveredNTA · 15 sub-topics
Force and inertia
Newton's first law of motion
Momentum
Newton's second law of motion
Impulse
Newton's third law of motion
Law of conservation of linear momentum and its applications
Equilibrium of concurrent forces
Static and kinetic friction
Laws of friction
Rolling friction
Lubrication
Dynamics of uniform circular motion
Centripetal force
Examples of circular motion
Newton's Three Laws & Inertia
First law (law of inertia): If the net external force is zero, a body stays at rest or in uniform motion: Fnet=0⇒a=0. Inertia= resistance to change of state; mass measures it.
Frames of reference
▸Inertial frame: at rest or uniform velocity — Newton's laws hold.
▸Non-inertial (accelerating) frame: laws need a pseudo-force (page 4).
Second law
F=dtdp=ma,p=mv
F= net external force (N), p= momentum, m= mass (constant), a= acceleration; 1N=1kg m s−2
About the 2nd law
▸Vector law — one equation per axis: Fx=max, Fy=may.
▸Only external forces count; a is that of the centre of mass for a system.
▸Local: a now depends on F now, not on history.
Comparative: the three laws
Law
States
Gives
1st (inertia)
Fnet=0⇒a=0
defines inertial frame & force
2nd
F=dp/dt=ma
magnitude of force / accn
3rd
FAB=−FBA
forces in equal-opposite pairs
Third law
FAB=−FBA
FAB= force on A by B; to every action an equal & opposite reaction
About the 3rd law
▸Action & reaction act on different bodies — never cancel on one body.
▸They act at the same instant (no cause–effect order).
▸Internal forces of a system cancel in pairs ⇒ sum to zero.
★ Remember · Aristotle's fallacy
A force is not needed to keep a body in uniform motion — only to overcome friction. Rest and uniform motion are equivalent states (both a=0).
🚫 Examiner Trap · Newton's laws & inertia
(1) Action–reaction act on two different bodies, so they can NEVER cancel each other — don't pair N with mg on the same block (those are a 2nd-law balance, not a 3rd-law pair). (2) F=ma uses the net force; sum all forces first. (3) F=dp/dt=ma only when m is constant — for variable mass use dp/dt. (4) Newton's laws fail in an accelerating frame unless you add a pseudo-force.
⚡ Shortcut · Spotting an action–reaction pair
Swap the two bodies in the phrase 'force on A by B' → 'force on B by A'; same type, same line, equal magnitude, opposite sense, different body. If both forces act on the same body, it is NOT a 3rd-law pair.
Impulse, Momentum & Conservation
Linear momentum: p=mv — a vector, the 'quantity of motion'. Same force for the same time gives the same Δp to any mass.
Impulse–momentum theorem
J=∫Fdt=FavΔt=Δp
J= impulse (N s) = area under the F-t curve, Fav= average force, Δp= change in momentum
★ Remember · Impulsive force
A very large force for a very short time (bat–ball, collision). Increase Δt (bend knees, draw hands back) to cut the force for a given Δp.
Conservation of momentum
Fext=0⇒p=const;pA+pB=pA′+pB′
Fext= net external force; primes = after interaction; follows from 2nd + 3rd laws, holds for elastic or inelastic
Comparative: elastic vs inelastic (1-D)
Elastic
Perfectly inelastic
e
1
0
p
conserved
conserved
KE
conserved
max loss (stick together)
After
separate
common velocity v
Applications
▸Recoil (gun–bullet): mgvg=−mbvb.
▸Machine gun firing n bullets/s of mass m at speed v: force on the gunner F=nmv (rate of momentum given out).
▸Explosion: fragments' momenta add to the initial (often 0).
Variable mass (rocket)
Fthrust=vreldtdm;v=u+vrellnmm0
vrel= exhaust speed relative to rocket, m0= initial mass, m= instantaneous mass, u= initial speed; the ln result neglects gravity
Fext=Macm with M=m1+m2; if Fext=0, vcm const
🎯 Exam · Coefficient of restitution
e=speed of approachspeed of separation=u1−u2v2−v1 (e=1 elastic, 0 perfectly inelastic). Energy analysis of collisions → Work-Energy unit.
🚫 Examiner Trap · Momentum & impulse
(1) Momentum is a vector — conserve it component-wise; in 2-D explosions use px and py separately. (2) Momentum is conserved in every collision (elastic OR inelastic); only KE is lost in inelastic ones — don't say p is lost. (3) Impulse =Δp, so a ball bouncing back has Δp=m(v+u) (reversal), not m(v−u). (4) Fext=0 is required for conservation — gravity/normal during a long collision are usually negligible only over the SHORT impact time.
⚡ Shortcut · Perfectly inelastic speed
Two bodies stick: v=m1+m2m1u1+m2u2 (=vcm). KE lost =21m1+m2m1m2(u1−u2)2 (reduced mass μ) — the maximum loss among all e.
Force Analysis: FBD & Equilibrium
Common forces
▸Weight mg — vertically down.
▸Normal N — ⊥ to the contact surface (a push, never a pull).
▸Tension T — along the string; same throughout a massless string over a smooth pulley.
▸SpringF=−kx (restoring, ∝ deformation).
Comparative: contact-force facts
Force
Direction
Key fact
Normal N
⊥ surface
push only; N=mg in general
Tension T
along string
pull only; uniform if massless
Spring kx
along spring
F=−kx, restoring
Friction f
along surface
opposes relative slip
Equilibrium of a particle
Concurrent forces
∑F=0⇒∑Fx=0,∑Fy=0
∑F= vector sum of all forces; the forces form a closed polygon (head-to-tail)
Lami's theorem (3 concurrent forces)
sinαF1=sinβF2=sinγF3
α,β,γ are the angles opposite to F1,F2,F3; valid only for 3 concurrent coplanar forces in equilibrium
🎯 Exam · FBD method
(1) Isolate one body. (2) Draw only the external forces on it (weight, normal, tension, friction, applied). (3) Choose axes (along the motion / incline). (4) Apply ∑F=ma per axis.
Tips
▸On a smooth incline of angle θ: a=gsinθ, N=mgcosθ.
▸Massless string ⇒ same tension at both ends; massless rod can also push.
▸Two blocks in contact (force F on M1 touching M2): contact force N=M1+M2M2F.
★ Remember · Reading apparent forces
A weighing machine reads the normal reaction N; a spring balance reads the tension T — not necessarily mg.
🚫 Examiner Trap · FBD & equilibrium
(1) Never put a force on a body that another body exerts on a THIRD body — draw only what touches THIS body. (2) N=mg only on a horizontal surface with no vertical applied force; on an incline N=mgcosθ, and a downward push raises N. (3) Lami's angles are the ones opposite each force, not between them. (4) Tension is uniform only for a massless string over a smooth pulley — a heavy or accelerating string has different tensions.
⚡ Shortcut · 3-force equilibrium
For exactly 3 concurrent forces, either close the triangle (sides ∥ forces) or use Lami. If two forces are equal and the third bisects their angle, the system is symmetric — exploit it.
Connected Bodies, Pulleys, Pseudo-force & Lift
Atwood machine (smooth pulley)Two masses over a smooth, massless pulley.
Acceleration & tension
a=m1+m2(m2−m1)g;T=m1+m22m1m2g
m2>m1 assumed; a= accn of each block, T= string tension, g= gravity
▸Inextensible string: components of acceleration along the string are equal.
▸Movable (light) pulley: apulley=2a1+a2; tension on the support =2T.
▸Differentiate the length equation twice to get the acceleration constraint.
More set-ups (frequently asked)
▸Heavy rope (mass M, length L) pulled by F on a smooth floor: tension at distance x from the pulled end T=F(1−Lx). Hanging rope: T at height y above the free end =LMgy.
▸Chain on a rough table: the largest fraction that can hang over the edge without sliding is 1+μμ.
▸Block on a smooth wedge (angle θ): it stays at rest on the wedge if the wedge accelerates horizontally at a=gtanθ (then N=cosθmg).
Non-inertial frame & pseudo-force
Pseudo-force
Fpseudo=−ma0
m= body's mass, a0= acceleration of the (non-inertial) frame; add it on every body in that frame
Apparent weight N=m(g±a).
Apparent weight in a lift
N=m(g+a) up, m(g−a) down, 0 in free fall
N= reading of the floor/balance, a= lift acceleration magnitude; free fall (a=g) ⇒ weightlessness
Comparative: apparent weight in a lift
Lift motion
N reads
Felt
At rest / uniform v
mg
normal
Accel. up (or decel. down)
m(g+a)
heavier
Accel. down (or decel. up)
m(g−a)
lighter
Free fall a=g
0
weightless
🚫 Examiner Trap · Connected bodies & frames
(1) On a frictionless pulley a single string has ONE tension throughout — but the hanging and table blocks have the SAME acceleration magnitude, not the same forces. (2) A movable pulley splits/halves: apulley=(a1+a2)/2 and the supporting tension is 2T. (3) Pseudo-force −ma0 is added ONLY in the accelerating frame; never add it in the ground frame. (4) Apparent weight = true weight: N=m(g±a); deceleration flips the sign.
⚡ Shortcut · System acceleration
For bodies moving together, a=total massnet driving force (treat as one block). Then isolate one body to get the internal tension/contact force. Two-block contact: N=MtotalmaheadF, where mahead is the mass beyond the contact (the part being pushed).
Friction
Friction: Contact force parallel to the surface, opposing relative motion (or its tendency).
Static (self-adjusting)
fs≤μsN
fs= static friction, μs= static coeff, N= normal; fs adjusts to balance the applied force up to μsN
Block on a rough incline (angle θ), tending to slide down: friction acts up the slope.
Laws of friction
▸f∝N; independent of the apparent area of contact and of speed.
▸Rolling friction ≪ sliding < limiting static — smallest of the three.
Comparative: static vs kinetic
Static fs
Kinetic fk
Value
≤μsN (variable)
μkN (fixed)
When
no slipping (yet)
sliding
Max
μsN (limiting)
—
Order
larger (μs>μk)
smaller
Angle of friction / repose
tanλ=μs;tanθrep=μs
λ= angle of friction, θrep= angle of repose = max incline before sliding; both equal tan−1μs
Rough incline (angle θ)
adown=g(sinθ−μcosθ);aup=−g(sinθ+μcosθ)
adown= accn sliding down, aup= retardation of a block sent up; μ=μk while sliding
Minimum pull on a horizontal surface
Fmin=1+μ2μmg
applied at angle θ=tan−1μ above the horizontal (this angle minimises the pull)
🎯 Exam · Block on block
For a block sliding on another, friction acts on both surfaces (equal & opposite); check whether they move together (compare required friction with μsN).
🚫 Examiner Trap · Friction
(1) Static friction is ≤μsN, NOT =μsN — it equals only the force needed, up to the limit. Using μsN when the body isn't about to slip is the #1 error. (2) Friction is independent of contact AREA. (3) On an incline, friction enters N=mgcosθ via μcosθ, not μsinθ. (4) Friction opposes relative slipping, so it can act forward (e.g. it drives a car / a block carried by a sheet). (5) Once moving, use μk (smaller), not μs.
⚡ Shortcut · Will it slide?
On an incline a block stays put iff θ≤θrep=tan−1μs (i.e. tanθ≤μs). To just hold/start it, the required friction =mgsinθ; compare with μsmgcosθ.
Circular Dynamics: Level, Banking & Conical
Centripetal force
Fc=rmv2=mω2r
Fc= net inward force, v= speed, r= radius, ω= angular speed; not a new force — provided by tension/gravity/friction/normal
Vehicle on a level road
Friction provides Fc
rmv2≤μsmg⇒vmax=μsrg
vmax= max safe speed on a flat road; independent of mass m
Banked road (angle θ)Banking: Nsinθ points to the centre; tanθ=rgv2 (no friction).
v0: no friction needed; vmax: friction acts down the bank; vmin: friction acts up the bank (vmin=0 if μs≥tanθ); θ= bank angle
Comparative: providing the centripetal force
Setup
Provided by
Limit / key
Level road
friction
vmax=μsrg
Banked (no μ)
Nsinθ
tanθ=v2/rg
Conical pend.
Tsinθ
tanθ=v2/rg
Conical pendulumBob in a horizontal circle; string sweeps a cone.
Equations
Tcosθ=mg;Tsinθ=rmv2
T= string tension, θ= angle from vertical, r= circle radius; dividing gives tanθ=v2/rg
Angular speed & period
ω=Lcosθg;Tp=2πgLcosθ
L= string length, Tp= period, r=Lsinθ
★ Remember · Key idea
Always resolve forces toward the centre (=rmv2) and perpendicular to it (=0). The centripetal direction is the acceleration direction.
🚫 Examiner Trap · Circular dynamics
(1) Centripetal force is NOT a new/extra force — never add mv2/r as a separate arrow; it is the net inward component of real forces. (2) 'Centrifugal force' exists only in the rotating (non-inertial) frame as a pseudo-force; never use it in the ground frame. (3) Banking tanθ=v2/rg assumes NO friction — it gives v0, not vmax. (4) vmax and vmin on a banked road have friction acting down/up the slope respectively; sign of the μ term flips.
⚡ Shortcut · Banking & conical share tanθ
Frictionless banked road and conical pendulum give the same relation tanθ=rgv2=gω2r — both have a tilted normal/tension whose horizontal part is mv2/r and vertical part is mg.
Vertical Circle
At angle θ from the lowest point
v2=u2−2gl(1−cosθ);T=lmv2+mgcosθ
u= speed at the bottom, v= speed at angle θ, l= radius, T= string tension there
Just completing the loop (string): at the top T=0 and gravity alone supplies mv2/l.
Just completes the loop (string)
vtop=gl,vside=3gl,vbot=5gl
vtop,vside,vbot= minimum speeds at top/side/bottom; from energy conservation between points
Tensions at critical speed
▸Ttop=0, Tside=3mg, Tbot=6mg.
▸Condition to complete the loop: u≥5gl at the bottom.
Comparative: string vs rod (vertical circle)
String / track
Light rod
Top condition
vtop≥gl
vtop≥0
Min u (bottom)
5gl
4gl
Support can
pull only
push or pull
If too slow
goes slack / leaves
still rigid
🎯 Exam · Rod vs string
A light rod can push, so the bob just reaches the top with vtop=0 (u≥4gl). A string needs vtop≥gl (else it goes slack and the bob leaves the circle).
If 2gl<u<5gl (string)
▸The string goes slack between the horizontal and the top — the bob becomes a projectile.
▸For u≤2gl: the bob oscillates (never crosses the horizontal).
🚫 Examiner Trap · Vertical circle
(1) At the top the minimum speed is gl for a STRING/track (where T=0 and gravity alone supplies mv2/l), but 0 for a RIGID rod — don't use gl blindly. (2) Tbot−Ttop=6mg for any speed (energy + dynamics), a favourite result. (3) Speed at the top is NOT zero for a string — it must be ≥gl. (4) For 2gl<u<5gl on a string the bob doesn't oscillate AND doesn't loop — it leaves the circle as a projectile.
⚡ Shortcut · Top-to-bottom relations
At the critical (just-completes) case: vbot2=5gl, vside2=3gl, vtop2=gl (differ by 2gl each, from Δh). Tension always satisfies Tbot−Ttop=6mg regardless of u.
What are the most important Laws of Motion formulas for JEE Main?
This Laws of Motion formula sheet covers all the high-yield Physics formulas, definitions and theorems you need for JEE Main, across Force and inertia, Newton's first law of motion, Momentum, Newton's second law of motion, Impulse — each shown with the key result and, where useful, a worked example.
Is this Laws of Motion formula sheet free?
Yes — the full chapter formula sheet is free to read online, no login or payment required.
How should I revise Laws of Motion formulas?
Blurt the Laws of Motion formulas from memory, then check against this sheet to find your gaps — and practise a few previous-year questions on the chapter to make sure you can apply them under time pressure.