Intuition What this page is for
The parent note gave you the rule : momentum is conserved only when the net external force on your chosen system is zero (in a direction, or over a tiny instant). This page hunts down every kind of situation that rule can produce — every sign, every degenerate case, every trap — and works each one from scratch. If you finish this page, no exam scenario should surprise you.
Before anything else, three symbols we will lean on. If any feels shaky, this page re-earns it as we go.
Definition The three symbols we reuse
P = ∑ i m i v i — total momentum of the system: add up (mass × velocity) for every object we chose to track. It is a vector : it has a horizontal (x ) part and a vertical (y ) part, and they behave independently.
F e x t n e t — the net external force : add up (as vectors) only the pushes coming from outside the boundary we drew.
J = ∫ F d t = F a v g Δ t — impulse : force multiplied by the time it acts. This is the thing that actually changes momentum, from the Impulse–Momentum Theorem .
The parent's master equation ties them together:
d t d P = F e x t n e t ⟺ Δ P = J e x t
Read it as: "the only thing that can change the group's total momentum is an outside impulse."
Every problem this topic throws is one (or a mix) of these cells . The worked examples below are tagged with the cell they cover.
Cell
What makes it distinct
The trap it hides
A. Zero total, opposite signs
System starts at rest; parts fly apart with opposite-sign velocities
Forgetting the minus sign on the recoiling piece
B. One-axis conservation
External force acts along one axis only (gravity in a launch)
Claiming all momentum is conserved when only P x is
C. Boundary choice flips the answer
Same physics, momentum conserved or not depending on where you draw the system
Thinking "conserved" is a property of nature, not of your choice
D. Impulsive approximation
Collision + a background force (gravity, friction) acting during contact
Testing forces instead of impulses
E. Degenerate / limiting mass
One mass → ∞ (a wall) or → 0
Assuming momentum "vanishes" when a partner is a wall
F. 2-D angled collision
Velocities point at angles; must split into x and y
Adding speeds like scalars instead of vector components
G. Momentum yes, energy no
Inelastic collision — check both laws separately
Assuming KE is conserved because P is
H. Exam twist: continuous mass — stream hitting a target, and a rocket losing mass
Mass, not velocity, is what changes
Using F = ma when mass is changing
We now walk all eight cells (Cell H gets two examples: an inflow stream and a mass-losing rocket).
Worked example A firecracker at rest bursts into two pieces
A stationary firecracker of mass 5 kg bursts into two pieces on a frictionless table. A 2 kg piece flies right at 30 m/s. Find the velocity of the 3 kg piece.
Forecast: The other piece must go left . Faster or slower than 30 ? (It's heavier, so guess slower .)
Step 1 — Choose the system and check external force. System = both pieces. The bursting force is between the pieces ⇒ internal . Table is frictionless; gravity and normal are vertical and cancel. So horizontal F e x t = 0 .
Why this step? Only after confirming F e x t , x = 0 are we allowed to write P x = constant.
Step 2 — Write initial and final P x . Initially at rest: P x , i = 0 . Take right as + .
0 = ( 2 ) ( + 30 ) + ( 3 ) ( v )
Why this step? Conservation means "before = after"; we set them equal.
Step 3 — Solve.
v = 3 − 60 = − 20 m/s ⇒ 20 m/s to the left .
Why this step? The minus sign is the physics — it tells us the direction , matching the forecast.
Verify: Total after = ( 2 ) ( 30 ) + ( 3 ) ( − 20 ) = 60 − 60 = 0 = total before. ✓ Units: kg·m/s throughout. Heavier piece slower (20 < 30), as forecast. ✓
Worked example Cannon on the ground (revisited, both axes checked)
A cannon (M = 400 kg) fires a ball (m = 4 kg) horizontally at 200 m/s. Find the recoil speed, and explicitly show which axis is conserved and which is not.
Forecast: Horizontal is safe (nothing pushes sideways from outside). Vertical is not (gravity, normal). Guess recoil ≈ 2 m/s.
Step 1 — Split forces by axis. Firing force = internal. External: gravity (down) and ground normal (up) — both vertical . So F e x t , x = 0 but F e x t , y = 0 in general.
Why this step? Newton's law is one equation per axis ; we treat x and y separately.
Step 2 — Conserve P x only. Right = + , initially rest:
0 = M ( − V ) + m v ⇒ V = M m v = 400 4 ⋅ 200 = 2 m/s .
Why this step? We are forbidden from writing a P y conservation line — the ground supplies vertical impulse. We simply don't need y .
Verify: P x , after = 400 ( − 2 ) + 4 ( 200 ) = − 800 + 800 = 0 . ✓ In the figure, the pink (ball) and blue (cannon) horizontal arrows are equal-and-opposite; the green vertical ground arrow shows why P y is not conserved. Units: kg·m/s. ✓
Worked example A ball bounces off the floor
A 0.5 kg ball hits the floor moving down at 6 m/s and rebounds up at 4 m/s. (a) Is its momentum conserved? (b) What impulse did the floor deliver? (c) For which system is momentum conserved?
Forecast: For the ball alone, momentum clearly changed (it reversed) — so not conserved. The floor must have supplied the impulse.
Step 1 — System = ball alone. Take up = + . Before: p i = 0.5 ( − 6 ) = − 3 kg·m/s. After: p f = 0.5 ( + 4 ) = + 2 kg·m/s.
Why this step? With the ball alone, gravity and the floor's normal are external — so we expect P to change, and we compute by how much .
Step 2 — Impulse from the change.
J = Δ p = p f − p i = 2 − ( − 3 ) = + 5 N⋅s (upward) .
Why this step? Δ P = J e x t — the change is the impulse. This is the Impulse–Momentum Theorem doing the work.
Step 3 — Enlarge the system to ball + Earth. Now the floor's push and gravity are internal (Earth is inside). By Newton's 3rd law they cancel ⇒ total P (ball + Earth) is conserved. Earth recoils by an unmeasurably tiny amount.
Why this step? Shows the punchline: "conserved" is a statement about your chosen boundary, not about nature.
Verify: J = + 5 N·s is positive (upward), consistent with a floor that pushes up. Magnitude sanity: ∣ J ∣ = 5 > ∣ p i ∣ = 3 because the ball not only stopped (+ 3 ) but was thrown back up (+ 2 ). ✓
Worked example Two pucks collide in mid-air
Two pucks (combined mass 2 kg) collide during a contact lasting Δ t = 2 ms. A typical contact impulse in this hit is about 5 N·s. Show that gravity can be ignored during the collision, and quantify the tiny error.
Forecast: Gravity acts for only 2 ms during contact — its impulse should be minuscule next to 5 N·s.
Step 1 — Compute gravity's impulse during contact.
J g = m g Δ t = 2 × 9.8 × 0.002 = 0.0392 N⋅s .
Why this step? The correct test compares impulses , not forces — impulse is what changes P .
Step 2 — Form the ratio.
J c J g = 5 0.0392 ≈ 0.0078 = 0.78%.
Why this step? A ratio under 1% means treating P as conserved through the impact introduces under a percent of error.
Step 3 — Two-phase strategy. Conserve P through the collision (ignore gravity), then re-include gravity for the free flight before and after.
Why this step? This is how the approximation is actually used: it isolates the collision as an instantaneous event.
Verify: J g = 0.0392 N·s and ratio = 0.00784 < 0.01 . ✓ Units: (kg)(m/s²)(s) = kg·m/s = N·s. ✓
Worked example A ball bounces elastically off a fixed wall
A 0.2 kg ball hits a rigid wall at 10 m/s and rebounds at 10 m/s (elastic). Is the ball's momentum conserved? Is momentum conserved for ball + wall? What is the limiting picture as the wall's mass → ∞ ?
Forecast: The ball's momentum flips sign — not conserved for the ball alone. The wall (attached to Earth) absorbs the impulse.
Step 1 — Ball alone. Take incoming direction = + . Before p i = 0.2 ( + 10 ) = + 2 ; after p f = 0.2 ( − 10 ) = − 2 .
Δ p = − 2 − 2 = − 4 N⋅s .
Why this step? The wall's normal force is external to the ball, so a nonzero Δ p is expected.
Step 2 — The limit "wall = infinite mass". Momentum conservation of ball+wall says the wall gains + 4 N·s. Its velocity change is Δ V = J / M w a l l = 4/ M w a l l . As M w a l l → ∞ , Δ V → 0 : the wall stays still yet carries the momentum.
Why this step? This is the degenerate case — the "wall" is really an object so massive its velocity change is negligible, exactly like the Earth in Example 3.
Verify: lim M → ∞ 4/ M = 0 . ✓ Ball's KE before = 2 1 ( 0.2 ) ( 1 0 2 ) = 10 J, after = 10 J — elastic, KE conserved, consistent with speed unchanged. ✓
Worked example Glancing collision on a frictionless table
Ball A (1 kg) moves right at 4 m/s and strikes stationary ball B (1 kg). After impact, A moves off at 3 0 ∘ above the original line at 2 3 m/s. Find B's velocity vector.
Forecast: B must carry the "missing" sideways momentum downward to keep P y = 0 , and share the forward momentum.
Step 1 — Check external force, pick axes. Frictionless table ⇒ no horizontal external force ⇒ both P x and P y conserved. Let x = A's original direction.
Why this step? On a horizontal frictionless table the whole momentum vector is conserved — both axes are fair game.
Step 2 — Conserve P x . Before: ( 1 ) ( 4 ) + 0 = 4 .
4 = ( 1 ) ( 2 3 cos 3 0 ∘ ) + ( 1 ) v B x = 2 3 ⋅ 2 3 + v B x = 3 + v B x ⇒ v B x = 1.
Why this step? x -components add like ordinary numbers once resolved.
Step 3 — Conserve P y . Before: 0 .
0 = ( 1 ) ( 2 3 sin 3 0 ∘ ) + ( 1 ) v B y = 2 3 ⋅ 2 1 + v B y = 3 + v B y ⇒ v B y = − 3 .
Why this step? The initial sideways momentum was zero, so the two final sideways parts must cancel — B goes down .
Step 4 — Assemble. v B = ( 1 , − 3 ) , speed = 1 + 3 = 2 m/s at angle arctan ( 3 /1 ) = 6 0 ∘ below the line.
Why this step? Convert components back to a magnitude-and-direction answer.
Verify: P x : 3 + 1 = 4 ✓. P y : 3 − 3 = 0 ✓. In the figure the pink (A') and blue (B') arrows tip-to-tail rebuild the original yellow arrow — that's momentum conservation drawn as a vector triangle. Note A' at 3 0 ∘ and B' at 6 0 ∘ are perpendicular — the signature of an equal-mass elastic hit. ✓
Worked example Two clay lumps stick together
A 3 kg lump moving right at 4 m/s hits a 1 kg lump moving left at 4 m/s. They stick. Find the common velocity, then check kinetic energy.
Forecast: The heavier lump wins ⇒ they move right, but slower than 4 . KE will drop (clay deforms).
Step 1 — Conserve P x (frictionless, no external horizontal force). Right = + :
3 ( 4 ) + 1 ( − 4 ) = ( 3 + 1 ) v f ⇒ 12 − 4 = 4 v f ⇒ v f = 2 m/s (right) .
Why this step? Sticking is an internal force, so P is conserved regardless of the mess.
Step 2 — Compare kinetic energy before/after.
K E i = 2 1 ( 3 ) ( 4 2 ) + 2 1 ( 1 ) ( 4 2 ) = 24 + 8 = 32 J , K E f = 2 1 ( 4 ) ( 2 2 ) = 8 J .
Why this step? Momentum and energy have different conditions — we must test energy separately (see Elastic vs Inelastic Collisions ).
Step 3 — Interpret the loss. Δ K E = 8 − 32 = − 24 J, lost to heat and deformation. P still conserved; KE not.
Why this step? Directly refutes the parent's steel-manned mistake "momentum and energy conserved together or not at all."
Verify: P i = 12 − 4 = 8 = P f = 4 ( 2 ) = 8 ✓. K E f = 8 < 32 = K E i ✓. Fraction of KE lost = 24/32 = 75% . ✓
Before this example, one new symbol.
Definition Mass flow rate
m ˙
When matter flows continuously (water from a hose, gas from a rocket), we track how many kilograms pass a point each second. We call this the mass flow rate , written m ˙ (read "m-dot"; the dot means "rate of change per second," so m ˙ = d t d m ). Its units are kg/s. It answers: "how much mass arrives per unit time?" — the quantity we need because here mass, not velocity, is what keeps changing.
Worked example A stream of water hits a plate
Water leaves a hose at 20 m/s and strikes a wall horizontally at a rate of 3 kg/s, then falls straight down (no rebound). Find the horizontal force on the wall.
Forecast: Force = rate of momentum destroyed. Guess around 3 × 20 = 60 N.
Step 1 — Momentum arriving per second. In one second, m ˙ = 3 kg of water carrying horizontal velocity 20 m/s arrives:
Δ t Δ p x = m ˙ v = 3 × 20 = 60 kg⋅m/s per s .
Why this step? When mass flows, the right tool is F = d t d p = m ˙ v , not F = ma (mass isn't fixed).
Step 2 — All horizontal momentum is destroyed. Water leaves with zero horizontal velocity (it just slides down), so its horizontal momentum drops from m ˙ v to 0 each second.
F on water = Δ t Δ p x = 0 − 60 = − 60 N .
Why this step? The question asks for a horizontal force, so we track only the horizontal momentum; the wall must supply exactly the impulse per second that kills the incoming horizontal momentum. The minus sign says the wall pushes the water backward (against its motion).
Step 3 — Newton's 3rd law: force on the wall. The wall pushes the water with − 60 N; by Newton's Third Law the water pushes the wall with the opposite force:
F on wall = + 60 N (in the direction of the stream) .
Why this step? The question asked for the force on the wall , which is the reaction to the force on the water — so we flip the sign.
Verify: ∣ F on wall ∣ = m ˙ v = 3 ( 20 ) = 60 N, matching the forecast of "around 60 N." The sign is positive — the wall is pushed the way the water was going, exactly as a hose visibly shoves a plate. Units: (kg/s)(m/s) = kg·m/s² = N. ✓
The stream example added mass to a target. The mirror case is a rocket : it throws mass away to push itself forward. Same tool (F = m ˙ v ), opposite bookkeeping.
Definition The thrust idea (why exhaust pushes the rocket)
A rocket carries no wall to push against. Instead it ejects burnt gas backward at some speed u (relative to the rocket). By Newton's Third Law , throwing gas backward pushes the rocket forward. The forward push is called thrust , and it equals the rate at which backward momentum is flung out:
F thrust = u m ˙ ex ,
where m ˙ ex is how many kg of exhaust leave per second. This is the outflow twin of F = m ˙ v : instead of momentum being destroyed at a plate, momentum is created in the exhaust, and its equal-and-opposite reaction drives the rocket.
Worked example A hovering rocket
A rocket burns fuel at m ˙ ex = 4 kg/s, ejecting exhaust at u = 500 m/s relative to itself. (a) Find the thrust. (b) The rocket + unburnt fuel has mass 180 kg at this instant. Can it lift off (g = 9.8 m/s²)? (c) What is its instantaneous upward acceleration?
Forecast: Thrust = 4 × 500 = 2000 N. Weight ≈ 180 × 9.8 ≈ 1764 N. Thrust beats weight, so yes — it lifts, with a modest acceleration.
Step 1 — Thrust from the outflow rule.
F thrust = u m ˙ ex = 500 × 4 = 2000 N (upward) .
Why this step? Momentum is being poured into the exhaust at rate u m ˙ ex ; by Newton's 3rd law the reaction of that same size drives the rocket. We use F = m ˙ v , not F = ma , because the rocket's mass is dropping.
Step 2 — Compare thrust with weight (the external force here).
W = M g = 180 × 9.8 = 1764 N (down) .
Net upward force on the rocket body: F net = 2000 − 1764 = 236 N .
Why this step? Gravity is the genuine external force on the rocket system; thrust is the internal ejection reaction. Lift-off needs thrust > weight.
Step 3 — Instantaneous acceleration. Apply F net = M a at this instant (mass is 180 kg right now ):
a = M F net = 180 236 ≈ 1.31 m/s 2 upward .
Why this step? Once we have the net force, ordinary Newton's 2nd law gives the acceleration for that instant — the mass-change is already accounted for inside the thrust term.
Verify: Thrust 2000 N > weight 1764 N ⇒ lifts off. ✓ a = 236/180 = 1.3 1 m/s² > 0 , consistent with rising. Units: thrust (m/s)(kg/s) = kg·m/s² = N ✓; a in N/kg = m/s² ✓. Sanity: exhaust (500 m/s) far exceeds any rocket speed here, so treating u as the ejection speed is valid.
Recall Quick self-test across the matrix
Explosion from rest — sign of the second piece's velocity? ::: Opposite to the first (total stays zero).
Cannon fires horizontally — which momentum component is conserved? ::: Horizontal only; vertical is broken by gravity and normal.
Ball bounces off floor — conserved for ball alone? ::: No; yes for ball + Earth.
Correct test for ignoring gravity in a collision? ::: Compare impulses, not forces.
Ball off a fixed wall as M w a l l → ∞ — wall's velocity change? ::: Zero, yet it carries the momentum.
Sticking (inelastic) collision — is KE conserved? ::: No; only momentum is.
Water stream hitting a wall — which formula for force? ::: F = m ˙ v , not F = ma .
Rocket thrust from ejecting exhaust — formula? ::: F thrust = u m ˙ ex (exhaust speed × burn rate).
Mnemonic The 8-cell checklist
"A-BC-D-E-F-G-H" → A part (explosion), B oundary+axis, C hoice flips, D elta-t impulsive, E normous/tiny mass, F ull 2-D, G one energy, H ose and rocket (flowing mass, in and out).