Q.An aircraft executes a horizontal loop of radius 1.00km with a steady speed of 900km/h. Compare its centripetal acceleration with the acceleration due to gravity.
Uniform circular motion is motion along a circular path at constant speed. Although the speed stays the same, the velocity does not — its direction keeps changing at every instant — so the motion has an acceleration even though the speed never changes. This concept covers the kinematics of that motion; the force that causes it (centripetal force) belongs to the Laws of Motion unit.
1. Angular Quantities
As the body sweeps through an angle θ, its angular velocity is
ω=dtdθ
For one full revolution in a period T, at frequency f:
ω=T2π=2πf,T=f1
To convert rpm to rad/s:
ω=602π⋅(rpm)=30π(rpm)
The linear (rim) speed v and the angular speed ω are related by
v=ωr
2. Centripetal Acceleration
Even though the speed is constant, the velocity vector keeps turning — this produces an acceleration directed toward the centre of the circle:
ac=rv2=ω2r=T24π2r=4π2f2r
Use whichever form matches the data you are given. This acceleration is often expressed as a multiple of g (as ac/g, taking g=10m/s2).
3. Directions
The velocity is always tangential (along the direction of motion); the acceleration is centripetal — radial, pointing inward, and perpendicular to the velocity.
Because the direction of the velocity keeps changing, the change in the velocity vector over an angle Δθ has magnitude
∣Δv∣=2vsin(2Δθ)
So a quarter turn gives ∣Δv∣=v2, a half turn gives 2v, and a full turn gives 0.
The average acceleration over an arc is ∣Δv∣/Δt — this is smaller in magnitude than the instantaneous centripetal acceleration v2/r, and its direction lies along the perpendicular bisector of the chord joining the two points (which, for a circle, always passes through the centre) rather than being radially inward from either endpoint's own position.
4. Points on a Rotating Body
Every point on a rigid rotating body (a wheel, a disc, a clock hand, the Earth) shares the same ω, but the rim speed v=ωr grows with the radius.
Clock hands: the second hand turns at ω=602π rad/s, the minute hand at 36002π rad/s, the hour hand at 432002π rad/s.
The Earth spins with ω=864002π≈7.3×10−5 rad/s. A point on the equator moves at ωR≈465 m/s, and a point at latitude λ moves at ωRcosλ (since the circle of latitude has radius Rcosλ).
5. Connected Systems
Wheels joined by a belt (or two gears in mesh) share the same rim speed, so ω1r1=ω2r2 — the larger wheel turns with the smaller ω.
Wheels on the same axle (concentric) share the same ω, so the outer rim moves faster (v∝r).
6. Non-Uniform Circular Motion
If the speed also changes, there is a tangential acceleration
at=dtdv=rα
(from the angular acceleration α=dω/dt), in addition to the radial ac=v2/r. These two are perpendicular, so the total acceleration is
The centripetal acceleration of the aircraft is about 6.38 times the acceleration due to gravity. This is found by converting speed to m/s, using ac=v2/r, and dividing by g=9.8m/s2.
The problem asks you to compare two accelerations — one from circular motion, one from gravity. The comparison is just a ratio, but the real insight is that centripetal acceleration depends only on speed and radius, not on mass. So a plane, a car, or a satellite on the same circular path would all feel the same inward pull per unit mass.
The key formula is the centripetal acceleration:
ac=rv2
where v is the speed along the circular path and r is the radius. The acceleration due to gravity near Earth’s surface is g=9.8m/s2 (or 10m/s2 if an approximation is allowed, but we’ll use the standard value).
Now, the trap most students fall into: mixing units. The radius is given in kilometres, the speed in km/h. You cannot plug these directly into v2/r and expect to get m/s2. You must convert everything to SI units (metres and seconds) first.
Let’s work through it step by step.
Convert the radius to metres.
r=1.00km=1000m.
Convert the speed from km/h to m/s.
The conversion factor: 1km/h=3600s1000m=185m/s.
So v=900km/h=900×185m/s.
900÷18=50, then 50×5=250.
Hence v=250m/s.
Tip
A quick mental shortcut: to convert km/h to m/s, multiply by 5/18. For 900, just do 900/18=50, then 50×5=250. No calculator needed.
Concept: Centripetal Acceleration via the Period of the Loop
Method: Find the Loop's Time Period T First, Then Use ac=ω2r with ω=2π/T (Not the Direct v2/r Substitution)
The existing solutions substitute the converted speed and radius directly into ac=v2/r. This method instead finds how long the aircraft takes to complete one full loop (its period T), converts that into an angular speed ω, and only then computes ac=ω2r — a route through time rather than straight through speed.
Step 1 — Convert to SI units (unavoidable first step either way)
r=1.00km=1000m,v=900km/h=900×185=250m/s
Step 2 — Find the period: how long one full loop takes
The aircraft covers the circle's entire circumference, 2πr, once every period T:
T=v2πr=2502π(1000)=8πs≈25.13s
Step 3 — Convert the period into an angular speed
ω=T2π=8π2π=41=0.25rad/s
(This is consistent with ω=v/r=250/1000=0.25rad/s computed the direct way — a useful cross-check that the period was found correctly.)