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The Rifle That Cannot Aim True North

Irodov 1.111DifficultyDifficulty 3 of 5UniquenessUniqueness 3 of 5

Problem Irodov 1.111

A rifle at latitude φ=60∘\varphi=60^\circ fires a bullet horizontally due north, aimed at a vertical line on a target a horizontal distance s=1.0 kms=1.0\text{ km} away, with muzzle speed v=900 m/sv=900\text{ m/s}. Air drag is negligible, and the only effect considered besides gravity is the Earth’s rotation. Find the sideways distance hh by which the bullet misses the vertical aiming line, and the compass direction of the miss.

The Earth's angular velocity ω, along the polar axis, resolved at the rifle's latitude φ into a component ωφ along the local vertical Z and a component ωφ along the local horizontal, northward direction N.

The Earth’s angular velocity ω\vect\omega, along the polar axis, resolved at the rifle’s latitude φ\varphi into a component ωsin⁡φ\omega\sin\varphi along the local vertical ZZ and a component ωcos⁡φ\omega\cos\varphi along the local horizontal, northward direction NN.

Given
  • φ=60∘\varphi=60^\circ
  • v=900 m/sv=900\text{ m/s}
  • s=1.0 kms=1.0\text{ km}
Find
hh and its compass direction

Solution

Step 1Reference: the equation of motion in a rotating frame

In a reference frame rotating with constant angular velocity ω\vect\omega relative to an inertial frame, a particle of mass mm obeys

mw′=F+mω2ρ+2m (v′×ω)m\vect w' = \vect F + m\omega^{2}\vect\rho + 2m\,(\vect v'\times\vect\omega)
(1)

where w′\vect w' and v′\vect v' are the particle’s acceleration and velocity measured in the rotating frame, F\vect F is the resultant of the real (interaction) forces, and ρ\vect\rho is the position vector drawn perpendicularly from the rotation axis to the particle. The term mω2ρm\omega^{2}\vect\rho is the centrifugal force: it depends only on where the particle is and points away from the axis. The term 2m(v′×ω)2m(\vect v'\times\vect\omega) is the Coriolis force: it depends only on how the particle moves, is perpendicular to both v′\vect v' and ω\vect\omega, and has magnitude 2mv′ωsin⁡θ2mv'\omega\sin\theta, where θ\theta is the angle between v′\vect v' and ω\vect\omega. Both vanish in an inertial frame (ω=0\omega=0), and the Coriolis force does no work, since it is always perpendicular to v′\vect v'.

In this problem the rotating frame is the Earth itself, so ω\vect\omega is the Earth’s rotation about the polar axis and v′\vect v' is the bullet’s velocity relative to the ground, written simply v\vect v where its direction matters: horizontal, northward, of magnitude vv. The real forces F\vect F are gravity alone (drag is neglected), and the centrifugal term is vertical to a very good approximation, so it is already absorbed into the local plumb vertical and the measured value of gg and deflects nothing sideways. The whole sideways miss therefore comes from the Coriolis term, and of the two components into which ω\vect\omega splits at latitude φ\varphi it is the vertical one, ωsin⁡φ\omega\sin\varphi, that crosses a horizontal v′\vect v' into a horizontal deflection.

Step 2The vertical component of the Earth’s rotation

From the first figure, at latitude φ\varphi the component of ω\vect\omega along the local vertical is

ωz=ωsin⁡φ.\omega_z = \omega\sin\varphi.
Step 3The horizontal Coriolis acceleration

Dividing the Coriolis term of (1) by mm gives the bullet’s sideways acceleration. With v′\vect v' horizontal (northward, magnitude vv) and only the vertical component ωz\omega_z of ω\vect\omega contributing a horizontal deflection, the angle between the two is 90∘90^\circ there and the magnitude of the sideways acceleration is

ac=2ωzv=2ωvsin⁡φa_c = 2\omega_z v = 2\omega v\sin\varphi
(2)

directed to the right of the direction of travel in the northern hemisphere, i.e. eastward for a bullet flying north.

Step 4The sideways deflection at the target
What this step works out, in plan view from above: the bullet, aimed along the dashed north line ON, follows the solid path instead and reaches the target's range a distance h east of that aiming line.

What this step works out, in plan view from above: the bullet, aimed along the dashed north line ONON, follows the solid path instead and reaches the target’s range a distance hh east of that aiming line.

The flight time to cover the range ss at the (essentially unchanged) forward speed vv is t=s/vt=s/v. The sideways deflection built up from rest under the constant acceleration (2) is

h=12act2=12(2ωvsin⁡φ)(sv)2\begin{align*}h &= \frac{1}{2}a_c t^2 \\ &= \frac{1}{2}(2\omega v\sin\varphi)\left(\frac{s}{v}\right)^2\end{align*}
h=ωs2sin⁡φvh = \dfrac{\omega s^2\sin\varphi}{v}
(3)
Step 5Numerical value

The Earth’s sidereal angular velocity is ω=2π/(86164 s)\omega=2\pi/(86164\text{ s}), which evaluates to

ω=7.29×10−5 s−1.\omega = 7.29\times10^{-5}\text{ s}^{-1}.

With φ=60∘\varphi=60^\circ, s=1000 ms=1000\text{ m}, v=900 m/sv=900\text{ m/s}, substituting into (3),

h=(7.29×10−5 s−1)(1000 m)2sin⁡60∘900 m/s=0.0702 mh = \frac{(7.29\times10^{-5}\text{ s}^{-1})(1000\text{ m})^2\sin60^\circ}{900\text{ m/s}} = 0.0702\text{ m}
h=ωs2sin⁡φv≈7 cmh = \dfrac{\omega s^2\sin\varphi}{v} \approx 7\text{ cm}
(4)

The deflection is to the east of the aiming line.

Check

Dimensionally, ωs2/v\omega s^2/v is (s−1)(m2)/(m/s)=m(\text{s}^{-1})(\text{m}^2)/(\text{m/s})=\text{m}, a length, as required. At the equator (φ=0\varphi=0) the formula gives h=0h=0: a bullet fired due north along the equator experiences no eastward Coriolis deflection, since there the local vertical is entirely perpendicular to ω\vect\omega and ωz=0\omega_z=0, consistent with Step 2.

Remark

The deflection is eastward specifically because the bullet travels north in the northern hemisphere; the same rule (deflection to the right of the direction of travel) is why a north-flowing river there erodes its eastern bank more than its western one (Baer’s law). A bullet fired due south from the same rifle would deflect west of its aim line by the identical magnitude, since reversing v\vect v in −2ω×v-2\vect\omega\times\vect v reverses the deflection’s sense along with it.