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Coriolis Force Calculator

Calculate Coriolis force on a moving object from mass, velocity, and latitude.
Predicts apparent deflection on a rotating Earth for ballistics.

Coriolis Force

Coriolis Force

The Coriolis force is an apparent (or fictitious) force experienced by objects moving in a rotating reference frame, such as the surface of the Earth. It does not act on stationary objects — only those moving relative to the rotating frame.

Formula

For horizontal motion on Earth’s surface, the magnitude of the Coriolis force is:

F = 2 × m × v × Ω × sin(φ)

Where:

  • m = mass of the object (kg)
  • v = horizontal velocity (m/s)
  • Ω = angular velocity of Earth = 7.2921 × 10⁻⁵ rad/s
  • φ = latitude (in degrees, converted to radians for the sine)

Direction of Deflection

Hemisphere Deflection
Northern Hemisphere Right of motion
Southern Hemisphere Left of motion
Equator No horizontal Coriolis force (sin 0 = 0)
Poles Maximum effect (sin 90° = 1)

Worked Example — Long-Range Artillery

A 45 kg shell traveling at 800 m/s at 40° N latitude:

  • F = 2 × 45 × 800 × 7.29 × 10⁻⁵ × sin(40°)
  • F ≈ 3.38 N

Over a 30-second flight, this produces several meters of lateral deflection — which is why long-range gunnery, naval artillery, and ballistic missile guidance must compensate for the Coriolis effect.

Common Real-World Effects

Phenomenon Coriolis Role
Hurricane / typhoon rotation Sets the direction of cyclone spin
Trade winds Deflects equator-bound air westward
Foucault pendulum Plane of oscillation rotates
Long-range artillery Lateral correction needed
Ocean gyres Drives large-scale circulation
Atmospheric jet streams Maintains zonal flow pattern

Common Myths

The Coriolis force does not determine which way water spins down a drain — that is dominated by basin shape, residual currents, and asymmetries. The effect is too weak at small scales (a few seconds, a few meters) to matter compared to other forces.

Why “Fictitious”?

In a non-rotating inertial frame, no Coriolis force exists. The “force” is a mathematical bookkeeping term that lets us use Newton’s laws inside a rotating frame, just as the centrifugal force does. For long-range projectiles and atmospheric flow, however, treating it as a real force is the most practical way to model motion.


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