Degrees per second to Radian per hour

Because °/s maps intuitively to human motion. Tilting your phone 90° in half a second means 180°/s — you can visualise that immediately. The same rate in rad/s (π ≈ 3.14) requires mental conversion. Consumer IMU datasheets list full-scale range in °/s (±250, ±500, ±2000°/s) because the target audience — app developers and game designers — thinks in degrees, not radians.

A standard-rate turn in aviation is 3°/s (completing 360° in two minutes), used for instrument approaches. A fighter jet in a hard combat turn can sustain 15–25°/s, and instantaneous snap rates during aggressive maneuvers can exceed 60°/s. At 20°/s in a tight bank, the pilot experiences 4–6 g of centripetal acceleration, which is near the limit of what a g-suit can compensate for.

A basketball spinning on a fingertip typically rotates at about 3–5 revolutions per second, which is 1,080–1,800°/s. The Harlem Globetrotters can push past 2,000°/s for brief showpiece spins. A professional bowler's ball rotates at roughly 300–500 RPM off the hand, which translates to about 1,800–3,000°/s. Spin rate matters for curve, grip, and the physics of the bounce.

PTZ (pan-tilt-zoom) camera specs list maximum pan speed in °/s — typically 80–400°/s for preset movement and 0.1–5°/s for manual tracking. A camera that pans at 400°/s can whip from one side to the other in under a second, useful for switching between preset positions. The slower manual range lets an operator smoothly follow a walking person without jerky motion.

A standard-rate turn (Rate One) is defined as 3°/s, completing a full 360° circle in exactly two minutes. Air traffic controllers rely on this predictable rate to space aircraft in holding patterns and instrument approaches. The turn coordinator instrument in the cockpit marks the standard rate with reference lines. Faster rates exist (Rate Two is 6°/s), but standard rate keeps the bank angle comfortable at typical airspeeds.

When the object moves so slowly that rad/s and even rad/min produce inconveniently small numbers. Earth's rotation is 0.2618 rad/hr — much friendlier than 7.27 × 10⁻⁵ rad/s. Astronomical telescope tracking, tidal lock studies, and satellite orbital mechanics often involve motions where one rotation takes hours, days, or longer. Rad/hr keeps the numbers readable while preserving the radian basis.

The Moon completes one orbit (2π radians) in about 27.32 days, or roughly 655.7 hours. That gives approximately 0.00958 rad/hr. Compared to Earth's rotation at 0.2618 rad/hr, the Moon's orbital angular speed is about 27 times slower — which is why moonrise drifts about 50 minutes later each day.

Tectonic plates move at a few centimeters per year, but because they sit on a sphere, that linear drift corresponds to a tiny angular rotation about an Euler pole. The fastest plate — the Pacific — rotates at roughly 10⁻⁸ rad/hr (about 0.00000001 rad/hr). That is around a billion times slower than a clock hour hand. Geophysicists describe plate motion this way because angular velocity around an Euler pole neatly captures both the speed and the curved trajectory of every point on the plate.

A geostationary satellite orbits Earth once per sidereal day (~23.934 hours), matching Earth's rotation. Its angular speed is 2π ÷ 23.934 ≈ 0.2625 rad/hr — essentially the same as Earth's surface rotation. That is the whole point: the satellite appears stationary over one spot on the equator because it rotates at the same angular velocity as the ground below it.

Not typically as a primary readout, but it appears in computed outputs from navigation software, satellite tracking systems, and geophysics simulations. Inertial navigation units report gyro drift budgets in °/hr (degrees per hour), and converting to rad/hr is a single multiplication. The unit is more common in calculations and papers than on any physical gauge dial.