Physics

Stokes' Law: The 1851 Formula for How Slowly Small Things Fall

Stokes derived it in 1851 correcting pendulum clocks for air drag. Millikan used it in 1913 to weigh the electron, and got the number slightly wrong.

Last updated: 2026-09-02

An 1860s portrait photograph of Sir George Gabriel Stokes, the Cambridge mathematician and physicist who derived Stokes' law in an 1851 paper on pendulum motion
Photo: Unknown author, 1860s, via Smithsonian Institution Photography, public domain

Core summary

George Gabriel Stokes derived the law in an 1851 paper on pendulum motion, working out how strongly a viscous fluid resists a small sphere moving slowly through it: drag force equals six times pi times the fluid's viscosity, the sphere's radius, and its velocity. Combined with gravity and buoyancy, that formula gives a particle's terminal velocity, and it holds only in the Reynolds-number regime below roughly 1, where viscous forces dominate over inertial ones, a window that covers cloud droplets and fine sediment grains but not actual raindrops. Robert Millikan and Harvey Fletcher used the law between 1909 and 1913 to isolate the electron's charge from suspended oil droplets, publishing 1.592 x 10^-19 coulombs with a claimed 0.2 percent uncertainty; the modern value of 1.602 x 10^-19 coulombs differs by about half a percent, a gap later traced to the value Millikan plugged in for air's viscosity. The same formula, applied to soil and sediment settling through water, still underlies the hydrometer method labs use to sort particles by size, valid across a range of roughly 0.2 millimeters down to 0.0002 millimeters.

The pendulum problem Stokes was actually trying to solve

George Gabriel Stokes wasn't trying to explain how spheres fall through liquid when he worked out the formula that now carries his name. He was chasing a much narrower problem: in the mid-1800s, a swinging pendulum was one of the most precise instruments available for measuring g, the local acceleration due to gravity, and getting an accurate reading meant accounting for every force acting on the bob, including the drag of the surrounding air, which slows the swing and throws off the timing a clean gravitational calculation depends on. Stokes worked through the physics in a paper for the Transactions of the Cambridge Philosophical Society, "On the Effect of the Internal Friction of Fluids on the Motion of Pendulums," published in 1851, a decade into his career at Cambridge.

To correct for that drag, Stokes needed a general answer to a specific question: how much does a viscous fluid resist a small sphere moving slowly through it? He derived that the resisting force is proportional to the fluid's viscosity, the sphere's radius, and its velocity, a relationship now written as F = 6πηrv, where η stands for the fluid's viscosity, r for the sphere's radius, and v for its velocity. The formula answered Stokes' pendulum question, but it also turned out to describe something much broader than a swinging bob: how any small sphere settles through a viscous fluid under gravity, a fact that would matter far more to later physicists than the pendulum problem that produced it.

The formula, and what it actually predicts

Stokes' drag formula comes out of a simplified version of the Navier-Stokes equations for what fluid dynamicists call creeping flow, the regime in which a fluid's viscosity dominates the physics and the moving object's own inertia barely registers. Set that drag against the pull of gravity, minus the buoyant push from the fluid the sphere displaces, and the two balance out at a constant falling speed known as terminal velocity, v = d²gΔρ / (18η), where d is the sphere's diameter, g is gravitational acceleration, Δρ is the difference between the sphere's density and the fluid's, and η is the fluid's viscosity. Run in reverse, timing how fast a sphere of known size and density falls through a liquid whose viscosity is unknown, the same equation is still how a falling-ball viscometer measures viscosity directly, a piece of lab equipment built on 170-year-old physics.

Plugging in real numbers shows how slowly the formula predicts small things fall. A water droplet 40 micrometers across, roughly the width of a fine human hair and a realistic size for an individual droplet inside a cloud, has a density of about 1,000 kilograms per cubic meter settling through air, whose viscosity runs about 1.81 x 10^-5 pascal-seconds at 20°C. Working through Stokes' formula with those figures gives a terminal velocity of roughly 4.8 centimeters per second, slow enough that the droplet takes close to a minute to sink three meters, and slow enough that an ordinary updraft inside a cloud easily keeps it suspended rather than letting it fall. That size dependence is the same physics behind why a virga streak curves as it falls, where terminal velocity scales with the square of a shrinking droplet's diameter, and it only holds because the droplet stays inside a Newtonian fluid whose viscosity doesn't change no matter how fast it's falling through it.

Why the law breaks down for actual raindrops

That 4.8-centimeter-per-second droplet sits comfortably inside the regime where Stokes' formula holds. Fluid dynamicists express that regime using the Reynolds number, a ratio of inertial to viscous forces, and Stokes' law is considered reliable only below a Reynolds number of roughly 1, with error climbing above 2 percent once it passes about 0.1; the 40-micrometer droplet above works out to a Reynolds number around 0.13, safely inside that window. Solving Stokes' own formula for the diameter at which a falling water droplet in air first crosses a Reynolds number of 1 gives a value of about 80 micrometers, meaning the law's clean linear relationship between drag and velocity is only trustworthy for droplets smaller than roughly the width of a human hair.

Actual raindrops are ten to fifty times larger than that threshold, and they behave nothing like Stokes predicts. NASA's Global Precipitation Measurement mission describes drops smaller than about 1 millimeter as essentially spherical, held in shape by surface tension, but as a drop grows past that size and falls faster, the air pushing against its underside flattens the bottom while the top stays rounded, and once a drop reaches roughly 4 to 5 millimeters across it becomes unstable and splits apart entirely. None of that deformation exists in Stokes' math, which assumes a perfectly rigid, undistorted sphere. Once a falling drop is large enough to flatten under its own aerodynamic pressure, viscosity has stopped being the dominant force resisting its fall, and Stokes' 1851 formula no longer applies.

Real applications: weighing an electron and grading soil

The most famous use of Stokes' law came a good six decades after Stokes published it, and it wasn't about pendulums or raindrops at all. Between 1909 and 1913, Robert Millikan and Harvey Fletcher sprayed a fine mist of oil droplets into a chamber, applied a voltage across it, and used Stokes' formula to work out each droplet's radius from how fast it fell under gravity alone, then measured how strong an electric field was needed to hold a charged droplet motionless against that same gravity, which let them isolate the electric charge sitting on the droplet. Millikan published his result in August 1913, reporting an elementary charge of 1.592 x 10^-19 coulombs and claiming an uncertainty of only 0.2 percent. The modern accepted value is 1.602 x 10^-19 coulombs, a difference of roughly half a percent, and physicists later traced the gap to the specific value Millikan used for the viscosity of air in his Stokes' law calculation, a figure a Swedish researcher named Kellström measured as noticeably higher a couple of decades afterward. Get the viscosity term wrong and Stokes' formula quietly carries that error straight into the answer.

The same formula, run on particles settling through water instead of oil droplets falling through air, still underlies a standard soil-science technique called the hydrometer method: stir a soil sample into water, let it settle, and read a floating hydrometer at set time intervals to see how much material remains suspended, since Stokes' equation converts each settling time directly into a particle diameter. Guelph University researchers who validated the technique found it holds across roughly the range 0.2 millimeters down to 0.0002 millimeters, the same Reynolds-number ceiling that rules out raindrops capping the upper end, while particles finer than about 0.0002 millimeters get jostled around by random Brownian motion faster than gravity can settle them, so the same law that once corrected a pendulum clock is still how a soil lab sorts a handful of dirt into sand, silt, and clay.

Frequently asked questions

What is Stokes' law?

Stokes' law is an 1851 result describing the resistance a thick fluid puts up when a tiny sphere drifts through it. That resistance depends on three things at once: the fluid's thickness, the sphere's dimensions, and how fast it's traveling. Once that pushback matches gravity's pull, the sphere stops speeding up and falls at a constant rate, the speed physicists call terminal velocity.

What is the formula for Stokes' law?

The drag equation is F = 6πηrv, where r is the falling sphere's radius, v is its speed, and η is how viscous the surrounding fluid is. Once that drag cancels out the sphere's weight net of buoyancy, the steady fall rate left over works out to v = d²gΔρ / 18η, using diameter instead of radius and Δρ for the density gap between sphere and fluid.

Why did Stokes come up with this formula in the first place?

He wasn't investigating falling objects to begin with. Stokes needed to correct pendulum-based estimates of Earth's gravitational pull for the resistance a swinging weight meets from the air around it, and he set down the physics behind that correction in a lengthy academic paper published in 1851. Only later did other scientists realize the same reasoning applied just as well to a sphere sinking through any fluid.

Does Stokes' law explain how raindrops fall?

Only for droplets much smaller than a typical raindrop. The formula holds up well for water droplets up to roughly 80 micrometers in diameter, about the size found inside a cloud, but a falling raindrop is far bigger than that, moving fast enough for air pressure to press its underside flat, closer to a bun than a sphere, and drops that grow past around four or five millimeters wide break apart entirely, none of which the original 1851 math accounts for.

How is Stokes' law connected to Robert Millikan's electron charge experiment?

Millikan and a lab partner applied it in the early 1910s, working backward from how fast tiny charged oil droplets sank to figure out their size, a step needed to pin down a single electron's charge. The number he reported came in roughly six-tenths of one percent under what's accepted today. Researchers eventually pinned that shortfall on the specific air-viscosity number he had fed into his math.

What size range of particles can Stokes' law actually be applied to?

In practice, somewhere between two-tenths of a millimeter at the coarse end and two ten-thousandths of a millimeter at the fine end, the window a University of Guelph validation study confirmed for soil sedimentation testing. Go bigger than that and turbulence disrupts the smooth drag the formula assumes; go smaller and Brownian motion, the particle's random jitter from being struck by surrounding molecules, overwhelms gravity's own downward tug long before the particle can settle.

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