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Physics · Mechanics · Grade 10

Free fall and air

A coin and a feather fall differently in air but together in a vacuum — why?

Open the experiment

The situation

Until Galileo's time most people thought that a heavy body falls faster than a light one. And indeed, if you let go of a coin and a feather at the same moment, the coin hits the floor at once, while the feather flutters down through the air. The speed of a parachutist jumping from a plane also does not increase without limit — it levels off at about 200 km/h. What really decides how things fall: mass, air or the planet? We test this with Newton's tube, a parachutist, a thrown ball and light gates in the laboratory.

Topic

Free fall and air resistance. Feather and coin in a vacuum tube, a parachutist's terminal velocity

Key ideas

  • Acceleration of free fall
  • Air resistance
  • Terminal velocity

Formulas

v=gt,h=gt22

Free fall: no initial speed, no air resistance.

y=v0t−gt22,tk=v0g,hmax=v022g

An object thrown vertically upwards: time of ascent and maximum height.

Fq=12CρSv2,vch=2mgCρS

Air resistance at high speed; the terminal velocity comes from the condition Fd=mg.

g=GM(R+h)2

The acceleration of free fall depends on the distance to the planet's centre.

g=2(h2−h1)t22−t12,g=4π2LT2

Laboratory: the two-light-gate and simple pendulum methods.

Theory

Why do all objects fall alike?

The Earth pulls every object with a force proportional to its mass: F=mg. But the greater the mass, the harder it is to accelerate (inertia): a=F/m=g. The mass cancels — without air, a coin and a feather fall with the same acceleration. Pump the air out of Newton's tube: from a height of 0.90 m both land in 2h/g≈0.43 s. Motion under gravity alone, with no initial speed, is free fall, a special case of uniformly accelerated motion.

Air resistance depends on speed

At low speeds (a dust particle, a small ball in honey) the resistance is proportional to speed — Stokes' law (the “Viscosity and flow” experiment). At high speed it is proportional to the square of the speed: Fd=12CρSv2. As the speed increases, Fd grows; when Fd=mg the acceleration is zero and the object falls uniformly at its terminal velocity. For a feather this is ≈ 0.6 m/s, for a parachutist ≈ 55–60 m/s, and with an open parachute ≈ 5–6 m/s. If the air becomes thinner (ρ decreases), vt increases.

The parachutist

Just after the jump, a≈g; as the speed increases the resistance grows and the acceleration falls — the v(t) graph bends over and approaches the terminal velocity line (after ~15 s and ~600 m). Falling belly-down the area is large, head-down it is small, so the terminal velocity is higher. When the parachute opens, CS increases about 80 times: for a few seconds the resistance exceeds the weight and slows the person down (≈ 3–4 g), and then a new terminal velocity is established. At altitude the air is thinner, so at 4 km the terminal velocity is about 16 % higher than at 1 km.

Vertically and horizontally launched objects

For a vertical throw, y=v0t−gt2/2 and v=v0−gt. At the highest point v=0: tk=v0/g, hmax=v02/2g. Motion without air is symmetric: the fall also takes v0/g, the object returns to the hand with speed v0, and the strobe dots lie at the same heights. With air, the rise is shorter and the fall longer. For an object launched horizontally the two motions are independent: uniform horizontally and free fall vertically — it reaches the ground at the same moment as an object that is simply dropped. Launching at an angle to the horizontal is in the “Basketball: the free throw” experiment.

g far from the Earth

From the law of universal gravitation, mg=GMm/(R+h)2, so g=GM/(R+h)2: if the distance to the centre increases 2 times (h=R), g falls 4 times. On the International Space Station (≈ 400 km), g≈8.7 m/s² — the weightlessness there is not due to an absence of gravity but to free fall together with the station. Even on the Earth's surface g is not the same everywhere: ≈ 9.78 m/s² at the equator and ≈ 9.83 m/s² at the poles (because of the Earth's rotation and shape), and ≈ 9.80 m/s² in Tashkent.

Measuring g (laboratory work)

Two gates: a ball is released from rest, and a stopwatch shows t1 and t2; from h=gt2/2, g=2(h2−h1)/(t22−t12). If you plot the measurements on an h–t2 graph, the slope of the straight line is g/2. Simple pendulum: for a small angle T=2πL/g, g=4π2L/T2; measure the time for 10 oscillations and divide by 10, and keep the angle below 10° (at 20°, g comes out ≈ 1.5 % too low). For a physical (reversible) pendulum, T=2πI/(mgd); when the periods about the two pivots are equal, the distance between them equals the reduced length lk and g=4π2lk/T2 (in detail — “Swing”, “Spring pendulum”). The model: C is constant, there is no wind, the parachute uses the standard atmosphere, and elsewhere g and ρ are constant.

Did you know?

  • In 1971 David Scott, commander of the Apollo 15 mission, dropped a geological hammer and a falcon feather on the Moon's surface at the same moment — because there is no air, both reached the surface together.
  • In 2012 Felix Baumgartner jumped from a capsule carried by a stratospheric balloon at about 39 km and reached a speed of about 1358 km/h: the air there is so thin that he exceeded the speed of sound.

Inside the experiment

The experiment starts from a real-life situation: you predict the result, change the controls, run the experiment and draw a conclusion. Inside are missions, theory, a quiz and a guided tour in which the camera moves and explains the key points.

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