NCERT Solutions for Class 11 Physics Chapter 9: Mechanical Properties of Fluids
Complete NCERT Class 11 Physics Chapter 9 solutions: topper-format notes on pressure, Pascal’s law, hydraulic machines, streamline flow, Bernoulli’s principle, viscosity, Stokes’ law, surface tension, capillary rise, with all 20 exercise questions (9.1–9.20) solved step by step, NCERT figures redrawn and linked to the PDF pages, and two exam tips for every answer.
Chapter at a glance — complete revision notes
9.1 Introduction
Liquids and gases can flow, and are therefore called fluids. This is the basic property that separates fluids from solids. A fluid has no definite shape of its own: it takes the shape of its container. Solids and liquids have a fixed volume (at atmospheric pressure), whereas a gas fills the entire volume of its container. The volume of a solid, liquid or gas depends on the stress (pressure) acting on it; for solids and liquids the change in volume due to a change of external pressure is rather small, that is, they have much lower compressibility than gases (recall Chapter 8: B(water) = 2.2×109, B(air) = 1.0×105 N m−2).
The key property of fluids is that they offer very little resistance to shear stress; their shape changes under a very small shear stress. The shearing stress that a fluid can sustain is about a million times smaller than that of a solid. Fluids are everywhere: the atmosphere around the Earth, the two-thirds of its surface that is water, and the blood and sap inside living bodies. Understanding them is therefore essential in physics, engineering, medicine and biology.
- Fluid: a substance that can flow (liquid or gas).
- Liquid: practically incompressible, has a free surface of its own.
- Gas: compressible, expands to occupy all the space available.
- Fluid statics (9.2) deals with fluids at rest; fluid dynamics (9.3–9.5) deals with fluids in motion; surface tension (9.6) deals with the free surface of liquids.
9.2 Pressure
A sharp needle pierces the skin but the blunt back of a spoon pressed with the same force does not. An elephant stepping on a man’s chest would crack his ribs, yet a circus performer is saved by a large light plank placed on his chest. Both the force and the area over which it acts matter. The smaller the area, the greater the impact; this impact is called pressure.
A fluid at rest exerts a force on a submerged object, and this force is always normal (perpendicular) to the surface. The reason: if there were a component parallel to the surface, then by Newton’s third law the surface would exert an equal force on the fluid parallel to it; this would make the fluid flow, which cannot happen for a fluid at rest. The normal force at a point can be measured by an idealised gauge (an evacuated chamber with a spring and a piston) as in Fig. 9.1.
Pav = F/A P = limΔA→0 ΔF/ΔA
- Pressure is a scalar. The “force” in the definition is only the component of force normal to the area, not the vector force.
- SI unit: pascal (Pa) = N m−2, after Blaise Pascal (1623–1662). Dimensions [M L−1 T−2].
- 1 atm = 1.013×105 Pa (pressure of the atmosphere at sea level); 1 bar = 105 Pa; 1 torr = 1 mm of Hg = 133 Pa.
- Density ρ = m/V, dimensions [M L−3], unit kg m−3, a positive scalar. Liquids are nearly incompressible, so ρ is almost constant with pressure; gases show a large variation of density with pressure.
- Relative density = (density of substance)/(density of water at 4°C = 1.0×103 kg m−3): a pure number (aluminium: 2.7).
| Fluid | ρ (kg m−3) | Fluid | ρ (kg m−3) |
|---|---|---|---|
| Water | 1.00×103 | Air | 1.29 |
| Sea water | 1.03×103 | Oxygen | 1.43 |
| Mercury | 13.6×103 | Hydrogen | 9.0×10−2 |
| Ethyl alcohol | 0.806×103 | Interstellar space | ≈ 10−20 |
| Whole blood | 1.06×103 |
Table 9.1 (NCERT): densities of some common fluids at STP (0°C, 1 atm).
Worked Example 9.1 (NCERT) — pressure on the femurs
Q. The two thigh bones (femurs), each of cross-section 10 cm2, support the upper part of a human body of mass 40 kg. Estimate the average pressure sustained by the femurs.
Total area A = 2 × 10 cm2 = 20×10−4 m2; F = 40 kg wt = 400 N (g = 10 m s−2). So Pav = F/A = 400/(20×10−4) = 2×105 N m−2.
9.2.1 Pascal’s law
Pascal observed that the pressure in a fluid at rest is the same at all points at the same height. Take a very small right-angled prismatic element ABC-DEF inside the fluid (Fig. 9.2). The forces Fa, Fb, Fc on its faces are normal to those faces. For equilibrium Fb sinθ = Fc and Fb cosθ = Fa; by geometry Ab sinθ = Ac and Ab cosθ = Aa. Dividing,
Fb/Ab = Fc/Ac = Fa/Aa ⇒ Pb = Pc = Pa (9.4)
So pressure at a point in a fluid at rest is the same in all directions, and (taking a horizontal bar of fluid in equilibrium) the pressure is the same at all points in a horizontal plane. If the pressure were different at two points of a horizontal plane there would be a net force and the fluid would flow.
9.2.2 Variation of pressure with depth
Consider a vertical cylindrical element of fluid of base area A and height h at rest (Fig. 9.3). The forces in the vertical direction are P1A downwards at the top (point 1), P2A upwards at the bottom (point 2) and the weight mg downwards. For equilibrium (P2 − P1)A = mg, and m = ρhA, so
P2 − P1 = ρ g h (9.6)
If point 1 is on the free surface of a liquid open to the atmosphere (P1 = Pa), the pressure at depth h is
P = Pa + ρ g h (9.7)
- The excess P − Pa = ρgh is the gauge pressure at that depth.
- The area of the cylinder does not appear: only the height of the column matters, not its base area or the shape of the container. Pressure is the same at every point at the same horizontal level.
- Equation (9.7) holds if ρ is constant, i.e. for liquids (incompressible), not for gases over large height changes.
This leads to the hydrostatic paradox: vessels A, B, C of quite different shapes joined at the bottom by a horizontal pipe fill to the same level, though they hold different amounts of liquid, because the pressure at the bottom must be equal under each section (Fig. 9.4).
Worked Example 9.2 (NCERT) — swimmer
Q. What is the pressure on a swimmer 10 m below the surface of a lake? (g = 10 m s−2, ρ = 1000 kg m−3.) A. P = Pa + ρgh = 1.01×105 + 1000 × 10 × 10 = 2.01×105 Pa ≈ 2 atm, a 100% increase over the surface value. At a depth of 1 km the increase would be 100 atm, which is why submarines are built to withstand such pressures.
9.2.3 Atmospheric pressure and gauge pressure
The pressure of the atmosphere at a point equals the weight of a column of air of unit cross-section extending from that point to the top of the atmosphere. At sea level it is 1.013×105 Pa (1 atm). Torricelli (1608–1647) devised the mercury barometer: a long glass tube closed at one end and filled with mercury is inverted into a trough of mercury (Fig. 9.5(a)). The space above the column contains only mercury vapour at negligible pressure, so the pressure at A is 0. The pressure at B inside the column equals the pressure at C outside (same level), which is atmospheric:
Pa = ρ g h (9.8)
- The mercury column is about 76 cm (760 mm) at sea level: 1 atm. A fall of 10 mm or more is a sign of an approaching storm.
- 1 mm of Hg = 1 torr = 133 Pa (used in medicine and physiology); the bar and millibar (1 bar = 105 Pa) are used in meteorology.
- The open-tube manometer is a U-tube with a suitable liquid (a low-density liquid like oil for small pressure differences, mercury for large ones); one end is open to the atmosphere and the other joined to the system. The pressure at A equals the pressure at B at the same level in the same liquid; what we usually read is the gauge pressure P − Pa = ρgh, proportional to the manometer height h.
- Tyre-pressure gauges and the blood-pressure meter (sphygmomanometer) read gauge pressure.
Worked Example 9.3 (NCERT) — height of the atmosphere
Q. The density of the atmosphere at sea level is 1.29 kg m−3. Assume it does not change with altitude. How high would the atmosphere extend? A. ρgh = Pa ⇒ h = (1.01×105)/(1.29 × 9.8) = 7989 m ≈ 8 km. In reality the density of air decreases with height (and so does g), so the atmosphere extends with decreasing pressure over 100 km.
Worked Example 9.4 (NCERT) — submarine window
Q. At a depth of 1000 m in an ocean find (a) the absolute pressure, (b) the gauge pressure, (c) the force on a window 20 cm × 20 cm of a submarine whose interior is at sea-level atmospheric pressure. (ρsea = 1.03×103 kg m−3, g = 10 m s−2.)
- Absolute pressure P = Pa + ρgh = 1.01×105 + 1.03×103 × 10 × 1000 = 104.01×105 Pa ≈ 104 atm.
- Gauge pressure = ρgh = 1.03×103 × 10 × 1000 = 103×105 Pa ≈ 103 atm.
- Net pressure on the window = outside (Pa + ρgh) − inside (Pa) = gauge pressure. Area = 0.04 m2, so F = 103×105 × 0.04 = 4.12×105 N.
9.2.4 Hydraulic machines
Take a horizontal cylinder with a piston and three vertical tubes at different points (Fig. 9.6(a)). The liquid rises to the same level in all the tubes, and if the piston is pushed it rises equally in all of them. Hence whenever external pressure is applied to any part of a fluid contained in a vessel, it is transmitted undiminished and equally in all directions — the second form of Pascal’s law, which is the principle of all hydraulic machines.
In a hydraulic lift a small piston of area A1 exerts a force F1 on the liquid. The pressure P = F1/A1 is transmitted undiminished to the larger piston of area A2, which therefore supports a force
F2 = P A2 = F1 (A2/A1) mechanical advantage = A2/A1
The force is multiplied but not the work: since the liquid is incompressible, the volume swept by the small piston equals that swept by the large piston, A1L1 = A2L2, so the large piston moves a smaller distance L2 = L1(A1/A2) and F1L1 = F2L2 (energy is conserved).
Worked Example 9.5 (NCERT) — two syringes
Q. Two syringes of different cross-sections (without needles) filled with water are connected with a tightly fitted rubber tube filled with water. The diameters of the smaller and larger pistons are 1.0 cm and 3.0 cm. (a) Find the force on the larger piston when 10 N is applied to the smaller one. (b) If the smaller piston is pushed in through 6.0 cm, how much does the larger piston move out?
(a) F2 = F1(A2/A1) = 10 × (3/1)2 = 90 N. (b) A1L1 = A2L2 ⇒ L2 = 6.0 × (1/3)2 = 0.67 cm. (Atmospheric pressure acts on both pistons and has been ignored.)
Worked Example 9.6 (NCERT) — car lift
Q. In a car lift compressed air exerts a force F1 on a small piston of radius 5.0 cm. The pressure is transmitted to a second piston of radius 15 cm. If the mass of the car is 1350 kg, calculate F1 and the air pressure needed (g = 9.8 m s−2).
F1 = (A1/A2) mg = (5/15)2 × 1350 × 9.8 = 1470 N ≈ 1.5×103 N. Pressure P = F1/A1 = 1470/(π × (0.05)2) = 1.87×105 Pa ≈ 1.9×105 Pa, almost double the atmospheric pressure.
Hydraulic brakes work on the same principle: the small force on the pedal moves the master piston, the pressure is transmitted through the brake oil to a piston of larger area, and a large force pushes the brake shoes against the lining. Because the pressure is transmitted equally to all four wheel cylinders, the braking effort is equal on all wheels.
Conclusion: Pressure P = F/A is a scalar; it is the same in all directions at a point, the same at all points at the same level, increases with depth as P = Pa + ρgh, and any change applied to an enclosed fluid is transmitted undiminished (Pascal’s law).
9.3 Streamline Flow
So far we studied fluids at rest; the study of fluids in motion is fluid dynamics. When a tap is turned on slowly the water flows smoothly, but the smoothness is lost when the outflow speed is increased. In studying fluid motion we focus on what happens to the fluid particles at a particular point of space at a particular time. The flow is steady if at any given point the velocity of each passing fluid particle remains constant in time. This does not mean that the velocity is the same at different points: a particle may have different velocities at different points, but every particle passing a given point behaves exactly like the previous one.
The path taken by a fluid particle in steady flow is a streamline: a curve whose tangent at any point is in the direction of the fluid velocity at that point (Fig. 9.7(a)). No two streamlines can cross, for if they did an oncoming particle could go either way and the flow would not be steady. The collection of streamlines is a permanent map of the flow.
The equation of continuity
Choose planes P, R and Q perpendicular to the flow whose boundaries are determined by the same set of streamlines (Fig. 9.7(b)). The same number of fluid particles cross each plane. In time Δt the mass crossing area A with speed v is Δm = ρAvΔt, and the mass flowing in equals the mass flowing out:
ρP AP vP = ρR AR vR = ρQ AQ vQ (9.9)
For an incompressible fluid ρ is the same everywhere:
AP vP = AR vR = AQ vQ, i.e. A v = constant (9.10, 9.11)
- This is the equation of continuity: a statement of conservation of mass in the flow of incompressible fluids. Av is the volume flux (volume of fluid per second), the same everywhere along a pipe.
- Where the tube is narrower the streamlines are crowded and the speed is larger; where it is wider the speed is smaller (a fluid accelerates from R to Q in Fig. 9.7(b), and this is associated with a change of pressure in horizontal pipes).
- Steady flow is achieved at low speeds. Beyond a limiting value, the critical speed, the flow loses steadiness and becomes turbulent — for example the foamy whirlpool-like regions called “white water rapids” when a fast stream meets rocks.
- Fig. 9.8(a): laminar flow, in which velocities at different points may differ in magnitude but all are parallel; Fig. 9.8(b): a jet of air striking a flat plate perpendicular to it gives turbulent flow.
9.4 Bernoulli’s Principle
Fluid flow is complex, but for steady (streamline) flow useful results follow from conservation of energy. Consider an incompressible fluid in steady flow in a pipe of varying cross-section and height (Fig. 9.9). By continuity its velocity changes; a force is needed to change the velocity, and it is supplied by the surrounding fluid, so the pressure must differ in different regions. Daniel Bernoulli (Swiss physicist, 1738) obtained the relation between the pressure difference, the change of velocity (kinetic energy) and the change of elevation (potential energy).
Derivation
- In time Δt the fluid at B moves a distance v1Δt to C and the fluid at D moves v2Δt to E. The same volume ΔV = A1v1Δt = A2v2Δt passes through both regions (continuity).
- Work done on the fluid at the left end: W1 = P1A1(v1Δt) = P1ΔV. Work done by the fluid at the right end: W2 = P2ΔV (so −P2ΔV is done on it). Total work on the fluid = (P1 − P2)ΔV.
- The mass passing is Δm = ρΔV. Change of gravitational PE: ΔU = ρgΔV(h2 − h1). Change of KE: ΔK = ½ρΔV(v22 − v12).
- Work-energy theorem: (P1 − P2)ΔV = ½ρΔV(v22 − v12) + ρgΔV(h2 − h1). Divide by ΔV and rearrange.
P1 + ½ρv12 + ρgh1 = P2 + ½ρv22 + ρgh2 (9.12)
P + ½ρv2 + ρgh = constant (9.13)
Statement: as we move along a streamline, the sum of the pressure P, the kinetic energy per unit volume ½ρv2 and the potential energy per unit volume ρgh remains constant.
- Valid for steady, non-viscous, incompressible flow along a streamline. Viscosity (internal friction) converts kinetic energy to heat, so in real flow P2 is lower than Eq. (9.12) predicts. Bernoulli’s equation also does not hold for non-steady or turbulent flow (velocity and pressure fluctuate in time) and neglects the elastic energy of the fluid.
- When the fluid is at rest (v = 0) it reduces to P1 + ρgh1 = P2 + ρgh2, i.e. Eq. (9.6) for pressure variation with depth.
- In a horizontal pipe (h constant) the pressure is lower where the speed is higher.
9.4.1 Speed of efflux: Torricelli’s law
Take a tank with a small hole in its side at height y1 from the bottom; the liquid surface is at height y2 with pressure P above it (Fig. 9.10). By continuity v1A1 = v2A2. If the tank is much wider than the hole (A2 >> A1), v2 ≈ 0. At the hole P1 = Pa. Bernoulli’s equation at the hole and the top, with y2 − y1 = h, gives
v1 = √(2gh + 2(P − Pa)/ρ) (9.14)
If P >> Pa and 2gh may be ignored, the speed is fixed by the container pressure (rocket propulsion). If the tank is open (P = Pa):
v1 = √(2gh) (9.15)
This is Torricelli’s law; it is also the speed of a body falling freely through the height h.
9.4.2 Dynamic lift
Dynamic lift is the force that acts on a body such as an aeroplane wing, a hydrofoil or a spinning ball by virtue of its motion through a fluid. A spinning ball deviates from its parabolic path in cricket, tennis, baseball and golf; this can be partly explained by Bernoulli’s principle.
- (i) Ball without spin (Fig. 9.11(a)): the streamlines are symmetric, the air speed above and below corresponding points is the same, so the pressure difference is zero and there is no upward or downward force.
- (ii) Ball with spin (Fig. 9.11(b)): a spinning ball drags air along with it (more if rough). The ball moves forward, so relative to it the air moves backwards; the air above the ball moves faster relative to the ball and below it slower. The streamlines crowd above and are rarefied below, there is a pressure difference between the lower and upper faces and a net force on the ball. This dynamic lift due to spinning is the Magnus effect.
- (iii) Aerofoil (Fig. 9.11(c)): a solid shaped to give an upward dynamic lift when it moves horizontally through air (the cross-section of an aeroplane wing). The streamlines crowd above the wing more than below, the flow speed on top is higher, the pressure on top is lower and there is a net upward force which balances the weight of the plane.
Worked Example 9.7 (NCERT) — Boeing aircraft
Q. A fully loaded Boeing aircraft has mass 3.3×105 kg and total wing area 500 m2. It is in level flight at 960 km/h. (a) Estimate the pressure difference between the lower and upper surfaces of the wings. (b) Estimate the fractional increase in the speed of the air on the upper surface relative to the lower. (ρair = 1.2 kg m−3.)
(a) The weight is balanced by the lift: ΔP × A = mg ⇒ ΔP = (3.3×105 × 9.8)/500 = 6.5×103 N m−2. (b) Ignoring the small height difference, ΔP = ½ρ(v22 − v12) = ρvav(v2 − v1) with vav = 960 km/h = 267 m s−1, so (v2 − v1)/vav = ΔP/(ρvav2) ≈ 0.08. The speed above the wing needs to be only about 8% higher than that below.
Applications you should know (beyond the text, from the same principle)
- Spray gun, atomiser and carburettor: air blown fast across the top of a tube lowers the pressure there, and the liquid is pushed up the tube by the higher pressure.
- Venturi meter: the pressure drop at a constriction measures the flow speed.
- Roofs may be lifted off in a cyclone: fast wind above lowers the pressure and the higher pressure inside pushes the roof up.
- Two ships sailing close and parallel are drawn together because the fast flow between them lowers the pressure there.
Conclusion: Equation of continuity (Av = constant) is conservation of mass; Bernoulli’s equation (P + ½ρv2 + ρgh = constant) is conservation of energy for ideal fluid flow. Higher speed means lower pressure along a streamline.
9.5 Viscosity
Most fluids are not ideal; they offer some resistance to motion. This resistance to fluid motion is like an internal friction, analogous to friction when a solid slides over a surface, and is called viscosity. It exists when there is relative motion between layers of the fluid. Take oil between two glass plates (Fig. 9.12(a)); the bottom plate is fixed and the top plate moves with a constant velocity v. If the oil is replaced by honey a greater force is needed for the same velocity, so honey is more viscous than oil. The fluid layer in contact with a surface has the same velocity as the surface: the layer touching the top plate moves with v, the layer touching the fixed plate is at rest, and the velocities of the layers increase uniformly from zero (bottom) to v (top). Every layer is pulled forward by the layer above and backward by the layer below, so there is a force between layers. This type of flow is laminar: the layers slide over one another like the pages of a book when a horizontal force is applied to its top cover.
In a pipe the layer along the axis has maximum velocity, which decreases gradually towards the walls where it is zero; the velocity on any cylindrical surface in the tube is constant. A portion of liquid ABCD takes the shape AEFD in a short time Δt, so it has undergone a shear strain Δx/l. Unlike a solid, in a fluid the strain increases continuously with time; the stress is found to depend not on the strain but on the strain rate, i.e. Δx/(lΔt) = v/l. The coefficient of viscosity η (eta) is the ratio of shearing stress to the strain rate:
η = (F/A)/(v/l) = F l/(A v) (9.16)
- SI unit: poiseuille (Pl) = N s m−2 = Pa s. Dimensions [M L−1 T−1]. (CGS unit: poise; 1 Pa s = 10 poise.)
- Thin liquids (water, alcohol) are less viscous than thick liquids (coal tar, blood, glycerine).
- Blood is “thicker” than water; the relative viscosity of blood (η/ηwater) remains constant between 0°C and 37°C.
- Temperature: the viscosity of liquids decreases with temperature, that of gases increases (Points to Ponder 7: liquid atoms become more mobile on heating; in a gas the random motion increases).
| Fluid | T (°C) | Viscosity (mPl = 10−3 Pa s) | Fluid | T (°C) | Viscosity (mPl) |
|---|---|---|---|---|---|
| Water | 20 | 1.0 | Glycerine | 20 | 830 |
| Water | 100 | 0.3 | Honey | — | 200 |
| Blood | 37 | 2.7 | Air | 0 | 0.017 |
| Machine oil | 16 | 113 | Air | 40 | 0.019 |
| Machine oil | 38 | 34 |
Table 9.2 (NCERT): viscosities of some fluids.
Worked Example 9.8 (NCERT) — viscosity of a liquid film
Q. A metal block of area 0.10 m2 is connected to a 0.010 kg mass by a string over an ideal pulley (Fig. 9.13). A liquid film of thickness 0.30 mm is between the block and the table. When released, the block moves to the right with a constant speed 0.085 m s−1. Find the coefficient of viscosity.
The tension equals the weight of the hanging mass (constant speed): F = T = mg = 0.010 × 9.8 = 9.8×10−2 N. Shear stress = F/A = 0.98 N m−2; strain rate = v/l = 0.085/(0.30×10−3) = 283 s−1. So η = 0.98/283 = 3.46×10−3 Pa s.
9.5.1 Stokes’ law
When a body falls through a fluid it drags the layer of fluid in contact with it; relative motion between layers is set up, and the body feels a retarding force. A falling raindrop and a swinging pendulum bob are examples. The viscous force is proportional to the velocity of the object, opposite to its motion, and depends on the viscosity η of the fluid and the radius a of the sphere. Sir George G. Stokes (1819–1903) gave the viscous drag on a sphere:
F = 6 π η a v (9.17) (Stokes’ law; not derived in the text)
Consider a raindrop falling in air. It first accelerates under gravity; as v grows the retarding force grows. Finally, when the viscous force plus the buoyant force equals the force of gravity, the net force and the acceleration are zero and the sphere descends with a constant terminal velocity vt:
6πηa vt = (4π/3) a3 (ρ − σ) g ⇒ vt = 2a2(ρ − σ)g/(9η) (9.18)
Here ρ and σ are the mass densities of the sphere and of the fluid. The terminal velocity depends on the square of the radius (big drops fall faster than small ones) and inversely on the viscosity of the medium (compare Example 6.2).
Worked Example 9.9 (NCERT) — copper ball in oil
Q. The terminal velocity of a copper ball of radius 2.0 mm falling through oil at 20°C is 6.5 cm s−1. Find the viscosity of the oil. (Density of oil 1.5×103, copper 8.9×103 kg m−3.) A. η = 2a2(ρ − σ)g/(9vt) = 2 × (2×10−3)2 × (7.4×103) × 9.8/(9 × 6.5×10−2) = 9.9×10−1 kg m−1 s−1.
9.6 Surface Tension
Oil and water do not mix; water wets you and me but not ducks; mercury does not wet glass but water sticks to it; oil rises up a cotton wick in spite of gravity; sap and water rise to the top of the leaves of a tree; the hair of a paint brush do not cling together when dry or even when dipped in water but form a fine tip when taken out of it. All these are related to the free surfaces of liquids. Liquids have no definite shape but a definite volume, so they acquire a free surface when poured in a container. These surfaces possess some additional energy, a phenomenon known as surface tension. It concerns only liquids, as gases do not have free surfaces.
9.6.1 Surface energy
A liquid stays together because of attraction between its molecules. A molecule well inside the liquid is attracted equally by all the surrounding molecules (Fig. 9.14(a)); this attraction gives it a negative potential energy. The heat of evaporation needed to disperse the molecules far apart is large (for water about 40 kJ/mol), which supports this. A molecule near the surface (Fig. 9.14(b)) has only the lower half of its neighbours, so its negative potential energy is less negative — approximately half of that of an interior molecule. Hence molecules on the surface have extra energy compared with those in the interior. A liquid therefore tends to have the least surface area that the external conditions permit; increasing the surface area requires energy. The energy needed to bring a molecule to the surface is roughly half the energy required to remove it entirely from the liquid, i.e. half the heat of evaporation.
9.6.2 Surface energy and surface tension
Creating more surface (spreading) at fixed volume requires work. Consider a horizontal liquid film ending in a bar free to slide on parallel guides (Fig. 9.15). Move the bar by a small distance d against the internal force F; the work Fd is stored as additional surface energy. If S is the surface energy per unit area, the extra area is 2dl (the film has two sides, two surfaces) and
S(2dl) = F d ⇒ S = F/2l (9.19, 9.20)
- Surface tension S = surface energy per unit area = force per unit length exerted by the liquid on the movable bar. Unit N m−1 (equal to J m−2); dimensions [M T−2].
- S is a force per unit length (or energy per unit area) acting in the plane of the interface between the liquid and any other substance; it is the extra energy of the interface molecules compared with those in the interior. It depends on the materials on both sides of the interface (like or unlike molecules), so it is not the property of a single fluid alone.
- At any point of the interface, equal and opposite surface-tension forces S per unit length act perpendicular to an imagined line drawn on it, in the plane of the interface.
- The surface tension of a liquid usually falls with temperature.
| Liquid | Temp (°C) | Surface tension (N m−1) | Heat of vaporisation (kJ/mol) |
|---|---|---|---|
| Helium | −270 | 0.000239 | 0.115 |
| Oxygen | −183 | 0.0132 | 7.1 |
| Ethanol | 20 | 0.0227 | 40.6 |
| Water | 20 | 0.0727 | 44.16 |
| Mercury | 20 | 0.4355 | 63.2 |
Table 9.3 (NCERT): surface tension of some liquids with heats of vaporisation.
Measuring S. A flat vertical glass plate hangs from one arm of a balance with its horizontal edge just above the liquid (Fig. 9.16). The vessel is raised till the liquid just touches the plate, which is pulled down by surface tension. Weights are added till the plate just clears the liquid. If the extra weight is W = mg and the plate edge has length l:
Sla = W/2l = mg/2l (9.21)
9.6.3 Angle of contact
The surface of a liquid near the line of contact with another medium is generally curved. The angle of contact θ is the angle between the tangent to the liquid surface at the point of contact and the solid surface, measured inside the liquid. It depends on the pair of materials and decides whether a liquid spreads on a solid or forms droplets (Fig. 9.17: water forms droplets on a lotus leaf but spreads on a clean plastic plate). Three interfacial tensions act at the contact line: liquid-air Sla, solid-air Ssa and solid-liquid Ssl. In equilibrium
Sla cosθ + Ssl = Ssa (9.22)
- Obtuse θ if Ssl > Sla (as in water on a lotus leaf, water on a waxy or oily surface, mercury on glass): liquid molecules are strongly attracted to one another and weakly to the solid, it costs a lot of energy to create a liquid-solid interface, and the liquid does not wet the solid.
- Acute θ if Ssl < Sla (water on glass or plastic, kerosene on virtually anything): the molecules of the liquid are strongly attracted to those of the solid, Ssl is reduced, cosθ increases, the liquid wets the solid and spreads.
- Soaps, detergents and dyeing substances are wetting agents: they make the angle of contact small so that the liquid penetrates well. Water-proofing agents create a large angle of contact between water and fibres.
9.6.4 Drops and bubbles
Free liquid drops and bubbles are spherical if gravity can be neglected, because for a given volume a sphere has the least surface area and hence the least surface energy (a sphere is better than a cube in this respect). The pressure inside a spherical drop is more than outside. If the radius of a drop in equilibrium increases by Δr, the extra surface energy is [4π(r + Δr)2 − 4πr2]Sla = 8πrSlaΔr, balanced by the work (Pi − Po)4πr2Δr, so
Pi − Po = 2Sla/r (drop or cavity); Pi − Po = 4Sla/r (bubble, 2 surfaces) (9.25, 9.26)
In general, for a liquid-gas interface the concave side has the higher pressure than the convex side; an air bubble inside a liquid has higher pressure inside. A soap bubble has two interfaces, hence 4S/r. That is why one has to blow hard, but not too hard, to form a soap bubble: a little extra air pressure is needed inside.
9.6.5 Capillary rise
The pressure difference across a curved liquid-air interface explains why water rises in a narrow tube in spite of gravity (capilla = hair in Latin; the thinner the tube, the larger the rise). Consider a vertical capillary tube of circular cross-section (radius a) dipped in an open vessel of water (Fig. 9.19). The contact angle between water and glass is acute, the meniscus is concave, and the radius of curvature is r = a/cosθ = a secθ. The pressure just below the meniscus is less than atmospheric by
Pi − P0 = 2S/r = (2S/a) cosθ (9.27)
Take a point B inside the tube at the level of the water surface in the vessel, and a point A just below the meniscus. The pressure at B equals the atmospheric pressure P0 (same level as the free surface outside, in the same liquid). The pressure at A is lower than that at B by the weight of the column of height h: PA = P0 − hρg. But A lies just below the concave meniscus, where the pressure is lower than the atmospheric pressure above it by 2S cosθ/a (Eq. 9.27), so PA = P0 − (2S cosθ)/a. Equating the two expressions for PA and cancelling P0:
hρg = 2S cosθ / a ⇒ h = 2S cosθ / (ρ g a) (9.29)
- The capillary rise is due to surface tension and is larger for a smaller radius a; typically a few cm for fine capillaries. For water in a tube of a = 0.05 cm: h = 2 × 0.073/(103 × 9.8 × 5×10−4) = 2.98×10−2 m = 2.98 cm.
- If the meniscus is convex (as for mercury), cosθ is negative and the liquid is depressed in the capillary: it stands lower than the outside level.
Worked Example 9.10 (NCERT) — blowing a bubble under water
Q. The lower end of a capillary tube of diameter 2.00 mm is dipped 8.00 cm below the surface of water. What pressure is required in the tube to blow a hemispherical bubble at its end? Also calculate the excess pressure. (S = 7.30×10−2 N m−1, Pa = 1.01×105 Pa, ρ = 1000 kg m−3, g = 9.80 m s−2.)
There is only one liquid surface, so excess pressure = 2S/r with r = 1.00 mm (hemispherical bubble: radius = tube radius). Pressure outside the bubble Po = Pa + ρgh = 1.01×105 + 0.08 × 1000 × 9.80 = 1.01784×105 Pa. Excess = 2 × 7.3×10−2/10−3 = 146 Pa. Pressure inside Pi = 1.01784×105 + 146 = 1.02×105 Pa; excess pressure = 146 Pa. (For a bubble of liquid in a gas there are two surfaces and the formula is 4S/r.)
Conclusion: Surface tension S = F/l = W/A (surface energy per unit area) arises from the extra energy of surface molecules; it makes drops spherical, produces excess pressure 2S/r inside a drop, 4S/r inside a soap bubble and makes liquids rise in capillaries by h = 2S cosθ/(ρga).
Formula Sheet — Mechanical Properties of Fluids
| Topic | Formula | Remark / unit |
|---|---|---|
| Pressure | P = F/A | Pa = N m−2; scalar; 1 atm = 1.013×105 Pa |
| Density, relative density | ρ = m/V; RD = ρ/ρwater | kg m−3; RD has no unit |
| Variation with depth | P2 − P1 = ρgh; P = Pa + ρgh | gauge pressure = ρgh |
| Barometer | Pa = ρHg g h | 76 cm of Hg = 1 atm; 1 torr = 133 Pa |
| Hydraulic lift | F1/A1 = F2/A2; A1L1 = A2L2 | force multiplied, work conserved |
| Continuity | A1v1 = A2v2 | mass conservation (incompressible) |
| Bernoulli | P + ½ρv2 + ρgh = constant | ideal fluid, steady flow |
| Torricelli | v = √(2gh) | speed of efflux from open tank |
| Lift on wing | ΔP = ½ρ(v22 − v12) | Magnus effect for a spinning ball |
| Viscosity | η = F l/(A v) | Pa s; [M L−1 T−1] |
| Stokes’ law | F = 6πηav | viscous drag on a sphere |
| Terminal velocity | vt = 2a2(ρ − σ)g/(9η) | ∝ a2; ∝ 1/η |
| Surface tension | S = F/2l = W/2l (film); S = energy/area | N m−1 = J m−2 |
| Contact angle | Sla cosθ + Ssl = Ssa | acute: wets; obtuse: does not wet |
| Excess pressure | 2S/r (drop, cavity); 4S/r (soap bubble) | inside is higher |
| Capillary rise | h = 2S cosθ/(ρga) | ∝ 1/a |
Summary (NCERT, in short)
- The basic property of a fluid is that it can flow; its shape is governed by the shape of its container. A liquid is incompressible and has a free surface; a gas is compressible and expands to occupy all the space.
- Average pressure Pav = F/A (normal force per unit area); units: 1 atm = 1.01×105 Pa, 1 bar = 105 Pa, 1 torr = 133 Pa = 1 mm of Hg.
- Pascal’s law: pressure in a fluid at rest is the same at all points at the same height; a change in pressure applied to an enclosed fluid is transmitted undiminished to every point of the fluid and to the walls of the vessel.
- P = Pa + ρgh for a fluid of uniform density.
- Steady flow of an incompressible fluid: vA = constant (conservation of mass).
- Bernoulli’s principle: P + ρv2/2 + ρgy = constant along a streamline (conservation of energy for non-viscous fluid motion); viscosity converts kinetic energy into heat.
- The coefficient of viscosity is the ratio of the shear stress to the time rate of shearing strain.
- Stokes’ law: F = 6πηav. Surface tension is a force per unit length (or surface energy per unit area) acting in the plane of the interface between the liquid and the bounding surface.
Points to Ponder (NCERT) in simple words
- Pressure is a scalar; the “force” in F/A is the normal component only. Pressure exists at all points of a fluid, not only on the walls of a container.
- P = Pa + ρgh holds for incompressible fluids (practically, liquids), where ρ is constant with height.
- Gauge pressure P − Pa is what tyre gauges and the sphygmomanometer measure.
- In steady flow two streamlines never intersect (otherwise a particle would have two possible velocities at that point).
- Bernoulli’s principle does not hold in the presence of viscous drag: the work done by this dissipative force must be included and P2 will be lower than predicted by Eq. (9.12).
- As temperature rises the viscosity of a liquid falls, but that of a gas rises.
- Surface tension arises from the excess potential energy of molecules at the surface; it is present at the interface separating two substances at least one of which is a fluid.
Common Mistakes to Avoid
- Using absolute pressure instead of gauge pressure to find the net force on a window or dam (the atmosphere also pushes on the other side).
- Forgetting the factor 2 in S = F/2l (a film has two surfaces) and the factor 4S/r for a soap bubble (two surfaces) but 2S/r for an air bubble in a liquid.
- Using the pipe diameter in A v = constant without converting to area (A ∝ d2); using cm2 and m2 mixed.
- Using Bernoulli across a turbulent region or where viscosity is large (river rapid, narrow needle).
- Writing the unit of viscosity as N m−2 (it is N s m−2 = Pa s) and of surface tension as N m−2 (it is N m−1).
Conclusion: Fluid statics rests on Pascal’s law and P = Pa + ρgh; fluid dynamics on continuity (mass) and Bernoulli (energy); real fluids add viscosity (Stokes, terminal velocity) and surface tension (drops, bubbles, capillary rise).
Ex 9.1 — Blood pressure, atmospheric pressure and the scalar nature of pressure
Concept. Pressure in a fluid at rest increases with depth, P2 − P1 = ρgh (Pascal’s law and Eq. 9.6). Pressure is defined as normal force per unit area, so it has magnitude only.
Question. Explain why (a) the blood pressure in humans is greater at the feet than at the brain; (b) atmospheric pressure at a height of about 6 km decreases to nearly half of its value at sea level, though the height of the atmosphere is more than 100 km; (c) hydrostatic pressure is a scalar quantity even though pressure is force divided by area.
(a) Blood pressure at the feet and at the brain
The blood in the arteries and veins is a continuous liquid column. In a standing person the feet are about 1.7 m below the brain, so the vertical column of blood above the feet is longer. The hydrostatic pressure difference is Pfeet − Pbrain = ρgh, where ρ is the density of blood (1.06×103 kg m−3, Table 9.1) and h the height difference. With h ≈ 1.7 m this is about 1.06×103 × 9.8 × 1.7 ≈ 1.8×104 Pa (about 130 mm of Hg), added to the pressure produced by the heart. Hence the pressure at the feet is greater than at the brain. This is also why a person may feel faint on standing up suddenly.
(b) Atmospheric pressure halves at 6 km
The formula P = Pa + ρgh is valid only for an incompressible fluid of constant density, i.e. for liquids. Air is a gas, highly compressible: the lower layers are compressed by the weight of the air above, so the density of air is greatest at sea level and decreases with height (and g also decreases slightly). Atmospheric pressure at a height equals the weight of the air column above it; since the air is densest near the ground, about half of the mass of the atmosphere lies within the lowest 5–6 km. The pressure at 6 km is therefore nearly half the sea-level value, and the remaining half is spread over the enormous height of more than 100 km where the air is extremely thin. If the density were constant (as Example 9.3 assumes) the atmosphere would end at 8 km.
(c) Why hydrostatic pressure is a scalar
In the definition P = F/A the force that appears is only the component of force normal to the area, and the direction of this force is fixed by the orientation of the area, not by the pressure. At a given point in a fluid at rest the pressure is the same in all directions (Pascal’s law, Fig. 9.2): rotating the area at that point changes the direction of the force but not the pressure. Since no single direction can be assigned to it, pressure has magnitude only and so is a scalar, like other types of stress. It adds as ordinary numbers (P = Pa + ρgh).
Extra depth. A numerical check for (b): treat the atmosphere as isothermal with T = 288 K. Then P = P0 exp(−Mgh/RT) with scale height H = RT/(Mg) = (8.31 × 288)/(0.029 × 9.8) ≈ 8.4 km, so at h = 6 km P/P0 = e^(−6/8.4) ≈ 0.49. This is the beyond-the-book model, but it reproduces the NCERT statement that the pressure halves at about 6 km.
Conclusion: (a) the blood column is longer above the feet (ΔP = ρgh); (b) air is compressible so its density falls with height; (c) pressure is the normal force per unit area, equal in all directions, hence a scalar.
Ex 9.2 — Angle of contact, wetting, surface tension and spherical drops
Concept. Cohesion (attraction between like molecules) and adhesion (attraction between unlike molecules) decide the shape of a liquid surface at a solid wall: if adhesion is larger, the liquid wets the solid (acute angle); if cohesion is larger, it does not (obtuse angle).
Question. Explain why (a) the angle of contact of mercury with glass is obtuse, while that of water with glass is acute; (b) water on a clean glass surface tends to spread out while mercury on the same surface tends to form drops; (c) surface tension of a liquid is independent of the area of the surface; (d) water with detergent dissolved in it should have small angles of contact; (e) a drop of liquid under no external forces is always spherical in shape.
(a) Obtuse for mercury, acute for water
The angle of contact is determined by the balance Sla cosθ + Ssl = Ssa (Eq. 9.22). For mercury on glass the mercury molecules attract one another (cohesion) much more strongly than they are attracted by glass molecules (adhesion), so Ssl is large (Ssl > Sla), cosθ is negative and θ is obtuse (the meniscus is convex). For water on glass the attraction between water and glass molecules is greater than that between water molecules, Ssl is small (Ssl < Sla), cosθ is positive and θ is acute (concave meniscus).
(b) Water spreads on glass, mercury forms drops
Because of the acute angle, the water film on clean glass lowers the total surface energy by spreading: water wets glass. Because of the obtuse angle, mercury molecules prefer to stay together; it costs a lot of energy to create a mercury-glass interface, so mercury pulls itself into drops (minimum surface area) and does not wet glass.
(c) Surface tension is independent of the area
Surface tension is the force per unit length (equivalently the surface energy per unit area) in the plane of the interface. It depends on the nature of the liquid and the medium in contact and on temperature, but not on how large the surface is. When the area of a film is increased, molecules from the interior come to the surface until the surface has the same energy per unit area as before; the force per unit length on the bar remains F/2l, whatever the area. (This differs from a stretched rubber sheet where the force increases with stretching.)
(d) Detergent solution has small angle of contact
Detergents are wetting agents: they reduce the liquid-solid and liquid-air interfacial energies, so cosθ increases and θ becomes small. A small angle of contact means the solution spreads and penetrates the fibres of a cloth and carries the dirt away. (Water-proofing agents do the opposite: they produce a large angle of contact.)
(e) A free drop is spherical
A liquid-air interface has surface energy proportional to its area, and a system under no external forces takes the configuration of least energy. For a given volume, the surface with the least area is a sphere. Therefore a drop under no external forces (gravity, air resistance negligible) is spherical, as seen in tiny drops in a spray or the weightless water in a spacecraft.
Extra depth. For exact language: a drop of mercury on glass has cosθ = (Ssa − Ssl)/Sla negative ⇒ obtuse. Values: water-glass θ ≈ 0°–8°, mercury-glass θ ≈ 140°. A large drop is flattened by gravity, which is why only small drops are really spherical.
Conclusion: (a, b) cohesion vs adhesion decides the angle (acute for water, obtuse for mercury); (c) S is force per unit length; (d) detergents make θ small; (e) a sphere has the least surface area for a given volume.
Ex 9.3 — Fill in the blanks with the right word
Concept. Use the facts: S falls with temperature; viscosity of liquids falls and that of gases rises with temperature; fluids resist the rate of shear strain; continuity is conservation of mass; critical speed ∝ 1/(size) through the Reynolds number.
Question. Fill in the blanks using the word(s) from the list appended with each statement.
| Statement | Answer | Reason |
|---|---|---|
| (a) Surface tension of liquids generally … with temperature (increases / decreases) | decreases | molecules gain kinetic energy, cohesion weakens; S → 0 at the critical temperature |
| (b) Viscosity of gases … with temperature, whereas viscosity of liquids … with temperature (increases / decreases) | increases; decreases | gas: random motion and momentum transfer between layers increase; liquid: molecules become more mobile, cohesive forces weaken |
| (c) For solids with elastic modulus of rigidity, the shearing force is proportional to …, while for fluids it is proportional to … (shear strain / rate of shear strain) | shear strain; rate of shear strain | solid: F/A = Gθ; fluid: F/A = η(v/l) (Eq. 9.16) |
| (d) For a fluid in a steady flow, the increase in flow speed at a constriction follows … (conservation of mass / Bernoulli’s principle) | conservation of mass | continuity equation Av = constant; Bernoulli then gives the pressure drop that accompanies the higher speed |
| (e) For the model of a plane in a wind tunnel, turbulence occurs at a … speed for turbulence for an actual plane (greater / smaller) | greater | the critical speed vc = Rcη/(ρD) ∝ 1/D, the smaller model has a larger critical speed |
Explanations. (a) Surface tension is the extra energy of molecules at the surface; heating weakens the attraction between molecules, so S decreases (it is 0.0727 N m−1 for water at 20°C and smaller at 100°C). (b) The viscosity of a liquid falls on heating (honey flows faster when warm) but that of a gas rises (Points to Ponder 7). (c) In a solid the shear strain is determined by the force and G; in a fluid the strain keeps increasing with time under a constant stress, so the stress is related to the rate of change of strain. (d) The speed rises at a narrow part because the same volume per second must pass (A1v1 = A2v2); this is a mass-conservation statement. (e) Turbulence begins when the Reynolds number R = ρvD/η exceeds a critical value (the same for model and aeroplane for similar flows); the model has a much smaller size D, so a larger speed is needed to reach the critical Reynolds number.
Extra depth. In (e) the Reynolds number is the dimensionless combination ρvD/η that decides whether flow is laminar or turbulent: R < about 1000 laminar, R > about 2000 turbulent (for flow in a pipe). Since it contains the size D, flow around a small model at moderate speed corresponds to the flow around a big aeroplane only at a much larger speed — that is why wind tunnels use high speeds or pressurised air.
Conclusion: (a) decreases; (b) increases, decreases; (c) shear strain, rate of shear strain; (d) conservation of mass; (e) greater.
Ex 9.4 — Everyday applications of Bernoulli’s principle, continuity and Newton’s law
Concept. Link each situation to its law: pressure and speed (Bernoulli), flow rate and area (continuity), flow through a narrow tube (viscosity), momentum conservation (thrust), and spin (Magnus effect).
Question. Explain why (a) to keep a piece of paper horizontal you should blow over, not under, it; (b) when we try to close a water tap with our fingers, fast jets of water gush through the openings between our fingers; (c) the size of the needle of a syringe controls flow rate better than the thumb pressure exerted by a doctor while administering an injection; (d) a fluid flowing out of a small hole in a vessel results in a backward thrust on the vessel; (e) a spinning cricket ball in air does not follow a parabolic trajectory.
(a) Blow over, not under, the paper
When you blow over the paper the air above moves fast, so by Bernoulli’s principle (P + ½ρv2 = constant) the pressure above falls below the atmospheric pressure below the paper. The greater pressure beneath pushes the paper up and keeps it horizontal. If you blow under it, the pressure below falls and the larger atmospheric pressure above pushes the paper down.
(b) Jets of water between the fingers
Water leaves the tap at a fixed volume flow rate Q = Av. When we close the opening partly with fingers, the area A of the openings becomes much smaller. By the equation of continuity (Av = constant) the speed v through the small gaps increases greatly, so fast narrow jets gush out.
(c) Needle size controls the flow rate
The flow of a viscous liquid through a narrow tube of radius r and length L under pressure difference ΔP is given by Poiseuille’s formula Q = πr4ΔP/(8ηL) (a result of viscous flow; not derived in the text). The flow rate depends on the fourth power of the radius of the needle but only linearly on the pressure. A change of needle radius by a factor of two changes Q by 16 times, whereas the doctor’s thumb can change the pressure by only a small factor. Hence the size of the needle controls the flow rate far better than the thumb pressure.
(d) Backward thrust on the vessel
As the fluid leaves the hole with speed v it carries away momentum in the forward direction. By conservation of momentum (Newton’s third law, as in a rocket) the vessel gets an equal momentum in the opposite direction, i.e. a backward thrust F = (dm/dt)v = ρav2. For an open tank v = √(2gh) so F = 2ρgha (a = area of the hole). Also, the pressure of the liquid acts on the walls except on the area of the hole, leaving a net unbalanced force on the opposite wall.
(e) A spinning cricket ball does not follow a parabola
A spinning ball drags air along with it. Relative to the ball, the air on one side moves faster and on the other side slower, so the pressure on the two sides differs (Bernoulli) and there is a net sideways or upward force, the Magnus effect (dynamic lift). This extra force, beyond gravity, makes the path deviate from a parabola; it is the basis of swing and spin bowling.
Extra depth. The thrust in (d) is the principle of jet propulsion, garden sprinklers and rockets; for a hole of area 1 cm2 at 1 m depth of water the thrust is 2 × 103 × 9.8 × 1 × 10−4 = 1.96 N. In (c), blood-vessel or tube blockage also changes r4: a 20% reduction in the radius of an artery cuts the flow to about 40% unless the pressure rises.
Conclusion: (a) lower pressure above; (b) smaller area, larger speed (continuity); (c) flow ∝ r4 so the needle size controls it; (d) momentum of the jet gives a backward thrust; (e) Magnus effect.
Ex 9.5 — Pressure exerted by a high-heel shoe
Concept. Pressure = force/area. The force is the weight of the girl, mg, and the area is the circular heel, πr2 = πd2/4.
Question. A 50 kg girl wearing high-heel shoes balances on a single heel. The heel is circular with a diameter 1.0 cm. What is the pressure exerted by the heel on the horizontal floor?
Given
- Mass m = 50 kg, g = 9.8 m s−2 ⇒ F = mg = 490 N (acting normal to the floor)
- Diameter d = 1.0 cm = 1.0×10−2 m ⇒ r = 0.50 cm = 5.0×10−3 m
- Area A = πr2 = 3.14 × (5.0×10−3)2 = 7.85×10−5 m2
Solution
P = F/A = 490/(7.85×10−5) = 6.2×106 Pa
The pressure exerted by the heel is about 6.2×106 Pa, i.e. about 62 atmospheres (6.2×106/1.013×105 = 61.6 atm). This is why a stiletto heel can dent a wooden floor, while the same girl standing flat on both feet of area, say, 150 cm2 each would exert only 490/(300×10−4) ≈ 1.6×104 Pa, about 380 times smaller.
Extra depth. This is the pressure idea of Section 9.2: the same force over a smaller area gives a larger pressure (needle, knife, high heel), which is why a blunt object does not pierce the skin but a needle does, and why a wooden plank spreads the force on the performer’s chest. In real life the whole weight is not carried by one heel at once, so the pressure is smaller, but the question assumes balancing on a single heel.
More to know. Compare other everyday pressures: a sharp knife edge or needle tip (area of the order 10−9 m2) can produce pressures of 109 Pa for an ordinary hand force; the atmosphere itself presses on the human body (area about 1.5 m2) with a total force of 1.5 × 105 N — about 15 tonnes — without hurting us because the internal pressure of the body fluids is equal and the pressure is transmitted equally in all directions (Pascal’s law). Snow-shoes, skis, caterpillar tracks of tanks and wide tyres of tractors all increase the area to reduce the pressure.
Conclusion: P = mg/(πd2/4) = 6.2×106 Pa, about 60 times atmospheric pressure, because the contact area is very small.
Ex 9.6 — Height of a wine barometer
Concept. A liquid barometer balances atmospheric pressure by a column of liquid: Pa = ρgh. Hence h = Pa/(ρg), and the height is inversely proportional to the density.
Question. Torricelli’s barometer used mercury. Pascal duplicated it using French wine of density 984 kg m−3. Determine the height of the wine column for normal atmospheric pressure.
Given
- Normal atmospheric pressure Pa = 1.013×105 Pa
- Density of wine ρ = 984 kg m−3, g = 9.8 m s−2
Solution
h = Pa/(ρg) = (1.013×105)/(984 × 9.8) = 1.013×105/9643 = 10.5 m
So the wine column would be about 10.5 m high. For comparison, mercury (ρ = 13.6×103 kg m−3) gives h = 1.013×105/(13.6×103 × 9.8) = 0.76 m = 76 cm. Since h ∝ 1/ρ, the ratio is hwine/hHg = 13.6×103/984 = 13.8, and 0.76 × 13.8 ≈ 10.5 m: a good cross-check.
Extra depth. The barometer height depends on the density of the liquid but not on the cross-section or the shape of the tube (Eq. 9.7: only the height of the column matters). Water would need a tube about 10.3 m long (h = 1.013×105/(103 × 9.8)), which is why water barometers are impractical and why a suction pump cannot lift water by more than about 10 m. Mercury is used because it is dense (short tube) and has a negligible vapour pressure at room temperature; wine, being a solution of alcohol and water, has a larger vapour pressure that would depress the column slightly.
More to know. Torricelli (1608–1647) invented the mercury barometer in 1643, and Blaise Pascal repeated it with water and with red wine to show that the height of the column is inversely proportional to the density of the liquid; the experiment also made people accept that the atmosphere has weight. Pascal later sent his brother-in-law up the Puy de Dôme mountain with a barometer and found that the mercury column was shorter at the top, proving that atmospheric pressure decreases with height (the key idea of Ex 9.1(b)). Units to remember: 760 mm of Hg = 1 atm = 1.013×105 Pa = 10.3 m of water.
Quick table. Column height for Pa = 1.013×105 Pa (g = 9.8 m s−2): mercury (13.6×103) 0.760 m; sea water (1.03×103) 10.0 m; fresh water (1.00×103) 10.3 m; wine (984) 10.5 m; ethyl alcohol (0.806×103) 12.8 m. The less dense the liquid the taller the barometer.
Conclusion: h = Pa/(ρg) = 10.5 m for wine (density 984 kg m−3), compared with 0.76 m for mercury.
Ex 9.7 — Can an off-shore structure withstand the pressure at 3 km depth?
Concept. The structure at the bottom is compressed by the hydrostatic pressure P = ρgh (plus Pa if absolute). Compare this stress with the maximum stress the structure can withstand, 109 Pa.
Question. A vertical off-shore structure is built to withstand a maximum stress of 109 Pa. Is the structure suitable for putting up on top of an oil well in the ocean? Take the depth of the ocean to be roughly 3 km, and ignore ocean currents.
Given
- Depth h = 3 km = 3000 m, ρ = 103 kg m−3 (water), g = 9.8 m s−2
- Maximum stress the structure can withstand = 109 Pa
Solution
P = ρgh = 103 × 9.8 × 3000 = 2.94×107 Pa
If the atmospheric pressure at the surface (1.01×105 Pa) is added, the absolute pressure at the sea bed is 2.95×107 Pa; the difference is negligible. The compressive stress on the structure at the bottom is therefore about 2.9×107 Pa, which is less than the design limit of 109 Pa by a factor of about 34.
Conclusion: the structure is suitable. The greatest stress it will meet is the hydrostatic pressure at the sea bed, 2.9×107 Pa, much below the 109 Pa which it can withstand (ocean currents being ignored, as the question allows).
Extra depth. The pressure depends only on the depth and not on the shape of the structure (Fig. 9.4, hydrostatic paradox). In practice such structures must also be designed against the pressure of the oil in the well and against waves and currents, and the safety factor of 34 gives a big margin. Using g = 10 m s−2 and ρ = 1.03×103 kg m−3 for sea water would give 3.09×107 Pa; the conclusion is unchanged.
More to know. At the sea bed, 3 km deep, the pressure is about 290 times atmospheric pressure (2.94×107/1.013×105 = 290 atm). A force of this order acts on every square metre: 2.94×107 N, about 3000 tonnes wt. Submarines and deep-sea probes are therefore built as spherical or cylindrical pressure hulls so that the compressive stress is spread uniformly. In the problem, the structure is “vertical”, so the sideways pressure acts on its walls and the vertical hydrostatic force on its base; both are of order ρgh. The stress on its walls is the gauge pressure outside minus whatever pressure is maintained inside, so a hollow structure filled with air at 1 atm would face the full 2.9×107 Pa difference.
Conclusion: The maximum pressure at 3 km is ρgh = 2.94×107 Pa, far below 109 Pa, so the structure is suitable.
Ex 9.8 — Maximum pressure on the smaller piston of a hydraulic lift
Concept. By Pascal’s law the pressure in the liquid is the same everywhere in the lift, so the pressure on the small piston equals the pressure on the large piston, P = F2/A2.
Question. A hydraulic automobile lift is designed to lift cars with a maximum mass of 3000 kg. The area of cross-section of the piston carrying the load is 425 cm2. What maximum pressure would the smaller piston have to bear?
Given
- Maximum mass m = 3000 kg ⇒ load F2 = mg = 3000 × 9.8 = 2.94×104 N
- Area of the load piston A2 = 425 cm2 = 425×10−4 m2 = 4.25×10−2 m2
Solution
P = F2/A2 = (2.94×104)/(4.25×10−2) = 6.92×105 Pa
The pressure is transmitted undiminished through the liquid, so the smaller piston also has to bear a pressure of 6.92×105 Pa (about 6.8 atm), regardless of its own area. The area of the smaller piston decides only the force F1 needed: F1 = P A1, so a smaller A1 needs a smaller force.
Extra depth. This answer does not need the area of the small piston; the pressure in the lift is the same. If, for example, A1 were 10 cm2 the force needed would be 6.92×105 × 10−3 = 692 N (about 71 kg wt) to lift 3000 kg: a mechanical advantage of 425/10 = 42.5. Remember that the small piston must move 42.5 times farther than the load piston since A1L1 = A2L2.
More to know. A hydraulic lift is an application of the second form of Pascal’s law (pressure applied to an enclosed fluid is transmitted undiminished). It multiplies force, not energy or work. The designer chooses the area ratio A2/A1 so that an easily applied force F1 balances the heavy load; typical car lifts in garages use compressed air of a few atmospheres (6.9 atm here). Safety valves limit the pressure. Hydraulic brakes, dentist’s chairs, hydraulic jacks, excavators and aircraft control surfaces are other examples of the same principle.
Check in atmospheres. 6.92×105 Pa / 1.013×105 Pa = 6.8 atm gauge, or about 7.8 atm absolute if the atmospheric pressure is included. The question asks for the pressure that the smaller piston has to bear, which is the pressure in the liquid; if the pressure is expressed as gauge pressure then the figure above is the answer, and if in absolute terms add 1.01×105 Pa.
Conclusion: P = F2/A2 = 6.92×105 Pa on both pistons (Pascal’s law).
Ex 9.9 — Specific gravity of methylated spirit in a U-tube
Concept. At the same level in the same liquid (mercury) the pressure is equal in both arms. Hence the pressure from the water column equals the pressure from the spirit column: hwρwg = hsρsg.
Question. A U-tube contains water and methylated spirit separated by mercury. The mercury columns in the two arms are in level with 10.0 cm of water in one arm and 12.5 cm of spirit in the other. What is the specific gravity of spirit?
Solution
The mercury surfaces in the two arms are at the same level, so the pressure just above the mercury surface is the same on both sides (pressure is the same at the same level in the same liquid at rest):
Pa + hwρwg = Pa + hsρsg ⇒ ρs/ρw = hw/hs
Specific gravity of spirit = 10.0/12.5 = 0.80
Specific gravity (relative density) is the ratio of the density to that of water, so it has no unit. The density of the spirit is 0.80 × 103 = 800 kg m−3. A less dense liquid needs a taller column to give the same pressure, which is why the spirit column (12.5 cm) is taller than the water column (10.0 cm).
Extra depth. The atmospheric pressure acts on the top of both columns and cancels, and the mercury does not enter the calculation because its surfaces are at the same level; mercury only separates the two liquids. If the mercury levels were unequal (as in Ex 9.10), the difference in height times the density of mercury would also appear in the balance.
Conclusion: hwρw = hsρs gives the specific gravity of the spirit as 10.0/12.5 = 0.80.
Ex 9.10 — Difference in mercury levels after pouring more liquid
Concept. Equate the pressures at the lower mercury surface (the surface at the lower level on one side). The column on the other side is the other liquid plus an extra mercury column of height h.
Question. In the previous problem, if 15.0 cm of water and spirit each are further poured into the respective arms of the tube, what is the difference in the levels of mercury in the two arms? (Specific gravity of mercury = 13.6.)
Given
- Water column now 10.0 + 15.0 = 25.0 cm; spirit column 12.5 + 15.0 = 27.5 cm
- Specific gravity of spirit = 0.80 (from Ex 9.9), of mercury = 13.6, of water = 1
- Let the mercury level in the spirit arm be higher than in the water arm by h cm.
Solution
Pressure of the water column (25.0 cm) at the level of the lower mercury surface (the water side). The same level on the other side lies inside the mercury of the spirit arm, below its surface by h. The pressure there is the spirit column plus the extra mercury column of height h. Equating (and cancelling g and Pa):
25.0 × 1 = 27.5 × 0.80 + h × 13.6 ⇒ 25.0 = 22.0 + 13.6 h
h = 3.0/13.6 = 0.22 cm
The mercury is about 0.22 cm (2.2 mm) higher in the spirit arm than in the water arm. The difference is small because mercury is so dense: a pressure difference equivalent to 3.0 cm of water (294 Pa) needs only 0.22 cm of mercury.
Extra depth. The difference arises because the new columns are no longer in the ratio 1 : 0.8 × 1 to the original: the water column pressure, 25.0 gρw (in cm of water), is greater than the spirit column pressure, 27.5 × 0.8 = 22.0, by 3.0 cm of water. This difference pushes the mercury down in the water arm and up in the spirit arm until the extra mercury column of height h = 3.0/13.6 balances it (a U-tube manometer working in reverse).
Conclusion: Equating pressures: 25.0 = 27.5 × 0.80 + 13.6 h, so h = 0.22 cm, mercury higher in the spirit arm.
Ex 9.11 — Can Bernoulli’s equation describe water flowing through a river rapid?
Concept. Bernoulli’s equation P + ½ρv2 + ρgh = constant is derived for steady, streamline (laminar), non-viscous, incompressible flow. It can be applied only where these conditions hold.
Question. Can Bernoulli’s equation be used to describe the flow of water through a rapid in a river? Explain.
Answer: No
The flow of water through a rapid is turbulent and not steady. The water meets rocks and a steep, uneven bed; it forms eddies and whirlpools (white water), and at any point the velocity and the pressure change rapidly with time in magnitude and in direction. Bernoulli’s equation does not hold for non-steady or turbulent flow, since it assumes that the velocity at a point does not change with time and that the streamlines are smooth and do not cross (Section 9.4 and Points to Ponder 5 and 6).
| Condition needed for Bernoulli | Rapid in a river |
|---|---|
| steady flow (velocity at a point constant in time) | No — velocity fluctuates with time |
| streamline (laminar) flow along which energy is conserved | No — flow is turbulent with eddies and cross currents |
| negligible viscosity (no dissipation of energy) | No — much of the kinetic energy is lost as heat in the eddies |
| incompressible fluid | Yes (water) but this alone is not enough |
A large part of the mechanical energy of the water is converted into heat and sound in the turbulent region, so P + ½ρv2 + ρgh is not constant along the flow; it decreases downstream. Hence the equation cannot be used to calculate the speed or pressure at a point in a rapid.
Extra depth. Where could one use it in a river? In the smooth part of the river far from the rapids the flow is steady and nearly laminar, so the continuity equation and Bernoulli’s equation give a good first estimate (for instance the speed of the water as the river narrows and its depth changes). For the rapid itself one must use experiments, models with dimensionless numbers such as the Reynolds number, or computer simulation.
More to know. Even in the rapid, one can speak of an average flow, and the continuity equation holds for the time-averaged flow (the mass entering equals the mass leaving), because mass is conserved in any flow. It is only the energy equation that cannot be used in this simple form, since energy is dissipated by eddies. In engineering the head loss in such flows is found from empirical formulas; the Reynolds number R = ρvD/η is far above 2000 in a river rapid (for water η = 10−3 Pa s, v = 2 m s−1, D = 1 m, R = 2×106), confirming that the flow is turbulent.
Conclusion: No: the flow through a rapid is turbulent and non-steady, with energy loss to viscosity, so P + ½ρv2 + ρgh is not constant.
Ex 9.12 — Gauge pressure instead of absolute pressure in Bernoulli’s equation
Concept. In Bernoulli’s equation the pressures at two points enter in the form P1 − P2. Gauge pressure is P − Pa, so replacing P by (P − Pa) at both points subtracts the same Pa from both sides if the atmospheric pressure is the same at both points.
Question. Does it matter if one uses gauge instead of absolute pressures in applying Bernoulli’s equation? Explain.
Answer
Write Bernoulli’s equation for two points:
P1 + ½ρv12 + ρgh1 = P2 + ½ρv22 + ρgh2
With P1 = Pg1 + Pa1 and P2 = Pg2 + Pa2 (gauge + atmospheric), this becomes
Pg1 + ½ρv12 + ρgh1 + Pa1 = Pg2 + ½ρv22 + ρgh2 + Pa2
If the atmospheric pressure is the same at the two points (Pa1 = Pa2), the two Pa cancel and the equation has exactly the same form with gauge pressures. So it does not matter whether gauge or absolute pressure is used, as long as the same atmospheric pressure acts at both points. This is true in most laboratory and engineering situations (pipes, tanks, nozzles), and gauge pressure is often more convenient because it is what gauges read.
Exception: if the two points are at greatly different heights so that the atmospheric pressure differs appreciably between them (for example at the top and bottom of a tall mountain or a very high pipeline), the two Pa do not cancel and one must use absolute pressures, or add the difference of the atmospheric pressures. The same cancellation is used in Torricelli’s law, where Pa at the hole and at the top of an open tank is the same and only ρgh remains.
Extra depth. The “gauge pressure” form is what makes Ex 9.4(c) simple: the net force on the window of a submarine is PgA, since atmospheric pressure acts on both sides. In Bernoulli problems with an open tank one writes P1 = P2 = Pa and finds v = √(2gh) with no pressure term at all — the same idea.
Conclusion: It does not matter, because the atmospheric pressure cancels from both sides when it is the same at the two points; it would matter only if the atmospheric pressures differ significantly.
Ex 9.13 — Pressure difference for glycerine flowing steadily in a horizontal tube
Concept. For steady laminar flow of a viscous liquid in a horizontal tube of length L and radius r, the volume flow rate Q is given by Poiseuille’s formula Q = πr4ΔP/(8ηL), so ΔP = 8ηLQ/(πr4). (Poiseuille’s formula is a standard result of viscous flow; it is not derived in the text.)
Question. Glycerine flows steadily through a horizontal tube of length 1.5 m and radius 1.0 cm. If the amount of glycerine collected per second at one end is 4.0×10−3 kg s−1, what is the pressure difference between the two ends of the tube? (Density of glycerine = 1.3×103 kg m−3 and viscosity = 0.83 Pa s.) [Also check if the assumption of laminar flow in the tube is correct.]
Given
- L = 1.5 m, r = 1.0 cm = 1.0×10−2 m, η = 0.83 Pa s, ρ = 1.3×103 kg m−3
- Mass flow rate = 4.0×10−3 kg s−1
Step 1 — volume flow rate
Q = (mass per second)/ρ = (4.0×10−3)/(1.3×103) = 3.08×10−6 m3 s−1
Step 2 — pressure difference (Poiseuille)
ΔP = 8ηLQ/(πr4) = (8 × 0.83 × 1.5 × 3.08×10−6)/(3.14 × (10−2)4) = 3.07×10−5/(3.14×10−8) ≈ 9.8×102 Pa
Step 3 — is the flow laminar? (Reynolds number)
- Average speed v = Q/(πr2) = 3.08×10−6/(3.14×10−4) = 9.8×10−3 m s−1 (about 1 cm per second)
- Reynolds number R = ρvd/η = (1.3×103 × 9.8×10−3 × 2.0×10−2)/0.83 = 0.31
A flow in a tube is laminar if R is less than about 1000 and turbulent if R is more than about 2000 (a standard criterion; the textbook only mentions the critical speed). Here R = 0.31 << 1000, so the flow of the glycerine is laminar and the assumption is correct.
Extra depth. Because the tube is horizontal there is no height term in Bernoulli’s equation, but Bernoulli itself cannot be used because viscosity is significant: it would predict a pressure drop of zero (constant speed) in a uniform tube. The pressure drop of 9.8×102 Pa (about 7 mm of Hg) is entirely used to overcome viscous friction between the layers. The result ΔP ∝ 1/r4 is dramatic: halving the radius increases the required pressure difference sixteen times, which is why blocked arteries make the heart work much harder and why hypodermic needles control flow (Ex 9.4(c)).
Conclusion: ΔP = 8ηLQ/(πr4) ≈ 9.8×102 Pa and R ≈ 0.31, so the flow is laminar.
Ex 9.14 — Lift on a model aeroplane wing in a wind tunnel
Concept. The lift equals the pressure difference between the lower and upper surfaces times the wing area. Bernoulli’s equation for the two surfaces (same height): ΔP = ½ρ(vupper2 − vlower2) is the amount by which pressure below exceeds pressure above.
Question. In a test experiment on a model aeroplane in a wind tunnel, the flow speeds on the upper and lower surfaces of the wing are 70 m s−1 and 63 m s−1 respectively. What is the lift on the wing if its area is 2.5 m2? Take the density of air to be 1.3 kg m−3.
Given
- vupper = 70 m s−1, vlower = 63 m s−1, A = 2.5 m2, ρ = 1.3 kg m−3
Step 1 — Bernoulli’s equation for the two surfaces (negligible height difference)
Plower + ½ρvlower2 = Pupper + ½ρvupper2
ΔP = Plower − Pupper = ½ρ(vupper2 − vlower2) = ½ × 1.3 × (702 − 632)
702 = 4900 and 632 = 3969, so vupper2 − vlower2 = 931 m2 s−2 and ΔP = 0.65 × 931 = 605 Pa.
Step 2 — lift = pressure difference × area
Lift = ΔP × A = 605 × 2.5 = 1.51×103 N ≈ 1.5×103 N
The upward lift on the wing is about 1.5×103 N (the weight of about 154 kg), directed upward because the pressure below the wing is higher than above. The speed above is only 10% higher than below, yet the lift is large.
Extra depth. For comparison, in Example 9.7 a speed difference of only 8% produces the lift for a 3.3×105 kg aeroplane because its wing area is 500 m2 and the speeds are much larger (267 m s−1). Doubling the speed of the airflow quadruples the lift for the same wing (ΔP ∝ v2 difference), which is why aeroplanes need high speed on take-off.
Conclusion: Lift = ½ρ(vupper2 − vlower2)A = 1.5×103 N.
Ex 9.15 — Which flow figure (Fig 9.20) is incorrect?
Concept. For steady flow of a non-viscous liquid through a horizontal tube, the pressure is lower where the speed is higher (Bernoulli) and the speed is higher where the tube is narrower (continuity). The height of liquid in a vertical manometer tube measures the pressure there.
Question. Figures 9.20(a) and (b) refer to the steady flow of a (non-viscous) liquid. Which of the two figures is incorrect? Why?
Answer: Figure 9.20(a) is incorrect
- By the equation of continuity A1v1 = A2v2, the speed of the liquid is larger in the narrow part (the constriction) than in the wider part.
- By Bernoulli’s equation, for a horizontal tube P + ½ρv2 = constant, so where the speed is larger the pressure is smaller. So the pressure at the constriction is less than the pressure in the wider part.
- The height of the liquid in a vertical open tube is proportional to the (gauge) pressure at that point, P = ρgh. Thus the liquid level in the manometer at the constriction must be lower than the level in the manometer at the wide part.
- In Fig. 9.20(a) the level at the constriction is higher, which would mean a higher pressure where the speed is higher — contradicting Bernoulli’s principle. In Fig. 9.20(b) the level at the constriction is lower: correct.
The measurement of the pressure drop at a constriction in this way is the principle of the Venturi meter, used to find the flow speed of liquids in pipes: from the two heights, v22 − v12 = 2g(h1 − h2), and v1 follows from continuity.
Extra depth. The same argument explains why the two ships sailing closely side by side are drawn together (fast water in the gap, lower pressure), and why a fire hose or spray gun lifts liquid up a tube at the constriction (atomiser). In the diagram the pressure difference between the wide and narrow regions is ΔP = ½ρ(v22 − v12) = ρgΔh.
Conclusion: (a) is incorrect: the pressure (and hence the liquid level) must be lower at the constriction where the speed is higher.
Ex 9.16 — Speed of ejection from a spray pump
Concept. The volume of liquid flowing per second is the same through the tube and through all the holes (equation of continuity): A1v1 = A2v2, where A2 is the total area of all the holes.
Question. The cylindrical tube of a spray pump has a cross-section of 8.0 cm2, one end of which has 40 fine holes each of diameter 1.0 mm. If the liquid flow inside the tube is 1.5 m min−1, what is the speed of ejection of the liquid through the holes?
Given
- Cross-section of the tube A1 = 8.0 cm2 = 8.0×10−4 m2
- Speed in the tube v1 = 1.5 m min−1 = 1.5/60 = 0.025 m s−1
- Number of holes n = 40; diameter of each d = 1.0 mm ⇒ radius r = 0.5 mm = 5.0×10−4 m
Step 1 — total area of the holes
A2 = n π r2 = 40 × 3.14 × (5.0×10−4)2 = 40 × 7.85×10−7 = 3.14×10−5 m2
Step 2 — equation of continuity
v2 = A1v1/A2 = (8.0×10−4 × 0.025)/(3.14×10−5) = 2.0×10−5/3.14×10−5 = 0.64 m s−1
The liquid is ejected through the holes with a speed of 0.64 m s−1 (about 25 times the speed 0.025 m s−1 in the tube, because the total hole area is about 1/25 of the tube cross-section). The volume of liquid delivered per second is A1v1 = 2.0×10−5 m3 s−1 = 20 cm3 s−1.
Extra depth. Do not use the area of one hole: the same flow divides among 40 holes, and the continuity equation is written for the total cross-section A2 = 40πr2. An equivalent way: each hole delivers one-fortieth of the flow: v2 = (A1v1/40)/(πr2) gives the same answer. This is why a fine rose on a watering can or a shower head gives a fast spray: many small holes have a total area much smaller than the pipe.
Conclusion: v2 = A1v1/(40πr2) = 0.64 m s−1, because the total area of the holes is much smaller than the tube cross-section.
Ex 9.17 — Surface tension of a soap film supporting a weight
Concept. The film has two surfaces, each of which pulls on the slider with a force S l. At equilibrium the total upward force 2Sl equals the weight W supported, so S = W/2l.
Question. A U-shaped wire is dipped in a soap solution and removed. The thin soap film formed between the wire and the light slider supports a weight of 1.5×10−2 N (which includes the small weight of the slider). The length of the slider is 30 cm. What is the surface tension of the film?
Given
- Weight supported W = 1.5×10−2 N
- Length of the slider l = 30 cm = 0.30 m
Solution
The film has a front and a back surface, so the total length of the contact line which pulls on the slider is 2l. In equilibrium (Eq. 9.20 and 9.21):
S × 2l = W ⇒ S = W/2l = (1.5×10−2)/(2 × 0.30) = 2.5×10−2 N m−1
The surface tension of the soap film is 2.5×10−2 N m−1 (0.025 N m−1), about one-third of the value for pure water (7.27×10−2 N m−1, Table 9.3); the soap lowers the surface tension. The surface energy per unit area is the same number in J m−2: 2.5×10−2 J m−2 per surface.
Extra depth. The idea is the same as the measurement with the glass plate, S = mg/2l (Eq. 9.21), where the liquid film pulling on the plate is also two-sided (liquid on each of the two faces of the plate). A beginner’s error is to use S = W/l, which doubles the answer. If the film is stretched slowly by an extra distance d, the work done W d goes into surface energy S (2 l d), consistent with Eq. 9.19; the film does not need to support more weight as it is stretched, because S does not depend on area (Ex 9.2(c)).
Conclusion: S = W/2l = 1.5×10−2/(2 × 0.30) = 2.5×10−2 N m−1.
Ex 9.18 — Weight supported by liquid films of different shapes (Fig 9.21)
Concept. The force of surface tension on a movable bar depends only on S and the length of the line of contact: F = 2Sl. It does not depend on the shape or area of the film.
Question. Figure 9.21(a) shows a thin liquid film supporting a small weight of 4.5×10−2 N. What is the weight supported by a film of the same liquid at the same temperature in Fig. (b) and (c)? Explain your answer physically.
Answer
The weight supported by the film in (b) and in (c) is also 4.5×10−2 N.
Physical explanation
- The film pulls on the movable bar by surface tension, which is a force per unit length acting along the line of contact with the bar: F = S × (total length of the contact line) = S × 2l for a two-sided film.
- In all three diagrams the length of the bar is the same, 40 cm, and the liquid and temperature are the same, so S is the same. Hence the force of surface tension on the bar and the weight supported are the same in (a), (b) and (c).
- The surface area of the films is quite different (the film in (b) is longer and in (c) has a different shape), but surface tension, being a force per unit length (equivalently the energy per unit area), does not depend on the area of the film. Increasing the area does not increase the force, because fresh molecules come from the interior to the surface so that the surface energy per unit area stays the same.
| Film | Length of bar (cm) | Area of film | Weight supported |
|---|---|---|---|
| (a) | 40 | smaller | 4.5×10−2 N |
| (b) | 40 | larger (taller) | 4.5×10−2 N |
| (c) | 40 | different shape | 4.5×10−2 N |
Numerically, the surface tension of the liquid is S = W/2l = 4.5×10−2/(2 × 0.40) = 5.6×10−2 N m−1, the same in all three cases (a number comparable with soapy water).
Extra depth. This question tests the same idea as Ex 9.2(c): S is independent of the area. A film stretched like a rubber sheet would pull harder as it is stretched (Hooke’s law), but a liquid film does not — its restoring force per unit length remains constant as more surface is created.
Conclusion: In (b) and (c) the film supports the same weight 4.5×10−2 N, because the force 2Sl depends only on S and the 40 cm length, not on the area or shape.
Ex 9.19 — Pressure inside a mercury drop of radius 3.00 mm
Concept. A liquid drop has one liquid-air surface; the pressure inside is greater than that outside by the excess pressure 2S/r.
Question. What is the pressure inside the drop of mercury of radius 3.00 mm at room temperature? Surface tension of mercury at that temperature (20°C) is 4.65×10−1 N m−1. The atmospheric pressure is 1.01×105 Pa. Also give the excess pressure inside the drop.
Given
- r = 3.00 mm = 3.00×10−3 m
- S = 4.65×10−1 N m−1
- Po = Pa = 1.01×105 Pa
Step 1 — excess pressure (Eq. 9.25)
Pi − Po = 2S/r = (2 × 4.65×10−1)/(3.00×10−3) = 0.93/(3.00×10−3) = 310 Pa
Step 2 — pressure inside
Pi = Pa + 2S/r = 1.01×105 + 310 = 1.0131×105 Pa ≈ 1.01×105 Pa
The pressure inside the drop is 1.0131×105 Pa (to three significant figures 1.01×105 Pa) and the excess pressure is 310 Pa. The excess pressure is only 0.3% of the atmospheric pressure, but it is exactly this small pressure difference that holds the drop spherical.
Extra depth. The excess pressure depends inversely on the radius: a 0.3 mm mercury droplet would have an excess pressure ten times larger (3100 Pa). Mercury has a high S (0.465 N m−1 compared with 0.073 for water), so its drops are very nearly spherical when small and are flattened by gravity when large (ρgh = 13.6×103 × 9.8 × 3×10−3 = 400 Pa, the same order as 2S/r, so a 3 mm mercury drop is already slightly flattened).
More to know. Why do small drops tend to coalesce into bigger ones? The pressure inside a small drop is higher than inside a large one (2S/r is larger for small r), so if two drops of different size are connected by a tube, air or liquid flows from the smaller to the larger one — the small one shrinks and the large one grows. This is why a tiny drop of mercury runs into a larger drop when they touch. Worked comparison for mercury (S = 0.465 N m−1): r = 3.00 mm gives 310 Pa, r = 1.00 mm gives 930 Pa, r = 0.100 mm gives 9300 Pa. Only the tiniest drops have an excess pressure that is a measurable fraction of the atmospheric pressure.
Conclusion: Pi = Pa + 2S/r = 1.0131×105 Pa; excess pressure = 2S/r = 310 Pa.
Ex 9.20 — Excess pressure in a soap bubble and an air bubble in soap solution
Concept. A soap bubble in air has two liquid-air surfaces: excess pressure 4S/r. An air bubble formed inside a liquid has only one surface: excess pressure 2S/r, and the pressure outside it is Pa + ρgh.
Question. What is the excess pressure inside a bubble of soap solution of radius 5.00 mm, given that the surface tension of the soap solution at 20°C is 2.50×10−2 N m−1? If an air bubble of the same dimension were formed at a depth of 40.0 cm inside a container containing the soap solution (of relative density 1.20), what would be the pressure inside the bubble? (1 atmosphere = 1.01×105 Pa.)
Part 1 — soap bubble in air (two surfaces)
Pi − Po = 4S/r = (4 × 2.50×10−2)/(5.00×10−3) = 0.10/(5.00×10−3) = 20 Pa
Part 2 — air bubble at 40.0 cm depth (one surface)
- Density of the soap solution ρ = 1.20 × 103 kg m−3; depth h = 0.400 m
- Pressure outside the bubble Po = Pa + ρgh = 1.01×105 + (1.20×103)(9.8)(0.400) = 1.01×105 + 4704 = 1.0570×105 Pa
- Excess pressure for a single surface: 2S/r = (2 × 2.50×10−2)/(5.00×10−3) = 10 Pa
Pi = Po + 2S/r = 1.0570×105 + 10 = 1.06×105 Pa
So the excess pressure inside the soap bubble in air is 20 Pa, and the pressure inside the air bubble at 40.0 cm depth in the soap solution is 1.06×105 Pa (1.0571×105 Pa), of which only 10 Pa is due to surface tension and about 4.7×103 Pa due to the depth of the liquid.
Extra depth. Note how small the surface-tension contribution (10 Pa) is compared with the hydrostatic part (4700 Pa) for a bubble of 5 mm radius. The bubble of Example 9.10 (r = 1 mm at 8 cm depth) is similar: 146 Pa from surface tension, 784 Pa from depth. A soap bubble has two surfaces (the inner and the outer of the thin film), so its excess pressure is double that of an air bubble in liquid of the same radius and S.
Conclusion: Soap bubble in air: 4S/r = 20 Pa. Air bubble at 40 cm depth in the solution: Pi = Pa + ρgh + 2S/r = 1.06×105 Pa.